The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomyDick, Thomas
Science
The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomy
Dick, Thomas
Astronomical instruments; Astronomy; Telescopes
In the operation of the law of refraction in these and numerous other
instances, we have a specimen of the diversified and beneficent effects
which the Almighty can produce by the agency of a single principle in
nature. By the influence of the simple law of gravitation, the planets
are retained in their orbits, the moon directed in her course around
the earth, and the whole of the bodies connected with the sun preserved
in one harmonious system. By the same law the mountains of our globe
rest on a solid basis, the rivers flow through the plains toward the
seas, the ocean is confined to its prescribed boundaries, and the
inhabitants of the earth are retained to its surface and prevented
from flying upwards through the voids of space. In like manner the law
by which light is refracted produces a variety of beneficial effects
essential to the present constitution of our world and the comfort
of its inhabitants. When a ray of light enters obliquely into the
atmosphere, instead of passing directly through, it bends a little
downwards, so that the greater portion of the rays which thus enter the
atmospheric mass, descend by inflection to the earth. We then enjoy
the benefit of that light which would otherwise have been totally
lost. We perceive the light of day an hour before the solar orb makes
its appearance, and a portion of its light is still retained when
it has descended nearly eighteen degrees below our horizon. We thus
enjoy, throughout the year, seven hundred and thirty hours of light
which would have been lost, had it not been refracted down upon us
from the upper regions of the atmosphere. To the inhabitants of the
polar regions this effect is still more interesting and beneficial.
Were it not for their twilight, they would be involved, for a much
longer period than they now are, in perpetual darkness; but by the
powerful refraction of light which takes place in the frigid zones, the
day sooner makes its appearance towards spring, and their long winter
nights are, in certain cases, shortened by a period of thirty days.
Under the poles, where the darkness of night would continue six months
without intermission, if there were no refraction, total darkness does
not prevail during the one half of this period. When the sun sets, at
the North pole about the 23rd of September, the inhabitants (if any)
enjoy a perpetual aurora, till he has descended 18 degrees below the
horizon. In his course through the ecliptic the sun is two months
before he can reach this point, during which time there is a perpetual
twilight. In two months more he arrives again at the same point, namely
18 degrees below the horizon, when a new twilight commences, which is
continually increasing in brilliancy, for other two months, at the end
of which the body of this luminary is seen rising in all its glory.
So that, in this region, the light of day is enjoyed, in a greater or
less degree, for ten months without interruption, by the effects of
Public-domain text, read in full here on John Shaqi.
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