The isotopic composition of xenon has been determined in samples of the Navajo C-1 well gas, Wildcat Field, New Mexico. Our results indicate that xenon in the Navajo well gas contains radiogenic
129Xe and fissiogenic
131-136Xe. The fission yields across heavy xenon isotopes,
131-136Xe, match those reported for the spontaneous fission of
238U; the spontaneous fission of extinct
244Pu accounts for no more than 6% of the excess
136Xe in this well gas. Based on the high value of the ratio of radiogenic
129Xe to CO
2 in this gas, we suggest that most this decay product of extinct
129I may have been introduced in a carrier gas of primordial, abiogenic hydrocarbons. It is shown that values of the ratio of radiogenic
129Xe to
244Pu-derived
136Xe in this well gas, in air, and in other terrestrial samples are consistent with a very simple and straight-forward chronology of events in the early solar system that is also compatible with the I-Xe and Pu-Xe record of meteorites.
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