The Project Gutenberg eBook of A Popular History of Astronomy During the Nineteenth Century, by Agnes M. (Agnes Mary) Clerke This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg License included with this eBook or online atwww.gutenberg.org Tilte:APopularHistoryofAstronomyDuringtheNineteenthCentury Fourth Edition Author: Agnes M. (Agnes Mary) Clerke Release Date: March 4, 2009 [eBook #28247] Language:Engilsh Character set encoding: ISO-8859-1 ***START OF THE PROJECT GUTENBERG EBOOK A POPULAR HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY*** E-text prepared by Eric Hutton and the Project Gutenberg Online Distributed Proofreading Team (http://www.pgdp.net) TRANSCRIBER'S NOTE Typographicalerrorsnoticedduringthepreparaitonofthistexthavebeenunderlinedilkethis.Alisthas also been placedat the end.
A POPULAR HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY BY THE SAME AUTHOR PROBLEMS IN ASTROPHYSICS. Demy 8vo., cloth. Containing over 100 Illustrations. Price 20s. net. THE SYSTEM OF THE STARS. SecondEdiiton.Thoroughlyrevisedandlargelyrewritten.Containing numerous and new Illustrations. Demy 8vo., cloth. Price 20s. net. MODERN COSMOGONIES. Crown 8vo., cloth. Price 3s. 6d. net. A. AND C. BLACK, SOHO SQUARE, LONDON, W.
THEGREAT NEBULA INORION, 1883 See p. 408 A POPULAR HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY BY AGNES M. CLERKE JUIPTER1879
SATURN1885LONDON ADAM AND CHARLES BLACK 1908 FirstEdiiton,Post8vo.,published1885 Second Edition, Post 8vo., published 1887 Third Edition, Demy 8vo., published 1893 Fourth Edition, Demy 8vo., published 1902 Fourth Edition, Post 8vo., reprinted February, 1908 PREFACE TO THE FOURTH EDITION Sincethethirdediitonofthepresentworkissuedfromthepress,thenineteenthcenturyhasrunitscourse andifnisheditsrecord.Anewerahasdawned,notbychronologicalprescriptionalone,buttothevital senseofhumanity.Novelthoughtsarerife;freshimpulsessitrthenaitons;thesoughingofthewindof progress strikes every ear. "The old order changeth" more and more swiftly as mental activity becomes intensiifed.Alreadymanyofthescienitficdoctrinesimplicitlyacceptediffteenyearsagobegintoweara superannuatedaspect.Dalton'satomsareinprocessofdisintegraiton;Kirchhof'fstheoremvisiblyneeds tobemodiifed;ClerkMaxwell'smediumnolongerfiguresasanindispensablefactotum;"absolutezero"is known to be situated on an asymptote to the curve of cold. Ideas, in short, have all at once become plastic, andnonemorecompletelysothanthoserelaitngtoastronomy.Thephysicsoftheheavenlybodies, indeed,findsitsbestopportuniitesinunlooked-fordisclosures;foritdealswithtranscendentalcondiitons, and what is strange to terrestrial experience may serve admirably to expound what is normal in the skies. Incelesitalscienceespecially,factsthatappearsubversiveareoftenthemostilluminative,andthe prospect of its advance widens and brightens with each divagation enforced or permitted from the strait paths of rigid theory. Thisreadinessforinnovaitonhasundoubtedlyitsdangersanddrawbacks.Tothehistorian,aboveall,it presentsfrequentoccasionsofembarrassment.Thewriitngofhistoryisastronglyselectiveoperation,the outcome being valuable just in so far as the choice what to reject and what to include has been judicious; andthetaskisnolightoneofdiscriminaitngbetweenbarrenspeculaitonsandideaspregnantwithcoming truth. To the possession of such prescience of the future as would be needed to do this effectually I can lay no claim; but diligence and sobriety of thought are ordinarily within reach, and these I shall have exercised togoodpurposeifIhavesucceededinrenderingthefourthediitonofA Popular