Siderite precipitation in Paleoarchean oceans during hydrothermal venting

TL;DR

This study shows that iron carbonate (siderite) microparticles formed in ancient oceans through hydrothermal venting, offering new insights into early Earth's ocean chemistry.

Contribution

The discovery of iron-rich siderite microparticles in 3.49- to 3.25-Ga iron cherts provides evidence for hydrothermal venting-driven precipitation in anoxic oceans.

Findings

Iron-rich siderite microparticles were found in exhalative iron cherts from the Pilbara Craton.

Geochemical modeling suggests magnesium-rich siderite formed in seawater-dominated solutions.

Younger analogs show diagenetic formation of siderite from marine pore fluids, not hydrothermal processes.

Abstract

Siderite [iron(II) carbonate] is a major constituent of most iron formations. Its origin, which is currently disputed, affects interpretations about the composition of the ocean, atmosphere, and biosphere on early Earth. Direct precipitation from anoxic seawater is unlikely because of its prohibitively slow nucleation rate even in supersaturated solutions. However, recent modeling suggests that siderite may have precipitated at higher temperatures during hydrothermal fluid–seawater mixing in ancient anoxic oceans. Here, we report the presence of iron-rich siderite microparticles (<1.0 micrometers) in 3.49- to 3.25-Ga exhalative iron cherts from the Pilbara Craton, Australia, which we interpret to have formed during venting of iron(II)-rich hydrothermal fluids into anoxic water columns. Geochemical modeling suggests that coexisting magnesium-rich siderite formed in solutions dominated by seawater. The lack of hydrothermal iron siderite and predominance of magnesium siderite in younger analogs indicate that the bulk of siderite in iron formations is diagenetic and formed from marine pore fluids.

Seafloor hydrothermal venting of iron on early Earth may have triggered seawater precipitation of iron carbonate crystals.

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