第38届ICHO理论试题及答案.docx
《第38届ICHO理论试题及答案.docx》由会员分享,可在线阅读,更多相关《第38届ICHO理论试题及答案.docx(34页珍藏版)》请在冰豆网上搜索。
![第38届ICHO理论试题及答案.docx](https://file1.bdocx.com/fileroot1/2023-1/4/4f8869cc-355f-463a-96a1-4bb28c8cc15e/4f8869cc-355f-463a-96a1-4bb28c8cc15e1.gif)
第38届ICHO理论试题及答案
ChemistryforLife,
ChemistryforbetterLife
TheoreticalTest
GeneralDirections
-Writeyournameandcodenumberoneachpageoftheanswersheet.
-Youhave5hourstofinishthetask.FailuretostopaftertheSTOPcommandmayresultinzeropointsforthetask.
-Writeanswersandcalculationswithinthedesignatedbox.
-Useonlythepenandthecalculatorprovided.
-Thereare23pagesofProblemsand19pagesofAnswerSheet.
-AnEnglish-languageversionisavailable.
-Youmaygototherestroomwithpermission.
-Afterfinishingtheexamination,placeallsheetsincludingProblemsandAnswerSheetintheenvelopeandseal.
-Remainseateduntilinstructedtoleavetheroom.
Constantsandusefulformulas
GasconstantR=8.314JK-1mol-1
FaradayconstantF=96485Cmol-1
Useasstandardpressure:
p=1.013∙105Pa
Useasstandardtemperature:
T=25°C=298.15K
Avogadro’snumberNA=6.022∙1023mol-1
Planckconstanth=6.626∙10-34Js
Speedoflightc=3.00∙108ms-1
G=H-TSG=-nFE
G0=-RT∙lnKG=G0+RT∙lnQwithQ=
H(T1)=H0+(T1-298.15K)∙Cp(Cp=constant)
Arrheniusequationk=A∙
IdealgaslawpV=nRT
NernstequationE=E0+
Beer-LambertLawA=log
=∙c∙d
V(cylinder)=r2h
A(sphere)=4r2
V(sphere)=
r3
1J=1Nm1N=1kgms-21Pa=1Nm-2
1W=1AV=1Js-11C=1As
1.Avogadro'snumber(5pts)
Sphericalwaterdropletsaredispersedinargongas.At27oC,eachdropletis1.0micrometerindiameterandundergoescollisionswithargon.Assumethatinter-dropletcollisionsdonotoccur.Theroot-mean-squarespeedofthesedropletswasdeterminedtobe0.50cm/sat27oC.Thedensityofawaterdropletis1.0g/cm3.
1-1.Calculatetheaveragekineticenergy(mv2/2)ofthisdropletat27oC.Thevolumeofasphereisgivenby(4/3)πr3whereristheradius.
Ifthetemperatureischanged,thendropletsizeandspeedofthedropletwillalsochange.Theaveragekineticenergyofadropletbetween0oCand100oCasafunctionoftemperatureisfoundtobelinear.Assumethatitremainslinearbelow0oC.
Atthermalequlibrium,theaveragekineticenergyisthesameirrespectiveofparticlemasses(equipartitiontheorem).
Thespecificheatcapacity,atconstantvolume,ofargon(atomicweight,40)gasis0.31Jg-1K-1.
1-2.CalculateAvogadro'snumberwithoutusingtheidealgaslaw,thegasconstant,Boltzmann’sconstant).
2.DetectionofHydrogen(5pts)
Hydrogenisprevalentintheuniverse.Lifeintheuniverseisultimatelybasedonhydrogen.
2-1.Thereareabout1023starsintheuniverse.Assumethattheyarelikeoursun(radius,700,000km;density,1.4g/cm3;3/4hydrogenand1/4heliumbymass).Estimatethenumberofstellarprotonsintheuniversetoonesignificantfigure.
