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HARPER'S

NEW MONTHLY MAGAZINE.

MEMORIES OF MISS JANE PORTER.

BY MRS S. C. HALL.

The strength and glory of England are in the keeping of the wives and mothers of its men; and when we are questioned touching our "celebrated women," we may in general terms refer to those who have watched over, moulded, and inspired our "celebrated" men.

Happy is the country where the laws of God and nature are held in reverence--where each sex fulfills its peculiar duties, and renders its sphere a sanctuary! and surely such harmony is blessed by the Almighty--for while other nations writhe in anarchy and poverty, our own spreads wide her arms to receive all who seek protection or need repose.

The very young have never, perhaps read one of the tales of a lady whose reputation, as a novelist, was in its zenith when Walter Scott published his first novel. We desire to place a chaplet upon the grave of a woman once "celebrated" all over the known world; yet who drew all her happiness from the lovingness of home and friends, while her life was as pure as her renown was extensive.

Sir William Wallace has never lost his heroic ascendency over us, and we have steadily resisted every temptation to open the "popular edition" of the long-loved romance, lest what people will call "the improved state of the human mind," might displace the sweet memory of the mingled admiration and indignation that chased each other, while we read and wept, without ever questioning the truth of the absorbing narrative.

Yet, the "Scottish Chiefs" scarcely achieved the popularity of "Thaddeus of Warsaw," the first romance originated by the active brain and singularly constructive power of Jane Porter, produced at an almost girlish age.

The hero of "Thaddeus of Warsaw" was really Kosciuszko, the beloved pupil of George Washington, the grandest and purest patriot the Modern World has known. The enthusiastic girl was moved to its composition by the stirring times in which she lived; and a personal observation of, and acquaintance with some of those brave men whose struggles for liberty only ceased with their exile, or their existence.

This story brought her abundant honors, and rendered her society, as well as the society of her sister and brother, sought for by all who aimed at a reputation for taste and talent. Mrs. Porter, on her husband's death , sought a residence for her family in Edinburgh, where education and good society are attainable to persons of moderate fortunes, if they are "well born;" but the extraordinary artistic skill of her son Robert required a wider field, and she brought her children to London sooner than she had intended, that his promising talents might be cultivated. We believe the greater part of "Thaddeus of Warsaw" was written in London, either in St. Martin's-lane, Newport-street, or Gerard-street, Soho ; though as soon as Robert Ker Porter's abilities floated him on the stream, his mother and sisters retired, in the brightness of their fame and beauty, to the village of Thames Ditton, a residence they loved to speak of as their "home." The actual labor of "Thaddeus"--her first novel--must have been considerable; for testimony was frequently borne to the fidelity of its localities, and Poles refused to believe that the author had not visited Poland; indeed, she had a happy power in describing localities.

After her sister's death Miss Jane Porter was afflicted with so severe an illness, that we, in common with her other friends, thought it impossible she could carry out her plan of journeying to St. Petersburgh to visit her brother, Sir Robert Ker Porter, who had been long united to a Russian princess, and was then a widower; her strength was fearfully reduced; her once round figure become almost spectral, and little beyond the placid and dignified expression of her noble countenance remained to tell of her former beauty; but her resolve was taken; she wished, she said, to see once more her youngest and most beloved brother, so distinguished in several careers, almost deemed incompatible--as a painter, an author, a soldier, and a diplomatist, and nothing could turn her from her purpose: she reached St. Petersburgh in safety, and with apparently improved health, found her brother as much courted and beloved there as in his own land, and his daughter married to a Russian of high distinction. Sir Robert longed to return to England. He did not complain of any illness, and every thing was arranged for their departure; his final visits were paid, all but one to the Emperor, who had ever treated him as a friend; the day before his intended journey he went to the palace, was graciously received, and then drove home, but when the servant opened the carriage-door at his own residence he was dead! One sorrow after another pressed heavily upon her, yet she was still the same sweet, gentle, holy-minded woman she had ever been, bending with Christian faith to the will of the Almighty--"biding her time."

We did not think at our last leave-taking that Miss Porter's fragile frame could have so long withstood the Power that takes away all we hold most dear; but her spirit was at length summoned, after a few days' total insensibility, on the 24th of May.

