ALPINE STRUCTURE

AN intelligent observer of the geological changes progressing in

southern Europe in Eocene times would have seen little to inspire

him with a premonition of the events then developing. The

Nummulitic limestones were being laid down in that enlarged

Mediterranean which at this period, save for a few islands,

covered most of south Europe. Of these stratified remains, as

well as of the great beds of Cretaceous, Jurassic, Triassic, and

Permian sediments beneath, our hypothetical observer would

probably have been regardless; just as today we observe, with an

indifference born of our transitoriness, the deposits rapidly

gathering wherever river discharge is distributing the sediments

over the sea-floor, or the lime-secreting organisms are actively

at work. And yet it took but a few millions of years to uplift

the deposits of the ancient Tethys; pile high its sediments in

fold upon fold in the Alps, the Carpathians, and the Himalayas;

and--exposing them to the rigours of denudation at altitudes where

glaciation, landslip, and torrent prevail--inaugurate a new epoch

of sedimentation and upheaval.

146

In the case of the Alps, to which we wish now specially to refer,

the chief upheaval appears to have been in Oligocene times,

although movement continued to the close of the Pliocene. There

was thus a period of some millions of years within which the

entire phenomena were comprised. Availing ourselves of Sollas'

computations,[1] we may sum the maximum depths of sedimentary

deposits of the geological periods concerned as follows:--

Pliocene - - - - - 3,950 m.

Miocene - - - - - 4,250 m.

Oligocene - - - - 3,660 m.

Eocene - - - - - - 6,100 m.

and assuming that the orogenic forces began their work in the

last quarter of the Eocene period, we have a total of 13,400 m.

as some measure of the time which elapsed. At the rate of io

centimetres in a century these deposits could not have collected

in less than 13.4 millions of years. It would appear that not

less than some ten millions of years were consumed in the genesis

of the Alps before constructive movements finally ceased.

The progress of the earth-movements was attended by the usual

volcanic phenomena. The Oligocene and Miocene volcanoes extended

in a band marked by the Auvergne, the Eiffel, the Bohemian, and

the eastern Carpathian eruptions; and, later, towards the close

of the movements in Pliocene times, the south border

[1] Sollas, Anniversary Address, Geol. Soc., London, 1909.

147

regions of the Alps became the scene of eruptions such as those

of Etna, Santorin, Somma (Vesuvius), etc.

We have referred to these well-known episodes with two objects in

view: to recall to mind the time-interval involved, and the

evidence of intense crustal disturbance, both dynamic and

thermal. According to views explained in a previous essay, the

energetic effects of radium in the sediments and upper crust were

a principal factor in localising and bringing about these

results. We propose now to inquire if, also, in the more intimate

structure of the Alps, the radioactive energy may not have borne

a part.

What we see today in the Alps is but a residue spared by

denudation. It is certain that vast thicknesses of material have

disappeared. Even while constructive effects were still in

progress, denudative forces were not idle. Of this fact the

shingle accumulations of the Molasse, where, on the northern

borders of the Alps, they stand piled into mountains, bear

eloquent testimony. In the sub-Apennine series of Italy, the

great beds of clays, marls, and limestones afford evidence of

these destructive processes continued into Pliocene times. We

have already referred to Schmidt's estimate that the sedimentary

covering must have in places amounted to from 15,000 to 20,000

metres. The evidence for this is mainly tectonic or structural;

but is partly forthcoming in the changes which the materials now

open to our inspection plainly reveal. Thus it is impos-

148

sible to suppose that gneissic rocks can become so far plastic as

to flow in and around the calcareous sediments, or be penetrated

by the latter--as we see in the Jungfrau and elsewhere--unless

great pressures and high temperatures prevailed. And, according

to some writers, the temperatures revealed by the intimate

structural changes of rock-forming minerals must have amounted to

those of fusion. The existence of such conditions is supported by

the observation that where the.crystallisation is now the most

perfect, the phenomena of folding and injection are best

developed.[1] These high temperatures would appear to be

unaccountable without the intervention of radiothermal effects;

and, indeed, have been regarded as enigmatic by observers of the

phenomena in question. A covering of 20,000 metres in thickness

would not occasion an earth-temperature exceeding 500° C. if the

gradients were such as obtain in mountain regions generally; and

600° is about the limit we could ascribe to the purely passive

effects of such a layer in elevating the geotherms.

Those who are still unacquainted with the recently published

observations on the structure of the Alps may find it difficult

to enter into what has now to be stated; for the facts are,

indeed, very different from the generally preconceived ideas of

mountain formation. Nor can we wonder that many geologists for

long held

[1] Weinschenk, C. R. _Congrès Géol._, 1900, p. 321, et seq.

