翻訳と辞書 ・ (185851) 2000 DP107 ・ (19255) 1994 VK8 ・ (192642) 1999 RD32 ・ (19299) 1996 SZ4 ・ (19308) 1996 TO66 ・ (1952–19??) ・ (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
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(202421) 2005 UQ513 : ウィキペディア英語版 | (202421) 2005 UQ513
, also written as 2005 UQ513, is a cubewano with an absolute magnitude of 3.4.〔 Mike Brown's website lists it as a highly likely dwarf planet.〔 shows signs of weak water ice. Like Quaoar,〔Trujillo, C. A., Sheppard, S. S., & Schaller E. L. (2011). (A Photometric System for Detection of Water and Methane Ices on Kuiper Belt Objects )〕 it has a very〔 red spectrum,〔〔 which indicates that its surface probably contains a lot of complex, processed organic molecules.〔Pinilla-Alonso, N., Licandro, J., & Lorenzi, V. (2008). (Visible spectroscopy in the neighborhood of (Haumea) )〕 Its light curve shows variations of ''Δm''=0.3 mag, but no period has been determined.〔Snodgrass, C., Carry, B., Dumas, C., & Hainaut, O. (2009). (Characterisation of candidate members of (136108) Haumea’s family )〕 == Classification ==
has a perihelion of 37.3 AU.〔 The Minor Planet Center (MPC) classifies it as a cubewano〔 while the Deep Ecliptic Survey (DES) classifies it as ScatExt (scattered-extended).〔 Although dynamically it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum it is not.〔〔
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「(202421) 2005 UQ513」の詳細全文を読む
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