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      Late Cretaceous paleolatitude of the Hawaiian Hot Spot: New paleomagnetic data from Detroit Seamount (ODP Site 883) : PALEOLATITUDE OF DETROIT SEAMOUNT

      1 , 1
      Geochemistry, Geophysics, Geosystems
      American Geophysical Union (AGU)

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          Rock Magnetism

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            Propriétés magnétiques des ferrites ; ferrimagnétisme et antiferromagnétisme

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              The Emperor Seamounts: southward motion of the Hawaiian hotspot plume in Earth's mantle.

              J. Tarduno (2003)
              The Hawaiian-Emperor hotspot track has a prominent bend, which has served as the basis for the theory that the Hawaiian hotspot, fixed in the deep mantle, traced a change in plate motion. However, paleomagnetic and radiometric age data from samples recovered by ocean drilling define an age-progressive paleolatitude history, indicating that the Emperor Seamount trend was principally formed by the rapid motion (over 40 millimeters per year) of the Hawaiian hotspot plume during Late Cretaceous to early-Tertiary times (81 to 47 million years ago). Evidence for motion of the Hawaiian plume affects models of mantle convection and plate tectonics, changing our understanding of terrestrial dynamics.
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                Author and article information

                Journal
                Geochemistry, Geophysics, Geosystems
                Geochem. Geophys. Geosyst.
                American Geophysical Union (AGU)
                15252027
                November 2004
                November 2004
                November 20 2004
                : 5
                : 11
                : n/a
                Affiliations
                [1 ]Department of Earth and Environmental Sciences; University of Rochester; Rochester NY 14627 USA
                Article
                10.1029/2004GC000745
                fbc65260-80b5-4593-aeb3-2c99f9a31f63
                © 2004

                http://doi.wiley.com/10.1002/tdm_license_1.1

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