The Science of the StarsMaunder, E. Walter (Edward Walter)
History
The Science of the Stars
Maunder, E. Walter (Edward Walter)
Astronomy
The old proverb has it that "Science is measurement," and of none of
the sciences is this so true as of the science of astronomy. Indeed
the measurement of time by observation of the movements of the heavenly
bodies was the beginning of astronomy. The movement of the Sun gave
the day, which was reckoned to begin either at sunrise or at sunset.
The changes of the Moon gave the month, and in many languages the root
meaning of the word for _Moon_ is "measurer." The apparent movement of
the Sun amongst the stars gave a yet longer division of time, the year,
which could be determined in a number of different ways, either from
the Sun alone, or from the Sun together with the stars. A very simple
and ancient form of instrument for measuring this movement of the Sun
was the obelisk, a pillar with a pointed top set up on a level
pavement. Such obelisks were common in Egypt, and one of the most
celebrated, known as Cleopatra's Needle, now stands on the Thames
Embankment. As the Sun moved in the sky, the shadow of the pillar
moved on the pavement, and midday, or noon, was marked when the shadow
was shortest. The length of the shadow at noon varied from day to day;
it was shortest at mid-summer, and longest at midwinter, _i.e._ at the
summer and winter solstices. Twice in the year the shadow of the
pillar pointed due west at sunrise, and due east at {43} sunset--that
is to say, the shadow at the beginning of the day was in the same
straight line as at its end. These two days marked the two equinoxes
of spring and autumn.
The obelisk was a simple means of measuring the height and position of
the Sun, but it had its drawbacks. The length of the shadow and its
direction did not vary by equal amounts in equal times, and if the
pavement upon which the shadow fell was divided by marks corresponding
to equal intervals of time for one day of the year, the marks did not
serve for all other days.
But if for the pillar a triangular wall was substituted--a wall rising
from the pavement at the south and sloping up towards the north at such
an angle that it seemed to point to the invisible pivot of the heavens,
round which all the stars appeared to revolve--then the shadow of the
wall moved on the pavement in the same manner every day, and the
pavement if marked to show the hours for one day would show them for
any day. The sundials still often found in the gardens of country
houses or in churchyards are miniatures of such an instrument.
Public-domain text, read in full here on John Shaqi.
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