149

back from admitting views which appeared so extreme. Receptivity

is the first virtue of the scientific mind; but, with every

desire to lay aside prejudice, many felt unequal to the

acceptance of structural features involving a folding of the

earth-crust in laps which lay for scores of miles from country to

country, and the carriage of mountainous materials from the south

of the Alps to the north, leaving them finally as Alpine ranges

of ancient sediments reposing on foundations of more recent date.

The historian of the subject will have to relate how some who

finally were most active in advancing the new views were at first

opposed to them. In the change of conviction of these eminent

geologists we have the strongest proof of the convincing nature

of the observations and the reality of the tectonic features upon

which the recent views are founded.

The lesser mountains which stand along the northern border of the

great limestone Alps, those known as the Préalpes, present the

strange characteristic of resting upon materials younger than

themselves. Such mountains as the remarkable-looking Mythen, near

Schwyz, for instance, are weathered from masses of Triassic and

Jurassic rock, and repose on the much more recent Flysch. In

sharp contrast to the Flysch scenery, they stand as abrupt and

gigantic erratics, which have been transported from the central

zone of the Alps lying far to the south. They are strangers

petrologically,

150

stratigraphically, and geographically,[1] to the locality in

which they now occur. The exotic materials may be dolomites,

limestones, schists, sandstones, or rocks of igneous origin. They

show in every case traces of the severe dynamic actions to which

they have been subjected in transit. The igneous, like the

sedimentary, klippen, can be traced to distant sources; to the

massif of Belladonne, to Mont Blanc, Lugano, and the Tyrol. The

Préalpes are, in fact, mountains without local roots.

In this last-named essential feature, the Préalpes do not differ

from the still greater limestone Alps which succeed them to the

south. These giants, _e.g._ the Jungfrau, Wetterhorn, Eiger, etc.,

are also without local foundations. They have been formed from

the overthrown and drawn-out anticlines of great crust-folds,

whose synclines or roots are traceable to the south side of the

Rhone Valley. The Bernese Oberland originated in the piling-up of

four great sheets or recumbent folds, one of which is continued

into the Préalpes. With Lugeon[2] we may see in the phenomenon of

the formation of the Préalpes a detail; regarding it as a normal

expression of that mechanism which has created the Swiss Alps.

For these limestone masses of the Oberland are not indications of

a merely local shift of the sedimentary covering of the Alps.

Almost the whole covering has

[1] De Lapparent, _Traité de Géologie_, p. 1,785.

[2] Lugeon, _Bulletin Soc. Géol. de France_, 1901, p. 772.

151

been pushed over and piled up to the north. Lugeon[l] concludes

that, before denudation had done its work and cut off the

Préalpes from their roots, there would have been found sheets, to

the number of eight, superimposed and extending between the Mont

Blanc massif and the massif of the Finsteraarhorn: these sheets

being the overthrown folds of the wrinkled sedimentary covering.

The general nature of the alpine structure

{Fig. 8}

will be understood from the presentation of it diagrammatically

after Schmidt of Basel (Fig. 8).[2] The section extends from

north to south, and brings out the relations of the several

recumbent folds. We must imagine almost the whole of these

superimposed folds now removed from the central regions of the

Alps by denudation,

[1] Lugeon, _loc. cit._

[2] Schmidt, _Ec. Geol. Helvetiae_, vol. ix., No. 4.

152

and leaving the underlying gneisses rising through the remains of

Permian, Triassic, and Jurassic sediments; while to the north the

great limestone mountains and further north still, the Préalpes,

carved from the remains of the recumbent folds, now stand with

almost as little resemblance to the vanished mountains as the

memories of the past have to its former intense reality.

These views as to the origin of the Alps, which are shared at the

present day by so many distinguished geologists, had their origin

in the labours of many now gone; dating back to Studer; finding

their inspiration in the work of Heim, Suess, and Marcel

Bertrand; and their consummation in that of Lugeon, Schardt,

Rothpletz, Schmidt, and many others. Nor must it be forgotten

that nearer home, somewhat similar phenomena, necessarily on a

smaller scale, were recognised by Lapworth, twenty-six years ago,

in his work on the structure of the Scottish Highlands.

An important tectonic principle underlies the development of the

phenomena we have just been reviewing. The uppermost of the

superimposed recumbent folds is more extended in its development

than those which lie beneath. Passing downwards from the highest

of the folds, they are found to be less and less extended both in

the northerly and in the southerly direction, speaking of the

special case--the Alps--now before us. This feature might be

described somewhat differently. We might say that those folds

which had their roots farther

153

to the south were the most drawn-out towards the north: or again

we might say that the synclinal or deep-seated part of the fold

has lagged behind the anticlinal or what was originally the

highest part of the fold, in the advance of the latter to the

north. The anticline has advanced relatively to the syncline. To

this law one exception only is observed in the Swiss Alps; the

sheet of the Brèche (_Byecciendecke_) falls short, in its northerly

extension, of the underlying fold, which extends to form the

Préalpes.

