Warming Early Mars With A Dense Atmosphere Of Co2 And
H2: A Review Of Recent Numerical And Experimental
Advances
M. Turbet, F. Forget, J.M. Hartmann, H. Tran, W. Fakhardji, Laboratoire De Météorologie Dynamique,
Ipsl, Cnrs, Sorbonne Université, École Normale Supérieure, Psl Research University, École Polytechnique,
75005 Paris, France (Martin.Turbet@Lmd.Ipsl.Fr), D. Mondelain, Univ. Grenoble Alpes, Cnrs, Liphy, 38000
Grenoble, France, C. Boulet, Université Paris-Saclay, Cnrs, Institut Des Sciences Moléculaires D'Orsay (Ismo),
91405, Orsay, France, O. Pirali, Ailes Beamline Soleil Synchrotron, L'Orme Des Merisiers, Saint-Aubin
91190, France ; Institut Des Sciences Moléculaires D'Orsay, Cnrs, Université Paris-Saclay, Orsay 91405,
France.

Introduction: To This Day, The Enigma Of Mars'
Ancient Climate Remains Unexplained (Wordsworth Et
Al. 2016, Haberle Et Al. 2017, Kite 2019). What Was
The Atmosphere Of Mars Made Of At The Time When –
Near The Late Noachian Epoch – Lakes And Valley Networks (See E.G., Fassett & Head 2008a,B, Hynek Et Al.
2010, Goudge Et Al. 2015) Were Formed? Although
There Is A Broad Consensus To Date That Liquid Water Is
The Main Culprit, The Nature Of The Atmosphere At The
Time (I.E., The Atmospheric Pressure And Composition)