We can measure how fast tectonic plates are moving today, but how do
scientists know what the rates of plate movement have been over geologic
time? The oceans hold one of the key pieces to the puzzle. Because the
ocean-floor magnetic striping records the flip-flops in the Earth's
magnetic field, scientists, knowing the approximate duration of the
reversal, can calculate the average rate of plate movement during a given
time span. These average rates of plate separations can range widely. The
Arctic Ridge has the slowest rate (less than 2.5 cm/yr), and the East
Pacific Rise near Easter Island, in the South Pacific about 3,400 km west
of Chile, has the fastest rate (more than 15 cm/yr).
Evidence of past rates of plate movement
also can be obtained from geologic mapping studies. If a rock formation of
known age -- with distinctive composition, structure, or fossils -- mapped
on one side of a plate boundary can be matched with the same formation on
the other side of the boundary, then measuring the distance that the
formation has been offset can give an estimate of the average rate of
plate motion. This simple but effective technique has been used to
determine the rates of plate motion at divergent boundaries, for example
the Mid-Atlantic Ridge, and transform boundaries, such as the San Andreas
Fault.
Current plate movement can be tracked
directly by means of ground-based or space-based geodetic
measurements; geodesy is the science of the size and shape of the
Earth. Ground-based measurements are taken with conventional but very
precise ground-surveying techniques, using laser-electronic instruments.
However, because plate motions are global in scale, they are best measured
by satellite-based methods. The late 1970s witnessed the rapid growth of space
geodesy, a term applied to space-based techniques for taking precise,
repeated measurements of carefully chosen points on the Earth's surface
separated by hundreds to thousands of kilometers. The three most commonly
used space-geodetic techniques -- very long baseline interferometry (VLBI),
satellite laser ranging (SLR), and the Global Positioning System (GPS) --
are based on technologies developed for military and aerospace research,
notably radio astronomy and satellite tracking.
Among the three techniques, to date the GPS
has been the most useful for studying the Earth's crustal movements.
Twenty-one satellites are currently in orbit 20,000 km above the Earth as
part of the NavStar system of the U.S. Department of Defense. These
satellites continuously transmit radio signals back to Earth. To determine
its precise position on Earth (longitude, latitude, elevation), each GPS
ground site must simultaneously receive signals from at least four
satellites, recording the exact time and location of each satellite when
its signal was received. By repeatedly measuring distances between
specific points, geologists can determine if there has been active
movement along faults or between plates. The separations between GPS sites
are already being measured regularly around the Pacific basin. By
monitoring the interaction between the Pacific Plate and the surrounding,
largely continental plates, scientists hope to learn more about the events
building up to earthquakes and volcanic eruptions in the circum-Pacific
Ring of Fire. Space-geodetic data have already confirmed that the rates
and direction of plate movement, averaged over several years, compare well
with rates and direction of plate movement averaged over millions of
years. |