期刊
CHEMICAL GEOLOGY
卷 362, 期 -, 页码 105-114出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.chemgeo.2013.08.010
关键词
Mt. McRae Shale; Hamersley basin; Uranium isotopes; Uranium geochemical cycle; Earth surface oxygenation; Archean
资金
- National Science Foundation
- Agouron Institute
- NASA Astrobiology Institute
- Directorate For Geosciences
- Division Of Earth Sciences [0952216] Funding Source: National Science Foundation
Geochemical data from late Archean sedimentary rocks point to photosynthetic O-2 production and at least intermittent occurrences of locally mild oxidative weathering and surface ocean oxygenation (oxygen oases) prior to the early Paleoproterozoic Great Oxidation Event. For example, distinctive authigenic enrichments of Mo and Re in euxinic (anoxic and sulfidic) black shales are best explained by the oxidative mobilization of these metals from crustal sulfide minerals and their accumulation as oxyanions in seawater. In contrast, it is not clear if low U enrichments in the same shales reflect negligible oxidation of U from the upper crust or a very small oceanic U inventory that was derived from oxidative U mobilization. Here, we report U isotope data for the 2.50 Ga Mt. McRae Shale (Hamersley basin, Western Australia), which provides a more sensitive test for the presence or absence of authigenic U compared to U concentrations and enrichment factors normalized to average shale or upper crustal compositions (that may not be representative of the local detrital composition). We find instances where the U isotope composition in the upper Mt. McRae Shale (delta U-238 = -0.2 to 0.0 parts per thousand relative to standard SRM950a) is isotopically heavier than average upper crust (delta U-238 = -0.31 +/- 0.14 [2SD] based on granitoids and basalts). The high delta U-238 values point to U isotope fractionation in the late Archean marine environment and hence indicate the presence of a small amount of dissolved U in seawater and authigenic U in the Mt. McRae Shale. Volume-dependent equilibrium isotope fractionation during the reduction of dissolved UVI to insoluble U-IV, like that observed in the modern Black Sea, may explain the high delta U-238 signatures if U removal from bottom waters was not quantitative. Alternatively, quantitative U removal would require that late Archean seawater had high delta U-238, which could have arisen from the preferential sequestration of U-235 to Fe (oxyhydr) oxide minerals elsewhere in the Hamersley basin. The supracrustal delta U-238 signatures are associated with some of the highest Mo and Re enrichments in the Mt. McRae Shale as well as distinctive Mo, S and N isotope signatures that are indicative of mild environmental oxygenation. Hence, our findings suggest that small amounts of U were oxidatively mobilized from the upper crust at 2.50 Ga. Unlike Mo and Re, however, U oxidation may not have occurred on land. Instead, we hypothesize that oxidative U mobilization occurred by submarine weathering in an oxygen oasis. (C) 2013 Elsevier B. V. All rights reserved.
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