Knowledge (XXG)

Deuteronilus Mensae

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dust to be held in the atmosphere. Moisture in the atmosphere will fall as snow or as ice frozen onto dust grains. Calculations suggest this material will concentrate in the mid-latitudes. General circulation models of the Martian atmosphere predict accumulations of ice-rich dust in the same areas where ice-rich features are found. When the tilt begins to return to lower values, the ice sublimates (turns directly to a gas) and leaves behind a lag of dust. The lag deposit caps the underlying material so with each cycle of high tilt levels, some ice-rich mantle remains behind. Note, that the smooth surface mantle layer probably represents only relative recent material.
350: 435: 313: 224: 236: 362: 295: 338: 521: 212: 196: 561: 274: 463: 549: 533: 475: 613: 601: 248: 423:. The layering of the upper plains mantling unit and other mantling units are believed to be caused by major changes in the planet's climate. Models predict that the obliquity or tilt of the rotational axis has varied from its present 25 degrees to maybe over 80 degrees over geological time. Periods of high tilt will cause the ice in the polar caps to be redistributed and change the amount of dust in the atmosphere. 29: 4729: 267:, has been discovered in the mid-latitudes of Mars. First investigated in the Deuteronilus Mensae region, but it occurs in other places as well. The remnants consist of sets of dipping layers in craters and along mesas. Sets of dipping layers may be of various sizes and shapes—some look like Aztec pyramids from Central America. 391: 324: 488: 123:. It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of 576: 376:
of ice in the ground. Large areas of the Martian surface are loaded with ice that is protected by a meters thick layer of dust and other material. However, if cracks appear, a fresh surface will expose ice to the thin atmosphere. In a short time, the ice will disappear into the cold, thin atmosphere
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Hauber, E., D. Reiss, M. Ulrich, F. Preusker, F. Trauthan, M. Zanetti, H. Hiesinger, R. Jaumann, L. Johansson, A. Johnsson, S. Van Gaselt, M. Olvmo. 2011. Landscape evolution in Martian mid-latitude regions: insights from analogous periglacial landforms in Svalbard. In: Balme, M., A. Bargery, C.
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Some regions of the upper plains unit display large fractures and troughs with raised rims; such regions are called ribbed upper plains. Fractures are believed to have started with small cracks from stresses. Stress is suggested to initiate the fracture process since ribbed upper plains are common
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It is now widely believed that ice accumulated in many areas of Mars, including Deuteronilus Mensae, when the planet's orbital tilt was very different from now (the axis of Mars has considerable "wobble", meaning its angle changes over time). A few million years ago, the tilt of the axis of Mars was
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The upper plains unit is thought to have fallen from the sky. It drapes various surfaces, as if it fell evenly. As is the case for other mantle deposits, the upper plains unit has layers, is fine-grained, and is ice-rich. It is widespread; it does not seem to have a point source. The surface
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Studies have shown that when the tilt of Mars reaches 45 degrees from its current 25 degrees, ice is no longer stable at the poles. Furthermore, at this high tilt, stores of solid carbon dioxide (dry ice) sublimate, thereby increasing the atmospheric pressure. This increased pressure allows more
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when debris aprons come together or near the edge of debris aprons—such sites would generate compressional stresses. Cracks exposed more surfaces, and consequently more ice in the material sublimates into the planet's thin atmosphere. Eventually, small cracks become large canyons or troughs.
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Many features on Mars, including Deuteronilus Mensae, are believed to contain large amounts of ice. The most popular model for the origin of the ice is climate change from large changes in the tilt of the planet's rotational axis. At times the tilt has even been greater than 80 degrees Large
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Levy, J., J. Head, D. Marchant, D. Kowalewski. 2008. Identification of sublimation-type thermal contraction crack polygons at the proposed NASA Phoenix landing site: Implications for substrate properties and climate-driven morphological evolution. Geophys. Res. Lett. 35.
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Dipping layers, as seen by HiRISE under HiWish program Also, Ribbed Upper plains material is visible in the upper right of the picture. It is forming from the upper plains unit, and in turn is being eroded into brain
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Levy, J., J. Head, D. Marchant. 2009a. Thermal contraction crack polygons on Mars: Classification, distribution, and climate implications from HiRISE observations. J. Geophys. Res. 114. doi:10.1029/2008JE003273.
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Kostama, V.-P., M. Kreslavsky, Head, J. 2006. Recent high-latitude icy mantle in the northern plains of Mars: Characteristics and ages of emplacement. Geophys. Res. Lett. 33 (L11201). doi:10.1029/2006GL025946.
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Plaut, J., A. Safaeinili,, J. Holt, R. Phillips, J. Head, J., R. Seu, N. Putzig, A. Frigeri. 2009. Radar evidence for ice in lobate debris aprons in the midnorthern latitudes of Mars. Geophys. Res. Lett. 36.
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Madeleine, J., F. Forget, J. Head, B. Levrard, F. Montmessin. 2007. Exploring the northern mid-latitude glaciation with a general circulation model. In: Seventh International Conference on Mars. Abstract
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Baker, M. et al. 2010. Flow patterns of lobate debris aprons and lineated valley fill north of Ismeniae Fossae, Mars: Evidence for extensive mid-latitude glaciation in the Late Amazonian. Icarus: 207.
