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Science 24 June 1983:
Vol. 220. no. 4604, pp. 1374 - 1375
DOI: 10.1126/science.220.4604.1374
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Articles

Titan: Discovery of Carbon Monoxide in Its Atmosphere

BARRY L. LUTZ 1, CATHERINE DE BERGH 2, and TOBIAS OWEN 3

1 Planetary Research Center, Lowell Observatory, Flagstaff, Arizona 86002
2 Laboratoire d'Astronomie Infrarouge, Observatoire de Meudon, 92190 Meudon, France
3 Department of Earth and Space Sciences, State University of New York, Stony Brook 11794

The 3-0 rotation-vibration band of carbon monoxide in the near-infrared spectrum of Titan has been identified, and a reflecting layer model mixing ratio of carbon monoxide to molecular nitrogen of 6 x 10–5 has been determined. This result supports the probable detection of carbon dioxide by Samuelson and his co-workers and strengthens possible analogies between the atmosphere of Titan and conditions on primitive Earth.

Submitted on December 27, 1982
Revised on March 14, 1983


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Radar Reflectivity of Titan.
D. O. Muhleman, D. O. Muhleman, A. W. Grossman, B. J. Butler, and M. A. Slade (1990)
Science 248, 975-980
   Abstract »    PDF »
Microwave Measurements of Carbon Monoxide on Titan.
D. O. Muhleman, D. O. MUHLEMAN, G. L. BERGE, and R. T. CLANCY (1984)
Science 223, 393-396
   Abstract »    PDF »
Ethane Ocean on Titan.
J. I. Lunine, J. I. LUNINE, D. J. STEVENSON, and Y. L. YUNG (1983)
Science 222, 1229-1230
   Abstract »    PDF »


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Science. ISSN 0036-8075 (print), 1095-9203 (online)