The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling
HARTOGH, P.
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
< Réduire
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Langue
en
Communication dans un congrès
Ce document a été publié dans
LPI, Workshop on the Study of the Ice Giant Planets, held July 28-30, 2014 in Laurel, Maryland. LPI Contribution No. 1798, p.2011, Workshop on the Study of the Ice Giant Planets, held July 28-30, 2014 in Laurel, Maryland. LPI Contribution No. 1798, p.2011, 2014, Laurel. 2014-07, vol. 1798, p. 2011
Résumé en anglais
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 ...Lire la suite >
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.< Réduire
Origine
Importé de halUnités de recherche