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Structural and Thermal Icy Satellite Models: Preliminary Results

Published online by Cambridge University Press:  25 April 2016

P. J. Thomas
P. J. Thomas*
Affiliation:
Department of Mathematics, Monash University
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Extract

The satellites of the outer solar system appear to be composed principally of water ice and silicates, with the presence of ammonia and methane hydrates (Lewis 1971). Although these bodies are small (with radii typically < 1000 km) they can exhibit very active evolutionary histories, due to the low melting point of water ice.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 487 - 489
Copyright
Copyright © Astronomical Society of Australia 1984

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