 Marte Vallis based on THEMIS day-time image | |
| Coordinates | 15°00′N 176°30′W / 15°N 176.5°W / 15; -176.5 |
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Marte Vallis is a valley in the Amazonis quadrangle of Mars, located at 15 North and 176.5 West. It is 185 km long and was named for the Spanish word for "Mars". It has been identified as an outflow channel, carved in the geological past by catastrophic release of water from aquifers beneath the Martian surface. The surface material is thought to have been created out of 'a'ā and pāhoehoe lava flows from the Elysium volcanic province in the west.
Marte Vallis is the site of the first discovery of columnar jointing on Mars. Columnar jointing often forms when basalt lava cools.
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Streamlined Island in Marte Vallis, as seen by HiRISE. The enlarged image gives a good view of dark slope streaks. Island is just to the west of Pettit Crater. Scale bar is 500 meters long.
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Layers in old crater rim, in Marte Vallis as seen by HiRISE under HiWish program
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Close view of layers from previous image, as seen by HiRISE under HiWish program Some dark slope streaks are visible.
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Columinar Jointing in Yellowstone National Park.
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Columnar jointing in the basalt of the Giant's Causeway in Northern Ireland
References
- ^ Milazzo, M.P., Keszthelyi, L.P., Jaeger, W.L. Rosiek, M., Mattson, S., Verba, C., Beyer, R.A., Geissler, P.E., McEwen, A.S., and the HiRISE Team. (2009) Discovery of columnar jointing on Mars. Geology. 37(2), 171–174. Abstract
- "Home". planetarynames.wr.usgs.gov.
- Carr, M.H. (2006), The Surface of Mars. Cambridge Planetary Science Series, Cambridge University Press.
- Voigt, Joana R. C.; Hamilton, Christopher W. (2018-07-15). "Investigating the volcanic versus aqueous origin of the surficial deposits in Eastern Elysium Planitia, Mars". Icarus. 309: 389–410. Bibcode:2018Icar..309..389V. doi:10.1016/j.icarus.2018.03.009. ISSN 0019-1035. S2CID 125918565.
- Bates, R. and J. Jackson (eds.) 1976. Dictionary of Geological Terms. Doubleday, New York.
See also
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