The spatial distribution of long lived gas clouds emitted by satellites in the outer solar system

Details The spatial distribution of long lived gas clouds emitted by satellites in the outer solar system The spatial distribution of long lived gas clouds emitted by satellites in the outer solar system

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976p%26ss...24..577f&link_type=abstract

Planetary and Space Science, vol. 24, June 1976, p. 577-588. Research supported by the Association of Universities for Research

Mathematics

Probability

6

Gas Density, Hydrogen Clouds, Io, Natural Satellites, Sodium Vapor, Spatial Distribution, Titan, Jupiter (Planet), Lyman Alpha Radiation, Orbital Mechanics, Probability Density Functions, Saturn, Solar System

Scientific paper

Simple models are presented for the spatial distribution of gases emitted by satellites in the outer solar system, with emphasis on Io and Titan. The models, valid for long-lived species in regions of space outside the gravitational zone of the parent satellite, are applied to observed hydrogen and sodium clouds orbiting Jupiter and to an expected hydrogen cloud around Saturn.

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