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
The effect of refraction, in respect to _terrestrial_ objects, is
likewise of a beneficial nature. The quantity of this refraction
is estimated by Dr. Maskelyne at one-tenth of the distance of the
object observed, expressed in degrees of a great circle. Hence, if
the distance be 10,000 fathoms, its tenth part 1000 fathoms, is the
sixtieth part of a degree, or one minute, which is the refraction
in altitude. Le Gendre estimates it at one fourteenth; De Lambre at
one eleventh; and others at a twelfth of the distance; but it must
be supposed to vary at different times and places according to the
varying state of the atmosphere. This refraction, as it makes objects
appear to be raised higher than they really are, enlarges the extent
of our landscapes, and enables us to perceive distant objects which
would otherwise have been invisible. It is particularly useful to
the navigator at sea. It is one important object of the mariner when
traversing his course, to look out for capes and headlands, rocks and
islands, so as to descry them as soon as they are within the reach
of his eye. Now, by means of refraction, the tops of hills and the
elevated parts of coasts, are apparently raised into the air, so that
they may be discovered several leagues further off on the sea than
they would be, did no such refractive power exist. This circumstance
is therefore a considerable benefit to the science of navigation, in
enabling the mariner to steer his course aright, and to give him the
most early warning of the track he ought to take, or of the dangers to
which he may be exposed.
In short, the effects produced by the refraction and reflection of
light on the scenery connected with our globe, teach us that these
principles, in the hand of the Almighty, might be so modified and
directed, as to produce the most picturesque, the most glorious and
wonderful phenomena, such as mortal eyes have never yet seen, and of
which human imagination can form no conception; and in other worlds,
more resplendent and magnificent than ours, such scenes may be fully
realized, in combination with the operation of physical principles and
agents, with which we are at present unacquainted. From what we already
know of the effects of the reflection and the refraction of light, it
is not beyond the bounds of probability to suppose, that in certain
regions of the universe, light may be reflected and refracted through
different mediums, in such a manner, as to present to the view of
their inhabitants the prominent scenes connected with distant systems
and worlds, and to an extent, as shall infinitely surpass the effects
produced by our most powerful telescopes.
CHAPTER III.
ON THE REFRACTION OF LIGHT THROUGH SPHERICAL TRANSPARENT SUBSTANCES, OR
LENSES.
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