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ments and periods of binary systems, which now I have happened among the fired stars since the time form the most interesting portion of sidereal as- of Mr. Flamstead." In this paper, he notices, 1. tronomy.

The stars that have been lost, or undergone some To us who are in possession of the researches capital change since Flamstead's time; 2. Those on double stars, which we owe to Mr. Herschel that have changed their magnitude ; 3. Those that and his son, to Sir James South, and M. Struve, have newly become visible ; and the results which it is interesting to mark the first steps in this great he obtained were drawn from a review of all the inquiry.

stars in Flamstead's catalogue, as far as the twelfth “ I took pains,” says Mr. Herschel, “ to find out

magnitude, "to the amount of a great many thou-
what double stars had been recorded by astrono- sands of stars." Those changes which arise from
mers; but my situation permitted me not to consult a proper motion of the star, and a variation of
extensive libraries, nor indeed was it very material. magnitude, he suspects may be owing to every
For as I intended to view the heavens myself, Na- star in the heavens being more or less in motion ;
ture—that great volume—appeared to me to contain some, especially in slow motions, arising from
the best catalogue upon this occasion. However, their revolving round a large oparrue body—the
I remembered that the star in the head of Castor,
that in the breast of the Virgin, and the first star in stars undergoing occasional occultation, or present-
Aries, had been mentioned by Cassini as double ing to us large spots in their rotatory movements.
stars. I also found that the nebula in Orion was Hence he is led to believe, what Tobias Mayer had
marked in Huygens' Systema Saturnium as contain previously maintained, that the Sun and Solar
ing seven stars, three of which (now known to be System have analogous motions, and are advanc-

four) are very near together. With this small
stock I began, and, in the course of a few years' ing to a certain part of the heavens ; and he found
observations, have collected the stars contained in that this part was in the constellation Hercules,
my catalogue. I find, with great pleasure, that a

near the star 2, or a point somewhat further to the
very excellent observer, (Mr. Pigott,) has also, north.
though unknown to me, met with three of those Having finished, in the year 1783, a very good
stars that will be found in my catalogue; and upon twenty-feet reflector, with a large aperture, he em-
this occasion, I also beg leave to observe, that the ployed it in studying the remarkable luminous spots
astronomer-royal showed me, among other objects, at the pole of the planet Mars ; and he published
« Hercules as a double star, which he had discov-
ered some years ago. The Rev. Mr. Hornsby also, the results of his observations in the Philosophical
in a conversation on the subject of the stars that Transactions of 1784. By means of these spots,
have a proper motion, mentioned a Bootis as a he found that the axis of Mars was inclined to the
double star. It is a little hard upon young astrono- ecliptic 59° 42', and that its node was in 17° 47'
mers to be obliged to discover over again what has of Pisces, and he determined the ratio of its polar
already been discovered. However, the pleasure and equatorial diameters to be as 15 to 16.
that attended the view when I first saw these stars,

Towards the end of 1784, Mr. Herschel comhas made some amends for not knowing they had been seen before me.'

pleted a second catalogue, containing 434 double

stars; and in June, 1784, and February, 1785, he Mr. Herschel's first Catalogue of Double Stars communicated to the Royal Society two papers “On was read at the Royal Society on the 10th January, the Construction of the Heavens.” By means of 1787. It contains 269 double stars, 227 of which his twenty feet telescope, with an aperture of 1870 had not been noticed by any other person. It inches, and placed meridionally, he resolved into gives the comparative size of the stars, their color, stars the nebulæ discovered by Messier and Mechain, their distances, (as measured by a Lamp Microme- and also part of the Milky Way; and he discovered ter,t exhibiting two movable lights, with whose no fewer than 466 new nebulæ and clusters of stars, distance seen by the unassisted eye the distance of which were not within the reach of the best comthe stars seen in the telescope was compared,) mon telescopes then in use. In pursuing these their angle of position, and the dates of the obser- observations, he was led to the remarkable specuvation. The catalogue, which is divided into six lation, founded wholly on optical considerations, classes, contains not only double stars, but also that as the Milky Way" seemed to encompass the those that are triple, double-double, quadruple, whole heavens,” it might be regarded as an imdouble-triple, and multiple.

mense cluster of stars; and that our sun, with his Mr. Herschel had now removed to Datchet, near system .of planets, was in all probability placed Windsor, where he carried on his observations within it, but “ perhaps not in the very centre of under the immediate patronage of the king, with its thickness." In order to determine the sun's new zeal and corresponding success.