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Baker, D., J. Head. 2015. Extensive Middle Amazonian mantling of debris aprons and plains in Deuteronilus Mensae, Mars: Implication for the record of mid-latitude glaciation. Icarus: 260, 269–288.
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Milliken, R., et al. 2003. Viscous flow features on the surface of Mars: Observations from high-resolution Mars Orbiter Camera (MOC) images. J. Geophys. Res. 108 (E6). doi:10.1029/2002JE002005.
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45 degrees instead of its present 25 degrees. Its tilt, also called obliquity, varies greatly because its two tiny moons cannot stabilize it, like our relatively large moon does the Earth.
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Well developed ribbed upper plains material. These start with small cracks that expand as ice sublimates from the surfaces of the crack. Picture was taken with HiRISE under HiWish program
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Laskar, J., A. Correia, M. Gastineau, F. Joutel, B. Levrard, and P. Robutel. 2004. Long term evolution and chaotic diffusion of the insolation quantities of Mars. Icarus 170, 343–364.
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Mischna, M. et al. 2003. On the orbital forcing of martian water and CO2 cycles: A general circulation model study with simplified volatile schemes. J. Geophys. Res. 108. (E6). 5062.
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Possible moraine on the end of a past glacier on a mound in Deuteronilus Mensae, as seen by HiRISE, under the HiWish program. Location of this image is the box labeled A in previous image.
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Evolution of ribbed terrain from stress cracks—cracks to the left eventually will enlarge and become ribbed terrain toward the right side of picture, as seen by HiRISE under HiWish program
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Layered feature in Red Rocks Park, Colorado. This has a different origin than ones on Mars, but it has a similar shape. Features in Red Rocks region were caused by uplift of mountains.
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Mangold, N. 2003. Geomorphic analysis of lobate debris aprons on Mars at Mars Orbiter Camera scale: Evidence for ice sublimation initiated by fractures. J. Geophys. Res. 108, 8021.
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uncovered chunks of ice that disappeared in a few days. In addition, HiRISE has seen fresh craters with ice at the bottom. After a time, HiRISE saw the ice deposit disappear.
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Schon, et al. 2009. A recent ice age on Mars: Evidence for climate oscillations from regional layering in mid-latitude mantling deposits. Geophys. Res. Lett. 36, L15202.
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Complex surface around mound in Deuteronilus Mensae, as seen by HiRISE, under the HiWish program. Location of this image is in the black box labeled B in the CTX image above.
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on the Earth. Places on Mars that display polygonal ground may indicate where future colonists can find water ice. Patterned ground forms in a mantle layer, called
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Die-sized clumps of bright material in the enlarged "Dodo-Goldilocks" trench vanished over the course of four days, implying that they were composed of ice which
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Malin, M., Edgett, K. 2001. Mars Global Surveyor Mars Orbiter Camera: Interplanetary cruise through primary mission. J. Geophys. Res. 106 (E10), 23429–23540.
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persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. Recent evidence from the
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Mustard, J., et al. 2001. Evidence for recent climate change on Mars from the identification of youthful near-surface ground ice. Nature 412 (6845), 411–414.
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Kreslavsky, M.A., Head, J.W., 2002. High-latitude Recent Surface Mantle on Mars: New Results from MOLA and MOC. European Geophysical Society XXVII, Nice.
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View of stress cracks and larger cracks that have been enlarged by sublimation (ice changing directly into gas) This may be the start of ribbed terrain.
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Color versions of the photos showing ice sublimation, with the lower left corner of the trench enlarged in the insets in the upper right of the images.
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Mellon, M., B. Jakosky. 1995. The distribution and behavior of Martian ground ice during past and present epochs. J. Geophys. Res. 100, 11781–11799.
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Seibert, N., J. Kargel. 2001. Small-scale martian polygonal terrain: Implications for liquid surface water. Geophys. Res. Lett. 28 (5), 899–902. S
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Close up of field of high center polygons with scale, as seen by HiRISE under HiWish program Note: the black box is the size of a football field.
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Kreslavsky, M., Head, J. 2000. Kilometer-scale roughness on Mars: Results from MOLA data analysis. J. Geophys. Res. 105 (E11), 26695–26712.
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Madeleine, J. et al. 2007. Mars: A proposed climatic scenario for northern mid-latitude glaciation. Lunar Planet. Sci. 38. Abstract 1778.
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Head, J.W., Mustard, J.F., Kreslavsky, M.A., Milliken, R.E., Marchant, D.R., 2003. Recent ice ages on Mars. Nature 426 (6968), 797–802.
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Madeleine, J. et al. 2009. Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario. Icarus: 203. 300–405.
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Mangold, N. 2005. High latitude patterned grounds on Mars: Classification, distribution and climatic control. Icarus 174, 336–359.
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Layered features and brain terrain, as seen by HiRISE under HiWish program The upper plains unit often changes into brain terrain.
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Close-up of high center polygons seen by HiRISE under HiWish program Troughs between polygons are easily visible in this view.
