A Record of Solar System Scale Variation in Oxygen Isotopes at the Microscale: Cosmochemical Origins of CAIs and Their Wark-lovering Rims

Details A Record of Solar System Scale Variation in Oxygen Isotopes at the Microscale: Cosmochemical Origins of CAIs and Their Wark-lovering Rims A Record of Solar System Scale Variation in Oxygen Isotopes at the Microscale: Cosmochemical Origins of CAIs and Their Wark-lovering Rims

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1540s&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1540

Computer Science

Scientific paper

We measured O isotope variations in Allende CAI A37 and its surrounding
rim, using the NanoSIMS. At the μm scale, both the CAI and rim
exhibit significant variation in delta 17O that encompasses the range
observed for all solids in the solar system.

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