Main-belt comets (MBCs) are bodies orbiting within the asteroid belt which have shown comet-like activity during part of their orbit. The Jet Propulsion Laboratory defines a main-belt asteroid as an asteroid with a semi-major axis (average distance from the Sun) of more than 2 AU but less than 3.2 AU, and a perihelion (closest approach distance to the Sun) of no less than 1.6 AU. David Jewitt from UCLA points out that these objects are most likely not comets with sublimating ice, but asteroids that exhibit dust activity, and hence he and others started calling these class of objects active asteroids.
The first MBC was thought to be an asteroid when discovered and was named 1979 OW7. In 1996 it was found to have a tail by Eric Elst and Guido Pizarro. It is now given the cometary designation 133P/Elst-Pizarro.
Unlike comets, which spend most of their orbit at Jupiter-like or greater distances from the Sun, main-belt comets follow near-circular orbits within the asteroid belt that are undistinguishable from the orbits of many standard asteroids. While quite a few short-period comets have semimajor axes well within Jupiter's orbit, main-belt comets differ in having small eccentricities and inclinations similar to main-belt asteroids. The first three identified main-belt comets all orbit within the outer part of the asteroid belt.
It is not known how an outer Solar System body like the other comets could have made its way into a low-eccentricity orbit typical of the asteroid belt, which is only weakly perturbed by the planets. Hence it is assumed that unlike other comets, the main-belt comets are simply icy asteroids, which formed in an inner Solar System orbit close to their present positions, and that many outer asteroids may be icy.
Some main-belt comets display a cometary dust tail only for a part of their orbit near perihelion. Activity in 133P/Elst–Pizarro is recurrent, having been observed at each of the last three perihelia. The activity persists for a month or several out of each 5-6 year orbit, and is presumably due to ice being uncovered by minor impacts in the last 100 to 1000 years. These impacts are suspected to excavate these subsurface pockets of volatile material helping to expose them to solar radiation.
When discovered in January 2010, P/2010 A2 (LINEAR) was initially given a cometary designation and considered a member of this group, but P/2010 A2 is now believed to the remnant of an asteroid-on-asteroid impact. Observations of (596) Scheila indicated that large amounts of dust were kicked up by the impact of another asteroid of approximately 35 meters in diameter.
In October 2013, observations of P/2013 R3, taken with the 10.4 m Gran Telescopio Canarias on the island of La Palma (Spain) showed that this comet was breaking apart. Inspection of the stacked CCD images obtained on October 11 and 12 showed that the main-belt comet presented a central bright condensation that was accompanied on its movement by three more fragments, A,B,C. The brightest A fragment was also detected at the reported position in CCD images obtained at the 1.52 m telescope of the Sierra Nevada Observatory in Granada on October 12.
NASA reported on a series of images taken by the Hubble Space Telescope between October 29, 2013 and January 14, 2014 which show the increasing separation of the four main bodies. The Yarkovsky–O'Keefe–Radzievskii–Paddack effect, caused by sunlight, increased the spin rate until the centrifugal force caused the rubble pile to separate.
It has been hypothesized that main-belt comets may have been the source of Earth's water, since the deuterium-hydrogen ratio of the Earth's oceans is too low for classical comets to have been the principal source.
The term 'main-belt comet' is a classification based on orbit and the presence of an extended morphology. It does not imply that these objects are comets or that the material surrounding their nuclei was ejected by the sublimation of volatiles, as on comets.
