Collision rates and impact velocities for Trojan asteroids have been e
stimated by a robust numerical approach, based on a parallel computati
on of orbits over time spans of approximate to 10(4) year and the subs
equent statistical analysis of the resulting close encounter data base
s. The average intrinsic collision probabilities for the two Trojan sw
arms are 6.46 x 10(-18) km(-2) year(-1) (L(4)) and 5.30 x 10(-18) km(-
2) year(-1) (L(5)), namely about twice the corresponding value for the
main asteroid belt. Collision speeds range from approximate to 1 to 1
4 km/sec, with a mean value close to 5 km/sec. These findings suggest
that the intensity of the collisional process is about the same in the
Trojan swarms as in the main belt, and are consistent with the detect
ion of dynamical families among Trojans. The collisional flux in the T
rojan regions is very anisotropic, with a dominant component perpendic
ular to the invariable plane. Subtle dynamical mechanisms are likely t
o somewhat affect the Trojan collision rates, but their understanding
requires further work on the very longterm evolution of Trojan orbits.
(C) 1996 Academic Press,Inc.