Towards

place in this sidereal stratum, he gaged the hearens, the end of 1782, he completed his interesting paper or ascertained the quantity of stars, or the thick-“On the proper motion of the Sun and the Solar ness of the stratum, in various directions. In his System, with an account of several changes that paper of 1785, he gives a long table of star-gages ;

* After his catalogue was in the possession of the Royal and supposing the stars to be nearly equally scatSociety, Mr. Herschel received the fourth volume of the tered, and their numbers in a field of view of a Acta Academiæ Theodoro-Palatinæ, containing a paper by Tobias Mayer, giving "a pretty large list of double known angular diameter to be given, he determines stars,” some of which were the same with those in his the length of the visual ray, and gives a section catalogue, while 31 were not contained in it. + Described in the Philosophical Transactions, 1782, of the Milky Way, or nebulæ, (resembling a fish

with a long open mouth,) to which our system be

P. 163.

longs, and near the centre of which it is placed. I not been confirmed by subsequent observers. The We regret that we cannot allow ourselves to adopt nebular hypothesis to which they led, and which this noble and ingenious speculation ;* and there is has been carried to such an unwarrantable extent sufficient evidence to induce us to believe, as the in our own day, has been refuted by the discoveries celebrated Russian astronomer, M. F. G. W. of the Earl of Rosse ; and there is reason to beStruve, has stated, that Mr. Herschel himself was lieve that it has been renounced by Sir John Herobliged to abandon it. He found, even with his schel himself.* largest telescope, that the Milky Way could not be The interesting subject of the Construction of sounded; and as the same uncertainty prevails the Heavens was pursued by Dr. Herschel during respecting the limits of the visible stars in all other the rest of his life, and his observations are recorded directions of the celestial vault, M. Struve draws in ten memoirs published in the Philosophical the conclusion, that “if we regard all the fixed Transactions for 1791, 1794, 1796, 1799, 1802, stars that surround the sun as fôrming a great sys- 1806, 1811, 1814, 1817, and 1818. tem—that of the Milky Way- —we are perfectly ig- Having already, in other articles, given an acnorant of its extent, and cannot form the least idea count of the great 40 feet telescope constructed by of this immense system.'t Having, therefore, no Dr. Herschel, and of the various discoveries which visible limits, it cannot be regarded as a nebula, he made respecting the planets and satellites of our according to the hypothesis of Mr. Herschel. But own system,f we must bring to a close this brief nothough the Milky Way is a system whose form and tice of his sidereal labors. In the year 1816, when extent is not, and probably never will be, deter- in the 79th year of his age, the prince regent premined, yet, as Struve observes, there is evidently sented him with the decoration of the Guelphic a certain law of condensation towards a principal order of knighthood. In 1820, he was elected presplane, which law he has endeavored to determine. ident of the Astronomical Society, and in their TransLambert had imagined that the deviation of the actions, in 1821, he published an interesting memoir Milky Way from the form of a great circle, was on the places of 145 double stars. This paper was owing to the lateral position of the sun within it. the last which he lived to publish. His health had M. Struve, however, rejects this explanation, and begun to decline, and on the 24th August, 1822, is of opinion that the most condensed stratum of he sank under the infirmities of age, having comthe stars does not form a perfect plane, but rather pleted his 84th year. He was survived by his a broken plane, (plan brisé,) or perhaps this stra- widow Lady Herschel, by his sister Miss Caroline tum occurs in two planes inclined 10° to each other, Herschel, and by an only son, the present Sir and whose intersection is placed nearly in the plane John Herschel, whose labors and discoveries in of the celestial equator, the sun being at a small sidereal astronomy we shall now proceed to lay bedistance from this line of intersection towards the fore our readers. point 13 h. of the equator.

