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THE NEW ASTRONOMY.

V SIR WILLIAMMUGGINS'S DISrV ;■'.".'■•; coveries. \; AN: INTERESTING REVIEW.; - '•'] In ; reviewing tho • "Scientific Papers of Sir 'William Huggins".. the "Nation" says:— ■'.'■ ■: ys .'■'.'■'.•'■■ ' '.''.' : il'ri' 165G,: three..years " before Darwin .supplied.the key. in .his ''Origin ,of Species" ■ to. the evolution of man from lower'life-forms, the Kirchhoff hod unlocked the'secret of tho chemical constitution of thosun, Sir William (then Mr.) Huggins '. built V :modest observatory at i'ulse Hillwhich .was to become '.world-' famous in tho. annals of ■ astronomical 'discovery... I'or he "b'nilded' wisor. than he kiiew.". : At'tkat timoitseoincd that tho work of the observer of "that inverted bowl.wo, call the sky" was limited to the conventional' lines of ■■ his : predecessors. At intervals another minor planet would swim "into his ken"; or a; now star' flash and become extinguished; or, as recently iin tho case: of Jupiter,' another satellite ;be added, to the list of /'companions"; or tho number of stars whose distances can be '■ reckoned ', in light-years increased; But that the mystery of .the stuff of which the, heavenly bodies' aro modo would bo solved, was a speculation dismissed .wellnighas. soon as. broached,, for, how was it possible to establish any, physical, relation, between tho ohemistry of the earth and that of .A, mass of matter ninety-three million miles,distant! •■'•■.• ' ': '

:-As.'M.'Declaux. acutely said, "It, is because~scicnCo,>is sure ot (nothing thatiit is over advancing.", And'.in 1802 Wollaston's detection of (four 'dark- lines which.crossed'a, Eiihray:'at .right angles when broken on 'a prisiu, lines which are how- numbered by ;thousands,.set the workers, in celestial, physics :on. a. quest whose;.result, "in .the.hands, of Kirchhoff. was : tho discovery that sodium, iron, arid other terrestrial,'elements are present in the.sun. ..Thereby?Sir :William: Huggins, "dissatisfied," ho 'tolls lis,; "with, the rou- ■ tine; character, of .ordinary work," ; received. the "impetus;,to. the application ,: of : the speetrbscopo to analysis pf;/theT.light*:from.> the 7 so-called,."fixed": etarsi' : whereby, ;thoir :\ chemistry;"might, porehance,be,also known.-' His researches, carried .on-,for x some;,timo.:in conjunction 1 >vith ;'.tho - late' : Dr.:'Allen,'Miller, (and durlng''many.'yeilirft-t6: : th6''ripMsflnt'.time 1 in; still happier':collaboration.with Lady ■Muggins), ,'began ; 'in"-lBl!3:... In> : that .year.. Huxley, pushing Darivin's.; theory. to';iii iiiovitaMo. .conclusion, • demonstrated'/ the; fundamental; unity" of: man;-ipsychically lis;well as-physically,.',irith - every,'living ithing, .a.■ ■.demonstration! 'which rsyhchroulsed.with/the pr.b'pfs pf'fundamentalviihity. of- suii.arid stars,: dud-.tho '.dependence'of.. Jthe'."- orgartio;.on. the.; inorganic: being. no {matter 'of. : vquestion',' 'the tof..all:.phohomonawas.,made manifest.V;lt .was the; birth:of :the-;New.;'Ahthropblogy ;and, tho,-Now. 'Astronomy.: '/. Of •'.; tho .-;trinmphs .achievedf/'trahbeending tho..wild T est-.droduis- of an earlier, Sir. ;Willittm;.:-Hugi[ins,''fns, ypractieally,;.'. tho ..founder of; the 'science -of this majestic volume,;aiid;a preceding one, ;outitled; ■ "Au.;Atlas'.; of Jteprcsentativo ;Stollaiv Spectra," aro ■ alike tho witnesses and,:.tho;recbrd.'::;:' ! ;;;v i r;-:'V;:*, i ':/■-■■' ; ;;<■': :\

