Observations of water in comets with Odin

被引:60
作者
Lecacheux, A
Biver, N
Crovisier, J
Bockelée-Morvan, D
Baron, P
Booth, RS
Encrenaz, P
Florén, HG
Frisk, U
Hjalmarson, Å
Kwok, S
Mattila, K
Nordh, L
Olberg, M
Olofsson, AOH
Rickman, H
Sandqvist, A
von Schéele, F
Serra, G
Torchinsky, S
Volk, K
Winnberg, A
机构
[1] Observ Paris, CNRS, FRE 2461, F-92195 Meudon, France
[2] European Space Agcy, ESTEC, NL-2200 AG Noordwijk, Netherlands
[3] Noveltis, F-31520 Ramonville St Agne, France
[4] Onsala Space Observ, S-43992 Onsala, Sweden
[5] Observ Paris, CNRS, FRE 2460, F-75014 Paris, France
[6] SCFAB Albanova, Stockholm Observ, S-10691 Stockholm, Sweden
[7] Swedish Space Corp, S-17104 Solna, Sweden
[8] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
[9] Univ Helsinki Observ, Helsinki 00014, Finland
[10] Swedish Natl Space Board, S-17104 Solna, Sweden
[11] Astron Observ, S-75120 Uppsala, Sweden
[12] Ctr Etud Spatiale Rayonnements, F-31029 Toulouse, France
[13] Canadian Space Agcy, St Hubert, PQ J3Y 8Y9, Canada
关键词
comets : general; comets; individual; C/2001; A2; (LINEAR); 19P/Borrelly; C/2000; WM1; LINEAR); 153P/2002; C1; (Ikeya-Zhang); radio lines : solar system; submillimeter; VAPOR; LEE;
D O I
10.1051/0004-6361:20030338
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Odin satellite, which can observe the 1(10)-1(01) rotational line at 557 GHz of ortho water with a high spectral resolution (80 m s(-1)) and a spatial resolution of 2.1', is well suited for cometary studies. The intensity of this line provides an estimate of the water production rate. The line width gives a direct measure of the coma expansion velocity. The line centre position and shape are affected by the anisotropy of the outgassing and by optical depth effects. Comets observed with Odin up to now are C/2001 A2 (LINEAR) during the commissioning phase of the satellite, 19P/Borrelly at the time of the Deep Space 1 flyby, C/2000 WM1 (LINEAR), and 153P/2002 C1 (Ikeya-Zhang). For this last comet, thorough observations were made at the moment of its closest approach to Earth at the end of April 2002. A deep integration resulted in the detection of the 1(10)-1(01) line of (H2O)-O-18 at 548 GHz. No O-16/O-18 isotopic anomaly is found.
引用
收藏
页码:L55 / L58
页数:4
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