Lecture 17 Flashcards

1
Q

What is a Gas Giants

A

Relatively large planets that have deep atmospheres and have NO solid surfaces; have rings of particles around them, and many icy/rocky satellites

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2
Q

What is Jupiter’s atmosphere made of

A
  • 90% H2 and 10% He
  • little amounts of water,methane and ammonia
  • Clouds in jupiter are made of ammonia ice
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3
Q

Difference between Earth and Jupiter

A
  • Earth is composed of dense silicates while Jupiter is made up mostly of hydrogen and helium
  • Jupiters magnetic field is 20,000 times that of earth
  • Jupiter has a quicker period of rotation (9.9 hours)
  • Jupiter is also much colder than earth
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4
Q

Jupiter internal structure

A
  1. Atmosphere and Molecular Hydrogen Layer - beneath the atmosphere, there is a molecular hydrogen layer that extends to about 20,000 km.
  2. Metallic Hydrogen Layer
  3. Core - Jupiter has a volatile-rich core estimated to be 10-15 times the mass of Earth
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5
Q

Differences between Jupiter and Saturn

A
  1. Jupiters magnetic field is significantly stronger than Saturn (20,000 vs 0.4)
  2. They are composed of the same things in the atmosphere
  3. Jupiter is slightly warmer than Saturn
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6
Q

Saturns Atmosphere

A
  • 96% H2, 3% He, small amounts of Methane & Ammonia Clouds
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7
Q

What is the reason for Jupiters strong magnetic field (important)

A
  • Jupiter’s strong magnetic field is attributed to its Metallic Hydrogen layer, which extends from 30,000 to 40,000 km and acts as the source of the dynamo that generates the magnetic field
  • Other gas giants have a much smaller metallic hydrogen layer or they have dif internal structures (richer in ice and silicates)
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8
Q

Saturns internal structure

A
  • eddies and cyclones cause by heat released from the planets interior
    1. Atmosphere consists of H2 and He
    2. Molecular Hydrogen Layer: 30,000km thick composed of H2
    3. Metallic Hydrogen Layer: contains metallic H+
    4. Core: volatiles and silicates
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9
Q

Uranus compared to Jupiter

A
  • Uranus has a more complex composition than jupiter
  • Significantly weaker magnetic field than jupiter
  • Almost double the period of rotation of jupiter (uranus 17.2hr)
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10
Q

Uranus – Atmosphere & internal structure

A

Composition:
– 83% H2, 15% He, 2% CH4
- Internal Structure:
- rich in ice and silicates
- Core of volatiles and silicate rock

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11
Q

Uranus compared to Neptune

A
  • Both have a complex bulk composition
  • Same things make up the atmosphere
  • similar magnetic fields & temps
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12
Q

Neptune – Atmosphere & Internal Structure

A

Composition:
– 80% H2
– 18% He
– 1.5% CH4

  • Internal Struc: Higher density
  • Core of ice and silicate rock
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13
Q

How each planet gets their heat

A
  • Jupiter, Saturn have a greater internal heat than what they get from the sun
  • Uranus receives less heat from the Sun and its heat is not solar; it has more rocky components.
  • Neptune, despite being further from the Sun, generates more heat than it receives from the Sun. This heat is not solar and Neptune has the most rocky components among these planets.
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14
Q

Origins of gas Giants: Core Accretion Model

A
  • This model involves the accretion of rock-ice planetesimals to form a core that is 10 to 20 Earth masses, which takes about 1 million years (Ma).
  • The next step is the accretion of a massive gaseous envelope, which takes between 1 to 10 Ma.
  • The problem with this model is that the nebula was all gone by 10 Ma after the start of the solar system.
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15
Q

Origins of gas Giants: Disk Instability Model: (MORE LIKELY ONE)

A
  • This model involves the clumping of gas and dust in the disk.
  • There is a sudden gravitational collapse to form the planet, which takes only a few hundred or thousand years (within the first 1 Ma).
  • This model solves the problem of the nebula disappearing too quickly and is considered the most likely model for the formation of gas giants like Jupiter and Saturn
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