Книга Narrative and Miscellaneous Papers — Volume 2 - читать онлайн бесплатно, автор Томас Де Квинси. Cтраница 2
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Narrative and Miscellaneous Papers — Volume 2
Narrative and Miscellaneous Papers — Volume 2
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Narrative and Miscellaneous Papers — Volume 2

But, if this sounds in the ear of some a doubtful refinement, the doubt applies only to the lowest degrees of space. For the highest, it is certain that brutes have no perception. To man is as much reserved the prerogative of perceiving space in its higher extensions, as of geometrically constructing the relations of space. And the brute is no more capable of apprehending abysses through his eye, than he can build upwards or can analyze downwards the ærial synthesis of Geometry. Such, therefore, as is space for the grandeur of man's perceptions, such as is space for the benefit of man's towering mathematic speculations, such is the nature of our debt to Lord Rosse—as being the philosopher who has most pushed back the frontiers of our conquests upon this exclusive inheritance of man. We have all heard of a king that, sitting on the sea-shore, bade the waves, as they began to lave his feet, upon their allegiance to retire. That was said not vainly or presumptuously, but in reproof of sycophantic courtiers. Now, however, we see in good earnest another man, wielding another kind of sceptre, and sitting upon the shores of infinity, that says to the ice which had frozen up our progress,—'Melt thou before my breath!' that says to the rebellious nebulæ,—'Submit, and burst into blazing worlds!' that says to the gates of darkness,—'Roll back, ye barriers, and no longer hide from us the infinities of God!'

'Come, and I will show you what is beautiful.'

From the days of infancy still lingers in my ears this opening of a prose hymn by a lady, then very celebrated, viz., the late Mrs. Barbauld. The hymn began by enticing some solitary infant into some silent garden, I believe, or some forest lawn; and the opening words were, 'Come, and I will show you what is beautiful!' Well, and what beside? There is nothing beside; oh, disappointed and therefore enraged reader; positively this is the sum-total of what I can recall from the wreck of years; and certainly it is not much. Even of Sappho, though time has made mere ducks and drakes of her lyrics, we have rather more spared to us than this. And yet this trifle, simple as you think it, this shred of a fragment, if the reader will believe me, still echoes with luxurious sweetness in my ears, from some unaccountable hide-and- seek of fugitive childish memories; just as a marine shell, if applied steadily to the ear, awakens (according to the fine image of Landor [Footnote: 'Of Landor,' viz., in his 'Gebir;' but also of Wordsworth in 'The Excursion.' And I must tell the reader, that a contest raged at one time as to the original property in this image, not much less keen than that between Neptune and Minerva, for the chancellorship of Athens.]) the great vision of the sea; places the listener

'In the sun's palace-porch, And murmurs as the ocean murmurs there.'

Now, on some moonless night, in some fitting condition of the atmosphere, if Lord Rosse would permit the reader and myself to walk into the front drawing-room of his telescope, then, in Mrs. Barbauld's words, slightly varied, I might say to him,—Come, and I will show you what is sublime! In fact, what I am going to lay before him, from Dr. Nichol's work, is, or at least would be, (when translated into Hebrew grandeur by the mighty telescope,) a step above even that object which some four-and-twenty years ago in the British Museum struck me as simply the sublimest sight which in this sight-seeing world I had seen. It was the Memnon's head, then recently brought from Egypt. I looked at it, as the reader must suppose, in order to understand the depth which I have here ascribed to the impression, not as a human but as a symbolic head; and what it symbolized to me were: 1. The peace which passeth all understanding. 2. The eternity which baffles and confounds all faculty of computation; the eternity which had been, the eternity which was to be. 3. The diffusive love, not such as rises and falls upon waves of life and mortality, not such as sinks and swells by undulations of time, but a procession—an emanation from some mystery of endless dawn. You durst not call it a smile that radiated from the lips; the radiation was too awful to clothe itself in adumbrations or memorials of flesh.

