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
If rays proceeding from a distant object fall upon a concave speculum,
they will paint an image or representation of the object on its focus
_before_ the mirror. This image will be inverted, because the rays
cross at the points where the image is formed. We have already seen
that a convex glass forms an image of an object _behind_ it; the rays
of light from objects _pass through_ the glass, and the picture is
formed on the side farthest from the object. But in concave mirrors
the images of distant objects--and of all objects that are farther
from its surface than its principal focus--are formed _before_ the
mirror, or on the same side as the object. In almost every other
respect, however, the effect of a concave mirror is the same as that
of a convex lens, in regard to the formation of images, and the course
pursued by the rays of light, except that the effect is produced in the
one case by refraction, and in the other by reflection. The following
figure represents the manner in which images are formed by concave
mirrors. GF represents the reflecting surface of the mirror; OAB, the
object; and IAM, the image formed by the mirror. The rays
proceeding from O, will be carried to the mirror, in the direction OG,
and according to the law that the angle of incidence is equal to the
angle of reflection, will be reflected to I, in the direction GI. In
like manner the rays from B, will be reflected from F to M, the rays
from A, will be reflected to a, and so of all the intermediate rays, so
that an inverted image of the object OB, will be formed at IM. If the
rays proceeded from objects at a very great distance the image would be
formed in the real focus of the mirror, or at one-fourth the diameter
of the sphere from its surface; but near objects, which send forth
diverging rays, will have their images formed a little farther from the
surface of the mirror.
[Illustration: _figure 22._]
If we suppose a real object placed at IM, then OB will represent its
magnified image, which will be larger than the object, in proportion to
its distance from the mirror. This may be experimentally illustrated
by a concave mirror and a candle. Suppose a concave mirror whose focal
distance is five inches, and that a candle is placed before it, at
a little beyond its focus, (as at IM)--suppose at five and a half
inches,--and that a wall or white screen receives the image, at the
distance of five feet six inches from the mirror, an image of the
candle will be formed on the wall which will be twelve times longer
and broader than the candle itself. In this way concave mirrors may be
made to magnify the images of objects to an indefinite extent. This
experiment is an exact counterpart of what is effected in similar
circumstances by a convex lens, as described p. 74; the mirror
performing the same thing by reflection, as the lens did by refraction.
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