IAG-IASPEI 2017

Presentation information

Oral

IAG Symposia » G04. Earth rotation and geodynamics

[G04-1] Earth rotation and geodynamics I

Mon. Jul 31, 2017 8:30 AM - 10:00 AM Room 504+505 (Kobe International Conference Center 5F, Room 504+505)

Chairs: Jianli Chen (University of Texas at Austin) , Bernhard Steinberger (GFZ Germen Research Center for Goesciences)

8:30 AM - 8:45 AM

[G04-1-01] Limited True Polar Wander as evidence that Earth's non-hydrostatic shape is persistently triaxial

Bernhard Steinberger1, 2, Miriam-Lisanne Seidel3, Trond Torsvik1,2,4 (1.GFZ German Research Centre for Geosciences, Potsdam, Germany, 2.Centre for Earth Evolution and Dynamics, University of Oslo, Oslo, Norway, 3.Werner-von-Siemens Gymnasium, Berlin, Germany, 4.Geological Survey of Norway (NGU), Trondheim, Norway, 5.University of Witwatersrand, Wits, South Africa)

Earth's spin axis follows the maximum moment of inertia axis of mantle convection, with some delay due to adjustment of the rotational bulge. Here we compute this axis for geodynamic models based on subduction history, assuming constant slab sinking speed, with another contribution due to thermochemical piles. For a wide range of parameters, a large shift of approximately 90 degrees is predicted around 80 − 90 Ma. It can be largely attributed to a change in circum-Pacific subduction from predominantly in the North and South towards East and West. Actual amounts of true polar wander are much smaller, pointing towards additional inertia tensor contributions, possibly due to slabs in the lowermost mantle below both polar regions. These slabs would have been subducted before approximately 150 Ma, when plate motions in the Panthalassa basin are largely unknown. Matching predicted and observed true polar wander can serve at constraining such plate motions.