119
the subsequent upheaval, _the element of great depth of
accumulation seems a necessary condition and must evidently enter
as a factor into the Physical Processes involved_. The mountain
range can only arise where the geosyncline is deeply filled by
long ages of sedimentation.
Dana's description of the events attending mountain building is
impressive:
"A mountain range of the common type, like that to which the
Appalachians belong, is made out of the sedimentary formations of
a long preceding era; beds that were laid down conformably, and
in succession, until they had reached the needed thickness; beds
spreading over a region tens of thousands of square miles in
area. The region over which sedimentary formations were in
progress in order to make, finally, the Appalachian range,
reached from New York to Alabama, and had a breadth of 100 to 200
miles, and the pile of horizontal beds along the middle was
40,000 feet in depth. The pile for the Wahsatch Mountains was
60,000 feet thick, according to King. The beds for the
Appalachians were not laid down in a deep ocean, but in shallow
waters, where a gradual subsidence was in progress; and they at
last, when ready for the genesis, lay in a trough 40,000 feet
deep, filling the trough to the brim. It thus appears that epochs
of mountain-making have occurred only after long intervals of
quiet in the history of a continent."[1]
[1] Dana, _Manual of Geology_, third edition, p. 794
120
On the western side of North America the work of
mountain-building was, indeed, on the grandest scale. For long
ages and through a succession of geological epochs, sedimentation
had proceeded so that the accumulations of Palaeozoic and
Mesozoic times had collected in the geosyncline formed by their
own ever increasing weight. The site of the future Laramide range
was in late Cretaceous times occupied by some 50,000 feet of
sedimentary deposits; but the limit had apparently been attained,
and at this time the Laramide range, as well as its southerly
continuation into the United States, the Rockies, had their
beginning. Chamberlin and Salisbury[1] estimate that the height
of the mountains developed in the Laramide range at this time was
20,000 feet, and that, owing to the further elevation which has
since taken place, from 32,000 to 35,000 feet would be their
present height if erosion had not reduced them. Thus on either
side of the American continent we have the same forces at work,
throwing up mountain ridges where the sediments had formerly been
shed into the ocean.
These great events are of a rhythmic character; the crust, as it
were, pulsating under the combined influences of sedimentation
and denudation. The first involves downward movements under a
gathering load, and ultimately a reversal of the movement to one
of upheaval; the second factor, which throughout has been in
[1] Chamberlin and Salisbury, _Geology_, 1906, iii., 163.
121
operation as creator of the sediments, then intervenes as an
assailant of the newly-raised mountains, transporting their
materials again to the ocean, when the rhythmic action is
restored to its first phase, and the age-long sequence of events
must begin all over again.
It has long been inferred that compressive stress in the crust
must be a primary condition of these movements. The wvork
required to effect the upheavals must be derived from some
preexisting source of energy. The phenomenon--intrinsically one of
folding of the crust--suggests the adjustment of the earth-crust
to a lessening radius; the fact that great mountain-building
movements have simultaneously affected the entire earth is
certainly in favour of the view that a generally prevailing cause
is at the basis of the phenomenon.
The compressive stresses must be confined to the upper few miles
of the crust, for, in fact, the downward increase of temperature
and pressure soon confers fluid properties on the medium, and
slow tangential compression results in hydrostatic pressure
rather than directed stresses. Thus the folding visible in the
mountain range, and the lateral compression arising therefrom,
are effects confined to the upper parts of the crust.
The energy which uplifts the mountain is probably a surviving
part of the original gravitational potential energy of the crust
itself. It must be assumed that the crust in following downwards
the shrinking subcrustal magma, develops immense compressive
stresses in
122
its materials, vast geographical areas being involved. When
folding at length takes place along the axis of the elongated
syncline of deposition, the stresses find relief probably for
some hundreds of miles, and the region of folding now becomes
compressed in a transverse direction. As an illustration, the
Laramide range, according to Dawson, represents the reduction of
a surface-belt 50 miles wide to one of 25 miles. The marvellous
translatory movements of crustal folds from south to north
arising in the genesis of the Swiss Alps, which recent research
has brought to light, is another example of these movements of
relief, which continue to take place perhaps for many millions of
years after they are initiated.
