antecedent subaërial and the subsequent wave gradation, account for
most of the islands which affect indented coasts. Some of them are
high and some low for reasons which will be readily understood. The
long narrow belts of land constituting irregularities parallel to the
general trend of the coast (Figs. 319 and 320) are usually the result
of deposition in shallow water. They are usually sand or coral reefs,
built up above water-level by waves. The deposits at the debouchures
of streams give rise to projecting deltas. Most small irregularities
of angular form, especially if high (Pl. XX), indicate wave-erosion,
and their details of form are determined by the structure of the rock
along shore, while most irregularities of curved outline involve
something of shore-deposition, if not due wholly to it. Glaciation, or
glaciation and subsidence, may also give rise to peninsulas, capes, and
islands of curved outlines (Pl. XXIV, coast of Maine). Curving outlines
may, however, be developed by erosion alone in weak rock structures.
This is illustrated by the weak rock structures (clay, sand, etc.) of
most of the Atlantic coastal plain. Thus inspection of the horizontal
configuration of coasts will often indicate the processes which
have been dominant there in recent times. On the other hand, the
interpretations of many coastal irregularities, such as Hudson Bay,
Puget Sound, the Gulf of California, the Baltic Sea, etc., are not to
be read from the map. In such cases, diastrophism and gradation have
usually coöperated, but the relative importance of the two processes
can only be determined by detailed study in the field. When it is
remembered that the tendency of shore-erosion is to reduce great
irregularities of horizontal configuration, though not to obliterate
small ones if the coast be heterogeneous in composition (p. 353), and
that the tendency of shore-deposition is also to regularity, it is
clear that the great irregularities of coast-lines are due neither to
shore-erosion nor to shore-deposition, though minor ones may be due to
either.
THE WORK OF OCEAN-CURRENTS.
As agents of erosion, ocean-currents are not, in general, of great
importance. Currents which reach the bottom are comparable, in
their effects, to rivers of the same velocity and volume; but most
ocean-currents do not touch bottom, and, therefore, do not erode it.
Where the current agitates the bottom sensibly, as it often does in
shallow water, the bottom is abraded, and in the lee of such places
it is doubtless aggraded. Since ocean-currents do not, for the most
part, flow in shallow water, their erosive work is, on the whole,
relatively slight; but where they are forced through narrow and shallow
passageways, their abrasive work may be considerable. Thus the Gulf
Stream, where it issues from the Gulf, has a velocity of four or five
miles per hour, and its shallow and narrow channel is current-swept.
A rough test of the abrasive work of an ocean-current is found in the
nature of the bottom beneath it. If this be hard, it indicates that the
loose sediment on the floor of the ocean has been swept away, while the
presence of fine detritus indicates that the current is not wearing.
Thus the abrasive power of the Gulf Stream is known to continue
somewhat beyond its narrow channel, for on the Blake plateau (between
the Bahamas and Cape Hatteras), where the water is 600 fathoms and less
in depth, “the bottom of the Gulf Stream ... is swept clean of lime and
ooze and is nearly barren of animal life.”[168] Other illustrations
of the erosive power of currents have been noted near Gibraltar in
water 500 fathoms deep, and between the Canary Islands at depths of
1000 fathoms.[169] In spite of these examples, and of many others
which probably exist in similar situations, it yet remains true that
ocean-currents are on the whole but feeble agents of erosion.
As agents of transportation, ocean-currents are scarcely more important
than as agents of corrasion, for they transport only what they erode,
if the life which inhabits them be left out of consideration. This
phase of their work has probably been exaggerated through a confusion
of transporting energy and actual transportation. Ocean-currents which
do not touch bottom roll no sediment and carry only what may be held
in suspension. A river’s power of transporting sediment in suspension
is due largely to the cross-currents occasioned by the unevenness of
its resistant bottom (p. 117). If a particle of mud in suspension in
a river drops to the bottom, as it frequently does, it may be picked
up again and carried forward. If, on the other hand, a particle in
suspension in an ocean-current once escapes the moving water by
settling through it, the current which does not drag bottom has no
chance to pick it up again. Very fine sediment may be carried by an
ocean-current far beyond the point where it was acquired, but currents
which do not touch bottom are rarely strong enough to hold any but the
finest material for any considerable length of time. As transporters
of sediment, therefore, ocean-currents are at a great disadvantage as
compared with rivers.
How readily particles of extreme fineness may be kept in suspension,
and how little agitation is necessary to keep them from sinking, is
shown by the experiments of Sorby, who showed that while a sand grain
¹⁄₁₀₀ of an inch in diameter will settle one foot per second in still
water, fine particles of clay require days to sink through the same
distance. The Challenger found fine sediment derived from the land 400
miles from the coast of Africa, and that not opposite the debouchure of
any large river. Sediment settles more readily in salt water than in
fresh, despite the fact that the former is heavier. This is presumably
because the salt diminishes the cohesion of the water.
Deposition by ocean-currents is limited by their transportation. Only
where they erode their bottoms do they gather coarse materials, and
only in the lee of such places are their deposits coarse. Since the
material which they carry is generally fine, it is widely distributed
before deposition.
Ocean-currents have little influence on the configuration of
coast-lines.
DEPOSITS ON THE OCEAN-BED.
Something has already been said concerning the sediments which
accumulate in the shallow waters along shores; but the area of marine
sedimentation is as extensive as the ocean itself, and the deposits
must now be reviewed from another point of view.
Oceanic deposits may be conveniently divided into two chief groups,
dependent on the depth of the water in which they are made.[170] These
groups are (1) _shallow-water deposits_, made in water less than some
such depth as 100 fathoms, and (2) _deep-sea deposits_, laid down in
water of greater depth. The selection of the 100-fathom line as the
dividing depth is less arbitrary than it seems, for passing outward
from the shore, it is at about this depth that the bottom ceases to be
commonly disturbed by the action of currents and waves; that sunlight
and vegetable life cease to be important at the bottom; and that the
coarser sediments which predominate along shore give place, as a rule,
to muds and oozes. Furthermore, the 100-fathom line (or some line very
near it) is an important one in the physical relief of the globe, for
it appears to mark, approximately, the junction of continental plateaus
and ocean-basins. Only because the latter are a little over-full does
the water run over their rims, covering about 10,000,000 square miles
of the borders of the continents, converting them from land into
epicontinental seas.
Aside from the deposits made by organisms, shallow-water deposits are
divisible into two groups—(_a_) those immediately along the shore, the
_littoral deposits_, and (_b_) those made between the littoral zone
and the 100-fathom line. Both are terrigenous. The deep-sea deposits
likewise are divisible into two groups, (_a_) _terrigenous deposits_
formed close to land, and made up chiefly of materials derived
immediately from the disintegration of land formations; and (_b_) the
_pelagic deposits_, made up chiefly of the remains of pelagic organisms
and the ultimate products arising from the decomposition of rocks and
minerals. The former predominate in the less deep waters relatively
near shore; the latter in the deeper water far from land. The shallow-
and deep-water deposits grade into each other in a belt along the
100-fathom line.
_Shallow-water Deposits._
=Littoral deposits.=—The littoral zone is the zone between high- and
low-water marks. It is the zone in which bowlders, gravels, sands, and
all coarser materials accumulate, though muds are occasionally met
with in sheltered estuaries. Generally speaking, the nature of these
deposits is determined by the character of the adjoining lands and the
nature of the local organisms. “The heavier materials brought by rivers
from high terrestrial regions, or thrown up by the tides and waves
of the sea, are here arranged with great diversity of stratification
through the alternate play of the winds and waves. Twice in the
twenty-four hours the littoral zone is covered by water and exposed
to the direct rays of the sun or the cooling effects of the night.
There is a great range of temperature; mechanical agencies produce
their maximum effects,”[171] and physical conditions in general are
most varied. Still greater diversity is introduced by the fact that
the zone is inhabited by both marine and terrestrial organisms, while
the evaporation of the sea-water which flows over tidal marshes and
lagoons leads to the formation of saline deposits. If the length of
the coast-lines of the world be taken at 125,000 miles (about 200,000
kilometers), and the average width of this zone at half a mile, these
deposits are now forming over an area of 62,500 square miles (about
160,000 square kilometers) of the earth’s surface.
=Non-littoral, mechanical deposits in shallow water.=—These deposits
are laid down in the zone of the ocean between low-water mark and the
100-fathom line. They cover about 10,000,000 square miles.[172] Their
composition is much the same as that of the littoral deposits, with
which they are continuous, though on the whole they are finer. At
their lower limit they pass insensibly into the fine deposits of the
deep sea. Coarse material, such as gravel and sand, prevails, though
in special situations, such as depressions and inclosed basins, muddy
deposits are found. While some of the deposits are wholly composed
of inorganic débris, organic remains are freely mingled with others.
The mechanical effects of tides, currents, and waves are everywhere
present, but become less and less well marked as the 100-fathom line
is approached. The forms of vegetable and animal life are numerous,
though the former decrease as depths which exclude the sunlight are
approached.
Both littoral deposits and deposits in shallow water outside the
littoral zone have already been referred to in connection with the work
of waves and currents (pp. 355–66). A few additional points only need
here be added.
[Illustration: +Figs.+ 321 and 322.—Diagrams showing how shallow-water
deposits may attain considerable depth by the shifting of the zone of
deposition seaward.]
[Illustration: +Fig.+ 323.—Diagram showing the interwedging of gravel-,
sand-, and mud-beds.]
In general the coarser sediments are lodged near shore and those
farther from the land become progressively finer. Even the coarser
part of the material carried in suspension by the undertow is partly
left in the shallow water. On the other hand, waves of exceptional
strength may carry coarse material into water of some depth. Thus
coarse shingle (gravel) and even bowlders have been found at depths of
10 fathoms.[173] Coarse deposits may extend far out from land if the
waves are strong, and especially if the water is shallow, and since
the zone of shallow water may be extended seaward by the aggradation
of the bottom, shallow-water deposits may cover extensive areas. They
may become deep at the same time, for as the outer border of the
shallow-water zone is shifted seaward by aggradation, the vertical
space to be filled becomes greater (compare Figs. 321 and 322).
Again, if the coast be sinking, new deposits of coarse material may
be made on older ones. In this way also great thicknesses of sediment
may be accumulated, all parts of which were deposited in shallow water.
The great thickness of some of the conglomerate beds of the past shows
how far this process may go.
[Illustration: +Fig.+ 324.—Ripple-marks.]
[Illustration: +Fig.+ 325.—Rill-marks resembling impressions of
seaweeds. Beach at Noyes Point, R. I. (Walcott, U. S. Geol. Surv.)]
[Illustration: +Fig.+ 326.—Rill-marks. Same locality as 325. (Walcott.)]
As a rule, no definite line marks the seaward terminus of the coarse
detritus, since coarse material is carried farther out when the waves
run high (and the undertow is strong) than when they are feeble. In
calm weather, therefore, fine sediment may be deposited where coarse
had been laid down in the preceding storm, only to be covered in turn
by other deposits of a different character. Thus gravel grades off into
sand, with more or less overlapping or interwedging, and sand grades
off into silt in the same way. This is diagrammatically illustrated by
Fig. 323.
=Characteristics of shallow-water deposits.=—Clastic sediments laid
down in shallow water have several distinctive characteristics. While
they are, in the aggregate, coarse, they are characterized by frequent
variations in coarseness. The surfaces of successive beds are likely
to be ripple- and rill-marked (Figs. 324, 325, 326), and cross-bedding
(Fig. 327) is of common occurrence. Clayey sediments accumulated
between high and low water are often sun-cracked (Fig. 328), and the
tracks of land animals are sometimes preserved on their surfaces.
Shallow-water deposits often contain fossils of organisms which live
in waters of slight depth. These characteristics are sufficient to
differentiate sedimentary formations made in shallow water from those
made in deep water, even after they have been converted into solid
rock and after the rock has emerged from the sea. Many of these
characteristics are, however, shared by deposits made by streams on the
land. Subaërial and lacustrine sediments are usually distinguishable
from those made in the sea by their fossils, and sometimes by their
distribution.
[Illustration: +Fig.+ 327.—Cross-bedding. (Gilbert.)]
[Illustration: +Fig.+ 328.—Sun-cracks. These cracks were on the
mud-flats of the Missouri a few miles above Kansas City, but
the sun-cracks on shore-deposits are not essentially different.
(Calvin.)]
=Topography of shallow-water deposits.=—The shallow-water deposits
have, on the whole, a rather plane surface, though there are some
notable departures from flatness. The steep slopes of the delta fronts
and of wave-built terraces have already been spoken of. Barriers often
shut in depressions, and the disposition of the material deposited is
sometimes uneven, owing to shore and tidal currents. The result is that
the surface of the shallow-water deposits is often affected by low
elevations and by shallow depressions. The elevations and depressions
may be elongate, circular, or irregular in form. These general facts
are shown in Figs. 319, 320, and 329. This topography is sometimes
preserved on newly emerged lands, as at various points on the Coastal
Plain of the United States.
[Illustration: +Fig.+ 329.—Irregularities of topography of
shallow-water deposits. The depths of the water are shown in fathoms.
(Chart of C. and G. Surv.)]
=Chemical and organic deposits.=—There is no sharp line of distinction
between the deposits usually classed as chemical and those regarded as
organic. The latter are chemical in the broader sense of the term, but
as they are immediately associated with life and are dependent upon it,
it is a matter of practical convenience to separate them. Aside from
the organic deposits, the chemical deposits made in shallow sea-water
embrace (1) those due to reactions between constituents so brought
together that new and insoluble compounds are formed and precipitated,
and (2) those due to evaporation. The points of saturation for the
various substances dissolved in sea-water are reached at different
stages, and hence they are deposited more or less in succession.
