34 rosMO?.have tlieir origin in analogous kinds of motion (currents). ],is reserved for future ages to make great discoveries in relerenceto <strong>the</strong>se subjects. Light, and radiating heat, whicliis inseparable from it, constitute a main cause of motion andorganic life, both in <strong>the</strong> non-luminous celestial bodies and on<strong>the</strong> surface of our planet.^ Even far from its surface, in<strong>the</strong> interior of <strong>the</strong> earth's crust, penetrating heat calls for<strong>the</strong>lectro-magnetic currents, which exert <strong>the</strong>ir exciting influenceon <strong>the</strong> combinations and decompositions of matter— onall formative agencies in <strong>the</strong> kingdom— mineral on <strong>the</strong> disturbanceof <strong>the</strong> equilibrium of <strong>the</strong> atmosp<strong>here</strong>— and on <strong>the</strong>functions of vegetable and animal organisms. If electricitymoving in currents develops magnetic forces, and if, in accordancewith an early hypo<strong>the</strong>sis of Sir William Herschel,t<strong>the</strong> sun itself is in <strong>the</strong> condition of " a perpetual nor<strong>the</strong>rnlight" (I should ra<strong>the</strong>r say of an electro-magnetic storm), weshould seem warranted in concluding that solar light, transmittedin <strong>the</strong> regions of space by vibrations of e<strong>the</strong>r, may beaccompanied by electro-magnetic currents.Direct observations on <strong>the</strong> periodic changes in <strong>the</strong> declination,inclination, and intensity of terrestrial magnetism,have, it is true, not yet shown with certainty that <strong>the</strong>se conditionsare affected by <strong>the</strong> different positions of <strong>the</strong> sun ormoon, notwithstanding <strong>the</strong> latter's contiguity to <strong>the</strong> earth.The magnetic polarity of <strong>the</strong> earth exhibits no variationsthat can be referred to <strong>the</strong> sun, or which perceptibly affect<strong>the</strong> precession of <strong>the</strong> equinoxes. | The remarkable rotatoryor oscillatory motion of <strong>the</strong> radiating cone of light of Halley'scomet, which Bessel observed from <strong>the</strong> 12th to <strong>the</strong> 22d ofOctober, 1835, and endeavored to explain, led this great astronomerto <strong>the</strong> conviction that <strong>the</strong>re existed a 2^olar force,* Comparelli.e fine pnssage on rne influence of <strong>the</strong> sun's raj^s in SirJolm Herscliei's Outlines of Astronomy, p. 237: " By <strong>the</strong> vivifying actionof tlie sun's rays, vegetables are enabled to draw su})port from inorganicmatter, and become, in tfjeir tuni, <strong>the</strong> support of animals andof man, and <strong>the</strong> sources of those great deposits of dynamical efficiencytehich are laid uj) for human vse in our strata. By <strong>the</strong>m <strong>the</strong> watersof <strong>the</strong> sea are made to circulate in vnp t through <strong>the</strong> air, and ini-coo^,gate <strong>the</strong> land, producing springs and rivers. By <strong>the</strong>m are producedi all disturbances of <strong>the</strong> chemical equilibrium of <strong>the</strong> elements of nature,which, by a series of compositions and decompositions, give rise to ne'ivproducts, and oi'iginatea transfer of materials."t Philos. Transact, for 17.9.5, vol. Ixxxv., p. 318 ;John Herschelj Outflines of Astr., p. 238; see also Cosmos, vol. i., p. 189.t <strong>See</strong> Bessel, in Schumacher's Asfr. Nackr., bd. xiii., 183G, No. 300B. 201.
RADIATING HEAT. 35*'whose action differed considerably from gravitation or <strong>the</strong>ordinary attracting force of <strong>the</strong> sun ;since those portions of<strong>the</strong> comet which constitute <strong>the</strong> tail are acted upon by a re'fuUive force proceeding from <strong>the</strong> body of <strong>the</strong> sun."'^ Thasplendid comet of 1744, which was described by Heinsius,led my deceased friend to similar conjectures.The actions of radiating heat in <strong>the</strong> regions of space areregarded as less problematical than electro-magnetic phenomena.According to Fourier and Poisson, <strong>the</strong> temperature of<strong>the</strong> regions of space is <strong>the</strong> result of radiation of heat from <strong>the</strong>sun and all astral bodies, minus <strong>the</strong> quantity lostby absorptionin traversing <strong>the</strong> regions of space filled with e<strong>the</strong>r. fFrequent mention is made in antiquity by <strong>the</strong> Greek andRoman! writers of this stellar heat ; not only because, froma universally prevalent assumption, <strong>the</strong> stars aj)pertained to<strong>the</strong> region of <strong>the</strong> fiery e<strong>the</strong>r, but because <strong>the</strong>y were supposedto be <strong>the</strong>mselves of a fiery nature§— <strong>the</strong> fixed stars and th(?sun being, according to <strong>the</strong> d£)ctrine of Aristarchus of Samos,of one and <strong>the</strong> same nature. In recent times, <strong>the</strong> observationsof <strong>the</strong> above-m.entioned eminent French ma<strong>the</strong>maticians,Fourier and Poisson, have been <strong>the</strong> means of directingattention to <strong>the</strong> average determination of <strong>the</strong> temperatureof <strong>the</strong> regions of space and <strong>the</strong> more;strongly since <strong>the</strong>importance of such determinations on account of <strong>the</strong> radiation of heat from <strong>the</strong> earth's surface toward <strong>the</strong> vault ofheaven has at length been appreciated in <strong>the</strong>ir relation toall <strong>the</strong>rmal conditions, and to <strong>the</strong> very habitability of ourplanet. According to Fourier's Analytic Theory of Heat,<strong>the</strong> temperature of celestial space {^des cspaccs planetairesou celestes)is ra,<strong>the</strong>r below <strong>the</strong> mean temperature of <strong>the</strong>poles, or even, perhaps, below <strong>the</strong> lowest degree of cold hi<strong>the</strong>rtoobserved in <strong>the</strong> polar regions. Fourier estimates it atfrom —58^ to --76° (from —40° to —48° Reaum.). The icypole {^pble glacial), or <strong>the</strong> point of <strong>the</strong> greatest cold, no more* Bessel, op. ciL, s. 186-192, 229.t Fourier, Th^orie Analytique de la Chaleur, 1822, p. ix. (Annalcide Chimie e.t de Physique, torn, iii., 1816, p. 350; torn, iv., 1817, p. 128;torn, vi., 1817, p. 259 ; torn, xiii., 1820, p. 418.) Poisson, in his TheoriiMath6matlque de la Chaleur (§ 196, p. 436, § 200, p. 447, and $ 228, p.521), attempts to give <strong>the</strong> numerical estimates of <strong>the</strong> stellar heat {cho'letcr stellaire) lost by absorption in <strong>the</strong> e<strong>the</strong>r of <strong>the</strong> regions of space.X On <strong>the</strong> heating power of <strong>the</strong> stars, see Aristot., De Meteor., 1, 3,p. 340, lin. 28 ;and on <strong>the</strong> elevation of <strong>the</strong> atmospheric strata at whidiheat is at <strong>the</strong> minimum, consult Seneca, in Nat. Qncrst., ii., 10: ' Siiperiora enim aeris calorem vicinorum siilerum sentiu'H,"^ riut., De plac. Ph»''os., ii ,13.
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- Page 13 and 14: INTRODUCTION. 7tiiieiital masses in
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VELOCITY OF L-'GIIT. fc'5refraction
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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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