NASA GSFC, Planetary Environments Laboratory
8800 Greenbelt Rd., Bldg. 34, Rm. W160
Greenbelt, MD 20771
Gabrielle Suissa's current work primarily focuses on running GCMs (global circulation models) to simulate potentially habitable planets around M stars. She also works on simulating transit spectra from GCM outputs to assess how detectable these planetary systems would be. Modeled exoplanets of interest include terrestrial, Earth-sized aquaplanets and super-Earths/mini-Neptunes with hydrogen dominated atmospheres.
Gabrielle Suissa is a Visiting Research Assistant working in the Planetary Environments Laboratory. Suissa is interested in exoplanet characterization, atmospheric modeling, exoplanetary interiors, and biosignatures.
B.A in Astrophysics, Columbia University in the City of New York (Sept. 2015 - May 2019)
John Mather Nobel Scholar (2018 - Present)
- GESTAR-USRA Visiting Research Assistant (July 2019 - Present)
Running GCMs to simulate Super-Earths and mini-Neptunes with hydrogen atmospheres around M-dwarfs. Simulating transit spectra and phase curves using the outputs of these GCMs.
- Center for Astrobiology NASA Goddard Space Flight Center, Summer 2018
Simulated exoplanet transmission spectroscopy for ocean-covered earth-like planets synchronously rotating M- and K-type stars. Used GCMs as inputs to radiative transfer model in order to create and analyze spectra. Conducted exposure time calculations for TESS targets based on spectral trends.
- Cool Worlds Lab Columbia University, Summer 2017 – Spring 2018
Constructed model to constrain core sizes of rocky exoplanets by exploiting boundary conditions. Parametrically interpolated two-layer interior models. Created and released public code (HARDCORE) capable of calculating the minimum and maximum core radius fraction given just planetary mass and radius.
Suissa, G., Mandell, A., Kopparapu, R., Villanueva, G., and Wolf, E. Synchronously Rotating Ocean Earths Around Cool Stars: What to ExPECTRA. In preparation.
Suissa, G. and Kipping, D., 2018, Trappist-1e Has a Large Iron Core, RNAAS, 2, 2, 31.
Suissa, G., Chen, J., and Kipping, D., 2018, A HARDCORE model for constraining an exoplanet’s core size, MNRAS, 476, 2613.