The chemical deposits made in the shallow water of the sea, or in
shallow bodies of water isolated from the sea, are chiefly simple
precipitates resulting from evaporation; but new combinations are
sometimes made in the process of concentration and precipitation.
All substances in solution are necessarily precipitated on complete
evaporation, but since the sea-water is in general far from saturation,
so far as all its leading salts are concerned, only a few are
thrown down in quantity sufficient to have geological importance
where evaporation is incomplete. The leading deposits are lime
carbonate (CaCO₃), lime sulphate (gypsum, CaSO₄,2H₂O), common salt
(rock-salt, NaCl), and the magnesium salts, usually the chlorides and
sulphates, which are later changed to carbonates. In investigations
on Mediterranean water[174] which had an initial density of 1.02, no
deposit took place until concentration by evaporation had brought the
water to a specific gravity of 1.05. Between this density and that
of 1.13, lime carbonate and some iron oxide were deposited. Between
1.13 and 1.22, lime sulphate was the most abundant precipitate, while
between 1.22 and 1.31, 95% of the deposit was common salt. With still
further concentration, the remaining substances in solution, especially
the magnesium salts, were thrown down.
While there is somewhat more than ten times as much lime sulphate as
lime carbonate in the ocean (p. 324), the deposits of the carbonate
(including the organic) have been very much greater than those of the
sulphate. This is due partly to the fact that the sulphate is much more
soluble in natural waters than the carbonate. Rivers bring much more
carbonate than sulphate to the sea, so that the point of saturation for
the sulphate would normally be reached much later than that of the
carbonate. The more important fact, however, is that marine plants and
animals use lime carbonate freely for skeletal and housing purposes.
It is held by some that they get their lime from the sulphate, but if
so they convert it into carbonate before it takes the form of shells,
coral, etc., the sulphuric acid set free in the process reproducing,
directly or indirectly, more sulphate. The secretion of lime carbonate
by organisms is not dependent on the saturation of the water, but may
be carried on when the amount in solution is very small.
There can be little doubt that the chief deposits of lime carbonate
have been and are being made through the agency of plants and animals
in the form of shells, coral, bones, teeth, and other devices for
supporting, stiffening, housing, protecting, and arming themselves;
but while it is agreed that the larger part of the lime carbonate
deposited in the open sea is of organic origin, it is equally clear
that in closed seas subject to concentration from evaporation, simple
precipitation takes place freely. There is some difference of opinion
as to the importance of these two classes of deposits, past and
present. The debated point is whether simple precipitation takes place
in any appreciable degree under the usual oceanic conditions. There is
much more evidence of solution by sea-water than of precipitation from
it. The ocean appears to be under-saturated with lime carbonate on the
whole, though it is still possible that deposition may take place in
favorable situations, as, for example, where the very calcareous waters
of rivers are spread out in thin sheets on the surface of the heavier
salt water, and thus exposed to exceptional evaporation, or where there
is very exceptional agitation and aëration.[175]
Gypsum appears to be deposited in quantity only in the closed basins of
arid regions where concentration reaches an advanced state.
Since normal sea-water is far from saturation with common salt,
the latter is precipitated only in lagoons, closed seas, or other
situations favorable to great concentration. This is usually achieved
only in notably arid regions, and in basins that receive little or no
drainage from the land.
Deposits of salt usually, therefore, signify highly arid conditions,
and where they occur over wide ranges in latitude and longitude, as
in certain periods of the past, unusual aridity is inferred. Where
confined to limited areas, their climatic significance is less, for
topographic conditions may determine local aridity. The total area
where salt is now being precipitated is small, though on the whole
the present is probably to be regarded as a rather arid period of the
earth’s history. On the other hand, ancient deposits of salt preserved
in the sedimentary strata show that the area of salt deposition has
been much more considerable than now at one time and another in the
earth’s history. The salt and gypsum deposits of the past seem,
therefore, to tell an interesting tale of the climates of the past.
The magnesium salts are among the last to be thrown down as the
sea-water is evaporated, and they most commonly take the form of
sulphates and chlorides. They often form double salts with potassium,
a relatively small and soluble constituent of sea-water. In the
artificial evaporation of salt water to obtain common salt, the process
is usually stopped before the saturation-point for the magnesium salts
is reached, and the residue, the “mother-liquor,” or “bittern,” is
drawn off to prevent these “bitter” salts from mixing with the common
salt. The magnesium salts are among the last to be precipitated, not
only because they are readily soluble, but because their quantity is
small; yet in the original rock from which all the sea-salts came,
there is at least as much magnesium as sodium, while in the sea there
is about five times as much sodium as magnesium. Just what becomes of
the remaining magnesium is not yet well understood. It has a notable
disposition to form double salts with some other constituent, as noted
above. In the earlier marine strata, dolomite, that is, limestone
composed partly or wholly of the double carbonate of lime and magnesia,
(CaMg)CO₃, abounds. This appears to have been formed by a gradual
substitution of molecules of magnesium for those of calcium, but
just how and when and why it was done has not been fully worked out.
It appears to be a case where the saline matter of the sea made its
contribution to the sedimentary deposits by chemical reaction upon
them, rather than by precipitation because of saturation.
The relatively small amount of potash in the sea-water is probably due
to its disposition to remain united with the clays and earths of the
mantle rock and of the shaley deposits.
To some extent the salts in solution act directly on the earthy matter
brought down into the sea by rivers, but where sedimentation is rapid,
as it often is in shallow water, this action is limited and obscure.
In the main, the ocean-waters protect the sediments from weathering
and similar changes, except as organic matter buried with them induces
change.
While the lime deposits are by far the greatest of the chemical and
organic deposits of the sea, plants and animals also secrete notable
quantities of silica. Silica deposits of organic origin are relatively
much more important in the deep sea than in shallow water, and will be
mentioned in that connection.
=Limestone.=—Something concerning the origin of limestone has already
been given in the preceding paragraphs, but because of the importance
of this formation, it may be added by way of summary that shallow seas
free, or nearly free, from terrigenous sediment, and abounding in
lime-secreting life, furnish the conditions for nearly pure deposits
of limestone, and that most of the limestone within the areas of the
present continents appears to have originated under such conditions.
The common notion that limestone is normally a deep-water formation is
a serious error. Although limestones are formed in deep as well as in
shallow waters, by far the more important classes of lime-secreting
organisms are photobathic, i.e. are limited to the depths to which
light penetrates. In the shallow waters, these plants and animals are
in part free and in part attached. Within the areas of deep water they
are free and at the surface, and their remains drop to the bottom,
if not sooner dissolved. But few forms live on the deep, dark, cold
bottoms of abysmal depths. Clear waters, free from abundant terrigenous
sediments and abounding in lime-secreting life, rather than deep
waters, are, therefore, the most favorable conditions for the origin of
limestone.
The purely chemical deposits of limestone are probably all of
shallow-water origin. Once made, they are subject to solution,
redeposition, and other mutations like other deposits. As a result,
they often lose many of their original characteristics, but enough
usually remain to tell the story of their origin.
_Deep-sea Deposits._
=Contrasted with shallow-water deposits.=—The deep-sea deposits cover
the ocean-bottom below the 100-fathom line. Their area is considerably
more than half the earth’s surface. The characteristic deposits are
muds, organic oozes, and clays, which in their physical characteristics
are remarkably uniform. In regions of floating ice, greater diversity
is introduced from the varied nature of the materials which the ice
transports, but gravels and sands, comparable to those of shallow
water, are rarely found. “Tides, currents, and waves produce some
mechanical effects at the upper limits of the deep-sea region, but
on the whole there is an absence of the phenomena of erosion, and
mechanical action would appear to be absent except in the case of
submarine eruptions. The depth is too great for sunlight to penetrate,
and vegetable life is limited to the upper zone. Animal life is present
in the same zone and on the bottom, but absent or nearly so in the
middle depths. The temperature (at the bottom) is below 40° Fahr.
throughout the larger part of the area, and if subject to variation
with latitude or change of season, these changes affect only the depths
immediately beyond the 100-fathom line. Throughout the whole region
there is a very uniform set of conditions. In the shallow-water and
littoral zones, owing to the rapid accumulation and the mechanical
effects of transportation and erosion, the effects of chemical
modification are not very apparent in the deposits; but in deep-sea
deposits, in consequence of the less rapid rate of accumulation,
absence of transport, the nature and small size of the particles, many
evident chemical reactions have taken place, resulting in the formation
_in situ_ of glauconite, phosphatic and manganese nodules, zeolites,
and other secondary products.”[1] With increasing depth and distance
from the shore, the character of the deposits undergoes a change. There
is less and less material derived directly from the land, and more
“amorphous matter arising from the ultimate decomposition of minerals
and rocks, and accompanied, in all moderate depths, by an increase
[relative] of the remains of pelagic organisms. We thus pass insensibly
from those deep-sea deposits of a terrestrial origin, which we call
‘terrigenous,’ to those deep-sea deposits denominated ‘pelagic,’ in
which the remains of calcareous and siliceous organisms, clays and
other substances of secondary origin play the principal rôle.”[176]
The following table[177] shows the relations of the various groups of
marine deposits.
1. Deep-sea deposits beyond { Red clay } I. Pelagic deposits
100 fathoms { Radiolarian ooze } formed in deep
{ Diatom ooze } water removed
{ Globigerina ooze } from land.
{ Pteropod ooze }
{
{ Blue mud }
{ Red mud }
{ Green mud }
{ Volcanic mud } II. Terrigenous
{ Coral mud } deposits formed
} in deep and
2. Shallow-water deposits } Sands, gravels, } shallow water,
between low-water mark } muds, etc. } mostly close
and 100 fathoms } } to land.
}
3. Littoral deposits between } Sands, gravels, }
high- and low-water marks } muds, etc. }
=Sources.=—The pelagic deposits are made up in part of materials of
organic origin, and in part of materials of inorganic origin. The
inorganic materials may be of mechanical or chemical origin. Mechanical
pelagic deposits originate in various ways. They may come (1) from
the land by the ordinary processes of gradation, (2) from volcanic
vents, or (3) from extra-terrestrial sources. Chemical deposits may
be formed (1) _in situ_ by the chemical interaction of substances in
the sea-water on materials of organic and inorganic origin, and (2) by
direct precipitation from the sea-water.
=Mechanical inorganic deposits.=—The terrigenous materials which reach
the deep sea are, as a rule, only the finest products of land decay,
and are carried out by movements of water or by the winds. They are
not commonly recognized in the dredgings more than 200 miles from
the shore, but opposite the mouths of great rivers they extend much
farther,—1000 miles in the case of the Amazon. They are especially
abundant on the slopes of the continental shelves. Here occur the
_blue_, _green_, and _red muds_, with which are associated volcanic
and coral muds. The color of these various muds is dependent in part
on the changes which they have undergone since their deposition.
The green muds usually contain enough glauconite to give them their
color, and are most commonly found off bold coasts where sedimentation
is not rapid. The blue muds indicate lack of oxidation, or perhaps
deoxidation. Red muds are not common, though they have been found in
some situations. In general, these deposits are analogous to certain
shales, marls, etc., found within the continents.
Though coarse materials derived from the land are occasionally found in
the deep-sea deposits, their presence must be looked upon as in some
sense accidental. Occasional pebbles, or even bowlders, are carried out
into the ocean entangled in the roots of floating trees. Within limits,
too, icebergs have carried out land débris, though it is probable that
transportation by this means has been exaggerated. The amount which
icebergs might carry, if fully loaded, is far greater than the amount
which they do carry.
Of the identifiable inorganic materials in the deep sea, the most
abundant are of volcanic origin, and among these the most common is
pumice, which is frequently so light that it floats readily until it
becomes water-logged. Pieces of pumice brought up by the Challenger and
thoroughly dried were found to float for months in sea-water before
settling even through the depth of water contained in the vessel
in which the experiment was performed.[178] The next most abundant
substance of volcanic origin in pelagic deposits is _volcanic glass_.
This ranges from pieces of the size of a walnut down to the smallest
fragments, which often serve as centers for concretions. _Lapilli_
(cinders) and _volcanic ash_ also are abundant in parts of the deep
sea. The distribution of these volcanic products is essentially
universal, though by no means uniform. Some of them are probably from
submarine volcanoes.
The study of the deep sea deposits has revealed the presence of many
nodules and grains which are believed to be of extra-terrestrial
origin. Many of them are magnetic.[179] The dust of countless meteors
which enter the atmosphere daily settles on land and sea alike, and
enters into the sediment of the bottom of the latter. It is probably
no more abundant in deep water than in shallow, but it is relatively
more important, since other sedimentation is more meager. The number of
meteorites which enter the atmosphere daily has been estimated at from
15,000,000 to 20,000,000.[180] If on the average the meteorites weigh
ten grains each, probably a rather high estimate, the total amount of
extra-terrestrial matter reaching the earth yearly would be 5,000 to
7,000 tons, and something like three-fourths of this must, on the
average, fall into the sea. But even at this rate it would take some
fifty billion years to cover the sea-bottom with a layer one foot in
thickness.
