The exosphere of CoRoT7b

Details The exosphere of CoRoT7b The exosphere of CoRoT7b

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..987g&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.987

Physics

Scientific paper

CoRoT-7b is a rocky planet that orbits a solar-like star at a distance of only 4.5 stellar radii. It may thus resemble an extreme form of Mercury and may even have an exosphere. Alternatively it may be an extreme version of Io. Using in an out of transit spectroscopy firm upper limits for the exosphere is derived, and future prospects are discussed.

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