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Surface Features on Mars. Dr. Joshua Bandfield Mars Space Flight Facility Arizona State University. Mars has Many Types of Surface Features. Impact Craters Volcanic Features Fluvial/Water-Related Features Layers Aeolian/Wind Features. 2. All THEMIS visible images are ~18 km across.
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Surface Features on Mars Dr. Joshua Bandfield Mars Space Flight Facility Arizona State University
Mars has Many Types of Surface Features • Impact Craters • Volcanic Features • Fluvial/Water-Related Features • Layers • Aeolian/Wind Features 2
All THEMIS visible images are ~18 km across Crater Ejecta • Material that gets thrown out of a crater when a meteorite hits the surface • Sometimes looks rougher than the surrounding terrain Most THEMIS images are taken during the afternoon and the sun is shining from the left side of the image 7 Crater in Elysium Planitia 18N, 136E
Rampart Craters • Have distinct ejecta that looks like it flowed across the surface • Probably due to ice or liquid water in the subsurface when crater formed Rampart Crater in Acidalia Planitia 28N, 319E 8
Crater Morphology Central Peak • Morphology (shape) will look different based on age and size: • Large craters: Central peaks, rings and/or slumping walls • Old craters: Eroded and have ‘softer’ features • 3 ‘types’ of craters: • Preserved • Modified • Destroyed Slumps 9 Arabia Terra 18N, 6E
Orcus Patera 16N, 183E Ares Vallis 16N, 330E Modified Craters • Craters can be eroded or modified by: • Wind • Water • Lava 10
Volcanic Features • Many types of surface features are associated with volcanoes: • Volcanic structures • Lava flows • Calderas • Lava Tubes/Channels • Olympus Mons (shown here) is a shield-like volcano the size of the state of Arizona! 13 Olympus Mons 18N, 230E (Wide Angle)
Alba Patera Olympus Mons Ascraeus Mons Pavonis Mons Arsia Mons Volcanics on Mars • Volcanic activity has dominated the surface of Mars • Tharsis is a huge (1/3 of the planet) volcanic region that consists of 3 shield-like volcanoes • Olympus Mons, Alba Patera and other small volcanoes are evident in this area 14
Lava Flows • There are many lava flows on Mars of all ages • These are similar to lava flows that we see in places like Hawaii, but can be much larger! Daedalia Planum -26N, 232E 15
Apollinaris Patera Caldera Multiple basins in the caldera Channels along the flank Lat: 9.3 S Lon: 174.4 E THEMIS Day IR Mosaic 18 6
Dust Devil Tracks • Dust devils pick dust up in to the atmosphere • They can act like vacuum cleaners and leave dust-free tracks behind them Argyre Planitia -47N, 318E 35
Wind Streaks • Wind streaks form behind topographic features (such as crater rims) • Dust can be deposited or scoured in a wind streak 36 Syrtis Major 0N, 72E
Dunes • Dunes are wind blown piles of sand • Sand dunes on Mars are often dark because they are made of basaltic sand Sand Dunes in Kaiser Crater -47N, 19E 37
Surface Features on Mars • Impact Craters • Volcanic Features • Fluvial/Water-Related Features • Layers • Aeolian/Wind Features 39
Mars Maps • Mars Regions • Zoom in to see details • Also see: http://pubs.usgs.gov/imap/i2782/i2782_sh1.pdf 40