CHAPTER VII.

Of the first attempt to pass the Equatorial Tornado; and its tragical issue—Of the attempt to pass the Cloud-Screen.

These improvements in ship-building and ship-propelling were naturally followed by a great development of the science of navigation, to which the mathematical powers of the Hesperians formed an invaluable auxiliary. And thus all that was possible for them to ascertain concerning the physical universe was soon learned. The circumnavigation of the globe was easily effected, for the shape of the continent was such that it could be made without going out of sight of land. Other and more adventurous ships were sent on voyages of discovery in a southerly direction, and these made the discovery of the frightful tempest, mentioned before, which rages everlastingly in the equatorial zone. Not one of these ships succeeded in getting within two hundred miles of the equator itself. The crews reported unanimously that, even at that distance, the seas were simply terrific, and appeared to increase rapidly in violence towards the south. Some of them escaped from the vortex with extreme difficulty.

Whereupon two ships were specially constructed for the purpose of carrying out this exploration. They were of extraordinary strength, fitted with immensely powerful gas-engines, and provided with a seemingly inexhaustible supply of the necessary chemical agents. A crew of one hundred volunteers embarked in each, and they started together on their perilous expedition. After eighty-five days one of these ships returned, but only twenty-five of her crew were with her; the rest had vanished either by mortal lesion or metronomic misery. The survivors reported the existence of an absolute pandemonium. The crew had succeeded in forcing the ship about fifty miles further into the zone of tempests than any of the former explorers. But further progress was hopeless. The man who before described to me one of the waves as a wandering cataract was among those who escaped, and his escape was a very narrow one indeed. He told me himself that when he got back into port his negative metronomic balance wanted but a few units of the point which would have terminated his career. And though they succeeded in forcing their way out of the tornado, this was only accomplished by putting on such power as threatened to tear the sides out of the ship. One of the Niagara-like waves fell on the sister-ship, and she was never seen again.

After this tragedy an act was passed forbidding all attempts to enter the South Sea. Though many volunteers were ready to risk their lives, the legislature refused to sanction such peril.

So now the Hesperian knowledge of the Universe, at the period I speak of, may be shortly summed up as follows:—They knew that their place of abode was a spherical cap. Some had at first maintained that it was a circular plain; but this theory was soon exploded. The uniformly circular horizon visible at sea, and on every large plain, and the results obtained from a general survey of the continent by triangulation, combined to discredit the planar and establish the spherical theory. They knew, also, from pendulum and other experiments, that, at a spot coincident with the centre of the presumed sphere on which they lived, an unknown centre of force existed to which all bodies on the surface tended. And beyond this knowledge there was a great blank. What lay outside the cloud-screen or beyond the equatorial ocean had not entered into the Hesperian mind to conceive.

The attempt to pass the ocean, and the hopes of thereby being enabled to gain some further knowledge of the works of the Unknown Maker, having been completely baffled, the attention of the Hesperians was at once concentrated on their only remaining resource—the possibility of penetrating quite through the cloud-screen. Could this be passed, it was possible that something might be found beyond it which would throw some light on the dark problem of their origin. But difficulties, seemingly insuperable, lay directly in the way of any such attempt. I have already mentioned that a chain of gigantic mountains extends in a south-easterly direction for several thousands of miles from the vicinity of the North Pole, and that several of the peaks of this chain attain an altitude of not less than twenty miles. But, to the ancient Hesperians, the real height of these peaks was quite unknown. No man had ever seen their summits, for they were lost in the cloud-screen.

It might certainly be supposed that here was an obvious way of entering, and possibly penetrating through the screen. But a very short description of the physical features of the mountains will suffice to dispel any such notions.

All the engineers who had made a minute survey of the great mountain chain seem to have agreed that the particular peak which afforded the most favourable opportunity for ascent is one which is situated at about three thousand miles from the pole. It should be remembered that the level of the cloud-screen crosses these peaks at an altitude of about twenty miles, or, in round numbers, one hundred and five thousand feet.

At the place referred to, the several stages of the ascent would be as follows:—First, about twenty thousand feet of easy slopes lead to a wide table-land, a resort much frequented by Hesperian households on account of its delightfully cool and bracing climate. Then follow ten thousand feet of steep ascent to the glacier region. This region, which is commonly regarded as the most formidable obstacle to success, extends, at an average inclination of forty-five degrees, to a vertical height of twenty thousand feet more. The strata of rainclouds, which are as different in formation from the cloud-screen as water is from smoke, never attain a greater elevation than ten miles; so here we have the limit above which neither rain nor snow can be deposited, and where, consequently, the glacier region ends.

