Asteroid motions

被引：5

作者：

Sykes, MV

Moynihan, PD

机构：

[1] Steward Observatory, University of Arizona, Tucson

来源：

ICARUS | 1996年 / 124卷 / 02期

关键词：

D O I：

10.1006/icar.1996.0217

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Equations are derived which describe the apparent motion of an asteroid traveling on an elliptical orbit in geocentric ecliptic coordinates. At opposition, the equations are identical to those derived by Bowed et al. (Bowell, E., B. Skiff, and L. Wasserman 1990. In Asteroids; Comets, Meteors III (C.-I. Lagerkvist, M. Rickman, B. A. Lindblad, and M. Lindgren, Eds.), pp. 19-24. Uppsala Universitet, Uppsala, Sweden). These equations can be an important component in the optimization of search strategies for specific asteroid populations based on their apparent motions relative to other populations when observed away from opposition. (C) 1996 Academic Press, Inc.

引用

页码：399 / 406

页数：8

共 8 条

[1]

BOWELL E, 1990, ASTEROIDS COMETS MET, V3, P19

[2]

BOWELL E, 1995, B AM ASTRON SOC, V95, P1057

[3]

Bowell E., 1989, ASTEROIDS, VII, P524

[4] THE OPPOSITION EFFECT OF THE MOON - THE CONTRIBUTION OF COHERENT BACKSCATTER [J].