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
By making a hole in the screen LM opposite any one of the colours of
the spectrum, so as to allow that colour alone to pass--and by letting
the colour thus separated fall upon a second prism--Newton found that
the light of each of the colours was alike refrangible, because the
second prism could not separate them into an oblong image, or into
any other colour. Hence he called all the seven colours _simple_
or homogeneous, in opposition to _white_ light, which he called
_compound_ or heterogeneous. With the prism which this philosopher
used he found the lengths of the colours and spaces of the spectrum
to be as follows: Red, 45; Orange, 27; Yellow, 40; Green, 60; Blue,
60; Indigo, 48; Violet, 80: or 360 in all. But these spaces vary a
little with prisms formed of different substances, and as they are
not separated by distinct limits, it is difficult to obtain any thing
like an accurate measure of their relative extents. Newton examined
the ratio between the sines of incidence and refraction of these
decompounded rays (see p. 30,) and found that each of the seven primary
colour-making rays, had certain limits within which they were confined.
Thus let the sine of incidence in glass be divided into 50 equal
parts, the sine of refraction into air of the _least_ refrangible,
and the _most_ refrangible rays will contain respectively 77 and 78
such parts. The sines of refraction of all the degrees of _red_ will
have the intermediate degrees of magnitude, from 77 to 77 one-eighth;
_Orange_ from 77 one-eighth to 77 one-fifth; _Yellow_ from 77 one-fifth
to 77 one-third; _Green_ from 77 one-third to 77 one-half; _Blue_
from 77 one-half to 77 two-thirds; _Indigo_ from 77 two-thirds to 77
seven-ninths; and _Violet_ from 77 seven-ninths to 78.
From what has been now stated, it is evident that, in proportion as any
part of an optic glass bears a resemblance to the form of a prism, the
component rays that pass through it must be necessarily separated, and
will consequently paint or tinge the object with colours. The edges of
every convex lens approach to this form, and it is on this account that
the extremities of objects when viewed through them are found to be
tinged with the prismatic colours. In such a glass, therefore, those
different coloured rays will have _different foci_, and will form their
respective images at different distances from the lens. Thus, suppose
LN (fig. 32.) to represent a double convex-lens, and OB an object at
some distance from it. If the object OB was of a pure red colour, the
rays proceeding from it would form a red image at RR; if the
object was of a violet colour, an image of that colour would be formed
at VV, _nearer_ the lens; and if the object was white or any
other combination of the colour-making rays, those rays would have
their respective foci at different distances from the lens, and form a
succession of images, in the order of the prismatic colours, between
the space RR and VV.
[Illustration: _figure 32._]
Public-domain text, read in full here on John Shaqi.
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