VARIABLE MAGNIFICATION OPTICAL SYSTEM AND IMAGING APPARATUS

Information

  • Patent Application
  • 20220236543
  • Publication Number
    20220236543
  • Date Filed
    December 22, 2021
    3 years ago
  • Date Published
    July 28, 2022
    2 years ago
Abstract
The variable magnification optical system consists of, in order from an object side to an image side, a first lens group that has a positive refractive power, a plurality of lens groups, and a final lens group that has a positive refractive power. During changing magnification, a spacing between the first lens group and the lens group closest to the object side among the plurality of lens groups changes, all spacings between adjacent lens groups in the plurality of lens groups change, and a spacing between the lens group closest to the image side and the final lens group among the plurality of lens groups changes.
Description
CROSS-REFERENCE TO RELATED APPLICATIONS

The present application claims priority under 35 U.S.C. § 119 to Japanese Patent Application No. 2021-008221, filed on Jan. 21, 2021 and Japanese Patent Application No. 2021-182841, filed on Nov. 9, 2021. Each application above is hereby expressly incorporated by reference, in its entirety, into the present application.


BACKGROUND
Technical Field

The technology of the present disclosure relates to a zooming optical system and an imaging apparatus.


Related Art

In the related art, as a variable magnification optical system applicable to an imaging apparatus such as a broadcasting camera, a movie shooting camera, and a digital camera, for example, the lens systems described in JP2018-205332A, JP2019-139253A, and JP2020-012909A are known.


SUMMARY

In recent years, there has been a demand for a variable magnification optical system that has a small size and has favorable optical performance


The present disclosure has been made in view of the above circumstances, and an object of the present disclosure is to provide a variable magnification optical system, which is reduced in size and has favorable optical performance, and an imaging apparatus comprising the variable magnification optical system.


The variable magnification optical system according to an aspect of the technique of the present disclosure consists of, in order from an object side to an image side: a first lens group that has a positive refractive power; a plurality of lens groups; and a final lens group that has a positive refractive power. During changing magnification, a spacing between the first lens group and the lens group closest to the object side among the plurality of lens groups changes, all spacings between adjacent lens groups in the plurality of lens groups change, and a spacing between the lens group closest to the image side among the plurality of lens groups and the final lens group changes.


Assuming that a focal length of the first lens group in a state in which an infinite distance object is in focus is f1, a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, and an open F number of the variable magnification optical system at the telephoto end in the state in which the infinite distance object is in focus is FNt, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (1) represented by









1
<

f






1
/

(

ft
/
FNt

)



<
3.




(
1
)







Assuming that a maximum image height is Ims, and a focal length of the first lens group in a state in which an infinite distance object is in focus is f1, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (2) represented by










0
.
1

<


Ims
/
f






1

<

0.5
.





(
2
)







It is preferable that a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group. Assuming that a focal length of the fz group is ffz, and a maximum image height is Ims, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (3) represented by











0
.
0


5

<



Ims
/
ffz



<

0.6
.





(
3
)







It is preferable that a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group. Assuming that a lateral magnification of the fz group at the telephoto end in the state in which the infinite distance object is in focus is βfzt, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (4) represented by










-

0
.
3


<


1
/
β


fzt

<

0.3
.





(
4
)







It is preferable that a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group. Assuming that a focal length of the fz group is ffz, and a difference in an optical axis direction between a position of the fz group at the wide angle end and a position of the fz group at the telephoto end is Dpfz, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (5) represented by









0.3
<



Dpfz
/
ffz



<
3.




(
5
)







It is preferable that the plurality of lens groups include, in order from a position closest to the object side to the image side, a middle group, which includes one or more lens groups and has a negative refractive power as a whole, and a negative movable lens group, which has a negative refractive power and moves during changing magnification, and the negative movable lens group is positioned closest to the image side in the lens groups having negative refractive powers in the plurality of lens groups.


Assuming that a focal length of the middle group at a wide angle end in a state in which an infinite distance object is in focus is fMw, and a focal length of the negative movable lens group is fN, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (6) represented by










0
.
2

<

fMw
/
fN

<

0.7
.





(
6
)







In a configuration in which the negative movable lens group includes one or more negative lenses and one or more positive lenses, assuming that a maximum absolute value of a difference between an Abbe number of the negative lens included in the negative movable lens group based on a d line and an Abbe number of the positive lens included in the negative movable lens group based on the d line is μNdif, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (7) represented by









40
<

ν





Ndif

<
95.




(
7
)







In a configuration in which the middle group includes one or more positive lenses, assuming that an Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the middle group based on the d line is νM and a partial dispersion ratio thereof between a g line and an F line is θM, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (8) represented by











-

0
.
0



2

<


θ

M

+


0
.
0


0

18
×
ν





M

-

0.

6

4

8

3

3


<

0


.07
.






(
8
)







Assuming that a curvature radius of an image side surface of a negative lens closest to the object side in the middle group is RMnr, and a curvature radius of an object side surface of a lens disposed adjacent to the image side of a negative lens closest to the object side in the middle group is RMf, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (9) represented by










-

1
.
5


<


(

RMnr
+
RMf

)

/

(

RMnr
-
RMf

)


<

0.2
.





(
9
)







Assuming that a difference in an optical axis direction between a position of a lens surface closest to the image side in the middle group at a wide angle end and a position of a lens surface closest to the image side in the middle group at a telephoto end in a state in which an infinite distance object is in focus is DpM, a focal length of the variable magnification optical system at a wide angle end in the state in which the infinite distance object is in focus is fw, a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, and a maximum image height is Ims, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (10) represented by










0
.
2

<

DpM
/

{


(

f


t
/
fw


)

×
Ims

}


<

0.9
.





(
10
)







Assuming that an effective diameter of a lens surface closest to the object side in the middle group in a state in which an infinite distance object is in focus is EDMf, and an effective diameter of a lens surface closest to the image side in the middle group in the state in which the infinite distance object is in focus is EDMr, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (11) represented by









0.5
<

EDMf
/
EDMr

<

3.25
.





(
11
)







Assuming that a height of a principal ray from an optical axis at a maximum image height on a lens surface closest to the object side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMfb, a height of the on-axis marginal ray from the optical axis on the lens surface closest to the object side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMfa, a height of a principal ray from the optical axis at a maximum image height on a lens surface closest to the image side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMrb, and a height of an on-axis marginal ray from the optical axis on the lens surface closest to the image side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMra, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (12) represented by









1
<



(


HMfb/HMfa



)/(



HMrb/HMra


)



<
3.




(
12
)







The plurality of lens groups may be configured to consist of an middle group and a negative movable lens group.


The middle group may be configured to consist of a front lens group having a positive refractive power and a rear lens group having a negative refractive power in order from the object side to the image side, and a spacing between the front lens group and the rear lens group changes during changing magnification.


Groups, which are included in the plurality of lens groups and move by changing a spacing from an adjacent lens group during changing magnification, may be configured to consist of, in order from the object side to the image side, the middle group, the negative movable lens group, and a positive movable lens group having a positive refractive power.


Assuming that a maximum image height is Ims, and a focal length of the final lens group is fE, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (13) represented by










0

.1

<

Ims/fE

<

0.6
.





(
13
)







Assuming that an Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the final lens group based on the d line is νE and a partial dispersion ratio thereof between a g line and an F line is θE, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (14) represented by











0
.
0


2

<


θ

E

+


0
.
0


0

1

8
×
v

E

-


0
.
6


4

8

3

3


<

0.08
.





(
14
)







It is preferable that the variable magnification optical system of the above-mentioned aspect includes a focus group that performs focusing by moving along an optical axis. Assuming that a specific gravity of each lens in the focus group is Sgf and a refractive index thereof at a d line is Nf, an average value of Sgf/Nf of all lenses in the focus group is ave(Sgf/Nf), and a maximum value of refractive indexes of all the lenses in the focus group at the d line is Nfmax, it is preferable that the variable magnification optical system satisfies Conditional Expressions (15) and (16) represented by












2
.
0


5

<

ave


(

Sgf/Nf

)


<
2.55

,
and




(
15
)






1.7
<

Nf

max

<

2.2
.





(
16
)







It is preferable that in a case where a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, the number of the movable lens groups included in the variable magnification optical system is three or more, and the movable lens group closest to the object side among the movable lens groups included in the variable magnification optical system has a positive refractive power.


It is preferable that the movable lens group closest to the object side among the movable lens groups included in the variable magnification optical system consists of one positive lens having a convex surface facing toward the object side. In such a case, assuming that a curvature radius of an object side surface of the positive lens having the convex surface facing toward the object side is Rpf, and a curvature radius of an image side surface of the positive lens having the convex surface facing toward the object side is Rpr, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (17) represented by










-
6

<

(

Rpf
-

Rpr


)/(


Rpf

+
Rpr

)

<
1.




(
17
)







The first lens group may be configured to consist of, in order from the object side to the image side, a first A subgroup having a negative refractive power, a first B subgroup having a positive refractive power, and a first C subgroup having a positive refractive power, and focusing is performed by moving the first B subgroup along an optical axis.


Assuming that a maximum image height is Ims, and a focal length of the first C subgroup is f1C, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (18) represented by











0
.
0


5

<

Ims/f
1
C

<

0.3
.





(
18
)







Assuming that a focal length of the first lens group is f1, and a focal length of the first B subgroup is f1B, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (19) represented by










0

.3

<

f
1
/f
1
B

<

0.9
.





(
19
)







In a configuration in which the first B subgroup includes one or more positive lenses and one or more negative lenses, assuming that an Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the first B subgroup based on the d line is ν1Bp, and a partial dispersion ratio thereof between a g line and an F line is θ1Bp, and a minimum value of Abbe numbers of all the negative lenses included in the first B subgroup based on the d line is ν1Bn, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expressions (20) and (21) represented by












0
.
0


1

<


θ1





Bp

+

0.

0

0

1

8
×
v





1

Bp

-

0.

6

4

8

3

3


<
0.07

,
and




(
20
)






15
<

v





1

Bn

<
40.




(
21
)







It is preferable that the first A subgroup includes two or more negative lenses of which Abbe numbers based on a d line are 50 or more. Assuming that a minimum value of Abbe numbers of all the positive lenses included in the first A subgroup based on the d line is ν1Ap, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (22) represented by










1

5

<

v





1

Ap

<
40.




(
22
)







It is preferable that the first lens group remains stationary with respect to an image plane during changing magnification.


It is preferable that the final lens group remains stationary with respect to an image plane during changing magnification, and a stop is disposed closest to the object side in the final lens group. In such a case, it is preferable that a lens component disposed adjacent to the image side of the stop has a biconvex shape. It should be noted that one lens component is one single lens or one group of cemented lenses. Assuming that a curvature radius of a surface closest to the object side of the lens component disposed adjacent to the image side of the stop is REf, and a curvature radius of a surface closest to the image side of the lens component disposed adjacent to the image side of the stop is REr, it is preferable that the variable magnification optical system of the above-mentioned aspect satisfies Conditional Expression (23) represented by










-

0
.
7


<

(

REf
+

REr


)/(


REf

-
REr

)

<

0.7
.





(
23
)







Assuming that a temperature coefficient of a relative refractive index of a lens in the final lens group at a d line in a range of 20° C. to 40° C. is dN/dT and a unit of dN/dT is ° C.−1, it is preferable that the final lens group includes one or more lenses respectively having an Abbe number based on the d line of 65 or more and satisfying Conditional Expression (24), which is represented by









0
<

dN/dT

<

8
×
1



0

-
6


.






(
24
)







An imaging apparatus according to another aspect of the technique of the present disclosure includes a variable magnification optical system according to the above-mentioned aspect of the present disclosure.


In the present specification, it should be noted that the terms “consisting of ˜” and “consists of ˜” mean that the lens may include not only the above-mentioned constituent elements but also lenses substantially having no refractive powers, optical elements, which are not lenses, such as a stop, a filter, and a cover glass, and mechanism parts such as a lens flange, a lens barrel, an imaging element, and a camera shaking correction mechanism.


The term “˜ group that has a positive refractive power” in the present specification means that the group has a positive refractive power as a whole. Similarly, the term “˜ group having a negative refractive power” means that the group has a negative refractive power as a whole. The term “a lens having a positive refractive power” and the term “a positive lens” are synonymous. The term “a lens having a negative refractive power” and the term “negative lens” are synonymous. The terms “˜ lens group” and “˜ subgroup” are not limited to a configuration in which the lens group consists of a plurality of lenses, but the lens group may consist of only one lens.


The term “a single lens” means one lens that is not cemented. Here, a compound aspheric lens (a lens in which a spherical lens and an aspheric film formed on the spherical lens are integrally formed and function as one aspheric lens as a whole) is not regarded as cemented lenses, but the compound aspheric lens is regarded as one lens. Unless otherwise specified, the sign of refractive power, the surface shape, and the curvature radius of a lens including an aspherical surface are considered in terms of the paraxial region. The sign of the curvature radius of the surface convex toward the object side is positive and the sign of the curvature radius of the surface convex toward the image side is negative.


The “focal length” used in a conditional expression is a paraxial focal length. The values used in conditional expressions are values in the case of using the d line as a reference in a state in which the infinite distance object is in focus.


The partial dispersion ratio θgF between the g line and the F line of a certain lens is defined by θgF=(Ng−NF)/(NF−NC), where Ng, NF, and NC are the refractive indexes of the lens at the g line, the F line, and the C line. The “d line”, “C line”, “F line”, and “g line” described in the present specification are emission lines. In the present specification, it is assumed that the d line wavelength is 587.56 nm (nanometers), the C line wavelength is 656.27 nm (nanometers), the F line wavelength is 486.13 nm (nanometers), and the g line wavelength is 435.84 nm (nanometers).


According to the technique of the present disclosure, it is possible to provide a variable magnification optical system, which is reduced in size and has favorable optical performance, and an imaging apparatus comprising the variable magnification optical system.





BRIEF DESCRIPTION OF THE DRAWINGS


FIG. 1 is a cross-sectional view of a configuration of a variable magnification optical system according to an embodiment corresponding to the variable magnification optical system of Example 1, and is a diagram showing movement loci.



FIG. 2 is a cross-sectional view of the configuration of the variable magnification optical system shown in FIG. 1, and is a diagram showing luminous flux.



FIG. 3 is a diagram for explaining an effective diameter.



FIG. 4 is a diagram for explaining a symbol of Conditional Expression (12).



FIG. 5 is a diagram of aberrations of the variable magnification optical system of Example 1.



FIG. 6 is a cross-sectional view of the configuration of the variable magnification optical system of Example 2, and is a diagram showing movement loci.



FIG. 7 is a diagram of aberrations of the variable magnification optical system of Example 2.



FIG. 8 is a cross-sectional view of the configuration of the variable magnification optical system of Example 3, and is a diagram showing movement loci.



FIG. 9 is a diagram of aberrations of the variable magnification optical system of Example 3.



FIG. 10 is a cross-sectional view of the configuration of the variable magnification optical system of Example 4, and is a diagram showing movement loci.



FIG. 11 is a diagram of aberrations of the variable magnification optical system of Example 4.



FIG. 12 is a cross-sectional view of the configuration of the variable magnification optical system of Example 5, and is a diagram showing movement loci.



FIG. 13 is a diagram of aberrations of the variable magnification optical system of Example 5.



FIG. 14 is a cross-sectional view of the configuration of the variable magnification optical system of Example 6, and is a diagram showing movement loci.



FIG. 15 is a diagram of aberrations of the variable magnification optical system of Example 6.



FIG. 16 is a cross-sectional view of the configuration of the variable magnification optical system of Example 7, and is a diagram showing movement loci.



FIG. 17 is a diagram of aberrations of the variable magnification optical system of Example 7.



FIG. 18 is a cross-sectional view of the configuration of the variable magnification optical system of Example 8, and is a diagram showing movement loci.



FIG. 19 is a diagram of aberrations of the variable magnification optical system of Example 8.



FIG. 20 is a cross-sectional view of the configuration of the variable magnification optical system of Example 9, and is a diagram showing movement loci.



FIG. 21 is a diagram of aberrations of the variable magnification optical system of Example 9.



FIG. 22 is a cross-sectional view of the configuration of the variable magnification optical system of Example 10, and is a diagram showing movement loci.



FIG. 23 is a diagram of aberrations of the variable magnification optical system of Example 10.



FIG. 24 is a cross-sectional view of the configuration of the variable magnification optical system of Example 11, and is a diagram showing movement loci.



FIG. 25 is a diagram of aberrations of the variable magnification optical system of Example 11.



FIG. 26 is a cross-sectional view of the configuration of the variable magnification optical system of Example 12, and is a diagram showing movement loci.



FIG. 27 is a diagram of aberrations of the variable magnification optical system of Example 12.



FIG. 28 is a cross-sectional view of the configuration of the variable magnification optical system of Example 13, and is a diagram showing movement loci.



FIG. 29 is a diagram of aberrations of the variable magnification optical system of Example 13.



FIG. 30 is a cross-sectional view of the configuration of the variable magnification optical system of Example 14, and is a diagram showing movement loci.



FIG. 31 is a diagram of aberrations of the variable magnification optical system of Example 14.



FIG. 32 is a cross-sectional view of the configuration of the variable magnification optical system of Example 15, and is a diagram showing movement loci.



FIG. 33 is a diagram of aberrations of the variable magnification optical system of Example 15.



FIG. 34 is a diagram showing a schematic configuration of an imaging apparatus according to an embodiment.





DESCRIPTION OF EMBODIMENTS

Hereinafter, embodiments according to the technique of the present disclosure will be described with reference to the accompanying drawings.



FIG. 1 shows a cross-sectional view of the configuration at the wide angle end of the variable magnification optical system according to the embodiment of the present disclosure and shows movement loci. The example shown in FIG. 1 corresponds to the variable magnification optical system of Example 1 to be described later. FIG. 1 shows a state in which the infinite distance object is in focus, the left side thereof is an object side, and the right side thereof is an image side.



FIG. 1 shows an example in which an optical member PP having a parallel plate shape is disposed between a variable magnification optical system and an image plane Sim under assumption that the variable magnification optical system is applied to the imaging apparatus. The optical member PP is a member assumed to include various filters, a cover glass, and the like. The various filters include, for example, a low pass filter, an infrared cut filter, and a filter that cuts a specific wavelength region. The optical member PP is a member that has no refractive power. It is also possible to configure the imaging apparatus by removing the optical member PP.


The variable magnification optical system according to the present embodiment consists of, in order from the object side to the image side, a first lens group G1, a plurality of lens groups, and a final lens group GE. It should be noted that the term “lens group” in the present specification refers to a part including the at least one lens, which is a constituent part of the variable magnification optical system and is divided by an air spacing that changes during changing magnification. During changing magnification, the lens groups move or remain stationary, and the mutual spacing between the lenses in one lens group does not change.


The first lens group G1 is a lens group having a positive refractive power. By forming the lens group closest to the object side as the first lens group G1 having a positive refractive power, it is possible to achieve reduction in total length of the lens system. Thus, there is an advantage in achieving reduction in size. The final lens group GE is a lens group having a positive refractive power. By setting the final lens group GE closest to the image side as a lens group having a positive refractive power, it is possible to suppress an increase in angle at which the principal ray of the off-axis luminous flux is incident on the image plane Sim. As a result, there is an advantage in suppressing shading.


During changing magnification, a spacing between the first lens group G1 and the lens group closest to the object side among the plurality of lens groups changes, all spacings between adjacent lens groups in the plurality of lens groups change, and a spacing between the lens group closest to the image side among the plurality of lens groups and the final lens group GE changes.


For example, the variable magnification optical system in FIG. 1 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power. The plurality of lens groups correspond to the second lens group G2, the third lens group G3, and the fourth lens group G4. The final lens group GE corresponds to the fifth lens group G5.


In the example of FIG. 1, the first lens group G1 consists of eight lenses L1a to L1h in order from the object side to the image side. The second lens group G2 consists of one lens L2a. The third lens group G3 consists of eight lenses L3a to L3h in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side. It should be noted that the aperture stop St shown in FIG. 1 does not indicate a shape thereof, but indicates a position thereof in the direction of the optical axis.


In the example of FIG. 1, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim during changing magnification. Since the lens group closest to the object side and the lens group closest to the image side remain stationary during changing magnification, the distance from the lens surface closest to the object side to the lens surface closest to the image side does not change during changing magnification. According to this configuration, fluctuation in centroid of the lens system during changing magnification can be reduced. Therefore, the convenience during imaging can be enhanced.


Further, in the example of FIG. 1, during changing magnification, the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacings between the adjacent lens groups. In FIG. 1, arrows below respective lens groups indicate approximate movement loci of the second lens group G2, the third lens group G3, and the fourth lens group G4 during changing magnification from the wide angle end to the telephoto end.



