翻訳と辞書 ・ (196256) 2003 EH1
・ (2+1)-dimensional topological gravity
・ (2,2,3-Trimethyl-5-oxocyclopent-3-enyl)acetyl-CoA 1,5-monooxygenase
・ (2,2,3-trimethyl-5-oxocyclopent-3-enyl)acetyl-CoA synthase
・ (2,3,7) triangle group
・ (2,3-dihydroxybenzoyl)adenylate synthase
・ (2,4,6-Trimethylphenyl)gold
・ (2-Chlorophenyl)thiourea
・ (20026) 1992 EP11
・ (202421) 2005 UQ513
・ (208996) 2003 AZ84
・ (21083) 1991 TH14
・ (214869) 2007 PA8
・ (21900) 1999 VQ10
・ (225088) 2007 OR10
・ (225312) 1996 XB27
・ (229762) 2007 UK126
・ (230965) 2004 XA192
・ (23624) 1996 UX3
・ (237442) 1999 TA10
・ (242450) 2004 QY2
・ (24835) 1995 SM55
・ (248835) 2006 SX368
・ (24952) 1997 QJ4
・ (24978) 1998 HJ151
・ (251732) 1998 HG49
・ (26181) 1996 GQ21
・ (26308) 1998 SM165
・ (26375) 1999 DE9
・ (276033) 2002 AJ129
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| (225312) 1996 XB27 ： ウィキペディア英語版 |
(225312) 1996 XB27
, also written as 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.〔Evans, N. W. & Tabachnik, S. (1999). (Possible long-lived asteroid belts in the inner Solar System ). ''Nature''.〕
It is classified as an Amor asteroid〔 because its perihelion is less than 1.3 AU and does not cross Earth's orbit.
Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.〔(JPL close-approach data ) Retrieved 2011-09-04〕
==See also==
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