The nature of the physical worldEddington, Arthur Stanley, Sir
Philosophy
The nature of the physical world
Eddington, Arthur Stanley, Sir
Physics -- Philosophy; Science -- Philosophy
[23]
On the other hand a quantum (see chapter IX) has a
definite periodicity associated with it, so that it must be able to
measure itself against a time-extension. Anyone who contemplates the
mathematical equations of the new quantum theory will see abundant
evidence of the battle with the intervening symbol .
[24]
Hegel, Werke (1842 Ed.), Bd. 7, Abt. 1, p. 97.
[25]
Because I can attach no meaning to an orbit other than an
orbit in space and time, i.e. as located by measures. But I could not
assume that the alternative orbit would be meaningless (inconsistent
with possible measures) until I tried it.
[26]
See p. 236.
[27]
As a recent illustration of this attitude I may refer to
Bertrand Russell’s Analysis of Matter, p. 78—a book with which
I do not often seriously disagree. “Whereas Eddington seems to regard
it as necessary to adopt Einstein’s variable space, Whitehead regards
it as necessary to reject it. For my part, I do not see why we should
agree with either view; the matter seems to be one of convenience in
the interpretation of formulae.” Russell’s view is commended in a
review by C. D. Broad. See also footnote, p. 142.
[Pg 163]
Chapter VIII
MAN’S PLACE IN THE UNIVERSE
The Sidereal Universe. The largest telescopes reveal about a
thousand million stars. Each increase in telescopic power adds to the
number and we can scarcely set a limit to the multitude that must
exist. Nevertheless there are signs of exhaustion, and it is clear that
the distribution which surrounds us does not extend uniformly through
infinite space. At first an increase in light-grasp by one magnitude
brings into view three times as many stars; but the factor diminishes
so that at the limit of faintness reached by the giant telescopes a
gain of one magnitude multiplies the number of stars seen by only 1.8,
and the ratio at that stage is rapidly decreasing. It is as though we
are approaching a limit at which increase of power will not bring into
view very many additional stars.
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