FIG. 2 shows a cross-sectional view of the configuration of the variable magnification optical system and luminous flux in each zooming state in FIG. 1. In FIG. 2, the upper part labeled by “WIDE” shows the wide angle end state, the middle part labeled by “MIDDLE” shows the middle focal length state, and the lower part labeled by “TELE” shows the telephoto end state. FIG. 2 shows luminous flux including on-axis luminous flux wa and luminous flux wb at the maximum image height Ims at the wide angle end state, on-axis luminous flux ma and luminous flux mb at the maximum image height Ims at the middle focal length state, and on-axis luminous flux to and luminous flux tb at the maximum image height Ims at the telephoto end state. FIG. 2 shows a state in which the infinite distance object is in focus, the left side thereof is an object side, and the right side thereof is an image side. In FIG. 2, some reference numerals are not repeated in order to avoid complication of the drawings.


In the variable magnification optical system according to the present embodiment, Assuming that a focal length of the first lens group G1 in the state in which the infinite distance object is in focus is f1, a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, and an open F number of the variable magnification optical system at the telephoto end in the state in which the infinite distance object is in focus is FNt, it is preferable to satisfy Conditional Expression (1). By not allowing the corresponding value of Conditional Expression (1) to be equal to or less than the lower limit, it is possible to suppress an increase in emission angle of the on-axis marginal ray from the first lens group G1 at the telephoto end. As a result, during changing magnification from the wide angle side to the telephoto side, the second lens group G2 can be easily moved to the image side. Thus, there is an advantage in achieving an increase in magnification. Further, by not allowing the corresponding value of Conditional Expression (1) to be equal to or less than the lower limit, there is an advantage in preventing F drop. The F drop is a phenomenon in which the F number becomes remarkably large on the telephoto side from a certain focal length during changing magnification from the wide angle end to the telephoto end. In some conventional variable magnification optical systems, particularly, high magnification variable magnification optical systems, F drop is caused from the viewpoint of size and weight. However, in some cases, a user may request that the F number is substantially constant even during changing magnification from the wide angle end to the telephoto end. By not allowing the corresponding value of Conditional Expression (1) to be equal to or less than the lower limit, it is easy to meet such a request. By not allowing the corresponding value of Conditional Expression (1) to be equal to or greater than the upper limit, it is easy to prevent the emission angle of the on-axis marginal ray from the first lens group G1 at the telephoto end from becoming excessively small. As a result, it is possible to suppress an increase in height of the on-axis marginal ray passing through the second lens group G2 from the optical axis Z. Thus, there is an advantage in achieving reduction in diameter of the second lens group G2. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (1-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (1-2).









1
<

f
1
/(ft/FNt)

<
3




(
1
)






1.1
<

f
1
/(ft/FNt)

<
2.75




(

1-1

)






1.3
<

f
1
/(ft/FNt)

<
2.5




(

1-2)








Assuming that a maximum image height is Ims, and a focal length of the first lens group G1 in the state in which the infinite distance object is in focus is f1, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (2). By not allowing the corresponding value of Conditional Expression (2) to be equal to or less than the lower limit, the refractive power of the first lens group G1 can be ensured. Therefore, the spherical aberration can be suppressed from being insufficiently corrected, particularly on the telephoto side. Further, it is possible to suppress an increase in diameter of the second lens group G2. By not allowing the corresponding value of Conditional Expression (2) to be equal to or greater than the upper limit, the refractive power of the first lens group G1 is prevented from becoming excessively strong. Therefore, it is possible to suppress overcorrection of spherical aberration. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (2-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (2-2).










0
.
1

<


Ims
/
f






1

<
0.5




(
2
)






0.11
<


Ims
/
f






1

<
0.35




(

2


-


1

)






0.12
<


Ims
/
f






1

<
0.2




(

2


-


2

)







Further, it is preferable that the variable magnification optical system according to the present embodiment satisfies at least one of Conditional Expressions (3) to (5) with respect to the fz group defined below. In the present specification, a lens group that moves by changing the spacing from an adjacent lens group during changing magnification is referred to as a “movable lens group”.


Among the movable lens groups included in the variable magnification optical system, a movable lens group, of which the absolute value of the ratio of the lateral magnification of the movable lens group at the telephoto end to the lateral magnification of the movable lens group at the wide angle end is the maximum in a state where the infinite distance object is in focus, is defined as the fz group. That is, for each movable lens group included in the variable magnification optical system, assuming that a lateral magnification of the movable lens group at the wide angle end in a state where the infinite distance object is in focus is βw and a lateral magnification of the movable lens group at the telephoto end in a state where the infinite distance object is in focus is βt, the movable lens group having the maximum|βt/βw| is defined as the fz group.


In the example of FIG. 1, the movable lens group is the second lens group G2, the third lens group G3, and the fourth lens group G4. In the example of FIG. 1, of the three lens groups, the third lens group G3 is the fz group.


Assuming that a focal length of the fz group is ffz and a maximum image height is Ims, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (3). Among the movable lens groups included in the variable magnification optical system, the fz group defined by the above definition is a lens group having a main zooming effect. By not allowing the corresponding value of Conditional Expression (3) to be equal to or less than the lower limit, it is possible to ensure that the refractive power of the fz group is not weakened. Thereby, the amount of movement of the fz group at the time of zooming can be suppressed. As a result, there is an advantage in shortening the total length of the lens system, or there is an advantage in achieving an increase in magnification while maintaining the predetermined total length of the lens system. By not allowing the corresponding value of Conditional Expression (3) to be equal to or greater than the upper limit, the refractive power of the fz group is prevented from becoming excessively strong. Therefore, it is easy to suppress fluctuation in spherical aberration and fluctuation in field curvature due to zooming. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (3-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (3-2).











0
.
0


5

<



Ims
/
ffz



<
0.6




(
3
)






0.1
<



Ims
/
ffz



<
0.5




(

3


-


1

)






0.12
<



Ims
/
ffz



<
0.41




(

3


-


2

)







Assuming that a lateral magnification of the fz group at the telephoto end in the state in which the infinite distance object is in focus is βfzt, it is preferable that the fz group satisfies Conditional Expression (4). In a case where the lateral magnification of the fz group is within the range of Conditional Expression (4), it is easy to increase the magnification while shortening the total length of the lens system. In order to obtain more favorable characteristics, it is more preferable that the fz group satisfies Conditional Expression (4-1), and it is yet more preferable that the fz group satisfies Conditional Expression (4-2).











-
0


.3

<

1/β
fzt

<
0.3




(
4
)








-

0
.
2



5

<

1/β
fzt

<
0.1




(

4-1)









-

0
.
1



5

<

1/β
fzt

<
0.05




(

4-2)








Assuming that a focal length of the fz group is ffz and a difference in the optical axis direction between a position of the fz group at the wide angle end and a position of the fz group at the telephoto end is Dpfz, it is preferable that the fz group satisfies Conditional Expression (5). By not allowing the corresponding value of Conditional Expression (5) to be equal to or less than the lower limit, the amount of movement of the fz group can be ensured. Therefore, it is easy to increase the magnification. By not allowing the corresponding value of Conditional Expression (5) to be equal to or greater than the upper limit, the amount of movement of the fz group during changing magnification can be suppressed. As a result, there is an advantage in shortening the total length of the lens system. In order to obtain more favorable characteristics, it is more preferable that the fz group satisfies Conditional Expression (5-1), and it is yet more preferable that the fz group satisfies Conditional Expression (5-2).









0.3
<



Dpfz/ffz



<
3




(
5
)






0.45
<



Dpfz/ffz



<
2.5




(

5-1)







0.6
<



Dpfz/ffz



<
2




(5-2)







For example, FIG. 2 shows Dpfz in a case where the third lens group G3 is the fz group. In FIG. 2, Dpfz and DpM to be described later are the same, but this is an example. In the variable magnification optical system of the present disclosure, Dpfz and DpM may be different.


In the variable magnification optical system according to the present embodiment, the plurality of lens groups disposed between the first lens group G1 and the final lens group GE may be configured to include the middle group GM and the negative movable lens group GN in order from the position closest to the object side to the image side. The middle group GM is a group including one or more lens groups and having a negative refractive power as a whole. The negative movable lens group GN is a lens group having a negative refractive power positioned closest to the image side among the lens groups having a negative refractive power in the plurality of lens groups, and is a lens group that moves during changing magnification. In such a case, fluctuation in spherical aberration and fluctuation in chromatic aberration caused by the middle group GM during changing magnification can be reduced by the negative movable lens group GN. Therefore, there is an advantage in achieving both a small F number and an increase in magnification. In the above-mentioned phrase “a plurality of lens groups include an middle group GM and a negative movable lens group GN in order from the position closest to the object side to the image side”, the middle group GM and the negative movable lens group GN may be continuously disposed, and may be discontinuously disposed.


In a case where the variable magnification optical system includes the middle group GM, the middle group GM may be configured to consist of a front lens group having a positive refractive power and a rear lens group having a negative refractive power in order from the object side to the image side, and a spacing between the front lens group and the rear lens group changes during changing magnification. In such a case, it is easy to satisfactorily suppress fluctuations in various aberrations due to zooming.


In the example of FIG. 1, the middle group GM consists of the second lens group G2 and the third lens group G3. In the example of FIG. 1, the front lens group corresponds to the second lens group G2, the rear lens group corresponds to the third lens group G3, and the negative movable lens group GN corresponds to the fourth lens group G4.


As in the example of FIG. 1, the plurality of lens groups disposed between the first lens group G1 and the final lens group GE may be configured to consist of the middle group GM and the negative movable lens group GN. By limiting the group which is present between the first lens group G1 and the final lens group GE to only the middle group GM and the negative movable lens group GN, it is easy to reduce the size of the optical system.


With respect to the middle group GM and the negative movable lens group GN, it is preferable that the variable magnification optical system according to the present embodiment satisfies at least one of Conditional Expressions (6) to (12).


Assuming that a focal length of the middle group GM at a wide angle end in a state in which the infinite distance object is in focus is fMw, and a focal length of the negative movable lens group GN is fN, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (6). By not allowing the corresponding value of Conditional Expression (6) to be equal to or less than the lower limit, there is an advantage in suppressing fluctuations in various aberrations due to zooming. By not allowing the corresponding value of Conditional Expression (6) to be equal to or greater than the upper limit, there is an advantage in shortening the total length of the lens system, or there is an advantage in increasing the magnification while maintaining the predetermined total length of the lens system. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (6-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (6-2).










0
.
2

<

fMw
/
fN

<
0.7




(
6
)






0.25
<

fMw
/
fN

<
0.65




(

6


-


1

)






0.4
<

fMw
/
fN

<
0.6




(

6


-


2

)







In a configuration in which the negative movable lens group GN includes one or more negative lenses and one or more positive lenses. Assuming that a maximum absolute value of a difference between an Abbe number of the negative lens included in the negative movable lens group GN based on the d line and an Abbe number of the positive lens included in the negative movable lens group GN based on the d line is μNdif, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (7). By not allowing the corresponding value of Conditional Expression (7) to be equal to or less than the lower limit, it is easy to suppress fluctuation in chromatic aberration due to zooming. By not allowing the corresponding value of Conditional Expression (7) to be equal to or greater than the upper limit, a material having a high refractive index can be selected. Therefore, it is easy to satisfactorily suppress fluctuations in various aberrations due to zooming while achieving reduction in size and high magnification. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (7-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (7-2).









40
<

ν





Ndif

<
95




(
7
)






45
<

ν





Ndif

<
85




(

7


-


1

)






50
<

ν





Ndif

<
75




(

7


-


2

)







In a configuration in which the middle group GM includes one or more positive lenses, assuming that an Abbe number of the positive lens having a largest Abbe number based on the d line among the positive lenses included in the middle group GM is νM and a partial dispersion ratio thereof between the g line and the F line is θM, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (8). By satisfying Conditional Expression (8), it is easy to satisfactorily suppress fluctuation in secondary chromatic aberration due to the zooming. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (8-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (8-2).











-

0
.
0



2

<


θ

M

+


0
.
0


0

1

8
×
v

M

-


0
.
6


4

8

3

3


<
0.07




(
8
)







-
0.015

<


θ

M

+


0
.
0


0

1

8
×
v

M

-


0
.
6


4

8

3

3


<
0.065




(

8


-


1

)






0.02
<


θ

M

+


0
.
0


0

1

8
×
v

M

-


0
.
6


4

8

3

3


<


0
.
0


6





(

8


-


2

)







Since the middle group GM has a negative refractive power as a whole, the middle group GM includes one or more negative lenses. Among the negative lenses included in the middle group GM, assuming that a curvature radius of an image side surface of a negative lens closest to the object side in the middle group GM is RMnr, and a curvature radius of an object side surface of a lens disposed adjacent to the image side of a negative lens closest to the object side in the middle group GM is RMf, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (9). By not allowing the corresponding value of Conditional Expression (9) to be equal to or less than the lower limit, the refractive power of the negative lens closest to the object side in the middle group GM is prevented from becoming excessively strong. Therefore, it is easy to suppress fluctuations in various aberrations due to zooming. By not allowing the corresponding value of Conditional Expression (9) to be equal to or greater than the upper limit, the amount of movement of the middle group GM during changing magnification can be suppressed while maintaining a predetermined zoom magnification (that is, the magnification of the zooming). As a result, there is an advantage in achieving both reduction in size and an increase in magnification. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (9-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (9-2).










-

1
.
5


<


(

RMnr
+
RMf

)

/

(

RMnr
-
RMf

)


<
0.2




(
9
)







-
1

<


(

RMnr
+
RMf

)

/

(

RMnr
-
RMf

)


<
0.1




(

9


-


1

)







-

0
.
5


<


(

RMnr
+
RMf

)

/

(

RMnr
-
RMf

)


<

0.

0

5





(

9


-


2

)







Assuming that a difference in the optical axis direction between a position of a lens surface closest to the image side in the middle group GM at a wide angle end and a position of a lens surface closest to the image side in the middle group GM at a telephoto end in the state in which the infinite distance object is in focus is DpM, a focal length of the variable magnification optical system at a wide angle end in the state in which the infinite distance object is in focus is fw, a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, and a maximum image height is Ims, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (10). By not allowing the corresponding value of Conditional Expression (10) to be equal to or less than the lower limit, it is easy to satisfactorily suppress fluctuations in aberrations due to zooming. By not allowing the corresponding value of Conditional Expression (10) to be equal to or greater than the upper limit, there is an advantage in achieving both reduction in size and an increase in magnification. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (10-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (10-2).










0
.
2

<

DpM
/

{


(

f






t
/
fw


)

×
Ims

}


<
0.9




(
10
)






0.3
<

DpM
/

{


(

f


t
/
fw


)

×
Ims

}


<


0
.
8


5





(

10


-


1

)






0.45
<

DpM
/

{


(

f


t
/
fw


)

×
Ims

}


<
0.8




(

10


-


2

)







Assuming that an effective diameter of a lens surface closest to the object side in the middle group GM in the state in which the infinite distance object is in focus is EDMf, and an effective diameter of a lens surface closest to the image side in the middle group GM in the state in which the infinite distance object is in focus is EDMr, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (11). By not allowing the corresponding value of Conditional Expression (11) to be equal to or less than the lower limit, the negative refractive power acting on the off-axis luminous flux incident on the middle group GM is prevented from becoming excessively weak. Thus, there is an advantage in achieving reduction in size. By not allowing the corresponding value of Conditional Expression (11) to be equal to or greater than the upper limit, it is possible to suppress the amount of change in height of the ray from the optical axis Z in a case where the off-axis ray passes through the middle group GM. As a result, it is possible to suppress an increase in incidence angle of the off-axis luminous flux on the image plane Sim of the principal ray. Therefore, it is easy to ensure the amount of peripheral light. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (11-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (11-2).










0
.
5

<

E

DMf
/
EDMr

<

3
.25





(
11
)












0.6
<

E

DMf
/
EDMr

<
3




(

11
-
1

)












0.7
<

E

DMf
/
EDMr

<

2
.75





(

11
-
2

)







In the technique of the present disclosure, twice the distance to the optical axis Z from the intersection between the lens surface and the ray passing through the outermost side among rays incident onto the lens surface from the object side and emitted to the image side is the “effective diameter” of the lens surface. The “outside” here is the radial outside centered on the optical axis Z, that is, the side separated from the optical axis Z. In addition, the “ray passing through the outermost side” is determined in consideration of the entire area of zooming.


As an explanatory diagram, FIG. 3 shows an example of an effective diameter ED. In FIG. 3, the left side is the object side and the right side is the image side. FIG. 3 shows an on-axis luminous flux Xa and an off-axis luminous flux Xb passing through a lens Lx. In the example of FIG. 3, the ray Xb1, which is the upper ray of the off-axis luminous flux Xb, is the ray passing through the outermost side. Therefore, in the example of FIG. 3, twice the distance to the optical axis Z from the intersection between the ray Xb1 and the object side surface of the lens Lx is the effective diameter ED of the object side surface of the lens Lx. In FIG. 3, the upper ray of the off-axis luminous flux Xb is the ray passing through the outermost side, but which ray is the ray passing through the outermost side depends on the optical system.


It is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (12) for the on-axis marginal ray wa1 and the principal ray wb0 having the maximum image height Ims at the wide angle end in a state in which the infinite distance object is in focus. The symbols used in Conditional Expression (12) are shown in FIG. 4 as an example. FIG. 4 is a partially enlarged view of the middle group GM at the wide angle end of the variable magnification optical system of FIG. 1. HMfb is a height from the optical axis Z of the principal ray wb0 having the maximum image height Ims on the lens surface closest to the object side in the middle group GM at the wide angle end in the state in which the infinite distance object is in focus. HMfa is a height from the optical axis Z of the on-axis marginal ray wa1 on the lens surface closest to the object side in the middle group GM at the wide angle end in the state in which the infinite distance object is in focus. HMrb is a height from the optical axis Z of the principal ray wb0 of the maximum image height Ims on the lens surface closest to the image side in the middle group GM at the wide angle end in the state in which the infinite distance object is in focus. HMra is a height from the optical axis Z of the on-axis marginal ray wa1 on the lens surface closest to the image side in the middle group GM at the wide angle end in the state in which the infinite distance object is in focus. By not allowing the corresponding value of Conditional Expression (12) to be equal to or less than the lower limit, the negative refractive power acting on the off-axis luminous flux incident on the middle group GM is prevented from becoming excessively weak. Thus, there is an advantage in achieving reduction in size. By not allowing the corresponding value of Conditional Expression (12) to be equal to or greater than the upper limit, it is possible to suppress the amount of change in ray height in a case where the off-axis ray passes through the middle group GM. As a result, it is possible to suppress an increase in incidence angle of the off-axis luminous flux on the image plane Sim of the principal ray. Therefore, it is easy to ensure the amount of peripheral light. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (12-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (12-2).









1
<



(


HMfb
/

(

HMfb
/

(

HMrb
/
HMra

)





<
3







(
12
)






1.25
<




(

HMfb
/
HMfa

)

/

(

HMrb
/
HMra

)




<
2.75




(

12


-


1

)







1.5
<




(


HMfb
/

(
HMfa
)


/

(

HMrb
/
HMra

)




<
2.5





(

12


-


2

)







Further, it is preferable that the variable magnification optical system according to the embodiment of the present disclosure has the configuration described below.


Assuming that a maximum image height is Ims, and a focal length of the final lens group GE is fE, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (13). By not allowing the corresponding value of Conditional Expression (13) to be equal to or less than the lower limit, the positive refractive power of the final lens group GE is prevented from becoming excessively weak. Thus, there is an advantage in achieving reduction in size of the lens system. By not allowing the corresponding value of Conditional Expression (13) to be equal to or greater than the upper limit, the positive refractive power of the final lens group GE is prevented from becoming excessively strong. Therefore, it is easy to suppress fluctuations in various aberrations due to zooming. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (13-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (13-2).










0
.
1

<

Ims
/
fE

<
0.6




(
13
)












0.2
<

Ims
/
fE

<
0.5




(

13
-
1

)












0.25
<

Ims
/
fE

<
0.4




(

13
-
2

)







Assuming that an Abbe number of the positive lens having a largest Abbe number based on the d line among the positive lenses included in the final lens group GE is νE and a partial dispersion ratio thereof between the g line and the F line is θE, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (14). By satisfying Conditional Expression (14), there is an advantage in satisfactorily correcting secondary chromatic aberration in the entire region of zooming. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (14-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (14-2).











