The Asteroid moon reference article from the English Wikipedia on 24-Apr-2004
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Asteroid moon

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An asteroid moon is an asteroid that orbits another asteroid. It is thought that many asteroids may possess moons, in some cases quite substantial in size. An asteroid whose moon is roughly the same size as the asteroid itself may be referred to as a binary asteroid.

The origin of asteroid moons is not currently known with certainty, and a variety of possibilities exist. A widely accepted theory is that asteroid moons are formed from debris knocked off of the primary asteroid by an impact.

The first asteroid moon known is Dactyl which orbits 243 Ida. It was discovered by the Galileo probe in 1993. The second moon was discovered around 45 Eugenia in 1999. By February, 2004, nearly 37 more asteroid moons had been discovered by Earth-bound telescopes. Asteroid moons have been discovered orbiting main belt asteroids, Trojan asteroids, near-Earth objects, and Kuiper Belt objects.

An example of a binary asteroid is 90 Antiope, where two equal-sized components orbit each other.

Notable Double Asteroids

NameOrbital typeDiameter (km)Name of MoonDiameter of Moon (km)Distance between pair (km)
22 Kalliopemain belt181Linus381,063
45 Eugeniamain belt215Petit-Prince131,190
87 Sylviamain belt261S/2001 (87) 1151,370
90 Antiopemain belt85S/2000 (90) 185170
107 Camillamain belt223S/2001 (107) 191,000
121 Hermionemain belt209S/2002 (121) 113795
243 Idamain belt108Dactyl1.4108
283 Emmamain belt148S/2003 (283) 112370
617 PatroclusJupiter Trojan105S/2001 (617) 195610
762 Pulcovamain belt137unnamed20810
1509 Esclangonamain belt12unnamed20810
3671 Dionysusnear-Earth asteroid7S/2003 (1509) 10.4140
3749 Balammain belt1.5S/2002 (3749) 11.5350
(26308) 1998 SM165TNO465S/2001 (26308) 11806,000
(47171) 1999 TC36Plutino680S/2001 (47171) 12908,000
(66391) 1999 KW4near-Earth asteroid1.2S/1997 (3671) 10.42.2



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