Temperature effects on exoplanetary atmospheric (bio)markers
Langue
en
Communication dans un congrès
Ce document a été publié dans
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
Résumé en anglais
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 ...Lire la suite >
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.< Réduire
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