Australasian microtektites in a substrate: A new constraint on ferromanganese crust accumulation rates
DRS at CSIR-National Institute of Oceanography
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Title |
Australasian microtektites in a substrate: A new constraint on ferromanganese crust accumulation rates
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Creator |
ShyamPrasad, M.
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Subject |
Geology and Geophysics
Geology and Geophysics ferromanganese nodules geochemistry mineralogy growth extraterrestrial material ISW, Indian Ocean |
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Description |
Microtektites belonging to the Australasian tektite strewn field are found in the substrate of a ferromanganese crust dredged from the Central Indian Basin. They are identified on their physical appearance, geographic occurrence and chemical composition. The ferromanganese crust has a thickness range of 6-17 mm, and its chemistry and mineralogy indicate hydrogenic accretion. Because the Australasian strewn field has an age of approximately 0.77 Ma, this finding implies that the overlying Fe-Mn crust has minimum accretion rates of 7.8-22.1 mm/Myr, which are much higher than the average growth rates of hydrogenic crusts
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Date |
1997-07-05T10:06:25Z
2017-09-30T02:52:21Z 1997-07-05T10:06:25Z 2017-09-30T02:52:21Z 1994 |
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Type |
Journal Article
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Identifier |
Marine Geology, vol.116(3-4); 1994; 259-266
0025-3227 http://drs.nio.org/drs/handle/2264/7471 |
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Language |
en
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Relation |
Mar Geol
SCI |
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Publisher |
Elsevier
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