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The
ROTATION RATE is the length of time for an
object to spin once on its axis. Planetary rotation rates are measured
by using telescopes or space probes. Scientists carefully pick a particular
feature on the planet (a large crater, a mountain, a spot, etc.). The task
is then to determine how long the feature takes to rotate into the same
position again. This is the rotation rate. For example, the animated
image of our Sun at right has a rotation rate of about 25 days. After
a rotation rate is measured, it can be compared with values found for many
objects in the solar system (planets, asteroids, natural satellites, and
our Sun).
An example of planetary rotation
that caused astronomers quite a bit of confusion was the planet Mercury.
Because Mercury is located so close to our Sun, it was difficult to observe
the planet closely. In 1974, NASA sent the Mariner 10 space probe to investigate
Mercury. The plan was to have Mariner 10 orbit our Sun in such a way that
it passed by planet Mercury three times for every two orbits. Unfortunately
for the astronomers, Mercury has the same rotation around our sun,
three times every two orbits, resulting in Mariner 10 photographing the
SAME SIDE of Mercury every time!
Another
planet that is difficult to directly observe rotate is our own planet
Earth. This is because we live on Earth and rotate with it. Historically,
it was not until after Copernicus that the idea of the Earth's rotation
was accepted. Several experiments have been conducted to demonstrate directly
the rotation of Earth; one interesting example is the Foucault Pendulum
Experiment (ref
). Recently, NASA scientists were finally able to get great
movies of
Earth rotating when the Galileo
probe flew past Earth on its way to Jupiter in 1994.
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