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Asteroid pair

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Asteroid Asteroids Break Pair

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An asteroid pair, or (if more than two bodies) an asteroid cluster, are which at some point in the past had very small relative velocities, and are typically formed either by a collisional break-up of a parent body, or from which became gravitationally unbound and are now following similar but different orbits around the Sun.

A possible example of a pair are the 1583 Antilochus and 3801 Thrasymedes. The proposer of that pair, Andrea Milani, found five other potential asteroid clusters in the Greek camp, clustered around the asteroids 1437 Diomedes, 1647 Menelaus, 2456 Palamedes, 2797 Teucer and 4035 Thestor.

The youngest asteroid pairs discovered include the main-belt asteroids P/2016 J1-A/B (separated c. 2010) and / (separated c. 2003). The former pair is particularly remarkable for exhibiting active asteroid due to water ice sublimation and rotational break-up.

Categories: Asteroid Groups And Families, Asteroids