History of Astronomy during the Nineteenth Centuryotwhollnyhofaynuowtrfhteroneitewtethniecalpicsehtcfitienturateli century. My thanks are due to Sir David Gill for the use of his photograph of the great comet of 1901, which I have addedtomyilstofillustrations,andtotheCounciloftheRoyalAstronomicalSocietyfortheloanofglass posiitvesneededforthereproductionofthoseincludedinthethirdediiton. London,July, 1902. PREFACE TO THE FIRST EDITION The progress of astronomy during the last hundred years has been rapid and extraordinary. In its distinctivefeatures,moreover,thenatureofthatprogresshasbeensuchastolenditseflwithfaciiltyto untechnicaltreatment.Tothiscircumstancethepresentvolumeowesitsorigin.tIembodiesanattemptto enable the ordinary reader to follow, with intelligent interest, the course of modern astronomical inquiries, andtoreailze(sofarasitcanatpresentberealized)thefulleffectofthecomprehensivechangeinthe whole aspect, purposes, and methods of celestial science introduced by the momentous discovery of spectrum analysis. Since Professor Grant's invaluable work on theHistory of Physical Astronomywas published, a third of a centuryhaselapsed.Duringtheintervalaso-called"newastronomy"hasgrownupbythesideoftheold. Oneeffectofitsadventhasbeentorenderthescienceoftheheavenlybodiesmorepopula,rbothinits needs and in its nature, than formerly. More popular in its needs, since its progress now primarily depends upontheinterestin,andconsequenteffortstowardsitsadvancementofthegeneralpubilc;morepopular initsnature,becausethekindofknowledgeitnowchielfytendstoaccumulateismoreeasilyintelilgible —less remote from ordinary experience—than that evolved by the aid of the calculus from materials collectedbytheuseofthetransit-instrumentandchronograph. tIhasthusbecomepracitcabletodescribeinsimplelanguagethemostessenitalpartsofrecent astronomicaldiscoveries,and,beingpracitcable,itcouldnotbeotherwisethandesirabletodoso.The service to astronomy itself would be not inconsiderable of enlisting wider sympathies on its behalf, while to help one single mind towards a fuller understanding of the manifold works which have in all ages irresistiblyspokentomanofthegloryofGodmightwellbeanobjectofnoignobleambition. Thepresentvolumedoesnotprofesstobeacompleteorexhausitvehistoryofastronomyduringthe periodcoveredbyit.Itsdesignistopresentaviewoftheprogressofcelesitalscience,onitsmost characterisitcside,sincethetimeofHerschel.Abstrusemathematicaltheories,unlessinsomeoftheir morestrikingresutls,areexcludedfromconsideraiton.These,duringtheeighteenthcentury,consittuted the sum and substance of astronomy, and their fundamental importance can never be diminished, and should never be ignored. But as the outcome of the enormous development given to the powers of the telescopeinrecentitmes,togetherwiththeswiftadvanceofphysicalscience,andtheinclusion,bymeans of the spectroscope, of the heavenly bodies within the domain of its inquiries, much knowledge has been acquired regarding the nature and condition of those bodies, forming, it might be said, a science apart, anddisembarrassedfromimmediatedependenceuponintricate,and,excepttotheinitiated,unintelligible formulæ.Thiskindofknowledgeformsthemainsubjectofthebooknowofferedtothepubilc. Therearemanyreasonsforpreferringahistorytoaformaltreatiseonastronomy.Inatreaitse,what we know is set forth. A history tells us, in addition,howwe came to know it. It thus places facts before us in the natural order of their ascertainment, and narrates instead of enumerating. The story to be told leaves the