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Large negative Ti-50 anomalies in refractory inclusions from the Murchison carbonaceous chondrite - Evidence for incomplete mixing of neutron-rich supernova ejecta into the solar systemAn ion microprobe was used to measure Ti-50 variations in hibonite-rich inclusions from the Murchison chondrite. Both deficits and excesses of the isotope were found, depending on the inclusion being scanned. The anomalies were not correlated with the mineralogy, chemical composition, other isotopic anomalies of Ti, etc. The lack of correlations indicates that the cosmic chemical memory model (Clayton, 1981) cannot explain the observed variations. The Ti-50 concentrations may have originated when a supernova explosion triggered the collapse of a molecular cloud that formed the solar system. The solar system Ti-50 anomalies were from the cloud, not the progenitor star.
Document ID
19870044565
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hinton, Richard W.
(Chicago Univ. Chicago, IL, United States)
Davis, Andrew M.
(Chicago Univ. Chicago, IL, United States)
Scatena-Wachel, Debra E.
(Chicago, University IL, United States)
Date Acquired
August 13, 2013
Publication Date
February 1, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 313
ISSN: 0004-637X
Subject Category
Lunar And Planetary Exploration
Accession Number
87A31839
Funding Number(s)
CONTRACT_GRANT: NAG9-51
CONTRACT_GRANT: NAG9-111
Distribution Limits
Public
Copyright
Other

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