A theory that may be thought of as the
precursor to plate tectonics. It was proposed most clearly by
Alfred Wegener in 1912 and states that the continents are relatively
light objects that are floating and moving freely across
a substratum of oceanic crust. The theory was largely discredited
because it lacked a driving mechanism, and it seemed
implausible if not physically impossible to most geologists
and geophysicists at the time. However, many of the ideas of
continental drift were later incorporated into the paradigm of
plate tectonics.
Early geologists recognized many of the major tectonic
features of the continents and oceans. Cratons are very old
and stable portions of the continents that have been inactive
since the Precambrian and typically have subdued topography
including gentle arches and basins. Orogenic belts are
long, narrow belts of structurally disrupted and metamorphosed
rocks, typified (when active) by volcanoes, earthquakes,
and folding of strata. Abyssal plains are stable, flat
parts of the deep oceanic floor, whereas oceanic ridges are
mountain ranges beneath the sea with active volcanoes,
earthquakes, and high heat flow. In order to explain the
large-scale tectonic features of the Earth, early geologists proposed
many hypotheses, including popular ideas that the
Earth was either expanding or shrinking, forming ocean
basins and mountain ranges. In 1910–25, Alfred Wegener
published a series of works including his 1912 treatise on
The Origin of Continents and Oceans. He proposed that the
continents were drifting about the surface of the planet, and
that they once fit together to form one great supercontinent,
known as Pangea. To fit the coastlines of the different continental
masses together to form his reconstruction of Pangea,
Wegener defined the continent/ocean transition as the outer
edge of the continental shelves. The continental reconstruction
proposed by Wegener showed remarkably good fits
between coastlines on opposing sides of ocean basins, such as
the Brazilian Highlands of South America fitting into the
Niger delta region of Africa. Wegener was a meteorologist,
and since he was not formally trained as a geologist, few scientists
at the time believed him, although we now know that
he was largely correct.
Most continental areas lie approximately 985 feet (300
m) above sea level, and if we extrapolate present erosion
rates back in time, we find that continents would be eroded
to sea level in 10–15 million years. This observation led to
the application of the principle of isostasy to explain the elevation
of the continents. Isostasy, which is essentially
Archimedes’ Principle, states that continents and high topography
are buoyed up by thick continental roots floating in a
denser mantle, much like icebergs floating in water. The principle
of isostasy states that the elevation of any large segment
of crust is directly proportional to the thickness of the crust.
Significantly, geologists working in Scandinavia noticed that
areas that had recently been glaciated were rising quickly relative
to sea level, and they equated this observation with the
principle of isostatic rebound. Isostatic rebound is accommodated
by the flow of mantle material within the zone of low
viscosity beneath the continental crust, to compensate the rising
topography. These observations revealed that mantle
material can flow at rates of several centimeters per year.
In The Origin of Continents and Oceans, Wegener was
able to take all the continents and fit them back together to
form a Permian supercontinent, known as Pangea (or all
land). Wegener also used indicators of paleoclimate, such as
locations of ancient deserts and glacial ice sheets, and distributions
of certain plant and animal species, to support his
ideas. Wegener’s ideas were supported by a famous South
African geologist, Alexander L. Du Toit, who, in 1921,
matched the stratigraphy and structure across the Pangea
landmass. Du Toit found the same plants, such as the Glossopterous
fauna, across Africa and South America. He also
documented similar reptiles and even earthworms across narrow
belts of Wegener’s Pangea, supporting the concept of
continental drift.
Even with evidence such as the matching of geological
belts across Pangea, most geologists and geophysicists doubted
the idea, since it lacked a driving mechanism and it seemed
mechanically impossible for relatively soft continental crust
to plow through the much stronger oceans. Early attempts at
finding a mechanism were implausible and included ideas
such as tides pushing the continents. Because of the lack of
credible driving mechanisms, continental drift encountered
stiff resistance from the geologic community, as few could
understand how continents could plow through the mantle.
In 1928 Arthur Holmes suggested a driving mechanism
for moving the continents. He proposed that heat produced
by radioactive decay caused thermal convection in the mantle,
and that the laterally flowing mantle dragged the continents
with the convection cells. He reasoned that if the
mantle can flow to allow isostatic rebound following glaciation,
then maybe it can flow laterally as well. The acceptance
of thermal convection as a driving mechanism for continental
drift represented the foundation of modern plate tectonics. In
the 1950s and 1960s, the paleomagnetic data was collected
from many continents and argued strongly that the continents
had indeed been shifting, both with respect to the magnetic
pole and also with respect to each other. When seafloor
spreading and subduction of oceanic crust beneath island
arcs was recognized in the 1960s, the model of continental
drift was modified to become the new plate tectonic
paradigm that revolutionized and unified many previously
diverse fields of the Earth Sciences.
See also PLATE TECTONICS.














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