METEORITES.

Some years ago, a farmer living near Rowton, in Shropshire, noticed

on a path in a field a hole which had been suddenly made by some

mysterious and unknown agent. The laborers who were near told him they

had just heard a remarkable noise; and when the farmer put his hand

down into the hole, he felt something hot at the bottom of it. He took

a spade and dug up the strange body, and found it to be a piece of

iron, weighing about seven pounds. He was naturally amazed at such an

occurrence, and brought the body home with him.

Where did that piece of iron come from? It is plain that it could not

have been always in the ground. The noise and the recently made hole

showed that was not the case, and that is confirmed by the fact that

the iron was hot. A piece of iron within a few feet of the earth’s

surface cannot have remained warm for any length of time. It is

therefore clear that the iron must have tumbled from the sky. This is

a marvellous notion; in fact, it seems so incredible that at first

people refused to believe that such things as stones or solid lumps of

iron could have fallen from the heavens to the earth. But they had to

believe it; the evidence was too conclusive. Fortunately, however,

the occurrence is a comparatively rare one; indeed, our life on this

globe would have an intolerable anxiety added to it if showers of iron

hailstones like that at Rowton were at all of frequent occurrence. We

should want umbrellas of a more substantial description than those

which suffice for the rains we actually experience. There are, indeed,

instances on record of persons having been killed by the fearful blows

given by these bodies in falling.

The Rowton siderite is a comparatively small one; pieces weighing

hundredweights, and even tons, have been collected together in our

museums. I would recommend you to pay a visit to that interesting room

in our great British Museum in which these meteorites are exhibited.

There we see actual specimens of celestial bodies which we can feel

or weigh, and which our chemists can analyze. It may be noticed that

they only contain substances that we already know on this earth. This

celestial iron has often been made use of in primitive times before

man understood how to smelt iron from its ore and how to transform it

from cast iron to wrought iron. Nature seems to have taken heed of

their wants, and occasionally to have thrown down a lump or two for the

benefit of those who were so fortunate as to secure them.

That these stones or irons drop from the sky is absolutely certain,

but when we try to find out their earlier history we become involved

in not a few difficulties. Nobody really knows the true history of

these objects, but the view of their origin which seems to me to

possess fewer difficulties than any other view is that which we may

call the Columbiad Theory. I use this expression because every boy or

girl listening to me ought to have read Jules Verne’s wonderful book,

“From the Earth to the Moon,” and if any of you have not read it, the

sooner you do so the better. It is there narrated how the gun club of

Baltimore designed a magnificent cannon which was sunk deep into the

ground, and then received a terrific charge of guncotton, on which a

great hollow projectile was carefully lowered, containing inside the

three adventurous explorers who desired to visit the moon. Calculations

were produced with a view of showing that by firing on a particular

day the explosion would drive the projectile up to the moon. There

was, however, the necessary condition that the speed of projection

should be great enough. The gun club were accurate in saying that if

the cannon were able to discharge the projectile with a speed twenty

or thirty times as great as that which had ever been obtained with

any other cannon, then the missile would ascend up and up forever if

no further influence were exerted on it. No doubt we have to overlook

the resistance on the air and a few other little difficulties, but to

this extent, at all events, the gun club were right: that a velocity of

about six or seven miles a second would suffice to carry a body away

from the gravitation of the earth.

No one supposes that there were ever Columbiad cannons on our globe by

which projectiles were shot up into space; but it seems possible that

there may have been in very ancient days volcanoes on the earth with a

shooting power as great as that which President Barbicane designed for

the big cannon.

Even now we have some active volcanoes of great energy on our earth,

and we know that in former days the volcanoes must have been still more

powerful; that, in fact, the Vesuvius of the present must be merely

a popgun in comparison with volcanoes which have shaken the earth in

those primitive days when it had just cooled down from its original

fiery condition. Some of these early volcanoes, in the throes of their

mighty eruptions, appear to have shot forth pieces of iron and volcanic

substances with a violence great enough to carry them off into space.

Suppose that a missile were projected upwards, it would ascend higher

and higher, and gravity would, of course, tend to drag it back again

down to earth. It can be shown that with an initial speed of six or

seven miles a second the missiles would never return to the earth if

only influenced by its attraction. The subsequent history of such a

projectile would be guided by the laws according to which a planet

moves. The body is understood to escape the destination which was aimed

at by the Columbiad. I mean, of course, that it is not supposed to hit

the moon. Of course, this might conceivably happen; but most of the

projectiles would go quite wide of the mark, and would travel off into

space.

Though the earth would be unable to recall the projectile, the

attraction of the sun would still guide it, whether it was as big as

a paving-stone or ever so much larger or smaller. The body would be

constrained to follow a path like a little planet around the sun. This

track it would steadily pursue for ages. The wanderer would, however,

cross the earth’s track once during each of its revolutions at the

point from which it was projected. Of course, it will generally happen

that the earth will not be there at the time the meteorite is crossing,

and the meteorite will not be there at the time the earth is crossing.

Nothing will therefore happen, and the object goes again on its long

rounds. But sometimes it must occur that a meteor does not get past

the junction without coming so close to the earth that it plunges into

the air, often producing a noise and generating a streak of light like

a shooting star. Then it tumbles down, and is restored to that earth

whence it originally came.

If this be the true view--and I think there are less weighty objections

to it than to any other I know of--then the history of the piece

of iron that was found in Shropshire would be somewhat as follows.

Many millions of years ago, when the fires of our earth were much

more vigorous than they are in these dull times, a terrific volcanic

outbreak took place, and vast quantities of material were shot into

space, of which this is one of the fragments. During all the ages that

have since elapsed this piece of iron has followed its lonely track. In

a thousandth part of the time rust and decay would have destroyed it

had it lain on the earth, but in the solitudes of space there was found

no air or damp to produce corrosion. At last, after the completion of

its long travels, it again crashed down on the earth.

We have now briefly surveyed the extent of the solar system. We began

with the sun, which presides over all, and then we discussed the

various planets with their satellites, next we considered the eccentric

comets, and finally the minute bodies which, as shooting stars or

meteorites, must be regarded as forming part of the Sun’s system. In

our closing lecture we shall have to deal with objects of a far more

magnificent character.

Star-land: Being Talks With Young People About the Wonders of the Heavens · 第 95 / 146 题