We were haunted by the idea that the pretty cottage at Esher, where we spent those happy hours, had been treated even as "Mrs. Porter's Arcadia" at Thames Ditton--now altogether removed; and it was with a melancholy pleasure we found it the other morning in nothing changed; it was almost impossible to believe that so many years had passed since our last visit. While Mr. Fairholt was sketching the cottage, we knocked at the door, and were kindly permitted by two gentle sisters, who now inhabit it, to enter the little drawing-room and walk round the garden; except that the drawing-room has been re-papered and painted, and that there were no drawings and no flowers, the room was not in the least altered; yet to us it seemed like a sepulchre, and we rejoiced to breathe the sweet air of the little garden, and listen to a nightingale, whose melancholy cadence harmonized with our feelings.

"Whenever you are at Esher," said the devoted daughter, the last time we conversed with her, "do visit my mother's tomb." We did so. A cypress flourishes at the head of the grave; and the following touching inscription is carved on the stone:

HERE SLEEPS IN JESUS A CHRISTIAN WIDOW

JANE PORTER OBIIT JUNE 18TH, 1831, AETAT. 86;

THE BELOVED MOTHER OF W. PORTER, M.D., OF SIR ROBERT KER PORTER, AND OF JANE AND ANNA MARIA PORTER, WHO MOURN IN HOPE, HUMBLY TRUSTING TO BE BORN AGAIN WITH HER UNTO THE BLESSED KINGDOM OF THEIR LORD AND SAVIOUR. RESPECT HER GRAVE, FOR SHE MINISTERED TO THE POOR

FOOTNOTES:

'Seek for love, and fill her arms with bays.'

I bring her up in the best society, yet in the shade."

In his early days the President of the Royal Academy painted a very striking portrait of Jane Porter, as "Miranda," and Harlowe painted her in the canoness dress of the order of St. Joachim.

SHOOTING STARS AND METEORIC SHOWERS.

From every region of the globe and in all ages of time within the range of history, exhibitions of apparent instability in the heavens have been observed, when the curtains of the evening have been drawn. Suddenly, a line of light arrests the eye, darting like an arrow through a varying extent of space, and in a moment the firmament is as sombre as before. The appearance is exactly that of a star falling from its sphere, and hence the popular title of shooting star applied to it. The apparent magnitudes of these meteorites are widely different, and also their brilliancy. Occasionally, they are far more resplendent than the brightest of the planets, and throw a very perceptible illumination upon the path of the observer. A second or two commonly suffices for the individual display, but in some instances it has lasted several minutes. In every climate it is witnessed, and at all times of the year, but most frequently in the autumnal months. As far back as records go, we meet with allusions to these swift and evanescent luminous travelers. Minerva's hasty flight from the peaks of Olympus to break the truce between the Greeks and Trojans, is compared by Homer to the emission of a brilliant star. Virgil, in the first book of the Georgics, mentions the shooting stars as prognosticating weather changes:

"And on, before tempestuous winds arise, The seeming stars fall headlong from the skies, And, shooting through the darkness, gild the night With sweeping glories and long trains of light."

Various hypotheses have been framed to explain the nature and origin of these remarkable appearances. When electricity began to be understood, this was thought to afford a satisfactory explanation, and the shooting stars were regarded by Beccaria and Vassali as merely electrical sparks. When the inflammable nature of the gases became known, Lavosier and Volta supposed an accumulation of hydrogen in the higher regions of the atmosphere, because of its inferior density, giving rise by ignition to the meteoric exhibitions. While these theories of the older philosophers have been shown to be untenable, there is still great obscurity resting upon the question, though we have reason to refer the phenomena to a cause exterior to the bounds of our atmosphere. Upon this ground, the subject assumes a strictly astronomical aspect, and claims a place in a treatise on the economy of the solar system.

The first attempt accurately to investigate these elegant meteors was made by two university students, afterward Professors Brandes of Leipsic, and Benzenberg of Dusseldorf, in the year 1798. They selected a base line of 46,200 feet, somewhat less than nine English miles, and placed themselves at its extremities on appointed nights, for the purpose of ascertaining their average altitude and velocity. Out of twenty-two appearances identified as the same, they found,

The greatest observed velocity gave twenty-five miles in a second. A more extensive plan was organized by Brandes in the year 1823, and carried into effect in the neighborhood of Breslaw. Out of ninety-eight appearances, the computed heights were,

The velocities were between eighteen and thirty-six miles in a second, an average velocity far greater than that of the earth in its orbit.

