Al-26 in stony meteorites with gas losses

Details Al-26 in stony meteorites with gas losses Al-26 in stony meteorites with gas losses

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977gecoa..41.1526h&link_type=abstract

Geochimica et Cosmochimica Acta, vol. 41, Oct. 1977, p. 1526-1529.

Computer Science

1

Aluminum 26, Helium Isotopes, Meteoritic Composition, Outgassing, Stony Meteorites, Chondrites, Cosmic Rays, Gas Evolution, Gaseous Diffusion, Nuclides, Particle Flux Density

Scientific paper

The Al-26 content of a group of stony meteorites with low levels of He-3 (implying outgassing caused by near approach to the sun) was analyzed in a test of the possible role of cosmic radiation in determining the radionuclide concentration of meteorites. The Al-26 contents of the meteorites with He-3 losses were found to be indistinguishable from the Al-26 contents of L- and H-chondrites. It is concluded that if the He-3 outgassing occurred near the sun, the flux of particles producing Al-26 must have been nearly normal, or the diffusion process must have taken place very rapidly.

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