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A Closer Look: Supercontinents
Where did the idea of supercontinents come from?

Science studio diagram
of continental drift.
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Long before the theory of plate tectonics became accepted, there
was much speculation that the present day continents were the
fragmented pieces of pre-existing larger landmasses called
supercontinents. The belief that the modern continents have
not always been
in their
present positions has long been held. As early as the 1500s,
many geographers and mapmakers noticed the close match of the
coastlines of South America and Africa. The fit is even more
striking when the
continental shelves (submerged edge of a continental plate)
and the continental slopes (the true boundary of a continent)
are
compared
rather than the coastlines. It was not until 1912, however,
that the idea of moving continents was seriously considered
as a scientific
theory. This theory, called continental drift theory, was the
precursor to plate tectonics theory and was introduced by Alfred
Wegener.
How do scientists describe the history of supercontinents
on
Earth?
Scientists believe there have been several supercontinental
arrangements in the history of the Earth. The first known supercontinent
is
called Rodinia (from Russian, meaning "homeland"),
and it is thought to have formed about 1.1 billion years ago.
Although the exact size and configuration of Rodinia cannot be
estimated, rocks of ancestral North America are thought to have
formed the core of the giant continent. About 750 million years
ago, evidence suggests that Rodinia fragmented into pieces that
drifted apart. Approximately 600 million years ago, those pieces
collided again forming a new supercontinent, Pannotia.
Scientists
think Pannotia broke up about 550 million years ago into several
smaller fragments: Laurentia (the core of what is
now North America), Baltica (northern Europe), other small fragments,
and one very large fragment called Gondwanaland, which contained
the land from modern day China, India, Africa, South America,
and Antarctica. Between 550 and 350 million years ago, Laurasia,
a landmass comprised of North America and Eurasia, was formed.
Laurasia and Gondwanaland then joined to form the supercontinent
of Pangaea (from classical Greek, meaning "all lands").
Evidence suggests that Pangaea began to break up about 225 million
years ago, and continues to separate into the modern continents
we know today.
The process of supercontinent assembly, breakup,
dispersal and re-assembly takes, on average, about 500 million
years. This
supercontinent cycle is called the Wilson Cycle after J. Tuzo
Wilson, the Canadian geologist who first described it.
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