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Astronomy 171
Solar System Astronomy
Prof. Paul Martini

Lecture 29: The Moon


Key Ideas:

Surface of the Moon:
Old, heavily cratered highlands
Younger, darker Maria
Thick regolith of pulverized rock
Interior of the Moon
Crust and Mantle, but no Core(?)
No magnetic field
Origin of the Moon


Moon Rocks

Our most detailed knowledge of the Moon comes from ~382 kg of samples returned by 9 space missions:
United States:
6 Apollo Landings (Apollo 11-17) 1969-1972
12 astronauts visited maria and highlands
Soviet Union:
3 Luna robotic missions (1970, 1972, 1976)
returned samples by robotic capsule


Regolith

Layer of dust and fragmented rock
Product of repeated meteor impacts
Covers the surfaces of most moons and astroids in the Solar System
Lunar Regolith
Single-mineral grains and rock fragments
Impact Breccias: heat-fused grains and rocks
2-8 km thick in Maria
More than 15 km thick in the Highlands


Lunar History

The Moon's surface was shaped by impacts
Maria:
Younger (3.1-3.8 Gyr) and lightly cratered
Formed after the epoch of heavy bombardment
Highlands
Older (3.8-4.0 Gyr) and heavily cratered
Solidified ~4.3 Gyr ago, before which time the Moon was molten


Lunar Maria

Youngest Moon Terrains
Dark basalts rich in iron and magnesium
No water or hydrated minerals
10x more Titanium than Earth rocks
Magma flows from deep crust fractures
Caused by asteroid impacts
Ages of 3.1 to 3.8 Gyr


Cratered Highlands

Oldest Moon Terrains
Rocks pulverized by impacts
Older than the Maria (3.8 to 4.0 Gyr)
Marks the end of an intense period of bombardment that started 4.6 Gyr ago
Unusual mineral content
The Moon was molten 4.35 Gyr ago!


Is there a Lunar Core?

The Moon has no global magnetic field now
Doesn't have a molten core like the Earth
Did it have a core in the past?
"Fossil" magnetism in very old Moon rocks
Means they cooled in a strong magnetic field
The Moon had a molten core and magnetic field 3.6 to 3.8 Gyr ago, but it does not have one now.


Origin of the Moon

Moon origin theries must explain these facts:
Moon has much less iron than the Earth
Moon lacks water and other "volatiles"
Moon rocks most resemble the Earth's mantle
Identical proportions of Oxygen isotopes in Earth and Moon rocks (different from meteorites)
Four formation models have been proposed
All are testable with observations


Theories of Moon Formation

Co-Formation
Earth and Moon formed together in place
Cannot explain the lack of iron and volatiles
Capture
Earth gravitationally captured the Moon
Cannot explain lack of iron and volatiles, or the identical oxygen isotope ratios
Also hard to do (but not a theory-killer)
Fission:
Moon split off from a fast-spinning proto-Earth
Composition issues OK except the volatiles
Also hard to do
Giant Impact:
Proto-Earth hit by a Mars-sized body
Moon formed from the debris
Currently the favored theory (!)


Giant Impact Theory

The impact theory has many strong points
The impactor's iron would have been in its core, and so sunk into the Earth's mantle
A molten post-impact Moon would have boiled off all of its volatiles
Moon formed of mostly Earth's mantle debris, explaining the compositional similarities
Still questions, but it does the best so far.


See A Note about Graphics to learn why some of the graphics shown in the lectures are not reproduced with these notes.

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Updated: 2007 February 10 Copyright © Paul Martini All Rights Reserved.