Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997natur.386..154l&link_type=abstract
Nature, Volume 386, Issue 6621, pp. 154-156 (1997).
Astronomy and Astrophysics
Astrophysics
15
Scientific paper
The rotation rates of asteroids, which are deduced from periodic fluctuations in their brightnesses1, are controlled by mutual collisions2-8. The link between asteroid spin and collision history is usually made with reference to impact experiments on centimetre-scale targets, where material strength governs the impact response2,3,9-11. Recent work, however, indicates that for objects of the size of most observed asteroids (>=1 km in diameter), gravity rather than intrinsic strength controls the dynamic response to collisions12-14. Here we explore this idea by modelling the effect of impacts on large gravitating bodies. We find that the fraction of a projectile's angular momentum that is retained by a target asteroid is both lower and more variable than expected from laboratory experiments, with spin evolution being dominated by 'catastrophic' collisions that eject ~50 per cent of the target's mass. The remnant of an initially non-rotating silicate asteroid that suffers such a collision rotates at a rate of ~2.9 per day, which is close to the observed mean asteroid rotation rate of ~2.5 d-1. Moreover, our calculations suggest that the observed trend in the mean spin frequency for different classes of asteroids4 (2.2 d-1for C-type asteroids, 2.5 d-1 for S-type, and 4.0 d-1 for M-type) is due to increasing mean density, rather than increasing material strength.
Ahrens Thomas J.
Love Stanley G.
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