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3. A Former Major Planet of the Solar System

Published online by Cambridge University Press:  12 April 2016

Abstract

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Dynamical calculations by Ovenden, indicating the former existence of a 90-Earth-mass planet in the asteroid belt, have now been supported by a study of orbital element distributions of very-long-period comets. The indicated epoch for disintegration of the planet is just 5 x 106 years ago.

Type
Part VIII. The Origin of Comets
Copyright
Copyright © A.H. Delsemme 1977

References

Everhart, E. 1972, Astroph. Letters, 10, 131.Google Scholar
Marsden, B. G., and Sekanina, Z. 1973, Astron. J., 78, 1118.Google Scholar
Marsden, B. G. 1975, Catalogue of Cometary Orbits, Smithsonian Astrophysical Observatory, Cambridge, Mass.Google Scholar
Oort, J. H. 1950, Bull. Astron. Inst. Neth., 11, 91.Google Scholar
Ovenden, M. W. 1973, in Recent Advances in Dynamical Astronomy, Tapley, B. D. and Szebehely, V., eds.Google Scholar
Ovenden, M. W. 1972, Nature, 239, 508.Google Scholar