In that mode of sublimity, perhaps, I still adhere to my first opinion, that nothing so great was ever beheld. The atmosphere for this, for the Memnon, was the breathlessness which belongs to a saintly trance; the holy thing seemed to live by silence. But there is a picture, the pendant of the Memnon, there is a dreadful cartoon, from the gallery which has begun to open upon Lord Rosse's telescope, where the appropriate atmosphere for investing it must be drawn from another silence, from the frost and from the eternities of death. It is the famous nebula in the constellation of Orion; famous for the unexampled defiance with which it resisted all approaches from the most potent of former telescopes; famous for its frightful magnitude and for the frightful depth to which it is sunk in the abysses of the heavenly wilderness; famous just now for the submission with which it has begun to render up its secrets to the all-conquering telescope; and famous in all time coming for the horror of the regal phantasma which it has perfected to eyes of flesh. Had Milton's 'incestuous mother,' with her fleshless son, and with the warrior angel, his father, that led the rebellions of heaven, been suddenly unmasked by Lord Rosse's instrument, in these dreadful distances before which, simply as expressions of resistance, the mind of man shudders and recoils, there would have been nothing more appalling in the exposure; in fact, it would have been essentially the same exposure: the same expression of power in the detestable phantom, the same rebellion in the attitude, the same pomp of malice in the features to a universe seasoned for its assaults.

The reader must look to Dr. Nichol's book, at page 51, for the picture of this abominable apparition. But then, in order to see what I see, the obedient reader must do what I tell him to do. Let him therefore view the wretch upside down. If he neglects that simple direction, of course I don't answer for anything that follows: without any fault of mine, my description will be unintelligible. This inversion being made, the following is the dreadful creature that will then reveal itself.

Description of the Nebula in Orion, as forced to show out by Lord Rosse.—You see a head thrown back, and raising its face, (or eyes, if eyes it had,) in the very anguish of hatred, to some unknown heavens. What should be its skull wears what might be an Assyrian tiara, only ending behind in a floating train. This head rests upon a beautifully developed neck and throat. All power being given to the awful enemy, he is beautiful where he pleases, in order to point and envenom his ghostly ugliness. The mouth, in that stage of the apocalypse which Sir John Herschel was able to arrest in his eighteen- inch mirror, is amply developed. Brutalities unspeakable sit upon the upper lip, which is confluent with a snout; for separate nostrils there are none. Were it not for this one defect of nostrils; and, even in spite of this defect, (since, in so mysterious a mixture of the angelic and the brutal, we may suppose the sense of odor to work by some compensatory organ,) one is reminded by the phantom's attitude of a passage, ever memorable, in Milton: that passage, I mean, where Death first becomes aware, soon after the original trespass, of his own future empire over man. The 'meagre shadow' even smiles (for the first time and the last) on apprehending his own abominable bliss, by apprehending from afar the savor 'of mortal change on earth.'

——'Such a scent,' (he says,) 'I draw Of carnage, prey innumerable.'

As illustrating the attitude of the phantom in Orion, let the reader allow me to quote the tremendous passage:—

'So saying, with delight he snuff'd the smell Of mortal change on earth. As when a flock Of ravenous fowl, though many a league remote, Against the day of battle, to a field, Where armies lie encamp'd, come flying, lured With scent of living carcasses design'd For death, the following day, in bloody fight; So scented the grim feature, [Footnote: 'So scented the grim feature,' [feature is the old word for form or outline that is shadowy; and also for form (shadowy or not) which abstracts from the matter.] By the way, I have never seen it noticed, that Milton was indebted for the hint of this immortal passage to a superb line-and-a-half, in Lucan's Pharsalia.] and upturn'd His nostril wide into the murky air, Sagacious of his quarry from so far.'

