EVOLUTION OF THE YELLOWSTONE HOTSPOT TRACK: RETROSPECTIVE AND CURRENT IDEAS (Invited Presentation)
Many workers have embraced the notion of plume arrival at ~17-16 Ma, but since 2013 a growing volume of evidence supports a much older age to account for offshore volcanism and the accretion of the Siletzia oceanic plateau from 56-49 Ma, followed by overriding of the YHS by the North American plate from 42-34 Ma (Wells et al., 2014). Shielding of the YHS by the Farallon slab is marked by the lack of a geochemical plume signature in eruption products from 34-17 Ma. Instead, these back-arc eruptions are consistent with progressive thermomechanical erosion of the slab, associated with dehydration-melting and the melting of Farallon crust to produce an ENE-trending belt of adakite volcanism above the hotspot trend from 30-20 Ma (Camp et al., 2017). Seismic studies resolve a truncated Juan de Fuca plate at ~300 km depth and a large slab hole beneath the adakite/YHS trend (e.g., Obrebski et al., 2010) consistent with this period of slab disassociation. After a short volcanic hiatus, slab rupture resulted in the rapid rise and ponding of voluminous plume-modified mantle beneath the North American plate and eruption of the main phase of tholeiitic CRB from 17-15 Ma. This event was followed by a transition to age-progressive volcanism along the Yellowstone/Snake River Plain trend from 14 Ma to the present, modified by magmatism from plume-flux back-filling to the WSW.