Contemplating such a generalised section as Professor Schmidt's,

or, indeed, more particular sections, such as those in the Mont

Blanc Massif by Marcel Bertrand,[1] of the Dent de Morcles,

Diablerets, Wildhorn, and Massif de la Brèche by Lugeon,[2] or

finally Termier's section of the Pelvoux Massif,[3] one is

reminded of the breaking of waves on a sloping beach. The wave,

retarded at its base, is carried forward above by its momentum,

and finally spreads far up on the strand; and if it could there

remain, the succeeding wave must necessarily find itself

superimposed upon the first. But no effects of inertia, no

kinetic effects, may be called to our aid in explaining the

formation of mountains. Some geologists have accordingly supposed

that in order to account for

[1] Marcel Bertrand, _Cong. Géol. Internat._, 1900, Guide Géol.,

xiii. a, p. 41.

[2] Lugeon, _loc. cit._, p. 773.

[3] De Lapparent, _Traite de Géol._, p. 1,773.

154

the recumbent folds and the peculiar phenomena of increasing

overlap, or _déferlement_, an obstacle, fixed and deep-seated, must

have arrested the roots or synclines of the folds, and held them

against translational motion, while a movement of the upper crust

drew out and carried forward the anticlines. Others have

contented themselves by recording the facts without advancing any

explanatory hypothesis beyond that embodied in the incontestable

statement that such phenomena must be referred to the effects of

tangential forces acting in the Earth's crust.

It would appear that the explanation of the phenomena of

recumbent folds and their _déferlement_ is to be obtained directly

from the temperature conditions prevailing throughout the

stressed pile of rocks; and here the subject of mountain

tectonics touches that with which we were elsewhere specially

concerned--the geological influence of accumulated radioactive

energy.

As already shown[1], a rise of temperature due to this source of

several hundred degrees might be added to such temperatures as

would arise from the mere blanketing of the Earth, and the

consequent upward movement of the geotherms. The time element is

here the most important consideration. The whole sequence of

events from the first orogenic movements to the final upheaval in

Pliocene times must probably have occupied not less than ten

million years.

[1] _Mountain Genesis_, p. 129, et seq.

155

Unfortunately the full investigation of the distribution of

temperature after any given time is beset with difficulties; the

conditions being extremely complex. If the radioactive heating

was strictly adiabatic--that is, if all the heat was conserved and

none entered from without--the time required for the attainment of

the equilibrium radioactive temperature would be just about six

million years. The conditions are not, indeed, adiabatic; but, on

the other hand, the rocks upraised by lateral pressure were by no

means at 0° C. to start with. They must be assumed to have

possessed such temperatures as the prior radiothermal effects,

and the conducted heat from the Earth's interior, may have

established.

It would from this appear probable that if a duration of ten

million years was involved, the equilibrium radioactive

temperatures must nearly have been attained. The effects of heat

conducted from the underlying earthcrust have to be added,

leading to a further rise in temperature of not less than 500° or

600° . In such considerations the observed indications of high

temperatures in materials now laid bare by denudation, probably

find their explanation (P1. XIX).

The first fact that we infer from the former existence of such a

temperature distribution is the improbability, indeed the

impossibility, that anything resembling a rigid obstacle, or

deep-seated "horst," can have existed beneath the present

surface-level, and opposed the northerly movement of the

deep-lying synclines. For

156

such a horst can only have been constituted of some siliceous

rock-material such as we find everywhere rising through the

worn-down sediments of the Alps; and the idea that this could

retain rigidity under the prevailing temperature conditions, must

be dismissed. There is no need to labour this question; the horst

cannot have existed. To what, then, is the retardation of the

lower parts of the folds, their overthrow, above, to the north,

and their _déferlement_, to be ascribed?

A little consideration shows that the very conditions of high

temperature and viscosity, which render untenable the hypothesis

of a rigid obstacle, suffice to afford a full explanation of the

retardation of the roots of the folds. For directed translatory

movements cannot be transmitted through a fluid, pressure in

which is necessarily hydrostatic, and must be exerted equally in

every direction. And this applies, not only to a fluid, but to a

body which will yield viscously to an impressed force. There will

be a gradation, according as viscosity gives place to rigidity,

between the states in which the applied force resolves itself

into a purely hydrostatic pressure, and in which it is

transmitted through the material as a directed thrust. The nature

of the force, in the most general case, of course, has to be

considered; whether it is suddenly applied and of brief duration,

or steady and long-continued. The latter conditions alone apply

to the present case.

The Birth-Time of the World and Other Scientific Essays · 第 48 / 93 题