ASTRONOMY 1040


Class Notes #7

Chapter 8

Jupiter

  • known since ancient times
  • Named for the King of the Gods (but why?)
  • In appearance, Jupiter is slightly flattened due to its gaseous nature and high speed of rotation.
    • Jupiter is completely covered by clouds and has no solid surface.
    • Light zones and dark belts encircle the planet, giving it a striped appearance. the zones are areas of rising atmosphere, whereas the belts are falling atmosphere.
    • Numerous oval shaped cloud patterns can be seen, including the enormous Great Red Spot, which is something like an "anti-hurricane" that can be nearly three times the diameter of Earth. (Unlike earthly hurricanes, which are low pressure cells, the Great Red Spot is a highpressure cell.) It has faded considerably in recent years.
  • Jupiter is, on the average, 5.2 times the Earth's distance from the Sun.
  • Jupiter is huge, 11 times the diameter of Earth or about 143,000 km (roughly 88,000 miles)
  • In mass, it is 317 times the mass of Earth, or more that all the other planets combined.
  • In composition, it is really more like a star than a planet.
    • Composed mostly of Hydrogen and Helium
    • Thick gases get thicker the deeper you go, and pressure rise dramatically
    • At the visible surface of Jupiter -- the cloud tops -- the temperature is about 125 K or  235 d below zero  F.
    • At about 7000 km down, pressures have risen to 500,000 times that at the surface of Earth, and the temperature is 2000 K -- hotter than a blast furnace. Due to the pressure, hydrogen becomes liquid here.
    • At a depth of 14,000 km, pressure is 2 million times that at the surface of Earth, temperature is nearly that of the surface of the Sun (5000 K), and hyddrogen becomes "metallic"
    • At 60,000 km and 100 million atmospheres, Jupiter probably has a "small" core (still larger than the whole Earth) of rock, metals and hydrogen compounds. Temperature of the core is 20,000 K, more than 3 times that of the surface of the Sun!
  • Due to its internal heat, Jupiter radiates more energy into space than it receives from the Sun. Some of this energy goes into powering the complex weather patterns on the planet. Other energy is radiated away as radio waves and other electromagnetic energy. The planet also has an enormously strong magnetic field thought to be produced by free electrons accelerating in the metallic hydrogen interior.
  • Jupiter has a retinue of at least 63 natural satellites or "moons."  Except for Io, these are all icy worlds.
    • Four Moons are large enough to be seen with a small telescope of pair of binoculars
      • Io ("Eye-oh") is the closest large moon to Jupiter. About the size of Earth's Moon, Io is subject to great tidal forces from Jupiter. This heats and melts subsurface layers, forming volcanoes. Io is the first (and so far only) body in the Solar System  to show currently active volcanoes. "Fire and brimstone, thy name is Io." Neptune's Triton has what may be called "ice geysers," but that are not the same. Io's volcanic nature makes it an exception to the rule that most moons of outer planets are covered with ice, and fairly frequent flows of lava erase the evidence of impacts (it has virtually no impact craters visible.) There are a number of factors contributing to Io's volcanic activity, not the least of which is the enormous gravitational force of Jupiter, which exerts strong tidal forces on nearby Io. Other factors include gravitional tugs from other moons (especially Europa), possibly its own internal heat, and Io's elliptical orbit that strengthens the tidal flexing.
      • Europa is an ice-covered world slightly smaller than our Moon. Apparent movements in its icy crust point to a possible ocean of liquid water underneath. Europa is considered one of the best places in the Outer Solar System to look for life.
      • Ganymede is the largest planetary satellite in the Solar System, being larger than the planet Mercury. It has a complex and icy surface geology with strange features possibly related to a warm core (the possible evidence for which is the fact that it has a magnetic field). There is a slight chance of an ocean under the ice, but this is highly speculative.
      • Callisto is very slightly smaller than Mercury. It is an icy world largely covered with craters and some areas covered by a material darker than ice. Like Ganymede, Callisto may have a small magnetic field, possibly giving evidence of a slight internal heat source and/or a salty ocean beneath the crust -- but this is also highly speculative.
      • The at least 59 other moons are icy and small, with only a couple more than 100 kilometers in size, and most only a few kilometers across.
    • Some of the larger satellites ("moons") of Jupiter and the other Gas Giants are roughly spherical, which says that their gravity is strong enough to pull them into that shape. Smaller moons are irregular in shape because they do not have enough gravity to overcome the electromagnetic forces that bind them together.
    • Most moons of Jupiter and the other Outer Planets show many impact craters and in some cases evidence of crustal movement in cracks and fissures. Movement of ice is a major force in shaping the face of these worlds, and in some cases helps to erase the effects of previous changes. Jupiter's Io is an exception due to its volcanic surface.
  • Unknown until discovered by Voyager I in 1979, Jupiter has a faint, thin ring which could be composed of particles from Io's volcanic emissions.

