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USC - CHEM - 325BL
Chapter 16Aldehydes and Ketones INucleophilic Additions to the Carbonyl GroupGeneral Features of the Carbonyl GroupR':RThe general structure ofthe carbonyl group isC=OIn a molecular orbital description, the carbon and oxygen atomsare hybridized
USC - CHEM - 325BL
Nucleophilic Addition to the Carbon-Oxygen Double Bond!+ !"C=O:The reactivity of the carbon-oxygen doublebond is determined by the polarization:Because of the permanent dipole, nucleophiles add to theelectropositive carbon and electrophiles add to
USC - CHEM - 325BL
Addition of Hydrogen Cyanide: CyanohydrinsHydrogen cyanide (HCN) adds to aldehydes andunhindered ketones to produce cyanohydrins.OHRC-C NHOHRC-C NR'=ORCH + H-C N=ORCR' + H-C NunhinderedcyanohydrinsThe reaction is carried out by adding a m
USC - CHEM - 325BL
Chapter 17: Carboxylic Acids and their Deriva9ves Nucleophilic Addi9onElimina9on at the Acyl Carbon Carboxylic acids are a family of organic compoundswith the functional group=O-C-OHalso written as -CO2H or COOHThe carbon-oxygen do
USC - CHEM - 325BL
Nucleophilic Substitution at Acyl CarbonAldehydes and ketones undergo nucleophilic additionsto the carbonyl group:R-C-O:NuNu-HR'R:C=O+ Nu:-:R:R'R'C-O-H + Nu:NutetrahedralintermediateThe typical reaction with carboxylic acids and their
USC - CHEM - 325BL
AmidesORCNHR'2o==ORCNH21oSynthesis of Amides from Acyl Chlorides=ORCCl +-:NH3-OOH+RC-N-HH=RC-Cl+H-N-HH:NH3ORCNH2==OH+RC-N-H +HORC-Cl+H-N-HH+ Cl-+NH4+ORCNR'R'3o=Amides like amines are classifiedaccording to th
USC - CHEM - 325BL
NitrilesOne standard way of preparing a nitrile is by the dehydration ofthe corresponding primary amide with reagents such as P4O10(called phosphorous pentoxide, P 2O5) or refluxing aceticanhydride.=OCH3CH2CNH2propionamideP 2O585o C(-H2O)CH3CH
USC - CHEM - 325BL
Chapter 18!Reactions at the -Carbon of Carbonyl Compounds!Enols and Enolates!Acidity of the !-Hydrogens of Carbonyl CompoundsHydrogens ! to the carbonyl group are much more acidic thanordinary aliphatic hydrogens that have pKa values > 50.=-OR-C-C
USC - CHEM - 325BL
Lithium Enolates in Organic SynthesisThe extent to which a carbonyl compound with an !-H is convertedto its enolate anion depends on the acidity of the !-H and thestrength of the base.+ B:-?OC-C:==OHC-COCH3CCH3 + HO-=OCH3C-CH2pKa = 20weak
USC - CHEM - 325BL
The Malonic Ester Synthesis of Substituted Acetic AcidsBy a similar sequence of alkylation, hydrolysis, and decarboxylation,substituted acetic acids may be prepared from diethyl malonate.malonic ester synthesis==OOEtOCCH2COEtdiethyl malonateR-CH
USC - CHEM - 325BL
Synthesis of AminesNucleophilic Substitution Reactions: Direct Alkylation MethodThe nucleophilic substitution of alkyl halides with ammonia is ageneral synthesis of primary amines.+ R-Xaminium saltbase(-HX)::NH3+RNH3 X-RNH2primaryamineThe
USC - CHEM - 325BL
Reactions of AminesThe chemistry of amines is determined by the nonbonding electronpair on nitrogen. Amines are bases and nucleophiles.N:basenucleophileN:+H+N-H++N-R+R-X+ X-The amino group as a substituent on a benzene ringis a powerful a
USC - CHEM - 325BL
Phenols and Aryl HalidesNucleophilic Aromatic SubstitutionPhenolsPhenols have the hydroxyl group attached to a benzene ring.The name is derived from the aryl group name by dropping the"yl" in phenyl and adding "ol."Substituted phenols are named by t
USC - CHEM - 325BL
Aryl Halides and Nucleophilic Aromatic SubstitutionSimple aryl halides do noteasily undergo nucleophilicaromatic substitution.Cl+ NaOHH2Ono reactionheatSimilarly, vinylic halides do not react under these conditions.CH2=CHCl + NaOHH2Oheatno re
USC - CHEM - 325BL
Chapter 20 AminesAmines are organic bases. They are found widely in nature.Trimethylamine occurs in animal tissue while the distinctive odorof fish is due to amines. Amines isolated from plants are calledaNomenclature of which are pharmacologically im
USC - CHEM - 325BL
Notes for Practice Exam I Fall 2011, 322b OMIT: Problem numbers 2, 4, 5, 6, and 8 Note: On problem number 9 do not circle the major resonance contributor and ignore the lone pair of electrons on the Nitrog
USC - CHEM - 325BL
1 322b Fall 2011 Exam II Review Sheet Chapter 15 Note: Assignment #2 serves as the Chapter 14 review sheet for Exam II I.Multiple Choice. 1. The order of reactivity (fastest to slowest), ignoring the pos
USC - CHEM - 325BL
1 CHEM 322b Fall 2011 Practice Exam III I.Multiple Choice 1. Circle the reaction condition or conditions below that would convert the carboxylic acid below into an aldehyde, as shown (ignore workup steps).
