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Olympus Mons Mitchell Kirshner 3/11/14.

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Presentation on theme: "Olympus Mons Mitchell Kirshner 3/11/14."— Presentation transcript:

1 Olympus Mons Mitchell Kirshner 3/11/14

2 History 19th century Mariner 9 Viking Mars Global Surveyor

3 Location 18.65 °N, 226.2 °W Northwest of Tharsis
23 km tall, km, km 600 km across

4

5 Timeline MOC and THEMIS used to find that Noachian period >3.7Ga yielded global volcanism followed by vent volcanism in Tharsis, Elysium, and Circum-Hellas later just in Tharsis and Elysium Activity localized to Tharsis around 1.6Ga volcanism was active until Ma

6 Effusion rate of magma supply to Kilauea and Moana Loa averages .01 km3/yr Volume is estimated to be 2.6*10^6 km^3 Using rate accumulation values given in Hawaii, it would take 130 million years to construct shield volcano

7 Gravity

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9 Aureole Deposits Northwest East Flank failure-induced landslides
Ice-Lubricated Gravity Spreading Glacial Interactions

10 Escarpment 8 km Assymetry Northwest=shallow, southeast=steep Water
Mass movement Faults

11 Caldera SiO2 content Lava fountain  cinders

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13 Magma Chamber d<16 km Estimated depth of Martian primary melts

14 Atmospheric Effect Constant column density
~5 decrease in mass from bottom Low atmospheric density

15 Water Deep within volcano Shielded from radiation East flank- faults

16 Future Landings Difficult to study via rover 8km escarpment Parachute
Dust

17 The End


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