TY - JOUR
T1 - Paleomagnetic Records From Pulsed Magmatism in the Southwestern Laurentia Large Igneous Province and Cardenas Basalt Support Rapid Late Mesoproterozoic Plate Motion
AU - Zhang, Yiming
AU - Anderson, Nicolas S.
AU - Mohr, Michael T.
AU - Nelson, Lyle L.
AU - Macdonald, Francis A.
AU - Schmitz, Mark D.
AU - Thurston, Olivia G.
AU - Guenthner, William R.
AU - Karlstrom, Karl E.
AU - Swanson-Hysell, Nicholas L.
N1 - Project research was funded by NSF CAREER Grant EAR-1847277 to N.L.S.-H. Additional research support came from an H2H8 research Grant to Y.Z. as well as a UC Berkeley summer undergraduate research fellowship and a UC Berkeley Department of Earth Science Ramsden grant to N.S.A. We thank participants in the 2021 Grand Canyon Supergroup field forum for stimulating interactions in the canyon. National Park Service Permits for sampling within Grand Canyon National Park and Death Valley National Park are gratefully acknowledged.
Project research was funded by NSF CAREER Grant EAR\u20101847277 to N.L.S.\u2010H. Additional research support came from an H2H8 research Grant to Y.Z. as well as a UC Berkeley summer undergraduate research fellowship and a UC Berkeley Department of Earth Science Ramsden grant to N.S.A. We thank participants in the 2021 Grand Canyon Supergroup field forum for stimulating interactions in the canyon. National Park Service Permits for sampling within Grand Canyon National Park and Death Valley National Park are gratefully acknowledged.
PY - 2024/10
Y1 - 2024/10
N2 - 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, (Formula presented.) = 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.
AB - 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, (Formula presented.) = 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.
KW - Keweenawan track
KW - large igneous province
KW - paleogeography
KW - paleomagneticm
KW - Rodinia
KW - southwestern Laurentia
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UR - http://www.scopus.com/inward/citedby.url?scp=85206809680&partnerID=8YFLogxK
U2 - 10.1029/2024JB029036
DO - 10.1029/2024JB029036
M3 - Article
AN - SCOPUS:85206809680
SN - 2169-9313
VL - 129
JO - Journal of Geophysical Research: Solid Earth
JF - Journal of Geophysical Research: Solid Earth
IS - 10
M1 - e2024JB029036
ER -