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 darkened chamber is frequently exhibited in a manner somewhat
different from what we have above described, as in the following
scheme, (fig. 38) which is termed the _revolving camera obscura_. In
this construction, KH represents a plane mirror or metallic reflector,
placed at half a right angle to the convex lens HI, by which, rays
proceeding from objects situated in the direction O are reflected to
the lens, which forms an image of the objects on a round white table
at T, around which several spectators may stand, and view the picture,
as delineated on a horizontal plane. The reflector, along with its
case, is capable of being turned round, by means of a simple apparatus
connected with it, so as to take in, in succession, all the objects
which compose the surrounding scene. But as the image here is received
on a flat surface, the rays _fm_, _en_, will have to diverge farther
than the central rays _dc_; and hence the representation of the
object, near the sides, will be somewhat distorted; to remedy which,
the image should be received on a concave surface, as _ab_ or PS. This
is the general plan of those Camera Obscuras, fitted up in large wooden
tents, which are frequently exhibited in our large cities, and removed
occasionally from one town to another. Were an instrument of this
kind fitted up on a _small scale_, a hole might be made in one of the
sides, as at E, where the eye could be applied to view the picture. The
focal distances of the lenses used in large instruments of this kind,
are generally from eight to twelve feet, in which case they produce
a telescopic effect upon distant objects, so as to make them appear
nearer than when viewed with the naked eye.
[Illustration: _figure 38._]
[Illustration: _figure 39._]
Public-domain text, read in full here on John Shaqi.
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