After the death of his father, Sir John Herschel In 1786 Dr. Herschel, who had been honored had directed his attention principally to the science with the degree of Doctor of Laws from the Uni- of opties, but particularly to that branch of it which versity of Oxford, communicated to the Royal Soci- relates to the double refraction and polarization of ety a catalogue of 1000 new nebulæ and clusters of light. In this research, he obtained many new stars, which he had observed since 1783, with his and highly important results, which are recorded twenty-feet reflector; and this was followed, in in his Treatise on Light, published in the Encyclo1789, with another catalogue of a second thousand pædia Metropolitana, and certainly one of the most nebula. In these remarkable memoirs he regards valuable works on that subject which has ever been the round clusters and nebulæ, in which there is written. Astronomy, however, had a higher claim an apparent condensation towards a centre, as upon his genius ; and having inherited telescopes clusters or nebulæ in the act of formation. He of great magnitude and power, and been initiated supposes that a central power resides in the brightest into the difficult art of constructing them, he was portion ; that the clusters which have the most per- naturally led to quit the field of optical science, and fect spherical forms have been longest exposed to to cultivate the loftier domain of sidereal astronomy. the action of these forces; and that we may judge He had proposed to himself the arduous task of of the relative age and maturity of a sidereal sys- reëxamining the nebulæ and clusters of stars which tem from the disposition of its component parts ; had been discovered by his father in his “ sweeps while what he calls planetary nebulæ, where the of the heavens,” and recorded in the three catacompression is more equal, may be regarded as very logues which, as we have already seen, he preaged, and approaching to a period of change or dis- sented to the Royal Society in the years 1786, 1787, solution.

1802, and he began to execute it in the year 1925. These views, ingenious thongh they be, have In this reëxamination he spent eight years, and he

has given the results of it in a catalogne published * See review of Kosmos No. vii, pp. 228-30. in the Philosophical Transactions for 1832. This

+ In his memoirs of 1811 and 18:7, Mr. Herschel aban, dons altogether his postulate of the equal distribution of * North British Review, No. VI., p. 477, and No. stars in space.

VIII., p. 490. # Eludes d'Astronomie Stellaire, par F. G. W. Struve. + North British Review, No. mi., pp. 183-189 ; Nn. St. Petersbourg, 1847. p. 63.

VII., Art. yiii passim, and No. xl., Art. viii. passim, $ Etudes d'Astronomie Stellaire, par F. G. W. Struve. * Miss Caroline Herschel died at Hanover on the 9th St. Petersbourg, 1847. p. 82.

of January, in the 98th year of her age.

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catalogue contains 2306 nebulæ and clusters of Iquired than in England, was performed by himstars, of which 1781 are identical with those de- self with the requisite apparatus, which he had scribed by his father, and with those published by fortunately brought with him from England. Messier and Struve. The number of new nebulæ In the use of reflecting specula of considerable and clusters discovered by himself was 525. Dur- weight, it is of the utmost importance that the ing this reëxamination, he observed a great num- metal should be supported in its case so as not to ber of double stars, and took their places, to the suffer any change of figure from its own weight. amount of between three and four thousand, all of Sir John found that a speculum was totally spoiled which are described in the second, third, fourth, by allowing it to rest horizontally on three metallic sixth, and ninth volumes of the memoirs of the points at its circumference. The image of every Astronomical Society of London.

considerable star became triangular, throwing out These observations were made with a Newtonian long flaming caustics at the angles. Having on telescope of 20 feet focus, and 184 inches aperture, one occasion supported the speculum simply ayainst and having acquired by practice a "sufficient mas- a flat-board, at an elevation of about 45°, he found tery of the instrument,” and “ of the delicate that its performance was tolerably good ; but on process of polishing the specula,” he conceived the stretching a thin pack-thread vertically down the noble idea of attempting to complete the survey of middle of the board, so as to bring the weight of the whole surface of the heavens; and, with this the metal to rest upon this thread, the images of view, of “ transporting into the other hemisphere stars were lengthened horizontally “ to a preposthe same instrument which had been employed in terous extent, and all distinct vision utterly dethis, so as to give a unity to the results of both stroyed by the division of the mirror into two lobes, portions of the survey, and to render them com- each retaining something of its parabolic figure, parable with each other."

