Communication Dans Un Congrès LPI Année : 2014

The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling

Résumé

We will review the observations of species useful to constrain the O/H ratio in the interior of the ice giants. We will apply a comprehensive thermochemical and diffusion model to the ice giants and derive constraints on their deep O/H ratios.

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Dates et versions

hal-01059927 , version 1 (02-09-2014)

Identifiants

Citer

T. Cavalié, O. Venot, Franck Selsis, F. Hersant, P. Hartogh. The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. the Study of the Ice Giant Planets, 2014, Laurel, United States. pp.2011. ⟨hal-01059927⟩
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