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Science 2 November 2001:
Vol. 294. no. 5544, pp. 1089 - 1091
DOI: 10.1126/science.1064339

Reports

The Spin Temperature of NH3 in Comet C/1999S4 (LINEAR)

Hideyo Kawakita,1* Jun-ichi Watanabe,2 Hiroyasu Ando,3 Wako Aoki,2 Tetsuharu Fuse,3 Satoshi Honda,2 Hideyuki Izumiura,4 Toshitaka Kajino,2 Eiji Kambe,5 Satoshi Kawanomoto,2 Kunio Noguchi,2 Kiichi Okita,3 Kozo Sadakane,6 Bun'ei Sato,47 Masahide Takada-Hidai,8 Yoichi Takeda,9 Tomonori Usuda,3 Etsuji Watanabe,4 Michitoshi Yoshida4

A high-dispersion spectrum of Comet C/1999S4 (LINEAR) was obtained in the optical region with the high-dispersion spectrograph on the Subaru telescope when the comet was 0.863 astronomical units from the Sun before its disintegration. We obtained high signal-to-noise ratio emission lines of the cometary NH2 bands from which an ortho-to-para ratio (OPR) of 3.33 ± 0.07 was derived on the basis of a fluorescence excitation model. Assuming that cometary NH2 mainly originates from ammonia through photodissociation, the derived OPR of NH2 molecules should reflect that of ammonia, which provides information on the environment of molecular formation or condensation and of the thermal history of cometary ices. Assuming that the OPR of ammonia in comets was unchanged in the nucleus, the derived spin temperature of ammonia (28 ± 2 kelvin) suggests that a formation region of the cometary ammonia ice was between the orbit of Saturn and that of Uranus in the solar nebula.

1 Gunma Astronomical Observatory, 6860-86 Nakayama, Takayama, Agatsuma, Gunma 377-0702, Japan.
2 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan.
3 Subaru Telescope, National Astronomical Observatory of Japan, 650 North Aohoku Place, Hilo, HI 96720, USA.
4 Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata-cho, Okayama, 719-0232, Japan.
5 Department of Earth and Ocean Sciences, National Defense Academy, Hashirimizu 1-10-20, Yokosuka, Kanagawa 239-8686, Japan.
6 Astronomical Institute, Osaka Kyoiku University, Kashiwara-shi, Osaka, 582-8582, Japan.
7 Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan.
8 Liberal Arts Education Center, Tokai University, 1117 Kitakaname, Hiratsuka-shi, Kanagawa, 259-1292, Japan.
9 Komazawa University, Komazawa, Setagaya, Tokyo 154-8525, Japan.
*   To whom correspondence should be addressed. E-mail: kawakita{at}astron.pref.gunma.jp


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THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
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Z.-D. Sun, K. Takagi, and F. Matsushima (2005)
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