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High temperature condensates among meteorsIt is noted that two meteors which exhibited no lines of iron or sodium in their spectra have been tentatively attributed to aubrites in order to explain their lack of iron. It is shown, however, that no meteorites, including aubrites, have simultaneously low abundances of iron and sodium and that possible parent materials other than aubrites must be considered for the observed meteors. Other possible parent materials considered in this letter include melilite and diopside, two minerals containing both Ca and Mg but neither Fe nor Na. It is suggested that meteoroids rich in Ca and Mg but lacking Fe and Na might form a reservoir for the so-called 'lost' elements (Ca, Mg, Al, Ti, the lanthanides, and other refractory elements) which are depleted in ordinary and enstatite chondrites relative to cosmic abundances.
Document ID
19760033519
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wilkening, L. L.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
December 25, 1975
Publication Information
Publication: Nature
Volume: 258
Subject Category
Lunar And Planetary Exploration
Accession Number
76A16485
Funding Number(s)
CONTRACT_GRANT: NSG-7011
Distribution Limits
Public
Copyright
Other

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