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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
Shoemaker, E. M., Williams, J. G., Helin, E. F. and Wolfe, R. W., 1979, Asteroids, Gehrels, T. (ed), University of Arizona Press, Tucson, p. 253.Google Scholar
Zellner, B., 1979, Asteroids, T. Gehrels, (ed), University of Arizona Press, Tucson, p. 783.Google Scholar