Artigo Acesso aberto Revisado por pares

Detection of a Trailing (L5) Neptune Trojan

2010; American Association for the Advancement of Science; Volume: 329; Issue: 5997 Linguagem: Inglês

10.1126/science.1189666

ISSN

1095-9203

Autores

Scott S. Sheppard, Chadwick A. Trujillo,

Tópico(s)

Stellar, planetary, and galactic studies

Resumo

The orbits of small Solar System bodies record the history of our Solar System. Here, we report the detection of 2008 LC18, which is a Neptune Trojan in the trailing (L5) Lagrangian region of gravitational equilibrium within Neptune's orbit. We estimate that the leading and trailing Neptune Trojan regions have similarly sized populations and dynamics, with both regions dominated by high-inclination objects. Similar populations and dynamics at both Neptune Lagrangian regions indicate that the Trojans were likely captured by a migrating, eccentric Neptune in a dynamically excited planetesimal population.

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