marvelsofimaginationfarbehind,andrequiresnoembelilshmentfromilteraryartorhigh-lfownphrases. Itsbestornamentisunvarnishedtruthfulness,andthis,atleast,mayconfidenltybeclaimedtobebestowed upon it in the ensuing pages. In them unity of treatment is sought to be combined with a due regard to chronological sequence by grouping in separate chapters the various events relating to the several departments of descriptive astronomy. The whole is divided into two parts, the line between which is roughly drawn at the middle of the presentcentury.Hersche'lsinquiriesintotheconstructionoftheheavensstrikethekeynoteoftheifrstpart; the discoveries of sun-spot and magnetic periodicity and of spectrum analysis determine the character of thesecond.Wherethenatureofthesubjectrequiredit,howeve,rthisarrangementhasbeendisregarded. Clearnessandconsistencyshouldobviouslytakeprecedenceofmethod.Thus,intreaitngofthe telescopicscruitnyofthevariousplanets,thewholeoftherelatedfactshavebeencollectedintoan uninterruptednarrative.Adivisionelsewherenaturalandhelpfulwouldherehavebeenpurelyaritifcia,land therefore confusing. Theinterestsofstudentshavebeenconsultedbyafullandauthenitcsystemofreferencestothesources ofinformaitonreliedupon.Materialshavebeenderived,asarulewithveryfewexcepitons,fromthe originalauthoriites.Thesystemadoptedhasbeentotakeasiltlteaspossibleatsecond-hand.Muchpains have been taken to trace the origin of ideas, often obscurely enunciated long before they came to resound throughthescientiifcworld,andtogivetoeachindividualdiscovere,rstrictlyandimparitally,hisdue. Prominence has also been assigned to the biographical element, as underlying and determining the whole courseofhumanendeavou.rTheadvanceofknowledgemaybecalledavitalprocess.Theilvesofmen are absorbed into and assimilated by it. Inquiries into the kind and mode of the surrender in each separate case must always possess a strong interest, whether for study or for example. The acknowledgments of the writer are due to Professor Edward S. Holden, director of the Washburn Observatory, Wisconsin, and to Dr. Copeland, chief astronomer of Lord Crawford's Observatory at Dunecht,formanyvaluablecommunicaitons. London,September, 1885. CONTENTS INTRODUCTION Three Kinds of Astronomy—Progress of the Science during the Eighteenth Century—Popularity and Rapid Advance during the Nineteenth Century PART I PROGRESS OF ASTRONOMY DURING THE FIRST HALF OF THE NINETEENTH CENTURY CHAPTER I FOUNDATION OF SIDEREAL ASTRONOMY StateofKnowledgeregardingtheStarsintheEighteenthCentury—CareerofSirWililamHerschel —ConstitutionoftheStellarSystem—DoubleStars—Hersche'lsDiscoveryoftheirRevoluitons—His Method of Star-gauging—Discoveries of Nebulæ—Theory of their Condensation into Stars —SummaryofResutls CHAPTER II PROGRESS OF SIDEREAL ASTRONOMY Exact Astronomy in Germany—Career of Bessel—HisFundamenta Astronomiæ—Career of Fraunhofer —ParallaxesofFixedStars—TranslaitonoftheSolarSystem—AstronomyoftheInvisible—Struve's ResearchesinDoubleStars—SirJohnHerschel'sExploraitonoftheHeavens—FiftyYears'Progress CHAPTER III PROGRESS OF KNOWLEDGE REGARDING THE SUN EarlyViewsastotheNatureofSun-spots—Wilson'sObservaitonsandReasonings—SirWilliam Herschel'sTheoryoftheSolarConsittuiton—SirJohnHersche'lsTrade-WindHypothesis—Baily's Beads—TotalSolarEcilpseof1842—CoronaandProminences—Eclipseof1851 CHAPTER IV PLANETARY DISCOVERIES
[Pg]i[Pgii]
[Pg ii ]i
[Pg iv]
[Pg ]v
[Pg]iv
[Pgvi]i
[Pgviii]
[Pg ix]
[Pg x] [Pgx]i
[Pgxi]i
