Formation of asteroid pairs by rotational fission

P. Pravec*, D. Vokrouhlický, D. Polishook, D. J. Scheeres, A. W. Harris, A. Galád, O. Vaduvescu, F. Pozo, A. Barr, P. Longa, F. Vachier, F. Colas, D. P. Pray, J. Pollock, D. Reichart, K. Ivarsen, J. Haislip, A. Lacluyze, P. Kušnirák, T. HenychF. Marchis, B. MacOmber, S. A. Jacobson, Yu N. Krugly, A. V. Sergeev, A. Leroy

*Corresponding author for this work

Research output: Contribution to journalArticle

119 Scopus citations

Abstract

Pairs of asteroids sharing similar heliocentric orbits, but not bound together, were found recently. Backward integrations of their orbits indicated that they separated gently with low relative velocities, but did not provide additional insight into their formation mechanism. A previously hypothesized rotational fission process may explain their formation-critical predictions are that the mass ratios are less than about 0.2 and, as the mass ratio approaches this upper limit, the spin period of the larger body becomes long. Here we report photometric observations of a sample of asteroid pairs, revealing that the primaries of pairs with mass ratios much less than 0.2 rotate rapidly, near their critical fission frequency. As the mass ratio approaches 0.2, the primary period grows long. This occurs as the total energy of the system approaches zero, requiring the asteroid pair to extract an increasing fraction of energy from the primary's spin in order to escape. We do not find asteroid pairs with mass ratios larger than 0.2. Rotationally fissioned systems beyond this limit have insufficient energy to disrupt. We conclude that asteroid pairs are formed by the rotational fission of a parent asteroid into a proto-binary system, which subsequently disrupts under its own internal system dynamics soon after formation.

Original languageEnglish (US)
Pages (from-to)1085-1088
Number of pages4
JournalNature
Volume466
Issue number7310
DOIs
StatePublished - Aug 26 2010

ASJC Scopus subject areas

  • General

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    Pravec, P., Vokrouhlický, D., Polishook, D., Scheeres, D. J., Harris, A. W., Galád, A., Vaduvescu, O., Pozo, F., Barr, A., Longa, P., Vachier, F., Colas, F., Pray, D. P., Pollock, J., Reichart, D., Ivarsen, K., Haislip, J., Lacluyze, A., Kušnirák, P., ... Leroy, A. (2010). Formation of asteroid pairs by rotational fission. Nature, 466(7310), 1085-1088. https://doi.org/10.1038/nature09315