A cityless and countryless world : $b An outline of practical cooperative individualismOlerich, Henry
Science
A cityless and countryless world : $b An outline of practical cooperative individualism
Olerich, Henry
Cooperation; Social problems -- Miscellanea
“Geologists have partially examined the Marsian crust to a certain
depth, the same as you have examined the earth’s crust, but more
minutely and more thoroughly. Fossils (animal and vegetable remains
imbedded in the rock formation of the earth’s crust) of various kinds
are found in this rock formation composing the crust. Remains of the
most lowly organized plants and animals are found in the lowest strata,
and as we ascend the fossils become more and more complex. And the
present generation of organic beings living on the surface of Mars, or
on the surface of the earth, are more complex and more highly developed
than any fossil remains that have ever been buried on the respective
planets.
“The preceding consideration shows that the fossils testify to the fact
that there has been a slow, but gradual development during the almost
immeasurable eons of time that were required for the formation of these
sedimentary strata that contain the precious ‘Revolution written by the
finger of Time on the Rock of Ages, and by the ink of Death.’”
“What a long, long time must have been required to produce such changes
as you speak of. Have you any idea, Mr. Midith, how long the Marsian
crust was in forming?” asked Viola.
“It is not finished yet,” said Mr. Midith. “It is still forming the
same as ever. The crust is growing thicker every moment by internal
cooling and by external accretion of meteoric dust, etc., and fossils
of the present time are now being buried the same as they were during
all preceding geologic ages.
“Let us, in a few thoughts, endeavor to travel back from the present to
that primitive time, when nature imbedded the first organic remains in
the then forming strata. The proportion of water area to the land was
much greater then than it is at present. There were no high mountains,
because the solid crust was thin, and the doubling or folding up of a
thin crust can not produce a high fold, or mountain, and, therefore,
the Marsian crust, or surface, was at this primitive beginning not so
much diversified by mountains and depressions as it is at present.
It was more nearly spherical, and hence all, or nearly all, covered
with water; and what applies to Mars’ crust undoubtedly applies, under
similar conditions, equally to the surface of all other planets.
“Igneous rocks, as you know, are produced by the gradual cooling of
the heated matter of a planet, moon, or sun. They are formed next to
the internal fire, and can, therefore, contain no fossils. Before
fossils could be imbedded, igneous rocks had to be slowly disintegrated
by the action of heat and cold, wind and wave, rain and drought, and
other atmospheric phenomena. Clay, soil, sand, etc., is nothing but a
pulverized igneous rock.
Public-domain text, read in full here on John Shaqi.
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