From the Earth to the Moon Part 32

"No," answered Michel, "he is dead! There," added he, in a piteous tone, "that is embarra.s.sing. I much fear, my poor Diana, that you will leave no progeny in the lunar regions!"

Indeed the unfortunate Satellite had not survived its wound.

It was quite dead. Michel Ardan looked at his friends with a rueful countenance.

"One question presents itself," said Barbicane. "We cannot keep the dead body of this dog with us for the next forty-eight hours."

"No! certainly not," replied Nicholl; "but our scuttles are fixed on hinges; they can be let down. We will open one, and throw the body out into s.p.a.ce."

The president thought for some moments, and then said:

"Yes, we must do so, but at the same time taking very great precautions."

"Why?" asked Michel.

"For two reasons which you will understand," answered Barbicane.

"The first relates to the air shut up in the projectile, and of which we must lose as little as possible."

"But we manufacture the air?"

"Only in part. We make only the oxygen, my worthy Michel; and with regard to that, we must watch that the apparatus does not furnish the oxygen in too great a quant.i.ty; for an excess would bring us very serious physiological troubles. But if we make the oxygen, we do not make the azote, that medium which the lungs do not absorb, and which ought to remain intact; and that azote will escape rapidly through the open scuttles."

"Oh! the time for throwing out poor Satellite?" said Michel.

"Agreed; but we must act quickly."

"And the second reason?" asked Michel.

"The second reason is that we must not let the outer cold, which is excessive, penetrate the projectile or we shall be frozen to death."

"But the sun?"

"The sun warms our projectile, which absorbs its rays; but it does not warm the vacuum in which we are floating at this moment.

Where there is no air, there is no more heat than diffused light; and the same with darkness; it is cold where the sun's rays do not strike direct. This temperature is only the temperature produced by the radiation of the stars; that is to say, what the terrestrial globe would undergo if the sun disappeared one day."

"Which is not to be feared," replied Nicholl.

"Who knows?" said Michel Ardan. "But, in admitting that the sun does not go out, might it not happen that the earth might move away from it?"

"There!" said Barbicane, "there is Michel with his ideas."

"And," continued Michel, "do we not know that in 1861 the earth pa.s.sed through the tail of a comet? Or let us suppose a comet whose power of attraction is greater than that of the sun.

The terrestrial orbit will bend toward the wandering star, and the earth, becoming its satellite, will be drawn such a distance that the rays of the sun will have no action on its surface."

"That _might_ happen, indeed," replied Barbicane, "but the consequences of such a displacement need not be so formidable as you suppose."

"And why not?"

"Because the heat and cold would be equalized on our globe.

It has been calculated that, had our earth been carried along in its course by the comet of 1861, at its perihelion, that is, its nearest approach to the sun, it would have undergone a heat 28,000 times greater than that of summer. But this heat, which is sufficient to evaporate the waters, would have formed a thick ring of cloud, which would have modified that excessive temperature; hence the compensation between the cold of the aphelion and the heat of the perihelion."

"At how many degrees," asked Nicholl, "is the temperature of the planetary s.p.a.ces estimated?"

"Formerly," replied Barbicane, "it was greatly exagerated; but now, after the calculations of Fourier, of the French Academy of Science, it is not supposed to exceed 60@ Centigrade below zero."

"Pooh!" said Michel, "that's nothing!"

"It is very much," replied Barbicane; "the temperature which was observed in the polar regions, at Melville Island and Fort Reliance, that is 76@ Fahrenheit below zero."

"If I mistake not," said Nicholl, "M. Pouillet, another savant, estimates the temperature of s.p.a.ce at 250@ Fahrenheit below zero.

We shall, however, be able to verify these calculations for ourselves."

"Not at present; because the solar rays, beating directly upon our thermometer, would give, on the contrary, a very high temperature. But, when we arrive in the moon, during its fifteen days of night at either face, we shall have leisure to make the experiment, for our satellite lies in a vacuum."

"What do you mean by a vacuum?" asked Michel. "Is it perfectly such?"

"It is absolutely void of air."

"And is the air replaced by nothing whatever?"

"By the ether only," replied Barbicane.

"And pray what is the ether?"

"The ether, my friend, is an agglomeration of imponderable atoms, which, relatively to their dimensions, are as far removed from each other as the celestial bodies are in s.p.a.ce. It is these atoms which, by their vibratory motion, produce both light and heat in the universe."

They now proceeded to the burial of Satellite. They had merely to drop him into s.p.a.ce, in the same way that sailors drop a body into the sea; but, as President Barbicane suggested, they must act quickly, so as to lose as little as possible of that air whose elasticity would rapidly have spread it into s.p.a.ce.

The bolts of the right scuttle, the opening of which measured about twelve inches across, were carefully drawn, while Michel, quite grieved, prepared to launch his dog into s.p.a.ce. The gla.s.s, raised by a powerful lever, which enabled it to overcome the pressure of the inside air on the walls of the projectile, turned rapidly on its hinges, and Satellite was thrown out.

Scarcely a particle of air could have escaped, and the operation was so successful that later on Barbicane did not fear to dispose of the rubbish which enc.u.mbered the car.

CHAPTER VI

QUESTION AND ANSWER

On the 4th of December, when the travelers awoke after fifty-four hours' journey, the chronometer marked five o'clock of the terrestrial morning. In time it was just over five hours and forty minutes, half of that a.s.signed to their sojourn in the projectile; but they had already accomplished nearly seven-tenths of the way. This peculiarity was due to their regularly decreasing speed.

Now when they observed the earth through the lower window, it looked like nothing more than a dark spot, drowned in the solar rays. No more crescent, no more cloudy light! The next day, at midnight, the earth would be _new_, at the very moment when the moon would be full. Above, the orb of night was nearing the line followed by the projectile, so as to meet it at the given hour. All around the black vault was studded with brilliant points, which seemed to move slowly; but, at the great distance they were from them, their relative size did not seem to change.

The sun and stars appeared exactly as they do to us upon earth.

As to the moon, she was considerably larger; but the travelers'

gla.s.ses, not very powerful, did not allow them as yet to make any useful observations upon her surface, or reconnoiter her topographically or geologically.

Thus the time pa.s.sed in never-ending conversations all about the moon. Each one brought forward his own contingent of particular facts; Barbicane and Nicholl always serious, Michel Ardan always enthusiastic. The projectile, its situation, its direction, incidents which might happen, the precautions necessitated by their fall on to the moon, were inexhaustible matters of conjecture.

As they were breakfasting, a question of Michel's, relating to the projectile, provoked rather a curious answer from Barbicane, which is worth repeating. Michel, supposing it to be roughly stopped, while still under its formidable initial speed, wished to know what the consequences of the stoppage would have been.