GEO Test 3

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Last updated 4:57 PM on 4/28/25
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100 Terms

1
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What layers make up Ganymede’s internal structure?

Ganymede's internal structure consists of an iron core, a rock layer, and an ice layer.

2
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What evidence suggests Ganymede is fully differentiated?

The low moment of inertia is evidence for Ganymede's differentiation.

3
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How deep is Ganymede's potential subsurface ocean?

Ganymede may have a possible salt-water ocean approximately 200 km beneath the surface.

4
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What two factors contribute to Ganymede's internal heating?

Faster accretion that trapped heat inside and greater tidal heating due to gravitational interactions contribute to Ganymede's internal heating.

5
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What material is likely responsible for Ganymede's induced magnetic field?

Electrically conductive material, likely saltwater, is likely responsible for Ganymede's induced magnetic fields.

6
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Why is ice alone not sufficient to conduct electricity in Ganymede?

Ice alone is a poor conductor; saltwater conducts electricity well.

7
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What is the 4:2:1 resonance among Io, Europa, and Ganymede?

In the 4:2:1 resonance, Io orbits four times, Europa twice, and Ganymede once.

8
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How does orbital resonance increase tidal heating?

Resonance increases orbital eccentricity, leading to greater tidal and frictional heating.

9
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Why doesn’t Callisto experience significant tidal heating?

Callisto is not part of the resonance system, resulting in little orbital eccentricity and subsequent tidal heating.

10
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What is the composition of Europa’s surface?

Europa has a thin icy crust over a potential subsurface ocean.

11
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What surface features are observed on Europa?

Cracks, ridges, and grooves across Europa's surface suggest tectonic and/or cryovolcanic activity.

12
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What does the low number of impact craters on Europa suggest?

It suggests a young surface.

13
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What is Europa's approximate density?

Europa's density is approximately 2.99 g/cm³.

14
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What are the two proposed internal models for Europa?

One is a thick hard icy shell overlying a liquid water ocean; the other is a warm interior with soft convecting ice.

15
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What feature on Europa resembles icebergs?

The Conamara Chaos region resembles icebergs frozen in ice.

16
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What terrestrial feature does Conamara Chaos resemble?

It resembles Earth's ice shelves.

17
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Why is Europa considered a candidate for life?

Potential deep-sea hydrothermal vents could provide habitats for life.

18
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What mission is scheduled to launch to Europa in 2024?

The Europa Clipper mission is scheduled to launch in 2024.

19
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When is the Europa Clipper mission expected to arrive at Europa?

The mission is expected to arrive in 2030.

20
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What is the ESA JUICE mission?

The ESA JUICE Mission studies Europa, Ganymede, and Callisto.

21
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When was the ESA JUICE mission launched?

It was launched in 2023.

22
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When is the ESA JUICE mission expected to reach Jupiter?

The mission is expected to reach Jupiter in 2031.

23
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What makes Io’s surface unique in the solar system?

Io's surface is the most volcanically active body in the Solar System.

24
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Why are there no impact craters on Io?

Constant resurfacing from volcanic activity prevents the formation of impact craters.

25
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What is Io’s approximate density?

Io's density is approximately 3.53 g/cm³.

26
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What type of atmosphere does Io have?

Io has a thin sulfur dioxide atmosphere.

27
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What volcanic features are observed on Io?

Huge plumes extending hundreds of kilometers are observed.

28
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How were Io’s volcanic activities predicted?

They were predicted due to intense tidal heating.

29
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What is the composition of Io’s interior?

Io's interior consists of an iron core and silicate mantle.

30
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How much of Io’s mantle might be molten?

Io's mantle may be 10-20% molten.

31
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What are Saturn’s rings primarily made of?

Saturn's rings are primarily made of water ice and minor carbonaceous material.

32
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What is the typical particle size in Saturn’s rings?

Particle sizes range from 1 meter to less than 1 micrometer.

33
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How far do Saturn’s rings extend above the equator?

They extend from 7,000 to 80,000 km above Saturn's equator.

34
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How thick are Saturn’s rings?

Saturn's rings are very thin, approximately 10 meters thick.

35
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Name one theory about the formation of Saturn’s rings.

One theory suggests the destruction of a moon/planet within the Roche limit.

36
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What evidence suggests Saturn’s rings might be young?

Their brightness and 'cleanliness' suggest they might be younger than 4.5 billion years.

37
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What is the Roche limit?

the distance from a celestial body within which a satellite, held together solely by its own gravity, will disintegrate due to the stronger gravitational pull of the primary body's tidal forces

38
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How close to Saturn does the Roche limit extend?

It extends within approximately 90,000 km from Saturn.

39
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How large is Titan compared to other moons?

Titan is the second-largest moon.

40
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What is Titan's approximate diameter?

Titan's diameter is approximately 5,150 km.

41
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What is Titan’s density?

Titan's density is about 1.89 g/cm³.

42
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What is Titan’s atmosphere primarily composed of?

It's primarily composed of ~95% nitrogen and ~5% methane.

43
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What causes the organic haze in Titan’s atmosphere?

UV processing of methane and nitrogen causes the organic haze.

44
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What probe landed on Titan in 2004?

The Huygens probe landed on Titan.

45
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What surface features did the Huygens probe observe on Titan?

Dry riverbeds, lakebeds, and rounded ice rocks.

46
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What did Cassini’s radar detect on Titan?

Lakes of liquid methane, ethane, and propane.

47
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Why is the presence of methane in Titan’s atmosphere surprising?

Methane should be destroyed by sunlight, implying active replenishment.

48
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What does Titan serve as a natural laboratory for?

