Publication Date:
2019-07-13
Description:
The process responsible for the mass independent oxygen isotope variation observed in Solar System materials remains poorly understood. While self-shielding of CO, either in the early solar nebula, or precursor molecular cloud, appears to be a viable mechanism, alternative models have also been proposed.
Keywords:
Astrophysics; Lunar and Planetary Science and Exploration
Type:
JSC-CN-35141
,
Lunar and Planetary Science Conference; Mar 21, 2016 - Mar 25, 2016; The Woodlands, TX; United States
Format:
application/pdf
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