CHAPTER XIII

THE PEAKS AND MOUNTAIN RANGES

Not, indeed, from the valley itself, but from the mountains which

bound it, can be seen the second highest mountain in the world, and a

number of peaks of 25,000 feet and over. Kashmir is cradled amidst the

very loftiest mountains, and only Nepal can claim still higher peaks.

By a fortunate coincidence the Government of India have this year

published a remarkably interesting scientific treatise on the high

peaks and principal mountain ranges of Asia, by Colonel Burrard, R.E.,

F.R.S., the officiating Surveyor-General of India, and H. H. Hayden,

Superintendent in the Geological Survey of India. Both these officers

have unique qualifications for the task. Colonel Burrard has for years

made a special study of the Himalayas, and Mr. Hayden has for a great

part of his service been engaged in investigating the geology of

various districts of the Himalayas, and he accompanied me to Tibet.

The highest peak in the world is Mount Everest, which is taken to be

29,002 feet above sea-level, and is situated at the back of Nepal. The

_second_ highest is the peak K2 situated on the boundary between the

Kashmir State and Turkestan, and on the main watershed dividing the

rivers of India from the rivers of Central Asia. It is 28,250 feet

above the sea, and is visible from Haramokh on the northern range of

Kashmir.

It may be wondered why so high a peak has no name. The reason is that,

though high, it is not visible from any inhabited place. It is hidden

away in a remote mountain region behind other peaks of almost as great

magnitude, which being nearer overshadow it--as Mount Everest itself

is overshadowed from Darjiling by the Kinchinjunga range. There is no

village within six days' travel of K2 on either side, and,

consequently, until it was fixed by observation of the Survey, it was

unknown. Colonel Montgomerie, when making the survey of Kashmir,

discovered K2. It was among a series of peaks on what is known as the

Karakoram range, and each of these he designated by the capital letter

K, after Karakoram, and by a number, K1, K2, K3, etc. So it came

about that what proved to be the second highest mountain in the world

became known, not by any name, but by merely a letter and a number.

In 1887, on my way from Peking to India, I passed close under K2 on

its northern side, and in a paper read before the Royal Geographical

Society in the following year made some reference to it. At the

conclusion of my lecture, the late General Walker and Sir Henry

Rawlinson proposed the name of Godwin Austin, after the survey officer

who made the topographical survey of the southern portion of the

Karakoram range. This name was adopted by the Geographical Society,

and now appears on many maps. But it has never been accepted by the

Government of India, and Colonel Burrard in his above-mentioned

treatise now writes:--"Of all the designations suggested for the

supreme peak of the Karakoram that of K2 has now the widest vogue,

and it will be in the interests of uniformity if this symbol be

adopted in future to the exclusion of all others. The permanent

adoption of the symbol K2 will serve to record the interesting facts

that a mountain exceeding 28,000 feet in height had not been deemed

worthy of a name by the people living under its shades, and that its

pre-eminent altitude was unsuspected until it was brought to light by

trigonometrical observation."

With these observations I entirely agree.

K2 was, as I have said, discovered by Colonel Montgomerie in 1858. He

took the first observation to it from Haramokh, the conspicuous peak

on the north side of the valley of Kashmir, at a distance of 137

miles. I saw it first from the north from the Aghil range which I

discovered in 1887, and I subsequently passed close under it both then

and in 1889, and never shall I forget the impression it left on me as

I rounded a spur, and looking up a valley saw, quite unexpectedly,

this real mountain monarch towering almost immediately above me, very

abrupt and upstanding, and with immense masses of ice accumulated at

its base. I have also seen Mount Everest from the north, and it is

remarkable that both these peaks, which are so inconspicuous from the

southern side, should stand out so boldly from the north. K2 is not

so massive a mountain as Kinchinjunga and Nanga Parbat. It is rather

the bold culminating peak of a range.

The height of K2 is put down as 28,250 feet above the sea. How can we

be certain that this is right? The reply is that we cannot. The

observations have been made from immense distances, and are

consequently liable to certain errors which have been discussed by

Colonel Burrard.

It was observed from the following stations:--

Station. Height above Sea. Distance.

