TY - JOUR
T1 - Abiotic anoxic iron oxidation, formation of Archean banded iron formations, and the oxidation of early Earth
AU - Dodd, Matthew S.
AU - Wang, Haiyang
AU - Li, Chao
AU - Towner, Martyn
AU - Thomson, Andrew R.
AU - Slack, John F.
AU - Wan, Yu sheng
AU - Pirajno, Franco
AU - Manikyamba, Chakravadhanula
AU - Wang, Qiang
AU - Papineau, Dominic
PY - 2022/4/15
Y1 - 2022/4/15
N2 - Iron in the early anoxic oceans of Archean age (4000-2500 million years ago) is believed to have been oxidized to form banded iron formations (BIF). Previously, it has been proposed that iron was oxidized either by free oxygen, H2O2, microbial oxidation, or photo-oxidation. However, these mechanisms are difficult to reconcile with evidence for the oceans at that time having been largely devoid of dissolved oxygen and oxidants, together with the rarity of microbial remains in BIF and restrictively slow rates of photo-oxidation. Experiments reported here show that ferrous iron readily oxidizes in analogs of Archean anoxic seawater following the precipitation of ferrous hydroxide. Once precipitated, ferrous hydroxide undergoes decomposition to elemental iron that reacts with water at room temperature to form ferric iron and release hydrogen gas. The ferric iron may then be incorporated into green rust, a mixed ferrous-ferric phase that ages into iron minerals commonly found in BIF. Our finding suggests that anoxic iron oxidation may have contributed to the formation of oxide-facies BIF, especially Algoma-type BIF that likely formed in semi-restricted basins where ferrous hydroxide saturation was more easily achieved. Additionally, ferrous hydroxide decomposition would have contributed to early Earth's oxidation, as a result of hydrogen escape to space, thus providing new insights into environmental and biological conditions on early Earth.
AB - Iron in the early anoxic oceans of Archean age (4000-2500 million years ago) is believed to have been oxidized to form banded iron formations (BIF). Previously, it has been proposed that iron was oxidized either by free oxygen, H2O2, microbial oxidation, or photo-oxidation. However, these mechanisms are difficult to reconcile with evidence for the oceans at that time having been largely devoid of dissolved oxygen and oxidants, together with the rarity of microbial remains in BIF and restrictively slow rates of photo-oxidation. Experiments reported here show that ferrous iron readily oxidizes in analogs of Archean anoxic seawater following the precipitation of ferrous hydroxide. Once precipitated, ferrous hydroxide undergoes decomposition to elemental iron that reacts with water at room temperature to form ferric iron and release hydrogen gas. The ferric iron may then be incorporated into green rust, a mixed ferrous-ferric phase that ages into iron minerals commonly found in BIF. Our finding suggests that anoxic iron oxidation may have contributed to the formation of oxide-facies BIF, especially Algoma-type BIF that likely formed in semi-restricted basins where ferrous hydroxide saturation was more easily achieved. Additionally, ferrous hydroxide decomposition would have contributed to early Earth's oxidation, as a result of hydrogen escape to space, thus providing new insights into environmental and biological conditions on early Earth.
KW - banded iron formation
KW - early Earth
KW - green rust
KW - hydrogen escape
KW - iron cycle
UR - http://www.scopus.com/inward/record.url?scp=85126328884&partnerID=8YFLogxK
U2 - 10.1016/j.epsl.2022.117469
DO - 10.1016/j.epsl.2022.117469
M3 - Article
AN - SCOPUS:85126328884
VL - 584
JO - Earth & Planetary Science Letters
JF - Earth & Planetary Science Letters
SN - 0012-821X
M1 - 117469
ER -