=Organic constituents of pelagic deposits.=—With increasing distance
from shores, and especially with increasing depth of water, terrigenous
deposits become less and less abundant, and sediments derived from
pelagic life increase in relative importance. Beyond the upper part of
the outer slopes of the continental shelves, the pelagic deposits are
largely made up of shells and skeletons of marine organisms which live
in the surface-waters. Pelagic molluscs, foraminifera, and algæ secrete
shells of lime carbonate, while diatoms and radiolarians secrete shells
of silica. When the organisms die, they sink to the bottom with their
shells, and these mineral matters of organic origin are mingled with
the volcanic products which are universal over the sea-floor. Pelagic
deposits of organic origin are named according to their characteristic
constituents. Thus there are pteropod oozes, globigerina oozes, diatom
oozes, radiolarian oozes, etc.[181] It is not to be understood that
these oozes are made up exclusively of the shells which give them their
names. Diatom ooze is an ooze in which diatom shells are abundant, not
an ooze made up wholly of diatom shells; and globigerina ooze is an
ooze in which globigerina shells are abundant, though in many cases
they do not make up even the bulk of the matter. While samples of these
various oozes might be selected which are thoroughly distinct from one
another, there are all gradations between them, since pelagic life does
not recognize boundary-lines.
It is a significant fact that with increasing depth the proportion
of lime carbonate in the ooze decreases. Thus in tropical regions
remote from land where the depths are less than 600 fathoms, the
carbonate of lime of the shells of pelagic organisms may constitute
80% or 90% of the deposit. With the same surface conditions, but with
increasing depth, the percentage of lime carbonate decreases, until at
2000 fathoms it is less than 60%; at 2400 fathoms, 30%, and at 2600
fathoms, 10%. Beyond this depth there are usually no more than traces
of carbonate of lime. The data at hand show that the percentage of lime
carbonate falls off below 2200 fathoms more rapidly than at lesser
depths.
When the percentage of lime carbonate becomes very low, the calcareous
oozes grade off into the red clay with which the sea-floor below 2400
to 2600 fathoms is covered.
=Chemical deposits.=—The chemical deposits of the deep sea are chiefly
the alteration products of sediments which reach the sea-bottom
by mechanical means. All sediment deposited in the sea undergoes
more or less chemical change, but it is only when the change is
very considerable that the product is referred to this class. Where
sedimentation is rapid and the sediment coarse, the chemical change is
relatively slight; but where the sedimentation is slow and the sediment
fine, the chemical change is relatively great; for the longer exposure
to the sea-water and the greater proportion of surface exposed to
attack, both favor change. Both the area and the mass of sea-bottom
sediment radically changed in this way are large, but most of the
deposit does not correspond to any formation known on the land.
The red clay already referred to belongs to this class of deposits.
Its origin has been the subject of much discussion. It contains much
volcanic débris, various concretions, bones of mammals, zeolitic
crystals, and extra-terrestrial spherules, and doubtless the insoluble
products of the shells of pelagic life; but it is still a mooted
question how far the clay itself is the product of decomposed shells,
and how far the altered product of pulverized pumice, volcanic ash,
dust, etc. Pelagic life does not seem to be less abundant at the
surface where the water is deep than where it is shallow, and it would
appear that the shells must sink in such situations as elsewhere. If
the lime carbonate of globigerina ooze be removed by dilute acid, the
inorganic residue is similar to the red clay in the ocean-bottom. This
suggests that owing to the more complete solution in the very deep
water, the lime carbonate of the shells has been dissolved, leaving
the red clay as a residuum. The more complete solution at the bottom
might be the result either of the greater pressure, or of a greater
percentage of CO₂ in the water due to emanations from the sea-floor, or
to both; but the suddenness of the transition from oozes to red clay,
with increasing depth, does not seem to be fully explained by these
assumptions. The study of the dredgings has inclined the students of
these materials to the conclusion that volcanic materials, rather than
shells, are the principal source of the red clay.[182] The volcanic
materials are thought to have accumulated slowly and to have been long
exposed to the action of sea-water. The various nodules and crystals in
the clay are believed to be secondary products, the materials for which
were derived from the decomposition of the same materials. Eolian dust
may be a notable constituent of the red clay.
Various specific products of chemical change may be briefly referred
to. The decomposition of certain mineral particles, such as feldspar,
gives rise to _kaolin_, and kaolin is a very considerable constituent
of most of the clayey deposits of the ocean-bottom. The kaolinization
of feldspar may take place both on land and in the sea. _Manganiferous_
deposits are widespread in the ocean-bottom, occurring both as coatings
on grains of mechanical sediments, shells, etc., and as concretions
ranging in sizes from minute particles to nodules an inch or more in
diameter. The concretions are sometimes approximately spheroidal, but
often botryoidal. These manganiferous nodules are believed to have
arisen from the decay of fragments of volcanic rocks. In their decay,
the manganese and iron are believed to have been first changed to
carbonates, and subsequently to oxides. After manganese oxide, iron
oxide and silica are by far the most abundant constituents, but many
other substances enter into their composition in minor quantities.
Another substance somewhat widely distributed in the sea-bed, though
by no means universal, is _glauconite_, a complex silicate of alumina,
iron, potassium, etc. Glauconite is, on the whole, most abundant
along the edges of the continental shelves, though it is by no means
universal in this position. It is not commonly found in deep water,
nor very near the shore, but approximately at the “mud-line.” The
glauconite grains begin to form, as a rule, in tiny shells, chiefly
the shells of foraminifera. After filling the shell, the shell itself
may disappear, while the glauconite goes on accumulating around the
core already formed, until the grain attains considerable size.
Glauconite is believed to be an alteration product of certain sorts
of mechanical sediment, the change being effected under the influence
of the decaying organic matter in the shells.[183] It does not occur
where sedimentation is rapid, and its formation appears to be favored
by considerable changes of temperature. Glauconite deposits occur on
the land and are commonly known as _green sand marl_. Glauconite also
occurs sparingly in many other sedimentary rocks.
[Illustration: +Fig.+ 330.—Distribution of various sorts of deep-sea
deposits. (Murray. Challenger Reports.)]
Another substance which is somewhat widespread in the ocean-bottom is
_phosphate of lime_, which occurs in various sorts of oozes, in the
manganiferous nodules, in glauconite, and in independent nodules. Like
the grains of glauconite, the grains of phosphate of lime appear to
have started as concretions in shells, and to be the result of the
reaction of organic matter on the contents of sea-water. The immediate
source of the lime phosphate in the water appears to have been the
shells or bones of the numerous animals living in the sea.
Secondary minerals made from the constituents of volcanic matter which
has been decomposed occur not uncommonly in the bottom of the sea.
These minerals belong to the general class of _zeolites_, phillipsite
being the most abundant. Their distribution is somewhat wide, but their
quantity is slight.
Unfortunately, knowledge of the deep-sea deposits is limited to their
superficial layers. Soundings do not usually penetrate more than a few
inches, or at most a foot or two.
Unlike shallow-water deposits, those of the really deep sea seem to
find no correlatives in the known rock formations of the land.
LAKES.
Most of the phenomena of the ocean are repeated on a smaller scale in
lakes. The waves of lakes and their attendant undertows and littoral
currents are governed by the same laws and do the same sort of work
as the corresponding movements of the ocean. Tides are absent, or
insignificant, but slight changes of level, known as _seiches_,[184]
have been observed in many lakes. They are probably caused by sudden
changes in atmospheric pressure. While they are generally very slight,
they frequently amount to as much as a foot, and occasionally to
several feet. The seiches are oscillatory movements, and their period
is influenced by the length and depth of the lake. They have been
studied most carefully in Switzerland. Currents corresponding to those
of the ocean are slight or wanting in lakes, but since most lakes have
inlets and outlets, their waters are in constant movement toward the
latter. In most cases this movement is too slow to be readily noted, or
to do effective work either in corrasion or transportation. The work of
the ice, on the other hand, is relatively more important in lakes than
in the sea.
=Changes taking place in lakes.=—The processes in operation in lakes
are easily observed and readily understood. (1) The waves wear the
shores, and the material thus derived is transported, assorted, and
deposited as in the sea, and all the topographic forms resulting from
erosion or deposition along the seacoast are reproduced on their
appropriate scale in lakes. (2) Streams bear their burden of gravel,
sand, and mud into lakes and leave it there. (3) The winds blow dust
and sand into the lakes, and in some places pile the sand up into dunes
along the shores. (4) Animals of various sorts live in the lakes, and
their shells and bones give rise to deposits comparable to the animal
deposits in the sea. (5) Abundant plants grow in the shallow water
about the borders of many ponds and lakes, and as they die, their
substance accumulates on the bottom. (6) At the outlet the water is
constantly lowering its channel. The lowering of the outlet is often
slow, especially if the rock be coherent, for the outflowing water
is usually clear, and therefore inefficient in corrasive work. These
six processes are essentially universal, and all conspire against the
perpetuity of the lakes. (7) In lakes where the temperature is low
enough for ice to be formed, it crowds on the shores and develops
phenomena peculiar to itself. The ice of the sea may work in similar
ways, but its work is restricted to high latitudes. (8) In lakes in
arid regions, deposits are often made by precipitation from solution.
The first five and the last of these processes are filling the basins
of the lakes. As the sediment is deposited, a corresponding volume
of water is displaced, and, if there be outlets, forced out of the
basins; the sixth process is equally antagonistic to the lakes, while
the seventh has little influence on their permanence. Given time
enough, these processes must bring the history of any lake to an end.
The lowering of the outlet will alone accomplish this result if the
bottom of the basin is above base-level. Many lakes have already become
extinct, either through the filling or draining of their basins, or
through both combined. The antagonism of rivers and lakes long ago
led to the epigram “Rivers are the mortal enemies of lakes.” True as
this statement is, it does not follow that lakes will ever cease to
exist, for the causes which produce new lakes may be in operation
contemporaneously with those which bring lakes now in existence to an
end.
=Lacustrine deposits.=—The beds of sediment deposited in lakes are
similar in kind, in structure, and in disposition to beds of sediment
laid down in the sea, but river-borne sediment is more commonly
concentrated into deltas, since waves and shore-currents are less
effective. Even the limestone of the sea has its correlative in some
lakes. Some of it was made of the shells of fresh-water animals which
throve where the inwash of terrigenous sediment was slight, some of
it from the calcareous secretions of plants,[185] and some of it was
precipitated from solution.[186] Salt and iron-ore[187] deposits are
also sometimes made in lakes.
=Extinct lakes.=—The former existence of lakes where none now exist
may be known in various ways. If the lake basin was filled, its former
area is a flat, the beds of which bear evidence, in their composition,
their structure, and often in their fossil contents, of their origin
in standing water. Such a flat is commonly so situated topographically
that the basin would be reproduced if the lacustrine deposits were
removed. To this general rule there might be exceptions, as where a
glacier formed one side of the basin when it was filled. If the lake
was destroyed by the reduction of its outlet, or by the removal of some
other barrier, such as glacier ice, or by desiccation, shore phenomena,
such as beaches, spits, etc., may be found. In time such evidences are
destroyed by subaërial erosion, so that they are most distinct soon
after the lake becomes extinct.
Many lakes, some of them large[188] and many of them small, are known
to have become extinct, while many others are now in their last stages,
namely, marshes. Many others have been greatly reduced in size. Such
reductions are often obvious where deltas are built into lakes. Thus
the delta built by the Rhone into Lake Geneva is several miles in
length, and has been lengthened nearly two miles since the time of
the Roman occupation. The end of Seneca (N. Y.) lake has been crowded
northward some two miles by deposition at its head. Similar changes
have taken place and are now in progress in many other lakes.
=Lake ice.=[189]—Since fresh water is densest at 39° Fahr., ice does
not commonly form on the surface until the temperature from top to
bottom is reduced to this point. Cooled below this temperature, the
surface-water fails to sink, and with sufficient reduction freezes. If
the lake be small, and especially if it be shallow, it is likely to
freeze over completely in any region where the temperature is notably
below the freezing-point for fresh water for any considerable period
of time. It is under these circumstances that the ice becomes most
effective.
[Illustration: +Fig.+ 331.—Ice crowding upon low shore. Clear Lake, Ia.
(Calvin.)]
Suppose a lake in temperate latitudes, where the range of temperature
is considerable, to be frozen over when the temperature is 20° Fahr.
If now the temperature be suddenly lowered to -10°, and such change of
temperature is not uncommon in the northern part of the United States,
the ice contracts notably. In contracting, it either pulls away from
the shores or cracks. If the former, the water from which the ice is
withdrawn quickly freezes; if the latter, water rises in the cracks
and freezes there. In either case, the ice-cover of the lake is again
complete. If the temperature now rises to 20° the ice expands. The
cover is now too large for the lake, and it must either crowd up on the
shores (Fig. 331) or arch up (wrinkle) elsewhere. It follows the one
course or the other, or both, according to the resistance offered by
the shore.
If the water near the shore is very shallow, the ice freezes to the
sand, gravel, and bowlders at the bottom. If the adjacent land is low,
the ice in expanding may shove up over it, carrying the débris frozen
in its bottom. It may even push up loose gravel and sand in front of
its edge if they be present on the shore. Where bowlders are frozen
to the bottom of the ice, the shoreward thrust in expanding has the
effect of shifting them in the same direction, and even of lifting
them a little above the normal water-level. This constant process of
concentrating bowlders at the shore-line gives rise to the “walled”
lakes, which are not uncommon in the northern part of the United
States. The “wall” does not commonly extend entirely around a lake,
though it exists at various points on the shores of many lakes. In
making the walls, the ice shoved up by winds, especially in the spring
when the ice is breaking up, coöperates.
[Illustration: +Fig.+ 333.—Calcareous tufa domes. Pyramid Lake, Nev.
(Russell.)]
