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)
If you look at a landscape over a heated plain or bonfire or through
uneven glass you will see that the image is distorted and confused
because the rays of light are refracted and entangled as they pass
through this unequal medium. Yet each ray is going just as straight as
it can toward your eye.
Now to such familiar cases where a ray of light is bent out of its
straight course by the uneven density of the air or glass through
which it passes Einstein has added another and unsuspected effect,
namely, that light is likewise deflected in passing through a strong
gravitational field such as the vicinity of a large body like the sun.
It has long been known that the displacement of the earth in space and
time (that is to say, its motion) causes an apparent displacement of
the stars in space.
The astronomer does not point his telescope straight at a star. If he
did, he would not see it, for, owing to the forward motion of the
earth, the telescope moves out of range of the rays that otherwise
would have reached it.
[Illustration: Everyone knows that a ray of light is bent out of its
straight course as it passes from the air into a denser medium like
water or glass, and that this deflection apparently shifts the position
of the object from which the light comes. Einstein’s theory and the
British eclipse observations prove, what was not known before, that a
ray of light as it passes through the gravitational field of a large
body like the sun, is also perceptibly bent out of its straight course
and likewise makes an apparent shift in the position of its source,
the star.--From Black & Davis’ “Practical Physics.” Published by The
Macmillan Company.]
If you have ever tried to shoot a bird on the wing, or, better, a
prairie-dog from a train you will get the idea. Or, if you have not had
this experience, you have doubtless watched the raindrops running down
a car window and have noticed that when the rain is falling straight
down the drops strike the pane on a slant when the car is moving
forward. The faster the car moves the greater the deviation from the
perpendicular. If the train runs backward the rain-streaks slant in
the opposite direction. If then you should be asked to point out the
direction of the cloud from which the rain is coming you would--unless
you knew and made allowance for the movement of the train--point in
a line with the streaks on the pane, sometimes backward, sometimes
forward, but not straight upward where the raincloud really is.
Public-domain text, read in full here on John Shaqi.
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