Tellurium-H in interstellar diamonds

Details Tellurium-H in interstellar diamonds Tellurium-H in interstellar diamonds

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1163r&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 163.

Computer Science

2

Interstellar Matter, Diamonds, Tellurium, Allende Meteorite, Meteoritic Composition, Xenon Isotopes, Mass Spectroscopy, Hydrogen

Scientific paper

Analyses of interstellar diamond separates from the Allende meteorite indicate the presence of a Te component consisting essentially of Te-128 and Te-130 only. The composition of this 'Te-H' is not compatible with the predictions of the neutron burst model devised to explain the Xe-H pattern, but is consistent with the basic predictions from the recently suggested timescale model (although the Xe-128/Xe-130 ratio is found to be somewhat higher than predicted). A three-isotope diagram is presented of delta(Te-125/Te-128) vs delta(Te-124/Te-128); the data points fall on a mixing line joining approximately normal Te with a component that contains virtually no Te-124 and Te-125.

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