The result of this yielding of the crust is a buckling of the
surface which on the whole is directed upwards; but depression
also is an attendant, in many cases at least, on mountain
upheaval. Thus we find that the ocean floor is depressed into a
syncline along the western coast of South America; a trough
always parallel to the ranges of the Andes. The downward
deflection of the crust is of course an outcome of the same
compressive stresses which elevate the mountain.
The fact that the yielding of the crust is always situated where
the sediments have accumulated to the greatest depth, has led to
attempts from time to time of establishing a physical connexion
between the one and the other. The best-known of these theories
is that of Babbage and Herschel. This seeks the connexion in the
rise of the
123
geotherms into the sinking mass of sediment and the consequent
increase of temperature of the earth-crust beneath. It will be
understood that as these isogeotherms, or levels at which the
temperature is the same, lie at a uniform distance from the
surface all over the Earth, unless where special variations of
conductivity may disturb them, the introduction of material
pressed downwards from above must result in these materials
partaking of the temperature proper to the depth to which they
are depressed. In other words the geotherms rise into the sinking
sediments, always, however, preserving their former average
distance from the surface. The argument is that as this process
undoubtedly involves the heating up of that portion of the crust
which the sediments have displaced downwards, the result must be
a local enfeeblement of the crust, and hence these areas become
those of least resistance to the stresses in the crust.
When this theory is examined closely, we see that it only amounts
to saying that the bedded rocks, which have taken the place of
the igneous materials beneath, as a part of the rigid crust of
the Earth, must be less able to withstand compressive stress than
the average crust. For there has been no absolute rise of the
geotherms, the thermal conductivities of both classes of
materials differing but little. Sedimentary rock has merely taken
the place of average crust-rock, and is subjected to the same
average temperature and pressure prevailing in the surrounding
crust. But are there any grounds for the
124
assumption that the compressive resistance of a complex of
sedimentary rocks is inferior to one of igneous materials? The
metamorphosed siliceous sediments are among the strongest rocks
known as regards resistance to compressive stress; and if
limestones have indeed plastic qualities, it must be remembered
that their average amount is only some 5 per cent. of the whole.
Again, so far as rise of temperature in the upper crust may
affect the question, a temperature which will soften an average
igneous rock will not soften a sedimentary rock, for the reason
that the effect of solvent denudation has been to remove those
alkaline silicates which confer fusibility.
When, however, we take into account the radioactive content of
the sediments the matter assumes a different aspect.
The facts as to the general distribution of radioactive
substances at the surface, and in rocks which have come from
considerable depths in the crust, lead us to regard as certain
the widespread existence of heat-producing radioactive elements
in the exterior crust of the Earth. We find, indeed, in this fact
an explanation--at least in part--of the outflow of heat
continually taking place at the surface as revealed by the rising
temperature inwards. And we conclude that there must be a
thickness of crust amounting to some miles, containing the
radioactive elements.
Some of the most recent measurements of the quantities of radium
and thorium in the rocks of igneous origin--_e.g._ granites,
syenites, diorites, basalts, etc., show that the
125
radioactive heat continually given out by such rocks amounts to
about one millionth part of 0.6 calories per second per cubic
metre of average igneous rock. As we have to account for the
escape of about 0.0014 calorie[1] per square metre of the Earth's
surface per second (assuming the rise of temperature downwards,
_i.e._ the "gradient" of temperature, to be one degree centigrade
in 35 metres) the downward extension of such rocks might, _prima
facie_, be as much as 19 kilometres.
