The History of Creation, Vol. 1 (of 2): Or the Development of the Earth and its Inhabitants by the Action of Natural CausesHaeckel, Ernst
Philosophy
The History of Creation, Vol. 1 (of 2): Or the Development of the Earth and its Inhabitants by the Action of Natural Causes
Haeckel, Ernst
Evolution; Heredity; Human beings -- Origin
These phenomena and the mathematico-astronomical knowledge of the
structure of the universe justify the theory that, inconceivable ages
ago, long before the first existence of organisms, the whole earth was a
fiery fluid globe. Now, this theory corresponds with the grand theory of
the origin of the universe, and especially of our planetary system,
which, on the ground of mathematical and astronomical facts, was put
forward in 1755 by our critical philosopher Kant,(22) and was later more
thoroughly established by the celebrated mathematicians, Laplace and
Herschel. This cosmogeny, or theory of the development of the universe,
is now almost universally acknowledged; it has not been replaced by a
better one, and mathematicians, astronomers, and geologists have
continually, by various arguments, strengthened its position.
Kant’s cosmogeny maintains that _the whole universe, inconceivable ages
ago, consisted of a gaseous chaos_. All the substances which are found
at present separated on the earth, and other bodies of the universe, in
different conditions of density—in the solid, semi-fluid, liquid, and
elastic fluid or gaseous states of aggregation—originally constituted
together one single homogeneous mass, equally filling up the space of
the universe, which, in consequence of an extremely high degree of
temperature, was in an exceedingly thin gaseous or nebulous state. The
millions of bodies in the universe which at present form the different
solar systems did not then exist. They originated only in consequence of
a universal rotatory movement, or rotation, during which a number of
masses acquired greater density than the remaining gaseous mass, and
then acted upon the latter as central points of attraction. Thus arose a
separation of the chaotic primary nebula, or gaseous universe, into a
number of rotating nebulous spheres, which became more and more
condensed. Our solar system was such a gigantic gaseous or nebulous
ball, all the particles of which revolved round a common central point,
the solar nucleus. The nebulous ball itself, like all the rest, in
consequence of its rotatory movement, assumed a spheroidal or a
flattened globular form.
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