Article ID Journal Published Year Pages File Type
6430673 Earth and Planetary Science Letters 2012 8 Pages PDF
Abstract

Granitic and mafic magma pulses were sequentially accreted in the spectacularly exposed shallow crustal Torres del Paine laccolith, in southern Patagonia. This 12.5 Ma pluton forms a composite intrusion with a subvertical feeding system in the west and a laccolith in the east. A key unknown in the formation of sill complexes is how individual magma pulses are assembled over time and the geometry and localization of their feeding system. High resolution zircon CA-ID-TIMS U-Pb dating shows that the laccolith grew first by under-accretion of granitic sills over 90 ± 30 ka, linked to a 'sheet-like' feeding system, followed by underplating of mafic sills after ~ 20 ka of quiescence. In the mafic sills complex, individual sills were injected by over-accretion during 41 ± 11 ka. Our data show that successive granitic and mafic magmas emplacement generated a volume of ~ 88 km3 in 162 ± 11 ka.

► High resolution zircon CA-ID-TIMS U-Pb dating on Torres del Paine mafic rocks. ► Granite-mafic laccolith and stock-like feeding system construction over 162 ± 11 ka. ► Mafic sill complex over-accretion over 41 ± 11 ka, overlain by older granite. ► Pluton construction rate decreases from 0.0008 km3 y− 1 to 0.0002 km3 y− 1.

Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Earth and Planetary Sciences (General)
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