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Stonehenge. The
most famous megalithic site in the world. Construction was begun in about
2800 BCE. and continued for over 1000 years. It was first noted in 1721
that the central Avenue was directed toward the summer solstice sunrise.
More recently, many other astronomical relationships have been claimed,
to such an extent that some consider Stonehenge a sophisticated prehistoric
astronomical computer.
I don't believe that such a
conclusion can be made. It is important to realize that with the erosion
of the stones, and their settling and shifting over several thousand years,
it is not really possible to say with a high degree of precision what
their original positions were, nor where exactly on the stones measurements
should be made. With resulting position errors on the order of a degree
or more, no complex astronomical relationships can be ascertained (or
rather, any number of fanciful ones may be derived.) Certainly, like other
early henges, the stones were set up to either predict or indicate the
summer solstice, and possibly a few other seasonal events. The Neolithic
and Bronze Age farmers who built it must have long understood methods
of predicting the solstices given the importance of such knowledge to
their agriculture. It seems likely to me that Stonehenge was not an astronomical
site, but rather a religious one that was built the way it was in order
to make a spiritual connection with the forces of nature that so determined
the fate of its builders.
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Royal Greenwich Observatory.
Less ancient than Stonehenge by four and a half millennia, this observatory
marks one of the birthing grounds of modern positional astronomy. It was
chartered in 1675 by Charles II for the purpose of finding a method of determining
longitude by ships at sea. It had long been possible to accurately determine
latitude by measuring the altitude of Polaris, or the Sun or Moon crossing
the meridian. But measuring longitude requires an accurate knowledge of
the time, and accurate positions of the stars, Sun, Moon, planets, and even
the moons of Jupiter. For most of its history, these measurements were central
to the operation of the observatory. |
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