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 describing the common refracting telescope, (p. 228.) I have
noticed that three eye-glasses, placed at double their focal distances
from each other, formerly constituted the terrestrial eye-piece,
as represented in fig. 47. But this construction, especially for
achromatic instruments, has now become obsolete, and is never used,
except in small pocket spy-glasses formed with a single object lens. In
its place a four glassed eye-piece has been substituted, which is now
universally used in all good telescopes, and which, besides improving
the vision and producing an erect position of the images of objects,
presents a considerably larger field of view. During the progressive
stages of improvement made in the construction of erect eye-pieces by
Dollond and Ramsden, three, four, and five lenses were successively
introduced; and hence, in some of the old telescopes constructed by
these artists, we frequently find five lenses of different descriptions
composing the eye-piece. But four lenses, arranged in the manner I
am now about to describe, have ultimately obtained the preference.
In a telescope having a celestial eye-piece of the Huygenian form,
the image that is formed in the focus of the object glass, is that
which is seen magnified, and in an inverted position; but when a four
glassed eye-piece is used, which produces an erect view of the object,
the image is repeated, and the _second_ image, which is formed by
the inner pair of lenses AB on an enlarged scale, is that which the
pair of lenses CD at the eye-end render visible on a scale still more
enlarged. The modern terrestrial eye-piece, represented in fig. 79,
is, in fact, nothing else than a compound microscope, consisting of an
object lens, an amplifying lens, and an eye-piece composed of a pair
of lenses on the principle of the Huygenian eye-piece. Its properties
will be best understood by considering the first image of an object,
which is formed in the focus of the object glass, as a small luminous
object to be rendered visible, in a magnified state, by a compound
microscope. The object to be magnified may be considered as placed near
the point A, and the magnified image at _i_, which is viewed by the
lens D. Hence, if we look through such an eye-piece at a small object
placed very near the lens A, we shall find that it acts as a compound
microscope of a moderate magnifying power increasing, in some cases,
the diameter of the object about 10 times, and 100 times in surface.
[Illustration: _figure 79._]
Public-domain text, read in full here on John Shaqi.
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