A new approach to decipher the origin of the carbonaceous chondrite fission krypton and xenon

Details A new approach to decipher the origin of the carbonaceous chondrite fission krypton and xenon A new approach to decipher the origin of the carbonaceous chondrite fission krypton and xenon

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978e%26psl..39..358m&link_type=abstract

Earth and Planetary Science Letters, vol. 39, no. 3, May 1978, p. 358-362.

Computer Science

Carbonaceous Chondrites, Krypton, Meteoritic Composition, Nuclear Fission, Xenon, Fission Products, Solar System, Stellar Evolution, T Tauri Stars

Scientific paper

It is suggested that the carbonaceous chondrite fission krypton and xenon, as measured in the primitive meteorites, may have been produced by nuclear fission induced by CNO flare particles in the few-MeV/nucleon energy range on very heavy target elements such as Au, Hg, Tl, Pb, and Bi. It is speculatively proposed that the locale of this process has been the T-Tauri phase of our sun.

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