USC - CHEM - 325BL
1 Chemistry 322b Fall 2011 Practice Exam IV Section I. Multiple Choice. 1. The directed crossed aldol condensation of I and II below is best promoted by which procedure below. OOO+I II A. Ad
USC - CHEM - 325BL
Exam I Key Correc.on #16 In the original exam key four products (IIV below) were indicated as the Products B ClClClClIIIIIIIVStructure III and IV are equivalent, so only three products are actually formed.
USC - CHEM - 325BL
1 Section I. Multiple Choice. (24 points). 1. Circle the more stable carbocation of the pair. CH3CH3 2. According to MO theory, in the allyl cation (CH2=CHCH2+), the two electrons
USC - CHEM - 325BL
1 Practice Problem Set #2 322b Fall 2011 Chapter 14 Practice Problems Section I. Multiple Choice. 1. Circle the compound or compounds that are nonaromatic (as opposed to aromatic or antiaromatic). Assume
USC - CHEM - 325BL
1 Practice Problem Set #3 322b Fall 2011 Chapter 15 Practice Problems 1. O+OHBr 2. OO+ O O 3. Also use any 12 carbon compound as the only other carbon source. COOHBr
USC - CHEM - 325BL
Chapter 16 Practice Problems. Chemistry 322b Fall 2011 1. OH & any saturated alcohol as only carbon sources 2. OO O & any saturated alcohol or other 12 carbon source as only carbo
USC - CHEM - 325BL
Practice Problem Set #5 CHEM 322b Fall 2011 1. OOHOHNH2 2. O OOHOO 3. OOHOOH 4. OONHN & a 14 C source 5. O & any 13 carbon sources O
USC - CHEM - 325BL
Practice Problem Set #6 CHEM 322b Fall 2011 1. OOO+BrH 2. OCO2EtCO2EtCO2Et O& any 4 carbon source 3. O 4. NH2 5. OM eOMeMeOMeOOM eOM eNHNH2 & any 6 carbon source
USC - CHEM - 325BL
Practice Problem Set #7. CHEM 322b Fall 2011 1. FCNNH3Cl 2. NCH3LiBr 3. ClOMeNO 2CF 3CF 3 & any 1 carbon source 4. HNN 5. BrOHNO 2NH2
USC - CHEM - 325BL
@+LC9\+' ,-\.\(a7"lrt,yF.^l).1t )^Dc r yAl , h l'lg,hz,z , a .oIN O AO9o c ln?1.\/\n-t\7 Xcyl-Q'r / )tct3, 1,uJJr ,l )-oo?-,2- ) N "fufr3uSd-t-,+L l ). o +l), 1 )lcl3,cA.,fhr:\ifl? u 'utF,agaoVcoolP.0t1VoBr,
Boise State - PHYSICS - 104
3 Sept 2003Solar System - C. C. Lang1Check your knowledge-Northerners have cold days in January because:(a) the earth is farthest from the Sun in January(b) the orbital velocity of Earth is greatest in Jan.(c) the Sun is lower in the sky in January
Boise State - PHYSICS - 104
Water on Mars Geological Evidence for Water on Mars*- gullies, erosion channels- layers/sedimentary features The Physics of Water on Marspolar ice caps seasonal variationatmosphere - history Chemical Evidence for Water on Mars Theories for Water o
Boise State - PHYSICS - 104
Surface Exploration of Mars: Past & Future Martian Meteorites Martian Moons Martian Surface ExplorationThe Viking Landers (early 80s)Pathfinder (1997)Current Surface Explorers (three en route!)Future of Martian Exploration (astrobiology) Review of
Boise State - PHYSICS - 104
Solar System Planets: The Earth + MoonI. Moon- Atmosphere- Surface/Geological Features/Moon Rocks- Interior- OriginII. Mercury- Basic Facts- Exploration- Cratering13 Oct 2003Solar System - Dr. C.C. Lang1The Moon has no atmosphere allows us t
