Section 5. Giant planets Flashcards

(36 cards)

1
Q

What are the Gas giants?

A

Jupiter and Saturn
Radius and mass dominated by H + He gas

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2
Q

What are the ice giants?

A

Neptune and Uranus
Less gas, higher proportions of common ices

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3
Q

What is the equation of state for the giant planets?

A

P~Kρ2

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4
Q

What is the density equation for the giant planets?

A

ρ(r)=ρcsin(kr)/kr
Where k=sqrt(2πG/K)

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5
Q

What is the equation for the central density?

A

ρc=πM/4R3

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6
Q

What is the expected composition of the Gas giants?

A

Rocky/icy core then metallic hydrogen

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7
Q

Why do the Gas giants have global convection?

A

Bonding pattern extends into deep interior

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8
Q

Why do the Gas giants have strong magnetic fields?

A

Convection plus rotation plus conducting interior creates a magnetic dynamo

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9
Q

Why are the Gas giants oblate?

A

They rotate rapidly (< 0.5 days)

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10
Q

What do the magnetic fields of the Gas giants cause?

A

Aurorae at poles and radio emission via cyclotron/synchrotron emission by low/high energy electrons orbiting magnetic field lines

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11
Q

Why do the Gas giants have a very large magnetosphere?

A

Strong magnetic moment and lower solar wind flux

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12
Q

What is the equation for magnetic energy density?

A

uB=B20

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13
Q

What is the magnetic field for a dipole?

A

B(r)=μ0μ/2πr3

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14
Q

What is the K.E. density of the solar wind?

A

uW=1/2 ρWvW2

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15
Q

How do we find the radius of the magnetosphere?

A

Equate the magnetic energy density with the kinetic energy density of the solar wind

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16
Q

How does the radius of the magnetosphere scale?

A

Rm α (μa)1/3

17
Q

How do the magnetic moments of Neptune and Uranus compare to Earth?

A

50 and 25 times as large due to ionised cores at extreme pressures

18
Q

What is the source of internal heat for Jupiter?

A

Can be heat from grav pot energy left over from formation

19
Q

What is the source of internal heat for Saturn (and Jupiter)?

A

Ongoing differentiation from He rain out, releasing grav pot energy

20
Q

What is the source of internal heat for Neptune?

A

Ongoing differentiation of metals/rocks

21
Q

What is the description of the atmosphere of Jupiter?

A

Bright zones via reflective clouds of ice and dark belts

22
Q

What is the origin of the great red spot for Jupiter?

A

It is a storm at shearing boundary

23
Q

What is the description of the atmosphere of Saturn?

A

Similar bonding pattern to Jupiter, but muted due to clouds forming deeper in the colder atmosphere

24
Q

What is the description of the atmosphere of Neptune?

A

Colder with ice clouds deeper and bonding more muted

25
Why is the colour of Neptune blue?
Enhance methane abundance (CH4 absorbs in red optical light)
26
What is the description of the atmosphere of Uranus?
Very faint bonding Strong white clouds
27
How many moons does Jupiter have?
4
28
Why does Jupiter lack volatiles?
Tidal heating evaporates volatiles
29
What is the description of Io?
Rocky, volcanic with young surface
30
What is the description of Europa?
Rocky core and young icy surface
31
What is the description of Ganymede and Callisto?
Mass dominated by ice Older cratered surfaces
32
What is the description of Titan?
Thick nitrogen atmosphere Liquid methane rivers and lakes
33
What is the spin obliquity of Uranus?
98 degrees
34
What is the description of Titan?
Dwarf planet Has a retrograde orbit
35
What is the radius for the rings of Saturn?
aR=2.2 RP
36
What is the explanation for the rings of Saturn?
Tidally disrupted icy moon that migrated into its Roche limit