0
.
0


2

<


θ

E

+


0
.
0


0

1

8
×
v

E

-


0
.
6


4

8

3

3


<
0.08




(
14
)






0.025
<


θ

E

+


0
.
0


0

1

8
×
v

E

-


0
.
6


4

8

3

3


<
0.07




(

14


-


1

)






0.03
<


θ

E

+


0
.
0


0

1

8
×
v

E

-


0
.
6


4

8

3

3


<
0.06




(

14


-


2

)







The variable magnification optical system may be configured to include a group that performs focusing by moving along the optical axis Z (hereinafter, referred to as a focus group). That is, during the focusing, only the focus group moves along the optical axis Z. In a configuration in which the variable magnification optical system includes a focus group, assuming that a specific gravity of each lens in the focus group is Sgf and a refractive index thereof at the d line is Nf, an average value of Sgf/Nf of all lenses in the focus group is ave(Sgf/Nf), and a maximum value of refractive indexes of all the lenses in the focus group at the d line is Nfmax, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expressions (15) and (16). By not allowing the corresponding value of Conditional Expression (15) to be equal to or less than the lower limit, the refractive power of the focus group is prevented from becoming excessively strong. Therefore, it is easy to suppress the fluctuation in aberration due to focusing. By not allowing the corresponding value of Conditional Expression (15) to be equal to or greater than the upper limit, there is an advantage in reducing the weight of the focus group. By satisfying Conditional Expression (15) and not allowing the corresponding value of Conditional Expression (16) to be equal to or less than the lower limit, it is easy to reduce the weight of the focus group while the focus group has sufficient focusing ability. By satisfying Conditional Expression (15) and not allowing the corresponding value of Conditional Expression (16) to be equal to or greater than the upper limit, the refractive power of the focus group is prevented from becoming excessively strong. Therefore, it is easy to suppress the fluctuation in aberration due to focusing. Regarding the effect of the conditional expression (15), in order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (15-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (15-2). Regarding the effect of the conditional expression (16), in order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (16-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (16-2).











2
.
0


5

<

ave


(

S

g


f
/
Nf


)


<
2.55




(
15
)






2.1
<

ave


(

S

g


f
/
N


l

)


<
2.45




(

15


-


1

)






2.15
<

ave


(

S

g


f
/
N


l

)


<
2.35




(

15


-


2

)






1.7
<

N

f

max

<
2.2




(
16
)






1.75
<

N

f

max

<
2.1




(

16


-


1

)






1.8
<

N

f

max

<
2.05




(

16


-


2

)







The number of movable lens groups included in the variable magnification optical system may be three or more. Since there are provided three or more movable lens groups, there is an advantage in correcting spherical aberration and field curvature in each zooming state, and it is easy to increase the magnification.


Among the movable lens groups included in the variable magnification optical system, the movable lens group closest to the object side may be configured to have a positive refractive power. In such a case, there is an advantage in achieving reduction in size of the first lens group G1. Further, since there is an advantage in achieving reduction in size of the first lens group G1, there is an advantage in achieving reduction in effective diameter of the first lens group G1 in a case of trying to realize an optical system having a large aperture ratio.


The movable lens group closest to the object side may be configured to consist of one positive lens having a convex surface facing toward the object side. In such a case, there is an advantage in achieving reduction in size and weight.


In a configuration in which the movable lens group closest to the object side consists of one positive lens having a convex surface facing toward the object side, assuming that a curvature radius of an object side surface of the positive lens having the convex surface facing toward the object side is Rpf, and a curvature radius of an image side surface of the positive lens having the convex surface facing toward the object side is Rpr, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (17). By not allowing the corresponding value of Conditional Expression (17) to be equal to or less than the lower limit, the refractive power of this positive lens is prevented from becoming excessively strong. Therefore, it is easy to suppress fluctuations in various aberrations due to zooming. By not allowing the corresponding value of Conditional Expression (17) to be equal to or greater than the upper limit, the refractive power of this positive lens is prevented from becoming excessively weak. Therefore, the effect of aberration correction can be ensured. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (17-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (17-2).










-
6

<


(


R

p

f

-

R

p

r


)

/

(


R

p

f

+

R

p

r


)


<
1




(
17
)







-
3

<


(


R

p

f

-

R

p

r


)

/

(


R

p

f

+

R

p

r


)


<
0.75




(

17


-


1

)







-
1.5

<


(


R

p

f

-

R

p

r


)

/

(


R

p

f

+

R

p

r


)


<
0.5




(

17


-


2

)







The lens closest to the image side in the first lens group G1 has a convex object side surface, and may be configured such that the absolute value of the curvature radius of the image side surface is greater than the absolute value of the curvature radius of the object side surface. In such a case, it is easy to suppress fluctuation in astigmatism due to the zooming.


During changing magnification from the wide angle end to the telephoto end, it is preferable that the spacing between the first lens group G1 and the lens group closest to the object side in the plurality of lens groups increases. In such a case, it is easy to satisfactorily suppress fluctuations in various aberrations during changing magnification from the wide angle end to the telephoto end.


the first lens group G1 may be configured to consist of, in order from the object side to the image side, a first A subgroup G1A having a negative refractive power, a first B subgroup G1B having a positive refractive power, and a first C subgroup G1C having a positive refractive power. Then, the first B subgroup G1B may be configured to performing focusing by moving along the optical axis Z. That is, the first B subgroup G1B may be configured to be the focus group. In such a case, during focusing, the first B subgroup G1B moves along the optical axis Z, and the other groups remain stationary with respect to the image plane Sim. By adopting such a configuration, it is easy to suppress a change in angle of view due to focusing and fluctuations in various aberrations due to focusing due to a change in subject distance.


In the example of FIG. 1, the first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of two lenses L1g and L1h in order from the object side to the image side. The horizontal double-headed arrow below the first B subgroup G1B in FIG. 1 indicates that the first B subgroup G1B is the focus group.


In a case where the first lens group G1 consists of the first A subgroup G1A, the first B subgroup G1B, and the first C subgroup G1C, it is preferable that the variable magnification optical system according to the present embodiment satisfies at least one of Conditional Expressions (18) to (22).


Assuming that a maximum image height is Ims, and a focal length of the first C subgroup G1C is f1C, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (18). By not allowing the corresponding value of Conditional Expression (18) to be equal to or less than the lower limit, the refractive power of the first C subgroup G1C can be ensured. Therefore, particularly, it is possible to suppress insufficient correction of spherical aberration on the telephoto side. Further, it is possible to suppress an increase in size of the movable lens group closer to the image side than the first lens group G1. By not allowing the corresponding value of Conditional Expression (18) to be equal to or greater than the upper limit, the refractive power of the first C subgroup G1C is prevented from becoming excessively strong. Therefore, particularly, it is possible to suppress overcorrection of spherical aberration. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (18-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (18-2).











0
.
0


5

<

I

m


s
/
f






1





C

<
0.3




(
18
)






0.1
<


Ims
/
f






1

C

<
0.25




(

18


-


1

)






0.13
<

I

m


s
/
f






1

C

<
0.2




(

18


-


2

)







It is preferable that all the lenses included in the first C subgroup G1C have a positive refractive power. In such a case, the number of lenses can be minimized Therefore, the weight increase can be suppressed.


Assuming that a focal length of the first lens group G1 is f1, and a focal length of the first B subgroup G1B is f1B, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (19). By not allowing the corresponding value of Conditional Expression (19) to be equal to or less than the lower limit, the refractive power of the first B subgroup G1B is prevented from becoming excessively weak. Therefore, the amount of movement of the first B subgroup G1B during focusing can be suppressed. As a result, there is an advantage in achieving reduction in size. By not allowing the corresponding value of Conditional Expression (19) to be equal to or greater than the upper limit, the refractive power of the first B subgroup G1B is prevented from becoming excessively strong. Therefore, particularly, it is possible to suppress overcorrection of spherical aberration on the telephoto side. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (19-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (19-2).










0
.
3

<

f






1
/
f






1





B

<
0.9




(
19
)






0.4
<

f






1
/
f






1

B

<
0.8




(

19


-


1

)






0.5
<

f






1
/
f






1





B

<
0.7




(

19


-


2

)







The first B subgroup G1B has a positive refractive power, and thus includes one or more positive lenses. Assuming that an Abbe number of the positive lens, of which an Abbe number based on the d line is maximum, among the positive lenses included in the first B subgroup G1B based on the d line is ν1Bp, and a partial dispersion ratio thereof between a g line and an F line is θ1Bp, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (20). By satisfying Conditional Expression (20), it is easy to satisfactorily suppress fluctuation in secondary chromatic aberration due to focusing. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (20-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (20-2).











0
.
0


1

<


θ1





Bp

+

0.

0

0

1

8
×
v





1

B





p

-

0.6

4

8

3

3


<
0.07




(
20
)






0.02
<


θ1





Bp

+

0.0

0

1

8
×
v





1





Bp

-

0.

6

4

8

3

3


<
0.065




(

20


-


1

)






0.05
<


θ1





Bp

+

0.0

0

1

8
×
v





1

Bp

-

0.

6

4

8

3

3


<
0.06




(

20


-


2

)







In a configuration in which the first B subgroup G1B includes one or more negative lenses, assuming that a minimum value of the Abbe numbers of all the negative lenses included in the first B subgroup G1B based on the d line is ν1Bn, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (21). By satisfying Conditional Expression (21), it is easy to satisfactorily suppress fluctuations in axial chromatic aberration due to focusing. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (21-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (21-2).










1

5

<

v

1

Bn

<
40




(
21
)












20
<

v

1

Bn

<
35




(

21
-
1

)












23
<

v

1

Bn

<
30




(

21
-
2

)







In a configuration in which the first B subgroup G1B includes one or more positive lenses and one or more negative lenses, it is more preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expressions (20) and (21). Further, it is yet more preferable to satisfy not only Conditional Expressions (20) and (21) but also at least one of Conditional Expressions (20-1), (20-2), (21-1), or (21-2).


It is preferable that the first B subgroup G1B includes a meniscus-shaped negative lens having a convex surface facing toward the object side closest to the image side. In such a case, it is easy to suppress fluctuation in astigmatism due to focusing.


It is preferable that the first A subgroup G1A includes two or more negative lenses of which Abbe numbers based on the d line are 50 or more. Further, assuming that a minimum value of Abbe numbers of all the positive lenses included in the first A subgroup G1A based on the d line is ν1Ap, it is preferable that the variable magnification optical system according to the embodiment of the present disclosure satisfies Conditional Expression (22). By not allowing the corresponding value of Conditional Expression (22) to be equal to or less than the lower limit, it is possible to suppress overcorrection of axial chromatic aberration. By not allowing the corresponding value of Conditional Expression (22) to be equal to or greater than the upper limit, it is easy to correct axial chromatic aberration. In a case where the first A subgroup G1A includes two or more negative lenses of which Abbe numbers based on the d line are 50 or more and satisfies Conditional Expression (22), it is easy to satisfactorily correct axial chromatic aberration. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (22-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (22-2).










1

5

<

v

1

Ap

<
40




(
22
)












20
<

v

1

Ap

<
35




(

22
-
1

)












23
<

v

1

Ap

<
30




(

22
-
2

)







The first lens group G1 may be configured to be remaining stationary with respect to the image plane Sim during changing magnification. In such a case, it is easy to configure the lens system such that the total length of the lens system does not change even in a case where zooming is performed. According to this configuration, it is easy to reduce fluctuation in centroid of the lens system during changing magnification. Thus, there is an advantage in improving the convenience during imaging.


The final lens group GE may be remaining stationary with respect to the image plane Sim during changing magnification, and the aperture stop St may be disposed closest to the object side in the final lens group GE. In such a case, it is easy to suppress fluctuation in F number due to the zooming. In addition, there is an advantage in suppressing fluctuation in field curvature and fluctuation in spherical aberration due to zooming.


In a case where the aperture stop St is disposed closest to the object side in the final lens group GE, it is preferable that the lens component disposed adjacent to the image side of the aperture stop St has a biconvex shape. In such a case, there is an advantage in satisfactorily correcting the spherical aberration. In addition, in the present specification, one lens component means one single lens or one group of cemented lenses. In the example of FIG. 1, the lens component disposed adjacent to the image side of the aperture stop St is a cemented lens consisting of the lens L5a and the lens L5b.


In a case where the aperture stop St is disposed closest to the object side in the final lens group GE, assuming that a curvature radius of a surface of the lens component, which is closest to the object side and is disposed adjacent to the image side of the aperture stop St, is REf, and a curvature radius of a surface of the lens component, which is closest to the image side and is disposed adjacent to the image side of the aperture stop St, is REr, it is preferable that the variable magnification optical system according to the present embodiment satisfies Conditional Expression (23). By not allowing the corresponding value of Conditional Expression (23) to be equal to or less than the lower limit, there is an advantage in achieving reduction in size. By not allowing the corresponding value of Conditional Expression (23) to be equal to or greater than the upper limit, there is an advantage in satisfactorily correcting the spherical aberration in the entire region of the zooming. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (23-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (23-2).










-

0
.
7


<


(


R

E

f

+

R

Er


)

/

(

REf
-

R

E

r


)


<
0.7




(
23
)














-
0.5


5

<


(


R

E

f

+

R

Er


)

/

(

REf
-

R

E

r


)


<
0.55




(

23
-
1

)













-
0.45

<


(


R

E

f

+

R

Er


)

/

(

REf
-

R

E

r


)


<

0
.45





(

23
-
2

)







It is preferable that the final lens group GE includes one or more lenses of which Abbe numbers based on the d line are 65 or more and which satisfies Conditional Expression (24). In Conditional Expression (24), it is assumed that a temperature coefficient of a relative refractive index of a lens in the final lens group GE at the d line in a range of 20° C. to 40° C. is dN/dT and a unit of dN/dT is ° C.−1. The final lens group GE having a positive refractive power tends to use a material having low dispersion and abnormal dispersibility as a material for a positive lens in order to correct chromatic aberration. However, many such materials each have a negative temperature coefficient. By not allowing the corresponding value of Conditional Expression (24) to be equal to or less than the lower limit, a positive lens using a material having a positive temperature coefficient can be disposed in the final lens group GE, which is caused by a temperature change. Therefore, it is easy to satisfactorily correct fluctuation in image formation position. By not allowing the corresponding value of Conditional Expression (24) to be equal to or greater than the upper limit, it is possible to prevent the correction amount for suppressing fluctuation in image formation position from becoming excessive. In order to obtain more favorable characteristics, it is more preferable that the variable magnification optical system satisfies Conditional Expression (24-1), and it is yet more preferable that the variable magnification optical system satisfies Conditional Expression (24-2).









0
<

d


N
/
d


T

<

8
×
1


0

-
6







(
24
)







1.5
×
1


0

-
6



<

d


N
/
d


T

<

7
×
1


0

-
6







(

24


-


1

)







3
×
1


0

-
6



<

d


N
/
d


T

<

6
×
1


0

-
6







(

24


-


2

)







The example shown in FIG. 1 is an example, and various modifications can be made without departing from the scope of the technology of the present disclosure. For example, the number of the plurality of lens groups disposed between the first lens group G1 and the final lens group GE, the number of lens groups included in the middle group GM, the number of movable lens groups included in the middle group GM, and the number of lenses included in each lens group may be different from the numbers shown in FIG. 1.


Specifically, for example, groups, which are included in the plurality of lens groups disposed between the first lens group G1 and the final lens group GE and move by changing the spacing between adjacent lens groups during changing magnification, may be configured to consist of, in order from the object side to the image side, an middle group GM, a negative movable lens group GN, and a positive movable lens group having a positive refractive power. The middle group GM is a group including one or more lens groups and having a negative refractive power as a whole. The negative movable lens group GN is a lens group having a negative refractive power positioned closest to the image side among the lens groups having a negative refractive power in the plurality of lens groups, and is a lens group that moves during changing magnification. In such a case, it is easy to satisfactorily suppress fluctuations in various aberrations due to zooming.


Further, the middle group GM may be configured to consist of, in order from the object side to the image side, a front lens group having a positive refractive power, a central lens group having a negative refractive power, and a rear lens group having a negative refractive power. The middle group GM may be configured such that, during changing magnification, the spacing between the front lens group and the central lens group may change, and the spacing between the central lens group and the rear lens group may change. In such a case, it is easy to satisfactorily suppress fluctuations in various aberrations due to zooming.


Alternatively, the middle group GM may be configured to consist of only one lens group having a negative refractive power.


More specifically, each lens group can have, for example, the following configuration.


The first A subgroup G1A can be configured to consist of three lenses. The first A subgroup G1A may be configured to consist of two negative lenses and one positive lens in order from the object side to the image side. Alternatively, the first A subgroup G1A may be configured to consist of one negative lens, one positive lens, and one negative lens in order from the object side to the image side.


Alternatively, the first A subgroup G1A can be configured to consist of four lenses. In such a case, the first A subgroup G1A may be configured to consist of three negative lenses and one positive lens in order from the object side to the image side.


The first B subgroup G1B can be configured to consist of three lenses. In such a case, the first B subgroup G1B may be configured to consist of two positive lenses and one negative lens in order from the object side to the image side.


The first B subgroup G1B can be configured to consist of four lenses. In such a case, the first B subgroup G1B may be configured to consist of three positive lenses and one negative lens in order from the object side to the image side.


The first C subgroup G1C can be configured to consist of two or three lenses. In such a case, the first C subgroup G1C may be configured to consist of two or three positive lenses.


In a case where the middle group GM consists of the front lens group and the rear lens group described above, the middle group GM can be configured as follows. The front lens group can be configured to consist of one positive lens. Alternatively, the front lens group can be configured to consist of one negative lens and one positive lens. In such a case, the front lens group may be configured to consist of one group of cemented lenses. The rear lens group can be configured to consist of eight lenses. In such a case, the rear lens group may be configured to consist of five negative lenses and three positive lenses. Alternatively, the rear lens group can be configured to consist of seven lenses. In such a case, the rear lens group may be configured to consist of four negative lenses and three positive lenses, or may be configured to consist of five negative lenses and two positive lenses. Alternatively, the rear lens group can be configured to consist of six lenses. In such a case, the rear lens group may be configured to consist of three negative lenses and three positive lenses, or may be configured to consist of four negative lenses and two positive lenses.


In a case where the middle group GM consists of the front lens group, the central lens group, and the rear lens group, the middle group GM can be configured as follows. The front lens group can be configured to consist of one positive lens. The central lens group can be configured to consist of four lenses. In this case, the central lens group may be configured to consist of three negative lenses and one positive lens. The rear lens group can be configured to consist of three lenses. In this case, the rear lens group may be configured to consist of one negative lens and two positive lenses.


In a case where the middle group GM consists of only one lens group, the middle group GM can be configured as follows. The middle group GM can be configured to consist of six lenses. In such a case, the middle group GM may be configured to consist of four negative lenses and two positive lenses. Alternatively, the middle group GM can be configured to consist of seven lenses. In such a case, the middle group GM may be configured to consist of four negative lenses and three positive lenses.


The negative movable lens group GN can be configured to consist of two lenses. In such a case, the negative movable lens group GN may be configured to consist of one negative lens and one positive lens. The negative movable lens group GN may be configured to consist of one group of cemented lenses or may be configured to consist of two single lenses.


The positive movable lens group can be configured to consist of three lenses. In this case, the positive movable lens group may be configured to consist of two positive lenses and one negative lens.


The variable magnification optical system of the present disclosure may be a zoom lens or a varifocal lens.


The above-mentioned preferred configurations and available configurations including the configurations relating to Conditional Expressions may be any combination, and it is preferable to appropriately selectively adopt the configurations in accordance with required specification. It should be noted that the ranges of the possible conditional expressions are not limited to the conditional expressions described in the form of the expression, and the lower limit and the upper limit are selected from each of the preferable, more preferable, and yet more preferable conditional expressions. The ranges of the conditional expressions include ranges obtained through optional combinations.


Next, examples of the variable magnification optical system of the present disclosure will be described. The reference numerals attached to the lenses in the cross-sectional views of each example are used independently for each example in order to avoid complication of description and drawings due to an increase in the number of digits of the reference numerals. Therefore, even in a case where common reference numerals are attached in the drawings of different examples, components do not necessarily have a common configuration.


Example 1

The configuration and movement loci of the variable magnification optical system according to Example 1 are shown in FIG. 1, and the illustration method and configuration thereof are as described above, and thus, repeated description will be omitted.


Regarding the variable magnification optical system of Example 1, Tables 1A and 1B show basic lens data, Table 2 shows specification and variable surface spacings, and Table 3 shows aspherical coefficients. Here, the basic lens data is divided into two tables, Table 1A and Table 1B, in order to avoid lengthening of one table. Tables 1A, 1B, and 2 show data in a state in which the infinite distance object is in focus.


Tables 1A and 1B are described as follows. The column of Sn shows surface numbers in a case where the surface closest to the object side is the first surface and the number is increased one by one toward the image side. The column of R shows a curvature radius of each surface. The column of D shows a surface spacing between each surface and the surface adjacent to the image side on the optical axis. The column of Nd shows a refractive index of each constituent element at the d line. The column of νd shows an Abbe number of each constituent element based on the d line. The column of θgF shows a partial dispersion ratio of each constituent element between the g line and the F line. The column of ED shows an effective diameter at the diameter of each surface. The column of Sg shows a specific gravity of each constituent element. The specific gravity shows only the first lens group G1.


In Tables 1A and 1B, the sign of the curvature radius of the surface having a convex surface facing toward the object side is positive and the sign of the curvature radius of the surface having a convex surface facing toward the image side is negative. In Table 1B, in a place of a surface number of a surface corresponding to the aperture stop St, the surface number and a term of (St) are noted. Table 1B also shows the optical member PP. A value at the bottom place of the column of D in Table 1B indicates a spacing between the image plane Sim and the surface closest to the image side in the table. In Table 1A, the symbol DD[ ] is used for each variable surface spacing during changing magnification, and the object side surface number of the spacing is given in [ ] and is noted in the column of D.


