TUNABLE VARIABLE EMISSIVITY MATERIALS AND METHODS FOR CONTROLLING THE TEMPERATURE OF SPACECRAFT USING TUNABLE VARIABLE EMISSIVITY MATERIALS

Abstract
Tunable variable emissivity materials, methods for fabricating tunable variable emissivity materials, and methods for controlling the temperature of a spacecraft using tunable variable emissivity materials have been provided. In an exemplary embodiment, a variable emissivity material has the formula M1(1−(x+y))M2xM3yMnO3, wherein M1 comprises lanthanum, praseodymium, scandium, yttrium, neodymium or samarium, M2 comprises an alkali earth metal, M3 comprises an alkali earth metal that is not M2, and x, y, and (x+y) are less than 1. The material has a critical temperature (Tc) in the range of about 270 to about 320 K and a transition width is less than about 30 K.
Description

BRIEF DESCRIPTION OF THE DRAWINGS

The present invention will hereinafter be described in conjunction with the following drawing figures, wherein like numerals denote like elements, and wherein:



FIG. 1 is a schematic diagram of the atoms of a perovskite structure;



FIG. 2 is a graph of a ferromagnetic-paramagnetic transition of a variable emissivity material in accordance with an exemplary embodiment of the present invention;



FIG. 3 is a graph of a ferromagnetic-paramagnetic transition of La0.7Ba0.3MnO3;



FIG. 4 is a graph of a ferromagnetic-paramagnetic transition of La0.7Be0.3MnO3;



FIG. 5 is a graph of a ferromagnetic-paramagnetic transition of La0.5Ba0.25 Be0.25MnO3;



FIG. 6 is a contour map of the critical temperature Tc of La(1−(x−y))Bax BeyMnO3 based on the mole fraction of barium and beryllium;



FIG. 7 is a flow chart of a method for fabricating a variable emissivity material, in accordance with an exemplary embodiment of the present invention;



FIG. 8 is a flow chart of a method for fabricating a variable emissivity coating, in accordance with an exemplary embodiment of the present invention; and



FIG. 9 is a cross-sectional view of a substrate upon which is disposed a variable emissivity coating, in accordance with an exemplary embodiment of the present invention.





DETAILED DESCRIPTION OF THE INVENTION

The following detailed description of the invention is merely exemplary in nature and is not intended to limit the invention or the application and uses of the invention. Furthermore, there is no intention to be bound by any theory presented in the preceding background of the invention or the following detailed description of the invention.


The present invention is directed to various embodiments of a tunable variable emissivity material that can be fabricated to passively reduce the temperature extremes experienced by aerospace systems, such as satellites, high-altitude inflatables, deep-spacecraft, and the like. A material with a high emissivity efficiently radiates heat while a material with a low emissivity radiates less heat. A variable emissivity material is any material that, when heated above a critical temperature Tc, experiences a phase change that alters the material's emissivity. At Tc, the material transforms from a low emissivity metal into a high emissivity semiconductor. As a result of this behavior, the material tends to self-regulate its temperature near Tc, radiating heat at temperatures above Tc and retaining heat below Tc. The material can be applied to any surface where temperature control through radiative emission is required (e.g., satellite radiators).


In accordance with an exemplary embodiment of the present invention, a variable emissivity material can be represented by the following:





M1(1−(x+y))M2xM3yMnO3,


where M1 comprises lanthanum (La), scandium (Sc), yttrium (Y), praseodymium (Pr), neodymium (Nd), or samarium (Sm) and preferably is lanthanum. M2 is an alkali earth metal and M3 is an alkali earth metal that is not M2. In a preferred embodiment of the invention, M2 comprises beryllium (Be) or magnesium (Mg), more preferably Be, and M3 comprises barium (Ba), strontium (Sr), or calcium (Ca), more preferably Ba. The sum (x+y) is less than 1.