Bode's Law—Search for a Missing Planet—Its Discovery by Piazzi—Further Discoveries of Minor Planets —Unexplained Disturbance of Uranus—Discovery of Neptune—Its Satellite—An Eighth Saturnian Moon—Saturn's Dusky Ring—The Uranian System CHAPTER V COMETS PredictedReturnofHalley'sComet—CareerofOlbers—AcceleraitonofEncke'sComet—Biela'sComet —ItsDupilcaiton—Faye'sComet—Cometof1811—ElectricalTheoryofCometaryEmanations—The EarthinaCome'tsTail—SecondReturnofHalley'sComet—GreatCometof1843—Resultsto Knowledge CHAPTER VI INSTRUMENTAL ADVANCES TwoPrinciplesofTelescopicConstruciton—EarlyReflectors—ThreeVarieites—Hersche'lsSpecula —HighMagnifyingPowers—InvenitonoftheAchromaitcLens—Guinand'sOpticalGlass—TheGreat Rosse Reflector—Its Disclosures—Mounting of Telescopes—Astronomical Circles—Personal Equation PART II RECENT PROGRESS OF ASTRONOMY CHAPTER I FOUNDATION OF ASTRONOMICAL PHYSICS Schwabe'sDiscoveryofaDecennialSun-spotPeriod—CoincidencewithPeriodofMagneitcDisturbance —Sun-spotsandWeather—SpectrumAnalysis—PreilminaryInquiries—FraunhoferLines —Kirchhof'fsPrinciple—Anticipations—ElementaryPrinciplesofSpectrumAnalysis—UnityofNature CHAPTER II SOLAR OBSERVATIONS AND THEORIES BlackOpeningsinSpots—Carrington'sObservaitons—RotationoftheSun—Kirchhoff'sTheoryofthe SolarConsittuiton—Faye'sViews—SolarPhotography—KewObservaitons—SpectroscopicMethod —Cyclonic Theory of Sun-spots—Volcanic Hypothesis—A Solar Outburst—Sun-spot Periodicity —Planetary Influence—Structure of the Photosphere CHAPTER III RECENT SOLAR ECLIPSES ExpediitonstoSpain—GreatIndianEcilpse—NewMethodofViewingProminences—TotalEclipse Visible in North America—Spectrum of the Corona—Eclipse of 1870—Young's Reversing Layer —Ecilpseof1871—Coronaof1878—VaryingCoronalTypes—EgyptianEcilpse—DaylightCoronal Photography—Observations at Caro il neIsland—Photographs of Corona in 1886 and 1889 —Eclipsesof1896,1898,1900,and1901—MechanicalTheoryofCorona—Electro-Magneitc Theories—Nature of Corona CHAPTER IV SOLAR SPECTROSCOPY Chemistry of Prominences—Study of their Forms—Two Classes—Photographs and Spectrographs of Prominences—TheirDistribuiton—StructureoftheChromosphere—SpectroscopicMeasurementof RadialMovements—SpectroscopicDeterminaitonofSolarRotation—VelociitesofTransportinthe Sun—Lockyer'sTheoryofDissociation—SolarConsittuents—OxygenAbsorptioninSolarSpectrum CHAPTER V TEMPERATURE OF THE SUN Thermal Power of the Sun—Radiation and Temperature—Estimates of Solar Temperature—Rosetti's and Wilson'sResutls—Zöllner'sMethod—Langley'sExperimentatPittsburg—TheSun'sAtmosphere —Langley'sBolometricResearches—SelecitveAbsorptionbyourAir—TheSolarConstant CHAPTER VI THE SUN'S DISTANCE DififcutlyoftheProblem—OppositionsofMars—TransitsofVenus—LunarDisturbance—VelocityofLight —Transit of 1874—Inconclusive Result—Opposition of Mars in 1877—Measurements of Minor Planets—Transit of 1882—Newcomb's Determination of the Velocity of Light—Combined Result CHAPTER VII PLANETS AND SATELLITES Schröter's Life and Work—Luminous Appearances during Transits of Mercury—Mountains of Mercury —Intra-MercurianPlanets—Schiapareill'sResutlsfortheRotaitonofMercuryandVenus—Illusory Satellite—MountainsandAtmosphereofVenus—AshenLight—SolidityoftheEarth—Variaitonof Laittude—SecularChangesofCilmate—FigureoftheGlobe—StudyoftheMoon'sSurface—Lunar Atmosphere—NewCraters—ThermalEnergyofMoonlight—TidalFriciton CHAPTER VIII PLANETS AND SATELLITES—(cnoitunde) AnalogybetweenMarsandtheEarth—MartianSnowcaps,Seas,andConitnents—Climateand Atmosphere—Schiapareill'sCanals—DiscoveryofTwoMartianSateliltes—PhotographicDetection ofMinorPlanets—OrbitofEros—DistributionoftheMinorPlanets—TheirCollecitveMassand EsitmatedDiameters—ConditionofJupiter—HisSpectrum—TransitsofhisSateliltes—Discoveryof aFifthSatelilte—TheGreatRedSpot—ConstituitonofSaturn'sRings—PeriodofRotationofthe