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 following figures, 48, 49, 50 represent the manner in which the
rays of light are refracted through the glasses of the telescopes we
have now described. Fig. 48 represents the rays of light as they pass
from the object to the eye in the Galilean telescope. After passing in
a parallel direction to the object-glass, they are refracted by that
glass, and undergo a slight convergence in passing towards the concave
eye-glass, where they enter the eye in a parallel direction, but no
image is formed previous to their entering the eye, till they arrive
at the retina. Fig. 49 represents the rays as they pass through the
glasses of the astronomical telescope. The rays, after entering the
object-glass, proceed in a converging direction, till they arrive at
its focus, about A, where an image of the object is formed; they then
proceed diverging to the eye-glass, where they are rendered parallel,
and enter the eye in that direction. Fig. 50 represents the rays as
they converge and diverge in passing through the four glasses of
the common day-telescope described above. After passing through the
object-glass, they converge towards B, where the first image is formed.
They then diverge towards the first eye-glass where they are rendered
parallel; and passing through the second eye-glass, they again converge
and form a second image at C; from which point they again diverge,
and passing through the first eye-glass enter the eye in a parallel
direction. If the glasses of these telescopes were fixed on long pieces
of wood, at their proper distances from each other, and placed in a
darkened room, when the sun is shining, the beam of the sun’s light
would pass through them in the same manner as here represented.
[Illustration: _fig. 48._]
[Illustration: _fig. 49._]
[Illustration: _fig. 50._]
SECT. 5.--TELESCOPE FORMED BY A SINGLE LENS.
This is a species of telescope altogether unnoticed by optical writers,
so far as I know; nor has the property of a single lens in magnifying
distant objects been generally adverted to or recognised. It may not
therefore be inexpedient to state a few experiments which I have made
in relation to this point. When we hold a spectacle-glass of a pretty
long focal distance--say, from 20 to 24 inches--close to the eye, and
direct it to distant objects, they do not appear sensibly magnified.
But if we hold the glass about 12 or 16 inches from our eye, we shall
perceive a sensible degree of magnifying power, as if distant objects
were seen at less than half the distance at which they are placed. This
property of a spectacle-glass I happened to notice when a boy, and, on
different occasions since that period have made several experiments on
the subject, some of which I shall here relate.
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