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Beryllium-10 in Australasian tektites - Evidence for a sedimentary precursorEach of seven Australasian tektites contains about 100 micron atoms of beryllium-10 (half-life, 1.53 million years) per gram. Cosmic-ray bombardment of the australites cannot have produced the measured amounts of beryllium-10 either at the earth's surface or in space. The beryllium-10 contents of these australites are consistent with a sedimentary precursor that adsorbed from precipitation beryllium-10 produced in the atmosphere. The sediments must have spent several thousand years at the earth's surface within a few million years of the tektite-producing event.
Document ID
19830030848
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pal, D. K.
(Rutgers Univ. New Brunswick, NJ, United States)
Moniot, R. K.
(Rutgers Univ. New Brunswick, NJ, United States)
Kruse, T. H.
(Rutgers Univ. New Brunswick, NJ, United States)
Herzog, G. F.
(Rutgers University New Brunswick, NJ, United States)
Tuniz, C.
(Rutgers University New Brunswick, NJ; Trieste, Universita, Trieste, Italy)
Date Acquired
August 11, 2013
Publication Date
November 19, 1982
Publication Information
Publication: Science
Volume: 218
Subject Category
Lunar And Planetary Exploration
Accession Number
83A12066
Funding Number(s)
CONTRACT_GRANT: NAGW-142
Distribution Limits
Public
Copyright
Other

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