(323137) 2003 BM80
Mean diameter | 9.4 km (est. at 0.07)[4] | |
13.63[1] | ||
(323137) 2003 BM80,
Orbit and classification
2003 BM80 is a
The body's observation arc begins with its first precovery observation by the NEAT program in December 2001, more than a year before its official discovery observation at Anderson Mesa.[2]
In 2022 a team from Northern Arizona University determined that 2003 BM80 is a Quasi-Hilda Object with a sustained activity outburst, lasting over 15 months. Their dynamical simulations showed that this object has undergone at least five close encounters with Jupiter and one with Saturn over the last 180 years. It was likely a Centaur or Jupiter family comet 250 years ago. In the future, this object will have about 15 strong interactions with Jupiter, and 380 years in the future, it might become again a Jupiter family comet. But it could also become a main-belt asteroid.[5]
Numbering and naming
This
Physical characteristics
Based on a generic magnitude-to-diameter conversion, 2003 BM80 measures approximately 4.4 kilometers in diameter using an
As of 2021[update], no rotational
References
- ^ a b c d e f g "JPL Small-Body Database Browser: (323137) 2003 BM80" (2021-06-27 last obs.). Jet Propulsion Laboratory. Retrieved 19 October 2021.
- ^ a b c d "(323137) 2003 BM80". Minor Planet Center. Retrieved 19 October 2021.
- ^ a b Jonathan Shanklin. "(323137) = 2003 BM80 = 2003 FV112". University of Cambridge – Institute of Astronomy. Retrieved 19 October 2021.
- ^ a b "Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved 19 October 2021.
- arXiv:2208.08592 [astro-ph.EP].
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 25 February 2018.
External links
- 282P/(323137) 2003 BM80 (2021), MISAO project, Seiichi Yoshida
- Asteroid Lightcurve Database (LCDB), query form (simple query)
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (320001)-(325000) – Minor Planet Center
- (323137) 2003 BM80 at AstDyS-2, Asteroids—Dynamic Site
- (323137) 2003 BM80 at the JPL Small-Body Database