Session

poster

Location

Space Dynamics Laboratory, Auditorium Rooms D & E

Start Date

5-9-2022 9:55 AM

End Date

5-9-2022 10:45 AM

Description

Using three inputs, metallicity, effective temperature, and surface gravity, we can model a BD to simulate traits like pressure, temperature, density, spectra, etc.

By comparing the modeled spectra with observed spectra, we can make changes to our models to make them more accurate.

Available for download on Tuesday, May 09, 2023

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May 9th, 9:55 AM May 9th, 10:45 AM

Modeling Brown Dwarf Atmospheres in Preparation for JWST Observations

Space Dynamics Laboratory, Auditorium Rooms D & E

Using three inputs, metallicity, effective temperature, and surface gravity, we can model a BD to simulate traits like pressure, temperature, density, spectra, etc.

By comparing the modeled spectra with observed spectra, we can make changes to our models to make them more accurate.