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appearance of some regions of Mars is due to how this unit has degraded. It is a major cause of the surface appearance of
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Enlargement of the photo on the left showing cliff. Photo taken with high resolution camera of Mars Global Surveyor (MGS).
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is quite common in some regions of Mars. It is commonly believed to be caused by the sublimation of ice from the ground.
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Close-up of high center polygons seen by HiRISE under HiWish program Note: the black box is the size of a football field.
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Gallagher, S. Guta (eds). Martian Geomorphology. Geological Society, London. Special Publications: 356. 111–131
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Carr, M. 2001. Mars Global Surveyor observations of martian fretted terrain. J. Geophys. Res. 106, 23571-23593.
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Map showing the relation of Protonilus and Deuteronilus Mensae to other nearby regions. Colors refer to altitudes.
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Byrne, S. et al. 2009. Distribution of Mid-Latitude Ground Ice on Mars from New Impact Craters: 329.1674–1676
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Another view of eroded terrain in Deuteronilus Mensae, as seen by HiRISE, under the HiWish program.
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showing flat floored valleys and cliffs. Photo taken with Mars Orbiter Camera (MOC)on the
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Touma J. and J. Wisdom. 1993. The Chaotic Obliquity of Mars. Science 259, 1294–1297.
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Small cracks often contain small pits and chains of pits; these are thought to be from
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Hollowed out terrain in Deuteronilus Mensae, as seen by HiRISE under HiWish program.
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Jeffrey Plaut – Subsurface Ice – 21st Annual International Mars Society Convention
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Small valleys in the wall of a crater in Deuteronilus Mensae, as seen by THEMIS.
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Deuteronilus Mensae ridges that suggest movement of deposits, as seen by THEMIS.
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is the direct change of solid ice to a gas. This is similar to what happens to
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CTX Context image of Deuteronilus Mensae showing location of next two images.
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Group of small sets of dipping layers, as seen by HiRISE under HiWish program
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Large group of concentric cracks, as seen by HiRISE, under HiWish program.
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CTX context image showing location of next two HiRISE images. Location is
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Schorghofer, N., 2007. Dynamics of ice ages on Mars. Nature 449, 192–194.
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Hecht, M. 2002. Metastability of water on Mars. Icarus 156, 373–386
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Eroded terrain in Deuteronilus Mensae, as seen by HiRISE, under the
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has shown that parts of Deuteronilus Mensae do indeed contain ice.
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Image is of the top of a debris apron in Deuteronilus Mensae.
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changes in the tilt explains many ice-rich features on Mars.
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http://news.discovery.com/space/mars-ice-sheet-climate.html