The rush of luminous bodies through the sky of a more extraordinary kind, though a rare occurrence, has repeatedly been observed. They are usually discriminated from shooting stars, and known by the vulgar as fire-balls; but probably both proceed from the same cause, and are identical phenomena. They have sometimes been seen of large volume, giving an intense light, a hissing noise accompanying their progress, and a loud explosion attending their termination. In the year 1676, a meteor passed over Italy about two hours after sunset, upon which Montanari wrote a treatise. It came over the Adriatic Sea as if from Dalmatia, crossed the country in the direction of Rimini and Leghorn, a loud report being heard at the latter place, and disappeared upon the sea toward Corsica. A similar visitor was witnessed all over England, in 1718, and forms the subject of one of Halley's papers to the Royal Society. Sir Hans Sloane was one of its spectators. Being abroad at the time of its appearance, at a quarter past eight at night, in the streets of London, his path was suddenly and intensely illuminated. This, he apprehended at first, might arise from a discharge of rockets; but found a fiery object in the heavens, moving after the manner of a falling star, in a direct line from the Pleiades to below the girdle of Orion. Its brightness was so vivid, that several times he was obliged to turn away his eyes from it. The stars disappeared, and the moon, then nine days old, and high near the meridian, the sky being very clear, was so effaced by the lustre of the meteor as to be scarcely seen. It was computed to have passed over three hundred geographical miles in a minute, at the distance of sixty miles above the surface, and was observed at different extremities of the kingdom. The sound of an explosion was heard through Devon and Cornwall, and along the opposite coast of Bretagne. Halley conjectured this and similar displays to proceed from combustible vapors aggregated on the outskirts of the atmosphere, and suddenly set on fire by some unknown cause. But since his time, the fact has been established, of the actual fall of heavy bodies to the earth from surrounding space, which requires another hypothesis. To these bodies the term a?rolites is applied, signifying atmospheric stones, from ???, the atmosphere, and ?????, a stone. While many meteoric appearances may simply arise from electricity, or from the inflammable gases, it is now certain, from the proved descent of a?rolites, that such bodies are of extra-terrestrial origin.

Some of the instances in the table are of sufficient interest to deserve a notice.

The following are the principal facts with reference to the a?rolites, upon which general dependence may be placed. Immediately after their descent they are always intensely hot. They are covered with a fused black incrustation, consisting chiefly of oxide of iron; and, what is most remarkable, their chemical analysis develops the same substances in nearly the same proportions, though one may have reached the earth in India and another in England. Their specific gravities are about the same; considering 1000 as the proportionate number for the specific gravity of water, that of some of the a?rolites has been found to be,

Ensisheim stone 3233 Benares 3352 Sienna 3418 Gassendi's 3456 Yorkshire 3508 Bachelay's 3535 Bohemia 4281.

The greater specific gravity of the Bohemian stone arose from its containing a greater proportion of iron. An analysis of one of the stones that fell at L'Aigle gives:

Silica 46 per cent Magnesia 10 " Iron 45 " Nickel 2 " Sulphur 5 " Zinc 1 "

Iron is found in all these bodies, and in a considerable quantity, with the rare metal nickel. It is a singular fact, that though a chemical examination of their composition has not discovered any substance with which we were not previously acquainted, yet no other bodies have yet been found, native to the earth, which contain the same ingredients combined. Neither products of the volcanoes, whether extinct or in action, nor the stratified or unstratified rocks, have exhibited a sample of that combination of metallic and earthy substances which the meteoric stones present. During the era that science has admitted their path to the earth as a physical truth, scarcely amounting to half a century, few years have elapsed without a known instance of descent occurring in some region of the globe. To Izarn's list, previously given, upward of seventy cases might be added, which have transpired during the last forty years. A report relating to one of the most recent, which fell in a valley near the Cape of Good Hope, with the affidavits of the witnesses, was communicated to the Royal Society, by Sir John Herschel, in March, 1840. Previously to the descent of the a?rolites, the usual sound of explosion was heard, and some of the fragments falling upon grass, caused it instantly to smoke, and were too hot to admit of being touched. When, however, we consider the wide range of the ocean, and the vast unoccupied regions of the globe, its mountains, deserts, and forests, we can hardly fail to admit that the observed cases of descent must form but a small proportion of the actual number; and obviously in countries upon which the human race are thickly planted many may escape notice through descending in the night, and will lie imbedded in the soil till some accidental circumstance exposes their existence. Some, too, are no doubt completely fused and dissipated in the atmosphere, while others move by us horizontally, as brilliant lights, and pass into the depths of space. The volume of some of these passing bodies is very great. One which traveled within twenty-five miles of the surface, and cast down a fragment, was suppose to weigh upward of half a million of tons. But for its great velocity, the whole mass would have been precipitated to the earth. Two a?rolites fell at Braunau, in Bohemia, July 14, 1847.

