CHAPTER III.

NATURE OF THE STRATIFIED ROCKS.

The present constituents of the earth which are accessible for direct

study are divisible into three parts. The inner portion, consisting of

_rocks_, is known as the _lithosphere_; outside this, with portions of

the lithosphere projecting through into the outermost part, is the

_hydrosphere_, comprising the ocean, lakes, rivers, and all masses of

water which rest upon the lithosphere in a liquid condition. The

outermost envelope, which is continuous and unbroken is the

_atmosphere_, in a gaseous condition. It is well known that some of

the constituents of any one of these parts may be abstracted from it,

and become a component of either of the others; thus the atmosphere

abstracts aqueous vapour from the hydrosphere, and the lithosphere

takes up water from the hydrosphere, and carbonic anhydride from the

atmosphere.

The nebular hypothesis of Kant and Laplace necessitates the former

existence of the present solid portions of the lithosphere in a molten

condition, and accordingly the first formed solid covering of the

lithosphere, if this hypothesis be true, must have been formed from

molten material, or in the language of Geology, it was an _igneous

rock_. Consequently, the earliest _sedimentary rock_ was necessarily

derived directly from an igneous rock, with possible addition of

material from the early hydrosphere and atmosphere, and all

subsequently formed sedimentary rocks have therefore been derived from

igneous rocks (with the additions above stated) either directly, or

indirectly through the breaking up of other sedimentary rocks which

were themselves derived directly or indirectly from igneous rocks. The

observations of geologists show that this supposition that the

materials of sediments have been directly or indirectly obtained for

the most part from once-molten rocks is in accordance with the

observed facts, and so far their observations testify to the truth of

the nebular hypothesis. This being the case, the study of the

petrology of the igneous rocks is necessary, in order to arrive at a

true understanding of the composition of the sedimentary ones. The

igneous rocks are largely composed of four groups of minerals,

viz.--quartz, felspars, ferro-magnesian minerals, and ores. Of these

the quartz (composed of silica) yields particles of silica for the

formation of sedimentary rocks; the felspars, which are double

silicates of alumina and an alkali or alkaline earth, being prone to

decomposition furnish silicate of alumina and compounds of soda,

potash, lime, &c. The ferro-magnesian minerals (such as augite,

hornblende and mica) may undergo a certain amount of decomposition,

and yield compounds of iron, lime, &c. We may also have fragments of

any of these minerals, and of the ore group in an unaltered condition.

The composition of a sedimentary rock which has undergone no

alteration after its formation will therefore depend upon the

character of the rock from which it was derived, the chemical changes

which take place in the materials which compose it, before they enter

into its mass, and the mechanical sorting which they undergo prior to

their deposition.

In the above passage the terms igneous rock and sedimentary rock have

been used, and it is necessary to give some account of the sense in

which they were used.

An _igneous_ rock is one which has been _consolidated_ from a state of

_fusion_. It is not necessary to discuss here the exact significance

of the word fusion, and whether certain rocks which are included in

the igneous division were formed rather from solution at high

temperature than from actual fusion. This point is of importance to

the petrologist, but to the student of stratigraphical geology the

term igneous rock may be used in its most comprehensive sense. These

igneous rocks were consolidated either upon the surface of the

lithosphere or in its interior.

The other great group of rocks is one to which it is difficult to

apply a satisfactory name. They have been termed by different writers,

_sedimentary_, _stratified_, _derivative_, _aqueous_, and _clastic_,

but no one of these terms is strictly accurate. The term _sedimentary_

implies that they have settled down, at the bottom of a sheet of water

for instance. It can hardly be maintained that limestones formed by

organic agency, like the limestones of coral reefs, are sedimentary in

the strict sense of the term, and an accumulation like surface-soil

can only be called a sediment by straining the term. _Stratified_

rocks are those which are formed in strata or layers, but many of the

rocks which we are considering do not show layers on a small scale,

and igneous rocks (such as lava-flows) are also found in layers,

though such layers are not true strata in the sense in which the term

is used by geologists; the term _stratified_ is perhaps the least open

to objection of any of those named above. _Derivative_ implies that

the fragments have been derived from some pre-existing rock, but as

there are many ways in which fragments of one rock may be derived from

another, the term is too comprehensive. _Aqueous_ rocks should be

formed in water, and most of the class of rocks which we are

considering have been so formed, but others such as sand-dunes and

surface-soil have not. (The term Aerial or Æolian has been suggested

to include these rocks which are thus separated from the Aqueous rocks

proper; the objection to this is that the origin of these rocks is

closely connected with that of the true Aqueous rocks, and moreover

the group is too small to be raised to the dignity of a separate

subdivision.) Lastly, the name _clastic_ has been given, because the

rocks so called are formed by the _breaking up_ of pre-existing rocks.