About this calculation we have to observe that we assume the
average radioactivity of the materials with which we have dealt
at the surface to extend uniformly all the way down, _i.e._ that
our experiments reveal the average radioactivity of a radioactive
crust. There is much to be said for this assumption. The rocks
which enter into the measurements come from all depths of the
crust. It is highly probable that the less silicious, _i.e._ the
more basic, rocks, mainly come from considerable depths; the more
acid or silica-rich rocks, from higher levels in the crust. The
radioactivity determined as the mean of the values for these two
classes of rock closely agrees with that found for intermediate
rocks, or rocks containing an intermediate amount of silica.
Clarke contends that this last class of material probably
represents the average composition of the Earth's crust so far as
it has been explored by us.
[1] The calorie referred to is the quantity of heat required to
heat one gram of water, _i.e._ one cubic centimetre of
water--through one degree centigrade.
126
It is therefore highly probable that the value found for the mean
radioactivity of acid and basic rocks, or that found for
intermediate rocks, truly represents the radioactive state of the
crust to a considerable depth. But it is easy to show that we
cannot with confidence speak of the thickness of this crust as
determinable by equating the heat outflow at the surface with the
heat production of this average rock.
This appears in the failure of a radioactive layer, taken at a
thickness of about 19-kilometres, to account for the deep-seated
high temperatures which we find to be indicated by volcanic
phenomena at many places on the surface. It is not hard to show
that the 19-kilometre layer would account for a temperature no
higher than about 270° >C. at its base.
It is true that this will be augmented beneath the sedimentary
deposits as we shall presently see; and that it is just in
association with these deposits that deep-seated temperatures are
most in evidence at the surface; but still the result that the
maximum temperature beneath the crust in general attains a value
no higher than 270° C. is hardly tenable. We conclude, then, that
some other source of heat exists beneath. This may be radioactive
in origin and may be easily accounted for if the radioactive
materials are more sparsely distributed at the base of the upper
crust. Or, again, the heat may be primeval or original heat,
still escaping from a cooling world. For our present purpose it
does not much matter which view
127
we adopt. But we must recognise that the calculated depth of 19
kilometres of crust, possessing the average radioactivity of the
surface, is excessive; for, in fact, we are compelled by the
facts to recognise that some other source of heat exists
beneath.
If the observed surface gradient of temperature persisted
uniformly downwards, at some 35 kilometres beneath the surface
there would exist temperatures (of about 1000° C.) adequate to
soften basic rocks. It is probable, however, that the gradient
diminishes downwards, and that the level at which such
temperatures exist lies rather deeper than this. It is,
doubtless, somewhat variable according to local conditions; nor
can we at all approximate closely to an estimate of the depth at
which the fusion temperatures will be reached, for, in fact, the
existence of the radioactive layer very much complicates our
estimates. In what follows we assume the depth of softening to
lie at about 40 kilometres beneath the surface of the normal
crust; that is 25 miles down. It is to be observed that Prestwich
and other eminent geologists, from a study of the facts of
crust-folding, etc., have arrived at similar estimates.[1] As a
further assumption we are probably not far wrong if we assign to
the radioactive part of this crust a thickness of about 10 or 12
kilometres; _i.e._ six or seven miles. This is necessarily a
rough approximation only; but the conclusions at which
[1] Prestwich, _Proc. Royal Soc._, xii., p. 158 _et seq._
128
we shall arrive are reached in their essential features allowing
a wide latitude in our choice of data. We shall speak of this
part of the crust as the normal radioactive layer.
An important fact is evolved from the mathematical investigation
of the temperature conditions arising from the presence of such a
radioactive layer. It is found that the greatest temperature, due
to the radioactive heat everywhere evolved in the layer--_i.e._
the temperature at its base--is proportional to the square of the
thickness of the layer. This fact has a direct bearing on the
influence of radioactivity upon mountain elevation; as we shall
now find.