A multitude of theories have been devised to account for the origin of these remarkable bodies. The idea is completely inadmissible that they are concretions formed within the limits of the atmosphere. The ingredients that enter into their composition have never been discovered in it, and the air has been analyzed at the sea level and on the tops of high mountains. Even supposing that to have been the case, the enormous volume of atmospheric air so charged required to furnish the particles of a mass of several tons, not to say many masses, is, alone, sufficient to refute the notion. They can not, either, be projectiles from terrestrial volcanoes, because coincident volcanic activity has not been observed, and a?rolites descend thousands of miles apart from the nearest volcano, and their substances are discordant with any known volcanic product. Laplace suggested their projection from lunar volcanoes. It has been calculated that a projectile leaving the lunar surface, where there is no atmospheric resistance, with a velocity of 7771 feet in the first second, would be carried beyond the point where the forces of the earth and the moon are equal, would be detached, therefore, from the satellite, and come so far within the sphere of the earth's attraction as necessarily to fall to it. But the enormous number of ignited bodies that have been visible, the shooting stars of all ages, and the periodical meteoric showers that have astonished the moderns, render this hypothesis untenable, for the moon, ere this, would have undergone such a waste as must have sensibly diminished her orb, and almost blotted her from the heavens. Olbers, was the first to prove the possibility of a projectile reaching us from the moon, but at the same he deemed the event highly improbable, regarding the satellite as a very peaceable neighbor, not capable now of strong explosions from the want of water and an atmosphere. The theory of Chladni will account generally for all the phenomena, be attended with the fewest difficulties, and, with some modifications to meet circumstances not known in his day, it is now widely embraced. He conceived the system to include an immense number of small bodies, either the scattered fragments of a larger mass, or original accumulations of matter, which, circulating round the sun, encounter the earth in its orbit, and are drawn toward it by attraction, become ignited upon entering the atmosphere, in consequence of their velocity, and constitute the shooting stars, a?rolites, and meteoric appearances that are observed. Sir Humphry Davy, in a paper which contains his researches on flame, strongly expresses an opinion that the meteorites are solid bodies moving in space, and that the heat produced by the compression of the most rarefied air from the velocity of their motion must be sufficient to ignite their mass so that they are fused on entering the atmosphere. It is estimated that a body moving through our atmosphere with the velocity of one mile in a second, would extricate heat equal to 30,000? of Fahrenheit--a heat more intense than that of the fiercest artificial furnace that ever glowed. The chief modification given to the Chladnian theory has arisen from the observed periodical occurrence of meteoric showers--a brilliant and astonishing exhibition--to some notices of which we proceed.

