We present revised finite rotation parameters for Australia and East Antarc
tica in the Early Tertiary incorporating new magnetic data off of Wilkes La
nd, Antarctica. Reconstructions based on these and recently published rotat
ion parameters document a relatively stationary position of Broken Ridge ab
utted against Central Kerguelen Plateau between chron 34 (83 Ma) and chron
20 (43 Ma), prior to the commencement of seafloor spreading between the two
Late Cretaceous features. These reconstructions are significant as they ar
e the first which are consistent with geological and geophysical constraint
s in not producing an overlap of Broken Ridge and Kerguelen Plateau between
chron 34 and chron 24 (53 Ma) and not requiring significant extension or s
trike-slip motion within Kerguelen Plateau. We also find that the finite ro
tations for chrons 20 to 34 outline the area of rough topography inferred f
rom the satellite-derived free-air gravity for the Diamantina Zone and Labu
an Basin. A consequence of these rotations is that there is considerable ov
erlap of continental crust in the region of Tasmania, the South Tasman Rise
and East Antarctica in the Late Cretaceous. Solutions to this problem may
imply either post-Santonian (less than or equal to 79 Ma) extension or tran
sform motion in the Bass Strait, or late Cretaceous or Cenozoic extension i
n Wilkes Land. The reconstructions also agree with prior estimates of rough
ly 150 km of motion between East and West Antarctica since chron 20. (C) 20
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