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On November 8, the planet Mercury made one of its journeys across the face
of the sun, as seen from Earth. While following their own separate orbits
around the sun, it just so happened that on this date, Mecury and the Earth
were in a direct line with the sun. As Mercury is somewhat closer
to the sun, observers on Earth saw the planet move slowly across the sun's
disk.
The entire event started at about 11:12 (Pacific) and lasted about
5 hours.
In the image at left, which was taken about an hour into the transit,
Mercury can be seen as a small round dot at approximately the "one-o'clock"
position. (A sunspot also appears at the edge of the disk.)
In the image below right, taken about an hour later, Mercury has
moved noticeably. A closeup of the planet, which appears decidedly
round in shape, is in the image below.
(South
is at top, for all images on this page. )
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The full disk of the sun can be seen above, with Mercury now having moved
across the center line of the disk. More sunspots can be seen at the
left edge of the sun.
A transit event is much like a solar eclipse. In an eclipse.
the moon moves in front of the sun. Although much smaller in size
than the sun, the Moon is a great deal closer to us, so appears to be
approximately the same size as the sun in the sky; thus, it can block
the view of the solar disk.
This is generally the same general phenomenon that happens during
a transit. The difference is that the object that crosses the
sun appears to be much smaller than the sun itself, due to its size and
much greater distance from the earth.
In the last image, at right, Mercury has moved farther, and is
about 90 minutes from "egress"--the end of the transit, at which the
planet finally moves off the disk.
A transit of Mercury across the sun happens about 13 times per
century, and occurs only when Mercury, the Earth, and the sun are in
a direct line.
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