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Название книги:

The Wit and Humor of America, Volume V

Автор:
Marshall Pinckney Wilder
полная версияThe Wit and Humor of America, Volume V

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MR. DOOLEY ON EXPERT TESTIMONY

By Finley Peter Dunne

"Annything new?" said Mr. Hennessy, who had been waiting patiently for Mr. Dooley to put down his newspaper.

"I've been r-readin' th' tistimony iv th' Lootgert case," said Mr. Dooley.

"What d'ye think iv it?"

"I think so," said Mr. Dooley.

"Think what?"

"How do I know?" said Mr. Dooley. "How do I know what I think? I'm no combi-nation iv chemist, doctor, osteologist, polisman, an' sausage-maker, that I can give ye an opinion right off th' bat. A man needs to be all iv thim things to detarmine annything about a murdher trile in these days. This shows how intilligent our methods is, as Hogan says. A large German man is charged with puttin' his wife away into a breakfas'-dish, an' he says he didn't do it. Th' on'y question, thin, is Did or did not Alphonse Lootgert stick Mrs. L. into a vat, an' rayjooce her to a quick lunch? Am I right?"

"Ye ar-re," said Mr. Hennessy.

"That's simple enough. What th' coort ought to've done was to call him up, an' say: 'Lootgert, where's ye'er good woman?' If Lootgert cudden't tell, he ought to be hanged on gin'ral principles; f'r a man must keep his wife around th' house, an' whin she isn't there, it shows he's a poor provider. But, if Lootgert says, 'I don't know where me wife is,' the coort shud say: 'Go out, an' find her. If ye can't projooce her in a week, I'll fix ye.' An' let that be th' end iv it.

"But what do they do? They get Lootgert into coort an' stand him up befure a gang iv young rayporthers an' th' likes iv thim to make pitchers iv him. Thin they summon a jury composed iv poor, tired, sleepy expressmen an' tailors an' clerks. Thin they call in a profissor from a colledge. 'Profissor,' says th' lawyer f'r the State, 'I put it to ye if a wooden vat three hundherd an' sixty feet long, twenty-eight feet deep, an' sivinty-five feet wide, an' if three hundherd pounds iv caustic soda boiled, an' if the leg iv a ginea pig, an' ye said yesterdah about bicarbonate iv soda, an' if it washes up an' washes over, an' th' slimy, slippery stuff, an' if a false tooth or a lock iv hair or a jawbone or a goluf ball across th' cellar eleven feet nine inches—that is, two inches this way an' five gallons that?' 'I agree with ye intirely,' says th' profissor, 'I made lab'ratory experiments in an' ir'n basin, with bichloride iv gool, which I will call soup-stock, an' coal tar, which I will call ir'n filings. I mixed th' two over a hot fire, an' left in a cool place to harden. I thin packed it in ice, which I will call glue, an' rock-salt, which I will call fried eggs, an' obtained a dark, queer solution that is a cure f'r freckles, which I will call antimony or doughnuts or annything I blamed please.'

"'But,' says th' lawyer f'r th' State, 'measurin' th' vat with gas,—an' I lave it to ye whether this is not th' on'y fair test,—an' supposin' that two feet acrost is akel to tin feet sideways, an' supposin' that a thick green an' hard substance, an' I daresay it wud; an' supposin' you may, takin' into account th' measuremints,—twelve be eight,—th' vat bein' wound with twine six inches fr'm th' handle an' a rub iv th' green, thin ar-re not human teeth often found in counthry sausage?' 'In th' winter,' says th' profissor. 'But th' sisymoid bone is sometimes seen in th' fut, sometimes worn as a watch-charm. I took two sisymoid bones, which I will call poker dice, an' shook thim together in a cylinder, which I will call Fido, poored in a can iv milk, which I will call gum arabic, took two pounds iv rough-on-rats, which I rayfuse to call; but th' raysult is th' same.' Question be th' coort: 'Different?' Answer: 'Yis.' Th' coort: 'Th' same.' Be Misther McEwen: 'Whose bones?' Answer: 'Yis.' Be Misther Vincent: 'Will ye go to th' divvle?' Answer: 'It dissolves th' hair.'

"Now what I want to know is where th' jury gets off. What has that collection iv pure-minded pathrites to larn fr'm this here polite discussion, where no wan is so crool as to ask what anny wan else means? Thank th' Lord, whin th' case is all over, the jury'll pitch th' tistimony out iv th' window, an' consider three questions: 'Did Lootgert look as though he'd kill his wife? Did his wife look as though she ought to be kilt? Isn't it time we wint to supper?' An', howiver they answer, they'll be right, an' it'll make little diff'rence wan way or th' other. Th' German vote is too large an' ignorant, annyhow."

