Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...296l..17f&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 296, Sept. 1, 1985, p. L17-L20. Research supported
Astronomy and Astrophysics
Astrophysics
25
Carbonaceous Chondrites, Metallicity, Meteoritic Composition, Nuclear Fusion, Titanium Isotopes, Abundance, Allende Meteorite, Mass Spectroscopy, Pyroxenes, Solar System, Meteorites, Isotopes, Titanium 50, Enrichment, Carbonaceous Chondrites, Samples, Meteorite, Ion Probe, Anomalies, Murray, Inclusions, Hibonite, Contamination, Hypotheses, Formation, Abundance, Allende, Heterogeneity, Cv3 Chondrites, Cm2 Chondrites, Stony Meteorites
Scientific paper
The results of the first high mass resolution ion microprobe study of Ti isotopic compositions in individual refractory grains from primitive carbonaceous meteorites are reported. One hibonite from the Murray carbonaceous chondrite has a 10 percent excess of Ti-50, 25 times higher than the maximum value previously reported for bulk samples of refractory inclusions from carbonaceous chondrites. The variation of the Ti compositions between different hibonite grains, and among pyroxenes from a single Allende refractory inclusion, indicates isotopic inhomogeneities over small scale lengths in the solar nebula and emphasizes the importance of the analysis of small individual phases. This heterogeneity makes it unlikely that the isotopic anomalies were carried into the solar system in the gas phase.
Fahey Albert
Goswami Jitendra N.
McKeegan Kevin D.
Zinner Emst
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