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Echus Chasma

Echus Chasma is a chasma in the Lunae Planum high plateau north of the Valles Marineris canyon system of Mars. It is in the Coprates quadrangle.[1] Clay has been found within it, meaning that water once sat there for a time.[2] It may have been one of the many lakes that have been advanced for the Martian past.

Echus Chasma
View of Echus Chasma in mosaic of THEMIS infrared images.
Coordinates1°00′N 278°00′E / 1.0°N 278.0°E / 1.0; 278.0
Length100 km
Width10 km
Depth4 km

Research from 2010 suggests that Mars had lakes along parts of the equator, which is where Echus Chasma lies. Although earlier research had showed that Mars had a warm and wet early history that has long since dried up, these lakes existed in the Hesperian Epoch, a much later period. Using detailed images from NASA's Mars Reconnaissance Orbiter, the researchers speculate that there may have been increased volcanic activity, meteorite impacts or shifts in Mars' orbit during this period to warm Mars' atmosphere enough to melt the abundant ice present in the ground. Volcanoes would have released gases that thickened the atmosphere for a temporary period, trapping more sunlight and making it warm enough for liquid water to exist.

In this study, channels were discovered that connected lake basins near Ares Vallis. When one lake filled up, its waters overflowed the banks and carved the channels to a lower area where another lake would form.[3][4] These dry lakes would be targets to look for evidence (biosignatures) of past life.

Geography edit

Echus Chasma is approximately 100 km long and 10 km wide, with valleys ranging in depth from around 1 km to 4 km.[1] It is the source region of the Kasei Valles outflow channel, which extends northward from it. It is situated just west of Hebes Chasma, to which it does not connect.

See also edit

References edit

  1. ^ a b ESA (2008-07-14). Echus Chasma. Retrieved on 2008-07-15 from http://www.esa.int/esaSC/SEM4CATHKHF_index_0.html.
  2. ^ http://www.jhu/~gazette/21jul08/21wetmars.html [dead link]
  3. ^ . Sciencedaily.com. January 4, 2010. Archived from the original on August 23, 2016. Retrieved March 9, 2018.
  4. ^ Gupta, Sanjeev; Warner, Nicholas; Kim, Rack; Lin, Yuan; Muller, Jan; -1#Jung-, Shih- (2010). "Hesperian equatorial thermokarst lakes in Ares Vallis as evidence for transient warm conditions on Mars". Geology. 38 (1): 71–74. Bibcode:2010Geo....38...71W. doi:10.1130/G30579.1.{{cite journal}}: CS1 maint: numeric names: authors list (link)

External links edit

  • ESA - Space Science - Echus Chasma
  • NASA Astronomy Picture of the Day: Echus Chasma from Mars Express (23 July 2008)

echus, chasma, chasma, lunae, planum, high, plateau, north, valles, marineris, canyon, system, mars, coprates, quadrangle, clay, been, found, within, meaning, that, water, once, there, time, have, been, many, lakes, that, have, been, advanced, martian, past, v. Echus Chasma is a chasma in the Lunae Planum high plateau north of the Valles Marineris canyon system of Mars It is in the Coprates quadrangle 1 Clay has been found within it meaning that water once sat there for a time 2 It may have been one of the many lakes that have been advanced for the Martian past Echus ChasmaView of Echus Chasma in mosaic of THEMIS infrared images Coordinates1 00 N 278 00 E 1 0 N 278 0 E 1 0 278 0Length100 kmWidth10 kmDepth4 kmResearch from 2010 suggests that Mars had lakes along parts of the equator which is where Echus Chasma lies Although earlier research had showed that Mars had a warm and wet early history that has long since dried up these lakes existed in the Hesperian Epoch a much later period Using detailed images from NASA s Mars Reconnaissance Orbiter the researchers speculate that there may have been increased volcanic activity meteorite impacts or shifts in Mars orbit during this period to warm Mars atmosphere enough to melt the abundant ice present in the ground Volcanoes would have released gases that thickened the atmosphere for a temporary period trapping more sunlight and making it warm enough for liquid water to exist In this study channels were discovered that connected lake basins near Ares Vallis When one lake filled up its waters overflowed the banks and carved the channels to a lower area where another lake would form 3 4 These dry lakes would be targets to look for evidence biosignatures of past life Contents 1 Geography 2 See also 3 References 4 External linksGeography editEchus Chasma is approximately 100 km long and 10 km wide with valleys ranging in depth from around 1 km to 4 km 1 It is the source region of the Kasei Valles outflow channel which extends northward from it It is situated just west of Hebes Chasma to which it does not connect nbsp Layers in Echus Chasma as seen by HiRISE nbsp Layers in Echus Chasma as seen by HiRISE under HiWish program See also editChasma Climate on Mars Geography of Mars Geology of Mars Graben HiRISE Lakes on Mars Tectonics of Mars nbsp Wikimedia Commons has media related to Echus Chasma References edit a b ESA 2008 07 14 Echus Chasma Retrieved on 2008 07 15 from http www esa int esaSC SEM4CATHKHF index 0 html http www jhu gazette 21jul08 21wetmars html dead link Spectacular Mars images reveal evidence of ancient lakes Sciencedaily com January 4 2010 Archived from the original on August 23 2016 Retrieved March 9 2018 Gupta Sanjeev Warner Nicholas Kim Rack Lin Yuan Muller Jan 1 Jung Shih 2010 Hesperian equatorial thermokarst lakes in Ares Vallis as evidence for transient warm conditions on Mars Geology 38 1 71 74 Bibcode 2010Geo 38 71W doi 10 1130 G30579 1 a href Template Cite journal html title Template Cite journal cite journal a CS1 maint numeric names authors list link External links editESA Space Science Echus Chasma NASA Astronomy Picture of the Day Echus Chasma from Mars Express 23 July 2008 Portal nbsp Solar System Retrieved from https en wikipedia org w index php title Echus Chasma amp oldid 1176981872, wikipedia, wiki, book, books, library,

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