CHAPTER X.

THE ORIGIN OF COMETS AND METEORS.

The fact that comets and meteors, or at least a large proportion of such

bodies, have entered the solar system from stellar space, is now

admitted by all astronomers. The question, however, in regard to the

origin and nature of these cosmical clouds still remains undecided. The

theory that they consist of matter expelled with great velocity from the

fixed stars appears to harmonize the greatest number of facts, and is

accordingly entitled to respectful consideration. The evidence by which

it is sustained may be briefly stated as follows:

1. The observations of Zollner, Respighi, and others, have indicated the

operation of stupendous eruptive forces beneath the solar surface. The

rose-colored prominences, which Janssen and Lockyer have shown to be

masses of incandescent hydrogen, are regarded by Professor Respighi as

phenomena of eruption. "They are the seat of movements of which no

terrestrial phenomenon can afford any idea; masses of matter, the volume

of which is many hundred times greater than that of the earth,

completely changing their position and form in the space of a few

minutes." The nature of this eruptive force is not understood. We may

assume, however, that it was in active operation long before the sun

had contracted to its present dimensions.

2. With an initial velocity of projection equal to 380 miles per second,

the matter thrown off from the sun would be carried beyond the limits of

the solar system, never to return. With velocities somewhat less, it

would be transported to distances corresponding to those of the aphelia

of the periodic comets.

3. On the 7th of September, 1871, Professor Young, of Dartmouth

College,[29] witnessed an extraordinary explosion on the sun's surface.

The observer, with his telescope, followed the expelled matter to an

elevation of over 200,000 miles. The mean velocity between the altitudes

of 100,000 and 200,000 miles was 166 miles per second. This rate of

motion _in vacuo_ would indicate an initial velocity of about 260 miles

per second. But the sun is surrounded by an extensive atmosphere, whose

resistance must have greatly retarded the velocity of the outrush before

reaching the height of 100,000 miles. The original velocity of these

hydrogen clouds was therefore sufficient, in all probability, to have

carried them, if unresisted, beyond the solar domain. Solid or dense

matter propelled with equal force would doubtless have been driven off

never to return.[30]

[29] Boston Journal of Chemistry, November, 1871.

[30] See Mr. Proctor's interesting discussion of this subject in

the Monthly Notices of the R.A.S., vol. xxxii.

4. This eruptive force, whatever be its nature, is probably common to

the sun and the so-called fixed stars. If so, the dispersed fragments

of ejected matter ought to be found in the spaces intervening between

sidereal systems. Accordingly, the phenomena of comets and meteors have

demonstrated the existence of such matter, widely diffused, in the

portions of space through which the solar system is moving.

5. According to Mr. Sorby the microscopic structure of the aerolites he

has examined points evidently to the fact that they have been at one

time in a state of fusion from intense heat,--a fact in striking harmony

with this theory of their origin.

6. The velocity with which some meteoric bodies have entered the

atmosphere has been greater than that which would have been acquired by

simply falling toward the sun from any distance, however great. On the

theory of their sidereal origin, this excess of velocity has been

dependent on the primitive force of expulsion. The shower of aerolites

which fell at Pultusk, Poland, on the 30th of January, 1868,[31] is not

only a remarkable illustration of the fact here stated, but also of

another which may be accounted for by the same theory, viz.: that

meteoric bodies sometimes enter the solar system in groups or clusters.

[31] See Chapter VII.

7. A striking argument in favor of this theory may be derived from the

researches of the late Professor Graham, considered in connection with

those of Dr. Huggins and other eminent spectroscopists. Professor Graham

found large quantities of hydrogen confined in the pores or cavities of

certain meteoric masses. Now, the spectroscope has shown that the sun's

rose-colored prominences consist of immense volumes of incandescent

hydrogen; that the same element exists in great abundance in many of the

fixed stars, and even in certain nebulæ; and that the star in the

Northern Crown, whose sudden outburst in 1866 so astonished the

scientific world, afforded decided indications of its presence.

THE END.

_BY THE AUTHOR OF THIS VOLUME._

METEORIC ASTRONOMY:

A TREATISE ON

SHOOTING STARS, FIRE BALLS,

AND AEROLITES.

BY DANIEL KIRKWOOD, LL.D.

12mo. Extra Cloth. $1.50.

For sale by Booksellers generally, or will be sent by mail,

postpaid, on receipt of the price by

J. B. LIPPINCOTT & CO., Publishers,

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Transcriber's Note: Obvious errors in spelling and punctuation have been

corrected. Footnotes have been renumbered and moved from the page end to

the end of the paragraph. Images have been moved from the

middle of a paragraph to the closest paragraph break.

Comets and Meteors Their phenomena in all ages; their mutual relations; and the theory of their origin. · 第 10 / 10 章