The Cambridge natural history, Vol. 01 (of 10)Hickson, Sydney J. (Sydney John)
Science
The Cambridge natural history, Vol. 01 (of 10)
Hickson, Sydney J. (Sydney John)
Animals
FLINTS.—The ultimate source of all the silica in the sea and fresh-water
areas is to be found in the decomposition of igneous rocks such as granite.
The quantity of silica present in solution in sea water is exceedingly
small, amounting to about one-and-a-half parts in 100,000; it certainly is
not much more in average fresh water. This is no doubt due to its
extraction by diatoms, which begin to extract it almost as soon as it is
set free from the parent rock. It is from this small quantity that the
siliceous sponges derive the supply from which they form their spicules.
Hence it would appear that for the formation of one {242}ounce of spicules
at least one ton of sea water must pass through the body of the sponge.
Obviously from such a weak solution the deposition of silica will not occur
by ordinary physical agencies; it requires the unexplained action of living
organisms. This may account for the fact that deposits of flint and chert
are always associated with organic remains, such as Sponges and Radiolaria.
By some process, the details of which are not yet understood, the silica of
the skeleton passes into solution. In Calcareous deposits, a replacement of
the carbonate of lime by the silica takes place, so that in the case of
chalk the shells of Foraminifera, such as _Globigerina_ and _Textularia_
and those of Coccoliths, are converted into a siliceous chalk. Thus a
siliceous chalk is the first stage in the formation of a flint.
A further deposition of silica then follows, cementing this pulverulent
material into a hard white porous flint. It is white for the same reason
that snow is white. The deposition of silica continues, and the flint
becomes at first grey and at last apparently black (black as ice is black
on a pond). Frequently flints are found in all stages of formation:
siliceous chalk with the corroded remains of sponge spicules may be found
in the interior, black flint blotched with grey forming the mass of the
nodule, while the exterior is completed by a thin layer of white porous
flint. This layer must not be confused with the white layer which is
frequently met with on the surface of weathered flints, which is due to a
subsequent solution of some of the silica, so that by a process of
unbuilding, the flint is brought back to the incompleted flint in its
second stage. In the chalk adjacent to the flints, hollow casts of large
sponge spicules may sometimes be observed, proving the fact, which is
however unexplained, of the solution of the spicular silica. The formation
of the flints appears to have taken place, to some extent at least, long
after the death of the sponge, and even subsequent to the elevation of the
chalk far above the sea-level, as is shown by the occurrence of layers of
flints in the joints of the solid chalk.[282]
COELENTERATA AND CTENOPHORA
BY
S. J. HICKSON, M.A., F.R.S.
Formerly Fellow and now Honorary Fellow of Downing College, Beyer Professor
of Zoology in the Victoria University of Manchester.
Public-domain text, read in full here on John Shaqi.
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