Wegener (Martian crater)
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Wegener is an
impact crater An impact crater is a circular depression in the surface of a solid astronomical object formed by the hypervelocity impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal collapse, impact crater ...
in the Argyre quadrangle of
Mars Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, only being larger than Mercury. In the English language, Mars is named for the Roman god of war. Mars is a terrestrial planet with a thin at ...
, located at 64.6°S latitude and 4.0°W longitude. It measures approximately in diameter and was named after German geophysicist
Alfred Wegener Alfred Lothar Wegener (; ; 1 November 1880 – November 1930) was a German climatologist, geologist, geophysicist, meteorologist, and polar researcher. During his lifetime he was primarily known for his achievements in meteorology and ...
(1880–1930). The name was approved by IAU's
Working Group for Planetary System Nomenclature The International Astronomical Union (IAU; french: link=yes, Union astronomique internationale, UAI) is a nongovernmental organisation with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach ...
in 1973.


Description

Dark spots appear on dunes in the higher latitudes of Mars. In these spots mineral grains may be covered with a thin film of water that may affect chemical weathering of minerals and may help possible Martian organisms to survive. Studies have shown that thin films of water could exist at times on the Martian surface at certain times and in certain locations. In places, thin layers of liquid water could be present for 38 sols (Martian days) in the warmer periods of the day. Dark spots appear on dunes in the higher latitudes of Mars. Sometimes geysers form near the spots. They have two main features (dark dune spots and spider channels) that appear at the beginning of the Martian spring on dune fields covered with carbon dioxide (CO2 or 'dry ice'), mainly at the ridges and slopes of the dunes; by the beginning of winter, they disappear. Dark spots' shape is generally round, on the slopes it is usually elongated. With the stronger sunshine of spring in certain regions, carbon dioxide gas jets shoot dark dust in the air. This dark dust will increase the absorption of light and cause the temperature to rise to where water can exist for short periods.Kereszturi, A., E. Rivera-Valentin. 2012. "Locations of thin liquid water layers on present-day Mars". ''Icarus'': 221, 289–295.


See also

* List of craters on Mars


References

{{Geography of Mars Argyre quadrangle Impact craters on Mars