Opticks : $b or, A treatise of the reflections, refractions, inflections and colours of lightNewton, Isaac
Science
Opticks : $b or, A treatise of the reflections, refractions, inflections and colours of light
Newton, Isaac
Optics -- Early works to 1800
Having given my Observations of these Colours, before I make use of them
to unfold the Causes of the Colours of natural Bodies, it is convenient
that by the simplest of them, such as are the 2d, 3d, 4th, 9th, 12th,
18th, 20th, and 24th, I first explain the more compounded. And first to
shew how the Colours in the fourth and eighteenth Observations are
produced, let there be taken in any Right Line from the Point Y, [in
_Fig._ 6.] the Lengths YA, YB, YC, YD, YE, YF, YG, YH, in proportion to
one another, as the Cube-Roots of the Squares of the Numbers, 1/2, 9/16,
3/5, 2/3, 3/4, 5/6, 8/9, 1, whereby the Lengths of a Musical Chord to
sound all the Notes in an eighth are represented; that is, in the
Proportion of the Numbers 6300, 6814, 7114, 7631, 8255, 8855, 9243,
10000. And at the Points A, B, C, D, E, F, G, H, let Perpendiculars
A[Greek: a], B[Greek: b], &c. be erected, by whose Intervals the Extent
of the several Colours set underneath against them, is to be
represented. Then divide the Line _A[Greek: a]_ in such Proportion as
the Numbers 1, 2, 3, 5, 6, 7, 9, 10, 11, &c. set at the Points of
Division denote. And through those Divisions from Y draw Lines 1I, 2K,
3L, 5M, 6N, 7O, &c.
Now, if A2 be supposed to represent the Thickness of any thin
transparent Body, at which the outmost Violet is most copiously
reflected in the first Ring, or Series of Colours, then by the 13th
Observation, HK will represent its Thickness, at which the utmost Red is
most copiously reflected in the same Series. Also by the 5th and 16th
Observations, A6 and HN will denote the Thicknesses at which those
extreme Colours are most copiously reflected in the second Series, and
A10 and HQ the Thicknesses at which they are most copiously reflected in
the third Series, and so on. And the Thickness at which any of the
intermediate Colours are reflected most copiously, will, according to
the 14th Observation, be defined by the distance of the Line AH from the
intermediate parts of the Lines 2K, 6N, 10Q, &c. against which the Names
of those Colours are written below.
[Illustration: FIG. 6.]
Public-domain text, read in full here on John Shaqi.
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