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Pacific-Antarctic-Australia motion and the formation of the Macquarie Plate Steven C. Cande, Scripps Institution of Oceanography Joann M. Stock, California Institute of Technology
ABSTRACT: Magnetic anomaly and fracture zone data on the Southeast Indian Ridge
(SEIR) are analysed in order to constrain the kinematic history of the
Macquarie Plate, the region of the Australian Plate roughly east of 145
degreesE and south of 52 degreesS. Finite rotations for Australia-Antarctic
motion are determined for nine chrons (2Ay, 3Ay, 5o, 6o, 8o, 10o, 12o, 13o and
17o) using data limited to the region between 88 degreesE and 139 degreesE.
These rotations are used to generate synthetic flowlines which are compared
with the observed trends of the easternmost fracture zones on the SEIR. An
analysis of the synthetic flowlines shows that the Macquarie Plate region has
behaved as an independent rigid plate for roughly the last 6 Myr. Finite
rotations for Macquarie-Antarctic motion are determined for chrons 2Ay and 3Ay.
These rotations are summed with Australia-Antarctic rotations to determine
Macquarie-Australia rotations. We find that the best-fit Macquarie-Australia
rotation poles lie within the zone of diffuse intraplate seismicity in the
South Tasman Sea separating the Macquarie Plate from the main part of the
Australian Plate. Motion of the Macquarie Plate relative to the Pacific Plate
for chrons 2Ay and 3Ay is determined by summing Macquarie-Antarctic and
Antarctic-Pacific rotations. The Pacific-Macquarie rotations predict a smaller
rate of convergence perpendicular to the Hjort Trench than the
Pacific-Australia rotations. The onset of the deformation of the South Tasman
Sea and the development of the Macquarie Plate appears to have been triggered
by the subduction of young, buoyant oceanic crust near the Hjort Trench and
coincided with a clockwise change in Pacific-Australia motion around 6 Ma. The
revised Pacific-Australia rotations also have implications for the tectonics of
the Alpine Fault Zone of New Zealand. We find that changes in relative
displacement along the Alpine Fault have been small over the last 20 Myr. The
average rate of convergence over the last 6 Myr is about 40 per cent smaller
than in previous models.
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