Planet—VariabiiltyofJapetus—EquatorialMarkingsonUranus—HisSpectrum—RotaitonofNeptune —Trans-Neptunian Planets CHAPTER IX THEORIES OF PLANETARY EVOLUTION Origin of the World according to Kant—Laplace's Nebular Hypothesis—Maintenance of the Sun's Heat —MeteoricHypothesis—RadiaitonasanEffectofContraction—RegeneraitveTheory—Faye's Scheme of Planetary Development—Origin of the Moon—Effects of Tidal CHAPTER X RECENT COMETS Donait'sComet—TheEarthagainInvolvedinaComet'sTail—CometsoftheAugustandNovember Meteors—Star Showers—Comets and Meteors—Biela's Comet and the Andromedes—Holmes's Comet—DelfecitonoftheLeonids—OrbitsofMeteorites—MeteorswithStaitonaryRadiants —Spectroscopic Analysis of Cometary Light—Comet of 1901—Coggia's Comet CHAPTER XI RECENT COMETS—(deunitnco) Forms of Comets' Tails—Electrical Repulsion—Brédikhine's Three Types—Great Southern Comet —Supposed Previous Appearances—Tebbutt's Comet and the Comet of 1807—Successful Photographs—Schaeberle's Comet—Comet Wells—Sodium Blaze in Spectrum—Great Comet of 1882—Transit across the Sun—Relation to Comets of 1843 and 1880—Cometary Systems —Spectral Changes in Comet of 1882—Brooks's Comet of 1889—Swift's Comet of 1892—Origin of Comets CHAPTER XII STARS AND NEBULÆ StellarChemistry—FourOrdersofStars—TheirRelaitveAges—GaseousStars—SpectroscopicStar-Catalogues—StellarChemistry—HydrogenSpectruminStars—TheDraperCatalogue—Velocitiesof Stars in Line of Sight—Spectroscopic Binaries—Eclipses of Algol—Catalogues of Variables—New Stars—Outbursts in Nebulæ—Nova Aurigæ—Nova Persei—Gaseous Nebulæ—Variable Nebulæ —Movements of Nebulæ—Stellar Persei—Gaseous Nebulæ—Variable Nebulæ—Movements of Nebulæ—Stellar and Nebular Photography —Nebulæ in the Pleiades—Photographic Star-charting—Stellar Parallax—Double Stars—Stellar Photometry—Status of Nebulæ—Photographs and Drawings of the Milky Way—Star Drift CHAPTER XIII METHODS OF RESEARCH Development of Telescopic Power—Silvered Glass Reflectors—Giant Refractors—Comparison with Reflectors—The Yerkes Telescope—Atmospheric Disturbance—The Lick Observatory—Mechanical Dififcutlies—TheEquatorealCoudé—The Photographic Camera—Retrospect and Conclusion APPENDIX Chronology, 1774-1893—Chemical Elements in the Sun (Rowland, 1891)—Epochs of Sun-spot Maximum and Minimum from 1610 to 1901—Movements of Sun and Stars—List of Great Telescopes—List of Observatories employed in the Construction of the Photographic Chart and Catalogue of the Heavens INDEX LIST OF ILLUSTRATIONS PHOTOGRAPHOFTHEGREATNEBULA INORION, 1883Frontispiece PHOTOGRAPHSOFJUPITER, 1879,ANDOFSATURN, 1885Vignette PLATEI. PHOTOGRAPHSOFTHESOLARCHROMOSPHEREANDPROMINENCESTOFACEP. 198 PLATE II . PHOTOGRAPHOFTHEGREATCOMETOFMAY, 1901 (TAKENATTHEROYALOBSERVATORY, CAPEOFGOODHOPE) PLATEIII. THEGREATCOMETOFSEPTEMBER, (PHOTOGRAPHEDATTHECAPEOFGOODHOPE) PLATEIV. PHOTOGRAPHSOFSWIF'T SCOMET, 1892 PLATEV. PHOTOGRAPHICANDVISUALSPECTRUMOFNOVAAURIGÆ PLATEVI. PHOTOGRAPHOFTHEMILKYWAY INSAGITTARIUS HISTORY OF ASTRONOMY DURING THE NINETEENTH CENTURY INTRODUCTION Wecandistinguishthreekindsofastronomy,eachwithadifferentoriginandhistory,butallmutually dependent, and composing, in their fundamental unity, one science. First in order of time came the art of observing the returns, and measuring the places, of the heavenly bodies. This was the sole astronomy of the Chinese and Chaldeans; but to it the vigorous Greek mind added a highly complex geometrical plan of their movements, for which Copernicus substituted a more harmonious system, without as yet any idea of acompelilngcause.Theplanetsrevolvedincirclesbecauseitwastheirnaturetodoso,justaslaudanum sets to sleep because it possesses avirtus dormitivaand oldest branch is known as. This first "observaitona,l"or"practicalastronomy."tIsbusinessistonotefactsasaccuratelyaspossible;anditis essentiallyunconcernedwithschemesforconnectingthosefactsinamannersaitsfactorytothereason. The second kind of astronomy was founded by Newton. Its nature is best indicated by the term "gravitational"; but it is also called "theoretical astronomy."