PLATE
TECTONICS
In 1912 a German meteorologist named
Alfred Wegener proposed the theory of continental drift. He based
his theory in part on the matching coastlines of South America and
Africa as well as on similarity of plant and animal fossils found
on different continents. Wegener’s view of the drifting continents
was controversial. Not until geomagnetic surveys showed a pattern
of matching strips of newly formed ocean floor on either side of
the mid-Atlantic ridge could scientists begin to understand how
tectonic processes from deep inside Earth could drive the continents
apart. Wegener’s work and the discovery that lava emerging
at mid-oceanic ridges creates new oceanic crust led to the development
of the theory of plate tectonics, now one of the most important
theories in earth sciences. We now understand that the plates do
not wander randomly on Earth’s surface, so the term “continental
drift” has been retired.
Earth is made up of three main layers, the crust, the mantle, and
the core, (moving from the outside in). Continental crust, which
is about 30 kilometers thick, and oceanic crust, which is only about
five kilometers thick, make up part of the lithosphere. (The two
types of crust differ in their mineralogic and chemical composition.)
The lithosphere also includes the uppermost part of the mantle,
which is a dense, hot layer of semisolid rock about 2900 kilometers
thick and is composed of iron, magnesium, and calcium. The core,
making up Earth’s center, is nearly twice as dense as the
mantle because it is made of a metallic iron-nickel alloy. The core
has outer and inner portions. The outer core is a liquid, 2200 kilometers
thick. The mechanism that generates Earth’s magnetic field,
the geodynamo, originates in the electrically conducting outer core.
The solid inner core, 1250 kilometers thick, is roughly the size
of the moon, but it is as hot as the surface of the sun.
The theory of plate tectonics states that Earth’s lithosphere
consists of plates that ride on hotter, more mobile material. In
geologic terms, a plate is a large rigid slab of solid rock. The
word tectonics is derived from a Greek word meaning “to build”
and refers to the deformation of Earth’s crust and the structural
features that result.
Earth has seven large plates and a dozen or so smaller plates. The
plates are generally internally rigid and move relative to each
other. Each plate is about 80 kilometers (50 miles) thick and consists
of a shallow part that deforms by elastic bending or by brittle
breaking and a deeper part made up of material that deforms without
rupturing (plastic deformation). By using the Global Positioning
System (GPS), we can determine the direction and rate of movement.
Plates move from one to 13 centimeters per year.
Tectonic plates can move into, away from, or past one another. These
three relative motions correspond to the three major types of plate
boundaries, or margins: convergent, spreading, and transform, respectively.
Two of the most common forms of convergent margins are subduction
zones and collision zones. Subduction occurs when a higher-density
plate moves beneath a lower-density plate and plunges as much as
several hundred kilometers into Earth’s interior. On the west
coast of South America, for example, the Nazca Plate dives underneath
the South American Plate. Collision occurs when two plates of relatively
low density converge, and neither can be subducted into the denser,
deep Earth. Collision leads to orogenesis, or the creation of mountain
ranges, one of the most dramatic effects of tectonic forces. Beginning
around 40 to 50-million years ago and especially within the past
10 million years, for example, the Himalaya Mountains and the Tibetan
Plateau were forced up when the Indian Plate moved northward and
collided with the Eurasian Plate. The collision created the Earth’s
tallest mountains, more than 8800 meters high.
Most spreading margins are deep under the oceans. They occur where
hot magma from Earth’s interior spews into the mid-oceanic
ridges between plates and forms new oceanic plate material. The
Mid-Atlantic Ridge, the boundary between the North American and
Eurasian Plates, is a spreading margin. Sometimes spreading margins
are on continents, as in the Red Sea/African Rift Valley system
at the boundary between the African and Arabian Plates.
Transform margins occur when one plate slides past another. One
of the most familiar examples is the San Andreas Fault Zone on the
west coast of North America where the Pacific Plate slides northward
relative to the North American Plate.
Plate margins are some of the most geologically active parts of
Earth’s surface. Volcanoes, for example, are not randomly
distributed; they are normally concentrated on the edges of the
continents, on island chains, or along large mountain ranges beneath
the sea. Their distribution usually coincides with plate boundaries.
More than half of the world’s active volcanoes above sea level
encircle the Pacific Plate to form the circum-Pacific “Ring
of Fire.” In addition, 90% of the world’s earthquakes
occur along boundaries where plates are colliding or scraping past
one another.
Because the movement of plates correlates directly with the prevalence
of geologic hazards, it is generally riskier to live near plate
boundaries than on stable areas of the continents. People living
along active plate boundaries, where most earthquakes and volcanic
eruptions occur, need to be aware of the potential hazards. Major
earthquakes that occur along subduction zones can trigger tsunamis
that can affect coastal areas all around major ocean basins. These
seismic sea waves have historically been devastating for communities
along coasts and on islands.
The developing technologies of ocean-floor mapping, including exploration
of the ocean floor with deep-sea submersibles and compilations of
Earth’s paleomagnetic record, have proven invaluable to improving
our understanding of plate tectonics. The study of earthquakes and
advances in seismic instrumentation also provide important information
on Earth’s interior.
The forces that drive the movement of the plates are not precisely
known, but they likely relate to convective movement within Earth’s
mantle. One hypothesis holds that upward convection, or flow, of
hotter material within Earth’s mantle drives the plates apart
along mid-oceanic ridges. A different hypothesis proposes that gravity
pulls down on the older, colder, and heavier ocean floor at subducting
plate margins with more force than on the newer, lighter seafloor
along the mid-oceanic ridges, pulling the plates apart and allowing
lava to emerge at the mid-oceanic ridges.
In addition to driving plate tectonics, the dynamics of Earth’s
interior are also believed to produce Earth’s magnetic field
through the flow of liquid metal in the outer core. The paleomagnetic
record indicates that the geomagnetic field has existed for at least
three billion years. This record shows that at numerous times in
Earth’s history the polarity of the magnetic field has switched—the
north magnetic pole became the south magnetic pole, and the south
became north. This reversal of Earth’s magnetic field does
not occur at predictable or regular intervals, and its cause is
not fully understood, but the record provides a valuable dating
tool for earth scientists. For more information on paleomagnetics,
read about it in the “Dating Methods” section of this
web site.
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