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Moon,
name given to the natural satellite of Earth, and
sometimes applied to the satellites of the other planets
in the solar system. The diameter of Earth’s Moon is
about 3,480 km (about 2,160 mi), or about one-fourth that
of Earth, and the Moon’s volume is about one-fiftieth
that of Earth. The mass of Earth is 81 times greater than
the mass of the Moon. Thus the average density of the Moon
is only three-fifths, and the gravitational pull at the
lunar surface only one-sixth, that of Earth. The Moon has
no liquid water and essentially no atmosphere, so no
weather exists to change its surface; yet it is not
totally inert.
The Moon moves about
Earth at an average distance of 384,403 km (238,857 mi),
and at an average speed of 3,700 km/h (2,300 mph)
. It completes one
revolution in an elliptical orbit about Earth in 27 days 7
hours 43 minutes 11.5 seconds with reference to the stars.
For the Moon to go from one phase to the next similar
phase, or one lunar month, requires 29 days 12 hours 44
minutes 2.8 seconds. The Moon rotates once on its axis in
about the same period of time that elapses for its
sidereal period of revolution, accounting for the fact
that virtually the same portion of the Moon is always
turned toward the Earth. Although the Moon appears bright
to the eye, it reflects into space only 7 percent of the
light that falls on it. The reflectivity, or albedo, of
0.07 is similar to that of coal dust.
At any one time, an
observer can see only 50 percent of the Moon’s entire
surface. However, an additional 9 percent can be seen from
time to time around the apparent edge because of the
relative motion called libration. This is because of the
slightly different angles of view from Earth, due to
different relative positions of the Moon along its
inclined elliptical orbit.
The Moon shows
progressively different phases as it moves along its orbit
around Earth. Half the Moon is always in sunlight, just as
half Earth has day while the other half has night. The
phases of the Moon depend on how much of the sunlit half
can be seen at any one time. In the phase called the new
moon, the face is completely in shadow. About a week
later, the Moon is in first quarter, resembling a luminous
half-circle; another week later, the full moon shows its
fully lighted surface; a week afterward, in its last
quarter, the Moon appears as a half-circle again. The
entire cycle is repeated each lunar month. The Moon is
full when it is farther away from the Sun than Earth; it
is new when it is closer. When it is more than half
illuminated, it is said to be in gibbous phase. The Moon
is said to be waning when it progresses from full to new,
and to be waxing as it proceeds again to full.
Temperatures on its surface are extreme, ranging from a
maximum of 127°C (261°F) at lunar noon to a minimum of
-173°C (-279°F) just before lunar dawn.
This
information has brought it to you from Encarta 2002
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