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)
Now those of us who are not astronomers are not much concerned over
a discrepancy of a few hundredths of a second in the measurement of
an angle by the telescope. We do not care much where Mercury will be
five centuries hence, for we do not know quite where it is now. If
astronomers made the laws of Nature instead of merely discovering
them we might be afraid that at their next congress they might repeal
Newton’s law of gravitation and send us all flying off into space. But
fortunately they have no such power and even though they should all
become adherents of Einstein’s most revolutionary theories, Newton’s
laws of mechanics and Euclid’s laws of geometry would remain as true
as they ever were, not perhaps absolutely and universally true, as we
have assumed, but sufficiently accurate for all practical purposes.
Deviations from them can only become detectable when we come to
consider movements as swift as light waves or electrons.
How a heavy object can alter space relations may be seen from this
simple illustration: Stretch a sheet of rubber over a hoop like a
drumhead. It is now level and flat and if parallel lines are drawn
across it in two directions so as to divide it up into squares like a
checkerboard all these lines are straight and equidistant and all the
squares are of equal size.
A row of worms, starting in an even rank and crawling along the
parallel lines across the drumhead, would keep even all the way. Now
lay a bullet on the center of the drumhead. The rubber sags down and
stretches, most in the middle, least at the edges. The “parallel”
lines are no longer equidistant. The squares are no longer equal. The
lines are no longer of the same length. If now we repeat our worm race
we shall find that those worms following lines close to the weight
have to go down hill and up again and so travel a greater distance to
traverse the same number of squares than those following lines nearer
the edge which lie comparatively flat and are nearly as short as
before. Consequently the worms will be slowed up in proportion to their
nearness to the center and the row of their heads will be swung around
at an angle to their former frontage.
Public-domain text, read in full here on John Shaqi.
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