Elements 112 to 119: Were They Present in Meteorites?

Details Elements 112 to 119: Were They Present in Meteorites? Elements 112 to 119: Were They Present in Meteorites?

May 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969sci...164..821a&link_type=abstract

Science, Volume 164, Issue 3881, pp. 821-823

Computer Science

38

Scientific paper

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.

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