the geology of mars flight into valles marineris

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Page 1: The Geology of Mars Flight into Valles Marineris
Page 2: The Geology of Mars Flight into Valles Marineris

The Geology of Mars

Page 4: The Geology of Mars Flight into Valles Marineris

Geological Processes

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Chaotic TerrainForms when subsurface water or ice causes a

loss of support and the ground collapses.

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Page 7: The Geology of Mars Flight into Valles Marineris

GrabenA depressed block of

land bordered by parallel faults (graben is German for ditch).

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Page 9: The Geology of Mars Flight into Valles Marineris

SappingSapping valleys are formed breaks the

surface and undermines rock and sediment,

causing it to collapse.

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Slumping

The grounds collapses and sinks or falls suddenly and

heavily.

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Subsidence

The sinking of ground surface due to the physical removal of ground surface.

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Landslides

Material that has fallen down a steep slope and material piles up at the

bottom.

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Layers

Formed by stacks of lava flows, ash from volcanoes,

dust, or by sediments deposited in water.

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Fractures/Faults

Result from breaks in the surface. They are

generally straight.

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Fracture Fault

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Gullies

Often found on crater walls or other slopes. May be

associated with past liquid water or areas once covered with snow.

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Fissures

Cracks that are found sometimes on the sides of

volcanoes. Lava flows may be seen moving away from the fissure, indicating

lava flow.

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Lava Flows

Formed by flowing lava. Flows can look “wavy” or

“fingery.” Flows are raised features.

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Collapsed Lava Tube

Look similar to channels. Lava once flowed

underground through a tunnel. Some aren’t

completely collapsed and look like a small chain of

craters.

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Page 29: The Geology of Mars Flight into Valles Marineris

Channels

Formed by consistent flow of water over a long period

of time. Has a curvy or meandering shape.

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Streamlined IslandsThought to be associated

with the plast flow of water around a feature. Often

found in outflow channels wher large amounts of

water flowed.

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Sand Dunes

Often seen in the bottom of craters or channels.

Look like ripples of material.

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Yardangs

Formed by sand-sized particles being blown

against a surface, wearing it away.

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Regions of Mars

Tharsis

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Volcanic Plateau on Mars.

 There are three enormous shield volcanoes Arsia

Mons, Pavonis Mons, and Ascraeus Mons, which are known as the Tharsis

Montes.

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Volcanic Plateau on Mars.

Arsia Mons Parvonus Mons

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Volcanic Plateau on Mars.

Ascraeus Mons

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Volcanic Plateau on Mars.

Olympus Mons is nearby.

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There are other small volcanoes.

Lava flows are common in the Tharsis region.

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Marineris

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Valles Marineris (the Grand Canyon of

Mars is found in this area.

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On Earth, it would stretch from San

Francisco, CA to New York, NY.

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There are many regions in Valles

Marineris.

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There are plateaus in the south, craters in the north and south, additional valleys in

the north

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Meridani

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A heavily cratered region.

Opportunity found evidence for water in

this region.

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The Aureum & Arsinoes Choases (chaotic terrain)

are found in Meridani.

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Syrtis Major

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This is a plateau & volcanic region.

You can see examples of wind

blow terrain.

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This is a highly cratered region.

Valleys and layering geology are found

here.

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Hesperia

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The southern part of the region is on a

plateau.

It is a highly cratered region in the south.

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Elysium Planitia is a major

volcanic region.

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Elysium Mons volcano found here.

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South and west from Elysium Mons you find

Elysium Chasma.

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Continue south and west and you find the Hyblaeus

Dorsa lava flows.

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Memnonia

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The southern part of the region has many

craters.

The craters in this region show evidence

of erosion.

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Tartarus Montes

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In the northeastern corner there are two

plains – Arcadia Planitia and Amazonus Planitia.