Evolution of iron formation to ore during Ediacaran to early Paleozoic tectonic stability

The enrichment of iron formation (IF) to form economically important hematitic iron ore has been linked to a range of mechanisms from interactions with hydrothermal or metamorphic fluids during active tectonics to chemical leaching driven by meteoric water in the very near surface. Direct geochronologic constraints on hematite that can link ore-forming processes to geologic events have only recently become possible. Here, we present spatially resolved hematite U-Pb and paleomagnetic data for Paleoproterozoic IF, and associated hematite ore bodies from Northern Michigan, USA, to assess the timing of hematite crystallization in these units. Our paired paleomagnetic and radiometric dating approach indicates that hematite crystallization in different iron oxide facies spanned the Proterozoic into the early Paleozoic. Notably, hematite ore enrichment occurred during a period of regional tectonic quiescence in the latest Neoproterozoic and early Paleozoic. At this time, Laurentia was at tropical paleolatitudes and for much of this interval Earth was in a particularly warm non-glacial interval. These results indicate that the hematite ore at the study locality developed through supergene process via the interaction of the host IF with warm meteoric water transported downward to the subsurface rather than hypogene hydrothermal fluids linked to tectonism in the Paleoproterozoic. • We present a novel paired in-situ U-Pb and paleomagnetic dataset on the hematite in iron formation and hematite ore. • The in-situ hematite U-Pb data show hematite enrichment spanned the Paleoproterozoic to early Phanerozoic. • Three ore samples yielded U-Pb ages from ca 560 to 460 Ma, extending ore formation in this region by 1 billion years. • The paleomagnetic directions from the ore are consistent with expected directions for the Ediacaran and early Phanerozoic. • Hematite ore development occurred in the shallow subsurface while Laurentia was at tropical latitudes.

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Publication Details

Journal
Earth and Planetary Science Letters
Published
2025-09-16
DOI
https://doi.org/10.1016/j.epsl.2025.119621
Citations
3
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
5.60
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article

Evolution of iron formation to ore during Ediacaran to early Paleozoic tectonic stability

Nicholas L. Swanson‐Hysell, Rebecca M. Flowers, Anthony J. Fuentes, Yiming Zhang et al.
3 citations
Earth and Planetary Science Letters
Geological and Geochemical Analysis
5.60
article

Evolution of iron formation to ore during Ediacaran to early Paleozoic tectonic stability

Nicholas L. Swanson‐Hysell, Rebecca M. Flowers, Anthony J. Fuentes, Yiming Zhang, Liam Courtney‐Davies
article en
3 citations

Abstract

The enrichment of iron formation (IF) to form economically important hematitic iron ore has been linked to a range of mechanisms from interactions with hydrothermal or metamorphic fluids during active tectonics to chemical leaching driven by meteoric water in the very near surface. Direct geochronologic constraints on hematite that can link ore-forming processes to geologic events have only recently become possible. Here, we present spatially resolved hematite U-Pb and paleomagnetic data for Paleoproterozoic IF, and associated hematite ore bodies from Northern Michigan, USA, to assess the timing of hematite crystallization in these units. Our paired paleomagnetic and radiometric dating approach indicates that hematite crystallization in different iron oxide facies spanned the Proterozoic into the early Paleozoic. Notably, hematite ore enrichment occurred during a period of regional tectonic quiescence in the latest Neoproterozoic and early Paleozoic. At this time, Laurentia was at tropical paleolatitudes and for much of this interval Earth was in a particularly warm non-glacial interval. These results indicate that the hematite ore at the study locality developed through supergene process via the interaction of the host IF with warm meteoric water transported downward to the subsurface rather than hypogene hydrothermal fluids linked to tectonism in the Paleoproterozoic. • We present a novel paired in-situ U-Pb and paleomagnetic dataset on the hematite in iron formation and hematite ore. • The in-situ hematite U-Pb data show hematite enrichment spanned the Paleoproterozoic to early Phanerozoic. • Three ore samples yielded U-Pb ages from ca 560 to 460 Ma, extending ore formation in this region by 1 billion years. • The paleomagnetic directions from the ore are consistent with expected directions for the Ediacaran and early Phanerozoic. • Hematite ore development occurred in the shallow subsurface while Laurentia was at tropical latitudes.

Earth and Planetary Science LettersVol. 671
University of Minnesota (US), Planetary Science Institute (US), University of Colorado Boulder (US)
Openalex Percentile: Top 4%
Geological and Geochemical Analysis
5.60
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