LECTURES ON ASTRONOMY

By John Phoenix

Introductory

The following pages were originally prepared in the form of a course of Lectures to be delivered before the Lowell Institute, of Boston, Mass., but, owing to the unexpected circumstance of the author's receiving no invitation to lecture before that institution, they were laid aside shortly after their completion.

Receiving an invitation from the trustees of the Vallecetos Literary and Scientific Institute, during the present summer, to deliver a course of Lectures on any popular subject, the author withdrew his manuscript from the dusty shelf on which it had long lain neglected, and, having somewhat revised and enlarged it, to suit the capacity of the eminent scholars before whom it was to be displayed, repaired to Vallecetos. But, on arriving at that place, he learned with deep regret, that the only inhabitant had left a few days previous, having availed himself of the opportunity presented by a passing emigrant's horse,—and that, in consequence, the opening of the Institute was indefinitely postponed. Under these circumstances, and yielding with reluctance to the earnest solicitations of many eminent scientific friends, he has been induced to place the Lectures before the public in their present form. Should they meet with that success which his sanguine friends prognosticate, the author may be induced subsequently to publish them in the form of a text-book, for the use of the higher schools and universities; it being his greatest ambition to render himself useful in his day and generation by widely disseminating the information he has acquired among those who, less fortunate, are yet willing to receive instruction.

JOHN PHOENIX.

San Diego Observatory, September 1, 1854.

Lectures on Astronomy—Part I

CHAPTER I

The term Astronomy is derived from two Latin words,—Astra, a star, and onomy, a science; and literally means the science of the stars. "It is a science," to quote our friend Dick (who was no relation at all of Big Dick, though the latter occasionally caused individuals to see stars), "which has, in all ages, engaged the attention of the poet, the philosopher, and the divine, and been the subject of their study and admiration."

By the wondrous discoveries of the improved telescopes of modern times, we ascertain that upward of several hundred millions of stars exist, that are invisible to the naked eye—the nearest of which is millions of millions of miles from the Earth; and as we have every reason to suppose that every one of this inconceivable number of worlds is peopled like our own, a consideration of this fact—and that we are undoubtedly as superior to these beings as we are to the rest of mankind—is calculated to fill the mind of the American with a due sense of his own importance in the scale of animated creation.

It is supposed that each of the stars we see in the Heavens in a cloudless night is a sun shining upon its own curvilinear, with light of its own manufacture; and as it would be absurd to suppose its light and heat were made to be diffused for nothing, it is presumed farther, that each sun, like an old hen, is provided with a parcel of little chickens, in the way of planets, which, shining but feebly by its reflected light, are to us invisible. To this opinion we are led, also, by reasoning from analogy, on considering our own Solar System.

The Solar System is so called, not because we believe it to be the sole system of the kind in existence, but from its principal body, the Sun, the Latin name of which is Sol. (Thus we read of Sol Smith, literally meaning the son of Old Smith.) On a close examination of the Heavens we perceive numerous brilliant stars which shine with a steady light (differing from those which surround them, which are always twinkling like a dewdrop on a cucumber-vine), and which, moreover, do not preserve constantly the same relative distance from the stars near which they are first discovered. These are the planets of the Solar System, which have no light of their own—of which the Earth, on which we reside, is one—which shine by light reflected from the Sun—and which regularly move around that body at different intervals of time and through different ranges in space. Up to the time of a gentleman named Copernicus, who flourished about the middle of the Fifteenth Century, it was supposed by our stupid ancestors that the Earth was the center of all creation, being a large, flat body resting on a rock which rested on another rock, and so on "all the way down"; and that the Sun, planets and immovable stars all revolved about it once in twenty-four hours.

This reminds us of the simplicity of a child we once saw in a railroad-car, who fancied itself perfectly stationary, and thought the fences, houses and fields were tearing past it at the rate of thirty miles an hour;—and poking out its head, to see where on earth they went to, had its hat—a very nice one with pink ribbons—knocked off and irrecoverably lost. But Copernicus (who was a son of Daniel Pernicus, of the firm of Pernicus & Co., wool-dealers, and who was named Co. Pernicus, out of respect to his father's partners) soon set this matter to rights, and started the idea of the present Solar System, which, greatly improved since his day, is occasionally called the Copernican system. By this system we learn that the Sun is stationed at one focus (not hocus, as it is rendered, without authority by the philosopher Partington) of an ellipse, where it slowly grinds on for ever about its own axis, while the planets, turning about their axes, revolve in elliptical orbits of various dimensions and different planes of inclination around it.

