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
Mr. Walker illustrates the manner in which we see our faces in a mirror
by the following figure (16). AB represents a mirror, and
OC, a person looking into it. If we conceive a ray proceeding from
the forehead CE, it will be sent to the eye at O,
agreeably to the angle of incidence and reflection. But the mind puts
CEO into one line, and the forehead is seen at H,
as if the lines CEO had turned on a hinge at E.--It
seems a wonderful faculty of the mind to put the two oblique lines
CE and OE into one straight line OH, yet
it is seen every time we look at a mirror. For the ray has really
travelled from C to E, and from E to
O, and it is that journey which determines the distance of the
object; and hence we see ourselves as far beyond the mirror as we stand
from it. Though a ray is here taken only from one part of the face, it
may be easily conceived that rays from every other part of the face
must produce a similar effect.
[Illustration: _figure 16._]
In every plain mirror, the image is always equal to the object, at what
distance soever it may be placed; and as the mirror is only at half
the distance of the image from the eye, it will completely receive an
image of _twice_ its own length. Hence a man six feet high may view
himself completely in a looking glass of three feet in length, and
half his own breadth; and this will be the case at whatever distance
he may stand from the glass. Thus, the man AC (fig. 17) will see the
whole of his own image in the glass AB, which is but one half
as large as himself. The rays from the head pass to the mirror in the
line AA, perpendicular to the mirror, and are returned to the
eye in the same line; consequently, having travelled twice the length
AA, the man must see his head at B. From his feet C rays
will be sent to the bottom of the mirror at B; these will be
reflected at an equal angle to the eye in the direction BA, as
if they had proceeded in the direction DBA, so that the man
will see his foot at D, and consequently his whole figure at BD.
[Illustration: _figure 17._]
Public-domain text, read in full here on John Shaqi.
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