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(121514) 1999 Uj7

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Title: (121514) 1999 Uj7  
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Subject: Mars trojan, (101429) 1998 VF31, Trojan (astronomy), Asopus Vallis, Moons of Mars
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(121514) 1999 Uj7

(121514) 1999 UJ7
Discovered by October 30, 1999 by LINEAR
Discovery site Socorro
2002 AC180[1]
Minor planet category Martian L4 Martian L4
Orbital characteristics[1]
Epoch 2455800.5 (2011-Aug-27.0)
Aphelion 1.5841307 AU
Perihelion 1.4647585 AU
1.5244446 AU
Eccentricity 0.0391527
687.4892520 d
1.88 yr
Inclination 16.74985°
Physical characteristics
Dimensions ~1 km[2]
Spectral type

(121514) 1999 UJ7 is a small asteroid orbiting near the of Mars (60 degrees ahead Mars on its orbit).[2] As of September 2011, (121514) 1999 UJ7 is the only known asteroid to orbit the leading of Mars, although at least three other asteroids orbit Mars's trailing L5 point: 5261 Eureka, (101429) 1998 VF31, and 2007 NS2.[2] Not only does (121514) 1999 UJ7 orbit on the other side of Mars from other similar asteroids, its spectrum is different as well, which is puzzling because all of the Martian trojans seem to be in very stable orbits.[3]


(121514) 1999 UJ7 orbits around the L4 point of Mars in a very stable orbit and is large enough that the Yarkovsky effect will not affect its orbit.[2]

Physical characteristics

Due to similarity in the measured brightness of (121514) 1999 UJ7 with other Martian trojans, it is thought to be a small asteroid with an effective diameter on the order of 1 kilometer (0.62 mi).[2] Its spectrum suggests that it is an X-type asteroid, which is different from 5261 Eureka and 1998 VF31,[3] and is somewhat puzzling since different mineral compositions suggest different origins for the two groups of asteroids. The long lifetime of the orbits for these asteroids makes the possibility of one or more of them being interlopers unlikely, however. This suggests that either one or more of the Martian trojans was captured in such a way as to give it a long-term stable orbit (and it is therefore not a primordial Martian asteroid), or that some fusion or combination of previous asteroids resulted in the presently observed ones.[3] The Yarkovsky effect may provide a potential capture mechanism but not enough is known about the shapes of these objects to provide a useful Yarkovsky model.[3]

See also


  1. ^ a b c d NASA JPL Small-Body Database Browser on (121514) 1999 UJ7
  2. ^ a b c d e Scholl, H.; Marzari, F.; Tricarico, P. (June 2005). "Dynamics of Mars Trojans".  
  3. ^ a b c d e Rivkin, A. S.; Binzel, R. P.; Howell, E. S.; Bus, S. J.; Grier, J. A. (October 2003). "Spectroscopy and photometry of Mars Trojans".  

External links

  • NASA JPL Small-Body Database Browser on (121514) 1999 UJ7
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