GSA Annual Meeting in Denver, Colorado, USA - 2016

Paper No. 7-9
Presentation Time: 10:40 AM

AN ALGORITHM TO COMBINE GRAVITY, TOPOGRAPHY, SEISMIC VELOCITY, AND HEAT FLOW APPLIED TO UNDERSTAND THE PROTEROZOIC EVOLUTION AND MODERN STRUCTURE OF THE MIDCONTINENT RIFT


LEVANDOWSKI, Will, US Geological Survey, Geologic Hazards Science Center, MS-966, PO BOX 25046, Denver, CO 80225, wlevandowski@usgs.gov

Gravity and topography are inherently non-unique functions of three-dimensional density structure; constraining density models with complementary information such as seismic velocity and heat flow yields more robust results. In this regard the North American Midcontinent Rift (MCR) poses a special challenge: A prominent gravity high sits within thermally homogenous and low-relief terrain, and shear-velocity models from surface wave dispersion suggest anomalously slow—rather than fast—mid-upper crust. Using seismic velocity models, heat flow data, and empirical relations between velocity and density as functions of temperature and composition, I generate an initial estimate of the 3-D density structure of the crust and upper mantle. Then, a random-walk Monte Carlo algorithm iteratively refines the density structure until it reproduces gravity and flexurally modulated topography to within 5 mGal and 50 meters across the region. Embracing the non-uniqueness of the solution, 1000 individual acceptable 3-D structures are derived. Similar to many other focused studies, this modeling reveal dense, mafic material throughout the crustal column beneath the MCR, including eclogitic lowermost crust to depths of ~55 km, consistent with pure-shear thickening during rift inversion. A secondary finding, however, is that the mantle lithosphere beneath the MCR is not anomalously buoyant (i.e., melt-depleted), suggesting that the primary source of rift-related melts was sublithospheric and that lithospheric partial melting played only a small role in magma generation. As such, there is reason to question the hypothesis that a mantle plume is necessary for the onset of rifting. Instead, I suggest that rifting began due to far-field stress and that a positive feedback between passive upwelling and retrogressive phase changes in the underlying asthenosphere focused extension and volcanism. Subsequent rift inversion exploited not only warm, recently faulted crust but also a gravitational potential energy low beneath the low-elevation, sediment-filled rift graben. This conception suggests that intraplate deformation can be focused by gravitational body forces, and this new methodology provides a means by which to quantify these stresses.