1. Paleomagnetic Records From Pulsed Magmatism in the Southwestern Laurentia Large Igneous Province and Cardenas Basalt Support Rapid Late Mesoproterozoic Plate Motion
- Author
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Zhang, Yiming, Anderson, Nicolas S., Mohr, Michael T., Nelson, Lyle L., Macdonald, Francis A., Schmitz, Mark D., Thurston, Olivia G., Guenthner, William R., Karlstrom, Karl E., and Swanson‐Hysell, Nicholas L.
- Abstract
Mafic intrusions, lava flows, and felsic plutons in southwestern Laurentia have been hypothesized to be associated with the emplacement of a late Mesoproterozoic (Stenian Period) large igneous province. Improved geochronologic data resolve distinct episodes of mafic magmatism in the region. The ca. 1,098 Ma main pulse of southwestern Laurentia large igneous province (SWLLIP) magmatism is recorded by mafic intrusions across southeastern California to central Arizona. A younger episode of volcanism resulted in eruptions that formed the ca. 1,082 Ma Cardenas Basalt, which is the uppermost unit of the Unkar Group in the Grand Canyon. With the updated geochronological constraints, we develop new paleomagnetic data from mafic sills in the SWLLIP. Overlapping poles between the Death Valley sills and rocks of similar age in the Midcontinent Rift are inconsistent with large‐scale Cenozoic vertical axis rotations in Death Valley. We also develop a new paleomagnetic pole from the ca. 1,082 Ma Cardenas Basalt (pole longitude = 183.9°E, pole latitude = 15.9°N, A95${\mathrm{A}}_{95}$= 7.4°, N= 18). The new paleomagnetic data are consistent with the pole path developed from time‐equivalent rocks of the Midcontinent Rift, supporting interpretations that changing pole positions are the result of rapid equatorward motion. These data add to the record of Laurentia's rapid motion from ca. 1,110 to 1,080 Ma that culminated in collisional Grenvillian orogenesis and the assembly of Rodinia. In Earth's geological record, voluminous magmatism over brief time frames are known as large igneous provinces. One such event took place approximately 1.1 billion years ago on the ancient North American continent (known as Laurentia) resulting in the formation of thick mafic sills. Previously, these intrusions across southwestern Laurentia were believed to have been emplaced simultaneously with the extrusive Cardenas Basalt lava flows in the Grand Canyon. We now know that the emplacement of the thick mafic intrusions represent a large igneous province, which predates the eruption of the Cardenas Basalt by 16 million years. By pairing this knowledge of the age with recorded magnetic directions in the lavas and intrusions, we can enrich our knowledge of Laurentia's motion leading up to the assembly of the supercontinent Rodinia. These data provide a new constraint on the position of the continent 1,082 million years ago and support the interpretation of rapid plate motion over the preceding 20 million years. Paleomagnetic directions from mafic sills in Death Valley are consistent with ca. 1,098 Ma LIP‐style magmatism in southwestern LaurentiaA paleomagnetic pole from the ca. 1,082 Ma Cardenas Basalt of the Grand Canyon corresponds with time‐equivalent Midcontinent Rift polesChanging southwestern Laurentia LIP pole positions support rapid equatorward motion of the continent recorded by the Keweenawan Track Paleomagnetic directions from mafic sills in Death Valley are consistent with ca. 1,098 Ma LIP‐style magmatism in southwestern Laurentia A paleomagnetic pole from the ca. 1,082 Ma Cardenas Basalt of the Grand Canyon corresponds with time‐equivalent Midcontinent Rift poles Changing southwestern Laurentia LIP pole positions support rapid equatorward motion of the continent recorded by the Keweenawan Track
- Published
- 2024
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