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
It is a remarkable circumstance, and which would naturally excite
admiration, were it not so common and well known, that _when the rays
of light from any object are refracted through a convex lens, they
paint a distinct and accurate picture of the object before it, in all
its colours, shades, and proportions_. Previous to experience, we
could have had no conception that light, when passing through such
substances, and converging to a point, could have produced so admirable
an effect,--an effect on which the construction and utility of all our
optical instruments depend. The following figure will illustrate this
position. Let L, N, represent a double convex lens, A, C, _a_, its
axis, and OB, an object perpendicular to it. A ray passing from the
extremity of the object at O, after being refracted by the lens at F,
will pass on in the direction FI, and form an image of that part of the
object at I. This ray will be the axis of all the rays which fall on
the lens from the point O, and I will be the focus where they will all
be collected. In like manner BCM, is the axis of that parcel of rays
which proceed from the extremity of the object B, and their focus will
be at M; and since all the points in the object between O, and B, must
necessarily have their foci between I and M, a complete picture of the
points from which they come will be depicted, and consequently an image
of the whole object OB.
[Illustration: _figure 13._]
It is obvious, from the figure, that the image of the object is
formed in the focus of the lens, in an _inverted position_. It must
necessarily be in this position, as the rays cross at C, the centre of
the lens; and as it is impossible that the rays from the upper part
of the object O, can be carried by refraction to the upper end of
the image at M. This is a universal principle in relation to convex
lenses of every description, and requires to be attended to in the
construction and use of all kinds of telescopes and microscopes. It
is easily illustrated by experiment. Take a convex lens of eight,
twelve, or fifteen inches focal distance, such as a reading glass, or
the glass belonging to a pair of spectacles, and holding it, at its
focal distance from a white wall, in a line with a burning candle, the
flame of the candle will be seen depicted on the wall in an inverted
position, or turned upside down. The same experiment may be performed
with a window-sash, or any other bright object. But, the most beautiful
exhibition of the images of objects formed by convex lenses, is made
by darkening a room, and placing a convex lens of a long focal distance
in a hole cut out of the window-shutter; when a beautiful inverted
landscape, or picture of all the objects before the window, will be
painted on a white paper or screen placed in the focus of the glass.
The image thus formed exhibits not only the proportions and colours,
but also the motions of all the objects opposite the lens, forming as
it were a living landscape.
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