Shapiro, M. N. (2005): Kinematics of the Campanian-Maastrichtian island arcs in northeastern Asia in light of drilling results on the Emperor Seamounts

Leg/Site/Hole:
ODP 145
ODP 197
Identifier:
2006-021128
georefid

Creator:
Shapiro, M. N.
Russian Academy of Sciences, Institute of Physics of the Earth, Moscow, Russian Federation
author

Identification:
Kinematics of the Campanian-Maastrichtian island arcs in northeastern Asia in light of drilling results on the Emperor Seamounts
2005
Geotectonics
MAIK Nauka/Interperiodica Publishing, Birmingham, AL, United States
39
5
408-415
The southward drift of the Hawaiian hotspot established by drilling on the Emperor Seamounts was not significant enough to suggest that the northern Emperor Seamounts and the Cretaceous island-arc sequences in the Olyutor-Kamchatka region were located at similar paleomagnetic latitudes. Furthermore, the obvious differences in the Late Cretaceous sedimentation on the Emperor Seamounts and in Kamchatka paleoarcs are caused not only by differences in their paleolatitudes. Therefore, the drilling results provide no serious grounds to revise the concept of substantial northern drift of the Cretaceous island arcs.
English
Serial
Coverage:Geographic coordinates:
North:50.0000
West:-180.0000East: -140.0000
South:20.0000

Solid-earth geophysics; Stratigraphy; Asia; biostratigraphy; boreholes; Campanian; Commonwealth of Independent States; Cretaceous; East Pacific Ocean Islands; Emperor Seamounts; Hawaii; hot spots; Invertebrata; island arcs; Kamchatka Peninsula; Leg 145; Leg 197; Maestrichtian; Mesozoic; microfossils; North Pacific; Northwest Pacific; Ocean Drilling Program; Oceania; Pacific Ocean; paleogeography; paleolatitude; paleomagnetism; plate tectonics; Polynesia; Protista; Radiolaria; Russian Federation; Russian Pacific region; Senonian; United States; Upper Cretaceous; West Pacific;

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