The variable emissivity material has a perovskite oxide structure 10, such as that illustrated in FIG. 1, having oxygen (O−2) atoms 12, manganese (Mn+3 or Mn+4) atoms 14, and rare earth or other +3 transition metal ions M1 16. A certain portion of the rare earth/+3 transition metal ions M1 16 are replaced with one of two different alkali earth metal ions, M2 and M3. The variable emissivity material undergoes a metal-insulator phase transition at a critical temperature Tc. Below Tc, the material is metallic and ferromagnetic and exhibits a low emissivity, that is, an emissivity ε of no greater than 0.5. At temperatures above Tc, the material behaves like a paramagnetic insulator with a high emissivity, that is ε of no less than about 0.6. Therefore, in the regime where thermal emission controls surface or structure temperature, the material tends to self regulate its temperature near Tc. Compared to a material with a constant ε, the variable emissivity material will radiate heat quickly at temperatures greater than Tc, thus cooling a substrate or structure upon which the material is disposed, and radiate heat slowly at temperatures below Tc, thus retaining heat. For space applications, it is desirable to maintain components or structures of spacecraft, such as electronic components or human occupants, at about room temperature, that is, about 270 K to about 320 K. Accordingly, in a preferred embodiment of the invention, the variable emissivity material has a Tc in the range of about 270 K to about 320 K. In a more preferred embodiment of the invention, the variable emissivity material has a Tc in the range of about 290 K to about 310 K.


The emissivity change at Tc is accompanied by a magnetic (ferromagnetic-paramagnetic) transition. Accordingly, it can be detected with a Superconducting Quantum Interference Device (SQUID). As the variable emissivity material is heated in the presence of a weak magnetic field, a large drop in the magnetic moment of the material will occur as it undergoes the ferromagnetic-paramagnetic transition. FIG. 2 is a graph 50 of this transition for a variable emissivity material of the present invention, with the x-axis 52 representing temperature (in degrees Kelvin) and the y-axis 54 representing the long moment (in electromagnetic units (emu)). The transition from the ferromagnetic to the paramagnetic state is indicated by the transition curve 56. The transition width 58 is the temperature difference that occurs when the slope of the curve 58 has about the highest magnitude. The critical temperature Tc 60 is the approximate temperature that occurs when the transition is at its half-way point. The narrower the transition width, the more the material will bias the substrate temperature towards Tc. In a preferred embodiment of the invention, the variable emissivity material has a transition width 58 of no more than about 30 K, more preferably no more than about 20 K.


The critical temperature Tc and the transition width of the variable emissivity material can be selected for or “tuned” to predetermined values by varying the identity and quantity of the alkali earth metal ions M2 and M3. For example, FIG. 3 is a graph 100 of the transition curve 102 of La0.7Ba0.3MnO3 and FIG. 4 is a graph 120 of the transition curve 122 of La0.7Be0.3MnO3. The x-axes in both figures, 110 and 130 respectively, represent the temperature of the material (in degrees Kelvin). The y-axes in the figures, 112 and 132 respectively, represent the long moment of the material (in electromagnetic units (emu)). The Tc 104 of La0.7Ba0.3MnO3 is approximately 295 K, while the Tc 124 of La0.7Be0.3MnO3 is only about 252 K. In contrast, the transition width 126 of La0.7Be0.3MnO3 is much narrower, about 25 K, than the transition width 106 of La0.7Ba0.3MnO3, which is about 70 K. For a given application, it may be desirable to fabricate a variable emissivity material that has the relatively higher Tc of La0.7Ba0.3MnO3 and the relatively narrow transition width of La0.7Be0.3MnO3. In accordance with an exemplary embodiment of the present invention, a variable emissivity material with a high Tc and a narrow transition width can be achieved with the specific selection of M2 and M3 and their respective mole fractions.


For example, in accordance with one embodiment of the invention, the variable emissivity material may be La0.5Ba0.25Be0.25MnO3. FIG. 5 is a graph 150 of the transition curve 160 of La0.5Ba0.25Be0.25MnO3. The x-axis 152 represents the temperature of the material in degrees Kelvin and the y-axis 154 represents the long moment of the material in electromagnetic units (emu). As illustrated in FIG. 5, La0.5Ba0.25Be0.25MnO3 has a relatively high Tc 156 of about 315 K and yet has a relatively narrow transition width 158 of about 25 to 30 K. FIG. 6 is a contour map 200 illustrating that by varying the mole fraction of barium (x-axis 202) and beryllium (y-axis 204) in La0.5BaxBeyMnO3, Tc can be tuned to a desired value.



FIG. 7 illustrates a method 230 for using a variable emissivity material M1(1−(x+y))M2xM3yMnO3 to control the temperature of a spacecraft. As described above, the variable emissivity material can comprise lanthanum (La), scandium (Sc), yttrium (Y), praseodymium (Pr), neodymium (Nd), or samarium (Sm), and preferably comprises lanthanum. The method comprises the step of selecting the identity of M2 and M3 and the quantity of M2 and M3, that is, x and y (step 232), and, if not already selected, M1. Preferably, the identity and quantity of M2 and M3 are selected so that the resulting variable emissivity material has a predetermined critical temperature Tc and a predetermined transition width. Once M2, M3, x, and y are selected, the variable emissivity material is formed (step 234) and is applied to a component of a spacecraft (step 236).


