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- W2056332308 abstract "Chondrites contain a small fission xenon component of unexplained origin. Evidence on the geochemical behavior of this component suggests that it was not derived from an actinide element (Z = 89 to 103), or from a transition metal between Z = 104 and 111, but from a more volatile progenitor. The most likely candidates are the superheavy elements between Z = 112 and 119, whose lighter congeners (mercury, tellurium, lead, and the like) are known to be strongly fractionated in meteorites." @default.
- W2056332308 created "2016-06-24" @default.
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- W2056332308 date "1969-05-16" @default.
- W2056332308 modified "2023-10-14" @default.
- W2056332308 title "Elements 112 to 119: Were They Present in Meteorites?" @default.
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- W2056332308 doi "https://doi.org/10.1126/science.164.3881.821" @default.
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