HALLEY’S COMET

From photograph taken by Professor E. E. Barnard, June 6, 1910, at the

Yerkes Observatory, Williams Bay, Wisconsin

]

Where is it now in its outward journey, at the present time of writing

(1925)? Science can answer the question as definitely as though it were

actually possessed of magic glasses, enabling it to follow the path of

the retreating comet, although it has long since passed beyond our range

of view. It is now approaching the orbit of the planet Neptune, crossing

it in 1933, and reaches its greatest distance outward from the sun in

1943, or 3,200 million miles. In 1964 it draws near to Neptune again,

and will be halfway between Neptune and Uranus in 1974, arriving at the

orbit of Saturn in 1984. Once more it will gladden the eyes of mortals

as it approaches the planet Jupiter, and draws near to pay its respects

to its mighty ruler, the sun.

At its return in 1758 the prediction erred on the side of thirty-two

days; at the return in 1835, by a margin of only two days; and in 1910,

by the amount of two and one-half days. Perchance, ere it makes its next

appearance in 1985,[10] the presence of another planet beyond Neptune

may have been detected, explaining the disturbing factor resulting in

that small discrepancy. The astronomers at that remote date (1984) may

succeed, therefore, in making a prediction so exact that the comet may

“swim into their ken” promptly to scheduled time. Few, if any, of the

present-time readers of this book (unless it falls into the hands of a

very youthful enthusiast) will be here to welcome the comet at its next

return, and even the youthful enthusiast may have the distressing

experience of the American astronomer Dr. Lewis Swift, who saw Halley’s

comet in 1835, and was able to welcome it at its return in 1910, but,

owing to failing eyesight, was unable to see it, much to his regret.

[Illustration:

The orbit of Halley’s Comet, which it passes over in 75 to 77 years,

showing where the comet is to be found now, and during its course

until its next return in 1985.

]

With regard to my first visit to the Yerkes Observatory, the following

facts regarding the great refractor may be of interest, as well as the

incident narrated to me by Miss Calvert while we were awaiting Professor

Barnard’s invitation to look for Halley’s comet, on that momentous

occasion. The story was deferred, in my account, to the final part of

this chapter, so as not to break the thread of the actual account of my

first view of the comet. Following the description of the telescope, the

story of a catastrophe which nearly ended its career is best told in

Professor Barnard’s own words, as quoted from the after-dinner speech,

in January, 1907, at Nashville, already referred to in this book.

“The tube of this instrument is about sixty-four feet long. In the

farther end of this tube is placed the great object glass, forty

inches clear in aperture. When one is looking overhead with this

giant telescope, he must be at a point some thirty feet or more

lower than when the tube is pointed toward the horizon. To avoid the

use of a high ladder to reach the observing end of the telescope in

its various positions, the floor of the dome itself is made into a

giant elevator, sixty-five feet in diameter. The rising and lowering

of this floor—which is done by electric motors—always keeps the

observer in a convenient and safe position with reference to the

eye-end. This floor is suspended by heavy steel cables which go over

wheels at the tops of four towers attached to the inside walls of

the dome. The floor is counterpoised by heavy iron weights at the

other ends of the cables.

“Within a little over a week after the completion of the instrument

and when we had seen through it only once or twice, the two south

cables pulled out of their sockets and the floor fell through fifty

feet to the ground and was destroyed. It was a terrible wreck. This

was on the morning of May 29, 1897, at 6.30 o’clock. Mr. Ellerman

and I had been working all night observing with the telescope. When

we quit at daylight we left the floor at its highest point for the

convenience of some workmen who were to be at work on the tube in

the morning. When the floor fell there was not a soul in the

building, and no one was injured. A couple of hours either way, and

death in all probability would have come to one or the other of us.

Only a few nights before this accident the president of the

University of Chicago and thirty or more trustees and prominent men

of the university had seen through the telescope, and the floor had

been up and down with them on it. If it had fallen then a heavy loss

of life would have been almost certain. A few days before that, Mr.

Clark, who made the great glass, had unpacked the forty-inch disks

on the floor at its highest point, and had put them in the cell

which he finally bolted to the end of the telescope. If the floor

had fallen then, the great lens would have been destroyed, with the

probability that no one would be able to make another, for Mr. Clark

died within a few days after he returned to Cambridge. It was

providential, then, that the floor fell when it did; for the fault

in the attachment of the cables made it certain that it must soon

have fallen.

