The Extinct Radionuclide Timescale of the Early Solar System

Details The Extinct Radionuclide Timescale of the Early Solar System The Extinct Radionuclide Timescale of the Early Solar System

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ssrv...92..123g&link_type=abstract

Space Science Reviews, v. 92, Issue 1/2, p. 123-132 (2000).

Computer Science

7

Isotope Geochemistry, Meteorites, Extinct Radionuclides, Solar System Chronology

Scientific paper

The tendency of iodine to be mobilised during secondary processing is reflected both in the presence of 129XeXS in secondary minerals and in the bulk 129XeXS/I ratios in meteorites. Comparison of absolute ages derived through calibration of chronometers based on 129Xe, 53Mn and 26Al against the Pb-Pb system yields a plausible timescale for the early solar system. In this system, the earliest chondrule ages are most readily interpreted as representing formation after the beginning of parent body processing.

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