;, Upturning: to} tho jspoctrum, :lurchhoff, identified .'sixty" lines' (since .iriorohsed to' more than .201)0) as'duo. to-tho presence, of il-oivand to this/is 'added proof ;of the;,prcsonco -ofj.caloimii, helium'.(which, was: liotidiscovercd oil' till- '; ;eartli till .some tlin6/-afterwards);'coppoi', zmo,- and., other, HiDlals.'■■'■': As tho 'planets'. a«- not. original Sources: of flight, vtheit T.pootra.reseiiibld:th<j'«uii'».spectrum, but somewhat' modified? ;by. I tho! absorptive: pjiai'a'cter-of,tlibiratniOsßliero/' .;.,:':,:;! ■■■ i'Bttt, ;in ■securing-. sucK; results;..-;the method of. analysis;-is simplicity,, itself; colufered ..with that which 'had'■■to.'.to- do? ■ vised vvheu tho Upeetruscbpe' attacked ''tho' .problem;: of ■•rstars' .'Whoee'''(listaiibe '.is''. measurable, not; iii nlilos,' .butviii /'lightyears;.'lv For'; starlight: appears'-as Vouly ? • a tromulous point,, whiclr.tbo most' power- 1 nil telescope, can .increase in brightness,hut.vehrihot 'Convei't; info'' a, disc "■''.; ,To' broaden, it into a .short lino, the star's- ■ image .hiis;' ; to. bo...t'hroßTi'. upon "a 1 narrow slitj-a spectroscope is fisfed to the eye, ond. of.; tho-.telc'scopo, j and ihonj-,by-moans of ii small; reflecting .prism placed .before one-half, -tho slit,,fighi;.front. V terrestrial solirco'at. tho side of .tho tele■scope';, is. sent, into' the 'instrument, to-' Kotherxwith., the .star's light,:. thereby .forming, a ..spectrum'/by ;tho side .of tho stellar spectrum \ for cOliiparisbit- with' it; IhiisJyrasKprcpared',tho;. apparatus:' for Analysis ;of -light radiated at the speed' of above eleven millions of miles per minute ifronr bodies which; in the case".of: Vega, ■ VIS 1 y; , o . n ?,% t y, thousand' millionth part w'the;'Jiglit,,received from' tho sun,-and' tho fact^.rovcaled.,.that': ; Bodium,': ihagrios-: :i^;'.?»f .ifoii :aro: present' iiutbat;star,- : .in-,Smud,:Pollux,'and;.without ;d6ubt,:in all-like.: self-luiriihous -bodies, in. the; infinite spaces,.; In, addition'.to. this, the ■ .nature of;the,'thousands of' hcbula'o, was once'and :for all; settled.'■ .The resolution, ,ot largo , of ; : theso';. into ■ clusters ■ ot minute .stars', by ■.powerful telescopes ■' lent strong support to the:theory that n\V, of them were of. the sahio constitution. But in : ISG4 .Sir William Hugging cx-'l ,aminatiqn,vof-.-.Hie. certain' nebulao disclosed ;tho: presen'co',,'of.brißlit linbs,; throe/of i.which, are due to'.'iy'droV gen.;, 1 bus : the , gaseous -. nature-p'roto-' plasm 'of. ; sidereal systems-of 'all ■■■true-; nebulae (in:which.the imposing nebulaiin Urioiv is included) was demonstrated, and broadly speaking, tho. like applies.ito the, ;I n .K? ut ';, b P.dies.- known- as comets.'- "Sir ■,\Villiam,-. applied',the'spocWoscopo:to the problenvfof. star, direction,, measuring the I '■<£ JHsv b,odies', .at;: : i'ncohceivablo' ?!&$m raced'imfromi.',oout.: S sim J '• ™* ■ivas.-'arrivcd ;0t ;by:;cttlcukt ug.'tho','relativo,vaisplace: I ,ment'of; the lines -in the' spectrum,,as, : tor example,,:a.minute.sliift ofithe For 'hydrogen ■;. line ,iii.;the. spectrum ''of; Sirius-, , mdicnted..that-that star 'is receding .from ■, ;,;tn« solar system' at'a.spoed of'eighteen ■ 'miles ; per, second' of: time: to-S. - f av °urablorcircumstances;" Sir 'William,; says,' "the . : spectroscOpo/ enables ■. ü ßjto.,mpastirß , .-to-,'nrithin*a''''niilo';pe'r--6e&'' oud, .or; even; less, .tho-'rate.'.of: motion. iw'-'t'ir ls3^" 11111 . w . nnt: of 6f the stellar lines with-tho sdnio lines pro-' ducod:,up6n;;tlievsarth'mby'-'safblyihe interpreted--: as'; revealing- tho'?.! velocity ■'' of approach«or:of.recessionsbetween'tho star and.;tho.earthy. »As;for'thb : :movcment; of • our-.tiystera,... it" appears'to "bo" towards a pointiin the.constellation -'Hereules; \rlulorecent;: observation, lends- support: to a theory .that the; stellar 'systenvis Vwhole comprises/,twO.'genoral; drifts:, of', stars rushing in nearly opposite directions', As the spectroscope "reveals What, appear to" bo stages: .-.pi., condensation- in -.the matter otthb-universe,-, it-'is probable: that the' conclusion as to star evolution and dissolution'drawn from their colours will be found.--.to ;be valid.- -;, That .fascinating branch of. cosmic dynamics 'has not escaped . tho- vigilant eye. of Sir 'William Huggina; but the life-history of .star's -re-' mains among speculations- which may bo' converted .into certainties when-wo know more i about, tho, disintegration of: the' so- , called clementsr' : '-■- ;:-•:■;■'-,■.. n To W s t-V st ' r ' of - r 'P reat ' iclii °wmcri(3':"(J)' : the establishment of the identity of stUlf bet,woen our system'/and, otter, stellar systems; (2)' of - the, direction. in which' the stars are?moving; (3)' of tho nature of many of tho nobulao; (4) the revelation of by the application of phbtog-. raphy—enough in themselves- to'. : represent', the ceaseless labours, of a long life—there might- be added.others, such, for example; as,the method.of viewing the prominences in, the uneclipsod'sun; bufthcir secondary ~importance, is warrant for. omission from the. present attempt to compress in nntochnical lnngudgo . tho main contents l of a volume with'which the expert alone can adequately.deal. -It is a talo'of wonder, tho effect .of which is deepened by' the .'absence of alt rhetoric and thepreseuco. of...modesty : in'.' the .'narration, .pulled, must.be tho intelligence which fails to be quickened. thereby; to poriderings over mail's: stupendous advance in knowledge, or to' bb touched .by the reflection with what added pathos the.final monition, "thus far shalt. Thou go, and po farther," : comes homo to. tho rare .truth-seeking souls typified- by theS an-' thor -whose discoveries are the subject-' matter of this volume.—"Tho Nation,"

Permanent link to this item
Hononga pūmau ki tēnei tūemi

https://paperspast.natlib.govt.nz/newspapers/DOM19100115.2.138

Bibliographic details
Ngā taipitopito pukapuka

Dominion, Volume 3, Issue 716, 15 January 1910, Page 15

Word count
Tapeke kupu
1,155

THE NEW ASTRONOMY. Dominion, Volume 3, Issue 716, 15 January 1910, Page 15

THE NEW ASTRONOMY. Dominion, Volume 3, Issue 716, 15 January 1910, Page 15

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