Table 2 shows the zoom magnification Zr, the focal length f, the back focal length Bf at the air conversion distance, the open F number FNo., the maximum total angle of view 2ω, the maximum image height Ims, and the variable surface spacing during changing magnification, based on the d line. In a case where the variable magnification optical system is a zoom lens, the zoom magnification is synonymous with the zoom ratio. (°) in the place of 2ω indicates that the unit thereof is a degree. In Table 2, the columns of WIDE, MIDDLE, and TELE show values in the wide angle end state, the middle focal length state, and the telephoto end state, respectively.


In basic lens data, the reference sign * is attached to surface numbers of aspherical surfaces, and numerical values of the paraxial curvature radius are written into the column of the curvature radius of the aspherical surface. In Table 3, the row of Sn shows surface numbers of the aspherical surfaces, and the rows of KA and Am show numerical values of the aspherical coefficients for each aspherical surface. It should be noted that m of Am is an integer of 3 or more, and differs depending on the surface. For example, on the first surface, m=3, 4, 5, . . . , 20. The “E±n” (n: an integer) in numerical values of the aspherical coefficients of Table 3 indicates “×10±n”. KA and Am are the aspherical coefficients in the aspheric equation represented by the following expression.







Z

d

=


C
×


h
2

/

{

1
+


(

1
-

KA
×

C
2

×

h
2



)


1
/
2



}



+

Σ

A

m
×

h
m







Here,


Zd is an aspherical surface depth (a length of a perpendicular from a point on an aspherical surface at height h to a plane that is perpendicular to the optical axis Z in contact with the vertex of the aspherical surface),


h is a height (a distance from the optical axis Z to the lens surface),


C is an inverse of the paraxial curvature radius,


KA and Am are aspherical coefficients, and


Σ in the aspheric equation means the sum with respect to m.


In data of each table, a degree is used as a unit of an angle, and mm (millimeter) is used as a unit of a length, but appropriate different units may be used since the optical system can be used even in a case where the system is enlarged or reduced in proportion. Further, each of the following tables shows numerical values rounded off to predetermined decimal places.









TABLE 1A







Example 1














Sn
R
D
Nd
νd
θgF
ED
Sg

















*1
19966.75539
4.400
1.73316
54.68
0.54436
146.17
4.13


2
256.96189
16.939



139.16


3
−385.40577
3.419
1.78403
49.60
0.55166
138.65
4.38


4
225.21207
9.401
1.84666
23.83
0.61603
138.14
5.51


5
773.30724
1.637



138.07


6
544.99170
16.600
1.50614
81.58
0.53913
138.27
3.56


7
−235.89997
0.199



138.20


8
138.37249
17.351
1.43875
94.66
0.53402
140.50
3.59


9
664.41960
0.201



140.00


10
181.53334
4.300
1.85478
24.80
0.61232
138.38
3.49


11
120.21551
43.844



133.43


12
137.33199
20.000
1.43875
94.66
0.53402
141.93
3.59


13
1457.05292
0.120



141.50


*14
152.38909
18.500
1.49700
81.54
0.53748
138.45
3.62


15
−2660.64421
DD[15]



137.44


*16
144.32402
3.974
1.43875
94.66
0.53402
85.78


17
204.56938
DD[17]



84.09


18
4016.52155
1.500
1.91171
36.83
0.57843
49.74


19
63.89848
6.659



46.87


20
−169.93294
1.984
1.59282
68.62
0.54414
46.74


21
130.63810
4.324



46.52


22
−143.84388
1.981
1.68344
57.33
0.54263
46.57


23
119.65744
7.095
1.70112
33.73
0.59318
47.99


24
−289.75477
2.340



48.79


25
−539.00664
2.020
1.58894
61.02
0.54280
49.49


26
245.56024
4.707
1.62898
35.10
0.58644
50.24


27
−269.21774
13.401



50.74


28
179.96575
9.820
1.68893
51.22
0.55235
55.89


29
−109.66190
1.510
1.53476
77.27
0.54055
56.09


30
1153.79118
DD[30]



56.10


31
−79.79343
1.300
1.49700
81.64
0.53714
56.45


32
227.23675
0.213



58.67


33
250.06516
2.500
1.84666
23.83
0.61603
58.69


34
1037.07126
DD[34]



58.90
















TABLE 1B







Example 1













Sn
R
D
Nd
νd
θgF
ED
















35(St)

1.969



59.73


36
258.55091
12.437
1.59504
61.34
0.54252
61.16


37
−58.20553
1.649
1.78748
47.99
0.55522
61.43


38
−111.36299
2.799



62.93


39
54.99693
19.647
1.53775
74.70
0.53936
62.88


40
−70.31665
1.388
1.54072
47.23
0.56511
61.63


41
−706.85120
7.045



58.00


42
46.02808
11.733
1.43875
94.66
0.53402
46.82


43
−83.26502
1.300
1.95375
32.32
0.59015
44.76


44
82.42912
4.998



41.61


45
−102.20122
5.623
1.84666
23.83
0.61603
41.53


46
−37.86090
1.410
1.76612
47.61
0.55688
41.52


47
−71.81824
19.232



41.20


48
40.85242
6.953
1.43875
94.66
0.53402
33.14


49
−81.00907
0.879



32.26


50
−88.48926
1.000
1.95375
32.32
0.59015
31.17


51
22.77130
8.404
1.60517
37.48
0.58160
29.17


52
−119.20658
1.675



29.24


53
−77.87165
4.552
1.52637
50.06
0.55898
29.12


54
−27.08668
0.900
1.84850
43.79
0.56197
29.23


55
95.16631
6.969



30.96


56
82.92367
4.773
1.80518
25.46
0.61572
37.78


57
−144.06667
45.091



38.07


58

4.150
1.51633
64.14


59

2.014
















TABLE 2







Example 1













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
50.018
152.397
385.642



Bf
49.842
49.842
49.842



FNo.
3.30
3.30
3.30



2ω(°)
50.2
16.8
6.8



Ims
23.4
23.4
23.4



DD[15]
1.470
22.522
69.501



DD[17]
3.399
59.638
51.984



DD[30]
85.932
14.049
18.085



DD[34]
51.349
45.940
2.580

















TABLE 3







Example 1










Sn
1
14
16





KA
1.0000000E+00
1.0000000E+00
1.0000000E+00


A3
−5.3857896E−09 
0.0000000E+00
1.7256063E−07


A4
1.1315386E−08
−5.4182092E−08 
1.2726346E−08


A5
1.8930570E−11
2.9141317E−10
7.5368315E−11


A6
1.7729498E−13
−1.1920877E−11 
1.6209835E−11


A7
−1.3582473E−14 
1.1786770E−13
−1.2891196E−13 


A8
−9.5033792E−17 
3.8936267E−16
−1.1200960E−14 


A9
9.3573784E−19
−1.1326430E−17 
6.0527364E−17


A10
1.1949393E−20
−9.5068469E−20 
2.9868130E−18


A11
−5.7431595E−23 
2.6816889E−22
4.8256342E−20


A12
2.4895462E−24
1.0744516E−23
4.2089104E−22


A13
1.0131116E−27
1.1132978E−25
−2.4606332E−24 


A14
−4.8777903E−28 
4.6458610E−28
−8.9024330E−25 


A15
7.0220562E−30
−5.4333594E−30 
−1.8662042E−26 


A16
−3.7920649E−33 
−1.4005746E−31 
6.4480795E−29


A17
1.3449455E−34
−1.5785270E−33 
7.0738863E−30


A18
−1.5602557E−35 
−1.8852320E−35 
1.1599279E−31


A19
−4.1366483E−37 
1.3050375E−38
2.7652334E−33


A20
5.9333966E−39
4.7589070E−39
−9.2994676E−35 










FIG. 5 shows a diagram of aberrations of the variable magnification optical system of Example 1 in a state in which the infinite distance object is in focus. FIG. 5 shows, in order from the left, spherical aberration, astigmatism, distortion, and lateral chromatic aberration. In FIG. 5, the upper part labeled by “WIDE” shows aberrations in the wide angle end state, the middle part labeled by “MIDDLE” shows aberrations in the middle focal length state, and the lower part labeled by “TELE” shows aberrations in the telephoto end state. In spherical aberration diagram, aberrations at the d line, the C line, the F line, and the g line are indicated by the solid line, the long broken line, the short broken line, and the two-dot chain line, respectively. In the astigmatism diagram, aberration in the sagittal direction at the d line is indicated by the solid line, and aberration in the tangential direction at the d line is indicated by the short broken line. In the distortion diagram, aberration at the d line is indicated by the solid line. In lateral chromatic aberration diagram, aberrations at the C line, the F line, and the g line are respectively indicated by the long broken line, the short broken line, and the two-dot chain line. In the spherical aberration diagram, the value of the open F number is shown after FNo.=. In other aberration diagrams, the value of the maximum half angle of view is shown after ω=.


Symbols, meanings, description methods, and illustration methods of the respective data pieces according to Example 1 are the same as those in the following examples unless otherwise specified. Therefore, in the following description, repeated description will be omitted.


Example 2


FIG. 6 shows a configuration and movement loci of the variable magnification optical system of Example 2. The variable magnification optical system of Example 2 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a positive refractive power, a fifth lens group G5 having a negative refractive power, and a sixth lens group G6 having a positive refractive power.


During changing magnification, the first lens group G1 and the sixth lens group G6 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, the fourth lens group G4, and the fifth lens group G5 move along the optical axis Z by changing the spacings from the adjacent lens groups. The middle group GM consists of the second lens group G2, the third lens group G3, and the fourth lens group G4. The negative movable lens group GN consists of a fifth lens group G5.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of four lenses L3a to L3d in order from the object side to the image side. The fourth lens group G4 consists of three lenses L4a to L4c in order from the object side to the image side. The fifth lens group G5 consists of two lenses L5a and L5b in order from the object side to the image side. The sixth lens group G6 consists of an aperture stop St and fourteen lenses L6a to L6n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 2, Tables 4A and 4B show the basic lens data, Table 5 shows the specifications and the variable surface spacings, Table 6 shows the aspherical coefficients, and FIG. 7 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 4A







Example 2














Sn
R
D
Nd
νd
θgF
ED
Sg

















*1
19988.03274
4.500
1.72916
54.68
0.54451
147.62
4.18


2
172.27220
1.216



147.00


3
173.57490
9.399
1.84666
23.84
0.62012
137.42
3.50


4
358.26008
12.949 



137.26


5
−378.60416
4.100
1.77250
49.62
0.55188
136.41
4.26


6
345.78380
7.946



136.29


7
1435.89354
13.739 
1.49700
81.64
0.53714
134.14
3.65


8
−222.05319
0.120



134.36


9
173.39471
17.558 
1.43875
94.66
0.53402
134.40
3.59


10
−1349.98175
0.120



136.38


11
224.59749
3.800
1.84666
23.84
0.62012
136.02
3.50


12
142.86358
43.675 



135.34


13
187.01575
19.199 
1.43875
94.66
0.53402
132.31
3.59


14
−963.84820
0.120



144.81


15
192.35345
12.660 
1.49700
81.64
0.53714
144.71
3.65


16
905.89200
0.120



142.32


17
115.33356
12.095 
1.49700
81.64
0.53714
141.69
3.65


18
208.41559
DD[18]



133.22


*19
133.14797
4.000
1.49700
81.64
0.53714
131.99


20
234.14102
DD[20]



64.76


21
2780.66501
1.500
1.90043
37.37
0.57668
63.20


22
56.78262
5.314



47.41


23
−429.01422
1.500
1.77250
49.62
0.55188
44.35


24
255.33442
6.572



44.31


25
−63.14256
1.444
1.84850
43.79
0.56197
44.25


26
431.97027
5.719
1.80518
25.43
0.61027
46.81


27
−98.69530
DD[27]



46.82


28
−96.54800
1.651
1.62846
59.17
0.55583
47.69


29
−220.02181
4.269
1.61266
44.46
0.56403
54.99


30
−83.50066
6.635



54.99


31
300.66861
4.500
1.74400
44.90
0.56308
55.52


32
−335.97977
DD[32]



58.94


33
−67.54701
1.671
1.43875
94.66
0.53402
59.04


34
220.65719
2.562
1.80518
25.43
0.61027
61.69


35
1054.77979
DD[35]



61.69
















TABLE 4B







Example 2













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.990



61.83


37
195.66024
13.008
1.55397
71.76
0.53931
62.65


38
−64.96103
1.650
1.81600
46.59
0.55661
64.41


39
−121.38468
2.800



64.41


40
57.19756
14.999
1.53775
74.70
0.53936
65.77


41
−190.00256
1.670
1.54072
47.23
0.56511
64.53


42
1604.41721
10.337



64.52


43
54.77964
10.145
1.49700
81.64
0.53714
62.29


44
−97.71354
1.300
1.90043
37.37
0.57668
49.83


45
85.41346
6.682



49.82


46
−172.36448
4.081
1.80518
25.43
0.61027
46.06


47
−61.22649
1.231
1.53775
74.70
0.53936
45.06


48
−95.77163
16.656



45.06


49
49.27767
7.738
1.43875
94.66
0.53402
44.25


50
−58.57296
1.000
1.90043
37.37
0.57668
33.64


51
26.58530
7.648
1.58144
40.98
0.57640
31.65


52
−259.96209
3.527



31.65


53
−58.50509
4.010
1.58313
59.37
0.54345
31.69


54
−30.24183
0.900
1.88300
40.69
0.56730
31.89


55
−270.81550
9.601



31.89


56
632.93983
3.737
1.80518
25.43
0.61027
33.55


57
−92.33303
57.093



39.10


58

4.150
1.51633
64.14


59

1.000
















TABLE 5







Example 2













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
50.014
152.384
385.608



Bf
60.830
60.830
60.830



FNo.
3.30
3.30
3.30



2ω(°)
50.2
16.8
6.8



Ims
23.4
23.4
23.4



DD[18]
1.401
61.013
112.889



DD[20]
1.671
18.471
1.771



DD[27]
17.660
18.342
17.931



DD[32]
72.888
9.241
25.734



DD[35]
67.324
53.877
2.620

















TABLE 6







Example 2











Sn
1
19







KA
1.0000000E+00
1.0000000E+00



A3
−5.3857896E−09 
1.7256063E−07



A4
1.6400269E−08
1.0893109E−07



A5
2.3508237E−10
1.0971148E−09



A6
−1.5235911E−11 
5.6637554E−11



A7
4.9670252E−13
−2.2920563E−12 



A8
−7.6409319E−15 
−1.9202370E−14 



A9
3.1570719E−17
4.7260463E−16



A10
3.4461939E−19
6.6562681E−18



A11
−7.7681344E−22 
2.1540998E−18



A12
−1.1578351E−23 
2.7181607E−20



A13
−2.8382718E−25 
−9.5470802E−22 



A14
4.5952417E−28
−7.4604126E−23 



A15
−2.5573237E−29 
−1.0282561E−24 



A16
2.4594128E−31
−1.5620019E−26 



A17
1.8989264E−33
2.8630617E−27



A18
1.0526064E−34
1.9178263E−29



A19
−3.8125305E−37 
2.2155451E−32



A20
−8.7483555E−39 
−3.1766565E−32 










Example 3


FIG. 8 shows a configuration and movement loci of the variable magnification optical system of Example 3. The variable magnification optical system in Example 3 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of two lenses L1g and L1h in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of eight lenses L3a to L3h in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 3, Tables 7A and 7B show the basic lens data, Table 8 shows the specifications and the variable surface spacings, Table 9 shows the aspherical coefficients, and FIG. 9 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 7A







Example 3














Sn
R
D
Nd
vd
θgF
ED
Sg

















*1
19271.78853
4.400
1.72916
54.09
0.54490
147.35
3.98


 2
252.10525
17.839



147.00



 3
−353.06322
3.419
1.76804
51.69
0.54848
139.84
4.28


 4
249.21816
8.920
1.84666
23.83
0.61603
138.34
5.51


 5
960.99204
1.480



138.34



 6
540.48281
16.420
1.50945
81.08
0.53930
138.29
3.56


 7
−241.75010
0.199



138.51



 8
140.62658
17.342
1.43875
94.66
0.53402
138.43
3.59


 9
731.45411
0.200



140.53



10
186.94200
4.299
1.85478
24.80
0.61232
140.00
3.49


11
122.10150
44.236



138.34



12
136.76463
20.001
1.43875
94.66
0.53402
133.47
3.59


13
1379.24472
0.119



141.94



*14 
151.90029
18.500
1.49700
81.54
0.53748
142.00
3.62


15
−2373.89846
DD[15]



138.41



*16 
141.15697
3.326
1.43875
94.66
0.53402
137.43



17
173.08616
DD[17]



88.15



18
882.03281
1.500
1.90043
37.37
0.57668
86.59



19
61.62679
7.548



51.07



20
−144.69746
1.964
1.59282
68.62
0.54414
48.00



21
127.82290
4.607



47.85



22
−159.27544
1.957
1.63153
59.92
0.54308
47.75



23
233.97006
5.977
1.73800
32.26
0.58953
49.09



24
−223.32010
1.830



49.09



25
−310.24481
2.000
1.52841
76.45
0.53954
49.80



26
129.73970
6.253
1.55345
45.09
0.56984
51.33



27
−249.65422
12.737



51.33



28
149.96629
9.528
1.60342
54.02
0.55040
51.75



29
−87.74754
1.510
1.52841
76.45
0.53954
55.81



30
1059.63429
DD[30]



55.81



31
−78.11539
1.300
1.49700
81.64
0.53714
55.82



32
222.92065
0.218



56.30



33
253.65662
2.499
1.84666
23.83
0.61603
58.61



34
1707.86188
DD[34]



58.60

















TABLE 7B







Example 3













Sn
R
D
Nd
νd
θgF
ED
















35(St)

1.970



58.79


36
254.22704
12.360
1.59410
60.47
0.55516
59.79


37
−58.35769
1.650
1.80577
43.86
0.56366
61.46


38
−108.61656
2.800



61.46


39
55.37270
20.001
1.53775
74.70
0.53936
62.96


40
−73.49141
1.377
1.54072
47.23
0.56511
61.10


41
−628.54906
6.567



61.09


42
46.39609
11.611
1.43875
94.66
0.53402
57.70


43
−84.14447
1.300
1.95375
32.32
0.59015
44.78


44
84.64250
4.978



44.77


45
−99.79374
5.001
1.84666
23.83
0.61603
41.64


46
−39.83899
1.410
1.75118
52.88
0.54695
41.55


47
−72.59238
20.191



41.55


48
42.22067
6.335
1.43875
94.66
0.53402
41.20


49
−82.33364
1.388



32.83


50
−86.04543
1.000
1.95375
32.32
0.59015
32.15


51
22.26164
7.667
1.59321
38.68
0.58204
28.73


52
−121.83579
1.442



28.73


53
−80.07575
4.511
1.55117
45.40
0.56927
28.83


54
−26.36830
0.900
1.84850
43.79
0.56197
28.95


55
94.56389
5.914



28.95


56
78.49034
4.398
1.80518
25.46
0.61572
30.82


57
−138.63520
44.999



37.13


58

4.150
1.51633
64.14


59

2.001
















TABLE 8







Example 3













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
50.001
152.343
385.504



Bf
49.737
49.737
49.737



FNo.
3.30
3.30
3.31



2ω(°)
50.2
16.8
6.8



Ims
23.4
23.4
23.4



DD[15]
1.466
26.102
64.416



DD[17]
3.466
58.858
57.105



DD[30]
89.216
13.333
21.241



DD[34]
50.973
46.829
2.359

















TABLE 9







Example 3










Sn
1
14
16





KA
1.0000000E+00
1.0000000E+00
1.0000000E+00


A3
−5.3857896E−09 
0.0000000E+00
1.7256063E−07


A4
8.6613357E−09
−5.6436664E−08 
1.1522478E−08


A5
4.8145204E−11
3.1182995E−10
6.5602143E−11


A6
−6.2326937E−15 
−1.2523650E−11 
1.6451849E−11


A7
−1.0869750E−14 
1.1451718E−13
−1.2838540E−13 


A8
−1.6426134E−16 
5.1308507E−16
−1.1170168E−14 


A9
1.4781502E−18
−1.2034245E−17 
6.2369017E−17


A10
2.2111089E−20
−9.1379324E−20 
2.9484419E−18


A11
−9.3150872E−23 
1.8999198E−22
5.1239276E−20


A12
1.9426906E−25
1.0561860E−23
4.4926424E−22


A13
2.3760241E−26
1.1613112E−25
−2.5001949E−24 


A14
−1.0533093E−27 
4.7242666E−28
−9.6227948E−25 


A15
6.8200149E−30
−4.2683902E−30 
−1.7801159E−26 


A16
3.7900040E−32
−1.3658557E−31 
5.2905524E−29


A17
1.5826565E−35
−1.5120340E−33 
6.6013263E−30


A18
8.0390213E−37
−2.0075291E−35 
1.1849862E−31


A19
−1.9500130E−37 
−8.5478889E−39 
2.7764059E−33


A20
1.5764736E−39
4.6940535E−39
−8.7655507E−35 









Example 4

The configuration and movement loci of the variable magnification optical system of Example 4 are shown in FIG. 10. The variable magnification optical system in Example 4 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 4, Tables 10A and 10B show the basic lens data, Table 11 shows the specifications and the variable surface spacings, Table 12 shows the aspherical coefficients, and FIG. 11 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 10A







