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The Planets .... brought to you by QuasArt Web Designs.
M
E R C U R Y (1st planet from the Sun)
In Roman mythology Mercury is the god of commerce, travel and thievery,
the Roman counterpart of the Greek god Hermes, the messenger of the
Gods.
The planet probably received this name because it moves so quickly across
the sky.
CHAPTERS
I
II
III
NO MOONS
INTRODUCTION
I


The
planet closest to the sun. Its mean distance from the sun is approximately
58 million km (about 36 million mi); its diameter is 4875 km (3030
mi); its volume and mass are about 1/18 that
of Earth; and its mean density is approximately equal to that of Earth.
Mercury revolves about
the sun in a period of 88 days. Radar observations of the planet show
that its period of rotation is 58.7 days, or two-thirds of its period
of revolution. The planet, therefore, rotates one and a half times
during each revolution. Because its surface consists of rough, porous,
dark-colored rock, Mercury is a poor reflector of sunlight. Mariner
10 also detected a magnetic field about 1 percent that of Earth, making
Mercury the only other planet with density and composition close to
that of Earth to have a magnetic field. Because it has a magnetic
field, the outer core of the planet must be a liquid iron compound,
which produces a magnetic field as it moves. Scientists believe Mercury's
crust acts as an effective insulator to keep the planet's outer core
liquid despite the very cold temperatures on the dark side of the
planet.

Spectroscopic studies indicate that only an extremely thin atmosphere,
containing sodium and potassium, exists on Mercury, its atoms apparently
diffusing from the crust of the planet. Collisions with other protoplanets
early in the history of the solar system may have stripped away lighter
materials, thereby accounting for Mercury's great density. The force
of gravity on the planet's surface is about one-third of that on Earth's
surface. The Mariner 10 spacecraft passed Mercury twice in 1974 and
once in 1975. It sent back pictures of a moonlike, crater-pocked surface
and reported temperatures to be about 430° C (about 810° F) on the
sunlit side and about -180° C (about -290° F) on the dark side. Unlike
that of Earth's moon, the surface of Mercury is criss-crossed by long
escarpments, or cliffs, dating perhaps from the period of contraction
the planet experienced as it cooled some time early in its history.
In 1991 powerful radio telescopes
on Earth revealed unmistakable signals of vast sheets of ice in Mercury's
polar regions, areas that had not been covered by Mariner 10. The
point in Mercury's orbit at which the planet is closest to the sun
(the perihelion) moves a tiny amount every orbit, but too much to
be accounted for by the force of gravity
from other planets. A full explanation of the changes in Mercury's
perihelion was one of the first confirmations of the theory of relativity.
TOP
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RECOMMENED READING
II
COMING
SOON
WEB LINKS
III
COMING SOON
TOP
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T
H E
P L A N E T S
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Planets
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Sun
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Mercury |
Venus | Earth
| Mars | Jupiter
| Saturn |
Uranus |
Neptune |
Pluto
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