Cenozoic mass accumulation rates in the equatorial Pacific based on high-resolution mineralogy of Ocean Drilling Program Leg 199

Vanden Berg, Michael D.; Jarrard, Richard D.

doi:10.1029/2003PA000928

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Cenozoic mass accumulation rates in the equatorial Pacific based on high-resolution mineralogy of Ocean Drilling Program Leg 199 : EQUATORIAL PACIFIC MASS ACCUMULATION

Author(s): Michael D. Vanden Berg ¹ , Richard D. Jarrard ¹

Publication date (Electronic): June 23 2004

Journal: Paleoceanography

Publisher: American Geophysical Union (AGU)

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Most cited references 14

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High-resolution (104years) deep-sea foraminiferal stable isotope records of the Eocene-Oligocene climate transition

James Zachos, Terrence Quinn, Karen A. Salamy (1996)

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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.