Xenon and other noble gases in shergottites

We have determined the isotopic composition of the xenon component trapped in EETA 79001 lithologies B and C, which we refer to as SPB-xenon. SPB-xenon is isotopically distinct from known xenon reservoirs, but differs in regular fashion. Normalized to ¹³²Xe, the light isotope ratios are indistinguishable from air, the ¹²⁹Xe/¹³²Xe ratio is about 2.4, and ¹³⁴Xe and ¹³⁶Xe are enhanced relative to the terrestrial atmosphere or AVCC. The apparent heavy-isotope enrichments are not generated by in situ fission and there is no spectral evidence for the presence of ²⁴⁴Pu fission xenon. However, the xenon composition does match that of fractionated AVCC except at ¹²⁹Xe, and consequently may be derived from or related to that component. ALHA 77005, Shergotty and EETA 79001 lithology A also have enhanced ¹²⁹Xe/¹³²Xe ratios in most temperature steps, and are seemingly consistent with varying mixtures of SPB-xenon and terrestrial xenon. Our results for neon and argon in EETA 79001 confirm earlier results on the exposure ages. We have also verified that the trapped ³⁸Ar/³⁶Ar ratio in lithology C is apparently substantially different from the terrestrial or meteoritic value. Krypton in EETA 79001,C is more fractionated with respect to AVCC than is terrestrial krypton and in the opposite direction as xenon. EETA 79001,C contains excess ⁸⁰Kr (and perhaps ⁸²Kr and ¹²⁸Xe), presumably from neutron capture on bromine and iodine, but these neutron captures do not appear to have occurred by in situ processes.