Other
Scientific paper
May 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983e%26psl..63..223n&link_type=abstract
Earth and Planetary Science Letters (ISSN 0012-821X), vol. 63, no. 2, May 1983, p. 223-228.
Other
23
Extraterrestrial Matter, Iron Meteorites, Manganese Isotopes, Marine Chemistry, Spherules, Stony Meteorites, Chemical Composition, Cosmic Rays, Neutron Activation Analysis, Ocean Bottom, Pacific Ocean
Scientific paper
Cosmic-ray-produced Mn-53 (half-life, 3.7 x 10 to the 6th yr) is measured in individual and groups of deep-sea iron and stony spherules by highly sensitive neutron activation analysis. The activities found are less than 20 dpm Mn-53/kg Fe (10 to the -5th-10 to the -6th dpm Mn-53/sample) in iron spherules, with the exception of one iron spherule, whose activity is 241 + or - 73 dpm Mn-53/kg Fe. It is believed that these low activities may indicate evaporative loss of Mn-53 caused by heating in the earth's atmosphere. On the other hand, all the stony spherules are found to contain 200-260 dpm Mn-53/kg Fe, which is similar to chondritic values. It is pointed out that these spherules may be ablation debris from large objects.
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