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Communication Dans Un Congrès Année : 2022

Day-Night Cloud Asymmetry Inhibits Early Ocean Formation on Venus and Telluric Planets

Résumé

We will present the results of new 3-D Global Climate Model (GCM) simulations aimed at reproducing the conditions of primordial surface water condensation and thus of the formation of ancient oceans on Venus.
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Dates et versions

insu-04493849 , version 1 (07-03-2024)

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M. Turbet, J. Leconte, T. Fauchez, F. Selsis, E. Bolmont, et al.. Day-Night Cloud Asymmetry Inhibits Early Ocean Formation on Venus and Telluric Planets. Ancient Venus Conference 2022, Jul 2022, Online, Unknown Region. pp.LPI Contribution No. 2680, id.2009. ⟨insu-04493849⟩
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