Origin of iron oxide spherules in the banded iron formation of the Bababudan Group, Dharwar Craton, Southern India

dc.contributor.author Orberger, Beate
dc.contributor.author Wagner, Christiane
dc.contributor.author Wirth, Richard
dc.contributor.author Quirico, Eric
dc.contributor.author Gallien, Jean Paul
dc.contributor.author Derré, Colette
dc.contributor.author Montagnac, Gilles
dc.contributor.author Noret, Aurélie
dc.contributor.author Jayananda, Mudlappa
dc.contributor.author Massault, Marc
dc.contributor.author Rouchon, Virgile
dc.date.accessioned 2022-03-26T23:50:21Z
dc.date.available 2022-03-26T23:50:21Z
dc.date.issued 2012-06-30
dc.description.abstract The banded iron formation of the Bababudan Group (Western Dharwar Craton, India) is composed of millimetric to centimetric alternating quartz and grey to red Fe-oxide bands. Major phases are quartz and martite (hematized magnetite) with minor Fe-sulfides and Ca-Mg-Fe-carbonates. Micrometric Fe-oxide spherules fill cavities in discontinuous micrometric layers of Fe-oxides that occur in the massive quartz layers and at the interface of massive Fe-oxide and quartz layers. The spherules are composed of micrometric radial plates of hematite intergrown with nanometric magnetite. These spherules contain carbonaceous matter (CM) with nanometric Fe-particles and have low N contents (∼900ppm; CM1). The spherule formation is attributed to a low temperature hydrothermal process (150-200°C) at around 2.52Ga, possibly favored by the presence of CM. These hydrothermal fluids dissolved diagenetic interstitial sulfides or carbonates creating cavities which, provided space for the spherule precipitation. Carbonaceous matter of semi-anthracite maturity is encapsulated in quartz grains adjacent to the Fe-oxide spherules (CM2) and it is thus concluded that CM1 and CM2 are most likely contemporaneous and of the same origin, either incorporated at the time of BIF formation or during the hydrothermal event at 2.52Ga from the underlying phyllitised black shales. Carbonaceous matter (CM3) was also found around the Fe-oxide spherules and the martite grains. CM3 has much higher N contents (>5000ppm), is of a lower maturity than CM1 and CM2, and is related to weathering, which is also indicated by the presence of goethite and kaolinite. The δ 13C of all CMs varies from -19.4 to -24.7‰, similar to values measured in the underlying phyllitised black shales and likely reflect denitrifying microbial activity. © 2012 Elsevier Ltd.
dc.identifier.citation Journal of Asian Earth Sciences. v.52
dc.identifier.issn 13679120
dc.identifier.uri 10.1016/j.jseaes.2012.02.008
dc.identifier.uri https://www.sciencedirect.com/science/article/abs/pii/S1367912012001228
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/2689
dc.subject Banded iron formations
dc.subject Carbonaceous matter
dc.subject FIB-TEM
dc.subject Hematite
dc.subject Raman spectroscopy
dc.subject Spherules
dc.title Origin of iron oxide spherules in the banded iron formation of the Bababudan Group, Dharwar Craton, Southern India
dc.type Journal. Article
dspace.entity.type
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