Gaps, Cavities, and Vortices: Carving Disks with Planets and Radiation

Information

  • NSF Award
  • 2407671
Owner
  • Award Id
    2407671
  • Award Effective Date
    9/1/2024 - 5 months ago
  • Award Expiration Date
    8/31/2027 - 2 years from now
  • Award Amount
    $ 300,408.00
  • Award Instrument
    Standard Grant

Gaps, Cavities, and Vortices: Carving Disks with Planets and Radiation

Disk features like gaps and cavities are commonly attributed to planets. But other mechanisms can create similar features, e.g. the radiation pressure instability, resulting from fundamental interactions of radiation, gas, and dust. Moreover, even when planets are the root cause of the disk’s features, such instabilities can be triggered. That effect needs to be taken into account to infer planetary properties using the features. Researchers at Clemson University, in the EPSCoR state of South Carolina, are funded to study these physical systems with PEnGUIn, an open-source, aggressively optimized hydrodynamics code that runs on Graphics Processing Units (GPUs). They aim to produce a unified picture of the co-evolution of super-Earth systems and their natal disks. The project will also design and carry out interdisciplinary projects with art students, giving scientists and artists a chance to learn from each other. It will also enhance the Emerging Scholar program at Clemson, promoting college-culture in the underprivileged areas of South Carolina. <br/><br/>The dynamics of radiation-gas-dust interaction in low-viscosity protoplanetary disks, with or without planets, still has many unknowns. Accurate simulations of these systems will require either high resolution to track complex gas flow in the disks, or tracking long term evolution over millions of years, or both. This project develops a more physically-motivated thermal treatment to replace the commonly assumed isothermal equation of state or simple thermal relaxation prescription. The researchers will study whether planet-shepherded rings remain stable against the Rossby wave instability. They will study whether super-Earths, the most abundant type of known planets, can open large cavities in disks; if so, the rarer giant planets will not need to be invoked to explain cavities. They will also study whether planets may drive disk evolution by quantifying the amount of planet-induced disk transport and whether gapped disks may turn into transition disks. Working with art students in both fine arts and in digital arts, art-pieces will be produced that can be used to engage the public. As part of the Emerging Scholar program, the PI will help design and teach summer classes for high school students and provide them with research opportunities within this project.<br/><br/>This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

  • Program Officer
    Daniel Fabryckydfabryck@nsf.gov7032928490
  • Min Amd Letter Date
    8/29/2024 - 5 months ago
  • Max Amd Letter Date
    8/29/2024 - 5 months ago
  • ARRA Amount

Institutions

  • Name
    Clemson University
  • City
    CLEMSON
  • State
    SC
  • Country
    United States
  • Address
    201 SIKES HALL
  • Postal Code
    296340001
  • Phone Number
    8646562424

Investigators

  • First Name
    Jeffrey
  • Last Name
    Fung
  • Email Address
    fung@clemson.edu
  • Start Date
    8/29/2024 12:00:00 AM

Program Element

  • Text
    PLANETARY ASTRONOMY
  • Code
    121400
  • Text
    OFFICE OF MULTIDISCIPLINARY AC
  • Code
    125300

Program Reference

  • Text
    THEORETICAL & COMPUTATIONAL ASTROPHYSICS
  • Code
    1206
  • Text
    EXP PROG TO STIM COMP RES
  • Code
    9150