Side-Lights on Astronomy and Kindred Fields of Popular ScienceNewcomb, Simon
Science
Side-Lights on Astronomy and Kindred Fields of Popular Science
Newcomb, Simon
Astronomy; Compass; Flying-machines; Hyperspace; Learning and scholarship; Rain-making
Within the past three years a wobbling of the earth's axis has been
discovered, which takes place within a circle thirty feet in radius and
sixty feet in diameter. Its effect was noticed in astronomical
observations many years ago, but the change it produced was so small
that men could not find out what the matter was. The exact nature and
amount of the wobbling is a work of the exact astronomy of the present
time.
We cannot measure across oceans from island to island. Until a recent
time we have not even measured across the continent, from New York to
San Francisco, in the most precise way. Without astronomy we should
know nothing of the distance between New York and Liverpool, except by
the time which it took steamers to run it, a measure which would be
very uncertain indeed. But by the aid of astronomical observations and
the Atlantic cables the distance is found within a few hundred yards.
Without astronomy we could scarcely make an accurate map of the United
States, except at enormous labor and expense, and even then we could
not be sure of its correctness. But the practical astronomer being able
to determine his latitude and longitude within fifty yards, the
positions of the principal points in all great cities of the country
are known, and can be laid down on maps.
The world has always had to depend on astronomy for all its knowledge
concerning times and seasons. The changes of the moon gave us the first
month, and the year completes its round as the earth travels in its
orbit. The results of astronomical observation are for us condensed
into almanacs, which are now in such universal use that we never think
of their astronomical origin. But in ancient times people had no
almanacs, and they learned the time of year, or the number of days in
the year, by observing the time when Sirius or some other bright star
rose or set with the sun, or disappeared from view in the sun's rays.
At Alexandria, in Egypt, the length of the year was determined yet more
exactly by observing when the sun rose exactly in the east and set
exactly in the west, a date which fixed the equinox for them as for us.
More than seventeen hundred years ago, Ptolemy, the great author of The
Almagest, had fixed the length of the year to within a very few
minutes. He knew it was a little less than 365 1/2 days. The dates of
events in ancient history depend very largely on the chronological
cycles of astronomy. Eclipses of the sun and moon sometimes fixed the
date of great events, and we learn the relation of ancient calendars to
our own through the motions of the earth and moon, and can thus measure
out the years for the events in ancient history on the same scale that
we measure out our own.
Public-domain text, read in full here on John Shaqi.
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