Be-B Isotope Systematics in CV and CM Hibonites: Implications for Solar Energetic Particle Production of Short-lived Nuclides in Early Solar System

Details Be-B Isotope Systematics in CV and CM Hibonites: Implications for Solar Energetic Particle Production of Short-lived Nuclides in Early Solar System Be-B Isotope Systematics in CV and CM Hibonites: Implications for Solar Energetic Particle Production of Short-lived Nuclides in Early Solar System

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1303m&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1303

Physics

11

Scientific paper

Presence of radiogenic 10B in HAL hibonite with extremely low initial
26Al/27Al ratio of ~5x10**-8 and in CM hibonites devoid of radiogenic
26Mg conclusively establish that the source of 10Be present in early
solar system didnot contribute significant amount of 26Al, 41Ca and
53Mn.

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