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
It is owing to refraction, that we cannot judge so accurately of
magnitudes and distances in water as in air. A fish looks considerably
larger in water than when taken out of it. An object plunged
_vertically_ into water always appears contracted, and the more so as
its upper extremity approaches nearer the surface of the water. Every
thing remaining in the same situation, if we take the object gradually
out of the water, and it be of a slender form, we shall see it become
larger and larger, by a rapid developement, as it were, of all its
parts. The distortion of objects, seen through a crooked pane of glass
in a window, likewise arises from its unequal refraction of the rays
that pass through it. It has been calculated that in looking through
the common glass of a window, objects appear about the one thirtieth of
an inch out of their real place, by means of the refraction.
Refraction likewise produces an effect upon the _heavenly bodies_, so
that their apparent positions are generally different from their real.
By the refractive power of the atmosphere, the sun is seen before he
comes to the horizon in the morning, and after he sinks beneath it in
the evening; and hence this luminary is never seen in the place in
which it really is, except when it passes the zenith at noon, to places
within the torrid zone. The sun is visible, when actually thirty-two
minutes of a degree below the horizon, and when the opake rotundity of
the earth is interposed between our eye and that orb, just on the same
principle as, in the experiment with the shilling and basin of water,
the shilling was seen when the edge of the basin interposed between it
and the sight. The refractive power of the atmosphere has been found
to be much greater, in certain cases, than what has been now stated.
In the year 1595 a company of Dutch sailors having been wrecked on
the shores of Nova Zembla, and having been obliged to remain in that
desolate region during a night of more than three months--beheld the
sun make his appearance in the horizon about sixteen days before the
time in which he should have risen according to calculation, and when
his body was actually more than four degrees below the horizon; which
circumstance has been attributed to the great refractive power of the
atmosphere in those intensely cold regions. This refraction of the
atmosphere, which renders the apparent rising and setting of the sun
both earlier and later than the real, produces at least one important
beneficial effect. It procures for us the benefit of a much longer day,
at all seasons of the year, than we should enjoy, did not this property
of the atmosphere produce this effect. It is owing to the same cause
that the disks of the sun and moon appear elliptical or oval, when seen
in the horizon, their horizontal diameters appearing longer than their
vertical--which is caused by the greater refraction of the rays coming
from the lower limb, which is immersed in the densest part of the
atmosphere.
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