If the lake be bordered by a low marsh, the ice and frozen earth of the
latter are really continuous with the ice of the lake, and the push of
the latter sometimes arches up the former into distinct anticlines,
the frozen part only being involved in the deformation. A succession
of colder and less cold periods may give rise to a succession of such
anticlines.[190] If the shore be steep and of non-resistant material,
the crowding of the ice produces different but not less striking
results. Where the thrust of the ice is against a low cliff of yielding
material, such as clay, it disturbs all above the shore-line. Where the
cliff is sufficiently resistant, it withstands the push of the ice, and
the ice itself is warped and broken.
=Saline lakes.=—A few lakes, especially in arid or semi-arid regions,
are salt, and others are “bitter.” Beside sodium chloride, salt
lakes usually contain magnesium chloride, and magnesium and calcium
sulphates. “Bitter” lakes usually contain much sodium carbonate, as
well as some sodium chloride and sulphate, and sometimes borax. The
degrees of saltness and bitterness vary from freshness on the one
hand to saturation on the other. The water of the Caspian Sea (lake)
contains, on the average, less salt than that of the sea; that of Great
Salt Lake contains about 18%; that of the Dead Sea, about 24%; and that
of Lake Van (eastern Turkestan), the densest body of water known, about
33%. See accompanying table.
Many salt lakes, such as the Dead Sea and Great Salt Lake, are
descended from fresh-water ancestors, while others, like the Caspian
and Aral Seas, are probably isolated portions of the ocean. Lakes of
the former class have usually become salt through a decrease in the
humidity of the region where they occur. The water begins to be salt
when the aridity is such that evaporation from the lake exceeds its
inflow. In this case the inflowing waters bring in small amounts of
saline and alkaline matter, which is concentrated as evaporation takes
place. The concentration may go on until the point of saturation is
reached, or until chemical reactions cause precipitation. In general
the least soluble minerals are precipitated first. Thus gypsum begins
to be deposited from sea-water when 37% of it has been evaporated; but
the saturation-point for salt is not reached until 93% of the water has
been evaporated (see p. 375). The relations in lakes are similar, and
gypsum deposits often underlie those of salt. Deposits of salt and
other mineral matters once in solution are making in some salt lakes
at the present time, and considerable formations of the same sort have
been so made in the past. Buried beneath sediments of other sorts, beds
of common salt or of other precipitates are preserved for ages. Lime
carbonate has been precipitated in quantity from some extinct lakes
(Fig. 333).
The lakes which originate by the isolation of portions of the sea
are salt at the outset. If inflow exceeds evaporation, they become
fresher and may ultimately become fresh; otherwise they remain salt.
If evaporation exceeds inflow they diminish in size and their waters
become more and more salt or bitter.
=Indirect effects of lakes.=—Lakes tend to modify the climate of
the region where they occur, both by increasing its humidity and
by decreasing its range of temperature. They act as reservoirs
for surface-waters, and so tend to restrain floods and to promote
regularity of stream flow. They purify the waters which enter them by
allowing their sediments to settle, and so influence the work and the
life of the waters below.
=Composition of lake-waters.=—The accompanying table[191] shows the
composition of various inclosed lake-waters, and gives some idea of
the wide range, both in kind and quantity, of the mineral matter
held in solution by them. It is to be noted that the table shows the
composition of the waters of exceptional, rather than common, lakes.
The waters of fresh lakes do not depart widely from those of rivers (p.
107).
TABLE—ANALYSES OF THE WATERS OF INCLOSED LAKES.
[+Reduced to Parts per 1000 by Dr. H. J. Van Housen.+]
+----------------+----------------+-----------------+---------------+--------------+
|Locality | Abert Lake, | Bogdo Lake |Caspian Sea. 2°|Caspian Sea, |
| | Oregon | | W. S. W. of | near mouth |
| | | | Pischina, at | of the Volga|
| | | | 15 feet | |
| | | | depth, wind, | |
| | | | W. S. W. | |
|Specific gravity| 1023.17 | | | |
| | | | | |
|Date | May 3, 1883 | | | |
| | | | | |
|Analyst | F. W. Taylor | Gobel | Gobel | H. Rose |
| | | | | |
|Reference |Fourth Ann. Rep.|Lariet Geological|Bischof’s |Bischof’s |
| | U. S. Geol. | Exploration of | Chemical | Chemical |
| | Survey, p. 454| Dead Sea, p. | Geology, Vol.| Geology, |
| | | 284 | I, p. 89 | Vol. I, p. 89|
+----------------+----------------+-----------------+---------------+--------------+
|Sodium, Na | 2.838 | 74.700 | 1.4440 | .3081 |
| | | | | |
|Potassium, K | 10.880 | 1.041 | .0398 | |
| | | | | |
|Rubidium, Rb | | ...... | ...... | ...... |
| | | | | |
|Calcium, Ca | ...... | 3.647 | .1854 | .1238 |
| | | | | |
|Magnesium, Mg | .002 | 13.777 | .4095 | .0728 |
| | | | | |
|Lithium, Li | | | | |
| | | | | |
|Iron, Fe | ...... | ...... | ...... | ...... |
| | | | | |
|Chlorine, Cl | 8.410 | 163.344 | 2.7376 | .4576 |
| | | | | |
|Bromine, Br | ...... | .043 | Trace | ...... |
| | | | | |
|Carbonic acid | | | | |
| gas, CO₂ | 4.653 | ...... | .1382 | .3746 |
| | | | | |
|Sulphuric acid, | | | | |
| H₂SO₄ | .509 | .198 | 1.3372 | .3109 |
| | | | | |
|Phosphoric acid,| | | | |
| HPO₄ | | | | |
| | | | | |
|Nitric acid, | | | | |
| NO₃ | | | | |
| | | | | |
|Boracic acid, | | | | |
| H₃BO₃ | ...... | | | |
| | | | | |
|Silica, SiO₂ | .064 | | | |
| | | | | |
|Alumina, | | | | |
| Al₂O₃ | ...... | | ...... | ...... |
| | | | | |
|Hydrogen in | | | | |
| bicarbonates, H| | | .0023 | .0062 |
| | | | | |
|Ammonium, NH₄ | | ...... | | |
| | | | | |
|Organic matter | ...... | ...... | ...... | ...... |
| +----------------+-----------------+---------------+--------------+
| | 27.357 | 256.750 | 6.2940 | 1.6540 |
+----------------+----------------+-----------------+---------------+--------------+
+-----------------+-----------------+-----------------+-----------------+--------------+--------------+
| Dead Sea, | Dead Sea, near |Dead Sea, at 393 |Dead Sea, at | Elton Lake | Elton Lake |
|Ras Dale, surface| the Island, | ft., between Ras| 656 ft., between| | |
| | surface | Feschkak and | Ras Feschkak | | |
| | | Ras Zerka | and Ras Zerka | | |
| | | | | | |
| 1.0216 | 1.1647 | 1.2225 | 1.2300 | | |
| | | | | | |
| Mar. 20, 1864 | Apr. 7, 1864 | Mar. 15, 1804 | Mar. 15, 1864 | April | August |
| | | | | | |
| Terreil | Terreil | Terreil | Terreil | Gobel | Erdman |
| | | | | | |
|Lartet Geological|Lartet Geological|Lartet Geological|Lartet Geological|Bischof’s |Bischof’s |
| Exploration of | Exploration of | Exploration of | Exploration of | Chemical | Chemical |
| Dead Sea, p. 278| Dead Sea, p. 278| Dead Sea, p. 278| Dead Sea, p. 278| Geology. Vol.| Geology, Vol.|
| | | | | I, p. 403–405| I, p. 403–405|
+-----------------+-----------------+-----------------+-----------------+--------------+--------------+
| .885 | 22.400 | 25.071 | 25.107 | 51.590 | 29.300 |
| | | | | | |
| .474 | 3.547 | 3.990 | 4.503 | 1.162 | |
| | | | | | |
| ...... | ...... | ...... | ...... | | ...... |
| | | | | | |
| 2.150 | 9.094 | 3.704 | 4.218 | ...... | .106 |
| | | | | | |
| 4.197 | 25.529 | 41.306 | 42.006 | 29.971 | 45.598 |
| | | | | | |
| ...... | ...... | ...... | ...... | | |
| | | | | | |
| Trace | Trace | Trace | Trace | ...... | ...... |
| | | | | | |
| 17.628 | 126.521 | 166.340 | 170.425 | 159.498 | 166.890 |
| | | | | | |
| .167 | 4.568 | 4.870 | 4.385 | .059 | ...... |
| | | | | | |
| Trace | Trace | Trace | Trace | ...... | .272 |
| | | | | | |
| .202 | .494 | .451 | .459 | 13.320 | 17.734 |
| | | | | | |
| | | | | | |
| | | | | | |
| | | | | | |
| | | | | | |
| | | | | | |
| ...... | ...... | ...... | ...... | | |
| | | | | | |
| .006 | Trace | Trace | Trace | | |
| | | | | | |
| Trace | Trace | Trace | Trace | | |
| | | | | | |
| ...... | ...... | ...... | ...... | | |
| | | | | | |
| Truce | Trace | Trace | Trace | ...... | ...... |
| | | | | | |
| Trace | Trace | Trace | Trace | Trace | 5.080 |
+-----------------+-----------------+-----------------+-----------------+--------------+--------------+
| 25.709 | 192.153 | 245.732 | 251.103 | 255.600 | 264.980 |
+-----------------+-----------------+-----------------+-----------------+--------------+--------------+
+-----------------+-----------------+-----------------+-----------------+-----------------+--------------+
| Elton Lake | Great Salt Lake | Great Salt Lake | Great Salt Lake | Humboldt[192] Lake| Indevak Lake |
| | | | | | |
| 1.27288 | 1.170 | 2.4 | 1.102 | 1.007 | ...... |
| | | | | | |
| October | 1850 | 1869 | Aug., 1873 | ...... | ....... |
| | | | | | |
| H. Rose | L. D. Gale | O. D. Allen | H. Bassett | O. D. Allen | Gobel |
| | | | | | |
|Bischof’s |Stambury’s |U. S. Geological | Amer. Chemist, |U. S. Geol. Expl.|Lartet Geol. |
| Chemical | Expedition to | Expl. 40th par.| 1874, p. 395 | 40th par. 1877, | Expl. of |
| Geology. Vol. | Great Salt | 1877, Vol. II, | | Vol. I, p. 528 | Dead Sea, |
| I, p. 403–405 | Lake, p. 410 | p. 435 | | | p. 284 |
+-----------------+-----------------+-----------------+-----------------+-----------------+--------------+
| 15.060 | 85.330 | 49.690 | 38.3 | .27842 | 94.050 |
| | | | | | |
| 1.204 | | 2.407 | 9.9 | .06083 | .529 |
| | | | | | |
| | ...... | ...... | ...... | ...... | ...... |
| | | | | | |
| ...... | Trace[196] | .255 | .6 | .01257 | .123 |
| | | | | | |
| 60.540 | .636 | 3.780 | 3.0 | .01648 | 5.076 |
| | | | | | |
| | | Trace | Trace | | |
| | | | | | |
| ...... | ...... | ...... | ...... | ...... | ...... |
| | | | | | |
| 171.936 | 124.454 | 83.946 | 73.6 | .29545 | 158.687 |
| | | | | | |
| | | Trace | | ...... | |
| | | | | | |
| ...... | ...... | ...... | ...... | .20126 | ...... |
| | | | | | |
| 42.560 | 12.400 | 9.858 | 8.8 | .03040 | 3.065 |
| | | | | | |
| | | | | .00069 | |
| | | | | | |
| | | ...... | | ...... | |
| | | | | | |
| | | Trace | | Trace | |
| | | | | | |
| | | ...... | | .03250 | |
| | | | | | |
| | | | | | |
| | | | | | |
| ...... | | | | | |
| | | | | | |
| Trace | ...... | ...... | ...... | ...... | ..... |
+-----------------+-----------------+-----------------+-----------------+-----------------+--------------+
| 291.300 | 222.820 | 149.936 | 134.2 | .92800 | 261.530 |
+-----------------+-----------------+-----------------+-----------------+-----------------+--------------+
+-----------------+-----------------+------------------+-----------------+-----------------+
| Soda Lake, near | Soda Lake, near | Mono Lake, Cal., | Urmiah Lake |Owen’s Lake, Cal.|
| Ragtown, Nev., | Ragtown, Nev., | at 1 foot below | | |
| at 1 foot below |at 100 feet below| surface | | |
| surface | surface | | | |
| | | | | |
| 1.101 | 1.101 | 1.048 | 1.155 | 1.051 |
| | | | | |
| ...... | ...... | July 16, 1883 | ...... | ...... |
| | | | | |
| T. M. Chatard | T. M. Chatard | T. M. Chatard | Hitchcock | O. Loew |
| | | | | |
| Ante, p. 70 | Ante, p. 70 | Bulletin No. 9. |Lartet Geological| Appendix JJ Ann.|
| | |U.S. Geol. Survey,| Exploration of | Rep. Chief |
| | | p. 26 |Dead Sea, p. 284 | Engineers, 1876 |
| | | | | p. 190 |
+-----------------+-----------------+------------------+-----------------+-----------------+
| 41.632 | 40.206 | 18.100 | 74.890 | 21.650 |
| | | | | |
| 2.290 | 2.425 | 1.111 | | 2.751 |
| | | | | |
| | | ...... | ...... | ...... |
| | | | | |
| ...... | ...... | .278 | .529 | Trace |
| | | | | |
| .245 | .245 | .125 | 2.914 | Trace |
| | | | | |
| | ...... | | | Trace |
| | | | | |
| ...... | ...... | ...... | ...... | ...... |
| | | | | |
| 41.496 | 40.206 | 11.610 | 119.496 | 13.440 |
| | | | | |
| ...... | ...... | ...... | | ...... |
| | | | | |
| 15.650[7] | 18.058[7] | 14.465[7] | ...... | 13.140 |
| | | | | |
| 11.771 | 11.943 | 6.520 | 7.671 | 9.362 |
| | | | | |
| | ...... | | | Trace |
| | | | | |
| ...... | ...... | ...... | | Trace |
| | | | | |
| .285 | .287 | .153 | | Trace |
| | | | | |
| .275 | .281 | .268 | | .164 |
| | | | | |
| ...... | | | | Trace |
| | | | | |
| | | | | ...... |
| | | | | |
| | | | | ...... |
| | | | | |
| ...... | ...... | ...... | ...... | Trace |
+-----------------+-----------------+------------------+-----------------+-----------------+
| 113.644 | 113.651 | 49.630 | 205.500 | 60.507 |
+-----------------+-----------------+------------------+-----------------+-----------------+
+----------------+-----------------+-----------------+-----------------+------------------+-----------------+
| | | | | | |
|Pyramid Lake,[193]| Sevier Lake, | Walker Lake,[194] | Winnemucca | Van Lake | Aral Sea |
| Nev. | Utah | Nev. | Lake, Nev. | | |
| | | | | | |
| ...... | ...... | 1.003 | 1.001 | | |
| | | | | | |
| Aug. 1882 | 1872 | Sept., 1882 | Aug., 1882 | | |
| | | | | | |
| F. W. Clarke | O. Loew | F. W. Clarke | F. W. Clarke | Chancourtois | |
| | | | | | |
| _Ante_, pp. 57 |U. S. Survey, W. | _Ante_, p. 70 | _Ante_, p. 63 |Bischof’s Chemical| Roth Chemical |
| and 58 |100 M., Vol. III,| | | Geology, Vol. I, | Geology, p. 465 |
| | p. 144 | | | p. 94 | |
+----------------+-----------------+-----------------+-----------------+------------------+-----------------+
| 1.1796 | 28.840 | .85535 | 1.2970 | 8.502[4] | 2.4512 |
| | | | | | |
| .0733 | | Trace | .0686 | .246 | .0584 |
| | | | | | |
| ...... | ...... | ...... | ...... | | .0022 |
| | | | | | |
| .0089 | .118 | .02215 | .0196 | ...... | .4581 |
| | | | | | |
| .0797 | 2.000 | .03830 | .0173 | .157[4] | .5965 |
| | | | | | |
| | | | | ...... | ..... |
| | | | | | |
| ...... | ...... | ...... | ..... | Trace[197] | .0008 |
| | | | | | |
| 1.4300 | 45.500 | .58375 | 1.6934 | 5.693 | 3.8386 |
| | | | | | |
| ...... | | ...... | ...... | ...... | .0029 |
| | | | | | |
| .4900[7] | ...... | .47445[7] | .3458[198] | 5.267[195] | .0918 |
| | | | | | |
| .1822 | 9.345 | .52000 | .1333 | 2.555 | 3.3368 |
| | | | | | |
| | | ...... | | | .0011 |
| | | | | | |
| | | | | | Trace |
| | | | | | |
| ...... | | ...... | | ...... | ...... |
| | | | | | |
| .0334 | | .00750 | .0275 | .180 | .0032 |
| | | | | | |
| | | | ....... | ...... | ...... |
| | | | | | |
| | | | | | ...... |
| | | | | | |
| | | | | | Trace |
| | | | | | |
| | | | | | Trace |
+----------------+-----------------+-----------------+-----------------+------------------+-----------------+
| 3.4861 | 86.403 | 2.50150 | 3.6025 | 22.600 | 10.8416 |
+----------------+-----------------+-----------------+-----------------+------------------+-----------------+
CHAPTER VII.
