A 15N-Poor Isotopic Composition for the Solar System As Shown by Genesis Solar Wind Samples

Details A 15N-Poor Isotopic Composition for the Solar System As Shown by Genesis Solar Wind Samples A 15N-Poor Isotopic Composition for the Solar System As Shown by Genesis Solar Wind Samples

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sci...332.1533m&link_type=abstract

Science, Volume 332, Issue 6037, pp. 1533- (2011).

Computer Science

15

Scientific paper

The Genesis mission sampled solar wind ions to document the elemental and isotopic compositions of the Sun and, by inference, of the protosolar nebula. Nitrogen was a key target element because the extent and origin of its isotopic variations in solar system materials remain unknown. Isotopic analysis of a Genesis Solar Wind Concentrator target material shows that implanted solar wind nitrogen has a 15N/14N ratio of 2.18 ± 0.02 × 10-3 (that is, ≈40% poorer in 15N relative to terrestrial atmosphere). The 15N/14N ratio of the protosolar nebula was 2.27 ± 0.03 × 10-3, which is the lowest 15N/14N ratio known for solar system objects. This result demonstrates the extreme nitrogen isotopic heterogeneity of the nascent solar system and accounts for the 15N-depleted components observed in solar system reservoirs.

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