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The size of the stability regions of Jupiter Trojans
2006
Astronomy and Astrophysics
Context. We have known about the Trojan group of asteroids since 1906. With a suspected number comparable to that of the mainbelt, they move around the Lagrangian points L 4 and L 5 of the Sun-Jupiter system. Aims. During the past century the Trojan asteroids were the topic of many studies of their orbital dynamics and stability. In recent years it has been possible to perform extensive numerical simulations of the motion of these asteroids and thus also to investigate the size and structure of
doi:10.1051/0004-6361:20054689
fatcat:rc4kd75osndwndj55nfiyoa54m