The first grand phenomena of a meteoric shower which attracted attention in modern times was witnessed by the Moravian Missionaries at their settlements in Greenland. For several hours the hemisphere presented a magnificent and astonishing spectacle, that of fiery particles, thick as hail, crowding the concave of the sky, as though some magazine of combustion in celestial space was discharging its contents toward the earth. This was observed over a wide extent of territory. Humboldt, then traveling in South America, accompanied by M. Bonpland, thus speaks of it: "Toward the morning of the 13th November, 1799, we witnessed a most extraordinary scene of shooting meteors. Thousands of bodies and falling stars succeeded each other during four hours. Their direction was very regular from north to south. From the beginning of the phenomenon there was not a space in the firmament equal in extent to three diameters of the moon which was not filled every instant with bodies of falling stars. All the meteors left luminous traces or phosphorescent bands behind them, which lasted seven or eight seconds." An agent of the United States, Mr. Ellicott, at that time at sea between Cape Florida and the West India Islands, was another spectator, and thus describes the scene: "I was called up about three o'clock in the morning, to see the shooting stars, as they are called. The phenomenon was grand and awful The whole heavens appeared as if illuminated with sky-rockets, which disappeared only by the light of the sun after daybreak. The meteors, which at any one instant of time appeared as numerous as the stars, flew in all possible directions, except from the earth, toward which they all inclined more or less; and some of them descended perpendicularly over the vessel we were in, so that I was in constant expectation of their falling on us." The same individual states that his thermometer, which had been at 80? Fahr. for four days preceding, fell to 56?, and, at the same time, the wind changed from the south to the northwest, from whence it blew with great violence for three days without intermission. The Capuchin missionary at San Fernando, a village amid the savannahs of the province of Varinas, and the Franciscan monks stationed near the entrance of the Oronoco, also observed this shower of asteroids, which appears to have been visible, more or less, over an area of several thousand miles, from Greenland to the equator, and from the lonely deserts of South America to Weimar in Germany. About thirty years previous, at the city of Quito, a similar event occurred. So great a number of falling stars were seen in a part of the sky above the volcano of Cayambaro, that the mountain itself was thought at first to be on fire. The sight lasted more than an hour. The people assembled in the plain of Exida, where a magnificent view presented itself of the highest summits of the Cordilleras. A procession was already on the point of setting out from the convent of Saint Francis, when it was perceived that the blaze on the horizon was caused by fiery meteors, which ran along the sky in all directions, at the altitude of twelve or thirteen degrees. In Canada, in the years 1814 and 1819, the stellar showers were noticed, and in the autumn of 1818 on the North Sea, when, in the language of one of the observers, the surrounding atmosphere seemed enveloped in one expansive ocean of fire, exhibiting the appearance of another Moscow in flames. In the former cases, a residiuum of dust was deposited upon the surface of the waters, on the roofs of buildings, and on other objects. The deposition of particles of matter of a ruddy color has frequently followed the descent of a?rolites--the origin of the popular stories of the sky having rained blood. The next exhibition upon a great scale of the falling stars occurred on the 13th of November, 1831, and was seen off the coasts of Spain and in the Ohio country. This was followed by another in the ensuing year at exactly the same time. Captain Hammond, then in the Red Sea, off Mocha, in the ship Restitution, gives the following account of it; "From one o'clock A.M. till after daylight, there was a very unusual phenomenon in the heavens. It appeared like meteors bursting in every direction. The sky at the time was clear, and the stars and moon bright, with streaks of light and thin white clouds interspersed in the sky. On landing in the morning, I inquired of the Arabs if they had noticed the above. They said they had been observing it most of the night. I asked them if ever the like had appeared before? The oldest of them replied it had not." The shower was witnessed from the Red Sea westward to the Atlantic, and from Switzerland to the Mauritius.

We now come to by far the most splendid display on record; which, as it was the third in successive years, and on the same day of the month as the two preceding, seemed to invest the meteoric showers with a periodical character; and hence originated the title of the November meteors. The chief scene of the exhibition was included within the limits of the longitude of 61? in the Atlantic Ocean, and that of 100? in Central Mexico, and from the North American lakes to the West Indies. Over this wide area, an appearance presented itself, far surpassing in grandeur the most imposing artificial fire-works. An incessant play of dazzlingly brilliant luminosities was kept up in the heavens for several hours. Some of these were of considerable magnitude and peculiar form. One of large size remained for some time almost stationary in the zenith, over the Falls of Niagara, emitting streams of light. The wild dash of the waters, as contrasted with the fiery uproar above them, formed a scene of unequaled sublimity. In many districts, the mass of the population were terror-struck, and the more enlightened were awed at contemplating so vivid a picture of the Apocalyptic image--that of the stars of heaven falling to the earth, even as a fig-tree casting her untimely figs, when she is shaken of a mighty wind. A planter of South Carolina, thus describes the effect of the scene upon the ignorant blacks: "I was suddenly awakened by the most distressing cries that ever fell on my ears. Shrieks of horror and cries for mercy I could hear from most of the negroes of three plantations, amounting in all to about six or eight hundred. While earnestly listening for the cause, I heard a faint voice near the door calling my name. I arose, and taking my sword, stood at the door. At this moment, I heard the same voice still beseeching me to rise, and saying, 'O my God, the world is on fire!' I then opened the door, and it is difficult to say which excited me most --the awfulness of the scene, or the distressed cries of the negroes. Upward of one hundred lay prostrate on the ground--some speechless, and some with the bitterest cries, but with their hands raised, imploring God to save the world and them. The scene was truly awful; for never did rain fall much thicker than the meteors fell toward the earth; east, west, north, and south, it was the same."

