Models of Jupiter and Saturn with a two-layer molecular envelope

Details Models of Jupiter and Saturn with a two-layer molecular envelope Models of Jupiter and Saturn with a two-layer molecular envelope

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..252g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, July-Sept. 1988, p. 252-261. In Russian.

Astronomy and Astrophysics

Astronomy

6

Gas Composition, Jupiter (Planet), Planetary Structure, Saturn (Planet), Abundance, Equations Of State, Mathematical Models, Molecular Gases

Scientific paper

A two-layer envelope model for Jupiter and Saturn is presented in which the I-component in the outer envelope is about 1.5-2 times greater than its solar abundance, while in the inner envelope the RI component is about 10 times greater than its solar abundance for Jupiter and about 17 times greater the solar abundance for Saturn. The transition from the outer to the inner envelope takes place at a pressure of 0.7 Mbar and a temperature of 6500 K for Jupiter and a pressure of 0.9 Mbar and a temperature of 6500 K for Saturn.

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