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 effects of _concave_ lenses are directly opposite to those of
convex. Parallel rays, striking one of those glasses, instead of
converging towards a point, are made to _diverge_. Rays already
divergent are rendered more so, and convergent rays are made less
convergent. Hence objects seen through concave glasses appear
considerably smaller and more distant than they really are. The
following diagram, fig. 12, represents the course of parallel rays
through a double concave lens, where the parallel rays T A, D E, I B,
&c., when passing through the concave glass A B, diverge into the rays
G L, E C, H P, &c., as if they proceeded from F, a point before the
lens, which is the principal focus of the lens.
[Illustration: _figure 12._]
The principal focal distance E F, is the same as in convex lenses.
Concave glasses are used to correct the imperfect vision of
short-sighted persons. As the form of the eye of such persons is too
convex, the rays are made to converge before they reach the optic
nerve; and therefore a concave glass, causing a little divergency,
assists this defect of vision, by diminishing the effect produced
by the too great convexity of the eye, and lengthening its focus.
These glasses are seldom used, in modern times, in the construction
of optical instruments, except as eye-glasses for small pocket
perspectives, and opera glasses.
_To find the focal distance of a concave glass._ Take a piece of
paste-board or card paper, and cut a round hole in it, not larger
than the diameter of the lens; and, on another piece of paste-board,
describe a circle whose diameter is just double the diameter of the
hole. Then apply the piece with the hole in it to the lens, and hold
them in the sun-beams, with the other piece at such a distance behind,
that the light proceeding from the hole may spread or diverge so as
precisely to fill the circle; then the distance of the circle from the
lens is equal to its virtual focus, or to its radius, if it be a double
concave, and to its diameter, if a plano-concave. Let _d, e_, (fig.
12,) represent the diameter of the hole, and _g, i_, the diameter of
the circle, then the distance C, I, is the virtual focus of the lens.[9]
The _meniscus_ represented at E, fig. 5, is like the crystal of a
common watch, and as the convexity is the same as the concavity,
it neither magnifies nor diminishes. Sometimes, however, it is
made in the form of a crescent, as at F, fig. 5, and is called a
_concavo-convex_ lens; and, when the convexity is greater than the
concavity, or, when it is thickest in the middle, it acts nearly in the
same way as a double or plano-convex lens of the same focal distance.
_Of the_ IMAGES _formed by convex lenses._
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