Format

Send to

Choose Destination
See comment in PubMed Commons below
Science. 2013 Aug 30;341(6149):994-7. doi: 10.1126/science.1238072.

A Uranian Trojan and the frequency of temporary giant-planet co-orbitals.

Author information

1
Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, Canada. mikea@astro.ubc.ca

Abstract

Trojan objects share a planet's orbit, never straying far from the triangular Lagrangian points, 60° ahead of (L4) or behind (L5) the planet. We report the detection of a Uranian Trojan; in our numerical integrations, 2011 QF99 oscillates around the Uranian L4 Lagrange point for >70,000 years and remains co-orbital for ~1 million years before becoming a Centaur. We constructed a Centaur model, supplied from the transneptunian region, to estimate temporary co-orbital capture frequency and duration (to a factor of 2 accuracy), finding that at any time 0.4 and 2.8% of the population will be Uranian and Neptunian co-orbitals, respectively. The co-orbital fraction (~2.4%) among Centaurs in the International Astronomical Union Minor Planet Centre database is thus as expected under transneptunian supply.

PMID:
23990557
DOI:
10.1126/science.1238072
Free full text
PubMed Commons home

PubMed Commons

0 comments
How to join PubMed Commons

    Supplemental Content

    Full text links

    Icon for HighWire
    Loading ...
    Support Center