METEORIC ASTRONOMY.

The number of the _Quarterly Journal of Science_ for May, 1872,

contains some articles of considerable interest. The first is by

the indefatigable Mr. Proctor, on “Meteoric Astronomy,” in which

he embodies a clear and popular summary of the researches which

have earned for Signor Schiaparelli this year’s gold medal of the

Astronomical Society. Like all who venture upon a broad, bold effort of

scientific thought, extending at all into the regions of philosophical

theory, Schiaparelli has had to wait for recognition. A simple and

merely mechanical observation of a bare fact, barely and mechanically

recorded without the exercise of any other of the intellectual

faculties than the external senses and observing powers, is at once

received and duly honored by the scientific world; but any higher

effort is received at first indifferently, or sceptically, and is only

accepted after a period of probation, directly proportionate to its

philosophical magnitude and importance, and inversely proportionate to

the scientific status of the daring theorist.

At first sight this appears unjust, it looks like honoring the laborers

who merely make the bricks, and despising the architect who constructs

the edifice of philosophy from the materials they provide. Many a

disappointed dreamer, finding that his theory of the universe has not

been accepted, and that the expected honors have not been showered

upon him, has violently attacked the whole scientific community

as a contemptible gang of low-minded mechanical plodders, void of

imagination, blind to all poetic aspirations, and incapable of any

grand and comprehensive flight of intellect.

Had these impulsive gentlemen been previously subjected to the strict

discipline of inductive scientific training, their position and

opinions would have been very different. Their great theories would

either have had no existence, or have been much smaller, and they

would understand that philosophic caution is one of the characteristic

results of scientific training.

Simple facts, which can be immediately proved by simple experiments

and simple observations, are at once accepted, and their discoverers

duly honored, without any hesitation or delay, but the grander efforts

of generalization require careful thought and laborious scrutiny for

their verification, and therefore the acknowledgment of their merits is

necessarily delayed; but when it does arrive full justice is usually

done.

Thus Grove’s “Correlation of the Physical Forces,” the greatest

philosophical work on purely physical science of this generation, was

commenced in 1842, when its author occupied but a humble position at

the London Institution. The book was but little noticed for many years,

and, had Mr. Grove (now Sir William Grove) not been duly educated

by the discipline above referred to, he might have become a noisy

cantankerous martyr, one of those “ill-used men” who have been made

familiar to so many audiences by Mr. George Dawson.

Instead of this, he patiently waited, and, as we have lately seen, the

well-deserved honors have now been liberally awarded.

In a very few years hence we shall be able to say the same of the once

diabolical Darwin, and eight or nine other theorists, who must all be

content to take their trial and patiently await the verdict; the time

of waiting being of necessity proportionate to the magnitude of the

issue.

The theories of Schiaparelli, which, as Mr. Proctor says, “after the

usual term of doubt have so recently received the sanction of the

highest astronomical tribunal of Great Britain,” are not of so purely

speculative a character as to demand a very long “term of doubt.” They

are directly based on observations and mathematical calculations which

bring them under the domain of the recognized logic of mathematical

probability. Those who are specially interested in the modern progress

of astronomy should read this article in the _Quarterly Journal of

Science_, which is illustrated with the diagrams necessary for the

comprehension of the researches and reasoning of Schiaparelli and

others who have worked on the same ground.

I can only state the general results, which are that the meteors which

we see every year, more or less abundantly, on the nights of the 10th

and 11th of August, and which always appear to come from the same point

in the heavens, are then and thus visible because they form part of an

eccentric elliptical zone of meteoric bodies which girdle the domain of

the sun; and that our earth, in the course of its annual journey around

the sun, crosses and plunges more or less deeply into this ellipse of

small attendant bodies, which are supposed to be moving in regular

orbits around the sun.

Schiaparelli has compared the position, the direction, and the velocity

of motion of the August meteors with the orbit of the great comet of

1862, and infers that there is a close connection between them, so

close that the meteors may be regarded as a sort of trail which the

comet has left behind. He does not exactly say that they are detached

vertebræ of the comet’s tail, but suggests the possibility of their

original connection with its head.

Similar observations have been made upon the November meteoric showers,

which by similar reasoning, are associated with another comet; and

further yet, it is assumed upon analogy that other recognized meteor

systems, amounting to nearly two hundred in number, are in like manner

associated with other comets.

If these theories are sound, our diagrams and mental pictures of the

solar system must be materially modified. Besides the central sun, the

eight planets and the asteroids moving in their nearly circular orbits,

and some eccentric comets traveling in long ellipses, we must add a

countless multitude of small bodies clustered in elliptical rings, all

traveling together in the path marked by their containing girdle, and

following the lead of a streaming vaporous monster, their parent comet.

We must count such comets, and such rings filled with attendant

fragments, not merely by tens or hundreds, but by thousands and tens of

thousands, even by millions; the path of the earth being but a thread

in space, and yet a hundred or two are strung upon it.