“But this is not the end of the story. When the floor fell, it

lurched against the great iron pier of the telescope and must have

given it a violent blow. There was some fear that the great glass

might have been injured by the shock. It was nearly a hundred feet

up in the air and could not be reached to see if it was unharmed. By

climbing up on the dome (which is one hundred and ten feet high) and

looking down at the glass, it was seen to be apparently uninjured.

Still, the test could only be made by examining the stars through

it, which was not possible until the floor was replaced by a new

one. Four months were occupied in taking out the wreck and putting

in the new floor.

“There was great anxiety to see the sky through the glass, and the

first night available it was turned to the stars. To our

consternation, there was a great, long flare of light running

through every bright star we examined. This was so strong and

conspicuous that it would make the instrument utterly useless. It

looked as if the lens had been injured by the shock of the floor

against the pier. We examined it in all positions of the instrument,

but we could not get rid of the glaring defect. As I had used the

glass more than anyone else before the accident, my statement that

the defect did not then exist made the matter all the more serious.

It was with heavy hearts that we waited for day to again critically

examine the lens. The next day we all examined the great glass very

carefully, but could see nothing wrong with it. Then Professor Hale

noticed that just back of the glass in the tube was a thick mass of

spider webs stretched across the tube, all running in the same

direction. Upon comparing notes we found that the direction of the

spider webs coincided with that of the flare of light seen the night

before. It seemed that a spider had evidently got in the tube before

the object glass was put on by Clark, and had been unable to get

out; for there was no opening in the tube. During the time the tube

remained at rest, while the new floor was being put in, he had

climbed up to the great glass in the direction of the light; and

when he found his egress barred by the great window, he spun his

web, perhaps as a signal of distress, or maybe in the hope that some

unlucky fly might get in through the glass that he could not get out

of—anyway, with the result that he caused several astronomers the

most uneasy time of their lives. When these webs were swept out by

one of the astronomers climbing up in the tube with a feather

duster, it was found that night, when the stars were examined, that

the flare had vanished and the mighty glass was uninjured.”

CHAPTER SEVEN

ORIGIN OF COMETS AND METEORS

(THEORIES ADVANCED BY THE LATE RICHARD A. PROCTOR.)

Among the author’s most treasured possessions is a clipping from the

Cincinnati _Daily Gazette_ for February 18, 1874, containing a report of

a lecture given by her father, on “Comets and Meteors,” from which the

following is an extract:

“In this lecture on comets and meteors, I promised to give some

account of what is expelled from the sun when great explosions take

place. If I were to say that the comets were shot out from the sun

you might be startled, or if I asserted that they were also thrown

out of Jupiter and Saturn. But the evidence in connection therewith

is very curious. In the first place, we know that matter is shot out

from the sun, with a velocity so great as to be carried away from

him altogether and so would travel into space. That has only been

observed a few times, but the occurrence is probably very frequent.

The matter which was expelled, if it struck the earth at all, would

strike in the daytime. The side of the earth facing the sun will be

the illuminated side. The meteoric matter coming from the sun can

only strike the illuminated part, and this can only happen in the

daytime. You throw a stone at any object, and it must strike the

side of the object you aim at, that is turned toward you. Humboldt

affirmed that the largest number of meteoric masses had fallen in

the daytime. The larger aërolites have been examined and their

microscopic structure studied. Sorby of Sheffield, who examined some

of them, says they consist of a number of small globules and were

originally in a vaporous state before assuming their present

condition. Then came a chemical analysis by Professor Graham and

Chandler Roberts of London. They found in the iron of the meteoric

mass more hydrogen than iron in a natural condition. Professor

Graham said that in his opinion meteors certainly contained iron,

and that probably they had been expelled from one of the stars that

people space. He drew attention to the fact that stars contained

hydrogen in their atmosphere. These are some of the facts concerned

with the larger meteoric masses.