Example 4














Sn
R
D
Nd
vd
θgF
ED
Sg

















*1
20015.99317
4.500
1.72916
54.68
0.54451
147.26
4.18


 2
278.88173
17.371



147.00



 3
−336.90848
4.120
1.77250
49.62
0.55188
140.34
4.26


 4
231.89924
9.383
1.84666
23.78
0.61923
138.14
3.50


 5
831.17307
3.394



138.14



 6
976.94620
14.693
1.59282
68.62
0.54414
138.07
4.13


 7
−233.57946
0.119



138.28



 8
160.27416
17.350
1.43875
94.66
0.53402
138.27
3.59


 9
3512.68676
0.119



140.43



10
255.67430
3.800
1.84666
23.78
0.61923
140.00
3.50


11
143.06427
46.801



138.54



12
191.98920
18.281
1.43875
94.66
0.53402
134.73
3.59


13
−915.96649
0.120



142.21



14
183.22841
11.298
1.55032
75.50
0.54001
142.00
4.09


15
573.33724
0.300



139.32



16
113.82582
11.947
1.49700
81.64
0.53714
138.64
3.65


17
207.66957
DD[17]



130.75



*18 
138.05623
4.037
1.43875
94.66
0.53402
129.50



19
265.27876
DD[19]



64.62



20
837.50172
1.500
1.90043
37.37
0.57668
63.07



21
56.89286
5.456



48.20



22
−426.91477
1.499
1.69560
59.05
0.54348
44.95



23
132.20113
6.002



44.88



24
−69.92114
1.996
1.88300
40.69
0.56730
44.34



25
511.90677
5.675
1.67270
32.21
0.59190
46.43



26
−102.13627
1.816



46.44



27
−115.08883
2.015
1.61720
53.97
0.55033
47.48



28
−186.58078
4.249
1.62004
36.37
0.58282
49.59



29
−84.73004
18.131



49.60



30
258.26706
4.475
1.78880
28.43
0.60092
50.47



31
−373.84758
DD[31]



57.71



32
−68.46537
1.320
1.43875
94.66
0.53402
57.83



33
240.13920
3.472
1.80518
25.43
0.61027
60.55



34
1893.01324
DD[34]



60.55

















TABLE 10B







Example 4













Sn
R
D
Nd
νd
θgF
ED
















35(St)

1.991



60.86


36
246.08533
13.478
1.59349
67.00
0.53667
61.68


37
−56.96983
1.650
1.77250
49.62
0.55188
63.22


38
−128.74560
2.800



63.22


39
53.73521
19.343
1.53775
74.70
0.53936
64.82


40
−87.79724
1.670
1.54072
47.20
0.56784
63.64


41
−1213.08505
7.569



63.63


42
45.48315
12.135
1.43875
94.66
0.53402
60.04


43
−90.50969
1.300
1.95375
32.32
0.59015
45.48


44
74.58134
4.515



45.47


45
−165.65036
5.878
1.84666
23.83
0.61603
41.96


46
−41.51517
1.230
1.78800
47.35
0.55597
41.75


47
−80.86869
19.483



41.75


48
54.64839
7.001
1.43875
94.66
0.53402
41.20


49
−53.11591
1.000
1.95375
32.32
0.59015
30.73


50
24.20585
7.621
1.64769
33.85
0.58860
29.44


51
−175.50585
1.887



29.44


52
−73.53897
4.444
1.51742
52.43
0.55649
29.63


53
−27.31579
0.900
1.84850
43.79
0.56197
29.94


54
−380.11638
7.190



29.94


55
106.32314
3.601
1.80518
25.43
0.61027
31.77


56
−279.79194
46.853



37.44


57

4.150
1.51633
64.14


58

0.989
















TABLE 11







Example 4













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
49.999
152.340
385.496



Bf
50.579
50.579
50.579



FNo.
3.30
3.30
3.30



2ω(°)
49.6
16.8
6.8



Ims
23.4
23.4
23.4



DD[17]
1.483
59.306
106.099



DD[19]
2.470
17.070
2.470



DD[31]
68.278
8.267
31.715



DD[34]
70.421
58.010
2.368

















TABLE 12







Example 4











Sn
1
18







KA
1.0000000E+00
1.0000000E+00



A3
−5.3857896E−09 
1.7256063E−07



A4
3.7872778E−09
1.1885030E−07



A5
2.4462612E−10
−1.8059320E−09 



A6
−1.5306688E−11 
1.0267909E−10



A7
5.1635354E−13
−7.6080811E−13 



A8
−8.6121829E−15 
−4.4255539E−14 



A9
4.0743938E−17
−6.9957786E−16 



A10
4.5417288E−19
−1.7013319E−17 



A11
−1.8056473E−21 
3.4005008E−18



A12
−1.7318465E−23 
3.6443030E−21



A13
−3.1472514E−25 
9.0084163E−22



A14
−1.7400242E−27 
−5.8505170E−23 



A15
−2.0027491E−29 
−1.6825507E−24 



A16
7.7081656E−31
4.2946000E−26



A17
3.6956738E−33
−1.1275985E−27 



A18
7.5521081E−35
−5.2190876E−29 



A19
−3.4871525E−37 
4.1305544E−30



A20
−1.2520730E−38 
−5.0103229E−32 










Example 5


FIG. 12 shows a configuration and movement loci of the variable magnification optical system of Example 5. The variable magnification optical system in Example 5 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 5, Tables 13A and 13B show the basic lens data, Table 14 shows the specifications and the variable surface spacings, Table 15 shows the aspherical coefficients, and FIG. 13 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 13A







Example 5














Sn
R
D
Nd
vd
θgF
ED
Sg

















*1
8205.66128
4.500
1.72916
54.68
0.54451
147.00
4.18


 2
170.01677
1.051



137.23



 3
169.27154
9.329
1.84666
23.84
0.62012
137.04
3.50


 4
332.18582
13.699



136.14



 5
−362.92401
4.100
1.77250
49.62
0.55188
136.03
4.26


 6
365.82303
6.842



134.13



 7
997.04627
14.226
1.49700
81.64
0.53714
134.38
3.65


 8
−226.41462
0.120



134.40



 9
177.95993
17.273
1.43875
94.66
0.53402
136.88
3.59


10
−1342.19481
0.120



136.55



11
225.89048
3.801
1.84666
23.84
0.62012
135.77
3.50


12
143.43738
42.945



132.69



13
186.71399
19.191
1.43875
94.66
0.53402
142.98
3.59


14
−829.47251
0.120



142.84



15
197.61097
11.944
1.49700
81.64
0.53714
140.43
3.65


16
895.75518
0.121



139.82



17
115.75622
11.999
1.49700
81.64
0.53714
131.82
3.65


18
213.25427
DD[18]



130.61



*19 
119.66301
4.001
1.49700
81.64
0.53714
66.08



20
222.20668
DD[20]



64.83



21
1544.71826
1.500
1.90043
37.37
0.57668
47.07



22
54.90034
5.543



43.90



23
−362.43501
1.500
1.77250
49.62
0.55188
43.82



24
223.29180
5.553



43.54



25
−63.62880
1.373
1.84850
43.79
0.56197
43.55



26
352.27252
4.939
1.80518
25.43
0.61027
45.92



27
−100.17466
17.899



46.51



28
−95.70171
1.654
1.61997
63.88
0.54252
52.54



29
−222.69281
4.269
1.61266
44.46
0.56403
54.16



30
−82.29980
6.290



54.69



31
286.25058
4.499
1.74400
44.90
0.56308
58.19



32
−322.82481
DD[32]



58.31



33
−67.13021
1.671
1.43875
94.66
0.53402
58.09



34
227.55028
2.890
1.80518
25.43
0.61027
60.97



35
1328.07583
DD[35]



61.16

















TABLE 13B







Example 5













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.990



62.00


37
197.07441
12.591
1.53775
74.70
0.53936
63.54


38
−65.79695
1.650
1.81600
46.59
0.55661
63.72


39
−118.97582
2.800



65.04


40
57.34935
14.414
1.53775
74.70
0.53936
64.90


41
−259.02339
1.670
1.54072
47.23
0.56511
63.79


42
1953.40832
10.132



62.01


43
54.45164
11.310
1.49700
81.64
0.53714
50.49


44
−99.12410
1.300
1.90043
37.37
0.57668
48.80


45
85.25076
6.535



45.18


46
−165.28070
4.001
1.80518
25.43
0.61027
44.31


47
−62.64231
1.409
1.53775
74.70
0.53936
44.14


48
−95.65383
17.043



43.36


49
48.54391
7.592
1.43875
94.66
0.53402
34.25


50
−57.96409
1.000
1.90043
37.37
0.57668
33.21


51
26.30450
7.659
1.58144
40.98
0.57640
31.34


52
−221.48432
2.483



31.40


53
−59.54995
4.025
1.58313
59.37
0.54345
31.37


54
−29.96692
0.900
1.88300
40.69
0.56730
31.65


55
−252.71900
9.609



33.29


56
632.94260
3.780
1.80518
25.43
0.61027
38.80


57
−94.19992
57.014



39.17


58

4.150
1.51633
64.14


59

0.994
















TABLE 14







Example 5













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
50.005
152.356
385.538



Bf
60.745
60.745
60.745



FNo.
3.30
3.30
3.30



2ω(°)
50.2
16.8
6.8



Ims
23.4
23.4
23.4



DD[18]
1.474
59.318
111.943



DD[20]
2.733
19.533
2.792



DD[32]
70.968
9.522
25.645



DD[35]
67.589
54.391
2.385

















TABLE 15







Example 5











Sn
1
19







KA
1.0000000E+00
1.0000000E+00



A3
−5.3857896E−09 
1.7256063E−07



A4
1.3877300E−08
9.0352072E−08



A5
1.9518303E−10
9.7583129E−10



A6
−1.4247728E−11 
7.1325586E−11



A7
4.9246088E−13
−2.2253642E−12 



A8
−7.7399125E−15 
−2.3301971E−14 



A9
3.1297320E−17
1.8937780E−16



A10
3.5660511E−19
−7.1216157E−18 



A11
−6.7930835E−22 
2.7351114E−18



A12
−1.0682671E−23 
3.7184629E−22



A13
−2.9321485E−25 
−6.8228596E−24 



A14
3.9253044E−28
−5.1627438E−23 



A15
−2.4799576E−29 
−1.0279215E−24 



A16
2.1727276E−31
−3.2528888E−26 



A17
1.2731769E−33
2.1469551E−27



A18
1.0798389E−34
5.3912796E−31



A19
−3.8971441E−37 
1.0885495E−30



A20
−7.7345659E−39 
−3.4464014E−32 










Example 6


FIG. 14 shows a configuration and movement loci of the variable magnification optical system of Example 6. The variable magnification optical system in Example 6 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of four lenses L1a to L1d in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1e to L1g in order from the object side to the image side. The first C subgroup G1C consists of two lenses L1h and L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and thirteen lenses L5a to L5m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 6, Tables 16A and 16B show the basic lens data, Table 17 shows the specifications and the variable surface spacings, Table 18 shows the aspherical coefficients, and FIG. 15 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 16A







Example 6














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
2112.12382
3.800
1.73402
54.60
0.54448
146.24
4.13


 2
305.99931
11.288



145.06



 3
−787.87764
3.801
1.74344
53.66
0.54583
139.31
4.17


 4
879.98837
9.929



139.21



 5
−336.59454
3.820
1.77250
49.60
0.55212
136.79
4.23


 6
335.14369
9.170
1.84666
23.83
0.61603
136.76
5.51


 7
−3517.81701
1.500



136.76



*8
316.09003
17.109
1.49700
81.54
0.53748
136.74
3.62


 9
−296.70000
0.200



136.20



10
169.21266
20.399
1.43875
94.66
0.53402
138.91
3.59


11
−882.55556
0.200



142.80



12
274.21910
3.601
1.85478
24.80
0.61232
142.60
3.49


13
140.71353
43.083



139.66



*14 
163.78127
20.099
1.53775
74.70
0.53936
135.25
3.64


15
−1361.49906
0.201



144.81



16
135.80126
18.394
1.49700
81.54
0.53748
143.80
3.62


17
1109.06277
DD[17]



137.98



18
241.88045
4.000
1.43875
94.66
0.53402
137.00



19
895.42383
DD[19]



63.61



*20 
2256.20719
1.621
1.90043
37.37
0.57668
51.07



21
57.70558
7.981



50.69



22
−102.74826
3.669
1.80706
47.75
0.55504
46.98



23
125.33668
5.784



46.89



24
740.58097
12.460
1.59270
35.31
0.59336
47.21



25
−67.52364
2.555
1.59282
68.62
0.54414
50.64



26
−133.67229
3.872



50.64



27
127.93660
9.987
1.78213
32.82
0.59360
52.17



28
−312.29512
1.583
1.49700
81.61
0.53887
54.33



29
2317.04449
1.150



54.33



30
−476.06392
2.713
1.67545
57.73
0.54287
54.06



31
782.31379
DD[31]



54.04



32
−72.24096
1.311
1.52271
77.69
0.53897
53.92



33
165.35287
3.000
1.84999
23.69
0.62126
56.31



34
478.33025
DD[34]



56.31

















TABLE 16B







Example 6













Sn
R
D
Nd
νd
θgF
ED
















35(St)

2.785



56.53


36
217.32899
7.353
1.70287
56.36
0.54348
57.32


37
−112.83667
1.818



59.24


38
−79.78275
1.701
1.73800
32.33
0.59005
59.39


39
−110.91198
2.801



59.38


40
70.23303
9.431
1.55532
66.05
0.53856
60.13


41
−359.62847
0.151



59.94


42
48.79175
12.838
1.43700
95.10
0.53364
59.44


43
−115.55063
1.601
1.90366
31.31
0.59481
51.83


44
112.02454
4.006



51.82


45
−408.45943
5.384
1.84661
23.88
0.62072
48.48


46
−75.08207
1.600
1.84850
43.79
0.56197
47.73


47
−127.38079
11.516



47.73


48
75.30319
6.136
1.49700
81.61
0.53887
47.07


49
−136.34693
0.233



35.17


50
519.90262
1.201
1.82684
46.59
0.55696
33.15


51
21.85654
7.579
1.43700
95.10
0.53364
28.71


52
−1161.38463
2.472



28.71


53
−363.17151
4.855
1.49700
81.61
0.53887
28.56


54
−29.03187
1.101
1.79754
48.25
0.55426
28.23


55
152.11880
22.175



28.23


56
211.33901
2.995
1.74460
28.54
0.60738
29.02


57
−196.47086
59.418



38.46


58

4.150
1.51680
64.20


59

1.010
















TABLE 17







Example 6













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
7.7



f
50.004
152.572
386.536



Bf
63.164
63.164
63.164



FNo.
3.30
3.30
3.30



2ω(°)
50.6
16.8
6.6



Ims
23.4
23.4
23.4



DD[17]
1.500
58.101
103.301



DD[19]
1.507
15.091
1.507



DD[31]
72.728
9.707
19.660



DD[34]
51.058
43.895
2.325

















TABLE 18







Example 6










Sn
8
14
20





KA
1.0000000E+00
 1.0000000E+00
1.0000000E+00


A4
−2.1692043E−08 
−2.7727773E−08
2.5320472E−07


A6
1.2768740E−12
−1.1067827E−12
2.1091895E−10


A8
−4.8788496E−16 
−2.3233665E−16
−7.1740421E−13 


A10
6.0679808E−20
 2.4327059E−19
7.8662068E−16


A12
−2.9066987E−24 
−6.8936760E−23
8.0200926E−19


A14
7.0801276E−28
 5.0247986E−27
−2.7607559E−21 


A16
−2.4183654E−31 
 1.3256291E−30
8.2237000E−25


A18
2.9233605E−35
−2.9285922E−34
3.1613332E−27


A20
−1.2019237E−39 
 1.6932459E−38
−2.4662852E−30 









Example 7


FIG. 16 shows a configuration and movement loci of the variable magnification optical system of Example 7. The variable magnification optical system in Example 7 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 7, Tables 19A and 19B show the basic lens data, Table 20 shows the specifications and the variable surface spacings, Table 21 shows the aspherical coefficients, and FIG. 17 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 19A







Example 7














Sn
R
D
Nd
vd
θgF
ED
Sg

















*1
2499.51160
4.500
1.72916
54.68
0.54451
148.22
4.18


 2
277.11484
16.918



147.00



 3
−326.07416
4.220
1.75500
52.32
0.54757
136.06
4.17


 4
244.14465
7.653
1.84666
23.84
0.62012
137.98
3.50


 5
582.65242
5.581



137.98



 6
1362.74691
13.839
1.59282
68.62
0.54414
137.75
4.13


 7
−237.95589
0.201



137.83



 8
168.74635
17.219
1.43875
94.66
0.53402
138.87
3.59


 9
34365.73168
0.200



140.36



10
253.77606
3.900
1.84666
23.84
0.62012
140.20
3.50


11
148.30858
45.916



139.16



12
202.87000
18.094
1.43875
94.66
0.53402
135.80
3.59


13
−1021.95507
0.201



145.51



14
209.06059
12.095
1.55032
75.50
0.54001
145.44
4.09


15
1049.16749
0.320



143.63



16
127.89764
14.177
1.49700
81.64
0.53714
143.03
3.65


17
318.59302
DD[17]



135.44



18
255.79334
4.001
1.43875
94.66
0.53402
134.11



19
−2257.14682
DD[19]



63.18



*20 
4164.96215
1.701
1.90043
37.37
0.57668
50.51



21
57.33914
8.408



50.30



22
−85.72601
6.000
1.75500
52.32
0.54757
46.47



23
165.19750
2.805



46.36



24
514.22796
9.009
1.59270
35.31
0.59336
47.20



25
−122.09232
2.799
1.59282
68.62
0.54414
49.64



26
−1465.25772
4.438



49.64



27
1532.23624
9.399
1.78880
28.43
0.60092
52.98



28
−112.23786
2.899
1.88300
40.76
0.56679
54.32



29
−407.72911
0.932



54.32



30
242.07778
6.999
1.67300
38.26
0.57580
55.53



31
−262.39281
DD[31]



56.63



32
−72.02829
1.411
1.43875
94.66
0.53402
56.95



33
211.19701
4.442
1.84666
23.83
0.61603
59.32



34
525.10338
DD[34]



59.32

















TABLE 19B







Example 7













Sn
R
D
Nd
νd
θgF
ED
















35(St)

2.500



59.75


36
259.55021
5.436
1.72916
54.68
0.54451
60.55


37
−217.15012
1.700
1.73800
32.33
0.59005
62.22


38
−256.41303
2.800



62.22


39
65.82243
10.567
1.53775
74.70
0.53936
62.42


40
−574.67204
1.311
1.54072
47.23
0.56511
61.59


41
−2932.07333
0.340



61.59


42
57.01484
14.236
1.43700
95.10
0.53364
60.86


43
−80.63266
1.601
1.88300
40.76
0.56679
54.62


44
163.92294
4.285



54.61


45
−162.46986
5.599
1.73800
32.33
0.59005
51.70


46
−56.32939
1.611
1.72916
54.68
0.54451
51.54


47
−86.86479
11.289



51.54


48
50.82282
6.764
1.51860
69.89
0.53184
51.25


49
−138.90444
2.001



39.16


50
−6131.02993
1.201
1.87070
40.73
0.56825
38.09


51
23.48588
6.384
1.43700
95.10
0.53364
30.22


52
152.88153
9.656



30.22


53
937.32783
5.874
1.49700
81.64
0.53714
30.01


54
−27.27776
1.100
1.81600
46.62
0.55682
28.99


55
153.58623
18.350



28.99


56
104.83403
3.734
1.78880
28.43
0.60092
29.92


57
−333.03023
57.970



39.87


58

4.150
1.51680
64.20


59

1.002
















TABLE 20







Example 7













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
7.7



f
49.993
152.539
386.452



Bf
61.708
61.708
61.708



FNo.
3.29
3.29
3.29



2ω(°)
50.0
16.8
6.8



Ims
23.4
23.4
23.4



DD[17]
2.166
62.577
104.679



DD[19]
1.715
12.451
1.716



DD[31]
68.059
8.015
29.459



DD[34]
66.731
55.628
2.817

















TABLE 21







Example 7











Sn
1
20







KA
1.0000000E+00
 1.0000000E+00



A4
7.7879396E−09
 1.6442102E−07



A6
6.9131651E−13
−1.9498855E−11



A8
−3.8836286E−16 
−1.0582242E−13



A10
9.0639926E−20
 1.6685707E−16



A12
−1.0085685E−23 
 1.3708912E−19



A14
9.2869034E−28
−4.8057576E−22



A16
−3.0706896E−31 
−8.4674094E−26



A18
5.3311497E−35
 7.2952808E−28



A20
−2.8029557E−39 
−3.5929459E−31










Example 8


FIG. 18 shows a configuration and movement loci of the variable magnification optical system of Example 8. The variable magnification optical system in Example 8 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of two lenses L2a and L2b in order from the object side to the image side. The third lens group G3 consists of six lenses L3a to L3f in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and thirteen lenses L5a to L5m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 8, Tables 22A and 22B show the basic lens data, Table 23 shows the specifications and the variable surface spacings, Table 24 shows the aspherical coefficients, and FIG. 19 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 22A