 

The demonstration of this system in all its perfection was left to Isaac Newton, an English Philosopher, who, seeing an apple tumble down from a tree, was led to think thereon with such gravity, that he finally discovered the attraction of gravitation, which proved to be the great law of Nature that keeps everything in its place. Thus we see that as an apple originally brought sin and ignorance into the world, the same fruit proved thereafter the cause of vast knowledge and enlightenment;—and indeed we may doubt whether any other fruit but an apple, and a sour one at that, would have produced these great results;—for, had the fallen fruit been a pear, an orange, or a peach, there is little doubt that Newton would have eaten it up and thought no more on the subject.

As in this world you will hardly ever find a man so small but that he has someone else smaller than he, to look up to and revolve around him, so in the Solar System we find that the majority of the planets have one or more smaller planets revolving about them. These small bodies are termed secondaries, moons or satellites—the planets themselves being called primaries.

We know at present of eighteen primaries, viz.: Mercury, Venus, the Earth, Mars, Flora, Vesta, Iris, Metis, Hebe, Astrea, Juno, Ceres, Pallas, Hygeia, Jupiter, Saturn, Herschel, Neptune, and another, yet unnamed. There are distributed among these, nineteen secondaries, all of which, except our Moon, are invisible to the naked eye.

We shall now proceed to consider, separately, the different bodies composing the Solar System, and to make known what little information, comparatively speaking, science has collected regarding them. And, first in order, as in place, we come to

THE SUN

This glorious orb may be seen almost any clear day, by looking intently in its direction, through a piece of smoked glass. Through this medium it appears about the size of a large orange, and of much the same color. It is, however, somewhat larger, being in fact 887,000 miles in diameter, and containing a volume of matter equal to fourteen hundred thousand globes of the size of the Earth, which is certainly a matter of no small importance. Through the telescope it appears like an enormous globe of fire, with many spots upon its surface, which, unlike those of the leopard, are continually changing. These spots were first discovered by a gentleman named Galileo, in the year 1611. Though the Sun is usually termed and considered the luminary of day, it may not be uninteresting to our readers to know that it certainly has been seen in the night. A scientific friend of ours from New England (Mr. R.W. Emerson) while traveling through the northern part of Norway, with a cargo of tinware, on the 21st of June, 1836, distinctly saw the Sun in all its majesty, shining at midnight!—in fact, shining all night! Emerson is not what you would call a superstitious man, by any means—but, he left! Since that time many persons have observed its nocturnal appearance in that part of the country, at the same time of the year. This phenomenon has never been witnessed in the latitude of San Diego, however, and it is very improbable that it ever will be. Sacred history informs us that a distinguished military man, named Joshua, once caused the Sun to "stand still"; how he did it, is not mentioned. There can, of course, be no doubt of the fact, that he arrested its progress, and possibly caused it to "stand still";—but translators are not always perfectly accurate, and we are inclined to the opinion that it might have wiggled a very little, when Joshua was not looking directly at it. The statement, however, does not appear so very incredible, when we reflect that seafaring men are in the habit of actually bringing the Sun down to the horizon every day at 12 Meridian. This they effect by means of a tool made of brass, glass, and silver, called a sextant. The composition of the Sun has long been a matter of dispute.

By close and accurate observation with an excellent opera-glass we have arrived at the conclusion that its entire surface is covered with water to a very great depth; which water, being composed by a process known at present only to the Creator of the Universe and Mr. Paine, of Worcester, Massachusetts, generates carburetted hydrogen gas, which, being inflamed, surrounds the entire body with an ocean of fire, from which we, and the other planets, receive our light and heat. The spots upon its surface are glimpses of water, obtained through the fire; and we call the attention of our old friend and former schoolmate, Mr. Agassiz, to this fact; as by closely observing one of these spots with a strong refracting telescope he may discover a new species of fish, with little fishes inside of them. It is possible that the Sun may burn out after a while, which would leave this world in a state of darkness quite uncomfortable to contemplate; but even under these circumstances it is pleasant to reflect that courting and love-making would probably increase to an indefinite extent, and that many persons would make large fortunes by the sudden rise in value of coal, wood, candles, and gas, which would go to illustrate the truth of the old proverb, "It's an ill wind that blows nobody any good."

Upon the whole, the Sun is a glorious creation; pleasing to gaze upon (through smoked glass), elevating to think upon, and exceedingly comfortable to every created being on a cold day; it is the largest, the brightest, and may be considered by far the most magnificent object in the celestial sphere; though with all these attributes it must be confessed that it is occasionally entirely eclipsed by the moon.

