On the Formation and Dissociation of Binary Asteroids and Comets

Details On the Formation and Dissociation of Binary Asteroids and Comets On the Formation and Dissociation of Binary Asteroids and Comets

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.1502c&link_type=abstract

American Astronomical Society Meeting 203, #15.02; Bulletin of the American Astronomical Society, Vol. 35, p.1231

Mathematics

Probability

Scientific paper

Close encounters of non-spherical bodies can form binary systems, since their orbital energy could become negative, at the expense of an increasing rotational energy. We illustrate these events by calculating the probabilities, P(v,L), for the capture of an spherical body by an initially at rest proloid, as a function of the initial relative speed (v) of the two bodies, and the parameter of impact (L). This probability function is applied to a system of bodies originally orbiting in a circular belt, and we find that the spherical body would be trapped by the proloid, essentially whenever L are less than a given value L0(r), where r is the original heliocentric position of the proloid. Values of L0 are determined for r in three regions: the asteroid belt, the Kuiper belt, and the Oort cloud.
We can also envision the inverse situation; where an initial binary system dissociates meanwhile the rotational energy is transferring into the orbital energy. Thus, for instance, under time reversal, the capture of a satellite, described in the above paragraph, imply satellite escaping from a couple system. An explicit example of this situation is illustrated in a computer simulation. The above investigation is relevant to the problem of formation of significant number of discovered binary asteroids and comets. On the other hand, it is also extremely important to study the instability of binary near-Earth asteroids and comets, since escaping objects represent collisional threats that are harder to predict.
We thanks to the NASA-Space Grant Consortium at Humaco

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