T239 Assembling Laurentia: Growth of the Western Continental Margin by Subduction, with or without Terrane Accretion, 190-70 Ma II
Friday, 30 October 2020
10:00 AM - 2:00 PM
Meeting Rooms
THE RECYCLING OF CHROMITITES IN THE PUERTO NUEVO OPHIOLITE (BAJA CALIFORNIA SUR, MEXICO)
Paper number: T239-14
Program: Technical Sessions
Time: 1:15 PM – 1:30 PM
Authors
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Cristina TalaveraCurtin University, Perth, WA
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Cristina TalaveraUniversity of Edinburgh, Edinburgh
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Julia Farré-de-PabloDepartament de Mineralogia, Petrologia i Geologia Aplicada, Barcelona
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Takako SatsukawaKyoto University, Kyoto
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José María González-JiménezUniversidad de Granada, Granada
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Antoni CamprubíUniversidad Nacional Autónoma de México, Mexico, DF
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William L. GriffinSydney, NSW
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Joaquín A. ProenzaUniversitat de Barcelona, Barcelona, Barcelona
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Elena Centeno-GarciaUniversidad Nacional Autónoma de México, Coyoacán, Mexico City
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Suzanne Y. O'ReillySydney, NSW
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Antonio Garcia-CascoUniversidad de Granada-CSIC, Armilla (Granada)
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Antonio Garcia-CascoUniversidad de Granada, Granada
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Elena A. BelousovaSydney, NSW
Abstract
Zircons recovered from these chromitites yield ages (2263±44 to 278±4 Ma) and Hf-O compositions (ɛHf(t)= −18.7 to +9.1 and δ18O= 5.9 to 12.4 ‰) that broadly match with those zircons reported in the nearby exposed Arteaga Complex (i.e., Potosi fan). Thus, we interpret that the chromitite zircons from the Puerto Nuevo sequence are xenocrysts from continent-derived sediments delivered into the mantle via subduction and transferred to the mantle wedge by cold plumes. In this scenario, chromites containing zircons were formed by the mixing of a Cr-rich boninitic melt formed by dissolution of orthopyroxene from harzburgite, and a more SiO2-rich melt formed by partial assimilation of the plume contaminated with crustal material. This is in agreement with the minor and trace elements composition of chromites, which are similar to those from high-Cr ophiolitic chromitites crystallized from melts similar to high-Mg island-arc tholeiites (IAT) and boninites in supra-subduction zone. In addition, the presence of clinopyroxene lamellae with preferred crystallographic orientation in our chromites evidence that the Puerto Nuevo chromitites have experienced HT-UHP conditions (<12 GPa and ~1600 °C). Hence, we propose a tectonic scenario that involves: 1) the formation of chromitite in the supra-subduction zone mantle wedge underlying the Vizcaino intra-oceanic arc ca. 250 Ma ago (Early Triassic), 2) deep mantle recycling, and 3) subsequent diapiric exhumation in the intra-oceanic basin (the San Hipólito marginal sea) generated during an extensional stage of the Vizcaino intra-oceanic arc ca. 221 Ma ago (Late Triassic).
Geological Society of America Abstracts with Programs. Vol. 52, No. 6
doi: 10.1130/abs/2020AM-359233
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