Mafic slab melt contributions to Proterozoic massif-type anorthosites

Author:

Keller Duncan S.1ORCID,Lee Cin-Ty A.1ORCID,Peck William H.2ORCID,Monteleone Brian D.3,Martin Céline4ORCID,Vervoort Jeffrey D.5ORCID,Bolge Louise6ORCID

Affiliation:

1. Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, TX 77005, USA.

2. Department of Earth and Environmental Geosciences, Colgate University, Hamilton, NY 13346, USA.

3. Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA.

4. Department of Earth and Planetary Sciences, American Museum of Natural History, New York, NY 10024, USA.

5. School of the Environment, Washington State University, Pullman, WA 99164, USA.

6. Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY 10964, USA.

Abstract

Massif-type anorthosites, enormous and enigmatic plagioclase-rich cumulate intrusions emplaced into Earth’s crust, formed in large numbers only between 1 and 2 billion years ago. Conflicting hypotheses for massif-type anorthosite formation, including melting of upwelling mantle, lower crustal melting, and arc magmatism above subduction zones, have stymied consensus on what parental magmas crystallized the anorthosites and why the rocks are temporally restricted. Using B, O, Nd, and Sr isotope analyses, bulk chemistry, and petrogenetic modeling, we demonstrate that the magmas parental to the Marcy and Morin anorthosites, classic examples from North America’s Grenville orogen, require large input from mafic melts derived from slab-top altered oceanic crust. The anorthosites also record B isotopic signatures corresponding to other slab lithologies such as subducted abyssal serpentinite. We propose that anorthosite massifs formed underneath convergent continental margins wherein a subducted or subducting slab melted extensively and link massif-type anorthosite formation to Earth’s thermal and tectonic evolution.

Publisher

American Association for the Advancement of Science (AAAS)

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