The normal radioactive layer of the Earth is composed of rocks
extending--as we assume--approximately to a depth of 12 kilometres
(7.5 miles). The temperature at the base of this layer due to the
heat being continually evolved in it, is, say, t1°. Now, let us
suppose, in the trough of the geosyncline, and upon the top of
the normal layer, a deposit of, say, 10 kilometres (6.2 miles) of
sediments is formed during a long period of continental
denudation. What is the effect of this on the temperature at the
base of the normal layer depressed beneath this load? The total
thickness of radioactive rocks is now 22 kilometres. Accordingly
we find the new temperature t2°, by the proportion t1° : t2° ::
12° : 22° That is, as 144 to 484. In fact, the temperature is more
than trebled. It is true we here assume the radioactivity of the
sediments
129
and of the normal crust to be the same. The sediments are,
however, less radioactive in the proportion of 4 to 3.
Nevertheless the effects of the increased thickness will be
considerable.
Now this remarkable increase in the temperature arises entirely
from the condition attending the radioactive heating; and
involves something _additional_ to the temperature conditions
determined by the mere depression and thickening of the crust as
in the Babbage-Herschel theory. The latter theory only involves a
_shifting_ of the temperature levels (or geotherms) into the
deposited materials. The radioactive theory involves an actual
rise in the temperature at any distance from the surface; so that
_the level in the crust at which the rocks are softened is nearer
to the surface in the geosynclines than it is elsewhere in the
normal crust_ (Pl. XV, p. 118).
In this manner the rigid part of the crust is reduced in
thickness where the great sedimentary deposits have collected. A
ten-kilometre layer of sediment might result in reducing the
effective thickness of the crust by 30 per cent.; a
fourteen-kilometre layer might reduce it by nearly 50 per cent.
Even a four-kilometre deposit might reduce the effective
resistance of the crust to compressive forces, by 10 per cent.
Such results are, of course, approximate only. They show that as
the sediments grow in depth there is a rising of the geotherm of
plasticity--whatever its true temperature may be--gradually
reducing the thickness of that part
130
of the upper crust which is bearing the simultaneously increasing
compressive stresses. Below this geotherm long-continued stress
resolves itself into hydrostatic pressure; above it (there is, of
course, no sharp line of demarcation) the crust accumulates
elastic energy. The final yielding and flexure occur when the
resistant cross-section has been sufficiently diminished. It is
probable that there is also some outward hydrostaitic thrust over
the area of rising temperature, which assists in determining the
upward throw of the folds.
When yielding has begun in any geosyncline, and the materials are
faulted and overthrust, there results a considerably increased
thickness. As an instance, consider the piling up of sediments
over the existing materials of the Alps, which resulted from the
compressive force acting from south to north in the progress of
Alpine upheaval. Schmidt of Basel has estimated that from 15 to
20 kilometres of rock covered the materials of the Simplon as now
exposed, at the time when the orogenic forces were actively at
work folding and shearing the beds, and injecting into their
folds the plastic gneisses coming from beneath.[1] The lateral
compression of the area of deposition of the Laramide, already
referred to, resulted in a great thickening of the deposits. Many
other cases might be cited; the effect is always in some degree
necessarily produced.
[1] Schmidt, Ec. Geol. _Helvelix_, vol. ix., No. 4, p. 590
131
If time be given for the heat to accumulate in the lower depths
of the crushed-up sediments, here is an additional source of
increased temperature. The piled-up masses of the Simplon might
have occasioned a rise due to radioactive heating of one or two
hundred degrees, or even more; and if this be added to the
interior heat, a total of from 800° to 1000° might have prevailed
in the rocks now exposed at the surface of the mountain. Even a
lesser temperature, accompanied by the intense pressure
conditions, might well occasion the appearances of thermal
metamorphism described by Weinschenk, and for which, otherwise,
there is difficulty in accounting.[1]
This increase upon the primarily developed temperature conditions
takes place concurrently with the progress of compression; and
while it cannot be taken into account in estimating the
conditions of initial yielding of the crust, it adds an element
of instability, inasmuch as any progressive thickening by lateral
compression results in an accelerated rise of the goetherms. It
is probable that time sufficient for these effects to develop, if
not to their final, yet to a considerable extent, is often
available. The viscous movements of siliceous materials, and the
out-pouring of igneous rocks which often attend mountain
elevation, would find an explanation in such temperatures.
