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Clayton’s results, published in a seminal 1973 paper, energized the emerging field of cosmochemistry, which uses chemistry as a way to learn not only about meteorite age, source and history but how the planets and bodies formed in the early solar system. Analyzing the isotopes in rock samples reveals information about the conditions under which that rock formed, and the oxygen-17 measurements showed that the meteorites formed by a very unusual chemical process or circumstance. What exactly those circumstances were, and their ramifications for our picture of the early solar system, are still hotly debated.
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mag(2011)
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Rapid Communications in Mass Spectrometryno. 6 (2010): 773-776
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