Chapter 14 Flashcards

(34 cards)

1
Q

What are Jovian planets?

A

Large, low-density planets composed mostly of gas and/or ice, including Jupiter, Saturn, Uranus, and Neptune.

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2
Q

What is the difference between gas giants and ice giants?

A

Gas giants (Jupiter, Saturn) are mostly hydrogen and helium, while ice giants (Uranus, Neptune) contain more water, ammonia, and methane ices.

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3
Q

What are the general characteristics of Jovian planets?

A

Thick atmospheres, no solid surface, many moons, ring systems, and strong magnetic fields.

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4
Q

What is the internal structure of Jovian planets?

A

A dense core surrounded by layers of hydrogen, helium, and/or ices, with no solid surface.

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5
Q

Why do Jovian planets have strong magnetic fields?

A

Due to electrically conducting materials (like metallic hydrogen) and rapid rotation creating a dynamo effect.

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6
Q

What is unique about Jupiter’s interior?

A

It contains liquid metallic hydrogen that generates a very strong magnetic field.

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7
Q

What causes Jupiter to emit more energy than it receives?

A

Leftover heat from its formation (gravitational contraction).

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8
Q

What are Jupiter’s belts and zones?

A

Alternating bands of clouds caused by atmospheric circulation.

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9
Q

What is the Great Red Spot?

A

A giant, long-lasting storm in Jupiter’s atmosphere.

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10
Q

What are the main cloud layers on Jupiter?

A

Ammonia (top), ammonium hydrosulfide (middle), and water (lower).

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11
Q

What is Jupiter’s magnetosphere?

A

; A huge region dominated by Jupiter’s magnetic field that interacts with solar wind and produces auroras.

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12
Q

What are Jupiter’s rings like?

A

Faint, dark rings made of small rocky particles.

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13
Q

What causes Io’s volcanic activity?

A

Tidal heating from gravitational interactions with Jupiter and other moons.

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14
Q

Why is Europa considered a candidate for life?

A

It likely has a subsurface liquid water ocean beneath an icy crust.

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15
Q

What is special about Ganymede?

A

It is the largest moon in the solar system.

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16
Q

What is Callisto like?

A

Heavily cratered and geologically inactive, indicating an old surface.

17
Q

What is unusual about Saturn’s density?

A

It is less dense than water.

18
Q

What are Saturn’s rings made of?

A

Billions of ice particles with some rock and dust.

19
Q

What are shepherd moons?

A

Small moons that maintain and shape planetary rings through gravity.

20
Q

Why are planetary rings not permanent?

A

They gradually disperse and must be replenished by collisions or other processes.

21
Q

What is unique about Titan?

A

It has a thick nitrogen atmosphere and methane exists as liquid, gas, and solid.

22
Q

What is special about Enceladus?

A

It has cryovolcanoes that eject water vapor and feed Saturn’s E-ring.

23
Q

Why does Uranus appear blue-green?

A

Methane in its atmosphere absorbs red light.

24
Q

What is unusual about Uranus’s rotation?

A

It is tilted about 98° and rotates on its side.

25
How does Uranus’s energy output compare to what it receives?
It emits about the same energy it receives from the Sun.
26
What is notable about Neptune’s atmosphere?
It is very active with storms like the Great Dark Spot and has the fastest winds in the solar system.
27
What is unique about Triton?
It orbits Neptune in a retrograde direction and was likely captured.
28
What are dwarf planets?
Objects that orbit the Sun and are spherical but have not cleared their orbital region.
28
What is the Roche limit?
The distance within which tidal forces prevent material from forming a moon, leading to ring formation instead.
29
What are key characteristics of Pluto?
Small, icy, eccentric orbit, thin atmosphere (N₂, CO, CH₄), and a large moon (Charon).
30
hat is the Kuiper Belt?
A region beyond Neptune containing icy bodies and dwarf planets like Pluto.
31
What is the Kelvin–Helmholtz mechanism?
A process where a Jovian planet slowly contracts under gravity, releasing heat and causing it to emit more energy than it receives from the Sun.
32
How do Uranus and Neptune differ in internal energy and atmospheric activity?
Uranus emits about the same energy it receives and has a less active atmosphere, while Neptune emits more energy than it receives and has a very active atmosphere with strong winds and storms.
33
What determines whether rings or moons form around a planet?
Inside the Roche limit tidal forces prevent material from forming moons, creating rings, while outside the Roche limit material can clump together to form moons.