Abstract:The terminal Mesoproterozoic was a period of widespread tectonic convergence globally, culminating in the amalgamation of the Rodinia supercontinent. However, in Laurentia, long-lived orogenesis on its eastern margin was punctuated by short-lived extension that generated the Midcontinent Rift ca. 1110–1090 Ma. Whereas this cratonic rift basin is typically considered an isolated occurrence, a series of new depositional ages demonstrate that multiple cratonic basins in northern Laurentia originated around this t… Show more
“…1) and the Southwestern Large Igneous Province 23 were major ma c magmatic events that required signi cant extension of the crust from 1.15 to 1.08 Gyr-ago 24 . Synchronously, major sedimentary basins were created by rifting 25 more than 3000 km towards the hinterland (Fig. 1).…”
Section: Main Textmentioning
confidence: 99%
“…Laurentia was thus a passive margin throughout most of the Mesoproterozoic, with access to sea water such as documented in sedimentary rocks of the MCR 26,27 . The extremely fast motion of Laurentia between 1.1 and 1.08 Gyr-ago dragged by slab avalanche, would likely have put the entire continent under extension and generated all the major sedimentary basins and large igneous province such as the MCR that formed during this period 24,25 . Moreover, our model better reconciles proxies of tectonic activities used to infer tectonic quiescence during the so-called "boring billion".…”
“…1) and the Southwestern Large Igneous Province 23 were major ma c magmatic events that required signi cant extension of the crust from 1.15 to 1.08 Gyr-ago 24 . Synchronously, major sedimentary basins were created by rifting 25 more than 3000 km towards the hinterland (Fig. 1).…”
Section: Main Textmentioning
confidence: 99%
“…Laurentia was thus a passive margin throughout most of the Mesoproterozoic, with access to sea water such as documented in sedimentary rocks of the MCR 26,27 . The extremely fast motion of Laurentia between 1.1 and 1.08 Gyr-ago dragged by slab avalanche, would likely have put the entire continent under extension and generated all the major sedimentary basins and large igneous province such as the MCR that formed during this period 24,25 . Moreover, our model better reconciles proxies of tectonic activities used to infer tectonic quiescence during the so-called "boring billion".…”
“…1,070 Ma (Henry et al., 1977; Slotznick et al., 2023). While there are some contemporaneous basins in northern Laurentia (Greenman et al., 2021), there is minimal basin development within Laurentia following the Grenvillian orogeny until the Rodinia supercontinent began to rift apart ca. 770 Ma (Macdonald et al., 2023).…”
The paleogeography of Laurentia throughout the Neoproterozoic is critical for reconstructing global paleogeography due to its central position in the supercontinent Rodinia. We develop a new paleomagnetic pole from red siltstones and fine‐grained sandstones of the early Neoproterozoic Jacobsville Formation which is now constrained to be ca. 990 Ma in age. High‐resolution thermal demagnetization experiments resolve detrital remanent magnetizations held by hematite. These directions were reoriented within siltstone intraclasts and pass intraformational conglomerate tests—giving confidence that the magnetization is detrital and primary. An inclination‐corrected mean paleomagnetic pole position for the Jacobsville Formation indicates that Laurentia's motion slowed down significantly following the onset of the Grenvillian orogeny. Prior rapid plate motion associated with closure of the Unimos Ocean between 1,110 and 1,090 Ma transitioned to slow drift of Laurentia across the equator in the late Mesoproterozoic to early Neoproterozoic. We interpret the distinct position of this well‐dated pole from those in the Grenville orogen that have been assigned a similar age to indicate that the ages of the poles associated with the Grenville Loop likely need to be revised to be younger due to prolonged exhumation.
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