This extraordinary spectacle commenced a little before midnight, and reached its height between four and six o'clock in the morning. The night was remarkably fine. Not a cloud obscured the firmament. Upon attentive observation, the materials of the shower were found to exhibit three distinct varieties:--1. Phosphoric lines formed one class apparently described by a point. These were the most abundant. They passed along the sky with immense velocity, as numerous as the flakes of a sharp snow-storm. 2. Large fire-balls formed another constituency of the scene. These darted forth at intervals along the arch of the sky, describing an arc of 30? or 40? in a few seconds. Luminous trains marked their path, which remained in view for a number of minutes, and in some cases for half an hour or more. The trains were commonly white, but the various prismatic colors occasionally appeared, vividly and beautifully displayed. Some of these fire-balls, or shooting-stars, were of enormous size. Dr. Smith of North Carolina observed one which appeared larger than the full moon at the horizon. "I was startled," he remarks, "by the splendid light in which the surrounding scene was exhibited, rendering even small objects quite visible." The same, or a similar luminous body, seen at New Haven, passed off in a northwest direction, and exploded near the star Capella. 3. Another class consisted of luminosities of irregular form, which remained nearly stationary for a considerable time, like the one that gleamed aloft over the Niagara Falls. The remarkable circumstance is testified by every witness, that all the luminous bodies, without a single exception, moved in lines, which converged in one and the same point of the heavens; a little to the southeast of the zenith. They none of them started from this point, but their direction, to whatever part of the horizon it might be, when traced backward, led to a common focus. Conceive the centre of the diagram to be nearly overhead, and a proximate idea may be formed of the character of the scene, and the uniform radiation of the meteors from the same source. The position of this radiant point among the stars was near Leonis. It remained stationary with respect to the stars during the whole of the exhibition. Instead of accompanying the earth in its diurnal motion eastward, it attended the stars in their apparent movement westward. The source of the meteoric shower was thus independent of the earth's rotation, and this shows its position to have been in the regions of space exterior to our atmosphere. According to the American Professor, Dr. Olmsted, it could not have been less than 2238 miles above the earth's surface.

The attention of astronomers in Europe, and all over the world, was, as may be imagined, strongly roused by intelligence of this celestial display on the western continent; and as the occurrence of a meteoric shower had now been observed for three years successively, at a coincident era, it was inferred that a return of this fiery hail-storm might be expected in succeeding Novembers. Arrangements were therefore made to watch the heavens on the nights of the 12th and 13th in the following years at the principal observatories; and though no such imposing spectacle as that of 1833 has been witnessed, yet extraordinary flights of shooting stars have been observed in various places at the periodic time, tending also from a fixed point in the constellation Leo. They were seen in Europe and America on November 13th, 1834. The following results of simultaneous observation were obtained by Arago from different parts of France on the nights of November 12th and 13th, 1830:

Place. Meteors.

Paris, at the Observatory 170 Dieppe 36 Arras 27 Strasburg 85 Von Altimarl 75 Angou 49 Rochefort 23 Havre 300

On November 12th, 1837, at eight o'clock in the evening, the attention of observers in various parts of Great Britain was directed to a bright, luminous body, apparently proceeding from the north, which, after making a rapid descent, in the manner of a rocket, suddenly burst, and scattering its particles into various beautiful forms, vanished in the atmosphere. This was succeeded by others all similar to the first, both in shape and the manner of its ultimate disappearance. The whole display terminated at ten o'clock, when dark clouds which continued up to a late hour, overspread the earth, preventing any further observation. In the November of 1838, at the same date, the falling stars were abundant at Vienna: and one of remarkable brilliancy and size, as large as the full moon in the zenith, was seen on the 13th by M. Verusmor, off Cherburg, passing in the direction of Cape La Hogue, a long, luminous train marking its course through the sky. The same year, the non-commissioned officers in the island of Ceylon were instructed to look out for the falling stars. Only a few appeared at the usual time; but on the 5th of December, from nine o'clock till midnight, the shower was incessant, and the number defied all attempts at counting them.

