1 . 06 Oxygen Isotopes in Meteorites

@inproceedings{Clayton200410,
  title={1 . 06 Oxygen Isotopes in Meteorites},
  author={Robert N. Clayton},
  year={2004}
}
Oxygen isotope abundance variations in meteorites are very useful in elucidating chemical and physical processes that occurred during the formation of the solar system (Clayton, 1993). On Earth, the mean abundances of the three stable isotopes are O: 99.76%, O: 0.039%, and O: 0.202%. It is conventional to express variations in abundances of the isotopes in terms of isotopic ratios, relative to an arbitrary standard, called SMOW (for standard mean ocean water), as follows: 
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