[1] Weinschenk, _Congrès Géol. Internat._, 1900, i., p. 332.
132
There is no more striking feature of the part here played by
radioactivity than the fact that the rhythmic occurrence of
depression and upheaval succeeding each other after great
intervals of time, and often shifting their position but little
from the first scene of sedimentation, becomes accounted for. The
source of thermal energy, as we have already remarked, is in fact
transported with the sediments--that energy which determines the
place of yielding and upheaval, and ordains that the mountain
ranges shall stand around the continental borders. Sedimentation
from this point of view is a convection of energy.
When the consolidated sediments are by these and by succeeding
movements forced upwards into mountains, they are exposed to
denudative effects greatly exceeding those which affect the
plains. Witness the removal during late Tertiary times of the
vast thickness of rock enveloping the Alps. Such great masses are
hurried away by ice, rivers, and rain. The ocean receives them;
and with infinite patience the world awaits the slow accumulation
of the radioactive energy beginning afresh upon its work. The
time for such events appears to us immense, for millions of years
are required for the sediments to grow in thickness, and the
geotherms to move upwards; but vast as it is, it is but a moment
in the life of the parent radioactive substances, whose atoms,
hardly diminished in numbers, pursue their changes while the
mountains come and go, and the
133
rudiments of life develop into its highest consummations.
To those unacquainted with the results of geological
investigation the history of the mountains as deciphered in the
rocks seems almost incredible.
The recently published sections of the Himalaya, due to H. H.
Hayden and the many distinguished men who have contributed to the
Geological Survey of India, show these great ranges to be
essentially formed of folded sediments penetrated by vast masses
of granite and other eruptives. Their geological history may be
summarised as follows
The Himalayan area in pre-Cambrian times was, in its southwestern
extension, part of the floor of a sea which covered much of what
is now the Indian Peninsula. In the northern shallows of this sea
were laid down beds of conglomerate, shale, sandstone and
limestone, derived from the denudation of Archæan rocks, which,
probably, rose as hills or mountains in parts of Peninsular India
and along the Tibetan edge of the Himalayan region. These beds
constitute the record of the long Purana Era[1] and are probably
coeval with the Algonkian of North America. Even in these early
times volcanic disturbances affected this area and the lower beds
of the Purana deposits were penetrated by volcanic outflows,
covered by sheets of lava, uplifted, denuded and again submerged
[1] See footnote, p. 139.
134
beneath the waters. Two such periods of instability have left
their records in the sediments of the Purana sea.
The succeeding era--the Dravidian Era--opens with Haimanta
(Cambrian) times. A shallow sea now extended over Kumaun, Garwal,
and Spiti, as well as Kashmir and ultimately over the Salt Range
region of the Punjab as is shown by deposits in these areas. This
sea was not, however, connected with the Cambrian sea of Europe.
The fossil faunas left by the two seas are distinct.
After an interval of disturbance during closing Haimanta times,
geographical changes attendant on further land movements
occurred. The central sea of Asia, the Tethys, extended westwards
and now joined with the European Paleozoic sea; and deposits of
Ordovician and Silurian age were laid down:--the Muth deposits.
The succeeding Devonian Period saw the whole Northern Himalayan
area under the waters of the Tethys which, eastward, extended to
Burma and China and, westward, covered Kashmir, the Hindu Kush
and part of Afghanistan. Deposits continued to be formed in this
area till middle Carboniferous times.
Near. the close of the Dravidian Era Kashmir became convulsed by
volcanic disturbance and the Penjal traps were ejected. It was a
time of worldwide disturbance and of redistribution of land and
water. Carboniferous times had begun, and the geographical
changes in
135
the southern limits of the Tethys are regarded as ushering in a
new and last era in Indian geological history the Aryan Bra.
