Models of Jupiter with different chemical compositions of the molecular and metallic envelopes

Details Models of Jupiter with different chemical compositions of the molecular and metallic envelopes Models of Jupiter with different chemical compositions of the molecular and metallic envelopes

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..371g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, April 1988, p. 371-378. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Atmospheric Composition, Chemical Composition, Jupiter Atmosphere, Metallicity, Molecular Gases, Atmospheric Models, Gravitational Fields, Hydrogen

Scientific paper

Models of the internal structure of Jupiter which describe recent observational data on the gravitational field and the atmospheric composition of Jupiter are presented. The models have various chemical compositions of the molecular and metallic envelopes. The molecular layer contains an ice component while the metallic layer contains an ice and/or a rock component. The modified adiabat of hydrogen is used to construct the models. The I + R component in Jupiter is about ten times more abundant than in primordial matter.

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