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
When light is thus refracted, or has taken a new direction, it then
proceeds invariably in a straight line till it meets with a different
medium,[7] when it is again turned out of its course. It must be
observed, however, that though we may by this means cause the rays of
light to make any number of angles in their course, it is impossible
for us to make them describe a curve, except in one single case,
namely, where they pass through a medium, the density of which either
uniformly increases or diminishes. This is the case with the light of
the celestial bodies, which passes downwards through our atmosphere,
and likewise with that which is reflected upwards through it by
terrestrial objects. In both these cases it describes a curve of the
hyperbolic kind; but at all other times, it proceeds in straight lines,
or in what may be taken for straight lines without any sensible error.
There are two circumstances essential to refraction. 1. That the rays
of light shall pass out of one medium into another of a different
density, or of a greater or less degree of resistance. 2. That they
pass in an _oblique_ direction. The denser the refracting medium, or
that into which the ray enters, the greater will be its refracting
power; and of two refracting mediums of the same density, that which
is of an oily or inflammable nature will have a greater refracting
power than the other. The nature of refraction may be more particularly
explained and illustrated by the following figure and description.
Let ADHI fig. 2, be a body of water, AD its surface, C a point in which
a ray of light BC enters from the air into the water. This ray, by the
greater density of the water, instead of passing straight forward in
its first direction to K, will be bent at the point C, and pass along
in the direction CE, which is called the _refracted_ ray. Let the line
FG be drawn perpendicular to the surface of the water in C, then it
is evident that the ray BC, in passing out of air, a _rare_ medium,
into a _dense_ medium, as water, is refracted into a ray CE which is
_nearer_ to the perpendicular CG than the incident ray BC, and on the
contrary, the ray EC passing out of a denser medium into a rarer will
be refracted into CB, which is _farther_ from the perpendicular.
[Illustration: _figure 2._]
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