42 COSMOS.The perfectionin <strong>the</strong> graduation of <strong>the</strong> arc would have failedentirely, or to a considerable extent, in affording that greaterprecision of observation at vv^hich it aimed, if optical andastronomical instruments had not been brought into accord,and <strong>the</strong> correctness of vision made to correspond with thatof measurem 3nt. The micrometer-application of fine tlu'eadsstretched in <strong>the</strong> focus of <strong>the</strong> telescope, to wliich that instrumentowes its real and invaluable importance, was first devised,six years afterward (1640), by <strong>the</strong> young and talentedGascoigne.^While, as I have already observed, telescopic vision, observation,and measurement extend only over a period ofabout 240 years in <strong>the</strong> history of astronomical science, wefind, without including <strong>the</strong> epoch of <strong>the</strong> Chaldeans, Egyptians,and Chinese, that more than nineteen centuries haveintervened between <strong>the</strong> age of Timochares and Aristillusfand <strong>the</strong> discoveries of Galileo, during which period <strong>the</strong> positionand cou^Tse of <strong>the</strong> stars were observed by <strong>the</strong> eye alone,unaided by instruments. AYhen we consider <strong>the</strong> numerousdisturbances which, during this prolonged period, checked <strong>the</strong>advance of cwilization, and <strong>the</strong> extension of <strong>the</strong> sp<strong>here</strong> ofideas among *,he nations inhabiting <strong>the</strong> basin of <strong>the</strong> Mediterranean,\y** are astonished that Hipparchus and Ptolemyshould have been so well acquainted with <strong>the</strong> precession of<strong>the</strong> equinoxes., <strong>the</strong> complicated naovements of <strong>the</strong> planets, <strong>the</strong>two principal inequalities of <strong>the</strong> moon, and <strong>the</strong> position of <strong>the</strong>stars ;that Copernicus should have had so great a knowledgeof <strong>the</strong> true Fystem of <strong>the</strong> universe and that ;Tycho Braheshould have been so familiar with <strong>the</strong> methods of practicalastronomy b-?fore <strong>the</strong> discovery of <strong>the</strong> telescope. Long tubes,272. Mfniu, ia his work, Scientia Longitudinum, which appeared in1G34, v/lritea .t^ follows: Applicatlo tuhi optlci ad alliidadam pro dellisfixis p-^ompte et accurate mensurandis a me excogitata est. Picard hadnot, up to <strong>the</strong> year 1667, employed any telescope on <strong>the</strong> mural circle:and Hevelius, when Halley visited him at Dantzic in 1679, and admiredtha precision of his measurement of altitudes, was observing throughImproved slits or * openings. (Baily's Catal. of Sfars, p. 38.)The unfortunate Gascoigue, whose merits remained so long unacknowledged,lost his life, when scarcely twenty-three years of age, at<strong>the</strong> battle of Marston Moor, fought by Cromwell against <strong>the</strong> Royalists.<strong>See</strong> Derham, in <strong>the</strong> Philos. Transact., vol. xxx., for 1717-1719, p. 603-610. To him belongs <strong>the</strong> merit of a discovery which was long ascribedto Picard and Auzout, and which has given an impulse previously unknownto practical astronomy, <strong>the</strong> principal object of which is to determinepoii4ions in <strong>the</strong> vault of heaven.t Cosmos, vol. ii., p. 177, ITS.
DIOPTRIC TUBES. 43wliich were certainly employed by Arabian astronomers, andvery probably also by <strong>the</strong> Greeks and Romans, may indeed,in some degree, liave increased <strong>the</strong> exactness of <strong>the</strong> observationsby causing <strong>the</strong> object to be seen througli diopters or slits.Abul-Hassan speaks very distinctly of tubes, to <strong>the</strong> extremitiesof which ocular and object diopters were attached ;andinstruments so constructed were used in <strong>the</strong> observatoiyfounded by Hulagu at Meragha. If stars be more easilydiscovered during twilight by means of tubes, and if a starbe sooner revealed to <strong>the</strong> naked eye through a tube thanwithout it, <strong>the</strong> reason lies, as Arago has already observed, in<strong>the</strong> circumstance that <strong>the</strong> tube conceals a great portion of <strong>the</strong>disturbing light {rayons 'pertiirhateurs^ diilused in <strong>the</strong> atmospheric strata between <strong>the</strong> star and <strong>the</strong> eye apphed to <strong>the</strong> tube.In like mamier, <strong>the</strong> tube prevents <strong>the</strong> lateral impression of <strong>the</strong>faint hght which <strong>the</strong> particles of air receive at night from all<strong>the</strong> o<strong>the</strong>r stars in <strong>the</strong> fimiament. The intensity of <strong>the</strong> imagoand <strong>the</strong> size of <strong>the</strong> star are apparently augmented. In a freqrjntly emendated and much contested passage of Strabo, inwhich mention is made of locking througli tubes, this " enlargedfomi of <strong>the</strong> stars" is expressly mentioned, and is erroneouslyascribed to refraction.'^* The passage in which Strabo (lib. iii., p. 138, Casaub.) atteni[)ts lorffute <strong>the</strong> views of Posidoiiius is given as follows, according to <strong>the</strong>manuscripts: ''The image of <strong>the</strong> sun is enlarged on <strong>the</strong> seas at its risingas well as at its setting, because at <strong>the</strong>se times a larger mass of exhalationsrises from <strong>the</strong> humid element; and <strong>the</strong> eye, looking through<strong>the</strong>se exhalations, sees images refracted into larger forms, as observedthroiigh tubes. The same thing happens when <strong>the</strong> setting sun or mo""!is seen throu£;h a dry and thin cloud, when those bodies likewise appea.reddish." This passage has recently been pronounced corrupt (seeKramer, in Strahonis Geogi:, 1844, vol. i., p. 211), and 61 vu/mv (throughglass sp<strong>here</strong>s) substituted for 61 av?iuv (Schneider, Eclog. Phys., vol. ii.,p. 273). The magnilying power of hollow glass sp<strong>here</strong>s, tilled withwater (Seneca, i., 6), was, indeed, as familiar to <strong>the</strong> ancients as <strong>the</strong> actionof burning-glasses or crystals (Aristoph., Nub., v. 765), and that ofNero's emerald (Plin., xxxvii., 5);but <strong>the</strong>se sp<strong>here</strong>s most assuredlycould not have been employed as astronomical measuring instruments,(Compare Cosmos, vol. ii., p. 245, and note %•) Solar altitudes, takenthrough thin, light clouds, or through volcanic vapors, exhibit no tracecf <strong>the</strong> influence of refraction. (Humboldt, Recueil d^Observ. Asir., vol.i-, p. 123.) Colonel Baeyer observed no angular deviation in <strong>the</strong> heliotropeon <strong>the</strong> ligii'. passage of streaks of mist, or even from artificially
