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Tarduno, John A. et al. (2003): The Emperor Seamounts; southward motion of the Hawaiian Hotspot plume in Earth's mantle
Leg/Site/Hole:
Related Expeditions:
ODP 197
ODP 197 1203
ODP 197 1204
ODP 197 1205
ODP 197 1206
Identifier:
ID:
2003-074851
Type:
georefid
ID:
10.1126/science.1086442
Type:
doi
Creator:
Name:
Tarduno, John A.
Affiliation:
University of Rochester, Department of Earth and Environmental Sciences, Rochester, NY, United States
Role:
author
Name:
Duncan, Robert A.
Affiliation:
Oregon State University, United States
Role:
author
Name:
Scholl, David W.
Affiliation:
Stanford University, United States
Role:
author
Name:
Cottrell, Rory D.
Affiliation:
Japan Marine Science and Technology Center, Japan
Role:
author
Name:
Steinberger, Bernhard
Affiliation:
University of Hawaii, United States
Role:
author
Name:
Thordarson, Thorvaldur
Affiliation:
University of Notre Dame, United States
Role:
author
Name:
Kerr, Bryan C.
Affiliation:
Massachusetts Institute of Technology, United States
Role:
author
Name:
Neal, Clive R.
Affiliation:
Okayama University of Science, Japan
Role:
author
Name:
Frey, Fred A.
Affiliation:
University of Toronto, Canada
Role:
author
Name:
Torii, Masayuki
Affiliation:
Role:
author
Name:
Carvallo, Claire
Affiliation:
Role:
author
Identification:
Title:
The Emperor Seamounts; southward motion of the Hawaiian Hotspot plume in Earth's mantle
Year:
2003
Source:
Science
Publisher:
American Association for the Advancement of Science, Washington, DC, United States
Volume:
301
Issue:
5636
Pages:
1064-1069
Abstract:
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.
Language:
English
Genre:
Serial
Rights:
URL:
http://www.sciencemag.org/content/301/5636/1064.full.pdf
Coverage:
Geographic coordinates:
North:51.1200
West:167.4400
East: 172.0900
South:34.5600
Keywords:
Solid-earth geophysics; Cenozoic; Cretaceous; demagnetization; Detroit Seamount; dynamics; Emperor Seamounts; Hawaiian Plume; hot spots; Koko Seamount; Leg 197; mantle; mantle plumes; Mesozoic; models; movement; Nintoku Seamount; North Pacific; Northwest Pacific; Ocean Drilling Program; ocean floors; ODP Site 1203; ODP Site 1204; ODP Site 1205; ODP Site 1206; Pacific Ocean; paleolatitude; paleomagnetism; plate tectonics; polar wandering; seamounts; Tertiary; West Pacific;
.
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