CHAPTER VII.

FURTHER RESEARCHES OF REICHENBACH--THEORY OF METEORS--STABILITY OF

THE SOLAR SYSTEM--DOCTRINE OF A RESISTING MEDIUM.

The able and original researches of the celebrated Reichenbach, who has

made meteoric phenomena the subject of long-continued and enthusiastic

investigation, have attracted the general attention of scientific men.

It is proposed to present, in the following chapter, a brief _resumé_

of his views and conclusions.

1. _The Constitution of Comets._--It is a remarkable fact that cometary

matter has no refractive power, as is manifest from the observations of

stars seen through their substance.[20] These bodies, therefore, are

not gaseous; and the most probable theory in regard to their nature is

that they consist of an infinite number of discrete, solid molecules,

at great distances from each other, with very little attraction among

themselves, or toward the nucleus, and having, therefore, great

mobility. Now Baron Reichenbach, having carefully examined a great

number of meteoric stones, has found them for the most part composed

of extremely minute globules, apparently cemented together. He hence

infers that they have been comets--perhaps very small ones--whose

component molecules have by degrees collected into single masses.

2. _The Number of Aerolites._--The average number of aerolitic falls

in a year was estimated by Schreibers, as previously stated, at 700.

Reichenbach, however, after a thorough discussion of the data at

hand, makes the number much larger. He regards the probable annual

average, for the entire surface of the earth, as not less than 4500.

This would give about twelve daily falls. They are of every variety

as to magnitude, from a weight of less than a single ounce to over

30,000 pounds. The Baron even suspects the meteoric origin of large

masses of dolerite which all former geologists had considered native

to our planet. In view of the fact that from the largest members of

our planetary system down to the particles of meteoric dust there is

an approximately regular gradation, and that the larger, at least

in some instances, appear to have been formed by the aggregation of

the smaller, he asks may not the earth itself have been formed by an

agglomeration of meteorites? The learned author, from the general scope

of his speculations, would thus seem to have adopted a form of the

nebular hypothesis somewhat different from that proposed by Laplace.

3. _Composition and mean Density of Aerolites._--A large proportion of

meteoric stones are similar in structure to the volcanic or plutonic

rocks of the earth; and _all_ consist of elements identical with

those in our planet's crust. Their mean density, moreover, is very

nearly the same with that of the earth. These facts are regarded by

Reichenbach as indicating that those meteoric masses which are daily

becoming incorporated with our planet, have had a common origin with

the earth itself. Baron Reichenbach's views, as presented by himself,

will be found at length in _Poggendorf's Annalen_ for December, 1858.

_Stability of the Solar System._--The well-known demonstrations of

the stability of the solar system, given by Lagrange and Laplace,

are not to be accepted in an unlimited sense. They make no provision

against the destructive agency of a resisting medium, or the entrance

of matter into the solar domain from the interstellar spaces. In

short, the conservative influence ascribed to these celebrated

theorems extends only to the major planets; and even in their case it

is to be understood as applying only to their mutual perturbations.

The phenomena of shooting-stars and aerolites have demonstrated the

existence of considerable quantities of matter moving in _unstable_

orbits. The amount of such matter within the solar system cannot now be

determined; but the term probably includes the zodiacal light, many,

if not all, of the meteoric rings, and a large number of comets. These

unstable parts of the system are being gradually incorporated with the

sun, the earth, and doubtless also with the other large planets. It is

highly probable that at former epochs the quantity of such matter was

much greater than at present, and that, unless new supplies be received

_ab extra_, it must, by slow degrees, disappear from the system.

The fact, now well established, of the extensive diffusion of meteoric

matter through the interplanetary spaces has an obvious bearing on

Encke's theory of a resisting medium. If we grant the existence of such

an ether, it would seem unphilosophical to ascribe to it one of the

properties of a material fluid--the power of resisting the motion of

all bodies moving through it--and to deny it such properties in other

respects. Its condensation, therefore, about the sun and other large

bodies must be a necessary consequence. This condensation existed in

the primitive solar spheroid, before the formation of the planets:

the rotation of the spheroid would be communicated to the coexisting

ether; and hence, _during the entire history of the planetary system,

the ether has revolved around the sun in the same direction with the

planets_. This condensed ether, it is also obvious, must participate in

the progressive motion of the solar system.

But again; even if we reject the doctrine of the development of the

planetary bodies from a rotating nebula, we must still regard the

density of the ether as increasing to the center of the system. The

sun's rotation, therefore, would communicate motion to the first and

denser portions; this motion would be transmitted outward through

successive strata, with a constantly diminishing angular velocity.

The motion of the planets themselves through the medium in nearly

circular orbits would concur in imparting to it a revolution in the

same direction. Whether, therefore, we receive or reject the nebular

hypothesis, the resistance of the ethereal medium to bodies moving

in orbits of small eccentricity and in the direction of the sun's

rotation, becomes an infinitesimal quantity.

The hypothesis of Encke, it is well known, was based solely on the

observed acceleration of the comet which bears his name. More recently,

however, a still greater acceleration has been found in the case of

Faye's comet. Now as the meteoric matter of the solar system is a

_known_ cause for such phenomena, sufficient, in all probability, both

in mode and measure, the doctrine of a resisting ethereal medium would

seem to be a wholly unnecessary assumption.

Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolites · 第 7 / 14 章