Combined effect of YORP and collisions on the rotation rate of small Main Belt asteroids
Résumé
► In this study we model the evolution of the rotation rate of small Main Belt asteroids under the effects of YORP and collisions. ► We find that cratering collisions coupled to YORP give non-linear effects which depend on the size of the bodies and are particularly relevant at slow rotation rates.These effects lead to the observed excess of slow rotators among small asteroids. ► Our model also shows that the rotational fission of small asteroids is a very frequent event and might explain objects like P/2010 A2 and its associated tail of millimeter-sized dust particles.
Domaines
Planète et Univers [physics]
Origine : Fichiers produits par l'(les) auteur(s)
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