36 COSMOS.corresponds with <strong>the</strong> terrestrial pole than does <strong>the</strong> <strong>the</strong>rmaleqitator, which connects toge<strong>the</strong>r <strong>the</strong> hottest points of allmeridians with <strong>the</strong> geographical equator. Arago concludes,from <strong>the</strong> gradual decrease of mean temperatures, thit <strong>the</strong>degree of cold at <strong>the</strong> nor<strong>the</strong>rn terrestrial pole is — 13^, if <strong>the</strong>maximum cold observed by Captain Back at Fort Rehance(62° 46' lat.) in Januar}^ 1834, w^ere actually —70° (—56^-6Cent., or — 45°-3 K-eaum.).^ The lowest temperature that,as far as we know, has as yet been observed on <strong>the</strong> earth, isprobably that noted by Neveroff, at Jakutsk (62° 2' lat.),on <strong>the</strong> 21st of January, 1838. The instruments used inthis observation were compared with his own by Middendorff,whose operations w^ere always conducted with extreme exactitude.Neveroff found <strong>the</strong> temperature on <strong>the</strong> day abovenamed to be — 76° (or— 48° Reaum.).Among <strong>the</strong> many grounds of uncertainty in obtaining anumerical result for <strong>the</strong> <strong>the</strong>rmal condition of <strong>the</strong> regions ofspace, must be reckoned that of our inability at present toascertain <strong>the</strong> mean of <strong>the</strong> temperatures of <strong>the</strong> poles of greatestcold of <strong>the</strong> two hemisp<strong>here</strong>s, owing to our insufficient acquaintance wdth <strong>the</strong> meteorology of <strong>the</strong> antarctic pole, fromwhich <strong>the</strong> mean annual temperature must be determined. Iattach but little physical probability to <strong>the</strong> hypo<strong>the</strong>sis of Poisson,that <strong>the</strong> different regions of space must have a very varioustemperature, owing to <strong>the</strong> unequal distribution of heatradiatmgstars, and that <strong>the</strong> earth, daringits motion with <strong>the</strong>* Arago, Snr la Tempiralure du Pole et des espaces Cilestes, in <strong>the</strong>Annuaire du Bureau des Long, jwnr 1825, p. 189, et pour 1834, p. 192;also Saigey, Physique du Globe, 1832, p. 60-76. Svvauberg found, fromconsiderations on refraction, that <strong>the</strong> temperature of <strong>the</strong> regions of spacewas — .58^.5. — Berzelius, Jahresbericht fur 1830, s. 54. Arago,— frompolar observations, fixed it at 70^ ; and Pectet at — 76°. Saigey, bycalculating <strong>the</strong> decrease of heat in <strong>the</strong> atmosp<strong>here</strong>, from 367 observationsmade by myself in <strong>the</strong> chain of <strong>the</strong> Andes and in Mexico, found it— 85°; and from <strong>the</strong>rmometrical measurements made — at Mont Blanc,and dui-ing <strong>the</strong> aeronautic ascent of Gay-Lussac, 107°-2. Sir JohnHorschel (Edinburgh Review, vol. 87, 1848, p. 223) gives it at —132°.We feel considerable surprisf ,and have our faith in <strong>the</strong> correctness of<strong>the</strong> methods hi<strong>the</strong>rto adopted somewhat shaken, when we find thatPoisson, notwithstanding that <strong>the</strong> mean temperature of Melville Island—(74° 47' N. lat.) is 1° 66', gives <strong>the</strong> mean temperature of <strong>the</strong> regionsof space at only 8°'6, having obtained his data from purely <strong>the</strong>oreticalpremises, according to which <strong>the</strong> regions of space are wai'mer than thaouter limits of <strong>the</strong> atmosp<strong>here</strong> (see <strong>the</strong> work already referred to, $ 227,p. .520) while Pouillet Stales ; it, from actinometric experiments, to ba•IS low as — 223^0. <strong>See</strong> Comptes Rcndus de VAcademic des Sciences.u,m vii., 1838 p. 25-65.
TEMPERATURE OF SPACE. 37whole solar system, receives its interna, heat from withoutwhile passing through hot and cold regions.*The question whe<strong>the</strong>r <strong>the</strong> <strong>the</strong>rmal conditions of <strong>the</strong> celestialregions, and <strong>the</strong> climates of individual portions of space,have sujSered important variations in <strong>the</strong> course of ages, depends mainly on <strong>the</strong> solution of a prohlem warmly discussedS^irby Wihiam Herschel : whe<strong>the</strong>r <strong>the</strong> nebulous masses aresubjected to progressive processes of formation, while <strong>the</strong> cosrriicalvapor is being condensed around one or more nuclei inaccordance "with <strong>the</strong> laws of attraction ?By such a condensationof cosmical vaiJor, heat must be liberated, as inevery transition of gases and fluids into a state of solidification.!If, in accordance with <strong>the</strong> most recent views, and<strong>the</strong> important observations of Lord R.osse and Mr. Bond, wemay assume that all nebulas, iiicluding those which <strong>the</strong> highestpower of optical instruments has hi<strong>the</strong>rto failed in resolving,are closely crowded stellar swarms, our faith in tliis perpetuallyaugmenting liberation of heat must necessarily bein some degree weakened. But even small consolidated cosmicalbodies Avhich appear on <strong>the</strong> field of <strong>the</strong> telescope asdistinguishable luminous points, may change <strong>the</strong>ir densityby combining in larger masses and ; many phenomena presentedby our own planetary system lead to <strong>the</strong> conclusionthat planets have been soUdified from a sfate of vapor, andthat <strong>the</strong>ir internal heat owes its origin to <strong>the</strong> fomiative processof conglomerated matter.Itmayat first sight seem hazardous to term <strong>the</strong> fearfullylow temperature of <strong>the</strong> regions of space (which varies between<strong>the</strong> freezing point of mercury and that of spirits ofwine) even indirectly henejicialto <strong>the</strong> habitable climates of<strong>the</strong> earth and to animal and vegetablelife. But in proof of<strong>the</strong> accuracy of <strong>the</strong> expression, we need only refer to <strong>the</strong> actionof <strong>the</strong> radiation of heat. The sun-warmed surface ofour planet, as well as <strong>the</strong> atmosp<strong>here</strong> to its outermost strata,freely radiate heat into space. The loss of heat which <strong>the</strong>yexperience arises from <strong>the</strong> difference of temperature between<strong>the</strong> vault of heaven and <strong>the</strong> atmospheric strata, and from <strong>the</strong>feebleness of tlie counter-radiation. How enormous wouldl?3 this loss of heat,$ if <strong>the</strong> regions of space,instead of <strong>the</strong>* <strong>See</strong> Poisson, ThioHe Mathim. de la Chalenr, p. 438.Accordingto him, <strong>the</strong> consolidation of <strong>the</strong> earth's strata began from <strong>the</strong> center, andadvanced gradually toward <strong>the</strong> surface; 'J 193, p. 429. Compare alsoCosmos, vol. i., p. 176, 177. t Cosmos, vol. i., p. 83, 84, 144.X" Were <strong>the</strong>re no atmosp<strong>here</strong>, a thcrmonietor freely exposed (at suit
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- Page 13 and 14: INTRODUCTION. 7tiiieiital masses in
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VELOCITY OF ELECTRICITY. STbe satis
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STELLAR LIGHT. 81)to such views bec
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MAGNITUDES OF STARSDir;40 stars of
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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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