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high center polygons seen by HiRISE under HiWish program
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Remnants of a 50–100 meter thick mantling, called the
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Concentric 679:Patrick Moore; Garry Hunt (1997). 14: 2002:Martian meteorites found on Earth 730:Rincon, Paul (19 December 2007). 4727: 732:"'Active glacier found' on Mars" 611: 599: 587: 575: 559: 547: 531: 519: 507: 487: 473: 461: 445: 433: 406: 390: 360: 348: 336: 323: 311: 293: 272: 246: 234: 222: 210: 194: 379:sublimation (phase transition) 374:sublimation (phase transition) 1: 1146:Scarps in Deuteronilus Mensae 1005:Morgenstern, A., et al. 2007 682:The atlas of the solar system 284:This unit also degrades into 175:Polygonal, patterned ground 141:Mars Reconnaissance Orbiter 4771: 1421:Mare Australe (South Pole) 170:Polygonal patterned ground 167: 164:Polygonal patterned ground 4750:Ismenius Lacus quadrangle 3484:Eagle (Acidalia Planitia) 2061: 2050: 1784:Classical albedo features 1510: 1497: 1216: 1205: 832:doi:10.1029/2007GL032813. 774:doi:10.1029/2008GL036379. 645:Ismenius Lacus quadrangle 568:Ismenius Lacus quadrangle 496:Ismenius Lacus quadrangle 187:latitude dependent mantle 121:Ismenius Lacus quadrangle 26: 3489:Eagle (Meridiani Planum) 1963:Meteorites found on Mars 1426:Mare Boreum (North Pole) 1114:Madeleine, et al. 2014. 119:and is included in the 1551:Concentric crater fill 1105:Head, J. et al. 2003. 1694:Swiss cheese features 3121:Angustus Labyrinthus 1724:discovery chronology 1669:Scalloped topography 1623:Lineated valley fill 1054:4 March 2016 at the 500:Mars Global Surveyor 454:Mars Global Surveyor 421:lobate debris aprons 377:in a process called 3076:Deuteronilus Mensae 2404:Syrtis Major Planum 2220:Syrtis Major Planum 1769:Observation history 1629:Lobate debris apron 890:"Refubium - Search" 401:following exposure. 99: /  78:Deuteronilus Mensae 56: /  23: 4502:Teisserenc de Bort 3126:Noctis Labyrinthus 3106:Nilokeras Scopulus 1436:Margaritifer Sinus 22:Deuteronius Mensae 4715: 4714: 4711: 4710: 4707: 4706: 3154:Tithoniae Catenae 3091:Protonilus Mensae 3086:Nilosyrtis Mensae 2976:Hephaestus Fossae 2349:Eridania Planitia 2319:Amazonis Planitia 2309:Acidalia Planitia 2046: 2045: 2042: 2041: 2007:Balsaltic Breccia 1709:Upper plains unit 1699:Terrain softening 1659:Ring mold craters 1634:North Polar Basin 1556:Dark slope streak 1493: 1492: 1489: 1488: 1318:Vastitas Borealis 1258:Hyperboreae Undae 1045:Bright Chunks at 692:978-0-7537-0014-3 660:Protonilus Mensae 655:Nilosyrtis Mensae 650:Martian dichotomy 265:upper plains unit 259:Upper plains unit 125:Protonilus Mensae 75: 74: 4762: 4732: 4731: 4730: 4723: 3041:Tithonium Fossae 2951:Ceraunius Fossae 2567:Tithonium Chasma 2379:Meridiani Planum 2344:Elysium Planitia 2324:Arcadia Planitia 2282:Ceraunius Tholus 2103:Apollinaris Mons 2063: 2052: 1983:Meridiani Planum 1649:Outflow channels 1639:Ocean hypothesis 1512: 1499: 1218: 1207: 1184: 1177: 1170: 1161: 1124: 1121: 1115: 1112: 1106: 1103: 1097: 1094: 1088: 1087: 1085: 1083: 1074:. Archived from 1068: 1059: 1042: 1036: 1033: 1027: 1024: 1018: 1015: 1006: 1003: 997: 994: 988: 985: 979: 976: 970: 967: 961: 958: 952: 949: 943: 940: 934: 931: 925: 922: 916: 913: 907: 903: 897: 896: 894: 886: 880: 876: 870: 867: 861: 858: 852: 848: 842: 839: 833: 829: 823: 820: 811: 808: 802: 799: 793: 790: 784: 781: 775: 771: 765: 760: 754: 753: 746: 740: 739: 727: 721: 720: 713: 707: 703: 697: 696: 676: 640:Glaciers on Mars 615: 603: 591: 579: 563: 551: 535: 523: 511: 491: 477: 465: 449: 437: 410: 394: 364: 352: 340: 327: 315: 297: 276: 250: 238: 226: 214: 198: 114: 113: 111: 110: 109: 104: 100: 97: 96: 95: 92: 71: 70: 68: 67: 66: 61: 57: 54: 53: 52: 49: 31: 24: 4770: 4769: 4765: 4764: 4763: 4761: 4760: 4759: 4740: 4739: 4738: 4728: 4726: 4718: 