Infiltration triggered by selective dissolution of pyroxenes is a major mode of melt migration in the mantle. A common view, supported by experiments and numerical models, is that the geometry of the melt plumbing system is governed by the stress field induced by solid-state flow of the host peridotite. Yet, salient melt migration structures frozen at an early stage of development in the mantle section of the Trinity ophiolite reveal that lithological heterogeneities drastically impact melt trajectories. Where melts reach a pyroxenite layer, dissolution-induced permeability abruptly increases, initiating a feedback loop confining melt migration to that layer regardless of its orientation relative to the stress field. This process results in the development of a network of interweaved dunitic channels evolving to thick tabular dunites where the melt reacts with closely spaced pyroxenite layers. This reacting melt was rich in alkali elements and water, as evidenced by the minerals (mostly amphibole and micas) encapsulated in the Cr-spinel grains that crystallized during the reaction. This “pioneer melt” differs from the volumetrically dominant depleted andesite that fed the crustal section. In fact, the migration of andesite benefited from the enhanced permeability provided by the dunites formed by the pioneer melt. As a result, dunites are palimpsests, the compositions of which record successive percolation events. The geometry of the melt pathways is extremely challenging to model because the abundance, spacing, and orientation of lithological heterogeneities cannot be predicted, being inherited from a long geological history.
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Research Article|
July 27, 2022
A Rosetta stone linking melt trajectories in the mantle to the stress field and lithological heterogeneities (Trinity ophiolite, California)
Georges Ceuleneer;
Georges Ceuleneer
1
Géosciences Environnement Toulouse, Toulouse University, CNRS, IRD, 14 Avenue E. Belin, 31400 Toulouse, France
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Mathieu Rospabé;
Mathieu Rospabé
2
Research Institute for Marine Geodynamics (IMG), Japan Agency for Marine-Earth Science and Technology (JAMSTEC), 2-15 Natsushima, Yokosuka, Kanagawa 237-0061, Japan3
Geo-Ocean, Univ Brest, CNRS, Ifremer, UMR6538, F-29280 Plouzané, France
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Tom Chatelin;
Tom Chatelin
1
Géosciences Environnement Toulouse, Toulouse University, CNRS, IRD, 14 Avenue E. Belin, 31400 Toulouse, France
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Hadrien Henry;
Hadrien Henry
1
Géosciences Environnement Toulouse, Toulouse University, CNRS, IRD, 14 Avenue E. Belin, 31400 Toulouse, France
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Romain Tilhac;
Romain Tilhac
4
Instituto Andaluz de Ciencias de la Tierra (IACT), Consejo Superior de Investigaciones Científicas (CSIC)–Universidad de Granada, 18100 Armilla, Granada, Spain
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Mary-Alix Kaczmarek;
Mary-Alix Kaczmarek
1
Géosciences Environnement Toulouse, Toulouse University, CNRS, IRD, 14 Avenue E. Belin, 31400 Toulouse, France
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Elisabeth le Sueur
Elisabeth le Sueur
5
53 rue Fontaine des Cerdans, 31520 Ramonville, France
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Geology (2022)
Article history
received:
26 Jan 2022
rev-recd:
12 May 2022
accepted:
25 May 2022
first online:
27 Jul 2022
Citation
Georges Ceuleneer, Mathieu Rospabé, Tom Chatelin, Hadrien Henry, Romain Tilhac, Mary-Alix Kaczmarek, Elisabeth le Sueur; A Rosetta stone linking melt trajectories in the mantle to the stress field and lithological heterogeneities (Trinity ophiolite, California). Geology 2022; doi: https://doi.org/10.1130/G50083.1
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