Mars: Fourth Order LandscapesSlide 2Slide 3Slide 4Slide 5Slide 6Slide 7Slide 8Slide 9Slide 10Mars: Fourth Order LandscapesSlide 12Slide 13Slide 14Slide 15Slide 16Slide 17Slide 18Slide 19Slide 20Slide 21Slide 22Slide 23Slide 24Slide 25Slide 26Slide 27Slide 28Slide 29Slide 30Slide 31Slide 32Slide 33Slide 34Slide 35Slide 36Slide 37Slide 38Slide 39Slide 40Slide 41Slide 42C.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesGeography 494-01S/07Dr. Christine M. RodrigueC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesThe “Orders of Relief” for Martian LandscapesThe first order was the great crustal dichotomy:Northern lowlands: ~ 1/3Southern highlands: ~2/3The second order was the large regional features: Tharsis and Elysium risesThe largest craters: Hellas, Argyre, Isidis, UtopiaValles MarinerisThe polar ice capsC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesThe “Orders of Relief” for Martian LandscapesThe third order was the somewhat smaller major regions associated with the araeological eras:In many ways, this is a cross-cutting categoryIt addresses the “geological column” or relative ages of all Martian landscapes in terms of the three regional units that gave the three-part sequences of Mars’ evolution their names:The Noachian EraThe Hesperian EraThe Amazonian EraC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesThe “Orders of Relief” for Martian LandscapesThe fourth order is “in order” now:These are smaller features (a few kilometers to a few hundred):They are landscapes dominated by one or two processesFluvial valleys Sapping alcoves Linear fossæFolded and faulted mountains of ThaumasiaLava tubes Layered mesas Patterned ground Dune fields Evidence of mass wastingC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly precipitation-fed overland and channelized surface flowEchus Chasma (Mars Odyssey Themis)Echus Chasma (Mars Express)C.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly precipitation-fed overland and channelized surface flowEchusC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly alluvial fans and deltasMelasC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly alluvial fans and deltasEberswalde Crater near Holden CraterC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly lake overflow channelsMa’adim Vallis, pouring into Gusev Crater, where Spirit landedC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly lake overflow channelsArgyre, Holden, Aram craters and Ares VallisNirgal Vallis tributary to that waterway, which still shows signs of water releasesC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly jökulhlaup-like outflowsKasei VallisAres VallisC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly jökulhlaup-like outflowsAres VallisAram Chaos and collapsed terrainC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly jökulhlaup-like outflowsDao, Niger, and Harmakhis valles in Hellas PlanitiaC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesValleys dominated by fluvial processes:Possibly jökulhlaup-like outflowsChasma BorealisKathryn Fischbaugh and James Head created a topographic map and profiles and used them to estimate volume of a catastrophic melt (perhaps subsurface vulcanism): 26,000 km3!Picked out deposits from such an event: could fill lowest portion of north polar basin to a few 10s of m!C.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesAlcoves, channels, aprons:Groundwater sappingEarth on right: Mt. St. HelensMartian crater gully on left: MGS’ Mars Orbital Camera (~-55 at 18)C.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesAlcoves, channels, aprons:Groundwater sappingEarth on top: sides of Houghton Crater, Devon Island, Canada North of Baffin IslandOnly Earth crater on a polar desert surfaceSite of NASA-Houghton ProjectMartian crater gully on left: MGS’ Mars Orbital Camera (where?)C.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesAlcoves, channels, aprons:Groundwater sappingFresh gullyingMGS’ Mars Orbital CameraC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesAlcoves, channels, aprons:Groundwater sappingThe triple point of waterC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLinear fossæ and catenæ:Extensional stress, faulting, downdropping of terrain between faultsCerberus FossæC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLinear fossæ and catenæ:Extensional stress, faulting, downdropping of terrain between faultsClaritas FossæC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLinear fossæ and catenæ:Extensional stress, faulting, downdropping of terrain between faultsAlba Patera FossæC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLinear fossæ and catenæ:Extensional stress, possibly with fluid extraction and subsidenceTithonium CatenæCoprates CatenæC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLinear fossæ and catenæ:Secondary cratering from a primary impact eventTHEMIS, +19 at 348 (Trouvelot Crater)MOC, +16 at 325Maybe a single object breaking up before hitting?MRO image of Candor Chasma wall with this weird chain cutting across at an angle to gravityC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesFolded and Faulted Mountains:Grabens and foldsThaumasiaC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLava Tubes:Lava flows under a crust, which may collapsePavonisCheck out catenaC.M. Rodrigue, 2007Geography, CSULBMars: Fourth Order LandscapesLayered Mensæ:Resistant caprocks protect less resistant
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