Example 8














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
−2092.05259
3.900
1.77250
49.60
0.55212
120.09
4.23


 2
160.85043
21.334



121.00



 3
−155.79649
5.199
1.84850
43.79
0.56197
113.32
5.08


 4
1552.62293
0.350



113.20



 5
907.26461
7.899
1.84666
23.84
0.62012
116.04
3.50


 6
−582.94373
6.432



116.82



 7
−312.95252
10.900
1.43875
94.66
0.53402
117.31
3.59


 8
−147.40107
0.200



118.26



 9
292.76666
15.356
1.55032
75.50
0.54001
121.35
4.09


10
−280.30347
0.200



122.56



11
262.26032
3.801
1.84666
23.84
0.62012
123.02
3.50


12
169.21456
24.288



124.56



13
246.65538
15.430
1.43875
94.66
0.53402
123.24
3.59


14
−396.56899
0.200



126.92



15
212.75394
10.852
1.55032
75.50
0.54001
127.10
4.09


16
3020.30811
0.320



126.96



17
122.62116
11.890
1.55032
75.50
0.54001
126.55
4.09


18
300.45730
DD[18]



121.39



19
406.08762
1.501
1.84666
23.78
0.62054
120.25



20
169.73028
5.081
1.43875
94.66
0.53402
51.63



21
−238.64231
DD[21]



51.62



*22 
4164.93188
1.701
1.95375
32.32
0.59015
45.55



23
40.47955
11.332



44.94



24
−39.65174
1.601
1.83400
37.16
0.57759
40.34



25
397.31662
3.389



40.21



26
−143.07299
4.305
1.78879
25.56
0.61605
45.44



27
−61.70130
0.121



44.01



28
−186.18557
3.046
1.59270
35.31
0.59336
45.05



29
−93.10425
1.701
1.59282
68.62
0.54414
46.98



30
−111.48612
0.121



46.98



31
174.05349
5.988
1.78737
27.99
0.60816
49.47



32
−117.18312
DD[32]



50.63



33
−53.09913
1.411
1.43875
94.66
0.53402
50.90



34
170.35545
3.209
1.78880
28.43
0.60092
54.35



35
2933.09642
DD[35]



54.35

















TABLE 22B







Example 8













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.600



54.58


37
120.47829
8.424
1.59282
68.62
0.54414
55.40


38
−117.46763
0.121



57.30


39
115.02056
4.391
1.59976
46.84
0.56463
57.36


40
1742.87794
0.121



55.71


41
81.11516
3.731
1.53775
74.70
0.53936
55.32


42
186.69095
1.500
1.54072
47.23
0.56511
52.41


43
123.85947
0.120



52.41


44
68.01632
12.752
1.43700
95.10
0.53364
51.08


45
−85.63704
1.601
1.88300
40.76
0.56679
46.57


46
57.54886
44.497



46.56


47
470.88608
6.893
1.56196
43.38
0.57306
43.63


48
−64.61931
13.569



49.00


49
48.37800
10.108
1.48749
70.24
0.53007
45.25


50
−132.81839
1.695



44.10


51
−109.66760
2.913
1.88300
40.76
0.56679
42.67


52
34.01968
12.195
1.52001
76.92
0.53806
38.46


53
−45.97127
0.120



38.46


54
−73.95460
4.113
1.49700
81.54
0.53748
38.44


55
−36.24778
1.101
1.86969
41.23
0.56776
37.17


56
59.10103
0.150



37.17


57
52.91858
6.209
1.67270
32.10
0.59891
38.18


58
−184.91465
63.876



38.82


59

4.100
1.51680
64.20


60

0.984
















TABLE 23







Example 8













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
7.7



f
36.224
110.525
279.646



Bf
67.563
67.563
67.563



FNo.
3.28
3.28
3.28



2ω(°)
68.2
23.0
9.4



Ims
23.4
23.4
23.4



DD[18]
2.124
72.163
100.360



DD[21]
1.401
8.538
11.734



DD[32]
81.923
8.986
20.569



DD[35]
49.106
44.867
1.890

















TABLE 24







Example 8










Sn
22







KA
 1.0000000E+00



A4
 1.4615104E−06



A6
 1.6250388E−10



A8
−5.8075217E−12



A10
 2.0908064E−14



A12
−3.0611068E−17



A14
−1.1150205E−20



A16
 8.1084157E−23



A18
−6.4259403E−26



A20
 8.6247942E−31










Example 9


FIG. 20 shows a configuration and movement loci of the variable magnification optical system of Example 9. The variable magnification optical system in Example 9 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of two lenses L1g and L1h in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of six lenses L3a to L3f in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and thirteen lenses L5a to L5m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 9, Tables 25A and 25B show the basic lens data, Table 26 shows the specifications and the variable surface spacings, Table 27 shows the aspherical coefficients, and FIG. 21 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 25A







Example 9














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
−962.21938
3.900
1.73002
55.00
0.54410
140.33
4.11


 2
315.58160
16.539



140.33



 3
−288.09065
3.900
1.74726
53.27
0.54639
142.71
4.19


 4
352.54236
0.186



136.86



 5
324.26593
8.016
1.84666
23.83
0.61603
136.53
5.51


 6
2466.25372
1.462



136.37



*7
837.13277
18.781
1.49700
81.54
0.53748
136.62
3.62


 8
−178.63525
0.120



136.64



 9
150.94320
16.882
1.43875
94.94
0.53433
138.79
3.62


10
1064.52242
0.530



138.79



11
429.52734
3.500
1.81008
26.49
0.61277
140.20
3.78


12
170.94625
44.185



139.70



*13 
172.91496
22.327
1.49700
81.54
0.53748
138.99
3.62


14
−628.30923
0.120



136.04



15
150.73545
18.472
1.43875
94.94
0.53433
146.17
3.62


16
2072.41802
DD[16]



146.17



17
802.92340
3.471
1.49700
81.64
0.53714
141.39



18
−1226.87707
DD[18]



140.36



*19 
278.34652
2.000
1.85740
42.24
0.56561
84.25



20
49.53050
12.435



83.43



21
−64.14608
1.600
1.59282
68.62
0.54414
57.21



22
129.74193
2.095



51.15



23
391.38931
4.792
1.85581
26.69
0.61103
51.15



24
−130.13512
1.510
1.59282
68.62
0.54414
51.53



25
−1020.94831
0.120



51.66



26
103.99598
11.249
1.61800
40.25
0.57772
51.66



27
−54.90794
1.500
1.90043
37.37
0.57720
51.97



28
−155.03440
DD[28]



51.93



29
−79.75372
1.510
1.49700
81.54
0.53748
51.93



30
172.02166
2.079
1.80518
25.42
0.61616
53.41



31
437.12766
DD[31]



55.49

















TABLE 25B







Example 9













Sn
R
D
Nd
vd
θgF
ED
















32(St)

1.501



55.49


33
71.39200
12.932
1.58710
51.23
0.55623
55.60


34
−99.18397
0.849



56.50


35
−90.07259
1.229
1.92673
28.97
0.60175
59.52


36
−115.21321
0.151



59.31


37
116.89128
4.701
1.65804
57.70
0.54334
59.06


38
−3477.55393
0.125



59.18


39
59.89228
12.140
1.43875
94.94
0.53433
56.11


40
−68.90697
1.300
2.00069
25.46
0.61364
50.93


41
157.05155
18.277



49.38


42
−65.25901
2.560
1.51984
53.16
0.55508
49.37


43
−48.30770
0.598



47.04


44
356.25689
6.211
1.90960
20.15
0.64151
43.14


45
−55.10284
1.888
1.84384
42.71
0.56487
41.06


46
−339.60147
4.982



40.64


47
46.28311
16.434
1.43875
94.94
0.53433
40.64


48
−66.86895
1.482
1.92463
35.50
0.58188
33.90


49
26.34668
1.635



27.33


50
29.29295
9.072
1.43875
94.94
0.53433
27.33


51
−28.61407
3.565
1.74812
53.19
0.54651
26.23


52
98.63170
22.285



26.25


53
92.40038
6.308
1.69253
48.70
0.55724
26.25


54
−142.65532
37.374



28.02


55

2.650
1.51633
64.14




56

0.980




















TABLE 26







Example 9













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
7.8



f
51.230
157.277
399.597



Bf
40.102
40.102
40.102



FNo.
3.35
3.35
3.35



2ω(°)
49.2
16.2
6.4



Ims
23.4
23.4
23.4



DD[16]
1.507
55.813
79.262



DD[18]
1.536
27.189
38.088



DD[28]
84.272
6.782
21.789



DD[31]
54.897
52.427
3.072

















TABLE 27







Example 9










Sn
7
13
19





KA
 1.0000000E+00
 1.0000000E+00
 1.0000000E+00


A4
−1.9790294E−08
−3.4219015E−08
 3.6836568E−07


A6
 1.0005871E−11
−5.2248275E−12
−2.8884327E−10


A8
−1.1960525E−14
 4.8142497E−15
 1.2636902E−12


A10
 8.7194764E−18
−3.1759469E−18
−1.6301333E−15


A12
−3.9978648E−21
 1.2884412E−21
−7.5500614E−18


A14
 1.1587458E−24
−3.2543866E−25
 3.4863792E−20


A16
−2.0608339E−28
 4.9870449E−29
−6.0583776E−23


A18
 2.0513816E−32
−4.2440131E−33
 5.0076896E−26


A20
−8.7423556E−37
 1.5381501E−37
−1.6309040E−29









Example 10


FIG. 22 shows a configuration and movement loci of the variable magnification optical system of Example 10. The variable magnification optical system of Example 10 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a negative refractive power, a third lens group G3 having a negative refractive power, and a fourth lens group G4 having a positive refractive power.


During changing magnification, the first lens group G1 and the fourth lens group G4 remain stationary with respect to the image plane Sim, and the second lens group G2 and the third lens group G3 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2. The negative movable lens group GN consists of a third lens group G3.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of two lenses L1g and L1h in order from the object side to the image side.


The second lens group G2 consists of six lenses L2a to L2f in order from the object side to the image side. The third lens group G3 consists of two lenses L3a and L3b in order from the object side to the image side. The fourth lens group G4 consists of an aperture stop St and thirteen lenses L4a to L4m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 10, Tables 28A and 28B show the basic lens data, Table 29 shows the specifications and the variable surface spacings, Table 30 shows the aspherical coefficients, and FIG. 23 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 28A







Example 10














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
−1285.31483
3.900
1.72599
54.86
0.54440
147.92
4.11


 2
313.65366
18.040



141.64



 3
−275.97010
3.900
1.71674
55.66
0.54379
141.32
4.07


 4
315.74766
0.266



140.97



 5
300.40423
8.679
1.84666
23.83
0.61603
141.19
5.51


 6
1820.42445
1.401



141.09



*7
793.39232
14.778
1.49700
81.54
0.53748
140.77
3.62


 8
−263.29676
0.120



141.35



 9
154.82343
23.841
1.43875
94.94
0.53433
144.52
3.62


10
−875.82123
1.658



143.83



11
253.71181
3.500
1.80518
25.42
0.61616
140.69
3.37


12
137.79690
47.003



136.35



*13 
158.00303
22.626
1.49700
81.54
0.53748
146.68
3.62


14
−829.82676
0.120



146.29



15
163.9556
17.1218
1.43875
94.94
0.53433
140.25
3.62


16
3967.1934
DD[16]



139.26



*17 
119.0258
2.0000
2.00100
29.13
0.59952
58.20



18
45.7411
12.9117



52.41



19
−82.9613
1.6000
1.59282
68.62
0.54414
52.22



20
148.5453
2.0949



52.19



21
209.3014
5.4597
1.88311
25.04
0.61745
52.49



22
−149.6083
1.5100
1.59282
68.62
0.54414
52.47



23
184.6792
0.1390



52.04



24
78.7031
11.6627
1.64484
34.48
0.59250
52.17



25
−66.8732
1.5000
1.90043
37.37
0.57720
52.03



26
−836.9307
DD[26]



52.54



27
−99.8606
1.5100
1.49700
81.54
0.53748
54.49



28
192.2612
2.4635
1.80518
25.42
0.61616
56.34



29
474.0611
DD[29]



56.54

















TABLE 28B







Example 10













Sn
R
D
Nd
vd
θgF
ED
















30(St)

1.5000



57.53


31
75.6891
12.8861
1.59711
50.80
0.55667
60.53


32
−105.8650
1.1448



60.32


33
−91.7619
1.2000
1.90973
30.30
0.59791
60.05


34
−123.6900
0.1200



60.22


35
94.3730
6.3113
1.61532
61.62
0.54313
57.34


36
−1789.2338
0.2981



56.60


37
56.6857
12.3733
1.43875
94.94
0.53433
51.32


38
−77.4296
1.9819
1.97999
27.01
0.60670
49.45


39
123.8422
18.4875



46.43


40
−89.2534
2.9893
1.54029
47.94
0.56458
41.56


41
−53.8350
0.9997



41.49


42
−592.7430
4.6568
1.91135
19.74
0.64405
38.63


43
−55.1196
1.6563
1.83200
44.80
0.56072
38.22


44
−211.6326
4.5019



36.88


45
36.3298
15.5093
1.43875
94.94
0.53433
30.23


46
−75.4122
1.9144
1.93410
34.47
0.58454
24.65


47
26.8763
2.0991



23.18


48
36.8052
9.4574
1.43875
94.94
0.53433
23.85


49
−24.7718
1.1999
1.77527
50.47
0.55041
24.24


50
90.5612
19.3814



25.71


51
83.2129
6.4045
1.66527
37.39
0.58362
42.28


52
−107.8393
37.1424



42.60


53

2.6500
1.51633
64.14
0.53531



54

0.988
















TABLE 29







Example 10













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
7.8



f
51.261
157.370
399.833



Bf
39.878
39.878
39.878



FNo.
3.30
3.30
3.32



2ω(°)
49.8
16.2
6.4



Ims
23.4
23.4
23.4



DD[16]
2.110
84.158
119.769



DD[26]
100.134
10.502
23.487



DD[29]
43.519
51.103
2.507

















TABLE 30







Example 10










Sn
7
13
17





KA
 1.0000000E+00
 1.0000000E+00
 1.0000000E+00


A4
−1.4424937E−08
−3.4710407E−08
 5.0925308E−08


A6
 8.6511285E−12
−6.6213150E−12
 3.1434924E−10


A8
−7.2090216E−15
 3.5648677E−15
−2.8030268E−12


A10
 3.5595347E−18
−1.3121584E−18
 1.2069904E−14


A12
−1.2289455E−21
 3.1219440E−22
−2.9274324E−17


A14
 2.9490477E−25
−5.2285338E−26
 4.1079045E−20


A16
−4.6599178E−29
 6.4473853E−30
−3.1855847E−23


A18
 4.3155201E−33
−5.4624566E−34
 1.1717531E−26


A20
−1.7586609E−37
 2.2752502E−38
−1.2320305E−30









Example 11


FIG. 24 shows a configuration and movement loci of the variable magnification optical system of Example 11. The variable magnification optical system in Example 11 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of four lenses L1d to L1g in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1h to L1j in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of six lenses L3a to L3f in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and thirteen lenses L5a to L5m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 11, Tables 31A and 31B show the basic lens data, Table 32 shows the specifications and the variable surface spacings, Table 33 shows the aspherical coefficients, and FIG. 25 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 31A







Example 11














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
−2058.83443
3.900
1.80493
47.51
0.55567
148.60
4.50


 2
261.15350
20.223



141.07



 3
−258.28392
3.900
1.72974
54.95
0.54417
140.72
4.11


 4
307.11074
0.120



140.55



 5
306.57986
9.760
1.84666
23.83
0.61603
140.62
5.51


 6
−15563.10980
1.351



140.66



*7
589.56688
11.839
1.49700
81.54
0.53748
140.95
3.62


 8
−429.82512
0.120



141.28



 9
−1015.59539
11.428
1.43875
94.94
0.53433
141.47
3.62


10
−212.86658
0.120



141.62



11
178.11518
12.876
1.43875
94.94
0.53433
136.58
3.62


12
845.26883
0.120



135.85



13
372.60266
3.500
1.84666
23.78
0.62054
135.54
3.54


14
181.63962
42.962



133.40



15
271.9276
15.8409
1.49700
81.54
0.53748
144.46
3.62


16
−765.7310
0.1200



144.45



17
499.0874
9.1667
1.43875
94.94
0.53433
143.58
3.62


18
−1178.2326
0.1201



143.30



19
163.8672
13.6622
1.49700
81.54
0.53748
138.31
3.62


20
662.8697
DD[20]



137.37



*21 
455.9303
3.2457
1.49700
81.64
0.53714
72.49



22
48096.9278
DD[22]



71.64



*23 
1244.1367
1.8000
2.00100
29.13
0.59952
54.96



24
59.9336
10.2626



50.40



25
−73.4695
1.6000
1.59282
68.62
0.54414
50.30



26
143.6538
2.0949



50.66



27
724.5225
5.1917
1.71098
29.45
0.60519
50.75



28
−90.1793
1.5100
1.55032
75.50
0.54001
50.90



29
−4756.1962
0.4245



51.37



30
113.7660
6.9043
1.69988
30.01
0.60390
51.85



31
−135.5507
1.5000
1.70240
43.96
0.56702
51.86



32
−432.9800
DD[32]



51.89



33
−89.4335
1.5100
1.49700
81.54
0.53748
52.56



34
155.1968
2.5931
1.80518
25.42
0.61616
54.57



35
358.0595
DD[35]



54.75

















TABLE 31B







Example 11













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.5000



55.47


37
122.4770
12.5054
1.59222
45.62
0.56738
57.44


38
−60.7844
1.0793



57.55


39
−58.1163
1.1999
1.86125
40.98
0.56863
57.03


40
−119.5327
2.5000



58.19


41
127.1840
7.2396
1.52227
75.97
0.53783
58.13


42
−172.5256
0.6901



57.90


43
50.6231
12.9515
1.43875
94.94
0.53433
53.17


44
−107.4967
2.8968
2.00069
25.46
0.61364
51.65


45
144.8824
14.7914



49.16


46
−182.9085
3.8422
1.57281
42.52
0.57447
46.19


47
−69.1159
0.2905



46.11


48
270.9285
7.1204
1.80518
25.43
0.61027
43.32


49
−53.6462
1.8391
1.79845
47.43
0.55609
42.64


50
−925.1673
4.7081



40.40


51
41.3191
15.6609
1.43875
94.94
0.53433
34.09


52
−154.2579
2.5887
1.88041
39.54
0.57177
27.91


53
25.5242
1.9214



25.56


54
29.39680
8.842
1.43875
94.94
0.53433
26.20


55
−30.12441
1.200
1.78953
46.15
0.55928
26.09


56
71.62301
23.253



26.93


57
76.34531
5.738
1.61181
41.26
0.57581
42.40


58
−188.47804
41.796



42.60


59

2.650
1.51633
64.14


60

0.991
















TABLE 32







Example 11













WIDE
MIDDLE
TELE
















Zr
1.0
3.1
8.2



f
45.517
142.925
370.968



Bf
44.535
44.535
44.535



FNo.
3.31
3.31
3.32



2ω(°)
57.0
18.0
7.0



Ims
23.4
23.4
23.4



DD[20]
1.563
69.044
103.774



DD[22]
2.464
26.030
33.146



DD[32]
112.139
14.697
14.368



DD[35]
37.397
43.793
2.275

















TABLE 33







Example 11










Sn
7
21
23





KA
 1.0000000E+00
 1.0000000E+00
 1.0000000E+00


A4
−1.9129049E−08
 3.7325949E−08
−4.0674003E−08


A6
−7.4602781E−13
−9.5183284E−11
 5.3090567E−10


A8
 1.5600772E−15
 2.6163401E−13
−3.1705419E−12


A10
−1.1407900E−18
−5.4284140E−16
 1.1326971E−14


A12
 5.0864661E−22
 7.6574840E−19
−2.5425680E−17


A14
−1.4463727E−25
−6.9712703E−22
 3.5106929E−20


A16
 2.5577733E−29
 3.8828941E−25
−2.8307328E−23


A18
−2.5524545E−33
−1.1974725E−28
 1.1734240E−26


A20
 1.0916617E−37
 1.5586811E−32
−1.7515774E−30









Example 12


FIG. 26 shows a configuration and movement loci of the variable magnification optical system of Example 12. The variable magnification optical system in Example 12 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of six lenses L3a to L3f in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and thirteen lenses L5a to L5m in order from the object side to the image side.


