Channel and physical models of the Jovian subnebula

Details Channel and physical models of the Jovian subnebula Channel and physical models of the Jovian subnebula

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982plap.nasa....4l&link_type=abstract

In its Planetary Atmospheres Program p 4-26 (SEE N82-22112 12-88)

Physics

1

Europa, Io, Jupiter (Planet), Planetary Nebulae, Mathematical Models, Reaction Kinetics, Solar Corona

Scientific paper

A semiempirical physical model of the Jovian subnebula was developed by analogy with the primitive solar nebula itself. The chemical aspects of this model are developed according to the principles developed in the study of the thermochemistry and gas kinetic behavior of the solar nebula, but with important modifications to take into account the higher pressures and densities in the Jovian subnebula. The bulk compositions and densities of the inner satellites of Jupiter are calculated. It is proposed that Europa differs from Io chiefly in that in has suffered a less severe thermal history. The general features of this model are applicable with minor modification to the systems of Saturn and Uranus.

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