| タイトル | Tectonic setting of Martian volcanoes and deep-seated intrusives |
| 本文（外部サイト） | http://hdl.handle.net/2060/19920001533 |
| 著者（英） | Dohm, James M.; Scott, David H. |
| 著者所属（英） | Geological Survey |
| 発行日 | 1991-06-01 |
| 言語 | eng |
| 内容記述 | More than 50 volcanoes have been mapped on Mars, and recent geologic studies indicate structural evidence of deep seated intrusive bodies. Most volcanoes in the Tharsis region are volcanotectonic features; they have been associated with large scale tectonic and volcanic processes. They occur along complex systems of faults and grabens having a dominant northwest to southwest trend closely coincident with a great circle, which extends along 90 deg of arc from Tempe Patera to probable volcanic mountains near lat. 40 deg S, long. 150 deg. Deep seated intrusive bodies are also concentrated in the Tharsis region and are recognized mostly where faults have been deflected around their cores. The Elysium Mons-Amphitrites Patera volcanic alignment is subparallel to that of Tharsis but is longer, extending through about 120 deg of arc; it transects the dichotomy boundary and is radial to the Hellas basin. Volcanoes in the Tharsis region have the widest age range of all volcanoes on Mars, as determined by the size-frequency distribution of their craters having diameters of 2, 5, and 16 km. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 92N10751 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/130514 |
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