India was now part of Gondwanaland; that vanished continent which
then reached westward to South Africa and eastward to Australia.
A boulder-bed of glacial origin, the Talchir Boulder-bed, occurs
in many surviving parts of this great land. It enters largely
into the Salt Range deposits. There is evidence that extensive
sheets of ice, wearing down the rocks of Rajputana, shoved their
moraines northward into the Salt Range Sea; then, probably, a
southern extension of the Tethys.
Subsequent to this ice age the Indian coalfields of the Gondwana
were laid down, with beds rich in the Glossopteris and
Gangamopteris flora. This remarkable carboniferous flora extends
to Southern Kashmir, so that it is to be inferred that this
region was also part of the main Gondwanaland. But its emergence
was but for a brief period. Upper Carboniferous marine deposits
succeeded; and, in fact, there was no important discontinuity in
the deposits in this area from Panjal times till the early
Tertiaries. During the whole of which vast period Kashmir was
covered with the waters of the Tethys.
The closing Dravidian disturbances of the Kashmir region did not,
apparently, extend to the eastern Himalayan area. But the
Carboniferous Period was, in this
136
eastern area, one of instability, culminating, at the close of
the Period, in a steady rise of the land and a northward retreat
of the Tethys. Nearly the entire Himalaya east of Kashmir became
a land surface and remained exposed to denudative forces for so
long a time that in places the whole of the Carboniferous,
Devonian, and a large part of the Silurian and Ordovician
deposits were removed--some thousands of feet in thickness--before
resubmergence in the Tethys occurred.
Towards the end of the Palaeozoic Age the Aryan Tethys receded
westwards, but still covered the Himalaya and was still connected
with the European Palæozoic sea. The Himalayan area (as well as
Kashmir) remained submerged in its waters throughout the entire
Mesozoic Age.
During Cretaceous times the Tethys became greatly extended,
indicating a considerable subsidence of northwestern India,
Afghanistan, Western Asia, and, probably, much of Tibet. The
shallow-water character of the deposits of the Tibetan Himalaya
indicates, however, a coast line near this region. Volcanic
materials, now poured out, foreshadow the incoming of the great
mountain-building epoch of the Tertiary Era. The enormous mass of
the Deccan traps, possessing a volume which has been estimated at
as much as 6,000 cubic miles, was probably extruded over the
Northern Peninsular region during late Cretaceous times. The sea
now began to retreat, and by the close of
137
the Eocene, it had moved westward to Sind and Baluchistan. The
movements of the Earth's crust were attended by intense volcanic
activity, and great volumes of granite were injected into the
sediments, followed by dykes and outflows of basic lavas.
The Tethys vanished to return no more. It survives in the
Mediterranean of today. The mountain-building movements continued
into Pliocene times. The Nummulite beds of the Eocene were, as
the result, ultimately uplifted 18,500 feet over sea level, a
total uplift of not less than 20,000 feet.
Thus with many vicissitudes, involving intervals of volcanic
activity, local uplifting, and extensive local denudation, the
Himalaya, which had originated in the sediments of the ancient
Purana sea, far back in pre-Cambrian times, and which had
developed potentially in a long sequence of deposits collecting
almost continuously throughout the whole of geological time,
finally took their place high in the heavens, where only the
winds--faint at such altitudes--and the lights of heaven can visit
their eternal snows.[1]
In this great history it is significant that the longest
continuous series of sedimentary deposits which the world has
known has become transfigured into the loftiest elevation upon
its surface.
