C.M. Rodrigue, 2007 Geography, CSULB Mars: Second Order Landscapes Geography 494-01 S/07 Dr....
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Transcript of C.M. Rodrigue, 2007 Geography, CSULB Mars: Second Order Landscapes Geography 494-01 S/07 Dr....
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
Geography 494-01
S/07
Dr. Christine M. Rodrigue
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The “Orders of Relief” for Martian Landscapes The first order was the great crustal dichotomy:
Northern lowlands: ~ 1/3 Southern highlands: ~2/3
The second order is tonight’s focus: Tharsis and Elysium rises The largest craters: Hellas, Argyre, Isidis, Utopia Valles Marineris The polar ice caps
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Volcanic Rises Tharsis
8,000 km across Nearly 10 km thick Single big hotspot plume?
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Volcanic Rises Tharsis
Impact-generated?
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes The Volcanic Rises
Elysium “Only” 6 km thick “Only” 2,000 km across
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Volcanic Rises Elysium
Recent volcanic activity: Hecates
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Volcanic Rises Elysium
Glacial features on Hecates? Argued to be snow derived during an ice age produced by a greater obliquity
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Huge: 30 of latitude by 50 of longitude ~2,300 km across ~8 km deep in local topography; 4 km below the geoid!
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Depositional features: volcanic outflows and wrinkle ridges
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Erosional features (MGS MOC): outflow channels Dao Vallis, Niger Vallis, and Harmakhis Vallis
along Hellas’ eastern wall ~ 1 km deep and 8-40 km wide (must have been some outflow)
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Erosional features (MGS MOC): boulder tracks down cliffs
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Depositional features (MGS MOC): lacustrine, shoreline
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Depositional features (MGS MOC): hunh? Water? Ice?
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Hellas Planitia
Depositional features (MGS MOC): dunes in southern Hellas
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Argyre Planitia
Hydraulic system
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Argyre Planitia
Wind deposition: dune (HRSC) Wind erosion: dust devils (MOC)
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Argyre Planitia
Fluvial erosion: gullies in Galle Complexity
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Isidis Planitia
Where Beagle was to land
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Isidis Planitia
Another complex history 1,500 km big impact
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Utopia Planitia
Lava basin antipodal to Argyre
Viking 2 frost documentation
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Impact Basins Utopia Planitia
Circular grabens, some of them double Draping of cover material (sediment?) over buried craters Folding and compaction into depressions creates grabens on
inner slopes of buried craters’ rims Sometimes shrinkage of cover material exerts tension
leading to grabens just beyond buried crater rim
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Subsidiary chasmata
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Not your ordinary grand canyon (east end is actually higher than the middle)
Valles cut into layered material (sediments? lava?) Extensional rifting (perhaps like East Africa?) Pitting (suggests extension) Alcoves (suggesting subsurface flow) Landsliding widens the rifts Massive jökulhlhaup-like outflows
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes The Great Canyons
Valles Marineris Looks like a canyon draining into Margaritifer and then Chryse But look at the elevations of the central and eastern ends
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Layering in walls of Melas Chasma
Dunes covering floor
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Layering in walls of Hebes Chasma And 100 in Candor Chasma below
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Extensional rifting in Tithonium Chasma Pitting (suggests extension)
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Valles Marineris
Extensional rifting in Coprates Chasma and Catena Pitting (suggests extension)
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Melas, Candor, Ophir Chasmata
Theatre-headed tributaries Like Canyonlands, Utah Sapping of groundwater
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Landslides
South Candor Chasma
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Jökulhlhaup?
On Earth, they are massive floods created when a glacier becomes a dam, as here at Russell Lake behind Hubbard Glacier in Alaska in 1986 and 2002, and the dam breaks
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Jökulhlhaup?
If Ares and Kasei valles were formed by outwash floods, here’s how they’d compare to various Earth measures!
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Great Canyons Cerberus Fossæ
Seem tectonic: faulting Lava flow from a fissure?
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Polar Ice Caps North Polar Cap
Water ice cap Seasonal CO2 veneer
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Polar Ice Caps North Polar Cap
Water ice cap Seasonal CO2 veneer
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Polar Ice Caps South Polar Cap
CO2 Water ice cap
underneath?
C.M. Rodrigue, 2007Geography, CSULB
Mars: Second Order Landscapes
The Polar Ice Caps South Polar Cap
Layering Drainage from beneath