separated by a vertical band in a state of distortion, The Cape of Good Hope was selected as the and of no figure at all !” The method which Sir most favorable locality for carrying on this survey ; John found the best was the following :-Between and having fitted up the instruments and packed the mirror and the back of the case he interposed them carefully for the voyage, he left England, 6 or 8 folds of thick woollen baize, or blanketing, with his family, on the 13th November, 1833, and of uniform thickness and texture, stitched together landed at Capetown on the 16th January, 1834, at their edges. The metal, when laid flat on this having providentially escaped from an awful hurri- bed, was shaken so as to be concentric with the cane to which he would have been exposed had rim of the case, and two supports, composed of his voyage been delayed. The spot which Sir several strips of similar baize, were introduced so John selected was the grounds and mansion of a as to occupy about 30° each, and to leave an arc Dutch proprietor, the name of which was Feldhau- of about 40° unoccupied opposite the point which

a spot charmingly situated on the eastern was to be the lowermost in the tube. When the side of the last gentle slope at the base of the Ta- case is raised into an inclined position, and slightly ble Mountain.” During the erection of the instru- shaken, the mirror takes its own free bearing on ments, Sir John resided at Welterfrieden, and so these supports, and preserves its figure. It is esquickly were his plans completed, that on the 22d sential, however, to the successful application of of February, 1834, he was enabled to gratify his this method that many thicknesses of the baize or curiosity by viewing, with his 20 feet reflector, a blanket should be employed, " by which only the Crucis, the interesting nebula about n Argus, and effect of flexure in the wooden back itself of the other remarkable objects ; and on the evening of case can be eliminated.” As the woollen fibres, the 5th March, to begin a regular series of obser- however, lose their elasticity, the baize should be vations. The observatory thus completed was occasionally taken out, and beaten or shaken up.* situated in south lat. 33° 58' 56 55', and long. 22° In conducting his observations with these fine 46'9".11 east from Greenwich, and its altitude instruments, Sir John Herschel observed several was 142 feet above the level of the sea in Table curious optical effects, arising from peculiar conBay.

ditions of the atmosphere, incident to the climate After erecting his observatory, and determining of the Cape. In the hot season, from October tr its geographical position, the attention of Sir John March, but particularly during the latter months Herschel was directed to the preparation of the of that season, “ the nights are for the most part telescopes with which his observations were to be superb" at a few miles distance from the mounmade. He carried out with him three specula, tains ; but occasionally during the excessive heat one of which was made by his father, and used by and dryness of the sandy plains, the “optical tranhim in his 20 feet sweeps and other observations ; quillity of the air” is greatly disturbed. In some another was made by Sir John, under his father's cases the images of the stars are violently dilated inspection and instructions; and the other, of the into nebular balls or puffs of upwards of 15' in very same metal as the last, was ground and figured diameter. At the end of March, 1834, for examby himself. They had all a clear diameter of 181 ple, when Saturn and y Virginis were both in the inches of polished surface, and were all equally re- * When Sir John adopted this very simple plan, he flective when freshly polished, and perfectly sim- was ignorant of the very ingenious method by which ilar in their performance. The operation of re- lum, and which we have already described in this jour

Lord Rosse affords an equable support to a large specupolishing, which was much more frequently re-Inal, vol. ii., p. 207.

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field of the 20 feet reflector, “ it could not have In studying the polarization of the atmosphere, been told which was the planet and which the the writer of this article has had occasion frestar." On other occasions, the stars form “ soft, quently to observe what appears to be the result quiet, round pellets of 3' or 4' diameter,” resem- of the same cause. When the sky was of a fine bling planetary nebulæ, and quite unlike the spu- blue color, and free from clouds, and the degree rious discs which they present when not defined. of polarization, as indicated by the polarimeter, ** In other cases, these pellets are seen to arise from very great, a sudden change frequently took place "an infinitely rapid vibratory movement of the without any apparent cause ; sometimes near the central point in all possible directions,” the lumi- horizon and not at considerable altitudes, and somenous discs presenting singular phenomena when times at considerable altitudes and not near the thrown out of focus, by pushing the eye-piece horizon. On some occasions the effect was limfurther in or pulling it further out than its princi- ited in its extent, and of a temporary kind. pal focus.*