The variable emissivity material, in accordance with various embodiments of the present invention, may be formed using any suitable method. For example, the variable emissivity material may be synthesized using ion-beam doping of M1MnO3 films with M2 and M3 atoms, oxidation of vapor-deposited stoichiometric metal films of M1, M2, M3 and Mn, or reaction under mechanically energetic conditions such as ball-milling, jar milling, or hand-grinding of reactant metal oxides M1O, M22O3, M32O3, and MnO3, followed by post-annealed compositions.



FIG. 8 illustrates a method 250 for synthesizing a variable emissivity material and a variable emissivity coating comprising a variable emissivity material, in accordance with exemplary embodiments of the present invention. Method 250 comprises the step of combining acetylacetonate (C5H7O2) (“acac”) ligand-complexed metal ions in a solvent according to the following equation:





(1−(x+y))M1(acac)3+xM2(acac)2+yM3(acac)2+Mn(acac)3→M1(1−(x+y))M2xM3yMnO3,


(step 252), to form a variable emissivity material. The solvent may be any material capable of dissolving the reactants. To form a film, the variable emissivity material may be deposited onto a binder, such as film of poly(vinyl alcohol) (PVA), and dried (step 254). The variable emissivity film then may be heat-treated to further crystallize the product (step 256). Alternatively, if the variable emissivity material is to be in the form of a powder, the material may be mixed with a PVA aqueous solution and dried (step 254). The mixture then is heat-treated to further crystallize the product (step 256). The heat-treated powder then may be mixed with an organic or inorganic binder so that it can be rolled, painted, sprayed, spin-coated, or the like onto a substrate or so that a substrate can be dipped in the mixture (step 258). As illustrated in FIG. 9, the methods 230 and 250 result in a variable emissivity coating 240 disposed on a substrate 242, where the coating comprises a variable emissivity material 244 that is coupled to the substrate via a binder 246.


The following is an example of the preparation of La0.5Ba0.25Be0.25MnO3 film, in accordance with an exemplary embodiment of the present invention. Lanthanum acetylacetonate (La(acac)3.H20), manganese acetylacetonate (Mn(acac)3), beryllium acetylacetonate (Be(acac)2) and barium acetylacetonate (Ba(acac)2) may be dissolved in a mixed 4:1 solution of propanoic acid and methanol to form a variable emissivity material. To form a film, a PVA aqueous solution (about 15%) may be spin-coated onto a substrate, and the variable emissivity material may be spin-coated on the PVA film, followed by drying at 150° C. for about 10 hours. The resulting film then may be heat-treated in air at 400 to 600° C., preferably 450 to 550° C. To form a powder, the perovskite product may be combined with a PVA aqueous solution until a viscous gel is formed (about 6 wt % PVA) and dried at about 150° C. for about 4 to about 10 hours. The resulting product then may be heat-treated in air at 1000° C. for about 5 hours. The heat-treated powder may be mixed with an inorganic or organic binder so that it can be rolled, painted, sprayed, spin-coated, or the like onto a substrate or so that a substrate can be dipped in the mixture. Suitable binders include potassium silicate, such as Kasil® available from PQ Corporation of Philadelphia, Pa., silicone-modified epoxy, polyurethane, poly(dimethylsiloxane), poly(dimethylsiloxane-co-methylphenylsiloxane), polyamide, Dow Corning® HC 2000, available from Dow Corning Corporation of Midland, Mich., or a combination thereof. For example, 300 g of the heat-treated powder may be mixed with 175 g of Kasil® and 100 g of H2O to form an inorganic-based paint.


Accordingly, a variable emissivity material, a method for fabricating a variable emissivity material, and a method for controlling the temperature of a spacecraft using a variable emissivity material have been presented. The variable emissivity material radiates heat quickly at temperatures above the material's critical temperature Tc and slowly at temperatures below Tc. The Tc and the transition width of the variable emissivity material can be tuned to desired values by the strategic selection of the identity and quantity of the components of the variable emissivity material. While at least one exemplary embodiment has been presented in the foregoing detailed description of the invention, it should be appreciated that a vast number of variations exist. It should also be appreciated that the exemplary embodiment or exemplary embodiments are only examples, and are not intended to limit the scope, applicability, or configuration of the invention in any way. Rather, the foregoing detailed description will provide those skilled in the art with a convenient road map for implementing an exemplary embodiment of the invention, it being understood that various changes may be made in the function and arrangement of elements described in an exemplary embodiment without departing from the scope of the invention as set forth in the appended claims and their legal equivalents.

