Is Sedna another Triton?

被引:57
作者
Barucci, MA [1 ]
Cruikshank, DP
Dotto, E
Merlin, F
Poulet, F
Ore, CD
Fornasier, S
de Bergh, C
机构
[1] Observ Paris, LESIA, F-92195 Meudon, France
[2] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[3] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
[4] Univ Paris 11, IAS, F-91405 Orsay, France
[5] SETI Inst, Mountain View, CA USA
[6] Dipartimento Astron, I-35122 Padua, Italy
关键词
TNOs; visible; infrared; spectroscopy; photometry;
D O I
10.1051/0004-6361:200500144
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
90377 Sedna is, so far, the largest and most distant trans-neptunian object. It was observed at visible and near-infrared wavelengths using simultaneously two 8.2 m telescopes at the Very Large Telescope of the European Southern Observatory. The spectrum of Sedna suggests the presence on its surface of different ices ( total abundance > 50%). Its surface composition is different from that determined for other trans-neptunian objects, and apparently resembles that of Triton, particularly in terms of the possible presence of nitrogen and methane ices.
引用
收藏
页码:L1 / L4
页数:4
相关论文
共 23 条
[1]   Visible and near-infrared spectroscopy of the Centaur 32532 (2001 PT13) -: ESO large program on TNOs and Centaurs:: First spectroscopy results [J].
Barucci, MA ;
Boehnhardt, H ;
Dotto, E ;
Doressoundiram, A ;
Romon, J ;
Lazzarin, M ;
Fornasier, S ;
de Bergh, C ;
Tozzi, GP ;
Delsanti, A ;
Hainaut, O ;
Barrera, L ;
Birkle, K ;
Meech, K ;
Ortiz, JL ;
Sekiguchi, T ;
Thomas, N ;
Watanabe, J ;
West, RM ;
Davies, JK .
ASTRONOMY & ASTROPHYSICS, 2002, 392 (01) :335-339
[2]  
BARUCCI MA, 2004, COMETS, V647
[3]  
BARUCCI MA, 2005, IN PRESS AJ, V130
[4]   Large-scale correlations in the Lyα forest at z=3-4 [J].
Becker, GD ;
Sargent, WLW ;
Rauch, M .
ASTROPHYSICAL JOURNAL, 2004, 613 (01) :61-76
[5]  
BROWN GN, 1979, ADV CRYOGEN ENG, V25, P662
[6]   Discovery of a candidate inner Oort Cloud planetoid [J].
Brown, ME ;
Trujillo, C ;
Rabinowitz, D .
ASTROPHYSICAL JOURNAL, 2004, 617 (01) :645-649
[7]   ICES ON THE SURFACE OF TRITON [J].
CRUIKSHANK, DP ;
ROUSH, TL ;
OWEN, TC ;
GEBALLE, TR ;
DEBERGH, C ;
SCHMITT, B ;
BROWN, RH ;
BARTHOLOMEW, MJ .
SCIENCE, 1993, 261 (5122) :742-745
[8]   Spectral models of Kuiper Belt objects and Centaurs [J].
Cruikshank, DP ;
Ore, CMD .
EARTH MOON AND PLANETS, 2003, 92 (1-4) :315-330
[9]   Water ice on Triton [J].
Cruikshank, DP ;
Schmitt, B ;
Roush, TL ;
Owen, TC ;
Quirico, E ;
Geballe, TR ;
de Bergh, C ;
Bartholomew, MJ ;
Ore, CMD ;
Douté, S ;
Meier, R .
ICARUS, 2000, 147 (01) :309-316
[10]   Water ice on the surface of the large TNO 2004 DW [J].
Fornasier, S ;
Dotto, E ;
Barucci, MA ;
Barbieri, C .
ASTRONOMY & ASTROPHYSICS, 2004, 422 (02) :L43-L46