When it was not temporary, it showed itself in a In the cooler months, from May to October, diminution of the blue tint of the sky, which is and especially in June and July, the state of the invariably' accompanied with a diminished polariair is habitually good, and after heavy rains have zation, and the whiteness of the sky often inceased for a day or two, the tranquillity of the creased till clouds were produced, terminating in image and the sharpness of vision, is such that rain. The cause of these phenomena was doubthardly any limit is set to magnifying power, but less 'a sudden secretion of aqueous vapor, somethat which arises from the aberration of the spec- times of local and of limited extent, and quickly ula. On occasions like these, optical phenomena reabsorbed ; and at other times general, and terof extraordinary splendor are produced by view- minating in a change of weather. When a cloud ing a bright star through diaphragms of card-board passed over a track of perfectly blue sky, without or zinc, pierced in regular patterns of circular occasioning any perceptible diminution of tint, the holes by machinery. These phenomena, arising polarization of the part of the sky over which it from the interferences of the intromitted rays, and passed was always diminished, owing, no doubt, produced less perfectly in a moderate state of the to its having left in its path a quantity of aqueous air, surprise and delight every person that sees vapor. them. A result of a more valuable kind is ob- The description of phenomena, and the tabutained when the aperture of the telescope has the lated observations contained in the interesting form of an equilateral triangle, the centre of which volume now before us, occupy seven chapters, coincides with the centre of the speculum. When extending over 450 closely printed pages, and are close double stars are viewed with the telescope, illustrated with seventeen beautifully executed having a diaphragm of this form, the discs of the plates, some of which are of a very great size. two stars, which are exact circles, are reduced to The valuable contents of these different chapters about a third of their size, and have a clearness would doubtless have appeared in a series of unand perfection almost incredible. These discs, connected memoirs in the transactions of the however, are accompanied with six luminous radi- Royal or Astronomical Societies, and with illusations, running from them at angles of 60°, form- trations very inferior, both in number and quality, ing perfectly straight, delicate, brilliant lines, like had it not been for the munificence of his grace brightly illuminated threads, running far out be- the late Duke of Northumberland, who destined yond the field of view, and, what is singular, a large sum for their publication as a single and capable of being followed like real appendages to separate work. This very amiable and publicthe star long after the star itself has left the field. spirited nobleman, to whom the observatory of

Another optical phenomenon, arising from a Cambridge owes the gift of the splendid Northpeculiar condition of the atmosphere, is described umberland achromatic telescope, through which by Sir John Herschel as a "nebulous haze.” the new planet Neptune was first seen, did not The effect of it is to encircle every star, of the live to witness the final fulfilment of his noble and 9th magnitude and upwards, with a faint sphere generous design ; but the present duke, the worof light of an extent proportioned to the bright- thy heir of the titles and the fortune of that disness of the star. This phenomenon presents tinguished nobleman, carried out, in the fullest itself very suddenly in a perfectly clear sky, free manner, the liberal intentions of his lamented from the slightest suspicion of cloud, and disap- brother, and thus added another claim to those pears as suddenly, lasting sometimes only for one which, as Lord Prudhoe, he had already earned, or two minutes. Sir John Herschel states that upon the gratitude and esteem of the literary and similar nebular affections occur in our English cli- scientific world. mate, but with much less frequency and sudden- The following are the subjects which are treated ness in their appearance and disappearance. He in the volume under our notice :at first suspected that the phenomenon arose from Chap. I. On the nebulæ and clusters of stars dew upon the eye-piece, but repeated examination in the southern hemisphere. satisfied him that its origin was really atmospheric.

* For an account of the polarization of the atmosphere, * Sir John snpposes that these phenomena may be pro- the reader is referred to Johnston and Berghaus Physical duced by ascending and descending currents or hot and Atlas, part vii., and London and Edinburgh Philosophicold air rotating spirally.

cal Magazine, December, 1847. Vol. xxi., pp. 441-466.

No.

Right Ascension.

North Po.ar Distance.

No, of stara laid down in the drawing.

II. On the double stars of the southern hem-time ruddy or orange yellow,) forming a fine conisphere.

trast with the white light of the exterior portion. III. Of astronomy, or the numerical expression There is a beautiful double star on the south preof the apparent magnitude of stars.

ceding edge of the last portion, but it is probably IV. Of the distribution of stars, and of the unconnected with the cluster. constitution of the galaxy, or Milky Way, in the Under the favorable circumstances in which he southern hemisphere.

was placed, our author eagerly availed himself of V. Observations of Halley's Comet, with re- the opportunity of studying the grand nebula in the marks on its physical condition, and that of comets sword-handle of Orion, which passed the meridian in general.

of the Cape at an altitude of 60°. He had himVI. Observations on the Satellites of Saturn. self delineated this remarkable nebula in 1824 : VII. Observations on the Solar spots.