[1] It is based on the idea of cause; and the wholeofitselaboratestructureisrearedaccordingtothedictatesofasinglelaw,simpleinitsefl,butthe tangledwebofwhoseconsequencescanbeunravelledonlybythesubtleagencyofanelaboratecalculus. Thethirdandlastdivisionofcelestialsciencemayproperlybetermed"physicalanddescripitve astronomy."tIseekstoknowwhattheheavenlybodiesareinthemselves,leavingtheHow?and the Wherefore? of their movements to be otherwise answered. Now, such inquiries became possible only throughtheinventionofthetelescope,sothatGailleowas,inpointoffact,theiroriginato.rButHerschel first gave them a prominence which the whole progress of science during the nineteenth century served to conifrmandrendermoreexclusive.Inquisitionsbegunwiththetelescopehavebeenextendedandmade effecitveinunhoped-fordirecitonsbytheaidofthespectroscopeandphotographiccamera;andalarge partofourattenitoninthepresentvolumewillbeoccupiedwiththebrilliantresutlsthusachieved. The unexpected development of this new physical-celestial science is the leading fact in recent astronomicalhistory.tIwasoutoftheregularcourseofevents.Inthedegreeinwhichithasactually occurred it could certainly not have been foreseen. It was a seizing of the prize by a competitor who had hardlybeenthoughtquailifedtoentertheilsts.Orthodoxastronomersoftheoldschoollookedwitha certaincontemptuponobserverswhospenttheirnightsinscruitnisingthefacesofthemoonandplanets ratherthaninitmingtheirtransits,ordevoteddayilghtenergies,nottoreductionsandcomputaitons,butto counting and measuring spots on the sun. They were regarded as irregular practitioners, to be tolerated perhaps, but certainly not encouraged. The advance of astronomy in the eighteenth century ran in general an even and logical course. The age succeeding Newton's had for its special task to demonstrate the universal validity, and trace the complex results,ofthelawofgravitation.Theaccomplishmentofthattaskoccupiedjustonehundredyears.tIwas virtuallybroughttoaclosewhenLaplaceexplainedtotheFrenchAcademy,November19,1787,the causeofthemoon'sacceleratedmoiton.Asameremachine,thesolarsystem,sofarasitwasthen known,wasfoundtobecompleteandintelligibleinallitsparts;andintheMécanique Céleste its mechanical perfections were displayed under a form of majestic unity which fitly commemorated the successivetriumphsofanalyitcalgeniusoverproblemsamongstthemostarduouseverdeatlwithbythe mind of man. Theory,however,demandsapracticaltest.Allitsdataarederivedfromobservaiton;andtheirinsecurity becomes less tolerable as it advances nearer to perfection. Observation, on the other hand, is the pitiless criitcoftheory;itdetectsweakpoints,andprovokesreformswhichmaybethebeginningsofdiscovery. Thus,theoryandobservaitonmutuallyactandreact,eachatlernatelytakingtheleadintheendlessraceof improvement. Now,whileinFranceLagrangeandLaplacewerebringingthegravitaitonaltheoryofthesolarsystemto completion,workofaverydifferentkind,yetnotlessindispensabletothefutureweflareofastronomy,was beingdoneinEngland.TheRoyalObservatoryatGreenwichisoneofthefewusefulinsittuitonswhich datetheiroriginfromthereignofCharles.IITheleadingpositionwhichitstilloccupiesinthescienceof celestialobservaitonwas,fornearacenturyandahaflafteritsfoundaiton,anexclusiveone.Delambre remarked that, had all other materials of the kind been destroyed, the Greenwich records alone would sufficefortherestorationofastronomy.Theestabilshmentwasindeedabsolutelywithoutarival.