Naturally, the public wouldn't stand for that, and the pendulum of opinion began to swing the other way. Cosmo helped his cause by sending to every newspaper a carefully prepared statement of his observations and calculations, in which he spoke with such force of conviction that few could read his words without feeling a thrill of apprehensive uncertainty. This was strengthened by published dispatches which showed that he had forwarded his warnings to all the well-known scientific bodies of the world, which, while decrying them, made no effective response.
And then came a note of positive alarm in a double-leaded bulletin from the new observatory at Mount McKinley, which affirmed that during the preceding night a singular obscurity had been suspected in the northern sky, seeming to veil many stars below the twelfth magnitude. It was added that the phenomenon was unprecedented, but that the observation was both difficult and uncertain.
Nowhere was the atmosphere of doubt and mystery, which now began to hang over the public, so remarkable as in Wall Street. The sensitive currents there responded like electric waves to the new influence, and, to the dismay of hard-headed observers, the market dropped as if it had been hit with a sledge-hammer. Stocks went down five, ten, in some cases twenty points in as many minutes.
The speculative issues slid down like wheat into a bin when the chutes are opened. Nobody could trace the exact origin of the movement, but selling-orders came tumbling in until there was a veritable panic.
From London, Paris, Berlin, Vienna, St. Petersburg, flashed dispatches announcing that the same unreasonable slump had manifested itself there, and all united in holding Cosmo Versál solely responsible for the foolish break in prices. Leaders of finance rushed to the exchanges trying by arguments and expostulations to arrest the downfall, but in vain.
In the afternoon, however, reason partially resumed its sway; then a quick recovery was felt, and many who had rushed to sell all they had, found cause to regret their precipitancy. The next day all was on the mend, as far as the stock market was concerned, but among the people at large the poison of awakened credulity continued to spread, nourished by fresh announcements from the fountain head.
Cosmo issued another statement to the effect that he had perfected plans for an ark of safety, which he would begin at once to construct in the neighborhood of New York, and he not only offered freely to give his plans to any who wished to commence construction on their own account, but he urged them, in the name of Heaven, to lose no time. This produced a prodigious effect, and multitudes began to be infected with a nameless fear.
Meanwhile an extraordinary scene occurred, behind closed doors, at the headquarters of the Carnegie Institution in Washington. Joseph Smith, acting under Cosmo Versál's direction, had forwarded an elaborate précis of the latter's argument, accompanied with full mathematical details, to the head of the institution. The character of this document was such that it could not be ignored. Moreover, the savants composing the council of the most important scientific association in the world were aware of the state of the public mind, and felt that it was incumbent upon them to do something to allay the alarm. Of late years a sort of supervisory control over scientific news of all kinds had been accorded to them, and they appreciated the fact that a duty now rested upon their shoulders.
Accordingly, a special meeting was called to consider the communication from Cosmo Versál. It was the general belief that a little critical examination would result in complete proof of the fallacy of all his work, proof which could be put in a form that the most uninstructed would understand.
But the papers, diagrams, and mathematical formulae had no sooner been spread upon the table under the knowing eyes of the learned members of the council, than a chill of conscious impuissance ran through them. They saw that Cosmo's mathematics were unimpeachable. His formulae were accurately deduced, and his operations absolutely correct.
They could do nothing but attack his fundamental data, based on the alleged revelations of his new form of spectroscope, and on telescopic observations which were described in so much detail that the only way to combat them was by the general assertion that they were illusory. This was felt to be a very unsatisfactory method of procedure, as far as the public was concerned, because it amounted to no more than attacking the credibility of a witness who pretended to describe only what he himself had seen—and there is nothing so hard as to prove a negative.
Then, Cosmo had on his side the whole force of that curious tendency of the human mind which habitually gravitates toward whatever is extraordinary, revolutionary, and mysterious.
But a yet greater difficulty arose. Mention has been made of the strange bulletin from the Mount McKinley observatory. That had been incautiously sent out to the public by a thoughtless observer, who was more intent upon describing a singular phenomenon than upon considering its possible effect on the popular imagination. He had immediately received an expostulatory dispatch from headquarters which henceforth shut his mouth—but he had told the simple truth, and how embarrassing that was became evident when, on the very table around which the savants were now assembled, three dispatches were laid in quick succession from the great observatories of Mount Hekla, Iceland, the North Cape, and Kamchatka, all corroborating the statement of the Mount McKinley observer, that an inexplicable veiling of faint stars had manifested itself in the boreal quarter of the sky.
When the president read these dispatches—which the senders had taken the precaution to mark "confidential"—the members of the council looked at one another with no little dismay. Here was the most unprejudiced corroboration of Cosmo Versál's assertion that the great nebula was already within the range of observation. How could they dispute such testimony, and what were they to make of it?
Two or three of the members began to be shaken in their convictions.
"Upon my word," exclaimed Professor Alexander Jones, "but this is very curious! And suppose the fellow should be right, after all?"
"Right!" cried the president, Professor Pludder, disdainfully. "Who ever heard of a watery nebula? The thing's absurd!"
"I don't see that it's absurd," replied Professor Jones. "There's plenty of proof of the existence of hydrogen in some of the nebulae."
"So there is," chimed in Professor Abel Able, "and if there's hydrogen there may be oxygen, and there you have all that's necessary. It's not the idea that a nebula may consist of watery vapor that's absurd, but it is that a watery nebula, large enough to drown the earth by condensation upon it could have approached so near as this one must now be without sooner betraying its presence."
"How so?" demanded a voice.
"By its attraction. Cosmo Versál says it is already less than three hundred million miles away. If it is massive enough to drown the earth, it ought long ago to have been discovered by its disturbance of the planetary orbits."
"Not at all," exclaimed Professor Jeremiah Moses. "If you stick to that argument you'll be drowned sure. Just look at these facts. The earth weighs six and a half sextillions of tons, and the ocean one and a half quintillions. The average depth of the oceans is two and one-fifth miles. Now—if the level of the oceans were raised only about 1,600 feet, practically all the inhabited parts of the world would be flooded. To cause that increase in the level of the oceans only about one-eighth part would have to be added to their total mass, or, say, one-seventh part, allowing for the greater surface to be covered. That would be one thirty-thousandth of the weight of the globe, and if you suppose that only one-hundredth of the entire nebula were condensed on the earth, the whole mass of the nebula would not need to exceed one three-hundredth of the weight of the earth, or a quarter that of the moon—and nobody here will be bold enough to say that the approach of a mass no greater than that would be likely to be discovered through its attraction when it was three hundred million miles away."
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