THE ORIGIN AND DESCENT OF ROCKS.
It has been the current opinion that the earth was once in a molten
state, and thence cooled to a solid condition, and hence that all the
primitive rocks were igneous. Even those who think that the earth may
never have passed through a molten state agree that the oldest known
rocks are either true igneous rocks, or rocks of very similar nature. A
molten magma may, therefore, be taken as the mother state of the rocks.
Starting with this conception, the natural order of events suggests the
inquiries (1) how rocks are formed from molten magmas, (2) what natures
they assume, (3) how other rocks are derived from them, (4) how still
other rocks are derived from these derivatives, and so on. To answer
these inquiries is to trace out the generations of rocks and learn the
general history of rock-formation.
(1) The process by which igneous rocks are formed from lavas is
actually taking place in existing volcanoes. As these are widely
scattered over the face of the earth, the material poured out by
them represents different parts of the interior and varies in nature
accordingly. This affords the means of studying the differences that
arise from differences of material. This is a radical consideration,
for variations in composition give rise to the most fundamental
distinctions between rocks, though by no means the only ones. Rocks
which have the same composition often differ greatly in texture or
structure, owing to the varying conditions under which they were
formed. In the solidification of rocks from the molten state, the
rate of cooling causes many differences. A means of studying this is
afforded by the various lava flows that are now being poured out on
the surface under different conditions; but a more important means is
afforded by extinct volcanoes, especially by those which have been
deeply cut open by erosion. In certain very ancient volcanoes, not
only have the solidified lava streams of the surface been cut across
by erosion, but the lava that remained in the crater, or in the neck
that led up from below, is laid bare for inspection. Exposures of even
more profound nature have been made by the great disruptions which
the outer part of the crust has suffered. In certain tracts there have
been profound fractures, and the formations on one side of these have
settled down and on the other side have been pushed up (faulted), so as
to expose parts that were once much below the surface. Sometimes also
the crust has been folded and crumpled, and the wrinkles thus formed
have afterwards been worn away or cut open by deep valleys, and rocks
that were once deeply buried have been laid bare. By the revelations
made in these and other ways, it has been learned that at various times
in the history of the earth molten matter has been thrust into fissures
or intruded between layers of the crust and cooled there, without
coming to the surface. Sometimes the lava appears to have forced its
way into the rocks, and sometimes to have lifted the upper beds and
formed great subterranean layers or tumor-like aggregates, called
bathyliths and laccoliths (Fig. 334). Such intruded bodies of molten
rock, solidifying under the varying conditions of such subterranean
situations, are a fruitful source of instruction respecting the
influence of varying rates and modes of cooling, as well as of other
attendant conditions.
[Illustration: +Fig.+ 334.—Diagram of a laccolith. (Gilbert.)]
It will thus be readily seen that the rate of cooling of the various
molten rocks must have differed very greatly. In the portions
poured out upon the surface there were sometimes narrow streams and
thin sheets, giving large exposure in proportion to the mass (Fig.
335), and sometimes thick flows and deep pondings in basins and
choked valleys, giving massive bodies with relatively small surface
exposure. There were explosions of the lava into minute particles
with almost instantaneous cooling, and there were eruptions beneath
the sea the peculiar effects of which are rather matters of inference
than of positive knowledge. In the portions underground there were
insinuations into thin fissures, on the one hand, and in-thrustings of
thick bodies, on the other. Some intrusions entered the upper part of
the crust where the rocks were cold and wet, and some were thrust into
the deeper portions where the rocks were warmer and less penetrated
by water. Sometimes the lava rose rapidly and was little cooled in
passage, sometimes slowly with more cooling en route, and sometimes
there were long halts between eruptions, with much opportunity to cool.
An almost infinite variety of conditions is thus presented, and with it
a rich field for the study of the modes of solidification.
[Illustration: +Fig.+ 335.—Fresh lava flow, with large surface
exposure. Holemaumau, Hawaii. (Libbey.)]
In the underground intrusions the additional factor of high pressure
was also present, and this is the third important condition in
determining the nature of igneous rocks.
The three factors, _composition_, _rate of cooling_, and _degree of
pressure_, require special consideration.
_Composition of Igneous Rocks._
All or nearly all the chemical elements known on the earth are found
in greater or less amounts in igneous rocks, and in a broad sense are
constituents of them. If there are any exceptions, they are most likely
to be found in the rarer elements in the atmosphere. Oxygen, nitrogen,
hydrogen, aqueous vapor, and carbonic acid, which make up the mass of
the present atmosphere, are all found in lavas and in their cooled
products. Probably all the rarer elements also occur in igneous rocks.
Helium is known to be given forth by springs.
=Leading elements.=—But although nearly or quite all the known chemical
elements enter into the igneous rocks, only a few of them are abundant.
These are regarded as normal or essential constituents, while the rarer
substances are regarded as incidental. By combining a large number of
the most trustworthy analyses of rocks of all sorts, F. W. Clarke[199]
has estimated the relative amounts of the more abundant elements in the
crust of the earth with the following result:
Percent. in
Element. Symbol. the Solid Crust.
Oxygen (O) 47.02
Silicon (Si) 28.06
Aluminum (Al) 8.16
Iron (Fe) 4.64
Calcium (Ca) 3.50
Magnesium (Mg) 2.62
Sodium (Na) 2.63
Potassium (K) 2.32
Titanium (Ti) .41
Hydrogen (H) .17
Carbon (C) .12
Phosphorus (P) .09
Manganese (Mn) .07
Sulphur (S) .07
Barium (Ba) .05
Strontium (Sr) .02
Chromium (Cr) .01
Nickel (Ni) .01
Lithium (Li) .01
Chlorine (Cl) .01
Fluorine (Fl) .01
------
100.00
It will be seen that only eight of the elements hold a high rank
in quantity. Many that are of the utmost importance in the history
of the earth and the affairs of men are low in the list, or do not
even appear in it at all, because their quantity is too small to be
estimated in percentages. The precious metals, and even some of the
more common metals, as lead, zinc, and copper, are too scarce to form
an appreciable percentage.
=Union of elements.=—In a general study of the igneous rocks we may
for the present neglect all but the first eight of these elements.
Out of these elements spring various chemical combinations, and out
of these combinations spring the various minerals, and out of the
combinations of minerals come the various rocks. The union of oxygen
with the other seven elements may be taken as a fundamental step in
this series of combinations. The result is the following oxides: Silica
(SiO₂), alumina (Al₂O₃), ferrous, ferric, and magnetic oxide (FeO,
Fe₂O₃, and Fe₃O₄), magnesia (MgO), calcium oxide or lime (CaO), soda
(Na₂O), and potash (K₂O). The oxygen sometimes unites in proportions
different from those here given, but such exceptions may be neglected
in a general study. We thus have nine leading oxides. Of these, silica
acts as an acid, or more strictly according to the newer chemical view,
as an acid anhydride. All the rest, except the magnetic oxide of iron,
and sometimes the oxide of aluminum, act as basic oxides.
In the older chemical philosophy these oxides were supposed to combine
by the simple union of an acid oxide with a basic oxide, and to remain
as oxide joined to oxide; thus silica (SiO₂) and lime (CaO) formed
silicate of lime (CaO,Si₂). The symbols express the idea better than
the words. This method is used in the older geological works and in
some of the later. But in the newer chemical doctrine, the oxides are
not believed to remain so distinct after their union, and the symbols
are written CaSiO₃, and the compound is named calcium silicate.
According to the modern doctrine of solution, some of the calcium,
silicon, and oxygen may exist as free ions in molten rock. The precise
way in which the elements are related to each other in these compounds
can scarcely be said to be known. For the general purposes of geology
it is most convenient to think of these oxides as uniting in the
simple fashion first named, and this involves no apparent geological
error in general studies, since they are oxides when they enter the
compound, and if the compound is decomposed they usually come forth
again as oxides; but in closer studies more complex unions, attended by
dissociations (ionization), must be recognized.
=Formation of minerals.=—As but one of the leading oxides that abound
in an average magma plays the part of an acid, the silica, a very
simple conception of the general nature of igneous rocks may be
reached by noting that they are mostly silicates of the seven leading
basic oxides—alumina, potash, soda, lime, magnesia, and the iron
oxides. This general idea is a very useful one and represents a most
important truth; but in its use we must not forget that there are many
exceptions. Sulphur, phosphorus, chlorine, and other elements unite
with the bases to form sulphates, sulphides, phosphates, phosphides,
chlorides, etc. So also there are many minor bases that form silicates;
and these minor bases unite with the minor acids to form many more or
less rare minerals. Again, there are native metals in some igneous
rocks. But altogether these hardly reach more than one or two percent.
of the whole.
There are, however, two exceptions of more importance. In the molten
magma the acid and basic elements are not always evenly matched. When
there is an excess of silica, a portion remains free and takes the
form of quartz (SiO₂). If there is an excess of the basic oxides, the
weakest one is usually left out of the combination. This is commonly
the iron oxide, which then usually takes the form of magnetite (Fe₃O₄).
It is a singular fact that quartz often forms when there is no excess
of silica, and magnetite when there is no excess of base. Quartz
(free acid anhydride) and magnetite (free basic oxide) sometimes
occur in the same rock. The explanation for this is yet to be found.
These form rather important exceptions to the generalization that the
igneous rocks are mostly made up of silicates, but, thus qualified,
it expresses the essential truth, and has the merit of embodying the
central chemical fact relative to these rocks.
