Physics
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..601n&link_type=abstract
In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed
Physics
Cometary Nuclei: Rotation
Scientific paper
In the classical comet nucleus model suggested b F. Whipple (1951), anisotropic ice sublimation due to solar radiation produces reactive torques that act on the nucleus. This should result in the slow variation of a nucleus' rotation state. In earlier papers the spin evolution of a few comet nuclei was investigated using numerical integration of the equations of nucleus rotation. We seek to develop a more systematic approach to the problem by studying the rotational evolution of a cometary nucleus using the averaging method. This approch allows us to extract the relevant physical parameters that control the evolution of a comet's rotation state. As an example we discuss some possible scenarios of rotational evolution for the nucleus of Borrelly comet.
Neishtadt A. I.
Scheeres Dan
Sidorenko Vladimir
Vasiliev Aleksey A.
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