Memorabilia Mathematica; or, the Philomath's Quotation-Book
Science
Memorabilia Mathematica; or, the Philomath's Quotation-Book
Mathematics; Mathematics -- Quotations, maxims, etc.
=1575.= The scientific part of Arithmetic and Geometry would be
of more use for regulating the thoughts and opinions of men than
all the great advantage which Society receives from the general
application of them: and this use cannot be spread through the
Society by the practice; for the Practitioners, however dextrous,
have no more knowledge of the Science than the very instruments
with which they work. They have taken up the Rules as they found
them delivered down to them by scientific men, without the least
inquiry after the Principles from which they are derived: and the
more accurate the Rules, the less occasion there is for inquiring
after the Principles, and consequently, the more difficult it is
to make them turn their attention to the First Principles; and,
therefore, a Nation ought to have both Scientific and Practical
Mathematicians.--WILLIAMSON, JAMES.
_Elements of Euclid with Dissertations
(Oxford, 1781)._
=1576.= _Where there is nothing to measure there is nothing to
calculate_, hence it is impossible to employ mathematics in
psychological investigations. Thus runs the syllogism compounded
of an adherence to usage and an apparent truth. As to the latter,
it is wholly untrue that we may calculate only where we have
measured. Exactly the opposite is true. Every hypothetically
assumed law of quantitative combination, even such as is
recognized as invalid, is subject to calculation; and in case of
deeply hidden but important matters it is imperative to try on
hypotheses and to subject the consequences which flow from them
to precise computation until it is found which one of the
various hypotheses coincides with experience. Thus the ancient
astronomers _tried_ eccentric circles, and Kepler _tried_ the
ellipse to account for the motion of the planets, the latter also
compared the squares of the times of revolution with the cubes of
the mean distances before he discovered their agreement. In like
manner Newton _tried_ whether a gravitation, varying inversely as
the square of the distance, sufficed to keep the moon in its
orbit about the earth; if this supposition had failed him, he
would have tried some other power of the distance, as the fourth
or fifth, and deduced the corresponding consequences to compare
them with the observations. Just this is the greatest benefit of
mathematics, that it enables us to survey the possibilities whose
range includes the actual, long before we have adequate definite
experience; this makes it possible to employ very incomplete
indications of experience to avoid at least the crudest
errors. Long before the transit of Venus was employed in the
determination of the sun’s parallax, it was attempted to
determine the instant at which the sun illumines exactly one-half
of the moon’s disk, in order to compute the sun’s distance from
the known distance of the moon from the earth. This was not
possible, for, owing to psychological reasons, our method of
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