CHAPTER II

We shall now proceed to the consideration of the several planets.

MERCURY

This planet, with the exception of the asteroids, is the smallest of the system. It is the nearest to the Sun, and, in consequence, can not be seen (on account of the Sun's superior light), except at its greatest eastern and western elongations, which occur in March and April, August and September, when it may be seen for a short time immediately after sunset and shortly before sunrise. It then appears like a star of the first magnitude, having a white twinkling light, and resembling somewhat the star Regulus in the constellation Leo. The day in Mercury is about ten minutes longer than ours, its year is about equal to three of our months. It receives six and a half times as much heat from the Sun as we do; from which we conclude that the climate must be very similar to that of Fort Yuma, on the Colorado River. The difficulty of communication with Mercury will probably prevent its ever being selected as a military post; though it possesses many advantages for that purpose, being extremely inaccessible, inconvenient, and, doubtless, singularly uncomfortable. It receives its name from the God, Mercury, in the Heathen Mythology, who is the patron and tutelary Divinity of San Diego County.

VENUS

This beautiful planet may be seen either a little after sunset or shortly before sunrise, according as it becomes the morning or the evening star, but never departing quite forty-eight degrees from the Sun. Its day is about twenty-five minutes shorter than ours; its year seven and a half months or thirty-two weeks. The diameter of Venus is 7,700 miles, and she receives from the Sun thrice as much light and heat as the Earth.

An old Dutchman named Schroeter spent more than ten years in observations on this planet, and finally discovered a mountain on it twenty-two miles in height, but he never could discover anything on the mountain, not even a mouse, and finally died about as wise as when he commenced his studies.

Venus, in Mythology, was a Goddess of singular beauty, who became the wife of Vulcan, the blacksmith, and, we regret to add, behaved in the most immoral manner after her marriage. The celebrated case of Vulcan vs. Mars, and the consequent scandal, is probably still fresh in the minds of our readers. By a large portion of society, however, she was considered an ill-used and persecuted lady, against whose high tone of morals and strictly virtuous conduct not a shadow of suspicion could be cast; Vulcan, by the same parties, was considered a horrid brute, and they all agreed that it served him right when he lost his case and had to pay the costs of court. Venus still remains the Goddess of Beauty, and not a few of her protégés may be found in California.

THE EARTH

The Earth, or as the Latins called it, Tellus (from which originated the expression, "Do tell us"), is the third planet in the Solar System, and the one on which we subsist, with all our important joys and sorrows. The San Diego Herald is published weekly on this planet, for five dollars per annum, payable invariably in advance. As the Earth is by no means the most important planet in the system, there is no reason to suppose that it is particularly distinguished from the others by being inhabited. It is reasonable, therefore, to conclude that all the other planets of the system are filled with living, moving and sentient beings; and as some of them are superior to the Earth in size and position, it is not improbable that their inhabitants may be superior to us in physical and mental organization.

But if this were a demonstrable fact, instead of a mere hypothesis, it would be found a very difficult matter to persuade us of its truth. To the inhabitants of Venus the Earth appears like a brilliant star—very much, in fact, as Venus appears to us; and, reasoning from analogy, we are led to believe that the election of Mr. Pierce, the European war, or the split in the great Democratic party produced but very little excitement among them.

To the inhabitants of Jupiter, our important globe appears like a small star of the fourth or fifth magnitude. We recollect, some years ago, gazing with astonishment upon the inhabitants of a drop of water, developed by the Solar Microscope, and secretly wondering whether they were or not reasoning beings, with souls to be saved. It is not altogether a pleasant reflection that a highly scientific inhabitant of Jupiter, armed with a telescope of (to us) inconceivable form, may be pursuing a similar course of inquiry, and indulging in similar speculations regarding our Earth and its inhabitants. Gazing with curious eye, his attention is suddenly attracted by the movements of a grand celebration of Fourth of July in New York, or a mighty convention in Baltimore. "God bless my soul," he exclaims, "I declare they're alive, these little creatures; do see them wriggle!" To an inhabitant of the Sun, however, he of Jupiter is probably quite as insignificant, and the Sun man is possibly a mere atom in the opinion of a dweller in Sirius. A little reflection on these subjects leads to the opinion that the death of an individual man on this Earth, though perhaps as important an event as can occur to himself, is calculated to cause no great convulsion of Nature or disturb particularly the great aggregate of created beings.