Shangruti 17,531 78.9

Biachuthusa 16,746 99.0

Marshala 16,906 58.6

Kastor 15,983 66.0

Thurigo 17,246 61.8

Haramokh 16,001 136.5

Kanuri-Nar 15,437 114.3

Barwai 16,304 88

Thalanka 16,830 74.7

And apart from the errors due to distance there are others which must

always be counted on. As he remarks, no telescope is absolutely

perfect; no level is entirely trustworthy; no instrumental graduations

are strictly exact; and no observer is infallible. Then, again, the

peaks themselves do not always have clearly defined summits, though

K2 happens in this respect to be a model for observation, and as it

has been observed on several occasions from different stations, the

errors in the mean value of height due to faults of observation are,

probably, in Colonel Burrard's opinion, less than ten feet. Another

source of error is the adoption of possibly erroneous altitudes

for the stations of observation. The altitude of K2 was observed from

Haramokh and other stations, but the altitude of Haramokh itself may

be a few feet wrong, and the altitude of K2 on this account may be

thirty feet in error. Another element of uncertainty in determining

the height of a peak is caused by the variation in the amount of snow

on its summit. There is clearly more snow on the summit of a peak in

winter than in summer, and in a hot, dry summer there may be less than

in a generally cloudy, snowy summer. A more complicated description of

error is introduced by the deviation of gravity from the normal in

great mountain ranges. The attraction of the great mass of the

Himalaya mountains and of Tibet pulls all liquids towards itself as

the moon attracts the ocean. The liquid in levels on the theodolites

with which observations of the peaks are made is similarly affected:

the plates to the theodolites in consequence cannot be exactly

adjusted, and when apparently truly levelled are in reality tilted

upwards towards the mountains. At Kurseong, near Darjiling, they would

be as much as 51" out of true level and at Mussouri about 37".

[Illustration: MOUNT HARAMOKH, FROM THE ERIN NULLAH]

But the most serious source of uncertainty in the measurement of the

altitude of a peak is the refraction of the atmosphere. A ray of light

from a peak to an observer's eye does not travel along a straight

line, but assumes a curved path concave to the earth. The ray enters

the observer's eye--I quote from Colonel Burrard--in a direction

tangential to the curve at that point, and this is the direction in

which the observer sees the peak. It makes the peak appear too high.

This refraction is greatest in the morning and evening, and least in

the middle of the day; it is different in summer from what it is in

winter. One of the great Himalayan peaks visible from the plains of

India would appear, from observations with a theodolite made to it

from the plains, to fall 500 feet between sunrise and the afternoon,

and to rise again 300 feet before sunset; and even in the afternoon,

when it would appear lowest, it would still be too high by perhaps 700

feet. This is obviously a very fruitful source of error, and the

difficulty of determining the error is increased by the fact that the

curvature of the ray varies with the rarefaction of the atmosphere. In

the higher altitude, when the rarefaction of the atmosphere increases,

the ray assumes a less curved path. All these possible sources of

error due to the rarefaction of the atmosphere have been most

carefully studied, but even now we must allow 10 to 30 feet as

possible error due to the rarefaction of the atmosphere.

[Illustration: A MOUNTAIN GLEN, BEFORE THE MELTING OF THE SNOWS]

Summarising the possible sources of error in fixing the height of K2

we may say the error may be from--

Errors of observation 20 ft.

Adoption of erroneous height for observing station 30 ft.

Variation of snow-level from the mean Unknown

Deviation of gravity Unknown

Atmospheric refraction 10 to 30 ft.

K2, as I have said, though on the borders of the Kashmir State, and

visible from the range which bounds the Kashmir valley, is not visible

from the valley itself. But Nanga Parbat can be seen from near

Baramula and from a few other parts of the valley, and is the most

striking object in the view from Gulmarg and other points of the

northward-facing slope of the Pir Panjal. It ranks eighth among the

mountains of the world, except K2 all the others being in the Nepal

Himalayas. The order of the mountains is:--

Feet.

Mount Everest 29,002

K2 28,250

Kinchinjunga 28,146

Makalu 27,790

T15 26,867

Dhaulagiri 26,795

XXX 26,658

Nanga Parbat 26,620

Being more accessible than the remote K2 the observations for its

height were made at much closer quarters, the nearest observation

point being 43 miles distant instead of 61 as in the case of K2. It

was observed in all from eleven different points, of which the most

remote was 133 miles. But until it had been measured by the Survey it

had been marked on maps as only 19,000 feet.