Early-Earth-like chemistry.

49
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What is the Dragonfly mission?

A drone exploration of Titan's surface and chemistry.

50
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When is the Dragonfly mission scheduled to launch?

It is scheduled to launch in 2034.

51
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What evidence suggests Titan has a subsurface ocean?

gravity measurements by the Cassini spacecraft, which revealed unusual tidal effects and deformation patterns indicating a large, likely liquid, interior layer beneath the icy crust

52
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Where are geysers observed on Enceladus?

Near the south pole of Enceladus.

53
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What provides the heat source for Enceladus’s activity?

Resonance with Dione provides heat.

54
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How does resonance with Dione affect Enceladus?

It provides heat for Enceladus's geological activity.

55
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What phenomenon causes localized heating on Enceladus?

Localized heating results from observed heat exceeding expectations, known as 'shear localization'.

56
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What has been detected in the plumes of Enceladus?

Salt and organic molecules.

57
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What does the presence of salt in Enceladus’s plumes suggest?

It suggests a liquid saltwater ocean exists beneath the surface.

58
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What organic molecules have been found in Enceladus's plumes?

Methane, propane, acetylene, and formaldehyde.

59
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Why is Enceladus considered a good candidate for astrobiology?

Its subsurface ocean could be in contact with a rocky core, important for life-supporting chemistry.

60
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Who began the search for Planet X?

Percival Lowell in 1906.

61
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When was Pluto discovered?

Pluto was discovered in 1930.

62
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Who discovered Pluto?

Clyde Tombaugh.

63
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What assumption led to Pluto's discovery?

It was based on incorrect assumptions about Uranus' orbit.

64
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What is Pluto classified as today?

Pluto is classified as a 'dwarf planet'.

65
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How does Pluto’s radius compare to Triton’s?

Pluto's radius is 1153 km, similar to Triton's at 1353 km.

66
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What is Pluto’s approximate density?

Pluto's density is around 2.0 g/cm³.

67
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What is Pluto primarily composed of?

A mix of rock (50-70%) and ice.

68
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What moon of Pluto was discovered in 1978?

Charon.

69
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What two additional moons of Pluto were discovered in 2005?

Nix and Hydra.

70
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What surface variations were observed on Pluto before New Horizons?

Brightness and color variations.

71
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What causes Pluto’s reddish surface color?

Organic molecules formed from methane and ammonia ice exposed to UV.

72
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What are the three layers in Pluto’s internal structure?

Layer 1: Frozen nitrogen, Layer 2: Water ice, Layer 3: Rock and iron core.

73
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What provides internal heat to Pluto?

Radioactive decay of potassium, uranium, and thorium.

74
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What surface feature would Pluto have if no subsurface ocean ever existed?

An equatorial bulge and mostly extensional tectonic features.

75
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What surface feature would indicate the presence of a subsurface ocean on Pluto?

Mostly compressional surface features such as wrinkle ridges.

76
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When was the New Horizons spacecraft launched?

In 2006.

77
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When did New Horizons fly by Pluto?

In July 2015.

78
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What shape is Pluto’s overall structure?

Pluto is almost perfectly spherical.

79
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What does Pluto’s shape suggest about its interior?

It suggests a subsurface ocean may have existed or still exists.

80
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What is Sputnik Planum?

A vast frozen nitrogen sea on Pluto.

81
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What is Sputnik Planum composed of?

Frozen nitrogen.

82
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What atmospheric component dominates Pluto’s atmosphere?

Nitrogen.

83
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How was Pluto’s atmospheric thickness measured?

By light refraction during the flyby.

84
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What surface processes are believed to occur in Sputnik Planum?

Convection within soft nitrogen ice.

85
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What are the surface features of Charon?

Large canyon systems, grabens, and hemispheric differences.

86
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What do Charon’s canyon systems suggest about its crust?

Charon experienced a violent geological past, likely due to internal processes like the expansion of a once-liquid ocean or tectonic activity as its water-ice crust cooled and contracted

87
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What hemispheric differences are seen on Charon?

The southern hemisphere is smoother; the northern hemisphere is rugged.

88
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What evidence on Charon supports a past subsurface ocean?

Similarity to Pluto suggests a possible past subsurface ocean.

89
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Why was Pluto reclassified as a dwarf planet?

Due to the discovery of many similar-sized Kuiper Belt objects.

90
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What Kuiper Belt object is similar in size to Pluto?

Eris.

91
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What is the Planet Nine hypothesis?

It suggests a massive unseen planet is causing strange clustering of distant Kuiper Belt objects.

92
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What clues suggest the existence of Planet Nine?

Strange clustering and non-random orientations in the perihelion of distant Kuiper Belt objects.

93
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How massive is the hypothetical Planet Nine thought to be?

It is thought to be greater than 10 Earth masses.

94
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How far from the Sun might Planet Nine be located?

At approximately 700 AU from the Sun.

95
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How does volcanic activity affect planetary habitability?

Volcanism can create a stable atmosphere necessary for planetary habitability.

96
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What role does Mars’s cooling play in its atmospheric loss?

Decreased volcanic activity led to a diminished magnetic field, allowing solar wind to erode the atmosphere.

97
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What determines the rotation rate of gas giants like Jupiter?

The rate of spin of their magnetic field axes.

98
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What makes Saturn’s magnetic field unusual?

Its behavior is more complex than expected with no precise rotation rate.

99
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What two observations support the idea of an ocean beneath Europa?

A lightly-cratered surface and tidal heating due to orbital eccentricity.

100
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Why are hydrogen and helium absent from terrestrial planet atmospheres?

Their low mass allows them to escape the atmospheres.