·         Saturn

      • Much of what has been said about Jupiter applies to Saturn as well.
      • It is nearly twice as far from the Sun, at about 9.57 AU.
      • Saturn is about 121,000 km in diameter (about 75,000 miles)
      • It is about 95 times the mass of Earth. (It's density is about 70 percent that of water)
      • It's structure is similar to Jupiter's, but because it is considerably less dense, it likely has less metallic hydrogen.
      • It has a magnetic field, probably due to the motions of free electrons in the metallic hydrogen core, but it is much less than that of hydrogen
      • The Ring System, by far the most spectacular among the planets,is composed of ice fragments that range in size of microscopic to the size of small boulders. Recent evidence suggests that some may be larger, and that in some rings the particles are "clumped" together rather than evenly spread out.
      • Saturn currently has 35 named moons, with probably more small ones to be discovered.
        • Most are small, with only 5 larger than 1000 km in diameter
        • The largest is Titan, larger than Mercury and the second largest moon behind Ganymede
          • Titan has a nitrogen atmosphere with an atmospheric pressure 1.5 times that of Earth
          • Titan is covered with clouds, and may have an ocean of methane or ethane
          • It is thought that there may be some chance of life on Titan
        • Some small Saturnian Moons are close enough to the rings -- within the rings in some cases -- to exert a gravitational force on them, causing them to have gaps in places. Others cause the shapes of the outer rings to be warped or "braided."

·         Uranus

      • Uranus is about 19.1 AU from the Sun, nearly twice the distance of Saturn
      • Uranus is smaller than Jupiter or Saturn, at about 51,000 km (32,000 miles) in diameter
      • Uranus is only 14.5 times the mass of the Earth (It's density is about 1.27 times that of water)
      • Uranus likely has no metallic hydrogen, but water, ice and a small core of rock
      • Uranus' axis of rotation is tilted to the plane of its orbit, as if it were "laying down."
      • It has a magnetic field, oddly tilted to its rotation axis
      • It does not emit much energy into space, and likely does not have a strong source of internal heat
      • Uranus has at least 21 moons, 5 of which are 1000 km or more in diameter
      • Uranus also has a thin set of rings

·         Neptune

      • Neptune is very similar to Uranus in most respects
      • It is nearly 30 AU from the Sun, about 50 percent farther than Uranus
      • It is slightly smaller (49,500 km) and denser (1.64) than Uranus
      • Like Uranus, Neptune likely has no metallic hydrogen, but water, ice and a small core of rock
      • Also like Uranus, Neptune also has a magnetic field, oddly tilted to its rotation axis
      • Neptune has at least 13 satellites, all small except Triton, which is 2700 km in diameter
        • Triton has a very interesting geology and "ice volcanoes" or "ice geysers" and "cantaloupe terrain"
        • Icy Triton may bear a strong resemblance to Pluto

 

END

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