The following sequence
of reconstructions incorporate palaeomagnetic, structural, faunal, chronological
and tectonic constraints on the evolution of the Iapetus Ocean in the Early
Palaeozoic. Rifting and opening of the Ocean took place in latest
Cambrian time, with final closure occuring in the Late Silurian.
Continuing research is focussing on delineating the drift history of many
of the Intra-Iapetan terranes. These maps are the results of extensive
collaborations with colleagues in the US, Canada, Norway, the UK, and Ireland.
PDF versions are available by clicking on the links in the right-hand column.
You will need to have Adobe Acrobat
installed to read the PDF versions
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[PDF Version] |
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By the late Early Ordovician subductions
was well under way on both margins and Avalonia had started to rift away
from the Gondwanan margin.
[PDF Version] |
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[PDF Version] |
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Late Ordovician time marks the rapid
narrowing of the ocean and faunal provinciality starts to break down.
We can also see a raft of rifted terranes to the south of Avalonia, which
will become involved in the later collisions that mark the Hercynian, or
Variscan, orogeny in central Europe.
[PDF Version] |
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[PDF Version] |
Much of the evidence for the presence of arcs and oceanic islands within
the Iapetus comes from palaeomagnetic analyses carried out in collaboration
with Rob Van der Voo,
Ben
van der Pluijm and various students in the Tectonophysics Group at
the University of Michigan, notably Arlo
Weil and
Allen McNamara.
The Figure below illustrates the pattern of terranes derived from palaeomagnetic
studies in the Northern Appalachians on the right, compared with the faunal
provinces indicated by statistical analyses of brachipod distributions
on the left. The brachipod analyses were carried out in collaboration
with Dave Harper of the Palaeontological Institute of the Danish Natural
History Museum.