4716: 4703: 3139: 3130: 3031:Tantalus Fossae 3016:Olympica Fossae 3006:Memnonia Fossae 2996:Mareotis Fossae 2986:Labeatis Fossae 2956:Cerberus Fossae 2946:Amenthes Fossae 2932: 2919: 2552:Juventae Chasma 2532:Hydraotes Chaos 2487:Coprates Chasma 2442: 2433: 2409:Utopia Planitia 2389:Planum Australe 2369:Isidis Planitia 2359:Hesperia Planum 2354:Hellas Planitia 2339:Daedalia Planum 2334:Chryse Planitia 2329:Argyre Planitia 2300: 2293: 2230:Tartarus Montes 2225:Tartarus Colles 2205:Nereidum Montes 2138:Charitum Montes 2133:Centauri Montes 2108:Ariadnes Colles 2088:Acidalia Colles 2081: 2074: 2070: 2057: 2038: 1978:Mackinac Island 1797: 1790: 1735: 1714:Valley networks 1608:Inverted relief 1583:Fretted terrain 1517: 1506: 1485: 1461:Phoenicis Lacus 1322: 1288:Sinus Meridiani 1273:Planum Australe 1212: 1201: 1188: 1133: 1128: 1127: 1122: 1118: 1113: 1109: 1104: 1100: 1095: 1091: 1081: 1079: 1078:on 4 March 2016 1070: 1069: 1062: 1056:Wayback Machine 1043: 1039: 1034: 1030: 1025: 1021: 1016: 1009: 1004: 1000: 995: 991: 986: 982: 977: 973: 968: 964: 959: 955: 950: 946: 941: 937: 932: 928: 923: 919: 914: 910: 904: 900: 892: 888: 887: 883: 877: 873: 868: 864: 859: 855: 849: 845: 840: 836: 830: 826: 821: 814: 809: 805: 800: 796: 791: 787: 782: 778: 772: 768: 761: 757: 748: 747: 743: 729: 728: 724: 715: 714: 710: 704: 700: 693: 678: 677: 673: 668: 630:Geology of Mars 626: 619: 616: 607: 604: 595: 592: 583: 580: 571: 564: 555: 552: 543: 536: 527: 524: 515: 512: 503: 492: 481: 478: 469: 466: 457: 450: 441: 438: 429: 414: 411: 402: 395: 368: 365: 356: 353: 344: 341: 332: 328: 319: 316: 301: 298: 280: 277: 261: 254: 251: 242: 239: 230: 227: 218: 215: 206: 199: 172: 166: 149: 129:Ismeniae Fossae 107: 105: 101: 98: 93: 90: 88: 86: 85: 80:is a region on 64: 62: 58: 55: 50: 47: 45: 43: 42: 34: 17: 12: 11: 5: 4768: 4766: 4758: 4757: 4755:Mensae on Mars 4752: 4742: 4741: 4737: 4736: 4713: 4712: 4709: 4708: 4705: 4704: 4702: 4701: 4696: 4691: 4686: 4681: 4676: 4671: 4666: 4661: 4656: 4651: 4646: 4641: 4636: 4631: 4626: 4621: 4616: 4611: 4606: 4605: 4604: 4594: 4589: 4584: 4579: 4574: 4569: 4564: 4559: 4554: 4549: 4544: 4539: 4534: 4529: 4524: 4519: 4514: 4509: 4504: 4499: 4494: 4489: 4484: 4479: 4474: 4469: 4464: 4459: 4454: 4449: 4444: 4439: 4434: 4429: 4424: 4419: 4414: 4409: 4404: 4399: 4394: 4389: 4384: 4379: 4374: 4369: 4364: 4359: 4354: 4349: 4344: 4339: 4334: 4329: 4324: 4319: 4314: 4309: 4304: 4299: 4294: 4289: 4284: 4279: 4274: 4269: 4264: 4259: 4254: 4249: 4244: 4239: 4234: 4229: 4224: 4219: 4214: 4209: 4204: 4199: 4194: 4189: 4184: 4179: 4174: 4169: 4164: 4159: 4154: 4149: 4144: 4139: 4134: 4129: 4124: 4119: 4114: 4109: 4104: 4099: 4094: 4089: 4084: 4079: 4074: 4069: 4064: 4059: 4054: 4049: 4044: 4039: 4034: 4029: 4024: 4019: 4014: 4009: 4004: 3999: 3994: 3989: 3984: 3979: 3974: 3969: 3964: 3959: 3954: 3949: 3944: 3939: 3934: 3929: 3924: 3919: 3914: 3909: 3904: 3899: 3894: 3889: 3884: 3879: 3874: 3869: 3864: 3859: 3854: 3849: 3844: 3839: 3834: 3832:Jarry-Desloges 3829: 3824: 3819: 3814: 3809: 3804: 3799: 3794: 3789: 3784: 3779: 3774: 3769: 3764: 3759: 3754: 3749: 3744: 3739: 3734: 3729: 3724: 3719: 3714: 3709: 3704: 3703: 3702: 3697: 3696: 3695: 3690: 3683:Columbia Hills 3680: 3679: 3678: 3673: 3668: 3661:Apollo 1 Hills 3653: 3648: 3643: 3638: 3633: 3628: 3623: 3618: 3613: 3608: 3603: 3598: 3593: 3588: 3583: 3578: 3573: 3568: 3563: 3558: 3553: 3548: 3543: 3538: 3533: 3528: 3523: 3522: 3521: 3519:Matijevic Hill 3511: 3506: 3501: 3496: 3491: 3486: 3481: 3476: 3471: 3466: 3461: 3456: 3451: 3446: 3441: 3436: 3431: 3426: 3421: 3416: 3411: 3406: 3401: 3396: 3391: 3386: 3381: 3376: 3371: 3366: 3361: 3356: 3351: 3346: 3341: 3336: 3331: 3326: 3321: 3316: 3311: 3306: 3301: 3296: 3291: 3286: 3281: 3276: 3271: 3266: 3261: 3256: 3251: 3246: 3241: 3236: 3231: 3226: 3221: 3216: 3211: 3206: 3201: 3196: 3191: 3186: 3181: 3176: 3171: 3166: 3161: 3159:Tractus Catena 3156: 