=Sources of complexity.=—But here simplicity ends. As we pass on to
the specific silicates that are formed, we encounter several sources
of complexity. In the first place, the silica unites with the bases in
different ratios and thus gives rise to unisilicates or orthosilicates
(ratio of oxygen of bases to oxygen of silica, 1:1), subsilicates
(ratio more than 1), bisilicates (ratio 1:2), trisilicates or
polysilicates (ratio 1:3 or higher), and combinations of these. All the
bases are not known to combine in all these ways, but many do in more
than one of them. Still, if the silica were content to unite with each
of the bases by itself alone, the results would remain comparatively
simple; but instead of this it unites with two or more at the same
time; and, more than that, it unites with them in varying amounts. The
case would still remain measurably simple if these chemical compounds
always crystallized out by themselves, each compound forming one
mineral, and but one; but the different silicates have the confusing
habit of crystallizing together in the same mineral. A crystal
may thus sometimes be seen, under the microscope, to be made up of
alternating layers of different silicates; e.g., a microscopic layer
of an aluminum-calcium silicate may be overlain by a microscopic layer
of an aluminum-sodium silicate, and the alternation may be repeated
throughout the crystal, giving it a banded structure. There is reason
to believe that this is true in many cases where the microscope fails
to detect it, and that less symmetrical comminglings of silicates may
take place. As such alternations or mixtures are not governed by any
known mathematical law, as is the case in chemical compounds, there is
no determinate limit to the number of combinations that may arise. As
a matter of fact, new ones are still being discovered in the progress
of research, and the total number that may ultimately be found can
scarcely be prophesied.
As a result of all this fertility of combination, the total number of
silicious minerals in igneous rocks is large. It is the function of the
mineralogist to treat of these minerals as such. The geologist deals
with them as constituents of the earth and as factors in its history.
Only a few of them are so abundant as to require special individual
notice in a general study of the earth. It may be remarked also that
only a few of them can be identified by simple inspection as they
occur in the rocks, partly because of the delicacy of the distinctions
between many of them, and partly because of their minuteness and
intricate intermixture. The resources of the polarizing microscope
are necessary for safe determination in most cases. The student need
not feel embarrassment or discouragement if he is often unable to
recognize the constituents of the intimately crystalline rocks. Their
determination has grown to be a profession by itself.
=The leading minerals of igneous rocks.=—Fortunately for the simplicity
of geological study, a few minerals make up the great mass of the
igneous rocks. These few are _quartz_, the _feldspathic minerals_,
the _ferromagnesian minerals_, and the _iron oxides_. Quartz (silica,
SiO₂) is the free acid already mentioned. The feldspathic and
ferromagnesian minerals are the leading silicates of the earth’s crust,
and vastly surpass all others in abundance. The feldspathic group
embraces minerals formed by silica in union with alumina, together
with either potash, soda, or lime, or two or more of these together.
The ferromagnesian group embraces minerals formed by the union of
silica with iron, magnesia, and lime, together with more or less of the
other basic oxides. These statements are only true in a very general
sense. Admixtures, replacements, and impurities are so frequent as to
break down all sharp, simple definitions. The feldspathic minerals
are normally light in color, ranging from white to red or gray. The
ferromagnesian minerals are normally dark (commonly greenish) from the
presence of iron, the great coloring element of rocks. But these color
distinctions do not hold good in detail and cannot be much trusted as a
means of identification.
=The feldspathic minerals= (p. 462) embrace the potash feldspars,
_orthoclase_ and _microcline_; the soda feldspar, _albite_; the lime
feldspar, _anorthite_; and the mixed feldspars intermediate between
albite and anorthite, viz., the soda-lime feldspar, _oligoclase_, the
lime-soda feldspar, _andesine_, in which lime and soda are nearly
equal, and the lime-soda feldspar, _labradorite_, in which the lime
predominates; together with _leucite_, a potash silicate higher in
alkali than orthoclase, and _nephelite_, a soda silicate higher in
soda than albite. Leucite and nephelite are usually classified as
_feldspathoids_, not as feldspars. It is to be understood that alumina
is normally present in all these. Additional details respecting these
minerals may be found in the reference list, p. 460.
Among the =ferromagnesian minerals= the most important are the
pyroxenes, the amphiboles, and the biotite type of mica. Olivine is
of subordinate importance. The pyroxenes (p. 465) and amphiboles
(p. 460) have nearly the same chemical composition, but differ in
crystallization and physical properties. _Hornblende_ (an amphibole)
has been melted, and on cooling under proper conditions found to take
on the form of _augite_ (a pyroxene). Pyroxene is sometimes altered
into _uralite_, one of the amphiboles. The pyroxenes and amphiboles
are the most abundant of the dark minerals in crystalline rocks.
The leading members of the pyroxene group are _augite_, _diallage_,
_hypersthene_, _enstatite_, and _soda pyroxene_. The chief members of
the amphibole group are _hornblende_ and the _soda amphiboles_. All are
essentially silicates of magnesia and iron oxide, with or without the
addition of lime, soda, and alumina. Details respecting these may be
found in the reference list.
The two leading =micas= are the iron-magnesia mica, _biotite_, and the
potash mica, _muscovite_, the familiar “isinglass” of the stove-door.
Chemically, muscovite should go with the potash feldspars, but it
is distinguished from them by its crystalline habit and physical
properties. The biotite should go chemically with the pyroxenes and
amphiboles, which it closely resembles except in its crystalline
properties. Details respecting the micas may be found in the reference
list, p. 464.
Two =iron oxides=, magnetite (Fe₃O₄) and hematite (Fe₂O₃) are widely
disseminated in igneous rocks. They constitute the free bases already
mentioned.
=Summary of salient facts.=—The salient facts are, therefore, (1) that
out of the seventy-odd chemical elements in the earth, eight form the
chief part of it; (2) that one of these elements uniting with the rest
forms nine leading oxides; (3) that one of these oxides acts as an
acid and the rest as bases; (4) that by their combination they form a
series of silicates of which a few are easily chief; (5) that these
silicates crystallize into a multitude of minerals of which again a few
are chief; and (6) that these minerals are aggregated in various ways
to form rocks. Possessed of these leading ideas, we are prepared to
turn to the consideration of some of the conditions under which these
combinations take place in the formation of rocks from molten magmas.
THE NATURE OF MOLTEN MAGMAS.
We easily fall into the habit of thinking of molten rock as we think
of a molten metal, merely as a substance which has passed from the
solid to the liquid condition because of high temperature. With the
return of low temperature a molten metal returns to the solid state
usually in the same molecular condition which it possessed before.
The point of fusion and the point of solidification are the same and
are rigidly fixed. If this were true of the constituents of a rock,
a definite order for the solidification of the several minerals
might be anticipated. As a matter of fact, the order is not the
same under all conditions, and, what is especially significant, the
order is far from being that in which the constituents would fuse
or would solidify separately. For instance, in a granite composed
chiefly of quartz, feldspar, and mica, the quartz is often the last
to take form, although it is more infusible than the feldspar or the
mica. This and other phenomena show that a molten magma is not to be
viewed simply as a fused substance, but rather as a _solution_ of
one silicate in another, or as a solution of several silicates in
one another mutually. The high temperature is to be regarded merely
as a condition prerequisite to solution, or as the condition of
fusion of some one constituent which then dissolves the others. If
crystals of snow, sugar, and salt be mixed at a low temperature and
compacted, the mass may be regarded as an artificial rock. On raising
the temperature, all will pass into solution while the temperature is
still somewhat below the melting-point of the snow, the most fusible,
and while it is much below that of either the sugar or the salt. This
particular case is instructive because the ice is not simply fused by
temperature; the affinity of the salt plays a part. If the temperature
were again lowered, the sugar and salt would not crystallize out at
their fusing-points, but would remain in solution down to and even
below the normal freezing-point of water; in other words, they would
remain in solution until the water crystallized out and forced them
to take the solid state. This holds good when the amounts of the
sugar and salt are small relative to the water. If, on the contrary,
their quantity is large relatively, crystallization will take place
at higher temperatures and before the water crystallizes to ice. From
this it appears that the salt and sugar might crystallize either before
the water or after it, according to the degree of concentration. The
behavior of mixtures of minerals in passing into and out of the molten
condition appears to be quite analogous to this, and hence a great
variety of results attend the process, dependent upon the number, the
nature, and the relative quantities of the ingredients. The approved
conception of the genesis of a rock from a molten magma (when ample
time is given) is that one compound after another crystallizes out
as the temperature falls and its point of _saturation_ for each is
reached, until the whole has been solidified. The modes of combination
of the elements in the molten magma are not necessarily the same as
those in the derivative crystals; indeed, the combinations doubtless
change as the process proceeds; certain constituents being taken out,
the remaining ones probably rearrange themselves.
=Time required in crystallization.=—The liquid magma of igneous rocks
is essentially a fluid glass or slag. It is analogous to common glass,
which is a silicate of potash, soda, or other base, except that
usually common glass is relatively free from iron and other coloring
substances, while these abound in the natural magmas and render them
dark and more or less opaque; but the fundamental nature is the
same, except that the natural lavas are usually mixtures of several
silicates, while the artificial glasses consist of only one, or at most
a few. Furnace slag is essentially an artificial lava.
When a lava is cooled quickly, the commingled silicates solidify in the
diffused condition essentially as they were in the liquid; for there
is no time for the silicate molecules of a like kind to come together,
particle by particle, in regular systematic order, as required in
crystallization. The essential feature of crystallization is this
systematic arrangement of the molecules according to a definite plan,
giving a specific crystal form, as a cube, a hexagonal prism, etc.
There are six (sometimes made seven) fundamental systems of
crystallization, and a multitude of variations of special form in each
system. The treatment of these forms belongs to mineralogy.
In a thick viscid liquid, this systematic arrangement of molecules
into definite crystal forms takes place slowly, for the crystalline
force in the silicates is far less energetic than that in water,
which crystallizes into ice with much rapidity and with great force.
Because of this slowness, the solidification of the lava may catch
the process of crystallization at any stage. If the lava is cooled
quickly, the result is a glass; if less quickly, part glass and part
crystals; if slowly enough, all becomes crystalline. In general the
slower the growth the larger the crystals. The solidification product
may, therefore, range from a glass to a mass of crystals; i.e., it may
be (1) wholly glass, (2) a glassy matrix with a few small crystals
scattered through it, (3) a less abundant glassy matrix with more and
larger crystals, (4) a mere remnant of glass in a mass of crystals, or
(5) a mass of crystals with no glass.
=Successive stages of crystallization.=—Since eruptions take place
intermittently, it is obvious that cooling of the lava may be in
progress in its hidden reservoir during the quiescent intervals between
eruptions. After a certain stage of partial crystallization has been
reached during such time of quiet, a renewal of eruption may take place
and the whole mass of lava be shifted into quite new conditions, and
a second phase of solidification may be superposed on the one already
started. The rock will then show two phases of crystallization: (1)
large crystals of the kind or kinds most prone to develop in the given
lava may have grown during the first long stage of slow subterranean
cooling, while the greater part of the lava still remained liquid; and
(2) small crystals or glass may have developed when the more rapid
cooling under the new conditions took place. The result would be large
crystals set in a matrix of small crystals or of glass, a combination
styled _porphyritic_. In such cases the lava, in its later stages,
carries the large crystals floating throughout its mass, and is not a
simple liquid.
THE FRAGMENTAL PRODUCTS OF SUDDEN COOLING.
=Pyroclastic rocks.=—The extreme example of sudden cooling is presented
when lavas are violently exploded into the air and solidify almost
instantly. The resulting glassy particles or filaments, if small,
constitute _volcanic ash_. The explosion appears to be due to steam and
other gases which are held in the deeper lava under great pressure, but
which, as they rise toward the surface of the lava where the pressure
is relieved, expand with explosive violence. It is probably also due in
part to progressive crystallization, which forces the gases out from
the part that crystallizes and overcharges the rest. Sometimes the
projected particles draw after themselves long _filaments_ like the
threads of spun glass, and sometimes while in the air they divide and
draw apart, spinning a filament of viscid lava between them. A variety
of this kind at the volcano of Kilauea in Hawaii is known as “Pele’s
hair.” These light filaments drift with the wind and lodge on the lee
side of the volcano, covering the surface “like mown grass” (Dana).
[Illustration: +Fig.+ 336.—Volcanic bomb. About half natural size.
(Photo. by Church.)]
When the exploded fragments are coarser they fall about the volcanic
vent and form the _tuffs_ (_tufa_) of which most steep volcanic cones
are chiefly built. In these larger fragments, crystals are not
infrequently found, and the same is even true of the volcanic ash.
These crystals are undoubtedly such as had already been formed in the
lava before it exploded, and their formation, as suggested above, may
have contributed to the explosion.
Fragments too large to be borne far away by the air, but still small,
are known as _lapilli_, especially if they are somewhat rounded and
gravel-like. A finer variety, of the nature of sand, much used in
making Portland cement, is locally known as _puzzolana_.
[Illustration: +Fig.+ 337.—Volcanic bomb of unusual form, 13 foot long.
Cinder Buttes, Idaho. (Russell, U. S. Geol. Surv.)]
The rougher, irregular fragments of a clinker-like nature ejected by
volcanoes are known as _scoriæ_ or _cinders_. They are more or less
distended by gas-bubbles and are hence light and pumiceous.
The larger masses of lava ejected into the air are often caused to
rotate by the unequal force of the projection, or by the unequal
friction of the air, and to assume spheroidal forms, the internal gases
at the same time often expanding and rendering the mass vesicular.
These rounded projectiles are known as _volcanic bombs_ (Figs. 336 and
337). Balls of lava that have originated in rolling movements of the
seething mass, or in other ways, are also styled bombs. Usage is not
altogether harmonious or consistent in the application of the term.
The larger masses that are projected into the air are more or less
vesicular from the expansion of included gases, as already noted, and
so the fragmental products of volcanic action grade into the vesicular.
