HÉBRARD, Eric; VENOT, O.; DOBRIJEVIC, M.; SELSIS, Franck

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HÉBRARD, Eric
SSE 2012

VENOT, O.
SSE 2012

DOBRIJEVIC, M.
SSE 2012

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Communication dans un congrès

Este ítem está publicado en

European Planetary Science Congress 2012, 2012espc.conf..688H - European Planetary Science Congress 2012, held 23-28 September, 2012 in Madrid, Spain - id. EPSC2012-688, 2012espc.conf..688H - European Planetary Science Congress 2012, held 23-28 September, 2012 in Madrid, Spain - id. EPSC2012-688, 2012, Madrid. 2012-09p. 688

Resumen en inglés

We have developed a photo-thermo-chemical model adapted to the study of the hot terrestrial atmospheres. Such a model is essential to interpret future observations and to predict the composition of hot extrasolar terrestrial planets. It is also important to understand the formation and the evolution of some of their key atmospheric species. We investigate here the effect of an increase of the temperature on the predicted abundances of some of these key species, such as ozone O3 and carbon dioxide CO2.< Leer menos

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Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804