User:VMKarnes/Aram Chaos

Aram Chaos
	Aram Chaos is the circular depression in the top left. Iani Chaos is in the bottom right.
Planet	Mars
Region	Margaritifer Terra
Coordinates	2°36′N 21°30′W / 2.6°N 21.5°W
Quadrangle	Oxia Palus
Diameter	280 kilometers (170 mi)
Depth	3 kilometers (1.9 mi)

Aram Chaos, centered at 2.6°N, 21.5°W, is a heavily eroded impact crater on Mars. It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis. Various geological processes have reduced it to a circular area of chaotic terrain. Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli, who named it after the Biblical land of Aram. Spectroscopic observation from orbit indicates the presence of the mineral hematite, likely a signature of a once aqueous environment.

Description

Aram Chaos is an impact crater on Mars measuring 280 kilometers (170 mi) in diameter. It lies in the Oxia Palus quadrangle in a region called Margaritifer Terra, and its exact coordinates on Mars are 2°36′N 21°30′W / 2.6°N 21.5°W / 2.6; -21.5. The Thermal Emission Imaging System (THEMIS) on the orbiter Mars Odyssey found gray crystalline hematite on the floor of Aram Chaos and CRISM, the spectroscope on the MRO, found hydrated sulfates, jarosite, and hematite. The floor of Aram Chaos also contains huge blocks of collapsed, or chaotic, terrain that formed when water or ice was catastrophically removed. Small, shallow outlet channels are also visible in the eastern wall of the impact crater, as well as a small outflow channel connecting Aram Chaos with the Ares Valles outflow channel.

Geology

Formation

Aram Chaos, as an impact crater, started its formation with the high velocity impact of an unknown smaller body on the surface of Mars. This formed the large, circular depression that originally made up the crater. This crater was then filled with sediments, likely carried by aeolian processes, that were deposited into Aram Chaos over time. Subsequently and in tandem with the compilation of these sedimentary layers, and aquifer formed beneath the surface of the crater.

Chaotic Terrain and Aqueous Environment

Following the deposition of sedimentary layers and the formation of the subsurface aquifer, a catastrophic geologic event occurred which caused the release of the subsurface aquifer and the subsequent catastrophic flooding, creating chaotic terrain within Aram Chaos. The repetition of this process led to layered terrains within Aram Chaos, including layers of the mineral hematite.^[1]^[2]^[3] Several minerals in Aram Chaos, including the hematite sulfate minerals and water-altered silicates, suggest that a lake probably once existed within the crater at some point in time.^[4]^[5] Scientists also suggest that flood channels within Aram Chaos were carved within just weeks or months by catastrophic outflows of groundwater from beneath Aram Chaos and nearby regions.^[6] Because forming hematite requires liquid water, which cannot exist without a thick atmosphere, the presence of hematite also suggests that Mars had a much thicker atmosphere at some time in the past. Tilting and erosion of Aram Chaos is also evident in satellite imagery taken of the crater.

Possible Volcanic Constructs

There is a possible volcanic component to the formation of outflow channels in Aram Chaos. By melting the permafrost or ground ice originally in the crater, geothermal activity may have caused the creation of the visible outflow channels in the impact crater.^[7] High resolution MOC images of the chaotic terrains in Aram Chaos show possible volcanic features within the crater, including hills resembling volcanoes, possible magmatic intrusions within the older rock layers, and possible volcanic ash deposits on the crater floor.

Mineralogical Composition

Not including dust and regolith common on the surface of Mars, two distinct sections of identifiable minerals have been determined to exist within Aram Chaos: a mixture of hematite and/or goethite and a mixture of ferric oxides and sulfates.^[8] Specifically, these minerals can be seen as two layers in Aram Chaos, described from top to bottom. The first layer consists mostly of nanophase iron oxides, which is about 250-500 meters thick, while the second layer is made up of a less than 500 m layer of polyhydrated sulfate and hematite. ^[9]^[10]

References

^ "The thermal infrared spectral characteristics of hematite and its origin in Aram Chaos, Mars - ProQuest". search.proquest.com. Retrieved 2021-05-08.
^ "Document unavailable - ProQuest". search.proquest.com. Retrieved 2021-05-08.
^ Glotch, Timothy D.; Christensen, Philip R. (2005). "Geologic and mineralogic mapping of Aram Chaos: Evidence for a water-rich history". Journal of Geophysical Research: Planets. 110 (E9). doi:10.1029/2004JE002389. ISSN 2156-2202.
^ Lichtenberg, K. A.; Arvidson, R. E.; Morris, R. V.; Murchie, S. L.; Bishop, J. L.; Glotch, T. D.; Noe Dobrea, E. Z.; Mustard, J. F.; Andrews-Hanna, J.; Roach, L. H.; CRISM Team (2009-03-01). "Stratigraphy and Relationship of Hydrated Minerals in the Layered Deposits of Aram Chaos, Mars". 40: 2326. {{cite journal}}: Cite journal requires |journal= (help)
^ Lichtenberg, Kimberly A.; Arvidson, Raymond E.; Morris, Richard V.; Murchie, Scott L.; Bishop, Janice L.; Remolar, David Fernandez; Glotch, Timothy D.; Dobrea, Eldar Noe; Mustard, John F.; Andrews‐Hanna, Jeffrey; Roach, Leah H. (2010). "Stratigraphy of hydrated sulfates in the sedimentary deposits of Aram Chaos, Mars". Journal of Geophysical Research: Planets. 115 (E6). doi:10.1029/2009JE003353. ISSN 2156-2202.
^ "HiRISE | Uplifted Blocks of Light-Toned Layered Deposits (ESP_054753_1825)". www.uahirise.org. Retrieved 2021-05-08.
^ Lanz, J. K.; Jaumann, R. (2001-03-01). "Possible Volcanic Constructs in Aram Chaos Revealed by MOC and Their Impact on Outflow Channel Genesis". 32. {{cite journal}}: Cite journal requires |journal= (help)
^ "Spectral Identification and Analyses of Hydrous Mineral Deposits: Implications for the Aqueous History of Aram Chaos and Melas Chasma, Mars - ProQuest". search.proquest.com. Retrieved 2021-05-08.
^ Lichtenberg, K.; Arvidson, R.; Bishop, J.; Glotch, T.; Noe Dobrea, E.; Murchie, S.; Mustard, J.; Roach, L.; CRISM Team (2008-12-01). "Mg- and Fe-Sulfate Layers in Aram Chaos, Mars". AGU Fall Meeting Abstracts. 44: P44A–09.
^ Massé, M.; Mouélic, S. Le; Bourgeois, O.; Combe, J.-P.; Deit, L. Le; Sotin, C.; Bibring, J.-P.; Gondet, B.; Langevin, Y. (2008). "Mineralogical composition, structure, morphology, and geological history of Aram Chaos crater fill on Mars derived from OMEGA Mars Express data". Journal of Geophysical Research: Planets. 113 (E12). doi:10.1029/2008JE003131. ISSN 2156-2202.