“How shall we account for those meteoric streams which travel close

to the path of Jupiter? All comets of short period have paths

closely approaching some of the large planets. The comet of 1680

went close to Jupiter, long before the explosive power of the sun

was noticed. I call them Jupiter’s family of comets. Sir John

Herschel said that it was very curious that they had that relation.

If we put forward the theory that Jupiter expelled these comets, we

have a very startling theory, but many of the theories which have

been propounded, some of the most important character and which have

been proved to be true, have been the most startling. It is said

that as Jupiter, Saturn, and Uranus go along their paths, they draw

in the comets which travel close to them, and capture them.

“I made a calculation about the November meteors to see how close

they must go to the path of Uranus in order to be captured, and

found that they must approach nearly as close as the nearest

satellite. Only those which came almost in contact with the planet

could be captured. Now, if they were shot out when Uranus was in a

sun-like condition, then it would be explained, whereas we find

great difficulty in imagining that a comet coming out of space would

be captured bodily by a planet like Uranus. Let us consider the

matter thus: if comets are expelled from a planet, they will be

carried along with the forward motion. If it could appear that some

of them went backward, then we would have no evidence of the theory

I have been advancing. If most of them travel forward, then we would

have some evidence for the theory. Now there is the curious fact

that among the comets of short period the whole of Jupiter’s family

travel forward. They do not travel in all directions of slope; all

have a very moderate slope to the paths of the planets. They do not

have the slope even of the asteroids. That is precisely what we

notice—that they travel very much with Jupiter. Taking the balance

between the two theories—that of expulsion and that of capture—it

seems to be in favor of the more startling one—that Jupiter has had

the power to expel these objects.”

It is interesting, in connection with this extract from the report of a

lecture given by my father some fifty years ago at present time of

writing (1925), to turn to a passage in the chapter on comets, by Dr. A.

C. D. Crommelin, in the _Splendour of the Heavens_, page 414, where he

refers as follows to the capture theory:

“The fact that the members of the Jupiter family (of comets) have

direct motion in all cases appears to give a fatal blow to the

capture theory. Practically as many comets would approach the planet

with retrograde motion as with direct; there is, indeed, the point

that those travelling in the same direction as the planet would

remain longer in its neighbourhood, and so have more time to be

perturbed, which would have some weight; but that out of some fifty

comets there is not a single retrograde one is too remarkable a fact

to pass over, and it clearly suggests that Jupiter played a

different part from that of a mere enslaver, and was concerned with

the origin of these bodies in a more intimate manner.

“Many of the considerations I have brought forward were stated by

Mr. R. A. Proctor some fifty years ago; they have therefore been

accessible to astronomers, who nevertheless have been, as a rule,

quite unaffected by them, so that it is time to state them afresh.

The consideration that the life of a short-period comet is limited

by the rapid wastage to which it is subject by the joint action of

the sun and Jupiter was not, I think, so fully realised, when

Proctor wrote as it is now. It serves further to invalidate the

capture theory, since it prevents our assigning to these bodies such

extended lives as that theory demands.”

According to my father’s theory, the giant planets are themselves the

parents of their comet-families, and he pictured their birth as having

occurred in a remote past, when the planets were more sun-like than they

are to-day. We have a great amount of evidence as to the energy of the

processes that are at work on Jupiter, as evidenced, for instance, by

the great Red Spot (though some have hinted at the possibility of its

being an early stage in the formation of a new satellite); Saturn,

Uranus, and Neptune also indicate vast upheavals, though distance in

their case hinders observation, and even on our own planet we have some

striking instances of the power of volcanic energy, as at the eruption

of Krakatoa in 1883. Sounds of the explosion were heard three thousand

miles away, and a huge volume of dust was blown to the highest regions

of the atmosphere, but we are entitled to expect much vaster convulsions

in Jupiter, which outweighs the earth three hundred times and is in a

much hotter state, judging by the deep envelope of vapours surrounding

it, and the rapid changes that are constantly taking place in its

appearance, on an enormous scale, as shown by the fine series of

photographs which have been obtained of the planet with the giant

telescopes.

