(101429) 1998 VF31
|Discovery site||Socorro, New Mexico|
|Discovery date||November 13, 1998|
1.00058445 Martian years
(101429) 1998 VF31 is a small asteroid that orbits near Mars's L5 Lagrangian point, on average trailing 60° behind it. Its orbit is highly stable, and was originally thought to be spectroscopically similar to 5261 Eureka, suggesting they may both be primordial Martian asteroids.
Spectroscopic observations through 2007 indicate that it has a large proportion of metal and achondrites on its surface (either with or without a mesosiderite contribution); which could also indicate that the surface regolith has undergone space weathering. These observations also reveal differences in the spectra with 5261 Eureka, suggesting they may not be related to each other after all.
- "JPL Small-Body Database Browser". Retrieved December 3, 2009.
- Rivkin, Andrew S.; Trilling, David E.; Thomas, Cristina A.; DeMeo, Francesca; Spahr, Timothy B.; Binzel, Richard P. (December 2007). "Composition of the L5 Mars Trojans: Neighbors, not Siblings". Icarus 192 (2): 434–441. arXiv:0709.1925. Bibcode:2007Icar..192..434R. doi:10.1016/j.icarus.2007.06.026.
- Rivkin, Andrew. S.; Binzel, R. P.; Howell, E. S.; Bus, S. J.; Grier, J. A. (October 2003). "Spectroscopy and photometry of Mars Trojans". Icarus 165 (2): 349–354. Bibcode:2003Icar..165..349R. doi:10.1016/S0019-1035(03)00211-2.
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