External Links

Gallery

Erosion in Aram Chaos, as seen by THEMIS
Badlands in Aram Chaos
Viking 1 Orbiter image
Eastern Floor of Aram Chaos
Minerals that form in water have been detected in the cliffs of the Aram Chaos region of Mars, as pictured.
Sediments in Aram Chaos
Gully landforms in Aram Chaos
Aram Chaos in perspective view
Aram Chaos in false color
Aram Chaos in black and white
Aram Chaos in true color
Aram Chaos, as seen by HiRISE
Hanging valleys in Aram Chaos, as seen by HiRISE under HiWish program
Blocks in Aram showing possible source of water, as seen by THEMIS.
Quadrangle map of Oxia Palus labeled with major features. Aram Chaos is near the bottom of the image.
Tography map of Oxia Palus region of Mars showing the location of a number of chaos regions, including Aram Chaos.

[1] "The thermal infrared spectral characteristics of hematite and its origin in Aram Chaos, Mars - ProQuest". search.proquest.com. Retrieved 2021-05-08.

[2] "Document unavailable - ProQuest". search.proquest.com. Retrieved 2021-05-08.

[3] Glotch, Timothy D.; Christensen, Philip R. (2005). "Geologic and mineralogic mapping of Aram Chaos: Evidence for a water-rich history". Journal of Geophysical Research: Planets. 110 (E9). doi:10.1029/2004JE002389. ISSN 2156-2202.

[4] Lichtenberg, K. A.; Arvidson, R. E.; Morris, R. V.; Murchie, S. L.; Bishop, J. L.; Glotch, T. D.; Noe Dobrea, E. Z.; Mustard, J. F.; Andrews-Hanna, J.; Roach, L. H.; CRISM Team (2009-03-01). "Stratigraphy and Relationship of Hydrated Minerals in the Layered Deposits of Aram Chaos, Mars". 40: 2326. {{cite journal}}: Cite journal requires |journal= (help)

[5] Lichtenberg, Kimberly A.; Arvidson, Raymond E.; Morris, Richard V.; Murchie, Scott L.; Bishop, Janice L.; Remolar, David Fernandez; Glotch, Timothy D.; Dobrea, Eldar Noe; Mustard, John F.; Andrews‐Hanna, Jeffrey; Roach, Leah H. (2010). "Stratigraphy of hydrated sulfates in the sedimentary deposits of Aram Chaos, Mars". Journal of Geophysical Research: Planets. 115 (E6). doi:10.1029/2009JE003353. ISSN 2156-2202.

[6] "HiRISE | Uplifted Blocks of Light-Toned Layered Deposits (ESP_054753_1825)". www.uahirise.org. Retrieved 2021-05-08.

[7] Lanz, J. K.; Jaumann, R. (2001-03-01). "Possible Volcanic Constructs in Aram Chaos Revealed by MOC and Their Impact on Outflow Channel Genesis". 32. {{cite journal}}: Cite journal requires |journal= (help)

[8] "Spectral Identification and Analyses of Hydrous Mineral Deposits: Implications for the Aqueous History of Aram Chaos and Melas Chasma, Mars - ProQuest". search.proquest.com. Retrieved 2021-05-08.

[9] Lichtenberg, K.; Arvidson, R.; Bishop, J.; Glotch, T.; Noe Dobrea, E.; Murchie, S.; Mustard, J.; Roach, L.; CRISM Team (2008-12-01). "Mg- and Fe-Sulfate Layers in Aram Chaos, Mars". AGU Fall Meeting Abstracts. 44: P44A–09.

[10] Massé, M.; Mouélic, S. Le; Bourgeois, O.; Combe, J.-P.; Deit, L. Le; Sotin, C.; Bibring, J.-P.; Gondet, B.; Langevin, Y. (2008). "Mineralogical composition, structure, morphology, and geological history of Aram Chaos crater fill on Mars derived from OMEGA Mars Express data". Journal of Geophysical Research: Planets. 113 (E12). doi:10.1029/2008JE003131. ISSN 2156-2202.

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