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Automated Computation of General Perturbations for the Flora Asteroidal Group

Published online by Cambridge University Press:  25 April 2016

M. F. He  and
Zhangjie
M. F. He
Affiliation:
Shanghai Observatory, Academia Sinica Shanghai, People’s Republic of China
Zhangjie
Affiliation:
Shanghai Observatory, Academia Sinica Shanghai, People’s Republic of China
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Abstract

The general perturbations of the asteroids of the Flora group (975″ < n < 1150″, n - the mean daily motion) due to Jupiter have been automatically computed on an IBM 4341 computer with the Hansen method by manipulating Broucke’s Symbolic Poisson Series Processor, and the results have been compared with that computed previously with the Bohlin group method.

Type
Solar & Solar System
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 149
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Bohlin, K., 1903, Astron. laktt. Unders. Stockholm Obs., 7, 1.Google Scholar
Broucke, R. A., 1980, IASOM TR80-3, University of Texas at Austin.Google Scholar
Herget, P., 1948, The Computation of Orbits, Edwards Brothers Inc., Michigan, USA, p. 114.Google Scholar
Strömbeig, G., 1916, Astron. laktt. Unders. Stockholm Obs., 10, 3.Google Scholar