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perfectly noticeable by our instruments. existed in greater quantity upon one side than upon another, it would have the general effect of making that side darker, and the revolution of the sun must, in such a case, give us a brighter and a fainter side, by regular alternations. Now, there are some of the fixed stars which present this appearance. They present us with periodical variations of light. From the splendour of a star of the first or second magnitude, they fade away into some of the inferior magnitudes-and one, by becoming invisible might give reason to apprehend that we had lost him altogether-but we can still recognize him by the telescope, till at length he re-appears in his own place, and, after a regular lapse of so many days and hours, recovers his original brightness. Now, the fair inference from this is, that the fixed stars, as they resemble our sun in being so many luminous masses of immense magnitude, they resemble him in this also, that each of them turns round upon his own axis; so that if any of them should have an inequality in the brightness of their sides, this revolution is rendered evident, by the regular variations in the degree of light which it undergoes.

Shall we say, then, of these vast luminaries, that they were created in vain? Were they called into existence for no other purpose than to throw a tide of useless splendour over the solitudes of immensity? Our sun is only one of these luminaries, and we know that he has worlds. in his train. Why should we strip the rest of this princely attendance? Why may not each of them be the centre of his own system, and give light to his own worlds? It is true that we see them not, but could the eye of man take its flight into those distant regions, it should lose sight of our little world, before it reached the outer limits of our system-the greater planets should disappear in their turn-before it had described a small portion of that

abyss which separates us from the fixed stars, the sun should decline into a little spot, and all its splendid retinue of worlds be lost in the obscurity of distance-he should, at last, shrink into a small indivisible atom, and all that could be seen of this magnificent system, should be reduced to the glimmering of a little star. Why resist any longer the grand and interesting conclusion? Each of these stars may be the token of a system as vast and as splendid as the one which we inhabit. Worlds roll in these distant regions; and these worlds must be the mansions of life and intelligence. In yon gilded canopy of heaven we see the broad aspect of the universe, where each shining point presents us with a sun, and each sun with a system of worlds-where the Divinity reigns in all the grandeur of his attributes-where he peoples immensity with his wonders; and travels in the greatness of his strength through the dominions of one vast and unlimited monarchy.

The contemplation has no limits. If we ask the number of suns and of systems, the unassisted eye of man can take in a thousand, and the best telescope which the genius of man has constructed can take in eighty millions. But why subject the dominions of the universe to the eye of man, or to the powers of his genius? Fancy may take its flight far beyond the ken of eye or of telescope. It may expiate in the outer regions of all that is visibleand shall we have the boldness to say, that there is nothing there? that the wonders of the Almighty are at an end, because we can no longer trace his footsteps? that his omnipotence is exhausted, because human art can no longer follow him? that the creative energy of God has sunk into repose, because the imagination is enfeebled by the magnitude of its efforts, and can keep no longer on the wing through those mighty tracts, which shoot far beyond what eye bath seen, or the heart of man hath con

ceived-which sweep endlessly along, and merge into an awful and mysterious infinity?

Before bringing to a close this rapid and imperfect sketch of our modern astronomy, it may be right to advert to two points of interesting speculation, both of which serve to magnify our conceptions of the universe, and, of course, to give us a more affecting sense of the comparative insignificance of this our world. The first is suggested by the consideration, that, if a body be struck in the direction of its centre, it obtains, from this course, a progressive motion, but without any movement of revolution being at the same time impressed upon it. It simply goes forward, but does not turn round upon itself. But, again, should the stroke not be in the direction of the centreshould the line which joins the point of percussion to the centre, make an angle with that line in which the impulse was communicated, then the body is both made to go forward in space, and also to wheel upon its axis. In this way, each of our planets may have had their compound motion communicated to it by one single impulse; and, on the other hand, if ever the rotatory motion be communicated by one blow, then the progressive motion must go along with it. In order to have the first motion without the second, there must be a twofold force applied to the body in opposite directions. It must be set agoing in the same way as a spinning-top, so as to revolve about an axis, and to keep unchanged its situation in space. The planets have both motions; and, therefore, may have received them by one and the same impulse. The sun, we are certain, has one of these motions. He has a movement of revolution. If spun round his axis by two opposite forces, one on each side of him, he may have this movement, and retain an inflexible position in space. But, if this movement was given him by one stroke, he must have a progressive motion, along with a whirling motion ;

or, in other words, he is moving forward; he is describing a tract in space; and, in so doing, he carries all his planets and all their secondaries along with him.

But at this stage of the argument, the matter only remains a conjectural point of speculation. The sun may have had his rotation impressed upon him by a spinning impulse; or, without recurring to secondary causes at all, this movement may be coeval with his being, and he may have derived both the one and the other from an immediate fiat of the Creator. But, there is an actually observed phenomenon of the heavens, which advances the conjecture into a probability. In the course of ages, the stars in one quarter of the celestial sphere are apparently receding from each other; and in the opposite quarter, they are apparently drawing nearer to each other. If the sun be approaching the former quarter, and receding from the latter, this phenomenon admits of an easy explanation, and we are furnished with a magnificent step in the scale of the Creator's workmanship. In the same manner as the planets, with their satellites, revolve round the sun, may the sun, with all his tributaries, be moving, in common with other stars, around some distant centre, from which there emanates an influence to bind and to subordinate them all. They may be kept from approaching each other, by a centrifugal force; without which, the laws of attraction might consolidate, into one stupendous mass, all the distinct globes of which the universe is composed. Our sun may, therefore, be only one member of a higher family-taking his part, along with millions of others, in some loftier system of mechanism, by which they are all subjected to one law, and to one arrangement-describing the sweep of such an orbit in space, and completing the mighty revolution in such a period of time, as to reduce our planetary seasons and our planetary movements, to a very humble and fractionary rank in the scale of a high

er astronomy. There is room for all this in immensity; and there is even argument for all this, in the records of actual observation; and, from the whole of this speculation, do we gather a new emphasis to the lesson, how minute is the place, and how secondary is the importance of our world, amid the glories of such a surrounding magnificence!

But, there is still another very interesting tract of speculation, which has been opened up to us by the more recent observations of astronomy. What we allude to, is the discovery of the nebulo. We allow that it is but a dim and indistinct light which this discovery has thrown upon the structure of the universe; but still it has spread before the eye of the mind a field of very wide and lofty contemplation. Anterior to this discovery, the universe might appear to have been composed of an indefinite number of suns, about equi-distant from each other, uniformly scattered over space, and each encompassed by such a planetary attendance as takes place in our own system. But, we have now reason to think, that, instead of lying uniformly, and in a state of equi-distance from each other, they are arranged into distinct clusters-that, in the same manner as the distance of the nearest fixed stars, so inconceivably superior to that of our planets from each other, marks the separation of the solar systems, so the distance of two contiguous clusters may be so inconceivably superior to the reciprocal distance of those fixed stars, which belong to the same cluster, as to mark an equally distinct separation of the clusters, and to constitute each of them an individual member of some higher and more extended arrangement. This carries us upwards through another ascending step in the scale of magnificence, and there leaves us wildering in the uncertainty, whether even here the wonderful progression is ended; and at all events fixes the assured conclusion in our minds, that, to an eye which could spread itself over the whole, the mansion

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