Hot Super-Earths around K- and M-stars

Details Hot Super-Earths around K- and M-stars Hot Super-Earths around K- and M-stars

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..816v&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

Computer Science

Scientific paper

Close-in super-Earths orbiting around K and M-stars will most likely be the first of the Super- Earths to be characterised. Model atmospheres and different planetary scenarios were simulated using a 1D-radiativeconvective atmospheric model to assess the habitability and general atmospheric and surface conditions on such planets. As a result, a catalogue of possible exoplanet scenarios is being compiled which can be used to classify future detection and search for suitable candidates of biomarker or habitability searches.

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