MARS TECTONICS & VOLCANOLOGY Zachary Gallegos University of New Mexico / Mars One.

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Transcript of MARS TECTONICS & VOLCANOLOGY Zachary Gallegos University of New Mexico / Mars One.

MARS TECTONICS & VOLCANOLOGYZachary Gallegos

University of New Mexico / Mars One

Mars Orbiter Laser Altimeter Map

Plate Tectonics• Lithospheric plates sliding

on the asthenosphere, above the mantle

• Exists on Earth

• Theory proposed in the early 1900’s

• Does it exist on other bodies in the solar system?

Plate Tectonics• Recycles material

• Regulates the atmosphere• CO2 sequestration and output

• Linked with mantle convection• Push new material to surface

at divergent boundaries• Pulls old material into the

Earth at convergent boundaries

Tectonics of Earth• Picture of plates

Plate boundaries

• Divergent• Spreading apart

• Convergent • Moving together

• Strike-slip• Sliding past

Divergent

• Mid-Atlantic ridge• Oceanic

• East African Rift• Continental

• Rio Grand Rift• Continental

Convergent

• Mariana Islands/Trench • oceanic-oceanic

• Pacific Northwest • oceanic-continental

• Himalayas • continental-continental

Strike-slip

• San Andres fault • right lateral

Tectonics of Mars

• Mars seems to lack global, Earth-like tectonics• Too small?• Not enough water?

• Large scale faulting

• HUGE scale rifting

Topography

• Mars’ planetary dichotomy• Not tectonic in origin

• Bolide impact , water resurfacing

• Slow sloping at the dichotomy• not pronounced

• Earth’s dynamic lithosphere• Tectonic in origin• Steeply sloping at the margins

• Continental and oceanic crust

Magnetics• Possible magnetic reversals recorded in early Martian crust

Interior of Mars• Smaller/colder

• Less water

Faulting on Mars• Thrust faulting

• Amenthes Rupes

• Normal faulting• Circum-Tharsis

• Strike-slip faulting??• Within Valles Marineris

Valles Marineris• Giant tectonic fissure in

the crust• Not the result of plates• Result of Tharsis uplift

• Length: > 4,000km

• Width: > 200km

• Depth: > 7km

• Largest known valley in the solar system

Valles Marineris• Nearly ¼ or the planets circumference

• Nine times longer than the grand canyon

Vallis Marineris

Volcanology of Earth• Most of Earth’s volcanism is related to plate tectonics

• Divergent and convergent boundaries

Volcanology of Mars• No planetary tectonics

• Shield forming• Hot spot volcanism (e.g. Hawaii)

• Mostly basaltic in compositions• From ultramafic komattiatic to dacitic

Why Basalt?• Hot spot volcanism produces basalt

Volcanism and Tectonics• With no tectonics, volcanoes grow to enormous size

Montes• Mons are large shield volcanoes

• Earth analogue: Hawaii

• Gentle slopes < 6°

Ascraeus Mons Pavonis Mons Arsia Mons

Tholi• Tholus is a term for

smaller, dome shaped volcanoes• Older than Mons

• Buried by later flows

• Steeper flanks

• Different material than Montes?

• Less material than Montes?

Patera• Term given to small volcanoes with large calderas

• Latin translation: shallow drinking bowl

• Larger calderas than the tholi

• Probably represent larger volcanoes

• Buried beneath flows and sediment

Rootless Volcanoes & Pseudocraters• Show no sign of magma conduit

• Analogues on Earth erupt due to a magma body flowing over a surface or subterranean water source

Martian Volcanic Provinces

Tharsis• Largest volcanic province on Mars

• 25% of the planets surface

• Avg. 7-10km above datum

• Youngest flows on Mars

Tharsis

Arsia Mons

Olympus Mons• Largest mountain in the solar system

• Height: > 22km

• Diameter: > 500km

• Slope: ~ 4°

• 6 nested calderas• 3.5km deep

Alba Mons• North of Tharsis buldge

• Very low slopes ~ .5°

• 1600km across

• Rises 3km above plains

Elysium• Second largest volcanic

province• 1,700x2,400 km

• Elysium Mons• 13km high

• Hecates Tholus• North

• Albor Tholus• South

Syrtis Major

• 1200km across

• 2km high

• 2 calderas• Nili Patera, Meroe Patera

• Silica rich rocks• Dacite & Granite

Isidis Basin

Questions?

Geography of Mars

Volcanic Provinces

Exploration Sites