PU-244 FISSION XENON AND PRIMORDIAL XENON IN LUNAR-SAMPLES AND METEORITES

Citation
Pk. Kuroda et Wa. Myers, PU-244 FISSION XENON AND PRIMORDIAL XENON IN LUNAR-SAMPLES AND METEORITES, Journal of radioanalytical and nuclear chemistry, 230(1-2), 1998, pp. 175-195
Citations number
75
Categorie Soggetti
Chemistry Inorganic & Nuclear","Chemistry Analytical","Nuclear Sciences & Tecnology
ISSN journal
02365731
Volume
230
Issue
1-2
Year of publication
1998
Pages
175 - 195
Database
ISI
SICI code
0236-5731(1998)230:1-2<175:PFXAPX>2.0.ZU;2-9
Abstract
Xenon found in lunar samples is a binary mixture of Pu-244 fission xen on and a trapped xenon, whose isotopic composition often shows a strik ing resemblance to that of TAKAOKA'S-1 primitive xenon. The decay prod uct of I-129 is conspicuously absent in lunar samples and this may be attributed to the facts that (a) the half-life of I-129 is much shorte r than that of Pu-244, and (b) the separation of xenon from plutonium may take place easily, since the former is a gaseous element, while th e latter is a refractory element. The separation of xenon from iodine may not take place easily, however,since the former is a gaseous eleme nt, while the latter is a volatile element. The isotopic compositions of the trapped xenon released from ordinary chondrites and achondrites resemble that of TAKAOKA's primitive xenon, which has been mass-fract ionated in such a manner that the heavier isotopes are systematically enriched relative to the lighter isotopes.