The type of this class is _pumice_, in which the gas cavities make up
by far the larger part of the volume of the whole mass, and the whole
is reduced to the condition of a solidified froth or foam. So thin are
the dividing films of glassy material in some cases that the whole is
pure white, though the same material in solid mass would be dark. This
solidified glassy froth is often lighter than water and floats freely
on the sea until it becomes “water-logged” and sinks. Dredgings of
the deep sea show that much pumice has accumulated there, and being
far from the land has escaped burial by the sediments borne in by the
rivers.
All of these fragmental rocks produced by volcanic action are known
as _pyroclastic_ (fire-fragmented) rocks, a general term of much
convenience in distinguishing them from lava-flows, on the one hand,
and from the fragmental rocks produced by air and water (ordinary
clastics), on the other.
THE GLASSY ROCKS.
=The solid glasses.=—The quick cooling of lava-flows into solid glasses
is chiefly dependent on their exposure at the surface. Hence it is
often the case that the exterior of a lava-flow is glassy in greater
or lesser degree, while the interior is more or less crystalline.
Quick cooling is sometimes also due to the intrusion of the lava in
thin sheets into fissures in cold rocks. When massive bodies of lavas
penetrate solid rocks, the lava does not usually cool so fast as to
prevent some degree of crystallization, and the crystallization may
even become complete; but if the intruded lava sheet be very thin,
the lava is liable to be cooled to a nearly perfect glass. The glassy
condition is, therefore, subject to indefinite gradations. As a rule,
the acid lavas are stiffer at the same temperature than the basic ones,
and crystallize more slowly, so that acid glasses are more common than
basic ones. The basic rocks usually crystallize pretty thoroughly,
except on the immediate surface of the flows.
=The first stages of crystallization.=—The microscopic study of the
volcanic glasses reveals great numbers of minute forms known as
_crystallites_, _microlites_, _globulites_, etc., that appear to
be first steps in crystallization, though many of them do not take
definite geometrical shapes and some do not show the optical characters
of crystals. There are minute globules (globulites), needles, and
hair-like bodies (trichites) of more or less indeterminate nature,
together with other forms that can be seen to be certainly the initial
forms of well-known minerals.
[Illustration: +Fig.+ 338.—Flow structure in rhyolite. Nearly natural
size. (Photo. by Church.)]
=The obsidians.=—Of the compact glassy rocks, _obsidian_ is the best
type. It is essentially a natural glass, formed usually of acid
silicates. It has the close texture, conchoidal fracture, and other
qualities of glass. It is usually black, but sometimes red, brown,
purple, bluish, or gray. While chiefly of glass, it usually contains
more or less of the incipient crystals above described, showing
that even here the first step in the gradation to the next or the
crystalline stage has been taken. These incipient crystals sometimes
become so abundant as to change the texture from the vitreous to the
stony order. In some cases, the stony texture seems to have been
developed in the obsidian after it was formed, the change being a part
of a subsequent process of devitrification, but in other cases the
crystals seem to be original. Besides these, there are often small
globular bodies known as spherulites.
Varieties of glassy rock in which the embryo crystals are more numerous
and the glassy texture less perfect, are known as _pitchstones_. The
fresh surfaces of these have rather the aspect of pitch or resin
than that of true glass; hence their name. Like the obsidians, they
are usually dark, but they take on greenish, brownish, yellowish,
and light-colored hues as well. Sometimes glassy rock fractures in
small spheroidal forms like pearls, and is known as _perlite_. Basic
glasses are relatively rare, and while usually included under the term
obsidian, are sometimes given special names.
[Illustration: +Fig.+ 339.—Flow structure in volcanic glass. About half
natural size. (Photo. by Church.)]
[Illustration: +Fig.+ 340.—Flow structure in porphyry, shown by the
position of the large crystals. About two-thirds natural size.
(Photo. by Church.)]
[Illustration: +Fig.+ 341.—Scoriaceous texture. About four-fifths
natural size. (Photo. by Church.)]
SPECIAL STRUCTURES.
=Flow structure.=—Lavas that cool into glassy rocks frequently contain
gas cavities, colored spots and variations of texture which, together
with the hair-like embryo crystals, are drawn out into lines, streaks,
and parallel belts by the flow of the viscous mass, giving rise to
_rhyolitic_ or flow structure (Figs. 338 and 339). Rocks in which this
is the most pronounced feature were formerly known as rhyolites, though
the term has drifted away from this original meaning and has been
applied to a class of acidic rocks. The obsidians and pitchstones may
be more or less rhyolitic under the microscope, though to the naked
eye they may appear only as a glassy or resinous mass. The rhyolites
generally have but an imperfect glassy texture, since the crystals
and the cavities sometimes make up a notable part of the mass, the
glassy portion being scarcely more than a matrix in which the crystals,
spherulites, and cavities are carried. By an increase of the crystals
in number and size, the rock passes by gradations into porphyry or
phanerite.
[Illustration: +Fig.+ 342.—Porphyritic texture. Two-thirds natural
size. (Photo. by Church.)]
=Amygdaloids.=—In lava-flows the included steam often collects in
bubbles near the surface as the lava cools and forms a vesicular
portion with a scoriaceous texture (Fig. 341). In its upper part,
the vapor bubbles may be numerous, while below they become more and
more scattered until they disappear. Similar bubbles are also often
found near the bottom of a sheet of lava. This is perhaps due to the
rolling under of the frontal surface of the lava-stream as it flows.
Later, these cavities often become filled with minerals deposited from
solution and the rock then becomes an amygdaloid, but this filling is a
secondary action.
[Illustration: +Fig.+ 343.—Porphyritic texture. Natural size. (Photo.
by Church.)]
THE PORPHYRITIC ROCKS.
When the conditions are such that after a part of the magma has formed
distinct crystals floating in the remaining liquid lava, there is
a change which causes the rest to solidify as a glass or as a mass
of small crystals, the structure is known as _porphyritic_, and the
rocks possessing it are called _porphyries_. This differentiation into
distinct crystals set in a ground-mass of minute crystals or of glass
often gives a mottled or variegated aspect to the rock, especially
if the matrix of glass or minute crystals differs in color from the
distinct crystals. This structure is much oftener developed in acidic
rocks than in basic ones, because the latter crystallize more readily.
The most common porphyritic crystals are feldspar and quartz, though
they are by no means the only ones. The matrix is also usually felsitic
or quartzose, but not necessarily so. The character is a structural
one, and is not dependent upon any special chemical or mineralogical
constitution. The distinct crystals are known as phenocrysts, and the
varieties of porphyries are named from the characteristic phenocryst,
e.g., quartzophyre (quartz-porphyry) if the conspicuous crystals
are quartz, orthophyre if orthoclase, augitophyre if augite, etc. A
convenient classification has recently been proposed[200] into (1)
_leucophyre_ (white porphyries), which have a light-colored ground-mass
set with phenocrysts of any kind, and (2) _melaphyres_ (black
porphyries), which have a dark-colored ground-mass, with phenocrysts
of any kind. While it is to be hoped this usage will prevail, it is to
be noted that these terms, especially the latter, have been used in a
different sense. (See reference list of rocks, p. 445.)
In many cases the ground-mass itself becomes minutely crystalline
and the porphyritic aspect is due simply to large distinct crystals
set in a mass of minute obscure ones. The rock is then really
_holocrystalline_, but the term porphyry is applied to it. In other
rocks the crystals of the ground-mass become more and more distinct,
the porphyritic aspect gradually disappears, and there is a graduation
into the next class.
THE PHANEROCRYSTALLINE ROCKS.
=The phanerites.=—When time enough is given for the cooling process the
molten magma becomes completely crystalline. The holocrystalline rocks
hence include a large series, ranging from the most acid to the most
basic. In this class the differentiation of the rock material and the
formation of distinct minerals reach a high stage, and as a natural
result the varieties of rock are numerous. Taken as a group they are
phanerites. If they are to be more particularly characterized, it is
usually done on the basis of the minerals of which they are composed.
The following are the leading types, beginning with those which are
rich in silica and poor in basic oxides, and ending with those which
are rich in basic oxides and poor in silica.
[Illustration: +Fig.+ 344.—Granitic texture. About half natural size.
(Photo. by Church.)]
=The granites.=—The term granite was originally used to designate
a granular, i.e., a distinctly crystalline, rock, and it is still
popularly and properly so used. In scientific treatises it has usually
been confined to a special aggregate of crystals of quartz, feldspar,
and mica. It has recently been proposed to give it again a more general
application, though not quite its original one, by including under it
all holocrystalline rocks composed of dominant quartz and feldspar
of any kind, with mica, hornblende, or other minerals in subordinate
amount. In scientific literature as it now stands, granite consists of
quartz, feldspar, and mica, the feldspar being of the alkali-potash
or soda variety (orthoclase, microcline, or albite), and the mica,
either muscovite or biotite. In the type form the crystals are distinct
and sometimes large (Fig. 344). They are intimately mingled with one
another, and in growing, interfered more or less with each other and
so became interlocked. The granites are among the most common and
easily recognized of the holocrystalline rocks. Their color is mainly
dependent upon the feldspar, the red and pink varieties of the mineral
giving rise to red granite, and the white varieties to gray granite.
[Illustration: +Fig.+ 345.—Graphic granitic (or pegmatitic) texture.
Nearly natural size. (Photo. by Church.)]
Very few granites conform strictly to the type. They vary by the
addition and substitution of other minerals, and these sometimes
become as prominent as the type minerals. The soda-lime feldspars
sometimes take the place of the orthoclase, or accompany it; hornblende
and other minerals take the place of the biotite, or occur with it;
and so on. Whenever one of these replacing or accessory minerals is
notable in quantity, its name is often prefixed, as hornblende-granite,
oligoclase-granite, zircon-granite, etc. In this way the rock grades
almost insensibly into the syenites, diorites, etc. Variations also
arise from the absence of one of the three leading minerals. If mica
is absent, the rock is termed an _aplite_ (quartz and feldspar). If
the feldspar is absent, it is called a _greisen_ (quartz and mica).
If quartz is absent, it is termed a _minette_ (feldspar and mica).
These varietal terms are neither universally nor always consistently
used, and it is to be hoped they will be replaced by the systematic
nomenclature recently proposed and outlined later (p. 451).
The granites were formed from a magma rich in silica, alumina, potash,
and soda, but generally poor in lime, iron, and magnesia. Incidentally
other substances were present. The alumina, potash, and other bases
united with so much of the silica as was required to form the feldspars
and micas, and the remaining silica crystallized into quartz.
Granite is normally a massive rock without foliation or banding. If
it takes on these characters, it becomes a _gneiss_, and passes into
the foliated or schistose class of rocks, to be discussed later. The
texture of graphic granite (see pegmatite) is notably peculiar, due to
the simultaneous crystallization of the quartz and feldspar (Fig. 345).
=The syenites.=—When the mica of a granite is replaced by hornblende,
the rock is now commonly known as a _hornblende-granite_, but it was
formerly called _syenite_, because found at Syene on the Nile. The term
syenite is now applied to a rock consisting essentially of feldspar
and hornblende or mica, but there is a complete gradation from the
granites to the syenites. The magma of the syenites was richer in
iron and magnesium than the typical granitic magma. The syenites also
grade into other classes, as do the granites, and are named by similar
prefixes, as augite-syenite, etc., and some of these varieties have
special names. The syenites are red or gray, according to the color of
the feldspar, and are usually darker than the granites. The texture of
syenite is like that of granite. In the scheme of field names recently
proposed, syenite is made to include all holocrystalline rocks composed
mainly of feldspar of any kind, with subordinate amounts of mica,
hornblende, pyroxene, and other minerals, but without a noticeable
amount of quartz.
=The diorites.=—These embrace rocks which were crystallized from a
magma still poorer in silica and the alkalies, and richer in the earthy
bases. In composition they closely approach the ideal average rock,
but usually fall a little below it in silica and the alkalies, and
rise a little above it in the earthy bases. In current usage, diorite
is defined as an intimate mixture of crystals of hornblende and a
plagioclase feldspar. It differs from the syenite in having plagioclase
feldspar instead of orthoclase. By substitutions and the addition of
accessory minerals, the diorites graduate toward the granites and
syenites on the one hand, as already noted, and into gabbros on the
other.
In the scheme recently proposed, all holocrystalline rocks in which
hornblende is dominant and feldspar subordinate are classed as diorites.
=The gabbros.=—The name gabbro was formerly applied to a coarse-grained
basic rock consisting of labradorite and diallage, but the name has
been gradually extended until it embraces a large group of rocks that
have essentially the same composition as the dolerites mentioned below,
but are coarser in crystallization, and the crystals do not embrace one
another (i.e., are not ophitic). The principal minerals are plagioclase
(normally labradorite) and pyroxene (normally diallage) with magnetite
or ilmenite. They are usually dark, heavy rocks. The pearly luster of
the cleavage faces of the diallage, when present, gives a peculiar
sheen to a fresh surface of the rock. In the recently proposed field
names, gabbro is made to include all phanerocrystalline rocks in which
pyroxene predominates, attended by feldspar of any kind in subordinate
quantity, with or without hornblende or mica.
=The peridotites.=—These stand at the basic end of the series, having
been formed from a magma in which the silica was low (39–45 per cent.),
as were also the alumina, lime, and alkalies, but in which the magnesia
was relatively very high, ranging from 35 to 48 per cent. The rock
consists very largely of olivine associated with pyroxene, magnetite,
and other very basic minerals. Little or no feldspar is present. The
peridotites are much less abundant than the preceding classes and
represent a very distinctive phase of the magma in which the magnesia
was greatly concentrated.