3151: 3149:Artynia Catena 3145: 3143: 3132: 3131: 3129: 3128: 3123: 3118: 3113: 3108: 3103: 3101:Claritas Rupes 3098: 3093: 3088: 3083: 3078: 3073: 3071:Cydonia Mensae 3068: 3063: 3058: 3053: 3051:Ulysses Fossae 3048: 3046:Tractus Fossae 3043: 3038: 3033: 3028: 3026:Sirenum Fossae 3023: 3018: 3013: 3008: 3003: 3001:Medusae Fossae 2998: 2993: 2988: 2983: 2978: 2973: 2971:Elysium Fossae 2968: 2963: 2958: 2953: 2948: 2942: 2940: 2921: 2920: 2918: 2917: 2916: 2915: 2910: 2905: 2900: 2899: 2898: 2888: 2883: 2878: 2873: 2868: 2863: 2858: 2853: 2848: 2843: 2838: 2833: 2828: 2823: 2818: 2813: 2808: 2803: 2798: 2793: 2788: 2783: 2778: 2773: 2768: 2763: 2758: 2753: 2752: 2751: 2741: 2736: 2731: 2726: 2721: 2716: 2711: 2706: 2701: 2696: 2691: 2686: 2681: 2676: 2671: 2666: 2661: 2656: 2651: 2646: 2641: 2636: 2631: 2626: 2621: 2616: 2611: 2606: 2601: 2596: 2591: 2586: 2581: 2574:List of valles 2570: 2569: 2564: 2559: 2554: 2549: 2544: 2539: 2534: 2529: 2527:Hydaspis Chaos 2524: 2519: 2517:Gorgonum Chaos 2514: 2509: 2507:Galaxias Chaos 2504: 2499: 2494: 2489: 2484: 2482:Chasma Boreale 2479: 2474: 2469: 2467:Atlantis Chaos 2464: 2462:Aromatum Chaos 2459: 2457:Arsia Chasmata 2454: 2448: 2446: 2435: 2434: 2432: 2431: 2429:Pityusa Patera 2426: 2421: 2416: 2411: 2406: 2401: 2396: 2391: 2386: 2381: 2376: 2371: 2366: 2361: 2356: 2351: 2346: 2341: 2336: 2331: 2326: 2321: 2316: 2311: 2305: 2303: 2295: 2294: 2292: 2291: 2290: 2289: 2287:Uranius Tholus 2284: 2279: 2269: 2267:Ulysses Tholus 2264: 2262:Tyrrhenus Mons 2259: 2257:Tharsis Tholus 2254: 2253: 2252: 2247: 2242: 2235:Tharsis Montes 2232: 2227: 2222: 2217: 2215:Phlegra Montes 2212: 2207: 2202: 2197: 2192: 2187: 2182: 2180:Hadriacus Mons 2177: 2172: 2167: 2166: 2165: 2163:Hecates Tholus 2160: 2155: 2145: 2140: 2135: 2130: 2125: 2123:Avernus Colles 2120: 2118:Ausonia Montes 2115: 2113:Astapus Colles 2110: 2105: 2100: 2095: 2090: 2084: 2082: 2078:list by height 2075: 2059: 2058: 2055: 2048: 2047: 2044: 2043: 2040: 2039: 2037: 2036: 2035: 2034: 2029: 2024: 2019: 2014: 2009: 1998: 1997: 1996: 1995: 1993:Shelter Island 1990: 1985: 1980: 1975: 1970: 1959: 1958: 1957: 1956: 1951: 1943: 1942: 1941: 1933: 1932: 1931: 1926: 1921: 1916: 1903: 1902: 1901: 1896: 1883: 1882: 1881: 1876: 1871: 1858: 1857: 1856: 1851: 1846: 1841: 1836: 1834:Jake Matijevic 1831: 1826: 1821: 1816: 1814:Bathurst Inlet 1802: 1800: 1792: 1791: 1789: 1788: 1787: 1786: 1781: 1766: 1761: 1756: 1751: 1745: 1743: 1737: 1736: 1734: 1733: 1728: 1727: 1726: 1716: 1711: 1706: 1701: 1696: 1691: 1686: 1681: 1676: 1674:Seasonal flows 1671: 1666: 1664:Rootless cones 1661: 1656: 1651: 1646: 1641: 1636: 1631: 1626: 1620: 1615: 1610: 1605: 1600: 1595: 1590: 1585: 1580: 1579: 1578: 1573: 1563: 1558: 1553: 1548: 1543: 1538: 1533: 1528: 1522: 1520: 1508: 1507: 1502: 1495: 1494: 1491: 1490: 1487: 1486: 1484: 1483: 1478: 1473: 1468: 1463: 1458: 1453: 1448: 1443: 1438: 1433: 1431:Mare Tyrrhenum 1428: 1423: 1418: 1416:Mare Acidalium 1413: 1408: 1406:Ismenius Lacus 1403: 1398: 1393: 1388: 1383: 1378: 1373: 1368: 1363: 1358: 1353: 1348: 1343: 1338: 1332: 1330: 1324: 1323: 1321: 1320: 1315: 1310: 1305: 1303:Terra Cimmeria 1300: 1295: 1290: 1285: 1280: 1275: 1270: 1265: 1260: 1255: 1250: 1245: 1240: 1235: 1233:Aspledon Undae 1230: 1224: 1222: 1214: 1213: 1210: 1203: 1202: 1189: 1187: 1186: 1179: 1172: 1164: 1158: 1157: 1152: 1143: 1132: 1131:External links 1129: 1126: 1125: 1116: 1107: 1098: 1089: 1060: 1037: 1028: 1019: 1007: 998: 989: 980: 971: 962: 953: 944: 935: 926: 917: 908: 898: 881: 871: 862: 853: 843: 834: 824: 812: 803: 794: 785: 776: 766: 755: 741: 722: 708: 698: 691: 685:. Chancellor. 