History of the inductive sciences, from the earliest to the present timeWhewell, William
History
History of the inductive sciences, from the earliest to the present time
Whewell, William
Science -- History
The peculiar characteristics of scientific ideas, which I have
endeavored to express by speaking of them as _distinct_ and
_appropriate to the facts_, must be more fully and formally set
forth, when we come to the philosophy of the subject. In the mean
time, the reader will probably have no difficulty in conceiving
that, for each class of Facts, there is some special set of Ideas,
by means of which the facts can be included in general scientific
truths; and that these Ideas, which may thus be termed
_appropriate_, must be possessed with entire distinctness and
clearness, in order that they may be successfully applied. It was
the want of Ideas having this reference to material phenomena, which
rendered the ancient philosophers, with very few exceptions,
helpless and unsuccessful speculators on physical subjects.
This must be illustrated by one or two examples. One of the facts
which Aristotle endeavors to explain is this; that when the sun's
light passes through a hole, whatever be the form of the hole, the
bright image, if formed at any considerable distance from the hole,
is round, instead of imitating the figure of the hole, as shadows
resemble their objects in form. We shall easily perceive this
appearance to be a necessary consequence of the circular figure of
the sun, if we conceive light to be diffused from the luminary by
means of straight rays proceeding from every point of the sun's disk
and passing through every point within the boundary of the hole. By
attending to the consequences of this mode of conception, it will be
seen that each point of the hole will be the vertex of a double cone
of rays which has the sun's disk for its base on one side and an
image of the sun on the other; and the figure of the image of the
hole will be determined by supposing a series of equal bright
circles, images of the sun, to be placed along the boundary of an
image equal to the hole itself. The figure of the image thus
determined will partake of the form of the hole, and {88} of the
circular form of the sun's image: but these circular images become
larger and larger as they are further from the hole, while the
central image of the hole remains always of the original size; and
thus at a considerable distance from the hole, the trace of the
hole's form is nearly obliterated, and the image is nearly a perfect
circle. Instead of this distinct conception of a cone of rays which
has the sun's disk for its basis, Aristotle has the following loose
conjecture.[57\1] "Is it because light is emitted in a conical form;
and of a cone, the base is a circle; so that on whatever the rays of
the sun fall, they appear more circular?" And thus though he applies
the notion of rays to this problem, he possesses this notion so
_indistinctly_ that his explanation is of no value. He does not
introduce into his explanation the consideration of the sun's
circular figure, and is thus prevented from giving a true account of
this very simple optical phenomenon.
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