The Origin and Evolution of Chondritic Water

Details The Origin and Evolution of Chondritic Water The Origin and Evolution of Chondritic Water

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1869a&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1869

Computer Science

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Scientific paper

Bulk CM H abundances and isotopes are inversely correlated and both
correlate with alteration indices. The estimated initial water
composition (δD ≤ -450‰) shows that most formed in the
inner nebula, but ≤20% could have come from the outer nebula.

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