Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996icar..124..399s&link_type=abstract
Icarus, Volume 124, Issue 2, pp. 399-406.
Other
4
Scientific paper
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 Bowell 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.
Moynihan Daniel P.
Sykes Mary V.
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