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Deuterium in comet C/1995 O1 (Hale-Bopp): detection of DCN

Authors :
Meier, R
Owen, T. C
Jewitt, D. C
Matthews, H. E
Senay, M
Biver, N
Bockel e-Morvan, D
Crovisier, J
Gautier, D
Source :
Science. 279(5357)
Publication Year :
1998
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1998.

Abstract

Deuterated 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.

Details

Language :
English
ISSN :
00368075
Volume :
279
Issue :
5357
Database :
NASA Technical Reports
Journal :
Science
Publication Type :
Report
Accession number :
edsnas.20040172751
Document Type :
Report
Full Text :
https://doi.org/10.1126/science.279.5357.1707