Abstract

Igneous dykes are the main magma transport pathways through the Earth's crust, and they are considered to contribute to tectonic extension in volcanic rifts. Dykes are typically considered to result from brittle fracturing, even in the ductile crust. A common assumption is that dyke orientation is controlled by tectonic stresses, such that dykes in rifts are expected to be vertical and perpendicular to extension. Here we report on detailed field observations of a spectacularly well-exposed dyke swarm to show that dykes were not systematically emplaced by purely brittle processes and that dyke orientation may differ from the dominant tectonic stress orientations. The dyke complex formed near the brittle-ductile transition during opening of the Iapetus Ocean and is now exposed in the Scandinavian Caledonides. Distinct dyke morphologies related to different emplacement mechanisms has been recognized: 1) Brittle dykes that exhibit straight contacts with the host rock, sharp tips, en-echelon segments with bridges exhibiting angular fragments; 2) Brittle-ductile dykes that exhibit undulating contacts, rounded tips, ductile folding in the host rock and contemporaneous brittle and ductile features; 3) Ductile “dykes” that exhibit rounded shapes and mingling between the soft ductile host rock and the intruding mafic magma. The brittle dykes exhibit two distinct orientations separated by c. 30° that are mutually cross-cutting, suggesting that the dyke swam did not consist of only vertical sheets perpendicular to regional extension, as expected in rifts. We were able to use the well-exposed host rock layers as markers to perform a kinematic restoration to quantify the average strain accommodating the emplacement of the dyke complex: it accommodated for >100% extension, but counter-intuitively it also accommodated for 27% crustal thickening. We infer that the magma influx rate was higher than the tectonic stretching rate, implying that magma was emplaced forcefully, as supported by field observations. Finally, our observations suggest that the fast emplacement of the dyke swarm triggered a rapid shallowing of the brittle-ductile transition, and lead to a considerable weakening of the crust. The interpretations presented here could potentially have large implications for surface topography and seismicity in active rifts and volcanic areas around the world.

Highlights

  • Dykes, and igneous sheet intrusions in general, are fundamental magma pathways through the Earth’s crust

  • We report on detailed field observations of a spectacularly exposed dyke swarm emplaced at mid-crustal levels in the magma-rich rifted margin related to a large igneous province that developed during the breakup of the palaeocontinents Baltica and Laurentia, ∼605 Ma ago

  • This paper presents detailed field observations of a spectacularly exposed dyke swarm emplaced at 10 to 15 km depth at a magma-rich rifted margin related to the breakup of the palaeocontinents Baltica and Laurentia at ∼606 Ma

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Summary

Introduction

Igneous sheet intrusions in general, are fundamental magma pathways through the Earth’s crust. Andersonian theory predicts that the emplacement of dykes is controlled at a first order by far-field crustal stresses (Anderson, 1936; Nakamura, 1977), implying that tectonic stresses dominate over stresses induced by magmatism. Such a scenario is likely when the magma influx rate is lower than the tectonic stretching rate. We report on detailed field observations of a spectacularly exposed dyke swarm emplaced at mid-crustal levels in the magma-rich rifted margin related to a large igneous province that developed during the breakup of the palaeocontinents Baltica and Laurentia, ∼605 Ma ago. Our observations allow us to reveal (1) the complex brittle/ductile emplacement of dykes in deep crustal levels, (2) magma emplacement mechanism and related crustal deformation associated with high magma influx rates, and (3) upward migration of the brittle-ductile transition (BDT) because of magmatism

Geological setting
Geological observations
Observations in Sarek area
Observations from the Corrovarre lens
Emplacement mechanisms of individual intrusions
Emplacement of the whole dyke swarm
Regional constraints
Tectonic and geodynamic implications for magma-rich margins
Findings
Mechanical implications
Conclusions
Full Text
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