Colonel Burrard says it is "the most isolated and perhaps the most

imposing of all the peaks of Asia." It certainly is remarkable for its

isolation. With the exception of subordinate pinnacles rising from its

own buttresses, no peak within 60 miles of it attains an altitude of

more than 17,000 feet. Throughout a circle of 120 miles' diameter

Nanga Parbat surpasses all other summits by more than 9000 feet. And

its upper 5000 feet are precipitous. It stands out therefore in

solitary nobleness, and it can be seen on its northern side rising

23,000 feet from the Indus, there only 3500 above the sea. But whether

it is of all mountains the really most imposing it is not easy to

say, and personally I almost cling to Kinchinjunga. Rakaposhi in

Hunza, which is 25,550 feet in altitude, and can be seen rising sheer

up from the Hunza River 5000 feet above sea-level, is also wonderfully

impressive. There is a peak on the Pamirs 25,146 feet high which can

be seen rising abruptly from the plains of Turkestan, which are but a

little over 3000 feet; and there is the Musherbrum Peak near K2 which

is 25,660 feet--all of which I have seen, and which I find it hard to

place exactly in order of relative impressiveness. But if Nanga Parbat

cannot be placed in unquestionably the first position, it will in most

men's estimation approximate to it, and must in any case be reckoned

among the few most striking sights in the world.

* * * * *

Of what are these great peaks built up? No one has yet ascended their

summits, and as Mr. Hayden points out, the geologist has to do his

work at close quarters, and not like the surveyor from a distance. So

the composition of the highest peaks is rarely known in any detail,

though the general character of the rocks can be ascertained with a

fair approximation to certainty, from observation of material on the

flanks, and from a distant view of the weathering character and

apparent structure of the peaks themselves. From such observations it

has been found that almost all the peaks of 25,000 feet or more in

height are composed of granite, gneiss, and associated crystalline

rocks. It had long be supposed that some of the granites found on the

flanks of the great peaks which presented a foliated appearance were

of sedimentary origin, and had therefore been once deposited beneath

the sea. But their truly intrusive nature was recognised by the late

Lieutenant-General M'Mahon, who proved conclusively that the great

central gneissose rock of the Himalayas was in reality a granite

crushed and foliated by pressure. It may certainly be taken that both

K2 and Nanga Parbat are composed of granite, and have been intruded

or compressed upward from beneath the earth's crust.

Mr. Hayden further concludes that the exceptional height of these

great peaks is due to their being composed of granite, for either the

superior power of the granite to resist the atmospheric forces tending

to their degradation has caused them to stand as isolated masses above

surrounding areas of more easily eroded rocks, or they are areas of

special elevation.

[Illustration: LAKE SHISHA NAG, LIDAR VALLEY]

Now it is found that the axes of the great mountain ranges are also

composed of granite, and it seems probable that special elevating

forces have been at work to raise certain parts of their ranges above

the general level of the whole. And when once such elevation has been

brought about, the disparity between the higher peaks and the

intervening less elevated area would undoubtedly be intensified by the

destructive forces at work, for the mantle of snow and ice, while

slowly carrying on its work of abrasion, would serve as a protection

for the peaks against the disintegrating forces of the atmosphere,

while the lower unprotected areas would be more rapidly eroded.

So argues Mr. Hayden, who further demonstrates that when, during the

development of the Himalayas as a mighty mountain range vast masses of

granite welled up from below, forcing their way through and lifting up

the pre-existing rocks superimposed upon them, it is probable that,

owing to dissimilarity of composition and to structural weaknesses in

certain portions of the earth's crust, movement was more intense at

some points than at others, and that the granite was raised into more

or less dome-like masses standing above the general level of the

growing range, and subsequently carved by the process of erosion into

clusters of peaks.

The great peaks being thus of intrusive origin, the question naturally

arises whether they are _still_ being intruded upward; whether those

great forces at work beneath the surface of the earth are still

impelling them upward; and if so, whether they are being forced upward

more rapidly than the atmospheric forces are wearing down their

summits. From the geological standpoint Mr. Hayden says that it is not

at present possible to say whether the elevatory movement is still in

progress, but he adds that many phenomena observable in the Himalayas

lead us to infer that local elevation has until quite recently been

operative, and the numerous earthquakes still occurring with such

frequency and violence forcibly remind us that the Himalayas have by

no means reached a period of even comparative rest. The surveyor can

as yet give us no more certain answer. Colonel Burrard says the

original observations of the great peaks made between 1850 and 1860

were not sufficiently prolonged at any one station to enable us to

rely with certainty on the values of the height then obtained. When a

slow variation in height has to be determined it is better to carry

out a long series of observations from one station only, rather

than to take a number of observations from different stations, as is

necessary and as was done in determining the absolute height of peaks.