Identified members of this morphology class include:
||Semi-major axis (a)
|133P/Elst–Pizarro [(7968) Elst–Pizarro, P/1996 N2]||Y||Y||3.15||2.64||2013-02-09|
|176P/LINEAR [(118401) LINEAR]||Y||Y||3.19||2.57||2011-07-01|
|238P/Read [P/2005 U1]||Y||Y||3.16||2.36||2011-03-11|
|259P/Garradd [P/2008 R1]||Y||Y||2.72||1.79||2013-01-25|
|P/2010 A2 (LINEAR)||N||Y||2.29||2.00||2013-05-23|
|P/2010 R2 (La Sagra)||Y||Y||3.10||2.62||2015-11-30|
|(300163) 2006 VW139||Y||Y||3.05||2.44||2011-07-18|
|P/2012 F5 (Gibbs)||N||Y||3.00||2.88||2010-03-26|
|P/2012 T1 (PANSTARRS)||Y||Y||3.15||2.41||2012-09-11|
|P/2013 R3 (Catalina-PANSTARRS)||Y||Y||3.03||2.20||2013-08-05|
- "JPL "Main-belt Asteroid" Orbit Classification". JPL Solar System Dynamics. Retrieved 2010-12-15.
- "Hubble Observes Six Tails from an Unusual Asteroid". Space Telescope Science Institute (STScI), official YouTube channel for the Hubble Space Telescope. Retrieved 2014-11-15.
- David Jewitt. "Main Belt Comets". UCLA, Department of Earth and Space Sciences. Retrieved 2010-12-15.
- Hsieh, Henry (January 20, 2004). "133P/Elst-Pizarro". UH Institute for Astronomy. Retrieved 22 June 2012.
- Harrington, J.D.; Villard, Ray (6 March 2014). "RELEASE 14-060 NASA's Hubble Telescope Witnesses Asteroid's Mysterious Disintegration". NASA. Retrieved 6 March 2014.
- Henry H. Hsieh (May 2010). "Main Belt Comets". Hawaii. Retrieved 2010-12-15. (older 2010 site)
- MPEC 2010-A51 : COMET P/2010 A2 (LINEAR)
- Jewitt, David; Weaver, Harold; Agarwal, Jessica; Mutchler, Max; Drahus, Michal (2010). "A recent disruption of the main-belt asteroid P/2010?A2". Nature 467 (7317): 817–9. Bibcode:2010Natur.467..817J. doi:10.1038/nature09456. PMID 20944743.
- Snodgrass, Colin; Tubiana, Cecilia; Vincent, Jean-Baptiste; Sierks, Holger; Hviid, Stubbe; Moissl, Richard; Boehnhardt, Hermann; Barbieri, Cesare et al. (2010). "A collision in 2009 as the origin of the debris trail of asteroid P/2010?A2". Nature 467 (7317): 814–6. doi:10.1038/nature09453. PMID 20944742.
- "Hubble witnesses an asteroid mysteriously disintegrating". ESA / HUBBLE. Retrieved 12 March 2014.
- Licandro, Javier. "Main Belt Comet P/2013 R3 is breaking apart". IAC Press Release. Retrieved 17 October 2013.
- Main-Belt Comets May Have Been Source Of Earths Water, Space Daily, Mar 23, (2006).
- Henry Hsieh's Main-Belt Comets page has extensive details on Main-belt comets
- David Jewitt. Main Belt Comets
- Planetary Society article on MBCs
- Discussion of possible differences in characteristics of the water in MBCs and other comets
- YouTube Interview with David Jewitt (discussion on main-belt comets starts around 9 minutes into video)
- Impact trigger mechanism diagram by David Jewitt
- Comet-like appearance of (596) Scheila
- Project T3: Finding Comets in the Asteroid Population
- The Active Asteroids (Dave Jewitt : 22 Dec 2011: arXiv:1112.5220)
- Discovery of Main-Belt Comet P/2006 VW139 by Pan-STARRS1 (Henry H. Hsieh : 9 Feb 2012: arXiv:1202.2126)
- New Comet: P/2012 T1 (PANSTARRS) (Remanzacco Observatory : 16 Oct 2012)
- The location of Asteroidal Belt Comets (ABCs), in a comets' evolutionary diagram: The Lazarus Comets (arXiv:1305.2621 : 14 May 2013)
- P/2013 R3: a Main Belt Comet that is breaking apart. J. Licandro New images obtained with the GTC