Re-Os isotope systematics in black shales from the Lesser Himalaya: their chronology and role in the 187Os/188Os evolution of seawater

Singh, Sunil K. ; Trivedi, J. R. ; Krishnaswami, S. (1999) Re-Os isotope systematics in black shales from the Lesser Himalaya: their chronology and role in the 187Os/188Os evolution of seawater Geochimica Et Cosmochimica Acta, 63 (16). pp. 2381-2392. ISSN 0016-7037

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Official URL: http://linkinghub.elsevier.com/retrieve/pii/S00167...

Related URL: http://dx.doi.org/10.1016/S0016-7037(99)00201-X

Abstract

Re and Os abundances and Os isotope systematics have been measured in a number of black shales sampled from outcrops and two underground phosphorite mines, Maldeota and Durmala, in the Lesser Himalaya. The Re and Os concentrations in these samples exhibit wide range, 0.2 to 264 ng/g and 0.02 to 13.5 ng/g, respectively, with a mean Re/Os of ~25. The 187Os/188Os of these samples also show a broad range 1.02 to 11.6, with many of them far more radiogenic than the currently eroding continental crust. The black shales from the Maldeota and Durmala mines, collected a few meters above the Krol-Tal (Pc-C) boundary and occurring in the same stratigraphic horizon, yield 187Re-187Os isochron ages of 554 ± 16 and 552 ± 22 Ma, respectively, consistent with fossil evidences and those assigned for the Pc-C boundary at various other locations. These results indicate closed system behaviour of Re and Os in these mine samples and reaffirm the validity of 187Re-187Os pair to date organic-rich sediments. The age of these mine samples from the outer belt seems to be a few hundred millions of years younger than the preliminary Re-Os age of 839 ± 138 Ma for black shales from Theog, collected from the inner belt. These initial results lean toward the hypothesis that the inner belt sediments were deposited earlier than the outer belt; however, more analyses of black shales are needed to confirm this. The role of weathering black shales from the Himalaya in contributing to the Os isotope evolution of seawater over the past ~25 Ma was assessed using a simple budget model for seawater Os and assuming values for Os fluxes and 187Os/188Os based on the available limited data on Os concentration and its 187Os/188Os in rivers and oceans. These calculations indicate that the required contributions from black shale weathering to account for the entire increase in oceanic 187Os/188Os over the past ~16 Ma is difficult to satisfy by varying only the Os flux from HTP rivers (187Os/188Os kept constant at 1.324) or their 187Os/188Os (188Os flux constant at today's value, ~131 moles/yr). The requirements to balance Os isotope budget in ocean through weathering of black shales, however, is easier to accommodate if both the Os flux from HTP (Himalayan-Tibetan Plateau) rivers and their 187Os/188Os are allowed to vary. Measurements of Os abundance in HTP rivers and its isotopic composition are needed to test the validity of the model results.

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