Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-13T00:56:17.377Z Has data issue: false hasContentIssue false

6. The Satellites of the Major Planets: Were they All Captured?

Published online by Cambridge University Press:  12 April 2016

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Jupiter, Saturn, and Uranus have 15 (or possibly up to 18) regular satellites (i.e., with eccentricities and inclinations near zero) which are generally assumed to have been formed along with the planets and near their present orbits. We present evidence for their having been formed much later in the history of the solar system and in initial orbits very close to their respective planets. They then evolved to their present orbits, principally by tidal friction. Their source may be captured material, possibly of cometary origin.

Type
Part II. The Orbital Evolution of Comets
Copyright
Copyright © A.H. Delsemme 1977

References

Alfven, H., and Arrhenius, G. 1975, Structure and Evolutionary History of the Solar System, D. Reidel Publishing Company, Dordrecht.CrossRefGoogle Scholar
Dermott, S. F. 1968, Mon. Not. Roy. Astr. Soc, 141, 363.Google Scholar
Goldreich, P. 1965, Astr. J., 70, 5.Google Scholar
Goldreich, P., and Ward, W. R. 1973, Ap.J., 183, 1051.Google Scholar
Kuiper, G. P. 1956, in Vistas in Astronomy, (ed. Beer, A.), pp. 16311666, Pergamon Press, New York.Google Scholar
Rickmann, H. 1977, this volume.Google Scholar
Safronov, V. S. 1972, Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets, NASA TTF-677.Google Scholar
Singer, S. F. 1968, Geophys. J. Roy. Astr. Soc, 15, 205.Google Scholar
Singer, S. F. 1975, Icarus, 25, 484.Google Scholar