Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativity — John Shaqi
Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativitySlosson, Edwin E. (Edwin Emery)
Science
Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativity
Slosson, Edwin E. (Edwin Emery)
Einstein, Albert, 1879-1955; Relativity (Physics)
The electro-magnetic theory of light, thought out by Clerk Maxwell
forty-five years ago, has proved to be an excellent guide to
research and led to many practical applications, such as wireless
telegraphy. According to this theory the miles-long Marconi waves,
the infinitesimal waves that we feel as heat or see as light and the
still more minute waves of the X-rays are movements of the same sort,
though differing in length, and all travel at the same speed in space
of 186,000 miles a second. It was one of the implications of Maxwell’s
theory, though it was not perceived until later, that light and all
such waves must exercise a certain pressure upon a body against which
they strike, just as a jet of water from a fireman’s hose pushes
against the side of a house. The pressure of light is so exceedingly
slight that it had never been noticed, but it has been actually
detected and measured by Professors E. F. Nichols of Yale and G. F.
Hull of Dartmouth. The sunshine falls upon the earth with a force of
160 tons. Both theory and experiment have shown that a beam of light
has inertia or mass, that is to say, a beam of light pushes like a
water jet, and it has now been proved, by the eclipse expedition, that
the pull of gravity deflects a beam of light as it does a water jet.
That is to say, a beam of light has weight, is attracted by gravity.
This deflection of a beam of light by gravity is extremely small, but
photographs taken during the recent total eclipse of the sun show that
star beams that passed near the sun are bent out of a straight path.
[Illustration: The eclipse expedition found that the stars seen about
the sun appear slightly shifted from the positions they occupy on a
map of the same region of the sky when the sun is not in their midst.
This shows that a ray from a star is refracted or bent as it passes
close to the sun and confirms Einstein’s theory that light is affected
by gravitation. The observed angle of deflection agrees closely with
that predicted by Einstein but is twice as great as that required by
Newton’s theory of gravitation. In this diagram of course the angle
of the deflected ray and the size of the sun and earth relative to
distance are greatly exaggerated.]
A better illustration of the eclipse observation than I could word is
given by Sir Oliver Lodge in his interesting article on “The New Theory
of Gravitation” in The _Nineteenth Century_ of December, 1915,
from which I therefore quote:
Take a fine silk thread of indefinite length, and stretch it straight
over the surface of a smooth table or floor. Imagine a star at one end
of the thread, and an eye at the other; and let the thread typify one
of the rays of light emitted in all directions by the star, viz. the
ray emitted in the direction of the observing eye.
Public-domain text, read in full here on John Shaqi.
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