Evolution of the obliquities for ten asteroids

Details Evolution of the obliquities for ten asteroids Evolution of the obliquities for ten asteroids

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996p%26ss...44.1177s&link_type=abstract

Planetary and Space Science, v. 44, p. 1177-1183.

Computer Science

9

Scientific paper

Using the method developed by Laskar and Robutel (Nature 361, 608-612, 1993), the evolution of the obliquities of ten large asteroids is investigated. These are compared with a frequency analysis. Generally, the orbits of the asteroids in the sample have orbital evolutions with characteristic frequencies higher than the typical precession frequencies. No indication of chaos is found during the 2 Myr examined for any initial obliquity of the objects.

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