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Dao Vallis

Coordinates:38°42′S272°06′W/ 38.7°S 272.1°W/-38.7; -272.1
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Dao Vallis
Dao Vallis is the leftmost channel, joined just above the center of the image byNiger Vallis.In each valley water flowed toward the bottom of the image. The caldera ofHadriacus Monsis at upper left.
Coordinates38°42′S272°06′W/ 38.7°S 272.1°W/-38.7; -272.1
Length816.0 km
NamingWord for "star" in Thai

Dao Vallisis a valley onMarsthat appears to have been carved by water. It runs southwestward intoHellas Planitiafrom the southern slopes of the volcanoHadriacus Mons,and has been identified as anoutflow channel.[1]It and itstributary,Niger Vallis,extend for about 1,200 km (750 mi).[2]

It is named after theThaiword forstar,and it was proposed as a potential landing site for the 2012Curiosity roverof theMars Science Laboratorymission.[3]In the fictional 2007 Canadian miniseriesRace to Mars,it is the landing site forGagarin,the lander.

Origin

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Dao Vallis begins near a large volcano, Hadriacus Mons, so it is thought to have received water when hot magma melted huge amounts of ice in the frozen ground. Much of this water may have been released in very large "outburst floods". The partially circular depressions on the left side of the channel in the image below suggests that groundwater sapping also contributed water more gradually.[4]

See also

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References

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  1. ^Carr, M.H. (2006), The Surface of Mars. Cambridge Planetary Science Series, Cambridge University Press.
  2. ^Crown, D. A.; Bleamaster, L. F.; Mest, S. C. (2003). "Geologic Evolution of Dao Vallis, Mars".AGU Fall Meeting Abstracts.2003:P11B–1035.Bibcode:2003AGUFM.P11B1035C.
  3. ^"MSL Workshop Summary"(PDF).April 27, 2007.RetrievedMay 29,2007.
  4. ^Dao Vallis (Released 7 August 2002)
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