Genesis of Fe–Ti Oxide-Bearing Ultramafic Intrusions in the Duluth Complex, Minnesota, USA

Author:

Kleinsasser Jackie M1ORCID,Simon Adam C1,Peterson Dean2,Kattemalavadi Amartya1,Goan Ian R1,Keller Tobias3,Hudak George J4,Koshurba Kaitlin1

Affiliation:

1. Department of Earth and Environmental Sciences, University of Michigan , 1100 N University Ave., Ann Arbor, MI 48109 , USA

2. Big Rock Exploration, LLC , 1620 Central Ave NE, Unit 104, Minneapolis, MN 55413 , USA

3. School of Ocean and Earth Sciences, University of Southampton , European Way, Southampton SO14 3ZH , UK

4. Natural Resources Research Institute, University of Minnesota–Duluth , 5013 Miller Trunk Hwy, Hermantown, MN 55811 , USA

Abstract

Abstract The Duluth Complex is a large mafic intrusive system located in northeastern Minnesota emplaced as part of the 1.1-Ga Midcontinent Rift. Several Fe–Ti oxide-bearing ultramafic intrusions are hosted along the Western Margin of the Duluth Complex, and are discordant bodies present in a variety of geometries, hosted in multiple rock types, and dominated by peridotite, pyroxenite, and semi-massive to massive Fe–Ti oxide rock types. Their origin has been debated, and here we present geochemical evidence and modeling that supports a purely magmatic origin for the Titac and Longnose Fe–Ti oxide-bearing ultramafic intrusions. Ilmenite and titanomagnetite textures indicate a protracted cooling process, and δ34S values of sulfides reveal little assimilation of the footwall Virginia Formation, a fine-grained pelitic unit that contains sulfide-rich bands. We model the crystallization of a hypothetical parental magma composition to the host intrusion of Longnose using Rhyolite-MELTS and demonstrate that the accumulation of Fe–Ti oxides in the discordant intrusions cannot be explained by density-driven segregation of crystallized Fe–Ti oxides. Instead, we show that the development of silicate liquid immiscibility, occurring by the unmixing of the silicate melt into conjugate Si- and Fe-rich melts, can result in the effective segregation and transportation of the Fe-rich melt. The Fe-rich melt is ~2 orders of magnitude less viscous than the Si-rich melt, allowing the Fe-rich melt to be more effectively segregated and transported in the mush regime (crystallinities >50%). This suggests that viscosity, in addition to density, plays a significant role in forming the discordant Fe–Ti oxide-bearing ultramafic intrusions. We propose a genetic model that could also be responsible for the Fe–Ti oxide-rich layers or bands that are hosted within the igneous stratigraphy of mafic intrusions of the Duluth Complex.

Funder

National Science Foundation

Society of Economic Geologists

American Association of Petroleum Geologists

U-M Rackham Graduate Student Research

U-M EES Turner Award

NSF EAR

U-M EES

NSF

Publisher

Oxford University Press (OUP)

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