| タイトル | Early Mars Climate Modeling and the Faint Young Sun Paradox. |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150021504 |
| 著者（英） | Haberle, Robert M. |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 2015-03-16 |
| 言語 | eng |
| 内容記述 | Today Mars is a cold, dry, desert planet. Liquid water is not stable on its surface. There are no lakes, seas, or oceans, and precipitation falls as snowfall. Yet early in its history during the Noachian epoch, there is geological and mineralogical evidence that liquid water from rainfall flowed on its surface creating drainage systems, lakes, and - possibly - seas and oceans. More recent observations by Curiosity in Gale crater hint that such conditions may have persited into the Hesperian. The implication is that early Mars had a wamer climate than it does today as a result of a thicker atmosphere with a more powerful greenhouse effect capable of producing an active hydrological cycle with rainfall, runoff, and evaporation. Since Mariner 9 began accumulating such evidence, researchers have been trying to understand what kind of a climate system could have created greenhouse conditions favorable for liquid water. Unfortunately, the problem is not yet solved. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | ARC-E-DAA-TN20333 |
| 権利 | No Copyright |
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