Moreux (crater)
 Map of Ismenius Lacus quadrangle which is located just north of Arabia, a large bright area of Mars. It contains large amounts of ice in glaciers that surround hills. | |
| Planet | Mars |
|---|---|
| Coordinates | 42°06′N 315°36′W / 42.1°N 315.6°W |
| Quadrangle | Ismenius Lacus |
| Diameter | 138 km |
| Eponym | Theophile Moreux, a French astronomer and meteorologist (1867-1954) |
Moreux is a crater in the Ismenius Lacus quadrangle on Mars with a diameter of 138 kilometers. It is located at 42.1° north latitude and 315.6° west longitude and was named by IAU's Working Group for Planetary System Nomenclature after Theophile Moreux, a French astronomer and meteorologist (1867–1954).[1]
Glaciers
Moreux Crater's appearance has been shaped by the action of glaciers. Recent research, using a variety of images from various cameras, discovered extensive glacial modification of the surfaces of Moreux Crater's rim, wall, and central peak. These changes were caused by the emplacement of ice-rich material when the climate underwent major changes.[2] The picture from HiRISE below shows possible kettles in Moreux Crater.
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MOLA map of Moreux Crater and other nearby craters. Colors indicate elevations. -
Moreux Crater moraines and kettle holes, as seen by HiRISE. -
Western edge of Moreux Crater, as seen by CTX (camera), on the Mars Reconnaissance Orbiter. Arrows indicate probable glacial moraines. Crater floor is to the right. -
Wide, glacial valleys in Moreux Crater, as seen by HiRISE under HiWish program. -
Glacier coming out of valley, as seen by HiRISE under HiWish program Location is rim of Moreux Crater.
Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak.[3] The peak is caused by a rebound of the crater floor following the impact.[4] Sometimes craters expose layers that were buried. Rocks from deep underground are tossed onto the surface. Hence, craters can show us what lies deep under the surface.
Dunes
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Wide view of dunes in Moreux Crater, as seen by HiRISE under HiWish program -
Enlarged view of dunes on the bottom of the previous image, as seen by HiRISE under HiWish program -
Close view of one large dune from the same location, as seen by HiRISE under HiWish program -
Close view of white spot among the dark dunes showing ripples and streaks
See also
- Climate of Mars
- Deuteronilus Mensae
- Fretted terrain
- Glacier
- Glaciers on Mars
- Lobate debris apron
- Protonilus Mensae
- Water on Mars
- List of craters on Mars
- Water on Mars
- Ore genesis
- Ore resources on Mars
- Hydrothermal circulation
References
- ^ "Gazetteer of Planetary Nomenclature | Moreux". usgs.gov. International Astronomical Union. Retrieved 4 March 2015.
- ^ Rishitosh K., S. Sinha, S. Murty. 2015. Amazonian modification of Moreux crater: Record of recent and episodic glaciation in the Protonilus Mensae region of Mars. Icarus 245:122-144.
- ^ http://www.lpi.usra.edu/publications/slidesets/stones/
- ^ Hugh H. Kieffer (1992). Mars. University of Arizona Press. ISBN 978-0-8165-1257-7. Retrieved 7 March 2011.
