331P/Gibbs
Discovery | |
---|---|
Discovered by | A. R. Gibbs (Mount Lemmon Survey) |
Discovery date | March 22, 2012 |
Orbital characteristics | |
Epoch | 4 February 2012 (JD 2455961.5) |
Observation arc | 11.3 years |
Number of observations | 148 |
Aphelion | 3.130 AU |
Perihelion | 2.877 AU |
Semi-major axis | 3.004 AU |
Eccentricity | 0.042 |
Orbital period | 5.21 years (1902 days) |
Inclination | 9.740° |
216.86° | |
Argument of periapsis | 177.40° |
Last perihelion | 29 September 2020[1] 16 June 2015 |
Next perihelion | 2025-Dec-25[1] |
TJupiter | 3.229 |
Earth MOID | 1.88 AU |
Jupiter MOID | 2.08 AU |
Physical characteristics | |
Dimensions | ~2-5 km |
Comet total magnitude (M1) | 12.3 |
Comet nuclear magnitude (M2) | 15.4 |
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
[edit]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
[edit]- ^ 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
[edit]- 331P in SDSS (26 August 2004)
- 331P confirmation observations, Malina River Observatory (23 March 2012) Archived 5 December 2021 at the Wayback Machine