PROTEROZOIC RIFT SYSTEMS AND THEIR INFLUENCE ON THE FORMATION OF THE LATE CRETACEOUS-EARLY CENOZOIC WYOMING SALIENT
The Uinta Range exposes the Neoproterozoic Uinta Mountain Group (UMG) along its anticlinal axial trace. On the western limit of the range, Cambrian strata rest on the UMG, however through most of its length, the UMG is disconformably overlain by Devonian-Mississippian strata, suggesting that the Uinta Range had been structurally inverted prior to this time. This Ordovician–Devonian (?) inversion (Cortez-Tooele arch) removed the efficient Cambrian Ophir/Gros Ventre detachment and was likely responsible for the dramatic reentrant in the thrust belt.
Although the Teton- Gros Ventre range apparently marks the northern buttress of the Wyoming salient, the Pioneer and Copper Basin thrusts, located ~150 km inboard, strike parallel to the northern boundary of the salient. The strike of these thrusts coincides with the Lemhi arch, an antecedent Neoproterozoic to early Paleozoic feature in east-central Idaho that precluded deposition of muddy Cambrian facies, likely thwarting the thrust belt’s eastward translation. Beginning in the Santonian, the leading edge of the thrust belt was also constrained by emergent basement-involved structures (e.g. Blacktail-Snowcrest uplift).
The spatial correlation between the thickness/distribution of early Paleozoic stratigraphy and the trace of the Wyoming salient speak to their interdependence and architectural control. We believe that the Wyoming salient would have formed in the absence of Laramide deformation.