Closely allied to the peridotites are rocks which are made up largely
of a single basic mineral, as _augitite_, _pyroxenite_, _hornblendite_,
rocks essentially formed of the minerals augite, pyroxene, and
hornblende respectively. It will be noted that in these rocks the magma
became quite simple in nature, just as at the acid end of the series
certain rocks become comparatively simple from the concentration of the
acid element, as in certain acidic granites, felsites, etc. (See pp.
523–524.)
=The basalts.=—The term basalt is used in a somewhat comprehensive
way to embrace dark, compact, igneous rocks that appear to be nearly
homogeneous, owing to the minuteness of the crystals, which are
usually so small as to be identifiable only under the microscope.
In some cases the crystals are scattered throughout a ground-mass
after the porphyritic fashion. In some of these cases there is a true
glassy base, and in such cases the rock does not strictly belong in
the holocrystalline group. In the more typical cases the constituent
minerals are very minutely crystallized and intimately intermixed. The
leading minerals are plagioclase (usually labradorite or anorthite)
and pyroxene (usually augite), with olivine and magnetite or ilmenite
usually present. There is a considerable range in chemical nature,
but the basalts are relatively poor in silica, usually also low in
potash and soda, but rich in lime, magnesia, and the iron oxides. They
are classed as basic and are sometimes highly so. The magmas of the
basalts are especially fluid, and when poured forth upon the surface
easily spread out in thin sheets. In cooling they are prone to take on
a columnar or basaltic structure, the columns standing at right angles
to the surfaces exposed to cooling. The columns are sometimes curved,
owing to the peculiar attitude of the cooling surface. The columns of
Giant’s Causeway and Fingal’s Cave are familiar examples.
=The dolerites.=—The basalts graduate insensibly into the dolerites;
indeed the dolerites may be regarded simply as basalts of coarser
crystallization. The minerals are evident to the eye and range up
to medium size. The more abundant minerals are plagioclase feldspar
(labradorite or anorthite), with one or more of the ferromagnesian
minerals (augite, olivine, or biotite), and magnetite or ilmenite. In
the growth of the minerals one crystal frequently embraces others,
giving an ophitic structure. The dolerites have many varieties, due
either to accessory minerals or to the development of some of the
constituents more amply than the rest. The type may be said to consist
of plagioclase and augite, the other minerals being regarded as
accessories. Magnetite or ilmenite is almost universally present. The
varieties are usually designated by prefixes, as olivine-dolerite,
enstatite-dolerite, etc., but special names are also used for some of
these.
[Illustration: +Fig.+ 346.—Conglomerate, Carboniferous series. Bancroft
Place, Newport, R. I. (Walcott, U. S. Geol. Surv.)]
The ancient dolerites have usually undergone internal changes and
such rocks are often called _diabases_. While the use of the term has
not been uniform, it accords with the better practice to regard the
diabases simply as partially altered dolerites and basalts. In general,
therefore, the diabases are but ancient dolerites.
_General names._
The difficulty of distinguishing many of the foregoing rocks from each
other by any means available in the field, owing to the minuteness
of the crystals, and to the gradation of one type of rock into
another, makes it desirable to employ certain general names which will
correctly express the leading character of the rock without implying a
knowledge of the precise mineral composition. A convenient term of this
kind is _greenstone_, which merely indicates that the ferromagnesian
minerals are prominent and usually give a greenish or dark cast to the
rock. The greenstones embrace the diorites, dolerites, some of the
gabbros and the basalts, and may even extend to the peridotites and
some of the more hornblendic of the granitoid rocks. Another convenient
name is _trap_, which may be used for any dark, heavy igneous rock. The
name (from _trappe_, stairs) refers to the step-like arrangement which
the edges of the superimposed sheets of lava often take, especially
when the lava is of the free-flowing, basaltic kind.
[Illustration: +Fig.+ 347.—Brecciated limestone, Calciferous formation.
One mile south of Highgate Falls, Vt.]
The term basalt is sometimes used to embrace any of the very
fine-grained dark igneous rocks. In such cases, it covers the very
fine-grained dolerites, diorites, peridotites, etc. The term granite
was used originally for any coarse-grained crystalline rock, and there
is a tendency to revive this early use. In general descriptions, some
of our best petrographers call any coarsely crystalline rock (e.g.,
coarse-grained syenites, diorites, gabbros, etc.) granite. The term
_granitoids_ may be used with strict propriety to cover all rocks of
this class.
DERIVATION OF SECONDARY ROCKS.
Rocks, though commonly made the symbol of the abiding, are subject
to constant slow changes. Through these changes newer rocks have
been derived from older ones, and still others in turn from these
derivatives, and so on in an endless chain. All derived rocks are
conveniently termed secondary, though they may be several generations
removed from the primitive rocks, and even the primitive rocks, as we
now understand them, may be themselves derived. The ordinary changes
of rock are most active at or near the surface, and the processes
of such change have already been discussed in part under the titles
“Weathering” (pp. 54 and 110), “Erosion” (pp. 119–123 and 342–349),
“Transportation” (pp. 115–119 and 354–355), and “Deposition” (pp.
177–204 and 355–363).
[Illustration: +Fig.+ 348.—Quartzitic breccia. About one-third natural
size. (Photo. by Church.)]
[Illustration: +Fig.+ 349.—Section of limestone showing abundant
fossils imbedded in a matrix made up of comminuted shell matter.
About two-thirds natural size. (Photo. by Church.)]
[Illustration: +Fig.+ 350.—Limestone composed chiefly of shells. About
three-fourths natural size. (Photo. by Church.)]
=Regolith.=—The first great product of the surface changes is
_mantle-rock_ (_regolith_), which comprehends all the loose matter
that springs from rock decay, wear, fracture, and other forms of
disintegration. It lies in an unconsolidated sheet on the face of the
land, whether as soil, sand, clay, earth, gravel, or loose rock.
=Disrupted products: arkose and wacke.=—In dry regions, in cold
regions, on mountain heights and precipitous slopes, and under other
conditions where sudden changes of temperature and frost action work
efficiently, rocks are broken down into fine fragments without much
chemical decomposition. Such _disaggregated_ rather than decomposed
matter, if derived from granitic and similar crystalline rocks, is
termed _arkose_, or arkose sand, and consists of fragments of quartz,
feldspar, mica, etc. Common sand consists essentially of quartz grains.
If the fine fragments are derived from the darker igneous rocks, and
consist mainly of grains of plagioclase feldspar, and ferromagnesian
minerals, it is sometimes called _wacke_. This term is not widely used
in just this sense, but there seems to be an important place for it,
and it will be so employed in this work. These disaggregated sands are
but special phases of the mantle-rock.
=Disintegrated products.=—When the surface-rock is chemically
decomposed, the residual material is confined mainly to the insoluble
portions, i.e., the silicious and clayey parts; while the lime,
magnesia, soda, potash, and similar substances are largely dissolved
and borne to the ocean. The potash is somewhat more disposed to remain
with the clays than the soda, lime, or magnesia; but residues of all
are usually present.
_Classes of Sedimentary Rocks._
=Shales, sandstones, and conglomerates.=—As already shown in the
discussion of the atmosphere and surface-waters, the mantle-rock is
constantly being borne away and redeposited in lodgment spots on the
land or in the basins of the sea, while it is constantly being renewed
below. It is an evanescent but ever-renewed derivative mantle. In this
process of renewal, removal, and redeposition, the mantle material is
usually assorted into mud, sand, and gravel; and these several classes
of material are laid down more or less separately, and usually take
the stratified form, because their deposition depends on different
degrees of motion of the transporting waters or wind. When these
several classes of material become cemented or otherwise hardened,
they give rise to _shales_ (cemented muds), _sandstones_ (cemented
sands), and _conglomerates_ (or pudding-stones, cemented gravel, Fig.
346). If the coarse material remains angular, they form _breccia_
instead of conglomerates (Figs. 347 and 348). For the most part, the
deposits of mud, sand, and gravel are made under the sea or in lakes
and estuaries, but they are also formed on the land in lodgment basins,
in low-gradient valleys, and on base-plains. The deposits of sediment
on land have received less recognition than they deserve. When formed
under the sea or in other life-sustaining waters, shells and other
organic material are liable to be entrapped and to form a part of the
rock. These organic remains, or fossils, greatly aid in interpreting
the deposits in which they occur. Fossils are less liable to be
preserved in sedimentary deposits formed on land. There is, therefore,
some ground to suspect that great series of sandstones and shales which
do not contain marine or fresh-water fossils were formed in lodgment
basins on land, though the absence of fossils cannot be regarded as
proof of such origin.
[Illustration: +Fig.+ 351.—Globigerina ooze. Magnified 20 times.
(Murray and Renard.)]
[Illustration: +Fig.+ 352.—Pteropod ooze. Magnified 4 times. (Murray
and Renard.)]
=Limestones and dolomites.=—Of the lime, magnesia, soda, and potash
leached out of the surface-rocks and carried to the ocean in solution,
the lime is largely extracted to form the shells, skeletons, teeth,
armor, and other hard parts of sea-animals and sea-plants. These limy
parts are at length left on the floor of the ocean and become more or
less disintegrated and help to form beds of lime-mud and lime-sand
which in time are cemented into _limestone_ (Figs. 349, 350, 351, and
352). A larger proportion of the magnesia remains in solution in the
sea-water, but in ways not yet well understood, the magnesia sometimes
unites with the lime to form _dolomite_, a double carbonate of lime
and magnesia (Ca,Mg)CO₃. This change is sometimes local, and sometimes
affects great series of beds, more commonly the ancient ones than the
modern. Sometimes the dolomization appears to have taken place long
after the original limestone was formed and probably sometimes after
it was lifted out of the sea, while in other cases it seems to have
taken place while the sediment was accumulating, or at least before the
next overlying beds were laid down. The potash in solution is to some
large extent taken up by the land- and sea-plants or is retained in the
clays, and through them becomes again incorporated in the sediments.
The soda largely remains in solution in the sea-water.
=Precipitates.=—When a portion of the ocean-water is isolated in a
region where evaporation from the surface of the water is greater than
the rainfall on it, and the inflow from the tributary basin, the lime,
magnesia, soda, potash, and other dissolved substances (solutes) are
concentrated until the water becomes saturated. The solutes are then
precipitated in the order in which they reach the point of saturation.
This order, when taken in strict and full detail, gives a very complex
series, but the leading deposits are calcium carbonate (_limestone_),
calcium sulphate (_gypsum_), and sodium chloride (_halite_ or _rock
salt_) (see p. 375). Isolated lakes in arid regions may give rise
to similar deposits. It has sometimes been thought that the ancient
limestones were produced largely by precipitation from concentrated
sea-water. While this is probably the case in some instances and to
some degree, it has not been demonstrated that the great limestone
formations were made to any large extent in this way. The more accepted
view is that the limestones in the main were made from organic remains.
The lime in solution in the ocean is chiefly in the form of the
sulphate.
[Illustration: +Fig.+ 353.—Diatom ooze. Magnified 150 times. (Murray.)]
=Iron Ore-beds.=—In a somewhat different way iron ore-deposits are
formed by the precipitation of iron oxide or iron carbonate from
solutions of ferrous compounds. The ferrous compounds in solution
were leached from iron-bearing rocks by percolating waters. The most
familiar case is that of iron-bearing springs. On exposure to the air,
the iron compounds in solution undergo change, and ferric oxide is
thrown down, usually forming _limonite_ (Fe₂O₃,3H₂O), but sometimes
_hematite_ (Fe₂O₃). This change is common in marshes and gives origin
to “bog-ore.” Similar deposits take place in certain shallow lakes, and
hence are known as “lake ore.” Iron ore sometimes also forms at the
bottom of a peaty bed or in muddy soil. In connection with the great
coal formations, beds of iron carbonate (_siderite_) occur. Organic
matter seems to play a great part both in the original solution and
the later deposition of these ores. From certain soils and clay-beds
on which the ancient coal-producing forests grew, the iron has been
almost completely removed, either by the action of the roots, or
more probably by organic acids arising from their decay and from the
decaying vegetation on the surface. On flowing into shallow bodies
of water or into marshes, the waters containing such dissolved iron
compounds usually throw down their iron content either as a carbonate
(siderite), or as a hydrous ferric oxide (limonite). The siderite is
formed where decaying vegetation is present to furnish abundant carbon
dioxide and to partially protect the iron solution from oxidation, and
the limonite where free oxidation takes place. Sand, silt, clay, or
calcium carbonate often accumulates with the iron precipitate, and the
result is an impure deposit which becomes an _ironstone_. Such deposits
often become segregated into nodules, as will be explained later. It
is thought that diatoms sometimes aid in the deposit of iron ore in
shallow waters.
=Silicious deposits.=—In the decomposition of igneous rocks, a certain
portion of the silica, as well as of the bases, is dissolved and
carried away in solution. Certain organisms extract this from solution
for their skeletons, just as others extract calcium carbonate. The
accumulation of these silicious skeletons often forms silicious
rocks. The _diatom_, _radiolarian_, and other oozes (Fig. 353) of
the deep sea are the great examples. Sometimes layers of infusorial
earth, _tripolite_, arise from the shells of diatoms and other aquatic
organisms secreting silica. The waters in which such earths accumulate
are rather shallow, and either fresh or salt. The most familiar
examples of indurated rocks formed in this general method are the
_flints_ and _cherts_ (impure flints) that occur in limestone and
chalk, chiefly as nodules, but sometimes in distinct beds.