Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
We know that sound is sent out in all directions through the medium of
the air, a substance invisible and impalpable, by means of a motion
that is communicated successively from one part of the air to the next;
and as this movement has the same speed in all directions, it must form
spherical surfaces that keep enlarging until at last they strike the
ear. Now there can be no doubt that light likewise reaches us from a
luminous substance through some motion caused in the matter lying in
the intervening space,--for we have seen above that this cannot take
place through transmission of matter from one place to another.
If, moreover, light requires time for its passage--a matter we shall
discuss in a moment--it will then follow that this movement is caused
in the substance gradually, and therefore is transmitted, like sound,
by surfaces and spherical waves. I call these _waves_ because of
their likeness to those formed when one throws a pebble into water,
which are examples of gradual propagation in circles, although from a
different cause and on a plane surface.
In regard to the question of light requiring time for its transmission,
let us consider whether there is any experimental evidence against it.
What experiments we can make here on the earth with sources of light
placed at great distances (although indicating that it does not take a
sensible time for light to pass over these distances) are subject to
the objection that these distances are yet too small, and that we can
only argue that the movement of light is enormously fast. M. Descartes
thought it to be instantaneous and based his opinion upon much better
reasons taken from the eclipse of the moon. Yet as I shall make clear,
even this evidence is not decisive. I shall state the matter in a
somewhat different way from his in order more easily to exhibit all the
consequences.
Suppose S to be the position of the sun, E A part of the orbit of the
earth, S E M a straight line intersecting in M, the orbit of the moon,
represented by the circle A M.
Now if light requires time--say an hour--to move the distance between
the earth and the moon, then [at the time of an eclipse] it follows
that when the earth has come to E its shadow, or the stoppage of the
light of the sun, will not yet have reached M [the moon], and will
not for an hour. Counting from the instant the earth reaches E, it
will be an hour before it will reach M if it is to be obscured there.
This eclipse will not be seen from the earth for yet another hour.
Suppose that during these two hours the earth has moved to X, the moon
appearing eclipsed at M, the sun still being seen at S. For I assume as
does Copernicus that the sun is fixed and since light moves in straight
lines, is always seen in its true position.
Public-domain text, read in full here on John Shaqi.
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