This brings us to an altitude of fifty thousand feet above the level of the ocean, and next comes the region of precipices which stretch up to the cloud-screen. This final ascent is divided into three gigantic steps; the first, and smallest of them, about ten thousand feet high, leads to a wide plateau; next comes the most awful of the three, not less than thirty thousand feet, terminating in a much narrower terrace, from which starts the last of the steps. This is not exactly a precipice, but a slope of seventy-five degrees; about fifteen thousand feet of this are visible; it then enters the cloud and is lost to view.

The above description has, I trust, made it manifest that an attempt to reach the screen by the mountain route would prove a very arduous undertaking. Vast labour and cost would be essential, and here the advantages of the great world-parliament became exceedingly conspicuous. The enterprise was cheerfully voted to be a world-work. There was no fear that it would come to an untimely end through lack of any material supplies. A committee of the ablest engineers was appointed to examine and report on the most favourable spot for commencing operations. They were not long in coming to an unanimous decision, and the works began.

It was resolved to drive a tunnel the whole way from the table-land under the glacier as far as its upper edge. This formidable work was found to be quite indispensable, in consequence of the incessant avalanches and ice-falls which, issuing from the glacier, fell down the steep slope to the table-land. Indeed, they were obliged to start the tunnel at a distance of fully five miles from the foot of the slope, as a security against the blocking of the entrance. Running nearly horizontally for these five miles, it then bent upwards at an angle of forty-five degrees, and, after a total rise of thirty thousand feet, issued at the top of the glacier, close to the foot of the first step in the series of precipices. The excavation of this tunnel, which was nearly thirteen miles long, was an exceedingly formidable task. But it was undertaken with such zeal and energy, and carried on with such perseverance, that the seemingly insuperable obstacles were at last overcome. Gangs of experienced miners, superintended by skilful engineers, relieved each other, night and day, at the work. Every material required was supplied in profusion. The new dynamical agent which had supplanted the vapour of water as a motor force, had been rendered available for instantaneous percussive action, after the manner of gunpowder, but with incomparably greater energy; and this was extensively utilised for the removal of the rocks. Still, as it was not possible to work at the tunnel except on one face, several years elapsed before the miners emerged into daylight at the top of the glacier.

Here, before beginning the assault on the region of precipices, an immense depôt was established. The tunnel was laid down with double lines of the same sort of parallel steel rods as those which I had noticed on the road at Lucetta. On these ran a series of small trucks, driven by an endless chain which was moved by the gas engine beforementioned; and by means of these all the stores required were easily brought up.

At the height of fifty thousand feet, which had now been reached, little or no difficulty in breathing was encountered. This was probably owing to the extreme density of the Hesperian atmosphere, which, as was noticed before, is so great that the mercury in the tube of Torricelli, at the sea level, stands at an average height of more than fifty-nine inches. Moreover, the slow rate at which it was observed to fall, during the ascent of the last few thousand feet, gave the engineers good hope that, even at the summit, a sufficiency of air to support life would be found.

The ascent of all the three stages of the precipice region was effected by the process of cutting open galleries, inclined at an angle of thirty degrees, in the face of the vertical cliff. The region of ice and snow having been passed, tunnelling was no longer necessary. Four zigzags, each a mile long, sufficed to reach the first terrace, where another depôt was constructed; and a few years’ more labour, and about a dozen similar zigzags, accomplished the ascent of the tremendous middle precipice, thus bringing them within fifteen thousand feet of the cloud-screen.

As the great work neared its completion, the anxiety and excitement, not only of those actually engaged in it, but of the entire population of the planet, rose to a scarcely conceivable intensity. It was now plain that the cloud level would be reached; but no light had as yet been thrown on the question whether the mountain top did or did not pass through the cloudy stratum. If it did not, all their labour of years had been merely thrown away, and they were left as before in absolute ignorance of the external universe. And the fact that the ascent which still remained to be scaled, was not absolutely vertical, but, sloping a little, even at its foot on the last terrace, appeared to diminish its inclination as it approached the cloud, gave reason to suspect that the actual summit of the mountain was not very far off. It may be added that the cloud itself, as they came nearer, presented an unpromising appearance of great density.

So, the final depôt having been constructed, the work on the last series of galleries was begun and carried on with greatly increased vigour, till an altitude only a few yards lower than the under surface of the cloud was gained. At this place the angle of inclination of the cliff had eased off to sixty-three degrees, and it was thought advisable, in view of the unknown possibilities of the mountain inside this thick screen, to establish, by blasting away the rock, a level surface of sufficient extent to enable them to build yet another storehouse, before venturing to proceed with the sloping gallery.