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・ (-)-endo-alpha-bergamotene synthase ((2Z,6Z)-farnesyl diphosphate cyclizing)
・ (-)-Endo-fenchol dehydrogenase
・ (-)-endo-fenchol synthase
・ (-)-gamma-cadinene synthase ((2Z,6E)-farnesyl diphosphate cyclizing)
・ (-)-germacrene D synthase
・ (-)-Isopiperitenone reductase
・ (-)-menthol dehydrogenase
・ (-)-menthol monooxygenase
・ (-)-sabinene synthase
・ (1+ε)-approximate nearest neighbor search
・ (1,1'-Bis(diphenylphosphino)ferrocene)palladium(II) dichloride
・ (1,2,5,6-Tetrahydropyridin-4-yl)methylphosphinic acid
・ (1-4)-a-D-glucan 1-a-D-glucosylmutase
・ (1-hydroxycyclohexan-1-yl)acetyl-CoA lyase
・ (10115) 1992 SK
(101429) 1998 VF31
・ (101869) 1999 MM
・ (10302) 1989 ML
・ (11351) 1997 TS25
・ (11435) 1931 UB
・ (11436) 1969 QR
・ (11671) 1998 BG4
・ (118228) 1996 TQ66
・ (118378) 1999 HT11
・ (118379) 1999 HC12
・ (118702) 2000 OM67
・ (119068) 2001 KC77
・ (119070) 2001 KP77
・ (119878) 2002 CY224
・ (119951) 2002 KX14


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(101429) 1998 VF31 : ウィキペディア英語版
(101429) 1998 VF31

is a small asteroid that orbits near Mars's 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.
== See also ==

* 5261 Eureka
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抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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