AN OVERVIEW OF THE PINWARE–BARABOO–PICURIS OROGEN: A 1.52–1.37 GA MESOPROTEROZOIC, TRANS–LAURENTIAN OROGENIC BELT
A convergent accretionary tectonic margin was proposed to explain the Pinware-Baraboo-Picuris orogenic belt. The Pinware orogen was envisioned as a rifted continental arc, with the formation of a peri-continental island arc that subsequently collided with the continental margin. The formation of a Mesoproterozoic continental arc in the southwest US and midcontinent region was more speculative. For the Picuris and Baraboo orogens an advancing and retreating subduction model, with varying subduction angles was envisioned to allow for both crustal thickening and extension within a continental retroarc or backarc setting. Unfortunately, a fundamental contradiction remains; this model is inconsistent with the dominantly, ferroan magmatism associated with the Mesoproterozoic of Laurentia. One possible modification to this accretionary tectonic model is to call upon the collision of the juvenile Granite-Rhyolite province with the Paleoproterozoic margin of Laurentia to account for the Picuris and Baraboo orogenies. However, finding a tectonic model that fully reconciles the evidence for crustal thickening and a continental scale orogenic belt with the trans-Laurentian ferroan magmatic event remains elusive.