Half Hours With Modern Scientists: Lectures and EssaysTyndall, John
Philosophy
Half Hours With Modern Scientists: Lectures and Essays
Tyndall, John
Science
It gives me pleasure to think that the facts and reasonings of this
discourse tend rather towards the justification of Mr. Darwin than
towards his condemnation, that they tend rather to augment than to
diminish the cubic space demanded by this soaring speculator; for
they seem to show the perfect competence of matter and force, as
regards divisibility and distribution, to bear the heaviest strain
that he has hitherto imposed upon them.
In the case of Mr. Darwin, observation, imagination, and reason
combined have run back with wonderful sagacity and success over a
certain length of the line of biological succession. Guided by
analogy, in his “Origin of Species” he placed as the root of life a
primordial germ, from which he conceived the amazing richness and
variety of the life that now is upon the earth’s surface, might be
deduced. If this were true it would not be final. The human
imagination would infallibly look behind the germ, and inquire into
the history of its genesis.
Certainty is here hopeless, but the materials for an opinion may be
attainable. In this dim twilight of speculation the inquirer
welcomes every gleam, and seeks to augment his light by indirect
incidences. He studies the methods of nature in the ages and the
worlds within his reach, in order to shape the course of imagination
in the antecedent ages and worlds. And though the certainty
possessed by experimental inquiry is here shut out, the imagination
is not left entirely without guidance. From the examination of the
solar system, Kant and Laplace came to the conclusion that its
various bodies once formed parts of the same undislocated mass; that
matter in a nebulous form preceded matter in a dense form; that as
the ages rolled away heat was wasted, condensation followed, planets
were detached, and that finally the chief portion of the fiery cloud
reached, by self-compression, the magnitude and density of our sun.
The earth itself offers evidence of a fiery origin; and in our day
the hypothesis of Kant and Laplace receives the independent
countenance of spectrum analysis, which proves the same substances
to be common to the earth and sun. Accepting some such view of the
construction of our system as probable, a desire immediately arises
to connect the present life of our planet with the past. We wish to
know something of our remotest ancestry.
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