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SNC1D6–Choo2018/19 Name:
Astrochemistry
LearningGoals/SuccessCriteria:Attheendofthislesson,Iwillbeableto:! Describewherethefirstelementscamefrom! Calculatetheageoftheuniversebasedonredshiftdata
Theamazingthingisthateveryatominyourbodycamefromastarthatexploded.
And,theatomsinyourlefthandprobablycamefromadifferentstarthanyourrighthand.ItreallyisthemostpoeticthingIknowaboutphysics:Youareallstardust.
―LawrenceM.Krauss,AUniversefromNothing:WhyThereIsSomethingRatherThanNothing
NewsFlash:BirthoftheFirstElements!Theprimordial(early)universewasaveryeventfulplace.Itwasanincrediblyhot,denseenvironmentthatcooledrapidlyastheuniverseexpanded.ThreeminutesaftertheBigBang,theuniversehadcooledenoughfornuclearfusiontotakeplace.Thisledtothecreationofthefirstatomicnucleithroughaprocesscalledprimordialnucleosynthesis.Howdidthesefirstnucleiformintheearlyuniverse?Whichelementswerecreated?Whatratioswerealltheelementspresentin?
SummaryoftheFacts
ConclusionHowwerethefirstatomicnucleiformedaftertheBigBang?Whichelementswerecreated,andhowmuchofeachelementwastherecomparedtootherelements?
Timeline of the Universe
TheSignatureoftheStarsRainbowsrevealthatwhitelightisacombinationofallthecolours.In1666,IsaacNewtonshowedthatwhitelightcouldbeseparatedintoitscomponentcoloursusingglassprisms.Soonscientistswereusingthisnewtooltoanalyzethelightcomingfromseveraldifferentlightsources.Somescientistslookedathotobjectsandgases;otherslookedatthestarsandplanets.Theyallmadeobservationsanddetectedpatterns,butittookabout250yearsforscientiststounderstandtheconnections.Part1:EveryElementHasaUniqueSignature.Everyelementemitsauniquerangeofcolourscalledanemissionspectrum.Asimilarspectrumisproducedwhenlightshinesthroughagas;however,inthiscasecertaincolours,orwavelengths,areabsorbedbythegas.Anabsorptionspectrumisthepatternofcoloursanddarklinesthatisproducedwhenlightshinesthroughagasandthegasabsorbscertainwavelengths.Thisisthesamepatternthatoccursintheemissionspectrumforthesamemedium.Figure1showssomesimplifiedabsorptionspectrallines.1. Scientistscanuseabsorptionspectratoanalyzeunknownsubstances.Identifytheelementspresent
inthesamplethatproducesthespectrainFigure2.
Part2:TheLightfromStarsContainsInformation. Thecoreofastarisveryhot(~15×106K),andveryhotobjectsglow.Thelightproducedbyastar’scorecontainsallthecoloursinthespectrum.Astronomerscanlearnmanythingsaboutastar’smotion,temperature,andcompositionbyanalyzingthestarlightthatreachesEarth.Aspectroscopeisaninstrumentthatseparateslightintoitsspectrum.Oneoftheearliestusesofthespectroscopewastoanalyzelightcomingfromastronomicalobjects.Thelightdirectedfromatelescopethroughaspectroscopeproducesanimagecalledaspectrograph.
Figure1Thelinesindicatethewavelengthsoflightthataremissingfromthelightafterpassingthroughthesample.Theweight(thickness)ofthelinesindicatestheamountoflightabsorbedatthatwavelength.Theheavier(orthicker)theline,themorelightisabsorbed.
Figure2Simplifiedabsorptionspectra
Part3:TheSpectrafromGalaxiesAreRedshifted.In1912,AmericanastronomerVestoSlipherbegantoobservemoredistantobjectsusingaspectrometer,andhenoticedthatmostofthemhadadistinctshifttowardtheredendofthespectrum.HerecognizedthisasaDopplershiftcausedbythemotionoftheobjects.Aredshiftmeansthatthesourceoflightismovingawayfromtheobserver.Figure3showsanemissionspectrumfromthequasarcalled3C273.Weseethattheemissionlinesduetohydrogenareshiftedtotheredendofthespectrum.Thelargertheredshift,thegreatertherelativemotion.
2. EdwinHubbleextendedthisobservationtomoreobjects,andforseveralobjectsplottedtheredshiftversusthedistancetotheobject.Tryitforyourself.InTable1,usetheredshiftofthespectrallinestodeterminethespeedofeachgalaxy.Todothis,usearulertoaligntheleftmostspectrallineprovidedwitheachgalaxywiththespeedscaleatthebottomofthetable.
Redshift3C 273
Comparison spectrum
RedBlue
HβHγHδ
HβHγHδ
600 nm500 nm400 nm
Figure3Redshiftedspectrumfromquasar3C273
Table1
3. PlotthespeedofeachgalaxyinTable1onthey-axisandthedistancetothegalaxyonthex-axis.Drawalineofbestfit.
4. Calculatetheslopeoftheline.Whatistheunitfortheslope?
5. TheslopeofthislineiscalledtheHubbleconstant,H0.WritetheequationforthislineusingH0asyourslope.Whatdoesittellyouabouttherelationshipbetweenthespeedofgalaxiesandtheirdistance?ThisrelationshipiscalledHubble’slaw.
6. Theageoftheuniverse,T,canbeapproximatedbytakingthereciprocal,orinverse,ofH0.Takethereciprocalofyourslope.Howoldistheuniverse(inyears)?