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The Gas Giants Astronomy 311 Professor Lee Carkner Lecture 16
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Gas Giant Basics The 4 largest planets of the solar system are the gas giants Does not include Pluto The gas giants have no real surface, all we see is atmosphere
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Missions to the Outer Planets 1972 Pioneer 10 -- Jupiter flyby 1973 Pioneer 11 -- Jupiter/Saturn flyby 1977 Voyager 1 -- Jupiter/Saturn flyby 1989 Galileo -- Jupiter orbiter and probe 1997 Cassini -- Saturn orbiter and Titan probe (Huygens) arrived 2004, currently taking data
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Voyager 2 Launched August 20, 1977 Only mission to Uranus or Neptune Most successful space probe ever launched Is still taking data on the edge of the solar system
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Voyager 2’s Grand Tour
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Gas Giant Facts Jupiter Diameter: 11.21 Mass: 317.83 Orbital Radius: 5.20 Saturn Diameter: 9.42 Mass: 95.16 Orbital Radius: 9.54 Uranus Diameter: 4.01 Mass: 14.50 Orbital Radius: 19.19 Neptune Diameter: 3.88 Mass: 17.20 Orbital Radius: 30.06 Numbers are relative to the Earth
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Orbits Orbital radii for the outer planets range from ~5-30 AU The outer planets cover a much larger region Gas giants don’t move much in the sky from our viewpoint
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Sizes of the Gas Giants Gas giants are all very large compared to the terrestrial planets Jupiter a little larger Uranus a little larger The gas giants contain 99% of the mass of the solar system (not including the Sun) Volume and mass go as radius cubed
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Densities The gas giants have very low densities Average density (kg/m 3 ) Jupiter: Saturn: Uranus: Neptune: For comparison Earth’s density is 5515 Saturn is less dense than water (it floats)
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Composition The gas giants have a low density because they are made up mostly of hydrogen and helium, the 2 lightest elements Hydrogen is the lightest and most abundant element in the universe (1 proton + 1 electron) Total composition ~5% heavier elements (methane, ammonia, water vapor etc.)
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Atmospheric Features Clouds small amounts of trace elements may produce the colors Bands adjacent bands move in opposite directions Storms some are very long lived (e.g. Great Red Spot)
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Odyssey to Jupiter Earth Jupiter at Conjunction Spacecraft Least Energy Orbit Jupiter at Opposition Spaceship Direct Boost
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Structure Degree of oblateness depends on mass distribution Models indicate that gas giants have a small, dense, rock-ice core Must have conducting liquid interiors
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Internal Structure of Jupiter
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Moons Number of satellites (larger than ~10 km) Jupiter -- Saturn -- Uranus -- Neptune -- Range in size from Ganymede (larger then Mercury) to small pieces of rock Including the very small ones, about 170 total
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Moon Properties Satellites tend to be composed of rock and ice Many have rocky cores and icy surfaces Io is very active and covered with volcanoes Europa may have a liquid water ocean
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Jupiter’s Satellites
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Saturn’s Satellites
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Rings All of the gas giants have rings of small particles The rings of the other planets are made of smaller darker particles and were only discovered by spacecraft This is the region where the tidal force from the planet is greater than the gravitational force holding the object together
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Differences Between the Gas Giants Uranus and Neptune are smaller, cooler and have less distinct cloud features
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Next Time Read 11.1-11.4, 11.6
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Summary Size: ~4-11 times Earth diameter Mass: ~15-318 Earth masses Composition: mostly hydrogen and helium Atmosphere: clouds of methane and ammonia also have large, long-lived storm systems and oppositely moving bands
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Summary: The Jovian Systems The gas giants have extensive satellite systems Many moons have icy exteriors with rocky cores Some are very large (~size of Earth’s Moon) All of the outer planets (not just Saturn have ring systems) rings composed of small particles Ring properties different for each planet
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