670: 669: 667: 664: 663: 662: 657: 652: 647: 642: 637: 632: 625: 622: 621: 620: 617: 610: 608: 605: 598: 596: 593: 586: 584: 581: 574: 572: 565: 558: 556: 553: 546: 544: 540:HiWish program 537: 530: 528: 525: 518: 516: 513: 506: 504: 493: 486: 483: 482: 479: 472: 470: 467: 460: 458: 451: 444: 442: 439: 432: 428: 425: 416: 415: 412: 405: 403: 396: 389: 383:Phoenix lander 370: 369: 366: 359: 357: 354: 347: 345: 342: 335: 333: 329: 322: 320: 317: 310: 303: 302: 299: 292: 282: 281: 278: 271: 260: 257: 256: 255: 252: 245: 243: 240: 233: 231: 228: 221: 219: 216: 209: 207: 203:HiWish program 200: 193: 168:Main article: 165: 162: 148: 145: 103:43.9°N 337.4°W 73: 72: 60:43.9°N 337.4°W 40: 36: 35: 32: 16:Mensae on Mars 15: 13: 10: 9: 6: 4: 3: 2: 4767: 4756: 4753: 4751: 4748: 4747: 4745: 4735: 4725: 4721: 4700: 4697: 4695: 4692: 4690: 4687: 4685: 4682: 4680: 4677: 4675: 4672: 4670: 4667: 4665: 4662: 4660: 4657: 4655: 4652: 4650: 4647: 4645: 4642: 4640: 4637: 4635: 4632: 4630: 4627: 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3795: 3793: 3790: 3788: 3785: 3783: 3780: 3778: 3775: 3773: 3770: 3768: 3765: 3763: 3760: 3758: 3755: 3753: 3750: 3748: 3745: 3743: 3740: 3738: 3735: 3733: 3730: 3728: 3725: 3723: 3720: 3718: 3715: 3713: 3710: 3708: 3705: 3701: 3700:Sleepy Hollow 3698: 3694: 3691: 3689: 3686: 3685: 3684: 3681: 3677: 3674: 3672: 3669: 3667: 3664: 3663: 3662: 3659: 3658: 3657: 3654: 3652: 3649: 3647: 3644: 3642: 3639: 3637: 3634: 3632: 3629: 3627: 3624: 3622: 3619: 3617: 3614: 3612: 3609: 3607: 3604: 3602: 3599: 3597: 3594: 3592: 3589: 3587: 3584: 3582: 3579: 3577: 3574: 3572: 3569: 3567: 3564: 3562: 3559: 3557: 3554: 3552: 3549: 3547: 3544: 3542: 3539: 3537: 3534: 3532: 3529: 3527: 3524: 3520: 3517: 3516: 3515: 3512: 3510: 3507: 3505: 3502: 3500: 3497: 3495: 3492: 3490: 3487: 3485: 3482: 3480: 3477: 3475: 3472: 3470: 3467: 3465: 3462: 3460: 3457: 3455: 3452: 3450: 3447: 3445: 3442: 3440: 3437: 3435: 3432: 3430: 3427: 3425: 3422: 3420: 3417: 3415: 3412: 3410: 3407: 3405: 3402: 3400: 3397: 3395: 3392: 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2966:Cyane Fossae 2961:Coloe Fossae 2639:Green Valley 2562:Ophir Chasma 2557:Melas Chasma 2522:Hebes Chasma 2492:Echus Chasma 2472:Aureum Chaos 2419:Orcus Patera 2399:Syria Planum 2374:Lunae Planum 2314:Aeolis Palus 2277:Uranius Mons 2210:Olympus Mons 2195:Libya Montes 2190:Jovis Tholus 2158:Albor Tholus 2153:Elysium Mons 2143:Echus Montes 2098:Anseris Mons 2022:Shergottites 2012:Chassignites 1968:Block Island 1906: 1886: 1861: 1806: 1471:Syrtis Major 1308:Terra Sabaea 1263:Ogygis Undae 1238:Arabia Terra 1228:Abalos Undae 1141:Mars Express 1119: 1110: 1101: 1092: 1080:. 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4437:Sklodowska 4392:Schaeberle 4372:Rutherford 4332:Richardson 4277:Ptolemaeus 4212:Perepelkin 4127:Montevallo 4122:Molesworth 4092:Milankovic 4067:McLaughlin 4017:Magelhaens 3942:Le Verrier 3767:Hipparchus 3561:Flammarion 3494:Eberswalde 3389:Copernicus 3304:Bonneville 3284:Boeddicker 3244:Barabashov 3021:Oti Fossae 2938:labyrinthi 2851:Shalbatana 2654:Her Desher 2547:Ius Chasma 2537:Iani Chaos 2502:Eos Chasma 2452:Aram Chaos 2056:Topography 1919:Home Plate 1914:Adirondack 1874:El Capitan 1849:Rocknest 3 1819:Coronation 1654:Polar caps 1618:Lava tubes 1531:Carbonates 1451:Oxia Palus 666:References 399:sublimated 4547:Trouvelot 4287:Quenisset 4267:Priestley 4237:Pickering 4207:Penticton 4197:Pangboche 4162:Nicholson 4097:Millochau 3987:Lomonosov 3817:Ibragimov 3752:Helmholtz 3737:Heaviside 3727:Hargraves 3651:Grindavik 3536:Escalante 3526:Endurance 3514:Endeavour 3509:Emma Dean 3504:Ejriksson 3429:Danielson 3409:Crommelin 3319:Burroughs 3299:Bonestell 3279:Bianchini 3259:Becquerel 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1376:Coprates 1371:Cebrenia 1346:Amenthes 1341:Amazonis 1243:Cerberus 1052:Archived 736:BBC News 706:186–209. 624:See also 331:terrain. 