Argyre
Colorized topographic map of Argyre basin and its surroundings, from the MOLA instrument of Mars Global Surveyor.
PlanetMars
Coordinates49°42′S 316°00′E / 49.7°S 316.0°E / -49.7; 316.0
QuadrangleArgyre
Diameter1,700 km (1,100 mi)[1]
Depth5.2 km (17,000 ft)
EponymLegendary island Argyre

Argyre Planitia[2] /ˈɑːrdʒəriː/ is a plain located within the impact basin Argyre[a] in the southern highlands of Mars. Its name comes from a map produced by Giovanni Schiaparelli in 1877; it refers to Argyre, a mythical island of silver in Greek mythology.

Argyre is centered at 49°42′S 316°00′E / 49.7°S 316.0°E / -49.7; 316.0 and lies between 35° and 61° S and 27° and 62° W in the Argyre quadrangle. The basin is approximately 1,700 km (1,100 mi) wide[1] and drops 5.2 km (17,000 ft) below the surrounding plains; it is the second-deepest impact basin on Mars after Hellas. The crater Galle, located on the east rim of Argyre at 51°S 31°W / 51°S 31°W / -51; -31, strongly resembles a smiley face.

The basin was formed by a giant impact during the Late Heavy Bombardment of the early Solar System, approximately 3.9 billion years ago, and may be one of the best preserved ancient impact basins from that period. Argyre is surrounded by rugged massifs which form concentric and radial patterns around the basin. Several mountain ranges are present, some of these mountain ranges include Charitum and Nereidum Montes.[4]

Past water flows

Four large Noachian epoch channels lie radial to the basin. Three of these channels (Surius Vallis, Dzígai Vallis, and Pallacopas Vallis) flowed into Argyre from the south and east through the rim mountains. The fourth, Uzboi Vallis, appears to have flowed out from the basin's north rim to the Chryse region and may have drained a lake of melting ice within the basin. A smaller outflow channel named Nia Valles is relatively fresh-looking, and probably formed during the early Amazonian after the major fluvial and lacustrine episodes had finished.[5]

The original basin floor is buried with friable, partially deflated layered material that may be lake sediment. No inner rings are visible; however, isolated massifs within the basin may be remnants of an inner ring.[4]

Past habitability

After the formation of the impact basin, heat from the impact event along with geothermal heating may have allowed for liquid water to persist for many millions of years. The lake's volume could have been equal to that of Earth's Mediterranean Sea. The basin would have supported a regional environment favorable for the origin and the persistence of life.[6] This region shows a great deal of evidence of glacial activity with flow features, crevasse-like fractures, drumlins, eskers, tarns, arêtes, cirques, horns, U-shaped valleys, and terraces. Because of the shapes of Argyre sinuous ridges, the authors agree with previous publications in which they are eskers.[7]

Based on morphometrical and geomorphological analysis of the Argyre eskers and their immediate surroundings, it was suggested that they formed beneath an approximately 2 km thick, stagnant (i.e., stationary) ice sheet around 3.6 billion years ago. This stagnant body of ice might have resembled a Piedmont-style glacier comparable to today's Malaspina Glacier in Alaska.[8]

Gallery

Interactive Mars map

Map of MarsAcheron FossaeAcidalia PlanitiaAlba MonsAmazonis PlanitiaAonia PlanitiaArabia TerraArcadia PlanitiaArgentea PlanumArgyre PlanitiaChryse PlanitiaClaritas FossaeCydonia MensaeDaedalia PlanumElysium MonsElysium PlanitiaGale craterHadriaca PateraHellas MontesHellas PlanitiaHesperia PlanumHolden craterIcaria PlanumIsidis PlanitiaJezero craterLomonosov craterLucus PlanumLycus SulciLyot craterLunae PlanumMalea PlanumMaraldi craterMareotis FossaeMareotis TempeMargaritifer TerraMie craterMilankovič craterNepenthes MensaeNereidum MontesNilosyrtis MensaeNoachis TerraOlympica FossaeOlympus MonsPlanum AustralePromethei TerraProtonilus MensaeSirenumSisyphi PlanumSolis PlanumSyria PlanumTantalus FossaeTempe TerraTerra CimmeriaTerra SabaeaTerra SirenumTharsis MontesTractus CatenaTyrrhena TerraUlysses PateraUranius PateraUtopia PlanitiaValles MarinerisVastitas BorealisXanthe Terra
The image above contains clickable linksInteractive image map of the global topography of Mars. Hover your mouse over the image to see the names of over 60 prominent geographic features, and click to link to them. Coloring of the base map indicates relative elevations, based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor. Whites and browns indicate the highest elevations (+12 to +8 km); followed by pinks and reds (+8 to +3 km); yellow is 0 km; greens and blues are lower elevations (down to −8 km). Axes are latitude and longitude; Polar regions are noted.
(See also: Mars Rovers map and Mars Memorial map) (view • discuss)


See also

Notes

  1. ^ Officially, Argyre is an albedo feature.[3]

References

  1. ^ a b Hiesinger, Harald; Head, James W., III (August 2002). "Topography and morphology of the Argyre Basin, Mars: implications for its geologic and hydrologic history". Planetary and Space Science. 50 (10–11): 939–981. Bibcode:2002P&SS...50..939H. doi:10.1016/S0032-0633(02)00054-5.((cite journal)): CS1 maint: multiple names: authors list (link)
  2. ^ "Argyre Planitia". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Retrieved 2013-11-29.
  3. ^ "Argyre". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Retrieved 2013-11-29.
  4. ^ a b 'Topography and morphology of the Argyre Basin, Mars Archived 2021-02-04 at the Wayback Machine.' Hiesinger & Head.
  5. ^ Argyre Planitia and the Mars Global Hydrologic Cycle'. Parker et al.
  6. ^ Fairén Alberto G.; Dohm James M.; Rodríguez J. Alexis P.; Uceda Esther R.; Kargel Jeffrey; Soare Richard; Cleaves H. James; Oehler Dorothy; Schulze-Makuch Dirk; Essefi Elhoucine; Banks Maria E.; Komatsu Goro; Fink Wolfgang; Robbins Stuart; Yan Jianguo; Miyamoto Hideaki; Maruyama Shigenori & Baker Victor R. (February 2016). "The Argyre Region as a Prime Target for in situ Astrobiological Exploration of Mars" (PDF). Astrobiology. 16 (2): 143–158. Bibcode:2016AsBio..16..143F. doi:10.1089/ast.2015.1396. PMID 26836592. Retrieved 2016-03-12.
  7. ^ Dohm, J.; Hare, T.; Robbins, S.; Williams, J.-P.; Soare, R.; El-Maarry, M.; Conway, S.; Buczkowski, D.; Kargel, J.; Banks, M.; Fairén, A.; Schulze-Makuch, D.; Komatsu, G.; Miyamoto, H.; Anderson, R.; Davila, A.; Mahaney, W.; Fink, W.; Cleaves, H.; Yan, J.; Hynek, B.; Maruyama, S. (2015). "Geological and hydrological histories of the Argyre province, Mars" (PDF). Icarus. 253: 66–98. Bibcode:2015Icar..253...66D. doi:10.1016/j.icarus.2015.02.017.
  8. ^ Bernhardt, H.; Hiesinger, H.; Reiss, D.; Ivanov, M. A.; Erkeling, G. (2013). "Putative eskers and new insights into glacio-fluvial depositional settings in southern Argyre Planitia, Mars". Planetary and Space Science Conference. 85: 261–278. Bibcode:2013P&SS...85..261B. doi:10.1016/j.pss.2013.06.022.

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