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8.3: Gas Giant Planets and Select Satellites Overviews

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    Solar System’s Gas Giant Planets at a Glance

    Jupiter

    Image of Jupiter.
    Public Domain | Image courtesy of NASA.

    Characteristics

    Atmosphere

    • Hydrogen (H 2 ), Helium (H e ), Methane (CH 4 ), Ammonia (NH 3 ), Water (H 2 O)

    Rotation

    • Short rotation — 9.8 hours

    Revolution

    • Long revolution — 11.86 years

    Rings

    • One thin ring detected by the Voyager 2 spacecraft

    Magnetic Field

    • A very strong magnetic field; 20,000 times that of Earth’s

    Satellites

    • 67

    The Bottom Line…

    • Largest solar system planet
    • Great Red Spot
    • Gives off more heat than receives
    • Small, dense rocky core surrounded by H 2 and H e
    • Radio source
    • Aurora
    • Lightning and thunderstorms

    Saturn

    Image of Saturn.
    Public Domain | Image courtesy of NASA.

    Characteristics

    Atmosphere

    • Hydrogen (H 2 ), Helium (H e ), Methane (CH 4 ), Ammonia (NH 3 ), Water (H 2 O)

    Rotation

    • Short rotation — 10.6 hours

    Revolution

    • Long revolution — 29.46 years

    Rings

    • An intricate system of rings:
      • Spokes
      • Twisted F ring
      • Giant outer ring

    Magnetic Field

    • Yes

    Satellites

    • 62

    The Bottom Line…

    • Spectacular / intricate rings
    • Would float in water
    • Small, dense rocky core surrounded by H2 and He
    • Polar hexagon
    • Aurora
    • Lightning

    Uranus

    Image of Uranus.
    Public Domain | Image courtesy of NASA.

    Characteristics to Compare

    Atmosphere

    • Hydrogen (H 2 ), Helium (H e ), Methane (CH 4 ), Ammonia (NH 3 ), Water (H 2 O)

    Rotation

    • Short rotation — 17.3 hours retrograde (backwards)

    Revolution

    • Long revolution — 84.01 years

    Rings

    • An intricate system of rings:
      • 13 rings total; first 9 found via airborne telescope

    Magnetic Field

    • Yes, tilted about 45 o . Reason for tilt unknown

    Satellites

    • 27

    The Bottom Line…

    • 1st planet discovered with a telescope
    • Ice Giant
    • Very small rocky core
    • Little atmospheric activity
    • Looks like a billiard ball
    • Aurora
    • Neptune’s twin

    Neptune

    Image of Neptune.
    Public Domain | Image courtesy of NASA.

    Characteristics to Compare

    Atmosphere

    • Hydrogen (H 2 ), Helium (H e ), Methane (CH 4 ), Ammonia (NH 3 ), Water (H 2 O)

    Rotation

    • Short rotation — 16.1 hours

    Revolution

    • Long revolution — 164.8 years

    Rings

    • A partial, twisted series of 5 rings confirmed by the Voyager 2 spacecraft

    Magnetic Field

    • Yes, tilted about 45 o . Reason for tilt unknown

    Satellites

    • 14

    The Bottom Line…

    • 1st planet predicted position mathematically
    • Ice Giant
    • Very small rocky core
    • Great Dark Spot, Scooters
    • Looks like a billiard ball
    • Aurora
    • Uranus’ twin

    Consider this…

    We consider the Gas Giant planets to be huge, especially Jupiter. But when compared to other stellar systems, they are small – even “king of the planets,” Jupiter. Many of these hot Jupiters are much closer to their star than our Gas Giant planets and dwarf Jupiter in size. And it is theorized that some of these so-called “Super Jupiters” might be failed stars, that is, not quite enough mass for the nuclear fusion process. Nuclear fusion is where two particles collide at high speed and form a particle of a higher mass and a lot of energy.

    Image of A Super Jupiter orbiting very close to its star.
    Public Domain | Image courtesy of NASA.
    CC licensed content, Original

    8.3: Gas Giant Planets and Select Satellites Overviews is shared under a CC BY 4.0 license and was authored, remixed, and/or curated by LibreTexts.

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