331P/Gibbs (P/2012 F5) is a small periodic Encke-type and rare main-belt comet, discovered by American amateur astronomer Alex Gibbs.[2]
Description
It is a rare type of comet called a main-belt comet. Although most comets come from the Oort cloud or the Kuiper belt, main-belt comets are instead members of the asteroid belt that have a coma and tail. As of 2016, it is one of only 15 known main-belt comets.[3]
Precovery observations of 331P/Gibbs in Sloan Digital Sky Survey data were found dating to August 2004, in which the object was visible as a regular asteroid. Further observations in 2014 by the Keck Observatory showed that the comet was fractured into 5 pieces and rotating rapidly, with a rotation period of only 3.2 hours. Due to the YORP effect, P/2012 F5 had begun to spin so quickly that, being a likely rubble pile, parts began to be thrown off, leaving a very long dust trail.[4] This is very similar to 311P/PANSTARRS, being the best-established cause for main-belt comets along with impacts between small asteroids (such as with 596 Scheila and P/2010 A2 (LINEAR)).
References
- ^ a b MPC
- ^ "JPL Small-Body Database Browser: (331P/Gibbs)" (last observation: 2015-12-14).
- ^ "JPL Small-Body Database Search Engine". Jet Propulsion Laboratory. NASA. Retrieved 10 December 2016.
- ^ "Active asteroid spun so fast that it exploded". Astronomy Now. Retrieved 10 December 2016.
External links
- 331P in SDSS (26 August 2004)
- 331P confirmation observations, Malina River Observatory (23 March 2012) Archived 5 December 2021 at the Wayback Machine
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