Writing in his magazine, _Knowledge_, for January 1, 1887, page 64, my

father states:

“The theory of ejection was adopted as the only theory by which the

chemical, physical, and microscopic structure of meteorites of all

orders—from bolosiderites to asiderites—can be accounted for. They

were certainly once exposed to such conditions as exist only in the

interior of large orbs—suns or planets. And as certainly they have

somehow come forth from such interiors. The expulsive force shown by

observation to reside in the only sun-like body we can examine,

indicates the only way in which such expulsion can conceivably have

been effected. Hence, I infer (for my own part I feel assured of the

weight of evidence) that all orders of meteorites were expelled from

some orbs at some time when such orbs were in the sun-like stage.

Generalizing, I include in this theory all orders of meteors, and

find all their most characteristic peculiarities explained, and all

orders of meteor systems or comets, finding their several orders

thus and thus only explicable (if we include all suns now and in the

past, all planets in all solar systems, in their past sun-like

state, among the sources of meteors and comets). No other general

theory seems to me possible.”

Again, in an article in _Knowledge_ for April, 1887, page 135, my father

makes the following statement regarding his theory concerning comets and

meteors:

“All comets and meteors are sun-born. But it is not to our own sun,

nor to those other suns, the stars, that I attribute all comets and

meteor systems. Many millions have come doubtless from our sun

during the many millions of years he has been a sun, though few of

his cometic children are known to terrestrial astronomers. Millions

of millions have come from the many millions of suns in our galaxy

during the many millions of years of their sun-like existence. But

the giant planets were once suns,[11] and in their sun-like state,

which must have lasted millions of years, they must have ejected

their smaller comets and meteor systems which even now, after

millions of years, have paths passing near the orbits of their

parent orbs. Our earth and her fellow terrestrial planets had their

sun-like stage of life, too, and it must have been while the earth

was a sun that the meteors explained specially by Tschermak’s theory

were expelled.”

According to his theory, Tschermak, noting the resemblance of structure

between meteorites and volcanic products, suggests that meteors of all

orders (which would include meteor streams, and therefore comets) were

shot out from the earth in the days when she was young. But though this

is better than the other theories, in at least suggesting some sort of

an origin for comets and meteors, it will not account for comets which

do not approach within many millions of miles of the earth’s orbit,[12]

and a theory which fails for some among the comets cannot be the true

general theory for meteors either.

Mr. Sorby of Sheffield, the eminent mineralogist already referred to,

deduced from the microscopic structure of certain meteorites the

startling theory that they had once been inside the sun; for there is

evidence that their substance once existed in the form of globules of

molten metal, which aggregated with large masses, which in turn were

exposed to violent friction, indicating conflicting motions of very high

velocities.

“Where else,” wrote Sorby, in 1864, “could such conditions exist, except

first in the interior, and afterwards in the immediate neighborhood of

our sun!” But it is absolutely certain that the theory as thus suggested

cannot possibly be true, either as a general explanation of comets and

meteors, or even as an explanation of any known meteor system or comet,

unless, perhaps, a few of the comets whose orbits pass very near the sun

were sun-born, and subsequently disturbed by planetary attractions so as

not to return to their parent orb.

According to my father’s views on the subject:

“A flight of meteors shot out from the sun, as Sorby suggested,

might have velocity enough to get away from him forever, in which

case we should never see a trace of it again, even though we waited

for millions of years. If, however, it could not get away, then it

must return to its starting-place—that is, back to the sun’s

globe—unless, passing near enough to one of the giant planets, it

were so far disturbed as only to return by grazing past the sun’s

surface. (The comets of 1843, 1880, and 1882, which all traveled in

paths near the sun, almost grazing his surface, may well have been

parts of a single meteor-flight shot out from his interior millions

of years ago.)”

After the appearance of the new comet of 1887 in the southern skies, it

was found to be following along the same track as the comets of 1843,

1880, and 1882, thus confirming my father’s theory that these comets

were parts of one large comet, dissipated, doubtless, some millions of

years ago.

These comets were so bright when near the sun that they could be seen at

noon with the naked eye. As regards the heat experienced by the comet of

1843 when near the sun, Sir John Herschel remarked:

“Imagine a glare 25,000 times fiercer than that of an equatorial

sunshine at noonday. In such a heat there is no solid substance we

know of which would not run like water—boil—and be converted into

smoke or vapor.”

[Illustration:

The romance of comets · 第 16 / 21 题