Four representations of it, differing essentially from In the first chapter, on nebulæ and clusters of his, had been subsequently published ; and it therestars, occupying 164 pages, our author proceeds, fore became an object of the deepest interest to after some introductory and explanatory remarks, discover the causes of these discrepancies, and to to give detailed descriptions and monographs of ascertain whether or not a change had taken place some of the more remarkable of the nebulæ. As either in the form or luminosity of the whole some of these nebulæ are visible in Europe, and nebula, or of any of its parts. Dr. Lamont of are all objects of singular interest, we shall lay Munich, had, in 1837, published " rather a coarsely before our readers a very brief notice of the most executed figure” of this nebula, but Sir John Herimportant of them.

schel acknowledges that it “contains some valuable particulars respecting the apparent breaking up

of the nebula into patches and knots," which had 1. 18h 11 106° 15'

44 2 17 52 113 1

27

been very unsatisfactorily expressed in his figure 3 5 27

94 57

26

of 1824, but “ in which his observations of 1834 4 5 40 159 11

105 and 1837, fully confirm Dr. Lamont's remarks." 5 17 53 27" 114 21 16" 186 The other drawings, by Sig. Derico, and Sig. 6 12 43 36 149 25 41 110

Rondoni, published in 1839, 1840 and 1841, are 7 0 16 24 163 1 58

too inaccurate to furnish any materials for specuNo. 1. This remarkable nebula, which is a lation. nebular line, with the figure of a horse-shoe at The splendid drawing of this nebula, which each end of it, has been observed and drawn by occupies a foot square, and forms the eighth plate Mr. Mason, an American astronomer, and Mr. La of the present work, is one of the noblest specimont, a native of Scotland, who has the charge of mens of astronomical research which is to be found the observatory at Munich. Mr. Mason, whose in the history of the science. We view it at first premature death is deeply to be regretted, used a with mute admiration of the skill and patience of reflecting telescope of 12 inches aperture, and 14 the observer, and even forget for a while the mysfeet focal length, constructed by himself. The terious assemblage of suns and of systems which fainter horse-shoe was seen neither by Mr. Mason it sets before us. No fewer than 150 stars are nor Mr. Lamont.

accurately laid down in this remarkable map, and No. 2. This nebula has also been figured by our failing vision can scarcely descry the faint Mr. Mason, and in this as well as in No. 1, his luminosity with which it shades away into the dark representation differs from that of Sir John Her- sky that encloses it. Neither in its general outschel.

line, nor in that of its individual portions, has it No. 4 is, in the author's opinion, one of the the least resemblance to any form natural or artimost singular and extraordinary objects which the ficial. The luminous portions have no relation heavens present. It is situated in the greater either in shape or intensity to the stars which benubecula of the Magellanic clouds.

spangle it, and the stars themselves, whether we No. 6. This cluster of stars, improperly set consider their magnitude or their distances, seem down as nebular by Lacaille, is, according to our to have no bond of union, and no symmetry of author, an extremely brilliant and beautiful ob- place. Knowing, as we now do, that Lord Rosse's ject, when viewed through an instrument of suffi- telescope has resolved the nebulous portion into cient aperture to show distinctly the very different stars, we can no longer satisfy ourselves with the colors of its constituent stars, which give it the speculation that the nebula is a collection of mineffect of a superb piece of fancy jewelry." Three utely subdivided matter, accidentally irregular in of the stars are greenish white, two green, one its outline and density, which may some time or blue green, one red, and another ruddy.

other be combined into stars and planets, but we No. 7, (47 Toucani,) is a most magnificent view it as a mighty galaxy of systems already globular cluster. The stars are immensely numer- formed, of suns radiant with light and heat, of ous and compressed. It is compared to a blaze worlds in harmonious revolution, teeming with orof light at the centre, the stars seeming to run ganic life, and rich with the bounties of their beneftogether. Sir John Herschel has observed the icent Creator. But even with these views the extraordinary fact that the inner or compressed mind does not rest satisfied. It seeks to know part of the cluster is rose-colored, (at another how these systems are combined in the irregular

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