A History of Science

第5章

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第5章

A History of Science Henry Smith Williams

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A History of Science
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  WhenwepasstothatthirdgreatAthenianteacher,Aristotle,thecaseisfardifferent。HerewasamanwhosenamewastobereceivedasalmostasynonymforGreekscienceformorethanathousandyearsafterhisdeath。AllthroughtheMiddleAgeshiswritingsweretobeacceptedasvirtuallythelastwordregardingtheproblemsofnature。Weshallseethathisfollowersactuallypreferredhismandatetothetestimonyoftheirownsenses。Weshallsee,further,thatmodernscienceprogressedsomewhatinproportionasitoverthrewtheAristoteliandogmas。Butthetraditionsofseventeenoreighteencenturiesarenoteasilysetaside,anditisperhapsnottoomuchtosaythatthenameofAristotlestands,eveninourowntime,asvaguelyrepresentativeinthepopularmindofallthatwashighestandbestinthescienceofantiquity。Yet,perhaps,itwouldnotbegoingtoofartoassertthatsomethinglikeareversalofthisjudgmentwouldbenearerthetruth。Aristotledid,indeed,bringtogetheragreatmassoffactsregardinganimalsinhisworkonnaturalhistory,which,beingpreserved,hasbeendeemedtoentitleitsauthortobecalledthe\"fatherofzoology。\"Butthereisnoreasontosupposethatanyconsiderableportionofthisworkcontainedmatterthatwasnovel,orrecordedobservationsthatwereoriginalwithAristotle;andtheclassificationsthereoutlinedareatbestbutavagueforeshadowingoftheelaborationofthescience。Suchasitis,however,thenaturalhistorystandstothecreditoftheStagirite。Hemustbecredited,too,withaclearenunciationofonemostimportantscientificdoctrine——namely,thedoctrineofthesphericalfigureoftheearth。WehavealreadyseenthatthistheoryoriginatedwiththePythagoreanphilosophersoutinItaly。Wehaveseen,too,thatthedoctrinehadnotmadeitswayinAtticainthetimeofAnaxagoras。Butintheinterveningcenturyithadgainedwidecurrency,elsesoessentiallyconservativeathinkerasAristotlewouldscarcelyhaveacceptedit。Hedidacceptit,however,andgavethedoctrineclearestandmostpreciseexpression。Herearehiswords:[2]

  \"Astothefigureoftheearthitmustnecessarilybespherical……Ifitwerenotso,theeclipsesofthemoonwouldnothavesuchsectionsastheyhave。Forintheconfigurationsinthecourseofamonththedeficientparttakesalldifferentshapes;itisstraight,andconcave,andconvex;butineclipsesitalwayshasthelineofdivisionsconvex;wherefore,sincethemooniseclipsedinconsequenceoftheinterpositionoftheearth,theperipheryoftheearthmustbethecauseofthisbyhavingasphericalform。Andagain,fromtheappearanceofthestarsitisclear,notonlythattheearthisround,butthatitssizeisnotverylarge;forwhenwemakeasmallremovaltothesouthorthenorth,thecircleofthehorizonbecomespalpablydifferent,sothatthestarsoverheadundergoagreatchange,andarenotthesametothosethattravelinthenorthandtothesouth。ForsomestarsareseeninEgyptoratCyprus,butarenotseeninthecountriestothenorthofthese;andthestarsthatinthenortharevisiblewhiletheymakeacompletecircuit,thereundergoasetting。Sothatfromthisitismanifest,notonlythattheformoftheearthisround,butalsothatitisapartofanotverylargesphere;forotherwisethedifferencewouldnotbesoobvioustopersonsmakingsosmallachangeofplace。WhereforewemayjudgethatthosepersonswhoconnecttheregionintheneighborhoodofthepillarsofHerculeswiththattowardsIndia,andwhoassertthatinthiswaytheseaisone,donotassertthingsveryimprobable。Theyconfirmthisconjecturemoreoverbytheelephants,whicharesaidtobeofthesamespeciestowardseachextreme;asifthiscircumstancewasaconsequenceoftheconjunctionoftheextremes。Themathematicianswhotrytocalculatethemeasureofthecircumference,makeitamounttofourhundredthousandstadia;

  whencewecollectthattheearthisnotonlyspherical,butisnotlargecomparedwiththemagnitudeoftheotherstars。\"

  ButingivingfullmeedofpraisetoAristotleforthepromulgationofthisdoctrineofthesphericityoftheearth,itmustunfortunatelybeaddedthattheconservativephilosopherpausedwithouttakingoneotherimportantstep。Hecouldnotaccept,but,onthecontrary,heexpresslyrepudiated,thedoctrineoftheearth’smotion。WehaveseenthatthisideaalsowasapartofthePythagoreandoctrine,andweshallhaveoccasiontodwellmoreatlengthonthispointinasucceedingchapter。IthasevenbeencontendedbysomecriticsthatitwastheadverseconvictionofthePeripateticphilosopherwhich,morethananyothersingleinfluence,tendedtoretardtheprogressofthetruedoctrineregardingthemechanismoftheheavens。

  Aristotleacceptedthesphericityoftheearth,andthatdoctrinebecameacommonplaceofscientificknowledge,andsocontinuedthroughoutclassicalantiquity。ButAristotlerejectedthedoctrineoftheearth’smotion,andthatdoctrine,thoughpromulgatedactivelybyafewcontemporariesandimmediatesuccessorsoftheStagirite,wasthendoomedtosinkoutofviewformorethanathousandyears。IfitbeacorrectassumptionthattheinfluenceofAristotlewas,inalargemeasure,responsibleforthisresult,thenweshallperhapsnotbefarastrayinassumingthatthegreatfounderofthePeripateticschoolwas,onthewhole,moreinstrumentalinretardingtheprogressofastronomicalsciencethatanyotheronemanthateverlived。

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