| タイトル | Crater Lakes on Mars: Development of Quantitative Thermal and Geomorphic Models |
| 本文（外部サイト） | http://hdl.handle.net/2060/20050201828 |
| 著者（英） | Moore, J.; Asphaug, E.; Barnhart, C. J.; Tulaczyk, S.; Kraal, E. R. |
| 著者所属（英） | California Univ. |
| 発行日 | 2005-01-01 |
| 言語 | eng |
| 内容記述 | Impact craters on Mars have served as catchments for channel-eroding surface fluids, and hundreds of examples of candidate paleolakes are documented [1,2] (see Figure 1). Because these features show similarity to terrestrial shorelines, wave action has been hypothesized as the geomorphic agent responsible for the generation of these features [3]. Recent efforts have examined the potential for shoreline formation by wind-driven waves, in order to turn an important but controversial idea into a quantitative, falsifiable hypothesis. These studies have concluded that significant wave-action shorelines are unlikely to have formed commonly within craters on Mars, barring Earth-like weather for approx.1000 years [4,5,6]. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/85479 |
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