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Silicate spherules from deep-sea sediments - Confirmation of extraterrestrial originSilicate spherules larger than 100 microns were extracted from 100 kg of box core samples of Pacific red clay taken in the mid-Pacific at a depth of 5 km, and the concentration of nonvolatile trace elements was determined for three spheres. One of the spheres shows excellent resemblance to C1 chondrite nonvolatile trace-element abundance patterns, and the relative abundances of the other two spheres are also very similar to those of C1 chondrites. One of these two spheres is depleted in Ir and Ru, while the other is depleted for Ni and Cr; possible explanations for the depletions are considered. Since the elemental abundances of the third sphere match the abundances of C1 chondrites, it is suggested that this sphere must be of extraterrestrial origin.
Document ID
19780067315
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ganapathy, R.
(J. T. Baker Chemical Co. Phillipsburg, N.J., United States)
Brownlee, D. E.
(California Institute of Technology Pasadena, Calif., United States)
Hodge, P. W.
(Washington, University Seattle, Wash., United States)
Date Acquired
August 9, 2013
Publication Date
September 22, 1978
Publication Information
Publication: Science
Volume: 201
Subject Category
Lunar And Planetary Exploration
Accession Number
78A51224
Funding Number(s)
CONTRACT_GRANT: NSG-9052
Distribution Limits
Public
Copyright
Other

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