[1] See A Sketch of the _Geography and Geology of the Himalaya
Mountains and Tibet_. By Colonel S. G. Burrard, R.E., F.R.S., and
H. H. Hayden, F.G.S., Part IV. Calcutta, 1908.
138
The diagrammatic sections of the Himalaya accompanying this brief
description arc taken from the monograph of Burrard and Hayden
(loc. cit.) on the Himalaya. Looking at the sections we see that
some of the loftiest summits are sculptured in granite and other
crystalline rocks. The appearance of these materials at the
surface indicates the removal by denudation and the extreme
metamorphism of much sedimentary deposit. The crystalline rocks,
indeed, penetrate some of the oldest rocks in the world. They
appear in contact with Archaean, Algonkian or early Palaeozoic
rocks. A study of the sections reveals not only the severe earth
movements, but also the immense amount of sedimentary deposits
involved in the genesis of these alps. It will be noted that the
vertical scale is not exaggerated relatively to the
horizontal.[1] Although there is no evidence of mountain
building
[1] To those unacquainted with the terminology of Indian geology
the following list of approximate equivalents in time will be of
use
Ngari Khorsum Beds - Pleistocene.
Siwalik Series - Miocene and Pliocene.
Sirmur Series - Oligocene.
Kampa System - Eocene and Cretaceous.
Lilang System - Triassic.
Kuling System - Permian.
Gondwana System - Carboniferous.
Kenawar System - Carboniferous and Devonian
Muth System - Silurian.
Haimanta System - Mid. and Lower Cambrian.
Purana Group - Algonkian.
Vaikrita System - Archæan.
Daling Series - Archæan.
139
on a large scale in the Himalayan area till the Tertiary
upheaval, it is, in the majority of cases, literally correct to
speak of the mountains as having their generations like organic
beings, and passing through all the stages of birth, life, death
and reproduction. The Alps, the Jura, the Pyrenees, the Andes,
have been remade more than once in the course of geological time,
the _débris_ of a worn-out range being again uplifted in succeeding
ages.
Thus to dwell for a moment on one case only: that of the
Pyrenees. The Pyrenees arose as a range of older Palmozoic rocks
in Devonian times. These early mountains, however, were
sufficiently worn out and depressed by Carboniferous times to
receive the deposits of that age laid down on the up-turned edges
of the older rocks. And to Carboniferous succeeded Permian,
Triassic, Jurassic and Lower Cretaceous sediments all laid down
in conformable sequence. There was then fresh disturbance and
upheaval followed by denudation, and these mountains, in turn,
became worn out and depressed beneath the ocean so that Upper
Greensand rocks were laid down unconforrnably on all beneath. To
these now succeeded Upper Chalk, sediments of Danian age, and so
on, till Eocene times, when the tale was completed and the
existing ranges rose from the sea. Today we find the folded
Nummulitic strata of Eocene age uplifted 11,000 feet, or within
200 feet of the greatest heights of the Pyrenees. And so they
stand awaiting
140
the time when once again they shall "fall into the portion of
outworn faces."[1]
Only mountains can beget mountains. Great accumulations of
sediment are a necessary condition for the localisation of
crust-flexure. The earliest mountains arose as purely igneous or
volcanic elevations, but the generations of the hills soon
originated in the collection of the _débris_, under the law of
gravity, in the hollow places. And if a foundered range is
exposed now to our view encumbered with thousands of feet of
overlying sediments we know that while the one range was sinking,
another, from which the sediments were derived, surely existed.
Through the "windows" in the deep-cut rocks of the Swiss valleys
we see the older Carboniferous Alps looking out, revisiting the
sun light, after scores of millions of years of imprisonment. We
know that just as surely as the Alps of today are founding by
their muddy torrents ranges yet to arise, so other primeval Alps
fed into the ocean the materials of these buried pre-Permian
rocks.
This succession of events only can cease when the rocks have been
sufficiently impoverished of the heat-producing substances, or
the forces of compression shall have died out in the surface
crust of the earth.
It seems impossible to escape the conclusion that in the great
development of ocean-encircling areas of
[1] See Prestwich, _Chemical and Physical Geology_, p. 302.
