Mars (Week 2) Flashcards

1
Q

What is mars planet profile

A

2 moons called phobos and deimos
1.9 years to orbit
surface ranges from -153 to 20
2nd millennium BC recorded by egyptian astronomers
largest dust storms
will one day have a ring

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2
Q

Why is Mars hostile

A
  • thin C02 atmosphere
  • gravity 0.38 of earth
  • air pressure 0.7 of earth
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3
Q

What is Mars core like

A
  • large and liquid
  • insight lander revealed this
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4
Q

Why will Mars eventually have rings

A
  • moons closer to surface and mars will break them apart to get rings
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5
Q

How does the mass of Mars compare to Earth

A
  • Mars is has 10 times less the mass- very small planet
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6
Q

What is the dominant crustal material

A
  • basaltic (on venus too)
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7
Q

What are the volcanoes on Mars like

A
  • many volcanoes
  • whole provinces- olympus = largest volcano in solar system
  • Tharsis igenous area made from 3 aligned volcanoes
  • Volcanic arcs dont exist- intraplate magmatism (like Hawaii)
  • Mars has a cooler geotherm due to thicker crust
  • deeper magma storage
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8
Q

What are magmatic intrusions like on Mars

A
  • brittle ductile transition is shallower on earth as mars has a thicker crust
    -deeper storage/ fractures deeper
  • implications for groundwater storgae
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9
Q

how are volcanoes like olympus formed

A
  • thicker crust
  • stagnant lid
    -lava flows build up due to lack of techtonics
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10
Q

What does extreme crustal dichotomy mean

A
  • northen hemisphere lower topographically
  • big impact event caused this
  • southern crust impacted much more
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11
Q

Examples of some martian rocks

A
  • shergottites ( basaltic to ultramafic, vast majority of martian asteroids, young, due to volcanic activity)
  • Nakhilites and Chassignites (ultramafic, formed at surface, come from same location and ejected same event)
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12
Q

How do we know these rocks are martian?

A
  • oxygen isotopes
  • turned into glass through to hostile pressure of space (measure gases from viking rovers)
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13
Q

what is the geological time scale of Mars

A
  • different to earth!
  • right now is called the amazonian which is based on rover observations
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14
Q

morphology of Mars for water

A
  • deltas
  • deltaic fans
  • giant pebbles from water flow shown by curiosity
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15
Q

does mars have a geodynamo

A
  • NOOOO
  • zero evidence
  • HOWEVER, mars once may have had one but may have
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