Claims
  • 1. A variable emissivity material having the formula M1(1−(x+y))M2xM3yMnO3 wherein: M1 comprises lanthanum, scandium, yttrium, praseodymium, neodymium or samarium;M2 comprises an alkali earth metal;M3 comprises an alkali earth metal that is not M2; andx, y, and (x+y) are less than 1; and
  • 2. The variable emissivity coating of claim 1, wherein M2 comprises barium, strontium, or calcium.
  • 3. The variable emissivity coating of claim 1, wherein M3 comprises beryllium or magnesium.
  • 4. The variable emissivity coating of claim 1, wherein the variable emissivity material has a critical temperature (Tc) in the range of about 290 K to about 310 K.
  • 5. The variable emissivity material of claim 1, wherein the variable emissivity material has a transition width of no more than 20 K.
  • 6. A method for fabricating a variable emissivity material, the method comprising the steps of: selecting a first alkaline earth metal M2;selecting a second alkaline earth metal M3, wherein M3 is not M2; andforming M1(1−(x+y))M2xM3yMnO3, wherein: M1 is selected from the group consisting of lanthanum, scandium, yttrium, praseodymium, neodymium or samarium; andx, y, and (x+y) are less than 1.
  • 7. The method of claim 6, wherein the step of selecting M2 comprise the step of selecting M2 from the group consisting of barium, strontium, and calcium.
  • 8. The method of claim 6, wherein the step of selecting M3 comprises the step of selecting M3 from the group consisting of beryllium or magnesium.
  • 9. A method for controlling the temperature of a spacecraft, the method comprising the steps of: selecting a first alkaline earth metal M2 and a second alkaline earth metal M3, wherein M3 is not M2;forming a variable emissivity material M1(1−(x+y))M2xM3yMnO3, wherein: M1 is selected from the group consisting of lanthanum, scandium, yttrium, praseodymium, neodymium or samarium; andx, y, and (x+y) are less than 1; andapplying the variable emissivity material to a component of a spacecraft.
  • 10. The method of claim 9, wherein the step of selecting comprises the step of selecting M2 and M3 so that the variable emissivity material has a critical temperature (Tc) in the range of about 270 to about 320 K and a transition width of no more than about 30 K.
  • 11. The method of claim 9, wherein the step of forming comprises the step of ion-beam doping of M1MnO3 films with M2 and M3 atoms.
  • 12. The method of claim 9, wherein the step of forming and the step of applying are performed substantially simultaneously and wherein the step of forming comprises the step of oxidizing vapor-deposited stoichiometric metal films of M1, M2, M3 and Mn.
  • 13. The method of claim 9, wherein the step of forming comprises the step of ball-milling, jar milling, or hand-grinding reactant metal oxides M1O, M22O3, M32O3, and MnO3.
  • 14. The method of claim 9, wherein the step of forming comprises the step of dissolving (1−(x+y))M1(acac)3, xM2(acac)2, yM3(acac)2 and Mn(acac)3 in a solvent to form the variable emissivity material M1(1−(x+y))M2xM3yMnO3, wherein (acac) is acetylacetonate.
  • 15. The method of claim 14, further comprising the steps of: drying the variable emissivity material; andheat-treating the variable emissivity material.
  • 16. The method of claim 14, wherein the step of dissolving comprises the step of dissolving 0.5La(acac)3, 0.25Ba(acac)2, 0.25Be(acac)2 and Mn(acac)3 in a solvent to form La0.5Ba0.25Be0.25MnO3.
  • 17. The method of claim 9, wherein the step of selecting comprises the step of selecting M2 from the group consisting of barium, strontium, and calcium.
  • 18. The method of claim 9, wherein the step of selecting comprises the step of selecting M3 from the group consisting of beryllium and magnesium.
  • 19. The method of claim 9, wherein the step of applying the variable emissivity material to a component of the spacecraft comprises the step of mixing the variable emissivity material with a binder comprising one selected from the group consisting of potassium silicate, silicone-modified epoxy, polyurethane, poly(dimethylsiloxane), poly(dimethylsiloxane-co-methylphenylsiloxane), polyamide, and a combination thereof.
  • 20. The method of claim 9, wherein the step of applying the variable emissivity material to a component of the spacecraft comprises the steps of rolling, painting, spraying, or spin-coating the variable emissivity material/binder mixture onto the component.