The Thirteenth, Greatest of CenturiesWalsh, James J. (James Joseph)
History
The Thirteenth, Greatest of Centuries
Walsh, James J. (James Joseph)
Civilization, Medieval -- 13th century; Universities and colleges -- History
It was not with regard to explosives alone, however, that Roger Bacon
was to make great advances and still more marvelous anticipations in
physical science. He was not, as is sometimes claimed for him, either
the inventor of the telescope or of the theory of lenses. He did more,
however, than perhaps anyone else to make the principles of lenses
clear and to establish them on a mathematical basis. His traditional
connection with the telescope can probably be traced to the fact that
he was very much interested in astronomy and the relations of the
heavens to the earth. He pointed out very clearly the errors which had
crept into the Julian calendar, calculated exactly how much of a
correction was needed in order to restore the year to its proper
place, and suggested the method by which future errors of this kind
could be avoided. His ideas were too far beyond his century to be
applied in a practical way, but they were not to be without their
effect and it is said that they formed the basis of the subsequent
correction of the calendar in the time of Pope Gregory XIII three
centuries later.
{44}
It is rather surprising to find how much besides the theory of lenses
Friar Bacon had succeeded in finding out in the department of optics.
He taught, for instance, the principle of the aberration of light,
and, still more marvelous to consider, taught that light did not
travel instantaneously but had a definite rate of motion, though this
was extremely rapid. It is rather difficult to understand how he
reached this conclusion since light travels so fast that as far as
regards any observation that can be made upon earth, the diffusion is
practically instantaneous. It was not for over three centuries later
that Römer, the German astronomer, demonstrated the motion of light
and its rate, by his observations upon the moons of Jupiter at
different phases of the earth's orbit, which showed that the light of
these moons took a definite and quite appreciable time to reach the
earth after their eclipse by the planet was over.
Public-domain text, read in full here on John Shaqi.
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