The Earth moves round the Sun from west to east in a year, and turns on its axis in a day; thus moving at the rate of 68,000 miles an hour in its orbit, and rolling around at the tolerably rapid rate of 1,040 miles per hour. As our readers may have seen that when a man is galloping a horse violently over a smooth road, if the horse from viciousness or other cause suddenly stops, the man keeps on at the same rate over the animal's head; so we, supposing the Earth to be suddenly arrested on its axis, men, women, children, horses, cattle and sheep, donkeys, editors and members of Congress, with all our goods and chattels, would be thrown off into the air at a speed of 173 miles a minute, every mother's son of us describing the arc of a parabola, which is probably the only description we should ever be able to give of the affair.

This catastrophe, to one sufficiently collected to enjoy it, would, doubtless, be exceedingly amusing; but as there would probably be no time for laughing, we pray that it may not occur until after our demise; when, should it take place, our monument will probably accompany the movement. It is a singular fact that if a man travel round the Earth in an eastwardly direction he will find, on returning to the place of departure, he has gained one whole day; the reverse of this proposition being true also, it follows that the Yankees who are constantly traveling to the West do not live as long by a day or two as they would if they had stayed at home; and supposing each Yankee's time to be worth $1.50 per day, it may be easily shown that a considerable amount of money is annually lost by their roving dispositions.

 

Science is yet but in its infancy; with its growth, new discoveries of an astounding nature will doubtless be made, among which, probably, will be some method by which the course of the Earth may be altered and it be steered with the same ease and regularity through space and among the stars as a steamboat is now directed through the water. It will be a very interesting spectacle to see the Earth "rounding to," with her head to the air, off Jupiter, while the Moon is sent off laden with mails and passengers for that planet, to bring back the return mails and a large party of rowdy Jupiterians going to attend a grand prize fight in the ring of Saturn.

Well, Christopher Columbus would have been just as much astonished at a revelation of the steamboat and the locomotive engine as we should be to witness the above performance, which our intelligent posterity during the ensuing year A.D. 2000 will possibly look upon as a very ordinary and common-place affair.

Only three days ago we asked a medium where Sir John Franklin was at that time; to which he replied, he was cruising about (officers and crew all well) on the interior of the Earth, to which he had obtained entrance through Symmes Hole!

With a few remarks upon the Earth's Satellite, we conclude the first Lecture on Astronomy; the remainder of the course being contained in a second Lecture, treating of the planets, Mars, Jupiter, Saturn and Neptune, the Asteroids, and the fixed stars, which last, being "fixings," are, according to Mr. Charles Dickens, American property.

THE MOON

This resplendent luminary, like a youth on the Fourth of July, has its first quarter; like a ruined spendthrift its last quarter, and like an omnibus, is occasionally full and new. The evenings on which it appears between these last stages are beautifully illumined by its clear, mellow light.

The Moon revolves in an elliptical orbit about the Earth in twenty-nine days twelve hours forty-four minutes and three seconds, the time which elapses between one new Moon and another. It was supposed by the ancient philosophers that the Moon was made of green cheese, an opinion still entertained by the credulous and ignorant. Kepler and Tyco Brahe, however, held to the opinion that it was composed of Charlotte Russe, the dark portions of its surface being sponge cake, the light blanc mange. Modern advances in science and the use of Lord Rosse's famous telescope have demonstrated the absurdity of all these speculations by proving conclusively that the Moon is mainly composed of the Ferrosesquicyanuret, of the cyanide of potassium! Up to the latest dates from the Atlantic States, no one has succeeded in reaching the Moon. Should anyone do so hereafter, it will probably be a woman, as the sex will never cease making an exertion for that purpose as long as there is a man in it.

Upon the whole, we may consider the Moon an excellent institution, among the many we enjoy under a free, republican form of government, and it is a blessed thing to reflect that the President of the United States can not veto it, no matter how strong an inclination he may feel, from principle or habit, to do so.

It has been ascertained beyond a doubt that the Moon has no air. Consequently, the common expressions, "the Moon was gazing down with an air of benevolence," or with "an air of complacency," or with "an air of calm superiority," are incorrect and objectionable, the fact being that the Moon has no air at all.

The existence of the celebrated "Man in the Moon" has been frequently questioned by modern philosophers. The whole subject is involved in doubt and obscurity. The only authority we have for believing that such an individual exists, and has been seen and spoken with, is a fragment of an old poem composed by an ancient Astronomer of the name of Goose, which has been handed down to us as follows:

 
"The man in the Moon came down too soon
        To inquire the way to Norwich;
The man in the South, he burned his mouth,
        Eating cold, hot porridge."
 

The evidence conveyed in this distich is, however, rejected by the skeptical, among modern Astronomers, who consider the passage an allegory. "The man in the South," being supposed typical of the late John C. Calhoun, and the "cold, hot porridge," alluded to the project of nullification.


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