Abstract
The effects of rotation of a cometary nucleus on the character of nongravitational parameters are discussed. It is suggested that the change of a nongravitational acceleration to deceleration (and vice versa) may be related to a precessional motion of the nucleus, or to secular variations in the lag angle coupled with severe orbital modifications.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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1. 10.4011/shikizai1937.51.549;Journal of the Japan Society of Colour Material;1978