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]
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Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
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en
Communication dans un congrès
Este ítem está publicado en
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
Resumen en inglés
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 ...Leer más >
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.< Leer menos
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