title: A retrograde co-orbital asteroid of Jupiter.
abstract: Recent theoretical work in celestial mechanics has revealed that an asteroid may orbit stably in the same region as a planet, despite revolving around the Sun in the sense opposite to that of the planet itself. Asteroid 2015 BZ509was discovered in 2015, but with too much uncertainty in its measured orbit to establish whether it was such a retrograde co-orbital body. Here we report observations and analysis that demonstrates that asteroid 2015 BZ509is indeed a retrograde co-orbital asteroid of the planet Jupiter. We find that 2015 BZ509has long-term stability, having been in its current, resonant state for around a million years. This is long enough to preclude precise calculation of the time or mechanism of its injection to its present state, but it may be a Halley-family comet that entered the resonance through an interaction with Saturn. Retrograde co-orbital asteroids of Jupiter and other planets may be more common than previously expected.
authors.affiliation: Department of Physics and Astronomy, The University of Western Ontario, London, Ontario N6A 3K7, Canada.|Centre for Planetary Science and Exploration (CPSX), London, Ontario N6A 3K7, Canada.
authors.forename: Paul
authors.initials: P
authors.lastname: Wiegert
authors.affiliation: Department of Physics and Astronomy, The University of Western Ontario, London, Ontario N6A 3K7, Canada.|Centre for Planetary Science and Exploration (CPSX), London, Ontario N6A 3K7, Canada.|Athabasca University Observatories, Athabasca, Alberta T9S 3A3, Canada.|Institute for Space-Earth Environmental Research, University of Nagoya, Nagoya 464-8601, Japan.|Department of Physics and Astronomy, University of Calgary, Calgary, Alberta T2N 1N4, Canada.
authors.forename: Martin
authors.initials: M
authors.lastname: Connors
authors.affiliation: Large Binocular Telescope Observatory, Tucson, Arizona 85721, USA.
authors.forename: Christian
authors.initials: C
authors.lastname: Veillet