Modelling the proto-Jovian atmospheres by a simple analytical algorithm

Details Modelling the proto-Jovian atmospheres by a simple analytical algorithm Modelling the proto-Jovian atmospheres by a simple analytical algorithm

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993em%26p...63..149d&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 63, no. 2, Proceedings of the second United Nations/European Space Agency Worksh

Astronomy and Astrophysics

Astronomy

Astronomical Models, Atmospheric Models, Jupiter Atmosphere, Neptune Atmosphere, Planetary Evolution, Protoplanets, Saturn Atmosphere, Stellar Interiors, Stellar Structure, Uranus Atmosphere, Algorithms, Atmospheric Density, Ideal Gas, Opacity, Stellar Luminosity, Stellar Models, Stellar Temperature

Scientific paper

This paper models the proto-Jovian atmospheres by a simple analytical algorithm, which does not require the use of a computer. This method, known as the MDV method, was used to model the present structures of the Jovian planets in Doorish (1992). The protoplanetary stages of the Jovian planets, known as stage 1 of development, can be described by the Stellar Interior Equations (SIE). These equations which basically dictate the structure of a star, can also be used to model the Jovian planets (Bodenheimer, 1986). We here include tabulated results.

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