Mercury is the closest
planet to the Sun and the eighth largest. Mercury is slightly
smaller in diameter than the moons Ganymede and Titan but more than
twice as massive.
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.
Since it is closer to the
Sun than the Earth, the illumination of Mercury's disk varies when
viewed with a telescope from our perspective. Galileo's telescope
was too small to see Mercury's phases but he did see the phases of
Venus.
Mercury's orbit is highly
eccentric; at perihelion it is only 46 million km from the Sun but
at aphelion it is 70 million. The position of the perihelion
precesses around the Sun at a very slow rate. 19th century
astronomers made very careful observations of Mercury's orbital
parameters but could not adequately explain them using Newtonian
mechanics. The tiny differences between the observed and predicted
values were a minor but nagging problem for many decades. It was
thought that another planet (sometimes called Vulcan) slightly
closer to the Sun than Mercury might account for the discrepancy.
But despite much effort, no such planet was found. The real answer
turned out to be much more dramatic: Einstein's General Theory of
Relativity! Its correct prediction of the motions of Mercury was an
important factor in the early acceptance of the theory.
Temperature variations on
Mercury are the most extreme in the solar system ranging from 90 K
to 700 K.
Mercury actually has a
very thin atmosphere consisting of atoms blasted off its surface by
the solar wind. Because Mercury is so hot, these atoms quickly
escape into space. Thus in contrast to the Earth and Venus whose
atmospheres are stable, Mercury's atmosphere is constantly being
replenished.
The
surface of Mercury exhibits enormous escarpments, some up to
hundreds of kilometers in length and as much as three kilometers
high. Some cut thru the rings of craters and other features in such
a way as to indicate that they were formed by compression. It is
estimated that the surface area of Mercury shrank by about 0.1% (or
a decrease of about 1 km in the planet's radius).
Mercury has a small
magnetic field whose strength is about 1% of Earth's.
Mercury
has no known satellites.
Mercury
is often visible with binoculars or even the unaided eye, but it is
always very near the Sun and difficult to see in the twilight
sky.
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