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Formation of the Moon. By Brad Shaver. Previous Models. Fission Capture Binary Accretion . Fission Model. Idea was Earth spinning at high rate. Tossed material off surface. Problem is that the moon should be orbiting at earth’s equator!. Capture Model.

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formation of the moon

Formation of the Moon

By Brad Shaver

previous models
Previous Models
  • Fission
  • Capture
  • Binary Accretion
fission model
Fission Model
  • Idea was Earth spinning at high rate.
  • Tossed material off surface.

Problem is that the moon should be orbiting at earth’s equator!

capture model
Capture Model
  • Moon formed in different location
  • Captured by earth

However, moon and earth have same composition!

binary accretion model
Binary Accretion Model
  • Moon formed from remains of earth
  • Similar to planets forming from remains of stars

Problem is moon doesn’t have much metallic iron!

along comes apollo
Along comes Apollo
  • Lunar samples show same makeup as earth
    • Density of moon is roughly equal to earth’s mantle
  • Have very little volatile elements
    • Formed in high temperature
  • Oxygen isotopes similar to earth

So…

The moon must be from earth!

kona meeting
Kona meeting
  • 1984 meeting in Hawaii
    • Discussed other ideas for origin of moon
    • Impact model became popular
      • Explained high angular momentum
      • Protoplanets helped form this idea

-collided with each other in early solar system

impact model
Impact Model
  • Basic Idea
    • Collision with earth
      • Caused material to be thrown off
      • Reaccreted to form moon
impact model continued
Impact Model continued
  • Accretion caused magma oceans
      • Lunar samples showed evidence for this
      • Hot enough to get rid of volatile elements
moons interior
Moons Interior
  • Crust
      • 60-150km, mostly anorthite
      • Regolith 3-5m in maria, 10-20m in highlands
      • Mantle
          • around 100km, makes up most of moons interior
          • Core
              • Might be partially molten

The cause of the offset center of mass may be due to the crust being uneven

after cooling
After cooling
  • Maria began to form from impacts
      • Lunar samples suggest came from mantle
      • Usually 1-2 km thick and low viscosity
volcanism
Volcanism
  • Volcanoes also contributed to maria
      • Dome and cone
      • Viscosity low
      • Large concentration of cones in Marius hills complex
impact model for other bodies
Impact model for other bodies?
  • Yes
  • Mercury is mostly core (60%)
      • Density is equal to iron density
  • Venus and Uranus rotation
references
References
  • "Moon." Wikipedia, The Free Encyclopedia. 11 Nov 2008, 15:56 UTC. 13 Nov 2008 <http://en.wikipedia.org/w/index.php?title=Moon&oldid=251118218>.
  • Spudis, Paul D. "Moon." World Book Online Reference Center. 2004. World Book, Inc. (http://www.worldbookonline.com/wb/Article?id=ar370060.)