Origin of xenon in carbonaceous chondrites

Physics

Scientific paper

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Carbonaceous Chondrites, Meteoritic Composition, Xenon, Mixtures, Plutonium 244, Ternary Systems

Scientific paper

Various existing hypotheses on the origin of xenon in carbonaceous chondrites are reviewed. A common drawback of all the hypotheses is the use of concepts on physical and cosmic processes, the nature and even existence of which are not clear. A new interpretation is proposed which, based exclusively on well-established experimental data, does not require recourse to concepts such as the presence of superheavy elements in carbonaceous chondrites, and where the answer is simply the mixing of spallogenic xenon with the spontaneous fission product Pu-244.

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