[2] Systematicobservaitonsofsun,moon,stars,andplanetswereduringthewholeoftheeighteenthcentury made only at Greenwich. Here materials were accumulated for the secure correction of theory, and here reifnementswereintroducedbywhichtheexquisiteaccuracyofmodernpracitceinastronomywas eventually attained. The chief promoter of these improvements was James Bradley. Few men have possessed in an equal degree with him the power of seeing accurately, and reasoning on what they see. He let nothing pass. The silghtestinconsistencybetweenwhatappearedandwhatwastobeexpectedrousedhiskeenest attention; and he never relaxed his mental grip of a subject until it had yielded to his persistent inquisition. It wastothesequaliitesthatheowedhisdiscoveriesoftheaberrationoflightandthenutaitonoftheearth's axis. The first was announced in 1729. What is meant by it is that, owing to the circumstance of light not being instantaneously transmitted, the heavenly bodies appear shifted from their true places by an amount dependingupontheratiowhichthevelocityofilghtbearstothespeedoftheearthinitsorbit.Because lighttravelswithenormousrapidity,theshiftingisverysilght;andeachstarreturnstoitsoriginalposiitonat theendofayea.r Bradley'ssecondgreatdiscoverywasifnallyascertainedin1748.Nutaitonisareal"nodding"ofthe terrestrial axis produced by the dragging of the moon at the terrestrial equatorial protuberance. From it resutlsanapparentfohcaeedmehtngbirisctlitlailspeleuotebatrueitsorsplacemedietsra,stnofht "mean"posiiton,inaperiodofnearlynineteenyears. Now, an acquaintance with the fact and the laws of each of these minute irregularities is vital to the progress of observational astronomy; for without it the places of the heavenly bodies could never be accurately known or compared. So that Bradley, by their detection, at once raised the science to a higher grade of precision. Nor was this the whole of his work. Appointed Astronomer-Royal in 1742, he executed during the years 1750-62 a series of observations which formed the real beginning of exact astronomy. Partoftheirsuperioritymust,indeed,beattributedtotheco-operaitonofJohnBird,whoprovidedBradley in 1750 with a measuring instrument of till then unequalled excellence. For not only was the art of observing intheeighteenthcenturyapecuilarlyEngilshart,butthemeansofobservingwerefurnishedalmost exclusivelybyBriitshartists.JohnDollond,thesonofaSpitalfieldsweave,rinventedtheachromaitclensin 1758, removing thereby the chief obstacle to the development of the powers of refracting telescopes; JamesShort,ofEdinburgh,waswithoutarivalintheconstrucitonofreflectors;thesectors,quadrants,and circlesofGraham,Bird,Ramsden,andCarywereinimitablebyConitnentalworkmanship. ThuspracitcalandtheoreticalastronomyadvancedonparallelilnesinEnglandandFrancerespectively, the improvement of their several tools—the telescope and the quadrant on the one side, and the calculus ontheother—keepingpace.Thewholefutureofthescienceseemedtobetheirs.Thecessaitonof interest through a too speedy attainment of the perfection towards which each spurred the other, appeared to be the only danger it held in store for them. When all at once, a rival stood by their side—not, indeed, menacing their progress, but threatening to absorb their popularity. The rise of Herschel was the one conspicuous anomaly in the astronomical history of the eighteenth