But in 1905 the Survey of India commenced a series of observations

from one station, and it is proposed to observe the heights of several

peaks for some years and at different seasons in each year. Then if a

reliable series of results be once obtained, a similar set of

observations can be repeated at a subsequent date, and any actual

change of height that has occurred in the interval may be discovered.

[Illustration: DISTANT VIEW OF NANGA PARBAT FROM THE KAMRI PASS]

Until these observations are made we cannot say for certain whether

the great peaks are still rising.

THE MOUNTAIN RANGES

So far we have considered the isolated peaks rather than the ranges

themselves. It remains to study these latter. All of them are

popularly regarded as forming part of the "Himalayas." But

Himalaya--pronounced with the stress on the second syllable--simply

means the "abode of snow"; and geographers have had to define the

separate ranges into which this great Himalayan region is divided. The

name of the Great Himalaya is consequently reserved for the supreme

range which extends from the western borders of China, carries the

great peaks, Mount Everest and Kinchinjunga, and runs through Kumaon

and Kashmir to Nanga Parbat, and possibly farther. This is the

culminating range of the earth's surface. The range to the north, on

which stands K2 and some satellite peaks of 26,000 feet, is neither

so long nor has it quite such lofty peaks. It is known as the

Karakoram range because a pass called the Karakoram Pass crosses it.

But a pass called the Mustagh also crosses it, and Mustagh means Ice

Mountain, whereas Karakoram means black gravel. Mustagh, therefore,

appears to me a much more appropriate name for this gigantic range of

ice-clad mountains. It so happens that I am the only European who has

crossed both passes. Each of them is close upon 19,000 feet in

altitude, but the Karakoram, very curiously, has in summer no snow

upon it, and the route leads over black gravel. It is a better known

pass than the former, and, consequently, the name of black gravel got

the start, and now this superb range of mountains is doomed for all

time to suffer from this absurd nomenclature.

[Illustration: MOUNT KOLAHOI, LIDAR VALLEY]

The range, however, lies far at the back of Kashmir, and it is

not so much with it as with the true Himalaya range that we are here

concerned. The mountain ranges which encircle the valley of Kashmir

are the final prolongations of that mighty range which runs from the

borders of Burma thirteen hundred miles away, and bifurcating at the

Sutlej River, forms with its subsidiary spurs the cradle in which the

Kashmir valley is set.

The southern branch of this bifurcation is known as the Pir Panjal

range, and is that which bounds Kashmir on the south. It is the

largest of all the lesser Himalayan ranges, and even at its extremity

in Kashmir it carries many peaks exceeding 15,000 feet; the Tatakuti

Peak, 30 miles south-west of Srinagar, 15,524 feet in height, being

the most conspicuous.

The northern branch of the bifurcation at the Sutlej River of the

great Himalayan range culminates in the Nun Kun peaks (23,410 feet and

23,250 feet), which stand conspicuously 3000 feet above the general

crest of the range, and can be seen on clear days from Gulmarg. From

near them, not far from the Zoji-la, an oblique range branches from

the great Himalayan range, and constitutes the parting between the

Jhelum River and the Kishenganga, the latter river draining the angle

formed by the bifurcation. The height of this North Kashmir range, as

Colonel Burrard calls it, is greatest near the point of bifurcation,

one of its peaks, Haramokh (16,890 feet), reaching above the

snow-line, and being the most conspicuous object which meets the eye

of a traveller entering the valley from the south. Farther westward

the range ramifies and declines.

The main line of the great range of the Himalayas has meanwhile

continued from the remarkable depression at the Zoji Pass along by the

Kamri Pass, to the immense mountain buttress of Nanga Parbat which,

overhanging the deep defiles of the Indus, seems to form a fitting end

to the mighty range which started on the confines of China. But there

are great mountains beyond the Indus also, and whether these form a

continuation of the great Himalayan axis which the river Indus would

in that case have merely cut through in the gorges below Nanga Parbat,

or whether the mountains west of the Indus are part of a separate

range, we shall not know till these latter have been geologically

examined.

Kashmir, described by Sir Francis Younghusband, painted by Major E. Molyneux · 第 13 / 14 章