Regarding the variable magnification optical system of Example 12, Tables 34A and 34B show the basic lens data, Table 35 shows the specifications and the variable surface spacings, Table 36 shows the aspherical coefficients, and FIG. 27 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 34A







Example 12














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
2180.90852
3.900
1.74393
53.61
0.54591
147.03
4.17


 2
214.98435
21.162



139.48



 3
−272.10755
3.900
1.73229
54.77
0.54428
139.28
4.12


 4
349.53428
0.120



139.19



 5
316.12676
8.614
1.84666
23.83
0.61603
139.46
5.51


 6
2677.43692
1.452



139.38



*7
454.27466
17.477
1.49700
81.54
0.53748
139.46
3.62


 8
−234.54919
0.120



139.68



 9
138.56004
20.952
1.43875
94.94
0.53433
135.71
3.62


10
−2126.25082
0.120



134.81



11
276.15823
3.500
1.81766
28.38
0.60618
131.68
3.95


12
128.21434
44.783



127.06



*13 
151.99613
18.208
1.49700
81.54
0.53748
137.60
3.62


14
−7291.32432
0.120



137.29



15
343.7853
6.8204
1.43875
94.94
0.53433
135.56
3.62


16
1439.7786
0.1201



135.07



17
165.5541
12.3522
1.49700
81.54
0.53748
130.56
3.62


18
721.6286
DD[18]



129.17



19
477.6475
3.2330
1.49700
81.64
0.53714
74.21



20
−3861.9068
DD[20]



73.02



*21 
2510.5174
1.8000
1.90043
37.37
0.57668
57.70



22
59.6083
11.4374



52.32



23
−75.7451
1.6000
1.59282
68.62
0.54414
51.92



24
133.3992
2.0949



51.79



25
386.8067
8.0737
1.72138
29.54
0.60467
51.89



26
−76.5498
1.5100
1.54163
73.60
0.53926
52.06



27
−932.9580
5.6455



52.01



28
118.8044
10.0239
1.58964
39.12
0.58091
51.63



29
−77.9414
1.5000
1.76950
39.14
0.57591
51.56



30
−449.0878
DD[30]



51.94



31
−75.9829
1.8100
1.49700
81.54
0.53748
52.51



32
121.2417
3.8525
1.80518
25.42
0.61616
55.09



33
261.8105
DD[33]



55.39

















TABLE 34B







Example 12













Sn
R
D
Nd
νd
θgF
ED
















34(St)

1.5000



56.37


35
131.2135
13.1539
1.59338
48.10
0.56227
58.44


36
−57.8310
0.9415



58.61


37
−55.4837
1.2000
1.81820
43.53
0.56396
58.18


38
−109.4473
2.5000



59.48


39
60.1599
11.5036
1.49700
81.64
0.53714
59.28


40
−193.0423
0.6262



58.74


41
52.3573
13.0886
1.43875
94.94
0.53433
51.40


42
−77.0480
1.4463
2.00069
25.46
0.61364
49.42


43
111.3966
12.5518



46.56


44
−139.0009
3.7132
1.71263
29.51
0.60498
44.14


45
−61.0088
0.3702



44.15


46
153.7009
6.9885
1.80518
25.43
0.61027
40.68


47
−50.1284
1.3914
1.72653
55.17
0.54401
40.03


48
144.0527
4.2720



36.56


49
34.8003
13.9019
1.43875
94.94
0.53433
31.69


50
−132.1199
1.2000
1.89345
38.66
0.57385
26.07


51
19.9114
0.6411



23.80


52
20.7417
8.5662
1.43875
94.94
0.53433
24.19


53
−23.8276
1.2000
1.82410
45.59
0.55927
24.12


54
129.40711
20.382



25.16


55
76.27008
4.475
1.71503
29.29
0.60562
39.46


56
−459.85567
39.236



39.64


57

2.650
1.51633
64.14
0.53531


58

0.983
















TABLE 35







Example 12













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.3



f
50.714
150.114
371.735



Bf
41.967
41.967
41.967



FNo.
3.30
3.30
3.30



2ω(°)
50.0
17.0
7.0



Ims
23.4
23.4
23.4



DD[18]
1.516
49.475
80.669



DD[20]
1.501
25.319
27.399



DD[30]
85.653
15.916
18.093



DD[33]
40.920
38.881
3.428

















TABLE 36







Example 12










Sn
7
13
21





KA
 1.0000000E+00
 1.0000000E4+00
 1.0000000E+00


A4
−2.1744660E−08
−1.9625182E−08
 2.0840144E−07


A6
 1.1024212E−12
−1.3810261E−12
−9.3840881E−11


A8
−6.8770552E−16
 4.2207417E−17
 1.0281018E−12


A10
 2.1567459E−19
 6.0418586E−22
−6.1899286E−15


A12
−1.1932753E−23
 7.0118444E−24
 2.0745645E−17


A14
−1.6602296E−26
−8.5120576E−27
−4.1481301E−20


A16
 5.9220472E−30
 2.9741153E−30
 4.8939763E−23


A18
−8.5286728E−34
−4.5136352E−34
−3.1299198E−26


A20
 4.7267599E−38
 2.5679162E−38
 8.3416755E−30









Example 13


FIG. 28 shows a configuration and movement loci of the variable magnification optical system of Example 13. The variable magnification optical system in Example 13 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 13, Tables 37A and 37B show the basic lens data, Table 38 shows the specifications and the variable surface spacings, Table 39 shows the aspherical coefficients, and FIG. 29 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 37A







Example 13














Sn
R
D
Nd
vd
θgF
ED
Sg

















*1
−11890.85451
4.500
1.72916
54.68
0.54451
145.19
4.18


 2
164.00374
1.439



145.19



 3
152.04434
9.700
1.84666
23.84
0.62012
145.00
3.50


 4
290.12322
13.598



135.22



 5
−397.92182
3.900
1.77250
49.62
0.55188
134.57
4.26


 6
305.75340
7.230



133.54



 7
819.14634
13.354
1.59282
68.62
0.54414
133.42
4.13


 8
−244.62778
0.120



130.46



 9
162.47532
16.657
1.49700
81.64
0.53714
133.40
3.65


10
8714.53049
0.120



133.40



11
233.31129
3.800
1.84666
23.84
0.62012
136.78
3.50


12
134.69889
41.314



136.49



13
223.13654
16.805
1.43875
94.66
0.53402
134.22
3.59


14
−761.19436
0.120



130.63



15
190.2046
13.5670
1.43875
94.66
0.53402
142.36
3.59


16
1416.8939
0.1200



142.38



17
131.1937
13.9916
1.49700
81.64
0.53714
141.26
3.65


18
356.8292
DD[18]



140.77



19
316.4461
3.4818
1.49700
81.64
0.53714
134.55



20
5633.1424
DD[20]



133.47



*21 
8447.2456
1.8000
1.90043
37.37
0.57668
74.88



22
51.4998
8.4400



74.09



23
−83.7200
1.6000
1.63246
63.77
0.54215
47.93



24
355.9513
3.6053



44.83



25
−133.8395
7.2470
1.59270
35.31
0.59336
44.83



26
−40.2135
1.5000
1.59282
68.62
0.14414
46.35



27
−170.3513
0.1201



47.03



28
133.4296
10.4051
1.67300
38.26
0.57580
47.04



29
−61.5853
1.5000
1.90043
37.37
0.57668
52.15



30
−990.5637
4.5118



52.37



31
−849.5464
3.7795
1.78880
28.43
0.60092
52.37



32
−135.1239
DD[32]



53.81



33
−80.2262
1.8100
1.49700
81.64
0.53714
55.35



34
137.4842
3.2131
1.80518
25.43
0.61027
57.12



35
314.3842
DD[35]



60.38

















TABLE 37B







Example 13













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.5001



60.38


37
368.5249
5.4430
1.80400
46.60
0.55755
60.60


38
−185.8917
0.1200



61.65


39
144.9291
13.4776
1.56883
56.04
0.54853
62.97


40
−66.5849
1.8000
1.83400
37.16
0.57759
63.43


41
−683.9448
2.5000



63.15


42
60.1964
15.5316
1.53775
74.70
0.53936
63.15


43
−115.3519
1.8100
1.54072
47.23
0.56511
63.42


44
−456.4774
0.1200



62.51


45
42.4155
12.7882
1.49700
81.64
0.53714
62.50


46
−220.4897
1.6000
1.91082
35.25
0.58224
52.63


47
44.1370
6.1916



50.44


48
566.4086
8.1145
1.80518
25.43
0.61027
44.23


49
−44.1956
1.4100
1.78800
47.35
0.55597
44.11


50
−113.9116
3.5878



43.74


51
46.7283
5.8790
1.49700
81.64
0.53714
43.74


52
−260.7841
0.0369



42.70


53
429.6595
1.2000
1.84850
43.79
0.56197
36.05


54
22.11894
13.054
1.48749
70.24
0.53007
34.39


55
−35.30710
1.200
1.81600
46.59
0.55661
30.95


56
63.63414
15.552



30.41


57
65.41679
4.106
1.67300
38.26
0.57580
30.41


58
544.15168
10.000



30.67


59

2.650
1.51633
64.14


60

63.402
















TABLE 38







Example 13













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
50.182
153.056
386.906



Bf
75.150
75.150
75.150



FNo.
3.27
3.27
3.28



2ω(°)
50.2
16.6
6.8



Ims
23.4
23.4
23.4



DD[18]
2.108
50.708
81.734



DD[20]
1.692
26.851
29.271



DD[32]
100.856
27.569
27.853



DD[35]
37.598
37.127
3.396

















TABLE 39







Example 13











Sn
1
21







KA
 1.0000000E+00
 1.0000000E+00



A4
 1.2770064E−08
 2.5682555E−07



A6
 9.9582435E−12
−8.0409658E−09



A8
−1.0700116E−14
 1.3472939E−10



A10
 2.3712566E−18
−1.2323956E−12



A12
 5.5363788E−21
 6.2406660E−15



A14
−6.3850349E−24
−1.4228254E−17



A16
 3.3426389E−27
−1.4701431E−20



A18
−9.6801893E−31
 1.7570664E−22



A20
 1.3183479E−34
−3.8231765E−25



A22
 6.7387458E−39
−1.8534199E−29



A24
−5.9339965E−42
 1.5867543E−30



A26
 1.0222996E−45
−3.1296884E−33



A28
−8.2190323E−50
 2.6759087E−36



A30
 2.6650298E−54
−8.9548630E−40










Example 14


FIG. 30 shows a configuration and movement loci of the variable magnification optical system of Example 14. The variable magnification optical system in Example 14 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a positive refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a negative refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2 and a third lens group G3. The negative movable lens group GN consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of one lens L2a. The third lens group G3 consists of seven lenses L3a to L3g in order from the object side to the image side. The fourth lens group G4 consists of two lenses L4a and L4b in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and fourteen lenses L5a to L5n in order from the object side to the image side.


Regarding the variable magnification optical system of Example 14, Tables 40A and 40B show the basic lens data, Table 41 shows the specifications and the variable surface spacings, Table 42 shows the aspherical coefficients, and FIG. 31 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 40A







Example 14














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
1293.92423
4.500
1.77250
49.60
0.53531
149.83
4.23


 2
180.82749
21.544



149.83



 3
−325.54926
3.900
1.77250
49.60
0.55212
147.00
4.23


 4
222.50454
0.406



135.69



 5
211.34135
8.945
1.84666
23.84
0.55212
135.04
3.50


 6
587.01026
6.471



133.68



 7
798.81429
12.225
1.59282
68.62
0.62012
134.09
4.13


 8
−295.33225
0.120



133.90



 9
170.29518
13.759
1.49700
81.64
0.54414
131.25
3.65


10
3907.11715
0.120



131.25



11
272.83622
3.800
1.84666
23.84
0.53714
128.11
3.50


12
144.48756
40.053



127.34



13
329.65569
11.179
1.43875
94.66
0.62012
123.06
3.59


14
−426.38305
0.120



118.98



15
220.6109
10.3612
1.43875
94.66
0.53402
117.97
3.59


16
−3673.3651
0.1201



118.20



17
154.0397
9.5433
1.49700
81.64
0.53402
119.07
3.65


18
469.1701
DD[18]



118.86



19
167.8602
8.0951
1.49700
81.64
0.53714
116.56



20
1044.0614
DD[20]



115.90



*21 
542.4660
1.8000
1.90043
37.37
0.53714
100.88



22
44.9066
10.0147



100.09



23
−66.6426
1.6000
1.63246
63.77
0.57668
50.05



24
124.4449
4.7489



41.36



25
−145.9557
5.6467
1.59270
35.31
0.54215
44.13



26
−45.5006
1.5100
1.58886
62.58

41.00



27
−160.7813
0.5151


0.59336
44.34



28
157.7734
10.6391
1.67300
38.26
0.54205
44.35



29
−42.9387
1.5000
1.90043
37.37

46.28



30
−114.5669
0.1200


0.57580
46.52



31
−1332.4921
2.5918
1.90006
34.46
0.57668
46.52



32
−188.0122
DD[32]



47.97



33
−66.5967
1.8100
1.49700
81.64
0.58551
48.19



34
144.9400
2.9224
1.80518
25.43

48.41



35
514.5830
DD[35]


0.53714
50.87

















TABLE 40B







Example 14













Sn
R
D
Nd
νd
θgF
ED
















36(St)

1.5000


0.61027
50.87


37
378.4574
3.8238
1.84674
33.82

51.11


38
−228.4897
0.1200



51.95


39
131.4780
11.5149
1.56883
56.04
0.58885
52.98


40
−56.0385
1.8000
1.83400
37.16

53.62


41
−447.6902
2.5000


0.54853
53.44


42
60.3416
14.0529
1.53775
74.70
0.57759
53.44


43
−137.7820
1.8100
1.54072
47.23

54.51


44
−163.5126
0.1200


0.53936
52.94


45
41.0665
12.2139
1.49700
81.64
0.56511
52.94


46
−93.6604
1.6000
1.95000
32.78

45.74


47
42.9905
6.3157


0.53714
43.30


48
−281.1713
12.3228
1.80518
25.43
0.58894
38.70


49
−30.9889
1.4000
1.84199
43.80

38.74


50
−61.7263
6.0218


0.61027
38.92


51
41.7224
9.9892
1.49700
81.64
0.56255
38.92


52
−67.1105
0.6259



39.22


53
−143.0786
1.2000
1.84850
43.79
0.53714
33.09


54
20.42273
18.475
1.48749
70.24

29.88


55
−27.07814
1.200
1.86215
41.78
0.56197
27.43


56
254.88111
14.471


0.53007
27.40


57
43.03289
3.174
1.67300
38.26
0.56660
27.40


58
68.87985
40.496



28.61


59

2.650
1.51633
64.14


60

0.997
















TABLE 41







Example 14













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
36.234
110.514
279.364



Bf
43.241
43.241
43.241



FNo.
3.27
3.27
3.27



2ω(°)
68.2
23.0
9.4



Ims
23.4
23.4
23.4



DD[18]
1.014
20.114
28.105



DD[20]
1.249
56.804
80.974



DD[32]
81.365
7.391
12.131



DD[35]
40.207
39.526
2.626

















TABLE 42







Example 14










Sn
21







KA
 1.0000000E+00



A4
 7.6072258E−07



A6
−1.8123448E−09



A8
 2.6415850E−11



A10
−2.2480917E−13



A12
 1.1568741E−15



A14
−3.6850778E−18



A16
 6.8056804E−21



A18
−4.8710434E−24



A20
−6.1399678E−27



A22
 1.4097486E−29



A24
−5.3494798E−34



A26
−2.2845342E−35



A28
 2.4742493E−38



A30
−8.5871607E−42










Example 15


FIG. 32 shows a configuration and movement loci of the variable magnification optical system of Example 15. The variable magnification optical system in Example 15 consists of, in order from the object side to the image side, a first lens group G1 having a positive refractive power, a second lens group G2 having a negative refractive power, a third lens group G3 having a negative refractive power, a fourth lens group G4 having a positive refractive power, and a fifth lens group G5 having a positive refractive power.


During changing magnification, the first lens group G1 and the fifth lens group G5 remain stationary with respect to the image plane Sim, and the second lens group G2, the third lens group G3, and the fourth lens group G4 move along the optical axis Z by changing the spacing from the adjacent lens groups. The middle group GM consists of a second lens group G2. The negative movable lens group GN consists of a third lens group G3. The positive movable lens group consists of a fourth lens group G4.


The first lens group G1 consists of a first A subgroup G1A, a first B subgroup G1B, and a first C subgroup G1C in order from the object side to the image side. The focus group is the first B subgroup G1B. The first A subgroup G1A consists of three lenses L1a to L1c in order from the object side to the image side. The first B subgroup G1B consists of three lenses L1d to L1f in order from the object side to the image side. The first C subgroup G1C consists of three lenses L1g to L1i in order from the object side to the image side.


The second lens group G2 consists of seven lenses L2a to L2g in order from the object side to the image side. The third lens group G3 consists of two lenses L3a and L3b in order from the object side to the image side. The fourth lens group G4 consists of three lenses L4a to L4c in order from the object side to the image side. The fifth lens group G5 consists of an aperture stop St and eleven lenses L5a to L5k in order from the object side to the image side.


Regarding the variable magnification optical system of Example 15, Tables 43A and 43B show the basic lens data, Table 44 shows the specifications and the variable surface spacings, Table 45 shows the aspherical coefficients, and FIG. 33 shows a diagram of aberrations in a state in which the infinite distance object is in focus.









TABLE 43A







Example 15














Sn
R
D
Nd
vd
θgF
ED
Sg

















 1
1342.19576
3.700
1.77250
49.60
0.53531
121.00
4.23


 2
162.25976
18.754



113.58



 3
−223.51842
3.500
1.85199
42.69
0.55212
113.19
4.81


 4
314.18830
0.121



114.38



 5
278.51041
6.972
1.84666
23.84
0.56463
114.78
3.50


 6
1656.17553
5.808



114.88



 7
3292.48069
10.063
1.59282
68.62
0.62012
115.70
4.13


 8
−222.73955
0.120



116.15



 9
209.55339
12.490
1.49700
81.64
0.54414
117.55
3.65


10
−755.75760
0.120



117.32



11
258.45005
3.000
1.84666
23.84
0.53714
114.88
3.50


12
153.12260
29.251



113.58



13
248.73941
13.918
1.49700
81.54
0.62012
118.89
3.62


14
−368.66208
0.127



118.98



15
166.82812
12.956
1.49700
81.54
0.53748
117.49
3.62


16
−4539.95216
0.120



116.98



17
129.14004
9.382
1.49700
81.54
0.53748
111.48
3.62


18
303.80387
DD[18]



110.43



*19 
−415.17314
1.800
1.91082
35.25
0.53748
40.37



20
38.45720
6.571



36.75



21
−141.54498
1.600
1.84850
43.79
0.58224
36.70



22
154.99727
2.923



37.06



23
−169.96739
8.693
1.68648
36.26
0.56197
37.36



24
−26.77275
1.500
1.86730
34.66

37.95



25
−140.23411
0.120


0.58616
41.57



26
−338.43238
10.027
1.70830
30.73
0.58585
42.19



27
−31.36026
1.500
1.87639
40.36

43.28



28
−79.86113
0.120


0.60173
47.53



29
268.13587
7.530
1.57871
40.24
0.56970
50.84



30
−70.04669
DD[30]



51.33



31
−67.35994
1.810
1.49700
81.64
0.57891
53.00



32
348.20748
2.917
1.80518
25.43

55.76



33
−700.36344
DD[33]


0.53714
56.07



34
262.52220
4.954
1.75485
52.51
0.61027
62.21



35
−275.94247
0.121



62.25



36
154.69560
11.990
1.58728
47.54
0.54748
61.65



37
−70.70324
1.800
1.81980
43.96

61.22



38
−847.11379
DD[38]


0.56364
60.66

















TABLE 43B







Example 15













Sn
R
D
Nd
νd
θgF
ED
















39(St)

1.523


0.56298
57.51


40
72.42845
9.405
1.53775
74.70

58.52


41
−255.53335
1.800
1.72559
28.72

58.17


42
−180.95542
3.472


0.53936
57.98


43
60.55588
10.847
1.49700
81.64
0.60724
51.49


44
−117.63585
1.600
1.91776
34.81

49.84


45
53.05283
48.123


0.53714
45.96


46
−5703.98718
9.649
1.80518
25.43
0.58403
49.44


47
−43.50207
1.400
1.88491
28.21

49.57


48
−86.67784
4.749


0.61027
50.22


49
44.37168
11.090
1.49700
81.64
0.60515
45.52


50
−124.40622
0.431



44.05


51
−161.45851
1.200
1.84850
43.79
0.53714
43.01


52
28.63255
17.360
1.48749
70.24

39.00


53
−49.93815
1.200
1.78912
33.45
0.56197
38.64


54
104.17511
4.769


0.53007
39.25


55
52.97077
6.197
1.67300
38.26
0.59155
42.86


56
129.19174
56.329



42.55


57

2.650
1.51633
64.14


58

1.012
















TABLE 44







Example 15













WIDE
MIDDLE
TELE
















Zr
1.0
3.0
7.7



f
36.246
110.551
279.459



Bf
59.089
59.089
59.089



FNo.
3.27
3.27
3.28



2ω(°)
69.0
23.0
9.4



Ims
23.4
23.4
23.4



DD[18]
2.734
78.918
110.797



DD[30]
83.685
1.866
21.219



DD[33]
39.510
43.276
1.177



DD[38]
9.220
11.090
1.957

















TABLE 45







Example 15










Sn
19







KA
 1.0000000E+00



A4
 2.0565523E−06



A6
−5.6853356E−09



A8
 1.5134896E−10



A10
−2.3325577E−12



A12
 2.0176465E−14



A14
−9.8333039E−17



A16
 2.1453611E−19



A18
 2.6418607E−22



A20
−2.7611169E−24



A22
 5.6162683E−27



A24
 1.1868486E−30



A26
−2.2634873E−32



A28
 3.5254923E−35



A30
−1.8405678E−38










Tables 46 to 48 show the corresponding values of Conditional Expressions (1) to (24) of the variable magnification optical system of Examples 1 to 15. In Tables 46 to 48, the columns where there is no corresponding item each show “-”. The corresponding values of Conditional Expression (24) of Example 7 are values relating to the lens L5i.










