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Deuterium in comet C/1995 O1 (Hale-Bopp): detection of DCNDeuterated hydrogen cyanide (DCN) was detected in a comet, C/1995 O1 (Hale-Bopp), with the use of the James Clerk Maxwell Telescope on Mauna Kea, Hawaii. The inferred deuterium/hydrogen (D/H) ratio in hydrogen cyanide (HCN) is (D/H)HCN = (2.3 +/- 0.4) x 10(-3). This ratio is higher than the D/H ratio found in cometary water and supports the interstellar origin of cometary ices. The observed values of D/H in water and HCN imply a kinetic temperature >/=30 +/- 10 K in the fragment of interstellar cloud that formed the solar system.
Document ID
20040172751
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Meier, R.
(Institute for Astronomy 2680 Woodlawn Drive, Honolulu, HI 96822, United States)
Owen, T. C.
Jewitt, D. C.
Matthews, H. E.
Senay, M.
Biver, N.
Bockel e-Morvan, D.
Crovisier, J.
Gautier, D.
Date Acquired
August 22, 2013
Publication Date
March 13, 1998
Publication Information
Publication: Science
Volume: 279
Issue: 5357
ISSN: 0036-8075
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Other
Keywords
Non-NASA Center
NASA Discipline Exobiology

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