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
Hence we may learn the absurdity and futility of attempting to
describe the extent of spaces in the heavens, by saying, that a
certain phenomenon was two or three feet or yards distant from
another, or that the tail of a comet appeared several yards in length.
Such representations can convey no definite ideas in relation to
such magnitudes, unless it be specified at what distance from the
eye, the foot or yard is supposed to be placed. If a rod, a yard
in length, be held at nine inches from the eye, it will subtend an
angle, or cover a space in the heavens, equal to more than one fourth
of the circumference of the sky, or about one hundred degrees. If
it be eighteen inches from the eye, it will cover a space equal to
fifty degrees; if at three feet, twenty-five degrees, and so on in
proportion to the distance from the eye; so that we can form no correct
conceptions of apparent spaces or distances in the heavens, when we
are merely told that two stars, for example, appear to be three yards
distant from each other. The only definite measure we can use, in such
cases, is that of degrees. The sun and moon are about half a degree
in apparent diameter, and the distance between the extreme stars in
_Orion’s belt_, three degrees, which measures being made familiar
to the eye, may be applied to other spaces of the heavens, and an
approximate idea conveyed of the relative distances of objects in the
sky.
From what has been stated above, it is evident that the magnitude
of objects may be considered in different points of view. The true
dimensions of an object, considered in itself, give what is called its
_real_ or _absolute magnitude_; and the opening of the visual angle
determines the _apparent magnitude_. The real magnitude, therefore, is
a constant quantity; but the apparent magnitude varies continually with
the distance, real or imaginary; and therefore, if we always judged
of the dimensions of an object from its apparent magnitude, every
thing around us would, in this respect, be undergoing very sensible
variations, which might lead us into strange and serious mistakes. A
fly, near enough to the eye, might appear under an angle as great as
an elephant at the distance of twenty feet, and the one be mistaken for
the other. A giant eight feet high, seen at the distance of twenty-four
feet, would not appear taller than a child two feet in height, at the
distance of six feet; for both would be seen nearly under the same
angle. But our experience generally prevents us from being deceived by
such illusions. By the help of touch, and by making allowance for the
different distances at which we see particular objects, we learn to
correct the ideas we might otherwise form from attending to the optical
angle alone, especially in the case of objects that are near us. By the
sense of touch we acquire an impression of the distance of an object;
this impression combines itself with that of the apparent magnitude,
Public-domain text, read in full here on John Shaqi.
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