A general solution for the puzzle of the xenon.

Kuroda, P. Κ.

doi:10.2343/geochemj.13.23

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1979

1986

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“…The initial ratio of 26A1 to 27A1 can be cal XENON ISOTOPE ANOMALIES According to KURODA (1971KURODA ( , 1975KURODA ( , 1976KURODA ( , 1979 and KURODA et al (1974KURODA et al ( , 1975, the difference in the isotopic compositions of xenon in the atmosphere and the carbonaceous chon drites can be attributed to a combined effect of (a) mass fractionation, (b) neutron caputre and (c) cosmic-ray irradiation processes which took place in the early solar system. The amount of cosmic-ray-produced 126Xe in car bonaceous chondrites can be calculated from the equations …”

Section: Introductionmentioning

confidence: 99%

Isotopic anomalies in the early solar system.

Kuroda

1979

Geochem. J.

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U.S.A.Isotopic anomalies observed in meteorites for 0, Mg, Ca, Xe, Ba, Nd and U can be attributed to a combined effect of mass fractionation, neutron capture and cosmic-ray irradiation processes which took place prior to and during the formation of the solar system. The total cosmic-ray neutron flux (time integrated) appears to have been such that the isotopic compositions of a number of elements were altered appreciably.INTRODUCTION N(R Ro t) = 2 X 10-12 f t RI (1),

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