THE TRAVELS OF THE SUN.

Some recent discussions of the constitution of the sun have turned in

part upon what is known as the sun's proper motion in space. This is

one of the most surprising and interesting things that science has

ever brought to light, and yet it is something of which comparatively

few persons have any knowledge. It is customary to look upon the sun

as if it were the center of the universe, an immovable fiery globe

around which the earth and other planets revolve while it remains

fixed in one place. Nothing could be further from the truth. The sun

is, in fact, the most wonderful of travelers. He is flying through

space at the rate of not less than a hundred and sixty millions of

miles in a year, and the earth and her sister planets are his fellow

voyagers, which, obeying his overpowering attraction, circle about him

as he advances. In other words, if we could take up a position in open

space in advance of the sun, we should see him rushing toward us at

the rate of some 450,000 miles a day, chased by his whole family of

shining worlds and the vast swarms of meteoric bodies which obey his

attraction.

The general direction of this motion of the solar system has been

known since the time of Sir William Herschel. It is toward the

constellation Hercules, which, at this season, may be seen in the

northeastern sky at 9 o'clock in the evening. As the line of this

motion makes an angle of fifty odd degrees with the plane of the

earth's orbit, it follows that the earth is not like a horse at a

windlass, circling around the sun forever in one beaten path, but like

a ship belonging to a fleet whose leader is continually pushing its

prow into unexplored waters.

The path of the earth through space is spiral, so that it is all the

time advancing into new regions along with the sun. She is on a

boundless voyage of discovery, and her human crew are born and die in

widely separated tracts of space. Think of the distance over which the

travels of the sun have borne the earth only since the beginning of

human history! Six thousand years ago the earth and sun were about a

million millions of miles further from the stars in Hercules than they

are to-day. Columbus and his contemporaries lived when the earth was

in a region of the universe more than sixty thousand millions of miles

from the place where it is now, so that since his time the whole human

race has been making a voyage through space, in comparison with which

his longest voyage was as the footstep of a fly.

Thus the great events in the history of the world may be said to have

occurred in different parts of the universe. An almost inconceivable

distance separates the spot which the earth occupied in the time of

Alexander from that which it occupied when Cæsar invaded Gaul. The sun

and the earth have wandered so far from their birthplace that the mind

staggers in the attempt to guess at the stupendous distance which now

probably separates them from it. It may be that the motion of the

solar system is orbital and that our sun and many of the stars, his

fellow suns, are revolving around some common center, but if so, no

means has yet been devised of detecting the form or dimensions of his

orbit. So far as we can see, the sun is moving in a straight line.

Since space is believed to be filled with some sort of ethereal

medium, curious consequences are seen to follow from the motions that

have been described. A solid globe like the earth rushing at great

speed through such a medium will encounter some resistance. If the

medium be exceedingly rare, as it must be in fact, the resistance will

be correspondingly small, but still there will be resistance. If the

sun stood still, the earth, owing to the inclination of its axis to

the plane of its orbit, around the sun, would encounter the resistance

of the ether principally on its northern hemisphere from summer to

winter, and on its southern hemisphere from winter to summer. But in

consequence of the motion of the sun shared by the earth, this law of

distribution is changed, and from summer to winter the earth plows

through the ether with its north pole foremost, while from winter to

summer, although the resistance of the ether is encountered more

evenly by the two hemispheres, yet it is still felt principally in the

northern hemisphere, and the south pole remains practically protected.

It follows that the southern hemisphere, and particularly the south

polar regions are more or less completely sheltered the whole year

around. It might then be supposed that the impact of the particles of

the ether shouldered aside by the earth in its swift flight and the

compression produced in front of the advancing globe would tend to

raise the temperature of the northern hemisphere as compared with the

southern hemisphere, while the south pole, being more or less directly

in the wake of the earth, and in a region of rarefaction of the ether,

would constantly possess a remarkably low temperature.

Now, it is known that the south polar regions are more covered with

ice and snow than those of the north, and that the temperature there

the year around is lower. Whether this difference is owing to the

effects of the earth's journey through the ether, is a question.

The sun, too, moves with his northern hemisphere foremost, and it is

worthy of remark that it has been suspected that the northern

hemisphere of the sun radiates more heat than the southern.

But whatever effect it may or may not have upon the meteorological

condition of the earth, the fact that the solar system is thus

voyaging through space is in itself exceedingly interesting. Not the

wildest traveler's dream presents to the imagination such a voyage as

this on which every inhabitant of the earth is bound. A glance at a

star map shows that the direction in which we are going is carrying us

toward a region of the heavens exceedingly rich in stars, many, and

perhaps most, of which are greater suns than ours. There can be little

doubt that when the sun arrives in the neighborhood of those stars, he

will be surrounded by celestial scenery very different from and much

more brilliant than that of the region of space in which he now is.

The inhabitants of the globe at that distant period will certainly

behold new and far more glorious heavens, though the earth may be

unchanged.--_N.Y. Sun._

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Scientific American Supplement, No. 388, June 9, 1883 · 第 66 / 79 题