There are two objections to this name. In the first place, some rocks

included under the head clastic are formed by solution of material and

its consolidation from a state of solution by chemical or organic

agency, though we may perhaps speak of rocks being broken up by

chemical as well as by mechanical action. The most important objection

is that many clastic rocks are formed by the breaking up of rocks

subsequently to their formation, and it has been proposed that rocks

of this nature should be termed _cataclastic_, while those which are

formed by the breaking up of pre-existing rocks upon the earth's

surface should be termed _epiclastic_; another group formed of

materials broken up within the earth, and accumulated upon its surface

as the result of ejection of fragmental material from volcanic vents

being termed _pyroclastic_. This classification is scientific, and

under special circumstances is extremely useful, but the older terms

have been used so generally, and with this explanation their use is so

unobjectionable, that they may be retained, and the term _stratified_

will be generally used to indicate all rocks which are not of igneous

origin or formed as mineral veins in the earth's interior.

The division of rocks into _three_ great groups, the Igneous,

Stratified and Metamorphic (the latter name being applied to those

rocks which have undergone considerable alteration since their

formation), is objectionable, since we have metamorphic igneous rocks

as well as metamorphic stratified ones. The most convenient

classification is as follows:--

A. Igneous 1. { Unaltered.

2. { Metamorphic.

B. Stratified 1. { Unaltered.

2. { Metamorphic.

It must be distinctly understood that all geological phenomena must be

taken into account by the stratigraphical geologist. The upheaval of

strata, the production of jointing and cleavage in them, their

intrusion by igneous material, their metamorphism, give indications of

former physical conditions equally with the lithological characters of

the strata, and their fossil contents. Nevertheless it is not proposed

to give a full account of the various phenomena displayed by rocks;

the student is referred to Text-books of General Geology for this

information. It will be as well here, however, to point out in a few

words the exact significance of the existence of strata in the

lithosphere.

The formation of strata and their subsequent destruction to supply

material for fresh strata are due to three great classes of changes.

Beginning with a portion of lithosphere composed of rock, it is found

that rock is broken up by agents of denudation, as wind, rain, frost,

rivers and sea. These agents perform their function mainly upon the

portion of the lithosphere which projects through the hydrosphere to

form _land_, and the land is the main area of denudation. The

materials furnished by denudation are carried away, and owing to

gravitation, naturally proceed from a higher to a lower level, often

resting on the way, but if nothing else occurs, ultimately finding

their way to the _sea_, where they are deposited as strata. The sea is

the principal area for the reception of this material, and it is there

accordingly that the bulk of stratified rock is formed. If nothing

else occurred, in time the whole of the land would be destroyed, and

the wreckage of the land deposited beneath the sea as stratified rock.

As it is there is a third class of change, underground change, causing

movements of the earth's crust (to use a term which can hardly be

defined in few words but which is generally understood), and as the

result of the relative uplift of portions of the earth's crust, the

stratified rocks formed beneath the oceans are raised above its level,

giving rise to new masses of land, which are once more ready for

destruction by the agents of denudation. This cycle of change (all

parts of which are ever proceeding simultaneously) is one of the

utmost importance to the stratigraphical geologist.

