Lecture 11 Flashcards

1
Q

What is the role of planetary size?

A
  • smaller worlds cool faster
  • larger worlds remain warmer, promoting volcanism and tectonics
  • larger worlds have more erosion because their gravity retains an atmosphere
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2
Q

How does the distance from the Sun effect erosion?

A
  • planets close to the sun are too hot for rain, snow and ice so erode less
    -hot planets have difficulty retaining an atmosphere
  • planets far from the sun are too cold for rain and so erode less
  • planets with liquid water have the most erosion
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3
Q

What is the effect of rotation on erosion and magnetic field strength?

A

-Planets with slower rotation have less weather, less erosion and a weak magnetic field
-Planets with faster rotation have more weather, more erosion and a stronger magnetic field

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4
Q

How can we use of the number of craters on a planet?

A

Craters can be used to approximate the age of a planet

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5
Q

What is evidence of tectonics on Mercury?

A

Long cliffs indicate that Mercury shrank early in its history after the mantle shrank

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6
Q

Why are some of the earlier craters on the moon smooth?

A

Some areas of the moon are heavily cratered. Younger regions were flooded by lava, which smoothed the surface.

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7
Q

Where is water on the Moon and how did it arrive?

A
  • water exists on the moon’s poles
  • the water was delivered by comets
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8
Q

What is a Lunar Maria?

A

Smooth, dark areas created by floods of runny lava

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9
Q

What is the process of formation of Lunar Maria?

A

-early surface is covered with craters
-large impact craters weaken the crust
-heat build-up allows lava to well up to the surface
-cooled lava is smoother and darker than surroundings

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10
Q

Why is the moon geographically dead?

A

The geological processes have virtually stopped

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11
Q

How do we map Venus?

A

The thick atmosphere means that radar must be used to image the surface

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12
Q

What did flowing lava do to the surface of Mercury?

A

Smoothed some of the surface

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13
Q

What are some surface features on Venus?

A

-Venus has impact craters (but not as many as the Moon)
-Shield volcanoes
-Fractures on the surface indicate tectonic stress on Venus- but not recent stress

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14
Q

How is continental motion measured on the Earth?

A

By GPS

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15
Q

How did the Himalayas form?

A

Collision between tectonic plates

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16
Q

How did the Red Sea form?

A

The red sea formed where plates pulled apart

17
Q

What is cratering like on Mars?

A

-Cratering differs greatly across the surface
-Many of the earlier craters have been erased

18
Q

What are volcanoes like on Mars?

A

Mars has many large volcanoes including the largest volcano in the solar system

19
Q

What was thought to have formed the Valles Marineris on Mars?

A

The Valles Marineris are thought to have originated from tectonics

20
Q

Was there liquid water on Mars?

A

Gullies and craters suggest liquid water may have existed less than one million years ago

21
Q

What does the erosion of Martian craters suggest?

A

Details found in some of the craters suggest that they were once filled with water

22
Q

What do Martian rocks show?

A

Mars rovers have found some rocks which look like they formed in water