Modeling the phase curve of hot rocky planets with 3D climate models

Details Modeling the phase curve of hot rocky planets with 3D climate models Modeling the phase curve of hot rocky planets with 3D climate models

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1344s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1344

Physics

Scientific paper

Using a 3D climate model, we study how the apparent emission of a hot terrestrial exoplanet varies with wavelength and orbital phase, for different atmospheric pressures, and inclinations, in the case of a tidally-locked planet. Based on these synthetic thermal phase curves, we investigate how the planet and its atmosphere could be characterized by spatiallyunresolved spectro-photometry of the system with JWST and EChO.

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