Mojave (crater)
outflow channel Tiu Valles snakes through the image south-north to the right of Mojave. | |
| Planet | Mars |
|---|---|
| Coordinates | 7°30′N 33°00′W / 7.5°N 33.0°W |
| Quadrangle | Oxia Palus |
| Eponym | Mojave, California, USA |
Mojave is a 58 km diameter impact crater in the Oxia Palus quadrangle of Mars, located at 7.5° N and 33.0° W. It was named after the town of Mojave in southern California, U.S.[1]
The crater is located within the Martian Xanthe Terra region.
Description
Mojave has alluvial fans that look remarkably similar to landforms in the Mojave Desert in the American southwest. Fans inside and around the outsides of the crater are closely similar to Earth's alluvial fans. As on Earth, the largest rocks are near the mouths of the fans. Because the channels start at ridge tops, it is believed they were formed by heavy downpours. Researchers have suggested that the rain may have been initiated by impacts.[2][3]
Some parts of the crater display a high concentration of closely spaced pits. Pits show little or no evidence of rims or ejecta. The pits are so close to each other that adjacent pits often share the same wall. It is believed that the pits form from steam produced when the heat from the impact process interacts with ice in the ground.[4][5]
The depth of Mojave is approximately 2,600 meters (1.63 miles). Based on its ratio of depth to diameter, researchers believe it is very young. It is not old enough to have accumulated much material and start to fill. Its relatively undegraded state helps scientists model impact processes on Mars.[6] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different.[7]
Mojave is a
Gallery
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Mojave as seen by CTX camera (on Mars Reconnaissance Orbiter). -
Alluvial fans in Mojave, as seen by HiRISE. The crater rim is on the right. A branched network of channels runs downward towards the left. -
Another view of Mojave from HiRISE. North is at bottom.
See also
References
- USGS. Retrieved 2014-03-06.
- ^ "HiRISE | Alluvial Fans in Mojave Crater: Did It Rain on Mars? (PSP_001415_1875)".
- ^ "HiRISE | Sedimentary Fans North of Mojave Crater (ESP_038851_1900)".
- ^ Boyce, J. et al. 2012. Origin of small pits in Martian impact craters. Icarus: 221, 262-275.
- ^ Tornabene, L., et al. 2012. Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process. Icarus: 220, 348-368.
- ^ "HiRISE | DTM".
- ^ Garvin, J., et al. 2002. Global geometric properities of martian impact craters. Lunar Planet Sci. 33. Abstract @1255.
- S2CID 206553043.
- ^ Aron, J. (2014-03-07). "Most Mars meteorites may be from same giant crater". New Scientist web site. New Scientist. Retrieved 2014-03-08.
External links
- Accurate animations of flights over Mars in at 100 meter altitude[permanent dead link]
- High resolution video by Seán Doran of an overflight of the northwest rim of Mojave, based on a NASA digital terrain model (see Fig. 4)
- Another video by Seán Doran of a south-to-north overflight of parts of Tiu Valles and Chryse Chaos, passing over Mojave in about the middle, based on Mars Express imagery