133:Glaciers 94:337°24′W 51:337°24′W 4669:Winslow 4649:Wegener 4644:Wallace 4577:Tyndall 4567:Tugaske 4542:Tooting 4442:Slipher 4402:Schmidt 4367:Russell 4337:Ritchey 4272:Proctor 4247:Pollack 4202:Pasteur 4172:Nipigon 4167:Niesten 4102:Mitchel 4077:Mellish 4072:McMurdo 4062:Maunder 4042:Mariner 4037:Maraldi 4032:Mandora 4022:Maggini 3972:Lockyer 3932:Lassell 3917:Lambert 3897:Korolev 3877:Kinkora 3827:Janssen 3807:Huygens 3787:Huggins 3742:Heimdal 3732:Hartwig 3712:Haldane 3688:Husband 3671:Grissom 3666:Chaffee 3621:Gilbert 3591:Freedom 3576:Fontana 3556:Firsoff 3541:Eudoxus 3474:Dromore 3454:Denning 3404:Crivitz 3359:Chapais 3349:Cerulli 3339:Cassini 3314:Briault 3274:Bernard 3249:Barnard 3239:Bamberg 3234:Baltisk 3219:Bacolor 3194:Arandas 3169:Agassiz 3141:craters 3136:Catenae 2913:Warrego 2836:Sabrina 2776:Naktong 2739:Mangala 2719:Maʼadim 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3419:Curie 3414:Cruls 3399:Crewe 3394:Corby 3374:Clark 3354:Chafe 3334:Canso 3184:Aniak 3164:Adams 2934:rupes 2908:Verde 2903:Vedra 2891:Uzboi 2886:Tyras 2871:Tinia 2866:Tader 2861:Stura 2856:Simud 2831:Sabis 2826:Reull 2811:Peace 2796:Padus 2786:Niger 2771:Minio 2756:Marte 2749:Labes 2709:Licus 2704:Lethe 2699:Ladon 2694:Labou 2689:Kasei 2684:Ituxi 2679:Indus 2589:Arnus 2579:Apsus 2250:Arsia 2027:Other 1909:rover 1889:rover 1864:rover 1809:rover 1796:Rocks 1719:Water 1625:(LVF) 1613:Lakes 1571:Hagal 1541:Color 1148:from 1139:from 906:K> 893:(PDF) 879:3096. 137:radar 4689:Yuty 4592:Very 4557:Trud 4552:Troy 4422:Sibu 4352:Ross 4312:Redi 4302:Rahe 4292:Rabe 4177:Onon 4027:Main 4007:Lyot 3892:Koga 3852:Joly 3812:Iazu 3717:Hale 3636:Gold 3626:Gill 3616:Gasa 3601:Gale 3586:Fram 3294:Bond 3269:Belz 3264:Beer 3199:Argo 3174:Airy 2821:Ravi 2729:Maja 2659:Hrad 2584:Ares 2032:List 1949:Face 1924:Mimi 1899:Yogi 1839:Link 1778:list 1679:Soil 1199:Mars 1193:and 1084:2015 687:ISBN 127:and 82:Mars 4087:Mie 3977:Lod 3937:Lau 3289:Bok 2896:ULM 2881:Tiu 2724:Mad 2619:Dao 1197:of 4746:: 2936:, 2927:, 1063:^ 1010:^ 815:^ 734:. 131:. 4722:: 3138:, 2931:, 2441:, 2080:) 2076:( 2069:, 1780:) 1776:( 1183:e 1176:t 1169:v 1086:. 895:. 752:. 738:. 719:. 695:. 570:. 542:. 502:. 456:.

Index

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43°54′N 337°24′W / 43.9°N 337.4°W / 43.9; -337.4
Mars
43°54′N 337°24′W / 43.9°N 337.4°W / 43.9; -337.4
Arabia Terra
Ismenius Lacus quadrangle
Protonilus Mensae
Ismeniae Fossae
Glaciers
radar
Mars Reconnaissance Orbiter
Polygonal patterned ground
Polygonal, patterned ground
Sublimation
dry ice
latitude dependent mantle
High-center polygons, as seen by HiRISE under HiWish program Image is of the top of a debris apron in Deuteronilus Mensae.
HiWish program
Close up of field of high center polygons with scale, as seen by HiRISE under HiWish program Note: the black box is the size of a football field.
Close-up of high center polygons seen by HiRISE under HiWish program Note: the black box is the size of a football field.
Close-up of high center polygons seen by HiRISE under HiWish program Troughs between polygons are easily visible in this view.
high center polygons seen by HiRISE under HiWish program
upper plains unit
Group of small sets of dipping layers, as seen by HiRISE under HiWish program
brain terrain
Layered features and brain terrain, as seen by HiRISE under HiWish program The upper plains unit often changes into brain terrain.
Well developed ribbed upper plains material. These start with small cracks that expand as ice sublimates from the surfaces of the crack. Picture was taken with HiRISE under HiWish program
Dipping layers, as seen by HiRISE under HiWish program Also, Ribbed Upper plains material is visible in the upper right of the picture. It is forming from the upper plains unit, and in turn is being eroded into brain terrain.
View of stress cracks and larger cracks that have been enlarged by sublimation (ice changing directly into gas) This may be the start of ribbed terrain.
Evolution of ribbed terrain from stress cracks—cracks to the left eventually will enlarge and become ribbed terrain toward the right side of picture, as seen by HiRISE under HiWish program

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