Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
The _longitude_ of a place may be found by any method, by which we may
ascertain how much its time of day differs from that of Greenwich at the
same moment. A place that lies eastward of another comes to the meridian
an hour earlier for every fifteen degrees of longitude, and of course
has the hour of the day so much in advance of the other, so that it
counts one o'clock when the other place counts twelve. On the other
hand, a place lying westward of another comes to the meridian later by
one hour for every fifteen degrees, so that it counts only eleven
o'clock when the other place counts twelve. Keeping these principles in
view, it is easy to see that a comparison of the difference of time
between two places at the same moment, allowing fifteen degrees for an
hour, sixty minutes for every four minutes of time, and sixty seconds
for every four seconds of time, affords us an accurate mode of finding
the difference of longitude between the two places. This comparison may
be made by means of a chronometer, or from solar or lunar eclipses, or
by what is called the lunar method of finding the longitude.
_Chronometers_ are distinguished from clocks, by being regulated by
means of a balance-wheel instead of a pendulum. A watch, therefore,
comes under the general definition of a chronometer; but the name is
more commonly applied to larger timepieces, too large to be carried
about the person, and constructed with the greatest possible accuracy,
with special reference to finding the longitude. Suppose, then, we are
furnished with a chronometer set to Greenwich time. We arrive at New
York, for example, and compare it with the time there. We find it is
five hours in advance of the New-York time, indicating five o'clock,
P.M., when it is noon at New York. Hence we find that the longitude of
New York is 5×15=75 degrees.[11] The time at New York, or any individual
place, can be known by observations with the transit-instrument, which
gives us the precise moment when the sun is on the meridian.
It would not be necessary to resort to Greenwich, for the purpose of
setting our chronometer to Greenwich time, as it might be set at any
place whose longitude is known, having been previously determined. Thus,
if we know that the longitude of a certain place is exactly sixty
degrees east of Greenwich, we have only to set our chronometer four
hours behind the time at that place, and it will be regulated to
Greenwich time. Hence it is a matter of the greatest importance to
navigation, that the longitude of numerous ports, in different parts of
the earth, should be accurately determined, so that when a ship arrives
at any such port, it may have the means of setting or verifying its
chronometer.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account