But the lower lip, which is drawn inwards with the curve of a conch shell,—oh what a convolute of cruelty and revenge is there! Cruelty!—to whom? Revenge!—for what? Ask not, whisper not. Look upwards to other mysteries. In the very region of his temples, driving itself downwards into his cruel brain, and breaking the continuity of his diadem, is a horrid chasm, a ravine, a shaft, that many centuries would not traverse; and it is serrated on its posterior wall with a harrow that perhaps is partly hidden. From the anterior wall of this chasm rise, in vertical directions, two processes; one perpendicular, and rigid as a horn, the other streaming forward before some portentous breath. What these could be, seemed doubtful; but now, when further examinations by Sir John Herschel, at the Cape of Good Hope, have filled up the scattered outline with a rich umbrageous growth, one is inclined to regard them as the plumes of a sultan. Dressed he is, therefore, as well as armed. And finally comes Lord Rosse, that glorifies him with the jewellery [Footnote: The jewellery of Stars. And one thing is very remarkable, viz., that not only the stars justify this name of jewellery, as usual, by the life of their splendor, but also, in this case, by their arrangement. No jeweller could have set, or disposed with more art, the magnificent quadrille of stars which is placed immediately below the upright plume. There is also another, a truncated quadrille, wanting only the left hand star (or you might call it a bisected lozenge) placed on the diadem, but obliquely placed as regards the curve of that diadem. Two or three other arrangements are striking, though not equally so, both from their regularity and from their repeating each other, as the forms in a kaleidoscope.] of stars: he is now a vision 'to dream of, not to tell:' he is ready for the worship of those that are tormented in sleep: and the stages of his solemn uncovering by astronomy, first by Sir W. Herschel, secondly, by his son, and finally by Lord Rosse, is like the reversing of some heavenly doom, like the raising of the seals that had been sealed by the angel, in the Revelations. But the reader naturally asks, How does all this concern Lord Rosse's telescope on the one side, or general astronomy on the other? This nebula, he will say, seems a bad kind of fellow by your account; and of course it will not break my heart to hear, that he has had the conceit taken out of him. But in what way can that affect the pretensions of this new instrument; or, if it did, how can the character of the instrument affect the general condition of a science? Besides, is not the science a growth from very ancient times? With great respect for the Earl of Rosse, is it conceivable that he, or any man, by one hour's working the tackle of his new instrument, can have carried any stunning revolutionary effect into the heart of a section so ancient in our mathematical physics? But the reader is to consider, that the ruins made by Lord Rosse, are in sidereal astronomy, which is almost wholly a growth of modern times; and the particular part of it demolished by the new telescope, is almost exclusively the creation of the two Herschels, father and son. Laplace, it is true, adopted their views; and he transferred them to the particular service of our own planetary system. But he gave to them no new sanction, except what arises from showing that they would account for the appearances, as they present themselves to our experience at this day. That was a negative confirmation; by which I mean, that, had their views failed in the hands of Laplace, then they were proved to be false; but, not failing, they were not therefore proved to be true. It was like proving a gun; if the charge is insufficient, or if, in trying the strength of cast iron, timber, ropes, &c., the strain is not up to the rigor of the demand, you go away with perhaps a favorable impression as to the promises of the article; it has stood a moderate trial; it has stood all the trial that offered, which is always something; but you are still obliged to feel that, when the ultimate test is applied, smash may go the whole concern. Lord Rosse applied an ultimate test; and smash went the whole concern. Really I must have laughed, though all the world had been angry, when the shrieks and yells of expiring systems began to reverberate all the way from the belt of Orion; and positively at the very first broadside delivered from this huge four- decker of a telescope.

But what was it then that went to wreck? That is a thing more easy to ask than to answer. At least, for my own part, I complain that some vagueness hangs over all the accounts of the nebular hypothesis. However, in this place a brief sketch will suffice.

Herschel the elder, having greatly improved the telescope, began to observe with special attention a class of remarkable phenomena in the starry world hitherto unstudied, viz.: milky spots in various stages of diffusion. The nature of these appearances soon cleared itself up thus far, that generally they were found to be starry worlds, separated from ours by inconceivable distances, and in that way concealing at first their real nature. The whitish gleam was the mask conferred by the enormity of their remotion. This being so, it might have been supposed that, as was the faintness of these cloudy spots or nebulæ, such was the distance. But that did not follow: for in the treasury of nature it turned out that there were other resources for modifying the powers of distance, for muffling and unmuffling the voice of stars. Suppose a world at the distance x, which distance is so great as to make the manifestation of that world weak, milky, nebular. Now let the secret power that wields these awful orbs, push this world back to a double distance! that should naturally make it paler and more dilute than ever: and yet by compression, by deeper centralization, this effect shall be defeated; by forcing into far closer neighborhood the stars which compose this world, again it shall gleam out brighter when at 2_x_ than when at x. At this point of compression, let the great moulding power a second time push it back; and a second time it will grow faint. But once more let this world be tortured into closer compression, again let the screw be put upon it, and once again it shall shake off the oppression of distance as the dew-drops are shaken from a lion's mane. And thus in fact the mysterious architect plays at hide-and-seek with his worlds. 'I will hide it,' he says, 'and it shall be found again by man; I will withdraw it into distances that shall seem fabulous, and again it shall apparel itself in glorious light; a third time I will plunge it into aboriginal darkness, and upon the vision of man a third time it shall rise with a new epiphany.'

