Mars: First Order LandscapesMars: First Order LandscapesSlide 3Slide 4Slide 5Slide 6Mars: First Order LandscapesSlide 8Slide 9Slide 10Slide 11Slide 12Slide 13Slide 14Slide 15Slide 16Slide 17Slide 18Slide 19Slide 20Slide 21Slide 22Slide 23Slide 24Slide 25Slide 26Slide 27Slide 28Slide 29Slide 30Slide 31Slide 32C.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesGeography 494-01S/07Dr. Christine M. RodrigueC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesOn Earth, the orders of relief schemeIs sometimes seen in geography textbooksOrganizes topographic variation in a scale-dependent mannerGeographers often focus on Spatial analysis of particular phenomenaRegional synthesis to integrate assemblages of phenomenaScales at which processes and regional patterns operateThe interactions among phenomena at different scalesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesExamples of interactions among scalesIn spatial statistics: the Modifiable Areal Unit Problem (MAUP) In human geography: local cultural and political responses to global economic and political processes Biogeography: alpha, beta, and gamma measures of biodiversity Geomorphology: "megageomorphology" has emerged as remote sensing technology has made the simultaneous examination of form and process at large scale (small map scale) possibleC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesFor Mars, a handy descriptive scheme for handling the regional variations in Mars’ physical landscapesThe “First Order of Relief” = the crustal dichotomyThe northern lowlands: Vastitas BorealisThe southern highlandsIf Earth’s oceans evaporated (which they will …), there would remain a crustal dichotomy hereFormer ocean basins: low elevation, thin crust, basaltic, with a veneer of pelagic sedimentsFormer continents: high elevation, thick crust, granitic rocks and their extrusive igneous, sedimentary, and metamorphic derivativesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisRegional subdivisions:Utopia Planitia North Polar BasinEmbayments: Acidalia PlanitiaChryse PlanitiaAmazonis PlanitiaArcadia PlanitiaIsidis PlanitiaC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisRelatively young surfaceSmooth with few cratersThis is exactly what you’d expect if Mars had had an oceanIt could be expected to receive sediments from rivers, floods, and coastal processes and create terrigenous sediments nearshoreThey would be turned into minerals that would eventually precipitate out of the water column onto the abyssal floorThe oceans would thus cover the underlying original rock surface, much as pelagic sediments here doC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisFurther suggestions of an ocean:Drainage of Martian outflow channels and valley networksThis is also exactly what you’d expect if Mars had had an ocean to serve as base level for stream networksC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisDrainage:Valles Marineris' outflow channels, which drain into Chryse PlanitiaNanedis north of GangesAres and Aram Chaos Argyre to Aram and AresC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisEven better: Coastlines!?Transition between the southern highlands and the northern lowlands is quite abruptC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisEven better: Coastlines!?Terraces on the Arcadia side of Alba PateraC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisEven better: Coastlines!?Tim Parker’s analysis of Viking imageryC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisEven better: Coastlines!?Tim Parker’s analysis of Viking imagery (1994)His and others’ re-analysis using MOC imagery seemed to debunk his argument, which even he admitted in 2001But it’s as though the new imagery is so fine in resolution that it can’t detect the coarser scale at which this putative ocean’s coastline features might existMOLA suggests that, in fact, at least one of the “coastlines” is at the same elevation (water seeks a level constant with respect to the geoid)C.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisPlot complicationThat "ocean" floor is dominated by andesitic rockNot sediments with minerologies consistent with precipitation out of water. No carbonates! No ocean?C.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisAbout those andesites"Surface Type 1" (basalts dominating the southern highlands)"Surface Type 2" (andesites and andesitic basalts dominating the northern lowlands)C.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesVastitas BorealisRampart cratersC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian LandscapesThe Southern HighlandsMostly 1-5 km above the mean Martian geoid Versus 0-3 km below for the northern lowlandsSharp ~1 km scarp dividing the twoC.M. Rodrigue, 2007Geography, CSULBMars: First Order LandscapesThe “Orders of Relief” for Martian
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