11 Proterozoic Growth and Evolution of Southern Laurentia
Saturday, 2 April 2005
8:20 AM - 12:10 PM
IS THE ARC-ACCRETION MODEL FOR THE 1780-1650 MA CRUSTAL EVOLUTION OF SOUTHERN LAURENTIA CORRECT? LET'S LOOK AT THE ROCKS!
Paper number: 11-2
Program: THEME SESSIONS
Time: 8:30 AM – 8:50 AM
Authors
-
Barbara M. HillSyracuse Univ, Syracuse, NY
Abstract
Hill and Bickford (2001) found inherited ca. 1850 and 2500 Ma zircons in ca. 1750 Ma bimodal rocks in central Colorado and proposed that they were derived from pre-existing ca. 1850 Ma (Trans-Hudson/Penokean) crust, a conclusion supported by Nd isotopic data. Inherited zircon and common Pb data indicate involvement of older crust in ca. 1750 Ma rocks of the Mojave Province of southeastern California and western Arizona and the bimodal volcanogenic rocks of the Hualapai block in west-central Arizona. Hawkins et al. (1996) determined a zircon age of 1840 +/-1 Ma for the Elves Chasm pluton in the Grand Canyon, demonstrating that rocks of Trans-Hudson/Penokean age are present in southwestern Laurentia.
These data suggest that if arc-accretion contributed to the growth of southern Laurentia, it occurred during ca. 1880-1840 Ma Trans-Hudson/Penokean orogeny, producing rocks across the southwest that are now mostly obscured. The bimodality of the ca. 1780-1650 Ma rocks across the southwest suggests that they were derived from this pre-existing crust, most likely during extension and partial melting associated with the development of transpressional crustal-scale shear zones.