In this article Mr. Proctor seems strongly disposed to return to

the theory which attributes solar heat and light to a bombardment

of meteors from without, and the solar corona and zodiacal light as

visible presentments of these meteors. Still, however, he clings to the

more recent explanation which regards the corona, the zodiacal light,

and the meteors as matter ejected from the sun by the same forces as

those producing the solar prominences. For my own part I shall not

be at all surprised if we find that, ere long, these two apparently

conflicting hypotheses are fully reconciled.

The progress of solar discovery has been so great since January, 1870,

when my ejection theory was published, that I may now carry it out

much further than I then dared, or was justified in daring to venture.

Actual measurement of the projectile forces displayed in some of the

larger prominences renders it not merely possible, but even very

probable, that some of the exceptionally great eruptive efforts of the

sun may be sufficiently powerful to eject solar material beyond the

reclaiming reach of his own gravitating power.

In such a case the banished matter must go on wandering through the

boundless profundity of space until it reaches the domain of some other

sun, which will clutch the fragment with its gravitating energies,

and turn its straight and ever onward course into the curved orbit.

Thus the truant morsel from our sun will become the subject of another

sun—a portion of another solar system.

What one sun may do, another and every other may do likewise, and, if

so, there must be a mutual bombardment, a ceaseless interchange of

matter between the countless suns of the universe. This is a startling

view of our cosmical relations, but we are driving rapidly towards a

general recognition of it.

The November star showers have perpetrated some irregularities this

year. They have been very unpunctual, and have not come from their

right place. We have heard something from Italy, but not the tidings of

the Leonides that were expected. Instead of the great display of the

month occurring on the 13th and 14th, it was seen on the 27th. We have

accounts from different parts of England, Ireland, Scotland, and Wales,

also from Italy, Greece, Egypt, etc.

Mr. Slinto, in a letter to the _Times_, estimates the number seen at

Suez as reaching at least 30,000, while in Italy and Athens about 200

per minute were observed. They were not, however, the Leonides, that

is, they did not radiate from a point in the constellation Leo, but

from the region of Andromeda. Therefore they were distinct from that

system of small wanderers usually designated the “November meteors,”

were not connected with Tempel’s comet (comet 1, 1866), but belong to

quite another set.

The question now discussed by astronomers is whether they are connected

with any other comet, and, if so, with which comet?

In the “Monthly Notices” of the Royal Astronomical Society, published

October 24th last, is a very interesting paper by Professor Herschel,

on “Observations of Meteor Showers,” supposed to be connected with

“Biela’s comet,” in which he recommends that “a watch should be kept

during the last week in November and the first week in December,”

in order to verify “the ingenious suggestions of Dr. Weiss,” which,

popularly stated, amount to this, viz., that a meteoric cloud is

revolving in the same orbit as Biela’s comet, and that in 1772 the

earth dashed through this meteoric orbit on December 10th. In 1826 it

did the same, on December 4th; in 1852 the earth passed through the

node on November 28th, and there are reasons for expecting a repetition

at about the same date in 1872.

The magnificent display of the 27th has afforded an important

verification of these anticipations, which become especially

interesting in connection with the curious history of Biela’s comet,

which receives its name from M. Biela, of Josephstadt, who observed it

in 1826, calculated its orbit, and considered it identical with the

comets of 1772, 1805, etc. It travels in a long eccentric ellipse, and

completes its orbit in 2410 days—about 6¾ years. It appeared again, as

predicted, in 1832 and 1846.

Its orbit very nearly intersects that of the earth, and thus affords

a remote possibility of that sort of collision which has excited so

much terror in the minds of many people, but which an enthusiastic

astronomer of the present generation would anticipate with something

like the sensational interest which stirs the soul of a London

street-boy when he is madly struggling to keep pace with a fire-engine.

The calculations for 1832 showed that this comet should cross the

earth’s orbit a little before the time of the earth’s arrival at the

same place; but as such a comet, traveling in such an orbit, is liable

to possible retardations, the calculations could only be approximately

accurate, and thus the sensational astronomer was not altogether

without hope. This time, however, he was disappointed; the comet was

punctual, and crossed the critical node about a month before the earth

reached it.

As though to compensate for this disappointment, the comet at its next

appearance exhibited some entirely new phenomena. It split itself into

two comets, in such a manner that the performance was visible to the

telescopic observer. Both of these comets had nuclei and short tails,

and they alternately varied in brightness, sometimes one, then the

other, having the advantage. They traveled on at a distance of about

156,000 miles from each other, with parallel tails, and with a sort

of friendly communication in the form of a faint arc of light, which

extended as a kind of bridge, from one to the other. Besides this, the

one which was first the brighter, then the fainter, and finally the

brighter again, threw out two additional tails, one of which extended

lovingly towards its companion.

