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Ecliptical Orthogonal Motion and Perihelion Distribution of the AAA Asteroids

Published online by Cambridge University Press:  25 April 2016

Suryadi Siregar
Suryadi Siregar*
Affiliation:
Bosscha Observatory and Department of Astronomy, Bandung Institute of Technology, Indonesia
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Abstract

This paper briefly discusses the Aten, Apollo and Amor asteroid types (collectively referred to as AAAs), their perihelion distribution and orthogonal motion. There are 90 objects in these classes: 6 Atens, 46 Amors and 38 Apollos. The maximum distance to the ecliptic plane of each class follows an exponential function.

Type
Solar & Solar System
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 2 , 1991 , pp. 315 - 316
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Kresak, L., 1979, Asteroids, Gehrels, T. (ed), University of Arizona Press, Tucson, p. 289.Google Scholar
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