But, says the objector, there is no such world; there is no world that has thus been driven back, and depressed from one deep to a lower deep. Granted: but the same effect, an illustration of the same law, is produced equally, whether you take four worlds, all of the same magnitude, and plunge them simultaneously into four different abysses, sinking by graduated distances one below another, or take one world and plunge it to the same distances successively. So in Geology, when men talk of substances in different stages, or of transitional states, they do not mean that they have watched the same individual stratum or phenomenon, exhibiting states removed from each other by depths of many thousand years; how could they? but they have seen one stage in the case A, another stage in the case B. They take, for instance, three objects, the same (to use the technical language of logic) generically, though numerically different, under separate circumstances, or in different stages of advance. They are one object for logic, they are three for human convenience. So again it might seem impossible to give the history of a rose tree from infancy to age: how could the same rose tree, at the same time, be young and old? Yet by taking the different developments of its flowers, even as they hang on the same tree, from the earliest bud to the full- blown rose, you may in effect pursue this vegetable growth through all its stages: you have before you the bony blushing little rose-bud, and the respectable 'mediæval' full-blown rose.

This point settled, let it now be remarked, that Herschel's resources enabled him to unmask many of these nebulæ: stars they were, and stars he forced them to own themselves. Why should any decent world wear an alias? There was nothing, you know, to be ashamed of in being an honest cluster of stars. Indeed, they seemed to be sensible of this themselves, and they now yielded to the force of Herschel's arguments so far as to show themselves in the new character of nebulæ spangled with stars; these are the stellar nebulæ; quite as much as you could expect in so short a time: Rome was not built in a day: and one must have some respect to stellar feelings. It was noticed, however, that where a bright haze, and not a weak milk- and-water haze, had revealed itself to the telescope, this, arising from a case of compression, (as previously explained,) required very little increase of telescopic power to force him into a fuller confession. He made a clean breast of it. But at length came a dreadful anomaly. A 'nebula' in the constellation Andromeda turned restive: another in Orion, I grieve to say it, still more so. I confine myself to the latter. A very low power sufficed to bring him to a slight confession, which in fact amounted to nothing; the very highest would not persuade him to show a star. 'Just one,' said some coaxing person; 'we'll be satisfied with only one.' But no: he would not. He was hardened, 'he wouldn't split.' And Herschel was thus led, after waiting as long as flesh and blood could wait, to infer two classes of nebulæ; one that were stars; and another that were not stars, nor ever were meant to be stars. Yet that was premature: he found at last, that, though not raised to the peerage of stars, finally they would be so: they were the matter of stars; and by gradual condensation would become suns, whose atmosphere, by a similar process of condensing, would become planets, capable of brilliant literati and philosophers, in several volumes octavo. So stood the case for a long time; it was settled to the satisfaction of Europe that there were two classes of nebulæ, one that were worlds, one that were not, but only the pabulum of future worlds. Silence arose. A voice was heard, 'Let there be Lord Rosse!' and immediately his telescope walked into Orion; destroyed the supposed matter of stars; but, in return, created immeasurable worlds.

