A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event

Abstract The oldest recognized proxies for low atmospheric oxygen are massive iron‐rich deposits. Following the rise of oxygen ∼2.4 billion years ago (Ga), massive iron formations (IFs) largely disappear from the geologic record, only to reappear in a pulse ∼1.88 Ga, which has been attributed to sea...

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Main Authors: Athena Eyster, Latisha A. Brengman, Claire I. O. Nichols, Zoe Levitt, Julia Wilcots, Kristin D. Bergmann
Format: Article
Language:English
Published: Wiley 2021-08-01
Series:Geochemistry, Geophysics, Geosystems
Online Access:https://doi.org/10.1029/2020GC009113
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author Athena Eyster
Latisha A. Brengman
Claire I. O. Nichols
Zoe Levitt
Julia Wilcots
Kristin D. Bergmann
author_facet Athena Eyster
Latisha A. Brengman
Claire I. O. Nichols
Zoe Levitt
Julia Wilcots
Kristin D. Bergmann
author_sort Athena Eyster
collection DOAJ
description Abstract The oldest recognized proxies for low atmospheric oxygen are massive iron‐rich deposits. Following the rise of oxygen ∼2.4 billion years ago (Ga), massive iron formations (IFs) largely disappear from the geologic record, only to reappear in a pulse ∼1.88 Ga, which has been attributed to sea‐level transgressions, changing ocean chemistry triggered by intense volcanism, or lowered atmospheric oxygen levels. The North American Gogebic Range is one of the rare records of this pulse and even more uniquely has exposures of both volcanics and IF, providing an ideal field locality to investigate triggers for this pulse of IF. To determine the environmental context and key factors driving IF deposition after the initial rise in oxygen, we made detailed observations of the stratigraphy and facies relationships and present updated mapping relationships of the Gogebic Range Ironwood Iron Formation and the Emperor Volcanics. This work expands existing mine datasets and logs to constrain variations in stratigraphy. Our results are the first to quantitatively constrain thickness variations along the entire Gogebic Range and tie them to syn‐sedimentary faulting along listric normal faults and half grabens. Furthermore, our dataset suggests that initiation of intense syn‐basinal volcanism linked to a large igneous province does not coincide with initial iron deposition, thus cannot be invoked as a causal trigger. Finally, the possibility of iron deposition in a shallow‐water environment suggests that the post‐GOE IF pulse may not reflect global marine transgressions, but instead a chemocline shallowing due to changing global atmospheric oxygen.
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spelling doaj.art-dcee38dcce1a449c9e06629f0ea942f82023-11-03T17:00:37ZengWileyGeochemistry, Geophysics, Geosystems1525-20272021-08-01228n/an/a10.1029/2020GC009113A New Depositional Framework for Massive Iron Formations After the Great Oxidation EventAthena Eyster0Latisha A. Brengman1Claire I. O. Nichols2Zoe Levitt3Julia Wilcots4Kristin D. Bergmann5Department of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge MA USADepartment of Earth and Environmental Sciences University of Minnesota Duluth Duluth MN USADepartment of Earth Sciences University of Oxford Oxford UKDepartment of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge MA USADepartment of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge MA USADepartment of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge MA USAAbstract The oldest recognized proxies for low atmospheric oxygen are massive iron‐rich deposits. Following the rise of oxygen ∼2.4 billion years ago (Ga), massive iron formations (IFs) largely disappear from the geologic record, only to reappear in a pulse ∼1.88 Ga, which has been attributed to sea‐level transgressions, changing ocean chemistry triggered by intense volcanism, or lowered atmospheric oxygen levels. The North American Gogebic Range is one of the rare records of this pulse and even more uniquely has exposures of both volcanics and IF, providing an ideal field locality to investigate triggers for this pulse of IF. To determine the environmental context and key factors driving IF deposition after the initial rise in oxygen, we made detailed observations of the stratigraphy and facies relationships and present updated mapping relationships of the Gogebic Range Ironwood Iron Formation and the Emperor Volcanics. This work expands existing mine datasets and logs to constrain variations in stratigraphy. Our results are the first to quantitatively constrain thickness variations along the entire Gogebic Range and tie them to syn‐sedimentary faulting along listric normal faults and half grabens. Furthermore, our dataset suggests that initiation of intense syn‐basinal volcanism linked to a large igneous province does not coincide with initial iron deposition, thus cannot be invoked as a causal trigger. Finally, the possibility of iron deposition in a shallow‐water environment suggests that the post‐GOE IF pulse may not reflect global marine transgressions, but instead a chemocline shallowing due to changing global atmospheric oxygen.https://doi.org/10.1029/2020GC009113
spellingShingle Athena Eyster
Latisha A. Brengman
Claire I. O. Nichols
Zoe Levitt
Julia Wilcots
Kristin D. Bergmann
A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
Geochemistry, Geophysics, Geosystems
title A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
title_full A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
title_fullStr A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
title_full_unstemmed A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
title_short A New Depositional Framework for Massive Iron Formations After the Great Oxidation Event
title_sort new depositional framework for massive iron formations after the great oxidation event
url https://doi.org/10.1029/2020GC009113
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