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 object of this construction is to render a small disc of
flint-glass available to perform the office of compensation to a much
larger one of crown-glass, and thus to render possible the construction
of telescopes of much larger aperture than are now common, without
hindrance from the difficulty at present experienced in procuring large
discs of flint-glass. It is well known to those who are acquainted
with telescopes, that in the construction of an ordinary achromatic
object-glass, in which a single crown lens is compensated by a single
one of flint, the two lenses admit of being separated only by an
interval too small to afford any material advantage, _in diminishing
the diameter of the flint lens_, by placing it in a narrower part
of the cone of rays--the actual amount of their difference in point
of dispersive power being such as to render the correction of the
chromatic aberration impossible, when their mutual distance exceeds
a certain limit. This inconvenience Mr. Rogers proposes to obviate,
by employing, as a correcting lens--not a single lens of flint, but a
compound one consisting of a convex crown and concave flint, whose foci
are such as to cause their combination to act as a plain glass on the
mean refrangible rays. Then it is evident, that by means of the greater
dispersive power of flint than of crown glass, this will act as a
concave on the violet, and as a convex on the red rays, and _that_ the
more powerfully, according as the lenses separately have greater powers
or curvature. If then, such a compound lens be interposed between the
object-glass of a telescope--supposed to be a single lens of plate or
crown-glass--and its focus, it will cause no alteration in the focus
for mean rays, while it will lengthen the focus for violet, and shorten
it for red rays. Now this is precisely what is wanted to produce an
achromatic union of all the rays in the focus; and as nothing in this
construction limits the powers of the individual correcting lenses,
they may therefore be applied any where that convenience may dictate;
and thus, theoretically speaking, a disc of flint-glass, however small,
may be made to correct the colour of one of crown however large.
Public-domain text, read in full here on John Shaqi.
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