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Chapter 9: The Outer Planets

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Formed from rock, iron and ices (water, ammonia and methane) ... Inner liquid core (rocks, iron and ices) about same size as Jupiter ... – PowerPoint PPT presentation

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Title: Chapter 9: The Outer Planets


1
Chapter 9 The Outer Planets
  • Dr. Michelle Arnold
  • October 14, 2009

2
Jupiter
  • Formed after the terrestrial planets
  • More dust to collect!
  • Formed from rock, iron and ices (water, ammonia
    and methane)
  • Collected a primary (hydrogen) atmosphere from
    the accretion disk
  • Kept its primary atmosphere
  • Larger gravity of the planet due to larger mass
  • Weaker solar winds, further from the Sun
  • Jupiters composition is very similar to the
    Suns (mostly hydrogen)
  • Not large enough for the hydrogen to ignite and
    form a star

3
Jupiter cont.
  • Most likely no solid portion
  • Hydrogen atmosphere
  • Liquid metallic hydrogen sea
  • More dense liquid core
  • Strong magnetic field
  • Metallic hydrogen and rotates once every 10 h!
  • 20 000x greater than Earths
  • Great red spot
  • Large storm on Jupiter
  • Galileo first saw with his telescope

4
Jupiter cont.
5
Jupiter cont.
6
Jupiter cont.
  • Jupiters ring
  • Image from Voyager

7
Jupiter cont.
  • Many moons (63?)
  • Galilean moons 4 largest
  • Io active volcanoes
  • Tidal forces from Jupiter and Europa
  • Europa ice, possible water (and life?) below
  • Ganymede big ice rock!
  • Callisto big ice rock

8
Saturn
  • Formed similar to Jupiter
  • Saturn formed after Jupiter, and the solar winds
    had already blown away some of the hydrogen gas
    in the disk before Saturn collected it
  • Inner liquid core (rocks, iron and ices) about
    same size as Jupiter
  • Liquid metallic hydrogen and gaseous hydrogen
    atmospheres are smaller than Jupiter
  • Strong magnetic field

9
Saturn cont.
  • Density 0.7 g/cm3
  • It would float in water!

10
Saturn cont.
  • Rings
  • Particles of dust and ice
  • Most likely remains of a recently destroyed moon,
    comet or asteroid
  • All four giant planets have rings, Saturns most
    visible
  • Rings are thin, disks

11
Saturn cont.
12
Saturn cont.
13
Saturn cont.
  • Many moons
  • Enceladus Cassini mission (arrived in 2004) has
    found that Enceladus has a surface of water ice
  • Deformations indicate that the ice may be resting
    on a liquid interior
  • Titan largest moon
  • Voyager found its thick atmosphere is mostly
    nitrogen, with sig. amounts of methane (carbon!)
  • Cassini sent the Huygens probe to surface and
    takes radio photoes of the surface from above
  • Surface has methane and ethane lakes!

14
Titans Surface
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