Essays: Scientific, Political, & Speculative; Vol. 2 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.Spencer, Herbert
Philosophy
Essays: Scientific, Political, & Speculative; Vol. 2 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.
Spencer, Herbert
Philosophy; Political science; Science
supposing that they revolved in circles whose centres revolved round
the earth; or by both. The discovery that this would account for the
appearances, was the discovery that in certain geometrical diagrams the
relations were such, that the uniform motion of points along curves
conditioned in specified ways, would, when looked at from a particular
position, present analogous irregularities; and the calculations of
Hipparchus involved the belief that the relations subsisting among
these geometrical curves were _equal_ to the relations subsisting among
the celestial orbits.
Leaving here these details of astronomical progress, and the
philosophy of it, let us observe how the relatively concrete science
of geometrical astronomy, having been thus far helped forward by
the development of geometry in general, reacted upon geometry,
caused it also to advance, and was again assisted by it. Hipparchus,
before making his solar and lunar tables, had to discover rules
for calculating the relations between the sides and angles of
triangles—_trigonometry_, a subdivision of pure mathematics. Further,
the reduction of the doctrine of the sphere to a quantitative form
needed for astronomical purposes, required the formation of a
_spherical trigonometry_, which {56} was also achieved by Hipparchus.
Thus both plane and spherical trigonometry, which are parts of the
highly abstract and simple science of extension, remained undeveloped
until the less abstract and more complex science of the celestial
motions had need of them. The fact admitted by M. Comte, that since
Descartes the progress of the abstract division of mathematics has
been determined by that of the concrete division, is paralleled by
the still more significant fact that even thus early the progress of
mathematics was determined by that of astronomy. And here, indeed, we
see exemplified the truth, which the subsequent history of science
frequently illustrates, that before any more abstract division makes a
further advance, some more concrete division suggests the necessity for
that advance—presents the new order of questions to be solved. Before
astronomy put before Hipparchus the problem of solar tables, there
was nothing to raise the question of the relations between lines and
angles: the subject-matter of trigonometry had not been conceived.
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