Mare Australe quadrangle
| Mare Australe quadrangle | |
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Map of Mare Australe quadrangle from Mars Orbiter Laser Altimeter (MOLA) data. The highest elevations are red and the lowest are blue. |
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| Coordinates | 75°S 0°W / 75°S -0°ECoordinates: 75°S 0°W / 75°S -0°E |
The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30).[1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap, and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe, a large plain surrounding the polar cap.[2]
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Notable features[edit]
Around the southern ice cap is a surface, called the Dorsa Argentea Formation that may be an old ice-rich deposit. It contains a group of sinuous, branched ridges that resembles eskers that form when streams are under glaciers. [3] The formation often contains pits: two major locations are named Cavi Angusti and Cavi Sisyphi. The pits have steep sides and an irregular shape. They are up to 50 km across and 1 km deep.[4]
The quadrangle also contains Angustus Labyrinthus, a formation of intersecting valley or ridges, nicknamed the "Inca City".[5] Researchers were surprised to see parts of the surface having a swiss-cheese appearance. Also, some areas showed strange spider-shaped forms, which were determined to be caused by carbon dioxide gas blowing dust around at certain times of the year.
Gallery[edit]
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Changes in South Pole surface from 1999 to 2001, as seen by Mars Global Surveyor.
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This HiRISE image shows layers running roughly up and down, along with faint polygonal fracturing. Polygonal fractures are mostly rectangular.
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South Pole layers, as seen by THEMIS.
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Close-up of Layers in wall of McMurdo Crater, as seen by HiRISE.
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Hutton Crater Area, as seen by HiRISE. Click on image to see patterned ground.
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Angustus Labyrinthus, as seen by THEMIS.
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Philips Crater Area, as seen by HiRISE.
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Pityusa Patera, as seen by HiRISE.
See also[edit]
- Climate of Mars
- Dust Devil Tracks
- Impact crater
- List of quadrangles on Mars
- Martian polar ice caps
- Swiss cheese features
- Water on Mars
References[edit]
- ^ Davies, M.E.; Batson, R.M.; Wu, S.S.C. (1992). "Geodesy and Cartography". In Kieffer, H.H.; Jakosky, B.M.; Snyder, C.W. et al. Mars. Tucson: University of Arizona Press. ISBN 978-0-8165-1257-7.
- ^ Patrick Moore and Robin Rees, ed. Patrick Moore's Data Book of Astronomy (Cambridge University Press, 2011), p. 130.
- ^ Kargel, J.; Strom, R. (1991). "Terrestrial glacial eskers: analogs for martian sinuous ridges" (PDF). LPSC XXII: 683–684. Bibcode:1991LPI....22..683K.
- ^ Carr, Michael H. (2006). The Surface of Mars. Cambridge University Press. p. [page needed]. ISBN 978-0-521-87201-0.
- ^ Hartmann, W. 2003. A Traveler's Guide to Mars. Workman Publishing. NY NY.
Mare Australe
| Quadrangles on Mars | |||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| MC-01 Mare Boreum (features) |
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| MC-05 Ismenius Lacus (features) |
MC-06 Casius (features) |
MC-07 Cebrenia (features) |
MC-02 Diacria (features) |
MC-03 Arcadia (features) |
MC-04 Acidalium (features) |
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| MC-12 Arabia (features) |
MC-13 Syrtis Major (features) |
MC-14 Amenthes (features) |
MC-15 Elysium (features) |
MC-08 Amazonis (features) |
MC-09 Tharsis (features) |
MC-10 Lunae Palus (features) |
MC-11 Oxia Palus (features) |
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| MC-20 Sinus Sabaeus (features) |
MC-21 Iapygia (features) |
MC-22 Mare Tyrrhenum (features) |
MC-23 Aeolis (features) |
MC-16 Memnonia (features) |
MC-17 Phoenicis Lacus (features) |
MC-18 Coprates (features) |
MC-19 Margaritifer Sinus (features) |
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| MC-27 Noachis (features) |
MC-28 Hellas (features) |
MC-29 Eridania (features) |
MC-24 Phaethontis (features) |
MC-25 Thaumasia (features) |
MC-26 Argyre (features) |
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| MC-30 Mare Australe (features) |
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