| タイトル | HDO in the Martian atmosphere - Implications for the abundance of crustal water |
| 著者（英） | Allen, Mark; Wen, Jun-Shan; Yung, Yuk L.; Pierce, Kathryn K.; Pinto, Joseph P. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech.|California Inst. of Tech. |
| 発行日 | 1988-10-01 |
| 言語 | eng |
| 内容記述 | A one-dimensional photochemical model is presently used to ascertain the nature of those chemical and physical processes of the Martian atmosphere responsible for the preferential escape of hydrogen over deuterium. A comparison of the present theoretical considerations with recent HDO observations indicates that Mars contains 0.2 m of (globally averaged) crustal water that is exchangeable with the atmosphere. This estimate, which is substantially lower than those obtained for Martian subsurface water on the basis of Viking image-derived geomorphological analyses, can be reconciled only if a small fration of the crustal water is exchangeable with the atmosphere. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 89A14393 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/367111 |
