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Titan and the Dispersal of the Proto-Saturnian Nebula

Published online by Cambridge University Press:  25 April 2016

K. Hourigan
K. Hourigan*
Affiliation:
Department of Mathematics, Monash University
*
* Present Address: CSIRO, Division of Energy Technology, Highett
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Extract

The NASA Voyager spacecraft missions to the outer planets have provided a wealth of observational data with regard to the physical and chemical properties of the attendant satellite systems. Although the gaseous nebula discs from which these satellites are suspected to have formed are no longer present, these data provide at least some basis from which the characteristics of individual nebula can be deduced.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 459 - 461
Copyright
Copyright © Astronomical Society of Australia 1984

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