141
deposition and crustal folding, the heat of radioactivity has
been a determining factor. We recognise in the movements of the
sediments not only an influence localising and accelerating
crustal movements, but one which, in subservience to the primal
distribution of land and water, has determined some of the
greatest geographical features of the globe.
It is no more than a step to show that bound up with the
radioactive energy are most of the earthquake and volcanic
phenomena of the earth. The association of earthquakes with the
great geosynclines is well known. The work of De Montessus showed
that over 94 per cent. of all recorded shocks lie in the
geosynclinal belts. There can be no doubt that these
manifestations of instability are the results of the local
weakness and flexure which originated in the accumulation of
energy denuded from the continents. Similarly we may view in
volcanoes phenomena referable to the same fundamental cause. The
volcano was, in fact, long regarded as more intimately connected
with earthquakes than it, probably, actually is; the association
being regarded in a causative light, whereas the connexion is
more that of possessing a common origin. The girdle of volcanoes
around the Pacific and the earthquake belt coincide. Again, the
ancient and modern volcanoes and earthquakes of Europe are
associated with the geosyncline of the greater Mediterranean, the
Tethys of Mesozoic times. There is no difficulty in understanding
in a
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general way the nature of the association. The earthquake is the
manifestation of rupture and slip, and, as Suess has shown, the
epicentres shift along that fault line where the crust has
yielded.[1] The volcano marks the spot where the zone of fusion
is brought so high in the fractured crust that the melted
materials are poured out upon the surface.
In a recent work on the subject of earthquakes Professor Hobbs
writes: "One of the most interesting of the generalisations which
De Montessus has reached as a result of his protracted studies,
is that the earthquake districts on the land correspond almost
exactly to those belts upon the globe which were the almost
continuous ocean basins of the long Secondary era of geological
history. Within these belts the sedimentary formations of the
crust were laid down in the greatest thickness, and the
formations follow each other in relatively complete succession.
For almost or quite the whole of this long era it is therefore
clear that the ocean covered these zones. About them the
formations are found interrupted, and the lacuna indicate that
the sea invaded the area only to recede from it, and again at
some later period to transgress upon it. For a long time,
therefore, these earthquake belts were the sea basins--the
geosynclines. They became later the rising mountains of the
Tertiary period, and mountains they
[1] Suess, _The Face of the Earth_, vol. ii., chap. ii.
143
are today. The earthquake belts are hence those portions of the
earth's crust which in recent times have suffered the greatest
movements in a vertical direction--they are the most mobile
portions of the earth's crust."[1] Whether the movements
attending mountain elevation and denudation are a connected and
integral part of those wide geographical changes which result in
submergence and elevation of large continental areas, is an
obscure and complex question. We seem, indeed, according to the
views of some authorities, hardly in a position to affirm with
certainty that such widespread movements of the land have
actually occurred, and that the phenomena are not the outcome of
fluctuations of oceanic level; that our observations go no
further than the recognition of positive and negative movements
of the strand. However this may be, the greater part of
mechanical denudation during geological time has been done on the
mountain ranges. It is, in short, indisputable that the orogenic
movements which uplift the hills have been at the basis of
geological history. To them the great accumulations of sediments
which now form so large a part of continental land are mainly
due. There can be no doubt of the fact that these movements have
swayed the entire history, both inorganic and organic, of the
world in which we live.
[1] Hobbs, _Earthquakes_, p. 58.
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To sum the contents of this essay in the most general terms, we
find that in the conception of denudation as producing the
convection and accumulation of radiothermal energy the surface
features of the globe receive a new significance. The heat of the
earth is not internal only, but rather a heat-source exists at
the surface, which, as we have seen, cannot prevail to the same
degree within; and when the conditions become favourable for the
aggregation of the energy, the crust, heated both from beneath
and from above, assumes properties more akin to those of its
earlier stages of development, the secular heat-loss being
restored in the radioactive supplies. These causes of local
mobility have been in operation, shifting somewhat from place to
place, and defined geographically by the continental masses
undergoing denudation, since the earliest times.
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