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- Tobias Owen
- Department of Earth and Space Sciences, State University of New York, Stony Brook, NY 11794
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- Jean Pierre Maillard
- Institut d'Astrophysique de Paris, F-75014 Paris, France
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- Catherine de Bergh
- Observatoire de Paris, 92195 Meudon, France
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- Barry L. Lutz
- Lowell Observatory, Flagstaff, AZ 86001
書誌事項
- 公開日
- 1988-06-24
- DOI
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- 10.1126/science.240.4860.1767
- 公開者
- American Association for the Advancement of Science (AAAS)
この論文をさがす
説明
<jats:p> Deuterium on Mars has been detected by the resolution of several Doppler-shifted lines of HDO near 3.7 micrometers in the planet's spectrum. The ratio of deuterium to hydrogen is (9 ± 4) × 10 <jats:sup>-4</jats:sup> ; the abundance of H <jats:sub>2</jats:sub> 0 was derived from lines near 1.1 micrometers. This ratio is enriched on Mars over the teiluric value by a factor of 6 ± 3. The enrichment implies that hydrogen escaped more rapidly from Mars in the past than it does now, consistent with a dense and warm ancient atmosphere on the planet. </jats:p>
収録刊行物
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- Science
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Science 240 (4860), 1767-1767, 1988-06-24
American Association for the Advancement of Science (AAAS)
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詳細情報 詳細情報について
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- CRID
- 1363670320818864256
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- NII論文ID
- 30020535701
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- ISSN
- 10959203
- 00368075
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