Photochemical Escape from Mars as a Climate Driver: How Important?
Résumé
Photochemical escape is the primary loss process for O, C, and N atoms from Mars. But C rates are 10 times lower than O, setting up a conundrum: where did all the carbon from an early thick CO2 atmosphere go?
Domaines
Planète et Univers [physics]Origine | Fichiers produits par l'(les) auteur(s) |
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