TABLE 46







Expression














Number

Example 1
Example 2
Example 3
Example 4
Example 5
















 (1)
f1/(ft/FNt)
1.568
1.410
1.551
1.358
1.410


 (2)
Ims/f1
0.128
0.142
0.129
0.148
0.142


 (3)
|Ims/ffz|
0.329
0.136
0.324
0.340
0.326


 (4)
1/βfzt
−0.051
0.004
−0.057
−0.018
−0.006


 (5)
|Dpfz/ffz|
1.638
0.651
1.614
1.520
1.539


 (6)
fMw/fN
0.446
0.468
0.435
0.405
0.453


 (7)
νNdif
57.81
69.23
57.81
69.23
69.23


 (8)
θM + 0.0018 × νM
0.056
0.036
0.056
0.056
0.036



−0.64833







 (9)
(RMnr + RMf)/(RMnr − RMf)
−0.453
−0.766
−0.403
−0.765
−0.737


(10)
DpM/{(ft/fw) × Ims}
0.646
0.620
0.646
0.580
0.613


(11)
EDMf/EDMr
1.529
2.239
2.462
2.244
1.133


(12)
|(HMfb/HMfa)
2.173
2.226
2.174
2.203
2.256



/(HMrb/HMra)|







(13)
Ims/fE
0.371
0.309
0.378
0.343
0.308


(14)
θE + 0.0018 × vνE
0.056
0.056
0.056
0.056
0.056



−0.64833







(15)
ave (Sgf/Nf)
2.25
2.28
2.25
2.33
2.28


(16)
Nfmax
1.85478
1.84666
1.85478
1.84666
1.84666


(17)
(Rpf − Rpr)/(Rpf + Rpr)
−0.173
−0.275
−0.102
−0.315
−0.300


(18)
Ims/f1C
0.145
0.157
0.145
0.158
0.158


(19)
f1/f1B
0.650
0.576
0.634
0.545
0.583


(20)
θ1Bp + 0.0018 × ν1Bp
0.134
0.056
0.056
0.056
0.056



−0.64833







(21)
ν1Bn
24.80
23.84
24.80
23.78
23.84


(22)
ν1Ap
23.83
23.84
23.83
23.78
23.84


(23)
(REf + REr)/(REf − REr)
0.398
0.234
0.401
0.313
0.247


(24)
dN/dT






















TABLE 47







Expression














Number

Example 6
Example 7
Example 8
Example 9
Example 10
















 (1)
f1/(ft/FNt)
1.314
1.315
1.503
1.524
1.444


 (2)
Ims/f1
0.152
0.152
0.183
0.132
0.134


 (3)
|Ims/ffz|
0.364
0.359
0.355
0.353
0.370


 (4)
1/βfzt
−0.011
−0.013
−0.035
−0.041
−0.143


 (5)
|Dpfz/ffz|
1.582
1.573
1.648
1.723
1.862


 (6)
fMw/fN
0.494
0.425
0.463
0.448
0.321


 (7)
νNdif
54.00
70.83
66.23
56.12
56.12


 (8)
θM + 0.0018 × νM
0.056
0.056
0.056
0.036
0.006



−0.64833







 (9)
(RMnr + RMf)/(RMnr − RMf)
−0.281
−0.198
0.010
−0.129
−0.289


(10)
DpM/{(ft/fw) × Ims}
0.563
0.567
0.601
0.626
0.645


(11)
EDMf/EDMr
2.535
2.368
2.375
2.723
1.108


(12)
|(HMfb/HMfa)
2.052
2.068
1.904
1.805
1.605



/(HMrb/HMra)|







(13)
Ims/fE
0.334
0.292
0.316
0.302
0.315


(14)
θE + 0.0018 × vνE
0.057
0.057
0.057
0.057
0.057



−0.64833







(15)
ave (Sgf/Nf)
2.27
2.33
2.34
2.34
2.27


(16)
Nfmax
1.85478
1.84666
1.84666
1.81008
1.80518


(17)
(Rpf − Rpr)/(Rpf + Rpr)
−0.575
−1.256
−5.926
−4.788



(18)
Ims/f1C
0.185
0.162
0.184
0.146
0.144


(19)
f1/f1B
0.562
0.524
0.484
0.586
0.607


(20)
θ1Bp + 0.0018 × ν1Bp
0.056
0.056
0.056
0.057
0.057



−0.64833







(21)
ν1Bn
24.80
23.84
23.84
26.49
25.42


(22)
ν1Ap
23.83
23.84
23.84
23.83
23.83


(23)
(REf + REr)/(REf − REr)
0.316
0.316
0.013
−0.163
−0.166


(24)
dN/dT

3.6 × 10−6




















TABLE 48







Expression














Number

Example 11
Example 12
Example 13
Example 14
Example 15
















 (1)
f1/(ft/FNt)
1.635
1.470
1.412
2.205
1.511


 (2)
Ims/f1
0.128
0.142
0.141
0.125
0.182


 (3)
|Ims/ffz|
0.365
0.378
0.395
0.383
0.379


 (4)
1/βfzt
−0.118
−0.062
−0.087
−0.068
−0.129


 (5)
|Dpfz/ffz|
2.071
1.695
1.811
1.750
1.752


 (6)
fMw/fN
0.403
0.475
0.423
0.495
0.328


 (7)
νNdif
56.12
56.12
56.21
56.21
56.12


 (8)
θM + 0.0018 × νM
0.036
0.036
0.036
0.036
−0.008



−0.64833







 (9)
(RMnr + RMf)/(RMnr − RMf)
−0.101
−0.119
−0.238
−0.195
−0.573


(10)
DpM/{(ft/fw) × Ims}
0.697
0.613
0.594
0.592
0.599


(11)
EDMf/EDMr
1.397
1.429
2.500
2.430
0.720


(12)
|(HMfb/HMfa)
1.648
1.987
2.120
2.233
2.099



/(HMrb/HMra)|







(13)
Ims/fE
0.326
0.390
0.357
0.421
0.116


(14)
θE + 0.0018 × vνE
0.057
0.057
0.036
0.036
0.036



−0.64833







(15)
ave (Sgf/Nf)
2.34
2.37
2.31
2.31
2.31


(16)
Nfmax
1.84666
1.81766
1.84666
1.84666
1.84666


(17)
(Rpf − Rpr)/(Rpf + Rpr)
−0.981
−1.282
−0.894
−0.723



(18)
Ims/f1C
0.138
0.152
0.160
0.153
0.199


(19)
f1/f1B
0.616
0.587
0.631
0.568
0.485


(20)
θ1Bp + 0.0018 × ν1Bp
0.057
0.057
0.056
0.056
0.036



−0.64833







(21)
ν1Bn
23.78
28.38
23.84
23.84
23.84


(22)
ν1Ap
23.83
23.83
23.84
23.84
23.84


(23)
(REf + REr)/(REf − REr)
0.337
0.388
0.329
0.247
−0.428


(24)
dN/dT














As can be seen from the data described above, the variable magnification optical systems of Examples 1 to 15 each have high optical performance with various aberrations satisfactorily corrected while being configured to have a small size. Further, the variable magnification optical systems of Examples 1 to 15 each have the F number at the telephoto end smaller than 3.4 and have almost no F drop while having a zoom magnification of seven times or more and achieving an increase in magnification.


Next, an imaging apparatus according to an embodiment of the present disclosure will be described. FIG. 34 shows a schematic configuration diagram of an imaging apparatus 100 using the variable magnification optical system 1 according to the embodiment of the present disclosure as an example of the imaging apparatus according to the embodiment of the present disclosure. Examples of the imaging apparatus 100 include a movie shooting camera, a broadcasting camera, a video camera, a surveillance camera, and the like.


The imaging apparatus 100 includes a variable magnification optical system 1, a filter 2 disposed on the image side of the variable magnification optical system 1, and an imaging element 3 disposed on the image side of the filter 2. It should be noted that FIG. 34 schematically shows a plurality of lenses comprising the variable magnification optical system 1.


The imaging element 3 converts an optical image formed by the variable magnification optical system 1 into an electric signal, and for example, a charge coupled device (CCD) or a complementary metal oxide semiconductor (CMOS) or the like can be used. The imaging element 3 is disposed such that the imaging surface thereof coincides with the image plane of the variable magnification optical system 1.


The imaging apparatus 100 also comprises a signal processing unit 5 that calculates and processes an output signal from the imaging element 3, a display unit 6 that displays an image formed by the signal processing unit 5, a changing magnification controller 7 that controls zooming of the variable magnification optical system 1, and a focusing controller 8 that controls focusing of the variable magnification optical system 1. Although FIG. 34 shows only one imaging element 3, a so-called three-plate imaging apparatus having three imaging elements may be used.


The technology of the present disclosure has been hitherto described through embodiments and examples, but the technology of the present disclosure is not limited to the above-mentioned embodiments and examples, and may be modified into various forms. For example, values such as the radius of curvature, the surface spacing, the refractive index, the Abbe number, and the aspherical coefficient of each lens are not limited to the values shown in the numerical examples, and different values may be used therefor.


variable magnification optical system

Claims
  • 1. A variable magnification optical system consisting of, in order from an object side to an image side: a first lens group that has a positive refractive power; a plurality of lens groups; and a final lens group that has a positive refractive power, wherein during changing magnification, a spacing between the first lens group and the lens group closest to the object side among the plurality of lens groups changes, all spacings between adjacent lens groups in the plurality of lens groups change, and a spacing between the lens group closest to the image side among the plurality of lens groups and the final lens group changes.
  • 2. The variable magnification optical system according to claim 1, wherein assuming that a focal length of the first lens group in a state in which an infinite distance object is in focus is f1,a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, andan open F number of the variable magnification optical system at the telephoto end in the state in which the infinite distance object is in focus is FNt,Conditional Expression (1) is satisfied, which is represented by
  • 3. The variable magnification optical system according to claim 1, wherein assuming that a maximum image height is Ims, anda focal length of the first lens group in a state in which an infinite distance object is in focus is f1,Conditional Expression (2) is satisfied, which is represented by
  • 4. The variable magnification optical system according to claim 1, wherein a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group, andassuming that a focal length of the fz group is ffz, anda maximum image height is Ims,Conditional Expression (3) is satisfied, which is represented by
  • 5. The variable magnification optical system according to claim 1, wherein a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group, andassuming that a lateral magnification of the fz group at the telephoto end in the state in which the infinite distance object is in focus is βfzt,Conditional Expression (4) is satisfied, which is represented by
  • 6. The variable magnification optical system according to claim 1, wherein a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, and a movable lens group having a maximum absolute value of a ratio of a lateral magnification of a movable lens group at a telephoto end to a lateral magnification of the movable lens group at a wide angle end among the movable lens groups included in the variable magnification optical system in a state in which an infinite distance object is in focus is a fz group, andassuming that a focal length of the fz group is ffz, anda difference in an optical axis direction between a position of the fz group at the wide angle end and a position of the fz group at the telephoto end is Dpfz,Conditional Expression (5) is satisfied, which is represented by
  • 7. The variable magnification optical system according to claim 1, wherein the plurality of lens groups include, in order from a position closest to the object side to the image side, a middle group, which includes one or more lens groups and has a negative refractive power as a whole, and a negative movable lens group, which has a negative refractive power and moves during changing magnification, andthe negative movable lens group is positioned closest to the image side in the lens groups having negative refractive powers in the plurality of lens groups.
  • 8. The variable magnification optical system according to claim 7, wherein assuming that a focal length of the middle group at a wide angle end in a state in which an infinite distance object is in focus is fMw, anda focal length of the negative movable lens group is fN,Conditional Expression (6) is satisfied, which is represented by
  • 9. The variable magnification optical system according to claim 7, wherein the negative movable lens group includes one or more negative lenses and one or more positive lenses, andassuming that a maximum absolute value of a difference between an Abbe number of the negative lens included in the negative movable lens group based on a d line and an Abbe number of the positive lens included in the negative movable lens group based on the d line is μNdif, Conditional Expression (7) is satisfied, which is represented by
  • 10. The variable magnification optical system according to claim 7, wherein the middle group includes one or more positive lenses, andassuming that an Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the middle group based on the d line is νM and a partial dispersion ratio thereof between a g line and an F line is θM, Conditional Expression (8) is satisfied, which is represented by
  • 11. The variable magnification optical system according to claim 7, wherein assuming that a curvature radius of an image side surface of a negative lens closest to the object side in the middle group is RMnr, anda curvature radius of an object side surface of a lens disposed adjacent to the image side of a negative lens closest to the object side in the middle group is RMf,Conditional Expression (9) is satisfied, which is represented by
  • 12. The variable magnification optical system according to claim 7, wherein assuming that a difference in an optical axis direction between a position of a lens surface closest to the image side in the middle group at a wide angle end and a position of a lens surface closest to the image side in the middle group at a telephoto end in a state in which an infinite distance object is in focus is DpM,a focal length of the variable magnification optical system at a wide angle end in the state in which the infinite distance object is in focus is fw,a focal length of the variable magnification optical system at a telephoto end in the state in which the infinite distance object is in focus is ft, anda maximum image height is Ims,Conditional Expression (10) is satisfied, which is represented by
  • 13. The variable magnification optical system according to claim 7, wherein assuming that an effective diameter of a lens surface closest to the object side in the middle group in a state in which an infinite distance object is in focus is EDMf, andan effective diameter of a lens surface closest to the image side in the middle group in the state in which the infinite distance object is in focus is EDMr,Conditional Expression (11) is satisfied, which is represented by
  • 14. The variable magnification optical system according to claim 7, wherein assuming that a height of a principal ray from an optical axis at a maximum image height on a lens surface closest to the object side in the middle group at the wide angle end in a state in which an infinite distance object is in focus is HMfb,a height of an on-axis marginal ray from the optical axis on the lens surface closest to the object side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMfa,a height of the principal ray from the optical axis at a maximum image height on a lens surface closest to the image side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMrb, anda height of the on-axis marginal ray from the optical axis on the lens surface closest to the image side in the middle group at the wide angle end in the state in which the infinite distance object is in focus is HMra,Conditional Expression (12) is satisfied, which is represented by
  • 15. The variable magnification optical system according to claim 7, wherein the plurality of lens groups consist of the middle group and the negative movable lens group.
  • 16. The variable magnification optical system according to claim 7, wherein the middle group consists of a front lens group having a positive refractive power and a rear lens group having a negative refractive power in order from the object side to the image side, anda spacing between the front lens group and the rear lens group changes during changing magnification.
  • 17. The variable magnification optical system according to claim 7, wherein groups, which are included in the plurality of lens groups and move by changing a spacing from an adjacent lens group during changing magnification, consist of, in order from the object side to the image side, the middle group, the negative movable lens group, and a positive movable lens group having a positive refractive power.
  • 18. The variable magnification optical system according to claim 1, wherein assuming that a maximum image height is Ims, anda focal length of the final lens group is fE,Conditional Expression (13) is satisfied, which is represented by
  • 19. The variable magnification optical system according to claim 1, wherein assuming that an Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the final lens group based on the d line is νE and a partial dispersion ratio thereof between a g line and an F line is θE, Conditional Expression (14) is satisfied, which is represented by
  • 20. The variable magnification optical system according to claim 1, wherein the variable magnification optical system includes a focus group that performs focusing by moving along an optical axis, andassuming that a specific gravity of each lens in the focus group is Sgf and a refractive index thereof at a d line is Nf,an average value of Sgf/Nf of all lenses in the focus group is ave(Sgf/Nf), and a maximum value of refractive indexes of all the lenses in the focus group at the d line is Nfmax,Conditional Expressions (15) and (16) are satisfied, which are represented by
  • 21. The variable magnification optical system according to claim 1, wherein in a case where a lens group that moves by changing a spacing from an adjacent lens group during changing magnification is a movable lens group, the number of the movable lens groups included in the variable magnification optical system is three or more, andthe movable lens group closest to the object side among the movable lens groups included in the variable magnification optical system has a positive refractive power.
  • 22. The variable magnification optical system according to claim 21, wherein the movable lens group closest to the object side among the movable lens groups included in the variable magnification optical system consists of one positive lens having a convex surface facing toward the object side.
  • 23. The variable magnification optical system according to claim 22, wherein assuming that a curvature radius of an object side surface of the positive lens having the convex surface facing toward the object side is Rpf, anda curvature radius of an image side surface of the positive lens having the convex surface facing toward the object side is Rpr,Conditional Expression (17) is satisfied, which is represented by
  • 24. The variable magnification optical system according to claim 1, wherein the first lens group consists of, in order from the object side to the image side, a first A subgroup having a negative refractive power, a first B subgroup having a positive refractive power, and a first C subgroup having a positive refractive power, andfocusing is performed by moving the first B subgroup along an optical axis.
  • 25. The variable magnification optical system according to claim 24, wherein assuming that a maximum image height is Ims, anda focal length of the first C subgroup is f1C,Conditional Expression (18) is satisfied, which is represented by
  • 26. The variable magnification optical system according to claim 24, wherein assuming that a focal length of the first lens group is f1, anda focal length of the first B subgroup is f1B,Conditional Expression (19) is satisfied, which is represented by
  • 27. The variable magnification optical system according to claim 24, wherein the first B subgroup includes one or more positive lenses and one or more negative lenses, andassuming thatan Abbe number of the positive lens, of which an Abbe number based on a d line is maximum, among the positive lenses included in the first B subgroup based on the d line is ν1Bp, and a partial dispersion ratio thereof between a g line and an F line is θ1Bp, anda minimum value of Abbe numbers of all the negative lenses included in the first B subgroup based on the d line is ν1Bn,Conditional Expressions (20) and (21) are satisfied, which are represented by
  • 28. The variable magnification optical system according to claim 24, wherein the first A subgroup includes two or more negative lenses of which Abbe numbers based on a d line are 50 or more, andassuming that a minimum value of Abbe numbers of all the positive lenses included in the first A subgroup based on the d line is ν1Ap, Conditional Expression (22) is satisfied, which is represented by
  • 29. The variable magnification optical system according to claim 1, wherein the first lens group remains stationary with respect to an image plane during changing magnification.
  • 30. The variable magnification optical system according to claim 1, wherein the final lens group remains stationary with respect to an image plane during changing magnification, anda stop is disposed closest to the object side in the final lens group.
  • 31. The variable magnification optical system according to claim 30, wherein in a case where one lens component is one single lens or one group of cemented lenses,a lens component disposed adjacent to the image side of the stop has a biconvex shape.
  • 32. The variable magnification optical system according to claim 31, wherein assuming that a curvature radius of a surface closest to the object side of the lens component disposed adjacent to the image side of the stop is REf, anda curvature radius of a surface closest to the image side of the lens component disposed adjacent to the image side of the stop is REr,Conditional Expression (23) is satisfied, which is represented by
  • 33. The variable magnification optical system according to claim 1, wherein assuming that a temperature coefficient of a relative refractive index of a lens in the final lens group at a d line in a range of 20° C. to 40° C. is dN/dT and a unit of dN/dT is ° C.−1,the final lens group includes one or more lenses respectively having an Abbe number based on the d line of 65 or more and satisfying Conditional Expression (24), which is represented by
  • 34. An imaging apparatus comprising the variable magnification optical system according to claim 1.
Priority Claims (2)
Number Date Country Kind
2021-008221 Jan 2021 JP national
2021-182841 Nov 2021 JP national