The principles of science : $b a treatise on logic and scientific methodJevons, William Stanley
Philosophy
The principles of science : $b a treatise on logic and scientific method
Jevons, William Stanley
Logic; Science -- Methodology
We must ascribe to Newton the honour of leading the way in methods of
minute measurement. He did not call waves of light by their right name,
and did not understand their nature; yet he measured their length,
though it did not exceed the 2,000,000th part of a metre or the one
fifty-thousandth part of an inch. He pressed together two lenses of
large but known radii. It was easy to calculate the interval between
the lenses at any point, by measuring the distance from the central
point of contact. Now, with homogeneous rays the successive rings of
light and darkness mark the points at which the interval between the
lenses is equal to one half, or any multiple of half a vibration of
the light, so that the length of the vibration became known. In a
similar manner many phenomena of interference of rays of light admit
of the measurement of the wave lengths. Fringes of interference arise
from rays of light which cross each other at a small angle, and an
excessively minute difference in the lengths of the waves makes a very
perceptible difference in the position of the point at which two rays
will interfere and produce darkness.
Fizeau has recently employed Newton’s rings to measure small amounts of
motion. By merely counting the number of rings of sodium monochromatic
light passing a certain point where two glass plates are in close
proximity, he is able to ascertain with the greatest accuracy and ease
the change of distance between these glasses, produced, for instance,
by the expansion of a metallic bar, connected with one of the glass
plates.[192]
[192] *Proceedings of the Royal Society*, 30th November, 1866.
Nothing excites more admiration than the mode in which scientific
observers can occasionally measure quantities, which seem beyond
the bounds of human observation. We know the *average* depth of the
Pacific Ocean to be 14,190 feet, not by actual sounding, which would
be impracticable in sufficient detail, but by noticing the rate of
transmission of earthquake waves from the South American to the
opposite coasts, the rate of movement being connected by theory with
the depth of the water.[193] In the same way the average depth of
the Atlantic Ocean is inferred to be no less than 22,157 feet, from
the velocity of the ordinary tidal waves. A tidal wave again gives
beautiful evidence of an effect of the law of gravity, which we could
never in any other way detect. Newton estimated that the moon’s force
in moving the ocean is only one part in 2,871,400 of the whole force of
gravity, so that even the pendulum, used with the utmost skill, would
fail to render it apparent. Yet, the immense extent of the ocean allows
the accumulation of the effect into a very palpable amount; and from
the comparative heights of the lunar and solar tides, Newton roughly
estimated the comparative forces of the moon’s and sun’s gravity at the
earth.[194]
[193] Herschel, *Physical Geography*, § 40.
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