Jovian Planet Moons and Rings - PowerPoint PPT Presentation

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Jovian Planet Moons and Rings

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Moons are mostly made of ice, so quite soft and can be more active than similar ... thick, temporary cracks Colored areas mostly mineral rich ices Probable 100 km ... – PowerPoint PPT presentation

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Title: Jovian Planet Moons and Rings


1
Jovian Planet Moons and Rings
  • Each planet has multiple moons and seem like
    mini-solar systems
  • Moons are mostly made of ice, so quite soft and
    can be more active than similar sized rocky
    planets/moons
  • Rings are made of individual small particles,
    orbiting like micromoons

2
A Mini-Solar System
  • Many moons, 4 big ones found by Galileo, another
    12 over 350 years from the Earth
  • Dozens more by spacecraft imaging on
    fly-bys/orbits most are captured asteroids
  • Jupiter also has a narrow, faint ring system

3
JUPITER The Galilean Moons
  • Io and Europa -- smaller, rockier, differentiated
  • Ganymede and Callisto -- further, bigger and
    icier Ganymede is the biggest Moon in SS

4
Jupiter Surrounded by Moons
  • Named after lovers of Jupiter from mythology
    Galilean all have synchronous orbits
  • Almathea inside them (181,000 km from center
    260 km diameter) -- discovered in 1892 by Barnard
  • 4 even smaller moons found inside Galilean (found
    by Voyagers and early Galileo)
  • 4 moons around 11,000,000 km out e and i high
    captured asteroid(s) known from Earth
  • 4 more captured moons around 23,000,000 km out
    these have retrograde orbits.
  • A total of 63 known in 2009 -- largest number of
    confirmed moons

5
IO most active object in SS
  • a 422,000 km D 3640 km M 1.22 MMoon
  • Multicolored surface yellow, orange, red, brown,
    and white sulfur S compounds
  • Rocky mantle Fe/FeS core ? 3.5 g/cm3
  • Strong tidal flexures P 1.77d 1/2 P(Europa)
    1/4 P(Ganymede) ? forced heating from resonant
    orbit
  • Sulfur volcanoes blasting out particles Very
    smooth, young ( lt 1 Myr) surfaceflows Fills up
    Jupiter's plasma torus ionized S atoms.

6
Io and its Volcanoes
7
EUROPA Icy Oceanic?
  • a 671,000 km D 3130 km M
    0.65 Mmoon ? 3.04 g/cm3
  • Icy crust kms thick, temporary cracks Colored
    areas mostly mineral rich ices Probable 100 km
    thick ocean -- LIFE EXISTS(ED) THERE ????
  • Surface lt 100 Myr old new ice replacing old
  • Less heating by tidal flexure than Io, but still
    a good bit warmed up from resonant orbits

8
Europa cracked, oozy ice
Liquid water ?on surface?
9
GANYMEDE King of the Moons
  • a 1,070,000 km D 5270 km
  • M 2.02 MMoon
  • ? 1.93 g/cm3 ? very thick ice layer
  • Rocky mantle, Fe/FeS core Many craters, many
    old ones survive Grooved terrain ? plate
    tectonics at 3 Gy in the past
  • Only satellite with a magnetic field

10
Ganymede
11
CALLISTO Deadest of All Biggies
  • a 1,880,000 km D 4800 km M 1.46
    Mmoon ? 1.83 g/cm3 ? mixture
    of rock and ice
  • More craters, fewer faults, than Ganymede
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