タイトル | Martian surface and crust - Review and synthesis. |
著者(英) | Hartmann, W. K. |
発行日 | 1973-08-01 |
言語 | eng |
内容記述 | The nature of the classical marking of Mars are studied on the basis of Mariner 9 data and some earlier data. The analysis leads to a model of the Martian crust. Evidence for petrologic distinctions between surface materials in dark and light regions is obtained. It is shown that the classical markings are a complex result of three factors: (1) availability of two types of rock material transportable by wind, (2) topographic control of deposition, and (3) prevailing winds producing quasi-permanent preferential deposition patterns. The crust, especially in the Tharsis region, bears strong evidence of mantle-induced uplift of a type existing on earth. Such uplifts have obliterated ancient craters, caused fractures and graben systems, and have resulted in intense volcanism. |
NASA分類 | SPACE SCIENCES |
レポートNO | 73A44543 |
権利 | Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/455796 |
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