_Stratification_ is the rock-structure of prime importance in

stratigraphical geology, and a few words must here be devoted to its

consideration, leaving further details to be dealt with hereafter. The

surface of the ocean-floor is, when viewed on a large scale, so level,

that it may be considered practically horizontal, and accordingly in

most places the materials which are laid down on the ocean-floor give

rise to accumulations which at all times have a general horizontal

surface (when the ocean-slopes depart markedly from horizontality the

deposits tend to abut against these slopes rather than to lie with

their upper surfaces parallel to their original angle). A practically

horizontal surface of this character may give rise to a _plane of

stratification_ (or _bedding-plane_) in more than one way. A pause may

occur during which there is a cessation of the supply of material, so

that the material which has already been accumulated has sufficient

time to become partially consolidated before the deposition of fresh

material upon it. In this way a want of coherence between the two

masses is produced, along the plane of junction, which after

consolidation of the deposits causes an actual divisional plane along

which the two deposits may be separated. This is a plane of

stratification. The pause may be produced in various ways, sometimes

between successive high tides, at others as the result of physical

changes which may have taken ages to happen. Again, after material of

one kind has been deposited, say sand, some other substance such as

clay may be accumulated on its upper surface, giving rise to a plane

of stratification between two deposits of different lithological

characters. If this occurs alone, there may be actual coherence

between the two strata, so that it is erroneous to speak of a plane of

stratification as if it were always one along which one deposit could

be readily split from the other, though as a general though by no

means universal rule, change from one kind of deposit to another is

also marked by want of coherence between the two. The material between

two planes of stratification forms a _stratum_ or _bed_, though if the

deposit be very thin it is known as a _lamina_, and the planes are

spoken of as _planes of lamination_ (no hard and fast line can be

drawn between strata and laminæ; several of the latter usually occur

in the space of an inch).

A _stratum_ will have its upper and lower surface apparently parallel,

though not really so, for no stratum extends universally round the

earth, and many of them disappear at no great distance when traced in

any direction. Parts of one stratum may be composed of different

materials from other parts when traced laterally, thus one stratum may

be found composed essentially of sand in one place, of mud in another,

and of a mixture of the two in an intervening locality. Whatever be

the composition of a stratum it dies out eventually, owing to the

coming together of the upper and lower bounding planes of

stratification. The stratum is thickest at some spot, from that spot

it becomes thinner in all directions, until it disappears at last by

the coalescence of the bounding-planes. This is spoken of as

_thinning-out_. Strata, then, consist of lenticular masses of rock,

separated from the underlying and overlying strata by planes of

stratification. The shape of the lenticle may vary immensely, the

thickness bearing no definite relationship to the horizontal extent.

Some strata, many feet in thickness, may thin out and disappear

completely in the course of a few yards, whilst others an inch or two

in thickness may be traced horizontally for many miles. We often find

thin strata of coal and limestone, extending for great distances,

strata of mud thinning out more rapidly, and sandstones still more

rapidly, but no universal rule connecting rapidity of thinning-out

with composition of the strata can be laid down.

Having seen what a stratum is, it now remains to speak of the

composition of the stratified rocks. They have been classified

according to their composition, and according to their origin.

According to composition they have been divided into:

_Arenaceous_ rocks, composed essentially of grains of sand.

_Argillaceous_ rocks, composed essentially of particles of

mud.

_Calcareous_ rocks, composed essentially of particles of

carbonate of lime.

_Carbonaceous_ rocks, composed largely of hydrocarbon

compounds.

_Siliceous rocks_, composed essentially of silica not in the

form of grains;

whilst according to their origin they have been separated into:--

_Mechanically-formed_ rocks, composed of fragments derived

from other rocks by mechanical fracture.

_Chemically-formed_ rocks, composed of particles which have

been chemically deposited from a state of solution.

_Organically-formed_ rocks, composed of materials which have

been derived from a state of solution or from the gaseous

condition by the agency of organisms.

Whichever classification be adopted (and each is useful for special

purposes), it must be noted that no hard and fast line can be drawn

between one division and another. A rock may be partly arenaceous and

partly calcareous, composed of a mixture of sand and lime, and the

same rock may similarly be partly mechanically and partly organically

formed, the sand being due to mechanical fracture, and the lime to the

agency of organisms, and so with the other divisions.

As many of the changes which have occurred in past times have been

concerned in destruction and obliteration, whilst deposition is the

cause of preservation, the study of deposits is peculiarly adapted for

testing the truth of the grand principle of geology that the changes

which have taken place in past times are generally speaking similar in

kind and in intensity of action to those which are in progress at the

present day, and a study of the modern deposits is specially important

as throwing light upon the characters of those which have been formed

in past times. It will be abundantly shown in the sequel that the

deposits of the strata are in general comparable in all essential

respects with those which are being formed at present, and accordingly

they give most valuable indications as to the nature of the physical

and other conditions under which they were laid down. The desert sand,

the precipitate of the inland sea, the reef-limestone and many another

deposit can thus be detected by an examination of their lithological

characters, combined with consideration of other kinds of evidence.

The petrology of the sedimentary rocks is still in its infancy, though

much has already been done, but it offers a wide field of inquiry to

the field-geologist and worker with the microscope[8].

[Footnote 8: The student will do well to consult _The Challenger

Report_ by Messrs Murray and Renard (1891), for information concerning

many modern sediments, and Harker's _Petrology for Students_ Section

D, for general information on the Petrology of the Stratified Rocks.]

The Principles of Stratigraphical Geology · 第 3 / 30 章