Inthe1920s,CeciliaPaynediscovered,byspectralanalysisofstarlight,thathydrogenisthemostabundantelementinmoststars.
2-2.Theelectronicenergyofahydrogenatomisgivenby-C/n2relativetozeroenergyatinfiniteseparationbetweentheelectronandtheproton(nistheprinciplequantumnumber,andCisaconstant).Fordetectionofthen=2→n=3transition(656.3nmintheBalmerseries),theelectroninthegroundstateofthehydrogenatomneedstobeexcitedfirsttothen=2state.Calculatethewavelength(innm)oftheabsorptionlineinthestarlightcorrespondingtothen=1→n=2transition.
2-3.AccordingtoWien'slaw,thewavelength(λ)correspondingtothemaximumlightintensityemittedfromablackbodyattemperatureTisgivenbyλT=2.9×10-3mK.Calculatethesurfacetemperatureofastarwhoseblackbodyradiationhasapeakintensitycorrespondingtothen=1→n=2excitationofhydrogen.
Thegroundstateofhydrogenissplitintotwohyperfinelevelsduetotheinteractionbetweenthemagneticmomentoftheprotonandthatoftheelectron.In1951,Purcelldiscoveredaspectrallineat1420MHzduetothehyperfinetransitionofhydrogenininterstellarspace.
2-4.Hydrogenininterstellarspacecannotbeexcitedelectronicallybystarlight.However,thecosmicbackgroundradiation,equivalentto2.7K,cancausethehyperfinetransition.Calculatethetemperatureofablackbodywhosepeakintensitycorrespondstothe1420MHztransition.
2-5.Wiengeneratedhydrogenionsbydischargeofhydrogengasataverylowpressureanddeterminedthee/m(charge/mass)value,whichturnedouttobethehighestamongdifferentgasestested.In1919,Rutherfordbombardednitrogenwithalpha-particlesandobservedemissionofapositivelychargedparticlewhichturnedouttobethehydrogenionobservedbyWien.Rutherfordnamedthisparticlethe“proton”.Fillintheblankintheanswersheet.
14N+4He→()+1H
3.InterstellarChemistry(5pts)
EarlyinterstellarchemistryisthoughttohavebeenapreludetolifeonEarth.Moleculescanbeformedinspaceviaheterogeneousreactionsatthesurfaceofdustparticles,oftencalledtheinterstellaricegrains(IIGs).ImaginethereactionbetweenHandCatomsontheIIGsurfacethatformsCH.TheCHproductcaneitherdesorbfromthesurfaceorfurtherreact,throughsurfacemigration,withadsorbedHatomstoformCH2,CH3,etc.
Dependingonhowenergeticallyamolecule“jumps”fromitsanchoredsite,iteitherleavesthesurfacepermanently(desorption)orreturnstoanewpositionatthesurface(migration).TheratesofdesorptionandmigratoryjumpfollowtheArrheniusformula,k=Aexp(-E/RT),wherekistherateconstantfordesorptionormigratoryjump,Athejumpingfrequency,andEtheactivationenergyfortherespectiveevent.
3-1.DesorptionofCHfromtheIIGsurfacefollowsfirst-orderkinetics.CalculatetheaverageresidencetimeofCHonthesurfaceat20K.AssumethatA=1x1012s-1andEdes=12kJmol-1.
3-2.ConsidertheshortesttimeitwouldtakeforoneCHunittomovefromitsinitialpositiontotheoppositesideofanIIGbysuccessivemigratoryjumps.Assumethattheactivationenergyformigration(Emig)is6kJmol-1,andtheIIGisaspherewitha0.1μmradius.Eachmigratoryjumplaterallyadvancesthemoleculeby0.3nm.Showworkandchooseyouranswerfrom(a)-(e)below.
