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′N21°30′W / 2.6°N 21.5°W / 2.6; -21.5. The Thermal Emission Imaging System (THEMIS) on the orbiterMars 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.
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 This formed the large, circular depression that originally made up the crater.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.
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.
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.
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]
^Glotch, Timothy D. (2004). The thermal infrared spectral characteristics of hematite and its origin in Aram Chaos, Mars (Thesis). OCLC63279533. ProQuest305210528.
^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. (March 2009). Stratigraphy and Relationship of Hydrated Minerals in the Layered Deposits of Aram Chaos, Mars. 40th Lunar and Planetary Science Conference. p. 2326. Bibcode:2009LPI....40.2326L.
^Lanz, J. K.; Jaumann, R. (March 2001). Possible Volcanic Constructs in Aram Chaos Revealed by MOC and Their Impact on Outflow Channel Genesis. 32nd Annual Lunar and Planetary Science Conference. p. 1574. Bibcode:2001LPI....32.1574L.
^Liu, Yang (2013). Spectral Identification and Analyses of Hydrous Mineral Deposits: Implications for the Aqueous History of Aram Chaos and Melas Chasma, Mars (Thesis). OCLC861698923. ProQuest1426182378.
^Lichtenberg, K.; Arvidson, R.; Bishop, J.; Glotch, T.; Noe Dobrea, E.; Murchie, S.; Mustard, J.; Roach, L. (December 2008). Mg- and Fe-Sulfate Layers in Aram Chaos, Mars. American Geophysical Union, Fall Meeting 2008. pp. P44A–09. Bibcode:2008AGUFM.P44A..09L.
