CHAPTER VIII.

LIKE JUPITER.

Yes! Like Jupiter.

At the time of that memorable meeting in honour of Michel Ardan—so

appropriately mentioned by the orator—if J. T. Maston had excitedly

exclaimed, “Let us right the Earth’s axis,” it was because the daring

and fantastical Frenchman, one of the heroes of the Moon Voyage, had

chanted his dithyrambic hymn in honour of the most important planets of

our solar system. In his superb panegyric he had celebrated the special

advantages of the giant planet, as we briefly reported at the time.

The problem solved by the calculator of the Gun Club was the

substitution of a new axis of rotation for the old one on which the

Earth had turned ever since in popular phrase, “the world was a world.”

This new axis of rotation would be perpendicular to the plane of its

orbit; and under such conditions the climatal situation of the old Pole

would be much the same as that of Trondhjem, in Norway, in spring-time.

The palæocrystic armour would thus naturally melt under the rays of the

Sun; and at the same time climate would be distributed over the Earth as

the climates are distributed in Jupiter.

The inclination of our planet’s axis, or in other terms, the angle which

its axis of rotation makes with the plane of its ecliptic is 66° 32′. A

few degrees would thus bring the axis perpendicular to the plane of the

orbit it describes round the Sun.

But—it is important to remark—the effort that the North Polar Practical

Association was about to make would not, strictly speaking, right the

Earth’s axis. Mechanically, no force, however considerable, could

accomplish that. The Earth is not like a chicken on a spit, that we can

take it in our hand and shift it as we will. But the making of a new

axis was possible—it may be said easy—if the engineers only had the

fulcrum dreamt of by Archimedes and the lever imagined by J. T. Maston.

But as it had been decided to keep the invention a secret until further

orders, all that could be done was to study the consequences. And to

begin with, the journals and reviews of all sorts appealing to the

learned and the ignorant devoted themselves to considering how Jupiter

was affected by the approximate perpendicularity of his axis to the

plane of his orbit.

Jupiter, like Mercury, Venus, the Earth, Mars, Saturn, Uranus, and

Neptune, forms part of the solar system, and sweeps round at nearly five

hundred million miles from the central fire; and his volume is about

fourteen times that of the Earth.

If there be such a thing as Jovian life, that is to say, if there are

any inhabitants on Jupiter, the following are the advantages they obtain

by living on the great planet—advantages so poetically brought into

relief at the memorable meeting above alluded to.

In the first place, during the diurnal rotation of Jupiter, which

occupies nine hours, fifty-five minutes, the days are always equal to

the nights in all latitudes; that is to say, the Jovian day is four

hours, fifty-seven minutes long, and the Jovian night lasts also four

hours and fifty-seven minutes.

“There,” said the admirers of Jovian existence, “you have something

suited to people of regular habits. They will be delighted to submit to

such regularity.”

That is what would happen to the Earth if Barbicane did what he

promised, only as the new axis would make no difference in the time of

rotation, twenty-four hours would still separate the successive noons,

and our spheroid would be blessed with nights and days each twelve hours

long, and we should live in a perpetual equinox.

“But the climatal phenomena would be much more curious; and no less

interesting,” said the enthusiasts, “would be the absence of the

seasons.”

Owing to the inclination of the axis to the plane of the orbit, we have

the annual changes known as spring, summer, autumn, and winter. The

Jovians could know nothing of these things, and the Terrestrians would

know them no more. The moment the new axis became perpendicular to the

ecliptic there would be neither frigid zones nor torrid zones, but the

whole Earth would rejoice in a temperate climate.

Why was this?

What is the Torrid zone? It is that part of the Earth comprised between

the Tropics of Cancer and Capricorn. Every place within this zone has

the Sun in the zenith twice a year.

What are the Temperate zones? The part comprised between the Tropics and

the Polar circles; between 23° 28′ and 66° 32′ of latitude, and in which

the Sun never rises to the zenith, but is above the horizon on every day

in the year.

What are the Frigid zones? That part of the circumpolar regions in which

the Sun does not rise above the horizon on every day in the year; while

at the Pole itself he does not rise for six months at a time.

The height of the Sun above the horizon is the cause of the excessive

heat of the Torrid zone, the moderate heat of the Temperate zone, and

the excessive cold within the Polar circles.

When the axis became perpendicular these things would be different. The

Sun would remain on the plane of the Equator. All the year round he

would pursue his imperturbable twelve-hour course, and rise to a

distance from the zenith according to the latitude of the place. In

countries of twenty degrees of latitude he would rise seventy degrees

above the horizon; in countries of forty-nine degrees of latitude he

would rise forty-one; in places of eighty-four degrees he would rise

six, and of ninety degrees (the Pole), he would just peep half his

diameter above the horizon. The days would be perfectly regular, and the

Sun would rise at the same time, and also at the same point on the

horizon, throughout the year.

“Look at the advantages!” said the friends of Barbicane. “Every man,

according to his temperament, can choose his own climate, which will be

invariable!”

Those modern Titans, the North Polar Practical Association, were going

to effect a complete change in the state of things which had existed

ever since the spheroid had been launched on its orbit to become the

Earth as we know it.

The astronomer might lose a few of the familiar constellations; the poet

might lose the long winter nights and the long summer days that figure

so frequently in modern verse; but what of that when we think of the

advantages that would be enjoyed by the majority of the human race?

As the newspapers in the Barbicane interest pointed out, the products of

the Earth being reduced to regularity, the farmer could always plant and

sow in the most favourable temperature.

“Be it so!” said the opposition. “But are we to have no rains, or hail,

or storms, or waterspouts, or other odds and ends that make matters

pleasant for the depressed agriculturist?”

“You may have them, of course,” said the Barbicanians, “but they will

probably be rarer, owing to the regularity of the climate having its

effect on the troubles of the atmosphere! Yes, humanity will profit

greatly by the new state of things. It will be quite a transformation of

the terrestrial globe. Barbicane & Co. will have conferred much good on

the present and future generations by destroying the inequality of the

days and nights and the irritating diversity of the seasons!”

And the _New York Sun_ of the 27th of December concluded one of its most

eloquent articles:—

“Honour to Impey Barbicane and his colleagues! Not only will they have

made the Earth more hygienically habitable, but they will have made it

more productive; for then we can sow as soon as we have harvested, for

no time will be wasted over the winter. Not only will our coal supplies

be increased by the new fields, which will insure a supply for many long

years, but the climatal conditions will be altered to our great

advantage! Honour, then, to Barbicane & Co., who will take the first

rank among the benefactors of mankind!”

The Purchase of the North Pole A sequel to "From the earth to the moon" · 第 8 / 20 章