(a)t≤1day(b)10day≤t≤102yr(c)103yr≤t≤106yr
(d)107yr≤t≤1010yr(e)t≥1011yr
3-3.ConsiderthereactionofCOwithH2toformH2CO.Theactivationenergyonametalcatalystis20kJmol-1,whichproducesformaldehydeatarateof1molecule/spersiteat300K.Esitmatetherateofformaldehydeformationpersiteifthereactiontakesplaceat20K.
3-4.Whichisasetofalltruestatements?
Circleone.
(a)MostCHspeciesdesorbfromtheIIGsurfacebeforeencounteringotherreactantsbysurfacemigration.
(b)IIGscanassisttransformationofsimplemoleculestomorecomplexonesininterstellarspace.
(c)ForareactionontheIIGtooccuratanappreciablespeedduringtheageoftheUniverse(1x1010yr),thereactionenergybarriermustbeabsentornegligible.
(a)(b)(c)(a,b)(a,c)(b,c)(a,b,c)
4.TheChemistryofDNA(5pts)
4-1.In1944OswaldAveryisolatedageneticmaterialandshowed,byelementalanalysis,thatitwasasodiumsaltofdeoxyribonucleicacid.AsegmentofDNAwithformulamassof1323.72isshown.
AssumingthatequimolaramountsofthefourbasesarepresentinDNA,writethenumberofHatomsperPatom.Calculate,to3significantfigures,thetheoreticalweightpercentageofHexpecteduponelementalanalysisofDNA.
4-2.ChargaffextractedtheseparatedbasesanddeterminedtheirconcentrationsbymeasuringUVabsorbance.TheBeer-Lambertlawwasusedtoobtainthemolarconcentration.ChargaffdiscoveredthefollowingmolarratioforbasesinDNA:
adeninetoguanine=1.43 thyminetocytosine=1.43
adeninetothymine=1.02 guaninetocytosine=1.02
Chargaff’sdiscoverysuggestedthatthebasesmightexistaspairsinDNA.WatsonandCrickmentionedintheircelebrated1953paperinNature:
"Ithasnotescapedournoticethatthespecificpairingwehavepostulatedimmediatelysuggestsapossiblecopyingmechanismforthegeneticmaterial."
DrawstructuresofthespecificpairingfoundinDNA.Indicatehydrogenbonds.Omitthesugar-phosphatebackbone.
4-3.Mutationcanoccurthroughbasepairingsdifferentfromtheabove.Drawstructuresofanythreealternativebasepairs.
4-4.TheplausibilityoftheformationofpurineandpyrimidinebasesintheprebioticatmosphereoftheEarthfromHCN,NH3,andH2Ohasbeendemonstratedinthelaboratory.WritetheminimumnumberofHCNandH2Omoleculesrequiredforformationofthefollowingcompounds.
5.Acid-BaseChemistry(5pts)
5-1.Calculate[H+],[OH-],[HSO4-],and[SO42-]ina1.0x10-7Msolutionofsulfuricacid(Kw=1.0x10-14,K2=1.2x10-2at25oC).Inyourworkyoumayusemass-andcharge-balanceequations.Answerwithtwosignificantfigures.
5-2.Calculatethevolumeof0.80MNaOHsolutionthatshouldbeaddedtoa250mLaqueoussolutioncontaining3.48mLofconcentratedphosphoricacidinordertoprepareapH7.4buffer.Answerwiththreesignificantfigures.(H3PO4(aq),purity=85%wt/wt,density=1.69g/mL,FW=98.00)(pK1=2.15,pK2=7.20,pK3=12.44).
5-3.Theefficacyofadrugisgreatlydependentonitsabilitytobeabsorbedintothebloodstream.Acid-basechemistryplaysanimportantroleindrugabsorption.
Assumethattheionicform(A-)ofaweaklyacidicdrugdoesnotpenetratethemembrane,whereastheneutralform(HA)freelycrossesthemembrane.AlsoassumethatequilibriumisestablishedsothattheconcentrationofHAisthesameonbothsides.Calculatetheratioofthetotalconcentration([HA]+[A-])