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ilOTOMETRIC METHODS. 1)3ing (in fro
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HOTOMETR'i'. 95Sir Jolin Herscliel
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PHOTOMETRY. 97his own words, the re
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PHOTOMETRIC SCALE. 99raoTOMi:TRic a
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PHOTOMETRIC SCALE. 101Stars of the
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tt.i.rfUMBER, DISTRIBUTION, AND COL
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NUMBER OF THE FIXED STARS. iOlHersc
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NUMliER OF TUB FIXED STARS. 101Tst
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NUMBER OF THE FIXED STARS. 109Star
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EARLY CATA'.OGUES. Illthat of Tycho
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PROGRESS OF ASTRONOMY. 113the labor
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STAR CATALOGUES 115La Caille, Tobia
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DISTRIBUTION OF THE FIXED STARS. 11
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ZODIACAL SIGNS. 119groups the for.n
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i,ODlACAL SIGNS. 121passage, pDjbaW
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AcliillesTHE FIXED STARS 123to tlio
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THE FIXED STARS. 123idea of transpa
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VELOCITY OF LIGHT.IS'/tne eye,diflr
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RAYS OF THE STARS. 12Switli a needl
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COLOU OF THE STARS. 131ifiope, ill
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SIRIU3. 133gjini,who invariably fol
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THE COLOR OF THE STARS 135Btars, St
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SOUTHERN STARS.ISTEentatioiis of De
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DISTRIBUTION OF STARS.13Sbeen made
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CLUSTERS OF STARS. 141tail of Scorj
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CLUSTERS OF STAR3. 143of Cambridge,
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MILKY WAY. 145be asciibed to irreso
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MILKY WA /. 147tioii of the souther
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MILKY WAY. 149of Ceplieus, and ther
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NEW STARS. 151ft1rat\im. is about e
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A^VV STARS. 153diminisii,. and the
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etweenTEMPORARY STARS. 155transitio
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TEMPORARY STARS.It>'/{g) March, 393
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TEMPORARY STARS. 159excitt
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N£VV STARS 161aetic process in the
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VANISHED STARS.1G3bricius as sudden
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PERIODICAL STARS. 165with uniform i
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VARIABLE STARS. 167That the periods
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VARIABLE STARS. 169perioJs of the m
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VARIABLE STARS. 171have loDg' appea
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VARIABLE STARS.17Jright ascension a
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VARIABLE STARS. 175The Huctaations,
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VARIABLE STARS. 11^lU brightuess at
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VARIABLE STARS. 179to the observati
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VARIABLE STARS. 181served by liLn.
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PROPER MOTION OF THE STARS. 183cuns
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_PROPER iMOTION OF THE STARS. If 5t
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PROPER MOTION OF THE STARS. 187A la
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DISTANCES OF THE STARS.Ibllniibsima
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DISTANCES OF THE STARS.19Jfiords, "
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Fixed Star.DISTANCES OF THE STARS.
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PROPER MOTION OF THE STARS. . 195li
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MOTION OF THE STARS. 197question na
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DOUBLE STARS. 199not the place to d
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OOUBLL STARS. 201distnnce from each
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DOUBLE &TAR3. 203The importance of
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DOUBLE STARS20ldation of this impor
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DOUBLE STARS 20*7most recent gives
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DOUBLE STARS.!2USstances In which a
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DOUBLE STARS.21 JOrion, we have a c
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DOUBLE STARS.213Elements ofthe Orbi
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neINDEX.Cosiiiical vnpor, question
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218 INDEX./^i-nerical rcctilta exce
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