The origin of volatile elements in the Earth-Moon system
Lars E Borg1, Gregory A Brennecka1, Thomas S Kruijer1,2
1Nuclear and Chemical Science Division, Lawrence Livermore National Laboratory, Livermore, CA 94550; borg5@llnl.gov brennecka2@llnl.gov kruijer1@llnl.gov.
Summary
Volatile elements in the Earth-Moon system were depleted before the Moon-forming Giant Impact. This suggests that the proto-Earth and impactor Theia inherited their volatile depletions from their solar system origins.
Area of Science:
- Planetary Science
- Geochemistry
- Cosmochemistry
Background:
- The origin of volatile elements like water in the Earth-Moon system is debated.
- Volatile loss during the Giant Impact is a major uncertainty.
- Rubidium-Strontium (Rb-Sr) isotope system tracks volatile element evolution.
Purpose of the Study:
- Constrain the timing of volatile element depletion in the Earth-Moon system.
- Investigate the role of the Giant Impact versus precursor inheritance.
- Determine the formation location of Earth and Theia.
Main Methods:
- Analyzing lunar highland rocks for 87Sr ingrowth.
- Utilizing the 87Rb to 87Sr decay chronometer.
- Comparing isotopic compositions to primitive meteorites.
Main Results:
- Lunar rocks crystallized ~4.35 billion years ago show minimal 87Sr ingrowth.
- Theia and proto-Earth were already volatile-depleted before accretion.
- Volatile depletions were inherited from the precursors.
Conclusions:
- The Giant Impact did not cause the Moon's volatile depletion.
- Precursor volatile element distributions were inherited by Earth and the Moon.
- Theia and proto-Earth likely formed in the inner solar system.
- The Giant Impact occurred late in solar system history.
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