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
Light, which embellishes with so much magnificence a pure and serene
sky, by means of innumerable bright starry orbs which are spread over
it, sometimes, in a dark and cloudy sky, exhibits an ornament which,
by its pomp, splendour and variety of colours, attracts the attention
of every eye that has an opportunity of beholding it. At certain
times, when there is a shower either around us, or at a distance from
us in an opposite quarter to that of the sun, a species of arch or
bow is seen in the sky, adorned with all the seven primary colours of
light. This phenomenon, which is one of the most beautiful meteors in
nature, has obtained the name of the RAINBOW. The rainbow was,
for ages, considered as an inexplicable mystery, and by some nations
it was adored as a deity. Even after the dawn of true philosophy,
it was a considerable time before any discovery of importance was
made, as to the true causes which operate in the production of this
phenomenon. About the year 1571, M. Fletcher of Breslau, made a certain
approximation to the discovery of the true cause, by endeavouring to
account for the colours of the rainbow by means of a double refraction
and one reflection. A nearer approximation was made by Antonio de
Dominis, bishop of Spalatro, about 1601. He maintained that the
double refraction of Fletcher, _with an intervening reflection_,
was sufficient to produce the colours of the bow, and also to bring
the rays that formed them to the eye of the spectator, without any
subsequent reflection. To verify this hypothesis, he procured a small
globe of solid glass, and viewing it when it was exposed to the rays
of the sun--with his back to that luminary--in the same manner as he
had supposed the drops of rain were situated with respect to them, he
observed the same colours which he had seen in the rainbow, and in
the same order. But he could give no good reason _why_ the bow should
be coloured, and much less any satisfactory account of the _order_ in
which the colours appear. It was not till Sir I. Newton discovered
the different refrangibility of the rays of light, that a complete
and satisfactory explanation could be given of all the circumstances
connected with this phenomenon.
As the full elucidation of this subject involves a variety of optical
and mathematical investigations, I shall do little more than explain
the general principle on which the prominent phenomena of the rainbow
may be accounted for, and some of the facts and results which theory
and observation have deduced.
Public-domain text, read in full here on John Shaqi.
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