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Deuterium in comet C/1995 O1 (Hale-Bopp): detection of DCN.
Meier, R; Owen, T C; Jewitt, D C; Matthews, H E; Senay, M; Biver, N; Bockel e-Morvan, D; Crovisier, J; Gautier, D.
Affiliation
  • Meier R; University of Hawaii, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA. meier@uhifa.ifa.hawaii.edu
Science ; 279(5357): 1707-10, 1998 Mar 13.
Article in En | MEDLINE | ID: mdl-9497286
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.
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Collection: 01-internacional Database: MEDLINE Main subject: Hydrogen Cyanide / Meteoroids / Deuterium Type of study: Diagnostic_studies Language: En Journal: Science Year: 1998 Document type: Article Affiliation country: United States
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Collection: 01-internacional Database: MEDLINE Main subject: Hydrogen Cyanide / Meteoroids / Deuterium Type of study: Diagnostic_studies Language: En Journal: Science Year: 1998 Document type: Article Affiliation country: United States
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