Computer Science
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icar..162..453m&link_type=abstract
Icarus, Volume 162, Issue 2, p. 453-459.
Computer Science
4
Scientific paper
We model with numerical algorithms the dynamical processes that possibly lead to the trapping of Jupiter's Trojans from a primordial population of planetesimals orbiting nearby a proto-Jupiter. The predictions of models based on mutual planetesimal collisions and on the mass growth of Jupiter are compared with observations. In particular, we concentrate on the distribution of the libration amplitude. The two mechanisms for trapping reproduce closely the libration amplitude distribution of the real Trojans only when the long-term dynamical diffusion described by , Nature 385, 42-44) is taken into account.
Marzari Francesco
Scholl Hans
Tricarico Pasquale
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