Jovian model with different chemical composition of molecular and metallic envelopes

Details Jovian model with different chemical composition of molecular and metallic envelopes Jovian model with different chemical composition of molecular and metallic envelopes

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rpsct...4....2g&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 2 (SEE N89-29354 24-12) Transl. into ENGLISH from Pisma v Astronomiche

Astronomy and Astrophysics

Astronomy

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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