Extinct comet

Extinct comet
Don Quixote (apmag 15) near perihelion in 2009.

Extinct comets are comets that have expelled most of their volatile ice and have little left to form a tail or coma. The volatile material contained in the comet nucleus evaporates away, and all that remains is inert rock or rubble that can resemble an asteroid. Comets may go through a transition phase as they come close to extinction. A comet may be dormant rather than extinct, if its volatile component is sealed beneath an inactive surface layer.


Nature of extinct comets

The eccentric (0.66) comet-like orbit of Hypnos.

Extinct comets are those that have expelled most of their volatile ice and have little left to form a tail or coma. Over time, most of the volatile material contained in a comet nucleus evaporates away, and the comet becomes a small, dark, inert lump of rock or rubble[1] that can resemble an asteroid.[2]

Other related types of comet include transition comets, that are close to becoming extinct, such as were looked for in the Hubble search for transition comets.[3] Comets such as C/2001 OG108 (LONEOS) may represent the transition between typical Halley Family/long period comets and extinct comets.[4] Damocloid asteroids have been studied as possible extinct cometary candidates due to the similarity of their orbital parameters with those of Halley Family comets.[4]

Dormant comets are those within which volatiles may be sealed, but which have inactive surfaces. For example, 14827 Hypnos may be the nucleus of an extinct comet that is covered by a crust several centimeters thick that prevents any remaining volatiles from outgassing.[5]

The term dormant comet is also used to describe comets that may become active but are not actively outgassing. For example 60558 Echeclus has displayed a cometary coma and now also has the cometary designation 174P/Echeclus. After passing perihelion in early 2008, centaur 52872 Okyrhoe significantly brightened.[6]

The distinction between comets and asteroids

When discovered, asteroids were seen as a class of objects distinct from comets, and there was no unified term for the two until "Small Solar System body" was coined in 2006 by the IAU. The main difference between an asteroid and a comet is that a comet shows a coma due to sublimation of near surface ices by solar radiation. A few objects have ended up being dual-listed because they were first classified as minor planets but later showed evidence of cometary activity. Conversely, some (perhaps all) comets are eventually depleted of their surface volatile ices and become asteroids. A further distinction is that comets typically have more eccentric orbits than most asteroids; most "asteroids" with notably eccentric orbits are probably dormant or extinct comets. Also, they are theorized to be common objects amongst the celestial bodies orbiting close to the Sun.[7]

Roughly six percent of the near-earth asteroids are thought to be extinct nuclei of comets which no longer experience outgassing.[5][8][9]

Comet nucleus of 9P/Tempel as imaged by the NASA Deep Impact space probe

Extinct comets

Suspected or theorized extinct comets include:

See also


  1. ^ "If comets melt, why do they seem to last for long periods of time?", Scientific American, November 16, 1998
  2. ^ "What is the difference between asteroids and comets?", Rosetta FAQ, ESA
  3. ^ Space Telescope Science Institute, 'Amateur Astronomers Will Use NASA's Hubble Space Telescope', Media Release STScI-1992-23, 10 September 1992, retrieved 18 March 2009.
  4. ^ a b Abell, P. A.; Fernandez; Pravec; French; Farnham; Gaffey; Hardersen; Kusnirak et al.; Fernandez, Y. R.; Pravec, P.;French, L.M.; Farnham, T.L.; Gaffey, M.J.; Hardersen, P.S.; Kusnirak, P.; Sarounova, L.; Sheppard, S.S. (2003). "Physical Characteristics of Asteroid-like Comet Nucleus C/2001 OG108 (LONEOS)". 34th Annual Lunar and Planetary Science Conference 34: 1253. Bibcode 2003LPI....34.1253A. 
  5. ^ a b c Whitman, Kathryn; Alessandro Morbidelli and Robert Jedicke (2006). "The Size-Frequency Distribution of Dormant Jupiter Family Comets". Icarus 183: 101. arXiv:astro-ph/0603106. Bibcode 2006Icar..183..101W. doi:10.1016/j.icarus.2006.02.016. 
  6. ^ Trigo-Rodríguez, Melendo, García-Hernández, Davidsson, Sánchez (2008). "A continuous follow-up of Centaurs, and dormant comets: looking for cometary activity" (PDF). European Planetary Science Congress. http://www.cosis.net/abstracts/EPSC2008/00291/EPSC2008-A-00291-1.pdf. Retrieved 2008-10-12. 
  7. ^ a b "SOHO's new catch: its first officially periodic comet". European Space Agency. 25 September 2007. http://www.esa.int/esaCP/SEMAU2C1S6F_index_0.html. Retrieved 2007-11-19. 
  8. ^ A. Morbidelli, W. F. Bottke Jr., Ch. Froeschlé, P. Michel (January 2002). W. F. Bottke Jr., A. Cellino, P. Paolicchi, and R. P. Binzel. ed. "Origin and Evolution of Near-Earth Objects" (PDF). Asteroids III (University of Arizona Press): 409–422. http://www.boulder.swri.edu/~bottke/Reprints/Morbidelli-etal_2002_AstIII_NEOs.pdf. 
  9. ^ a b c D.F. Lupishko, M. di Martino and T.A. Lupishko; Di Martino; Lupishko (September 2000). "What the physical properties of near-Earth asteroids tell us about sources of their origin?". Kinematika i Fizika Nebesnykh Tel Supplimen 3 (3): 213–216. Bibcode 2000KFNTS...3..213L. 
  10. ^ Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". arXiv:1009.2710 [astro-ph.EP]. 

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