As a hint for apprehending the delicacy and difficulty of the process in sidereal astronomy, let the inexperienced reader figure to himself these separate cases of perplexity: 1st, A perplexity where the dilemma arises from the collision between magnitude and distance:—is the size less, or the distance greater? 2dly, Where the dilemma arises between motions, a motion in ourselves doubtfully confounded with a motion in some external body; or, 3dly, Where it arises between possible positions of an object: is it a real proximity that we see between two stars, or simply an apparent proximity from lying in the same visual line, though in far other depths of space? As regards the first dilemma, we may suppose two laws, A and B, absolutely in contradiction, laid down at starting: A, that all fixed stars are precisely at the same distance; in this case every difference in the apparent magnitude will indicate a corresponding difference in the real magnitude, and will measure that difference. B, that all the fixed stars are precisely of the same magnitude; in which case, every variety in the size will indicate a corresponding difference in the distance, and will measure that difference. Nor could we imagine any exception to these inferences from A or from B, whichever of the two were assumed, unless through optical laws that might not equally affect objects under different circumstances; I mean, for instance, that might suffer a disturbance as applied under hypoth. B, to different depths in space, or under hypoth. A, to different arrangements of structure in the star. But thirdly, it is certain, that neither A nor B is the abiding law: and next it becomes an object by science and by instruments to distinguish more readily and more certainly between the cases where the distance has degraded the size, and the cases where the size being really less, has caused an exaggeration of the distance: or again, where the size being really less, yet co-operating with a distance really greater, may degrade the estimate, (though travelling in a right direction,) below the truth; or again where the size being really less, yet counteracted by a distance also less, may equally disturb the truth of human measurements, and so on.

A second large order of equivocating appearances will arise,—not as to magnitude, but as to motion. If it could be a safe assumption, that the system to which our planet is attached were absolutely fixed and motionless, except as regards its own internal relations of movement, then every change outside of us, every motion that the registers of astronomy had established, would be objective and not subjective. It would be safe to pronounce at once that it was a motion in the object contemplated, not in the subject contemplating. Or, reversely, if it were safe to assume as a universal law, that no motion was possible in the starry heavens, then every change of relations in space, between ourselves and them, would indicate and would measure a progress, or regress, on the part of our solar system, in certain known directions. But now, because it is not safe to rest in either assumption, the range of possibilities for which science has to provide, is enlarged; the immediate difficulties are multiplied; but with the result (as in the former case) of reversionally expanding the powers, and consequently the facilities, lodged both in the science and in the arts ministerial to the science. Thus, in the constellation Cygnus, there is a star gradually changing its relation to our system, whose distance from ourselves (as Dr. Nichol tells us) is ascertained to be about six hundred and seventy thousand times our own distance from the sun: that is, neglecting minute accuracy, about six hundred and seventy thousand stages of one hundred million miles each. This point being known, it falls within the arts of astronomy to translate this apparent angular motion into miles; and presuming this change of relation to be not in the star, but really in ourselves, we may deduce the velocity of our course, we may enter into our log daily the rate at which our whole solar system is running. Bessel, it seems, the eminent astronomer who died lately, computed this velocity to be such (viz., three times that of our own earth in its proper orbit) as would carry us to the star in forty-one thousand years. But, in the mean time, the astronomer is to hold in reserve some small share of his attention, some trifle of a side-glance, now and then, to the possibility of an error, after all, in the main assumption: he must watch the indications, if any such should arise, that not ourselves, but the star in Cygnus, is the real party concerned, in drifting at this shocking rate, with no prospect of coming to an anchorage. [Footnote: It is worth adding at this point, whilst the reader remembers without effort the numbers, viz., forty-one thousand years, for the time, (the space being our own distance from the sun repeated six hundred and seventy thousand times,) what would be the time required for reaching, in the body, that distance to which Lord Rosse's six feet mirror has so recently extended our vision. The time would be, as Dr. Nichol computes, about two hundred and fifty millions of years, supposing that our rate of travelling was about three times that of our earth in its orbit. Now, as the velocity is assumed to be the same in both cases, the ratio between the distance (already so tremendous) of Bessel's 61 Cygni, and that of Lord Rosse's farthest frontier, is as forty- one thousand to two hundred and fifty millions. This is a simple rule- of-three problem for a child. And the answer to it will, perhaps, convey the simplest expression of the superhuman power lodged in the new telescope:—as is the ratio of forty-one thousand to two hundred and fifty million, so is the ratio of our own distance from the sun multiplied by six hundred and seventy thousand, to the outermost limit of Lord Rosse's sidereal vision.]