Professor Olmsted, an eminent man of science, himself an eye-witness of the great meteoric shower on the American continent, after carefully collecting and comparing facts, proposed the following theory: The meteors of November 13th, 1833, emanated from a nebulous body which was then pursuing its way along with the earth around the sun; that this body continues to revolve around the sun in an elliptical orbit, but little inclined to the plane of the ecliptic, and having its aphelion near the orbit of the earth; and finally, that the body has a period of nearly six months, and that its perihelion is a little within the orbit of Mercury. The diagram represents the ellipse supposed to be described, E being the orbit of the earth, M that of Mercury, and N that of the assumed nebula, its aphelion distance being about 95 millions of miles, and the perihelion 24 millions. Thus, when in aphelion, the body is close to the orbit of the earth, and this occurring periodically, when the earth is at the same time in that part of its orbit, nebulous particles are attracted toward it by its gravity, and then, entering the atmosphere, are consumed in it by their concurrent velocities, causing the appearance of a meteoric shower. The parent body is inferred to be nebular, because, though the meteors fall toward the earth with prodigious velocity, few, if any, appear to have reached the surface. They were stopped by the resistance of the air and dissipated in it, whereas, if they had possessed any considerable quantity of matter, the momentum would have been sufficient to have brought them down in some instances to the earth. Arago has suggested a similar theory, that of a stream or group of innumerable bodies, comparatively small, but of various dimensions, sweeping round the solar focus in an orbit which periodically cuts that of the earth. These two theories are in substance the Chladnian hypothesis, first started to explain the observed actual descent of a?rolites. Though great obscurity rests upon the subject, the fact may be deemed certain that independently of the great planets and satellites of the system, there are vast numbers of bodies circling round the sun, both singly and in groups, and probably an extensive nebula, contact with which causes the phenomena of shooting stars, a?rolites, and meteoric showers. But admitting the existence of such bodies to be placed beyond all doubt, the question of their origin, whether original accumulations of matter, old as the planetary orbs, or the dispersed trains of comets, or the remains of a ruined world, is a point beyond the power of the human understanding to reach.

A FIVE DAYS' TOUR IN THE ODENWALD.

A SKETCH OF GERMAN LIFE.

BY WILLIAM HOWITT.

The Odenwald, or Forest of Odin, is one of the most primitive districts of Germany. It consists of a hilly, rather than a mountainous district, of some forty miles in one direction, and thirty in another. The beautiful Neckar bounds it on the south; on the west it is terminated by the sudden descent of its hills into the great Rhine plain. This boundary is well known by the name of the Bergstrasse, or mountain road; which road, however, was at the foot of the mountains, and not over them, as the name would seem to imply. To English travelers, the beauty of this Bergstrasse is familiar. The hills, continually broken into by openings into romantic valleys, slope rapidly down to the plain, covered with picturesque vineyards; and at their feet lie antique villages, and the richly-cultivated plains of the Rhine, here thirty or forty miles wide. On almost every steep and projecting hill, or precipitous cliff, stands a ruined castle, each, as throughout Germany, with its wild history, its wilder traditions, and local associations of a hundred kinds. The railroad from Frankfort to Heidelberg now runs along the Bergstrasse, and will ever present to the eyes of travelers the charming aspect of these old legendary hills; till the enchanting valley of the Neckar, with Heidelberg reposing amid its lovely scenery at its mouth, terminates the Bergstrasse, and the hills which stretch onward, on the way toward Carlsruhe, assume another name.

Every one ascending the Rhine from Mayence to Mannheim has been struck with the beauty of these Odenwald hills, and has stood watching that tall white tower on the summit of one of them, which, with windings of the river, seem now brought near, and then again thrown very far off; seemed to watch and haunt you, and, for many hours, to take short cuts to meet you, till, at length, like a giant disappointed of his prey, it glided away into the gray distance, and was lost in the clouds. This is the tower of Melibocus, above the village of Auerbach, to which we shall presently ascend, in order to take our first survey of this old and secluded haunt of Odin.

In order to make ourselves somewhat acquainted with this interesting district, Mrs. Howitt and myself, with knapsack on back, set out at the end of August, 1841, to make a few days' ramble on foot through it. The weather, however, proved so intensely hot, and the electrical sultriness of the woods so oppressive, that we only footed it one day, when we were compelled to make use of a carriage, much to our regret.

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