The time of return in 1852 was of course anxiously expected by

astronomers, and careful watch was kept for the wanderers. They came

again at the calculated time, still separated as before.

They were again due in 1859, in 1866, and, finally, at about the end of

last November, or the beginning of the present month. Though eagerly

looked for by astronomers in all parts of the civilized world, they

have been seen no more since 1852.

What, then, has become of them? Have they further subdivided? Have they

crumbled into meteoric dust? Have they blazed or boiled into thin air?

or have they been dragged by some interfering gravitation into another

orbit? The last supposition is the most improbable, as none of the

visible inhabitants of space have come near enough to disturb them.

The possibility of a dissolution into smaller fragments is suggested

by the fact that, instead of the original single comet, or the two

fragments, meteoric showers have fallen towards the earth at the time

when it has crossed the orbit of the original comet, and these showers

have radiated from that part of the heavens in which the comet should

have appeared. Such was the case with the magnificent display of

November 27th, and astronomers are inclining more and more to the idea

that comets and meteors have a common origin—the meteors are little

comets, or comets are big meteors.

In the latest of the “Monthly Notices,” of the Royal Astronomical

Society, published last week, is a paper by Mr. Proctor, in which he

expands the theory expounded three years ago by an author whom your

correspondent’s modesty prevents him from naming, viz., that the larger

planets—Jupiter, Saturn, Uranus, and Neptune—are minor suns, ejecting

meteoric matter from them by the operation of forces similar to those

producing the solar prominences.

Mr. Proctor subjects this bold hypothesis to mathematical examination,

and finds that the orbit of Tempel’s comet and its companion meteors

correspond to that which would result from such an eruption occurring

on the planet Uranus. An eruptive force effecting a velocity of about

thirteen miles per second, which is vastly smaller than the actually

measured velocity of the matter of the solar eruptions, would be

sufficient to thrust such meteoric or cometary matter beyond the

reclaiming reach of the gravitation of Uranus, and hand it over to the

sun, to make just such an orbit as that of Tempel’s comet and the

Leonides meteors.

He shows that other comets and meteoric zones are similarly allied to

other planets, and thus it may be that the falling stars and comets

are fragments of Jupiter, Saturn, Uranus, or Neptune. Verily, if an

astronomer of the last generation were to start up among us now, he

would be astounded at modern presumption.

The star shower of November 27th, and its connection with Biela’s

broken and lost comet, referred to in my last letter, are still

subjects of research and speculation. On November 30th Professor

Klinkerfues sent to Mr. Pogson, of the Madras Observatory, the

following startling telegram: “Biela touched earth on 27th. Search near

Theta Centauri.”

Mr. Pogson searched accordingly from comet-rise to sunrise on the two

following mornings, but in vain; for even in India they have had cloudy

weather of late. On the third day, however, he had “better luck,” saw

something like a comet through an opening between clouds, and on the

following days was enabled to deliberately verify this observation and

determine the position and some elements of the motion of the comet,

which displayed a bright nucleus, and faint but distinct tail.

This discovery is rather remarkable in connection with the theoretical

anticipation of Professor Klinkerfues; but the conclusion directly

suggested is by no means admitted by astronomers. Some, have supposed

that it is not the primary Biela, but the secondary comet, or offshoot,

which grazed the earth, and was seen by Mr. Pogson; others that it was

neither the body, the envelope, nor the tail of either of the comets

which formed the star shower, but that the meteors of November 27th

were merely a trail which the comet left behind.

A multitude of letters were read at the last and previous meeting of

the Astronomical Society, in which the writers described the details

of their own observations. As these letters came from nearly all parts

of the world, the data have an unusual degree of completeness, and

show very strikingly the value of the work of amateur astronomical

observers.

By the collation and comparison of these, important inductions are

obtainable. Thus Professor A. S. Herschel concludes that the earth

passed through seven strata of meteoric bodies, having each a thickness

of about 50,000 miles—in all about 350,000 miles. As the diameter

of the visible nebulosity of Biela’s comet was but 40,000 miles

when nearest the earth in 1832, the great thickness of these strata

indicates something beyond the comet itself.

Besides this, Mr. Hind’s calculation for the return of the primary

comet shows that on November 27th it was 250 millions of miles from the

earth.

Those, however, who are determined to enjoy the sensation of supposing

that they really have been brushed by the tail of a comet, still have

the secondary comet to fall back upon. This, as already described, was

broken off the original, from which it was seen gradually to diverge,

but was still linked to it by an arch of nebulous matter.

If this divergence has continued, it must now be far

distant—sufficiently far to afford me an opportunity of safely adding

another to the numerous speculations, viz., that we may, on November

27th, have plunged obliquely through this connecting arm of nebulous

matter, which was seen stretching between the parent comet and its

offshoot. The actual position of the meteoric strata above referred to

is quite consistent with the hypothesis.

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