Exam 3 Flashcards

(91 cards)

1
Q

What is impact cratering?

A

Arterial falling from space onto a world’s surface will create impact craters.

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2
Q

What do more craters indicate?

A

The number of craters can indicate the surface’s age. More craters means an older surface and minimal geologic activity.

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3
Q

Define Plate tectonics

A

The theory that explains how slow the motions within the Earth moves large segments of the crust (outer surface) gradual “drifting” of the continents.

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4
Q

How can volcanism change a surface?

A

Volcanic eruptions can erase craters.

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5
Q

What do we learn by studying earthquakes?

A

We learn about earth’s interiors. Earthquakes produce seismic waves, which travel differently through different materials.

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6
Q

Which of the following layers of the earths interior is composed of liquid metal?

A

The outer core

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7
Q

Define Convection

A

Rising and falling of hot/cold material

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8
Q

Crustal plates are moved by …

A

convection

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9
Q

How many major and smaller plates does earth have?

A

7 major plates and 6 smaller ones

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10
Q

Very fluid lava forms…

A

Shield volcanes

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11
Q

Viscous lava forms

A

Composite volcanoes

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12
Q

Define Erosion

A

On earth, liquid water strongly eroded the surface.

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13
Q

The geographic North Pole is magnetic North or South?

A

The magnetic South Pole

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14
Q

How was Earth’s crust shifted over time?

A

The movement of plate boundaries.

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15
Q

Define Continental drift

A

The movement of the earths crust. Proved by fossils near the riff zones.

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16
Q

How is Earth’s atmosphere unique?

A

Because of convection.

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17
Q

Define The green house effect

A

Carbon dioxide content of the retains heat from the sun through a process called the greenhouse effect.

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18
Q

How is the greenhouse effect beneficial or harmful?

A

Without, earth’s ocean would be frozen.

With, the earth is 40 degrees c hotter

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19
Q

The principal greenhouse gases in our present atmosphere are

A

Water vapor and carbon dioxide

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20
Q

Mercury Rotation

A

58 earth days

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21
Q

Mercury orbit

A

88 earth days

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22
Q

Mercury surface

A

Rocky, solid, and cratered surface much like the moon.

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23
Q

Mercury atmosphere

A

A thin atmosphere

Oxygen, sodium, hydrogen, helium, and potassium.

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24
Q

Mercury temperature

A

800 to -290 degrees.

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25
Mercury Magnetic field
Earth and mercury are the only terrestrial planets with a substantial magnetic field.
26
Mercury tilt
.04
27
Venus tilt
177.36
28
Venus rotation
243 earth days
29
Venus spin
Backwards
30
Is Venus habitable?
In its early history, Venus could have had shallow linguistic water ocean and habitable surface temperatures.
31
Venus surface
Volcanic with extensive plains featuring high volcanic mountains and vast ridged plate.
32
Venus temperature
900 degrees Runaway greenhouse effect
33
Venus habitable?
No. Unless you like acid rain and melting lead temperatures.
34
Earth tilt
23.5
35
Order of the atmosphere
``` Troposphere H20 clouds Stratosphere Ozone Mesosphere Thermosphere ```
36
Ionosphere
Many of the atoms are ionized by the loss of an electron, and this region is often called the ionosphere.
37
Earth’s atmosphere
Nitrogen Oxygen Argon Traces of water vapor and carbon dioxide
38
Earth habitable?
Heck yes The early atmosphere contained abundant carbon dioxide and some methane but no oxygen.
39
The moon atmosphere
The moon has no atmosphere
40
Moon surface
Most of the crust consists of silicate rocka and these regions are known as lunar highlands. Smooth features on the craters are attributed to gradual erosion, mostly due to impact cratering from meteorites.
41
Moon volcanism
The moon had past lava flows which smoothed out parts of its surface.
42
Moon temperatures
Rises above boiling water and drops down to -279.4 F
43
Lunar Maria are found...
Mostly on the side of facing earth
44
Mars tilt
25.19
45
Mars rotation
A little over 24 hours
46
Mars orbit
687 earth days
47
Mars atmosphere
Thin atmosphere Has seasons
48
Mars surface
Solid, altered by volcanoes, impacts, winds, crystal movement, and chemical reactions.
49
Mars tectonism
Mars shows evidence of extensive tectonism and boasts the massive chasm Valles Marineris.
50
Mars atmosphere
Thin | Carbon dioxide, argon, nitrogen, and a small amount of oxygen and water vapor.
51
Mars moons
2 moons
52
Mars surface
Red planet, because of iron minerals in the Martian soil oxidize causing the soul to look red.
53
Jupiter mass
317.8
54
Jupiter tilt
3.13
55
Jupiter composition
Hydrogen and helium
56
Jupiter rotation
10 hrs
57
Jupiter orbit
12 earth years
58
Jupiter moons
75 moons
59
Jupiter rings
Thin
60
Jupiter habitable
No
61
Jupiter moon’s habitable?
Maybe. Some have oceans that might support life.
62
Jupiter surface
String dark bands (belts) and light bands (zones) The colors are determined by their chemical composition
63
Jupiter magnetic field
Strong magnetic fields are generated by the motion of the conducting liquids. Stronger than the terrestrial planets.
64
Saturn mass
95
65
Uranus mass
14.5 times that of earth
66
Neptune mass
17.1
67
Saturn tilt
26.7
68
Uranus tilt
97.8
69
Neptune tilt
28.3
70
Saturn rotation
10.7 hours
71
Saturn orbit
29 earth years
72
Saturn atmosphere
Hydrogen and helium
73
Saturn moons
62 moons
74
Saturn rings
Most prominent rings
75
Saturn habitable?
No
76
Titan
Largest moon of Saturn and the second largest natural satellite in the solar system.
77
Cryovolcanoes
Cold geysers
78
Uranus composition
Ice giant, dense fluid of icy materials- water methane and ammonia.
79
Uranus rotation
17 hrs On its side, east to west.
80
Uranus orbit
84 earth years
81
Uranus atmosphere
Molecular hydrogen, atomic helium, small amount of methane.
82
Uranus rings
13 known rings
83
Uranus moons
27 known moons
84
Neptune rotation
16 hours
85
Neptune orbit
165 earth years
86
Neptune composition
Icy | Water, methane and ammonia
87
Neptune atmosphere
Molecular hydrogen, atomic helium, and methane.
88
Neptune rings
6 known rings
89
Neptune moons
13 moons
90
Has giants
Jupiter and Saturn
91
Ice giants
Uranus and Neptune