Boise State - PHYSICS - 104
Exploring the Solar System:all about spacecraft/spaceflightI. How can we explore the Solar System?- types of space missionsII. How do we get there?- launch & orbits- gravity assist- fuel/propulsionIII. Onboard Systems- everything but the kitchen
Boise State - PHYSICS - 104
BlackHolesBlackHolesTheintensegravitationalfieldleftwhenagiantstarcollapsesItiscalledablackholebecausenotevenlightcanescapePhotonSphereTheouteredgewherelightbendsbutisstillescapableEventHorizonThepointatwhichnolightcanescapeSingularityT
Boise State - PHYSICS - 104
Cosmic rays and solar flaresDraw in the back of your book thelife cycle of a starSolar flares and Cosmic raysYou should learn: Cosmic rays are fast-moving ionising particlesfrom the Sun. The Earths magnetic field prevents themfrom reaching us beca
Boise State - PHYSICS - 104
Comet Impact:July 4, 2005Impact Velocity:23,000 mphSpacecraft Size:Flyby spacecraft nearly as large as aVolkswagen Beetleautomobile.Impactor spacecraft about the samedimensions as atypical living roomcoffee table.Principal Investigator, Dr. Mi
Boise State - PHYSICS - 104
Exploring our Solar SystemP2f part 2ObjectivesIn this lesson we should learn: about the distances involved in spacetravel about manned and unmanned space flight how very large distances are measured inspaceOutcomesFoundation PaperYou should now
Boise State - PHYSICS - 104
Exploring our Solar SystemP2f part 1ObjectivesIn this lesson we should learn: about the bodies in space that make upthe Universe why planets and moons stay in orbits about the planets in our Solar System,producing a model of the Solar SystemOutco
Boise State - PHYSICS - 104
Free powerpoints at http:/www.worldofteaching.comFirststopMercury(e e k,re a lly h o th e re s o wo nts tic ka ro und to o lo ng ) wh e re g ra vity is 3N/kg.ontoVenus,theplanetofluuurrrvewheregravityis9N/kg(bitlikeEarth).AthomeonEarth,wh
Boise State - PHYSICS - 104
HowFarisFar?Earth to Mo o n Dis tanc eAverage of 238,000 MilesS un to Earth Dis tanc e1 As tro no mic al Mile s(AU)9 3,000,000 UnitB o dyMercuryVenusEarthMarsJ upiterSaturnUranusNeptunePlutoAU.39.721.01.55.29.519.230.139.5S o lar
Boise State - PHYSICS - 104
Whe re is Jupite r?5th P lanet from the Sun483,600,000 Miles(5.2 AngstromUnits)Plane t OrbitalP e rio ds(in Earth-Ye ars )29.461.88.24.6284.0111.86164.8247.7What is Jupite r?Gaseous Atmosphereof Hydrogen, Helium,Carbon Dioxide, Methane
Boise State - PHYSICS - 104
Meteors & Meteor ShowersMeteorsThe DifferencesThe Meteoroid,Meteorite, Meteor? Meteoroid- small, solid body moving withinsmall,the solar system.the Meteorite- solid remains of a meteor thatsolidfalls to the Earth.falls Meteor- (shooting star
Boise State - PHYSICS - 104
50:50Welcome toWho Wants tobe a Millionaire151413121110987654321$1 Million$500,000$250,000$125,000$64,000$32,000$16,000$8,000$4,000$2,000$1,000$500$300$200$100 H.M.Murphy- All Rights Reserved H.M.Murphy- All Rights Reser
Boise State - PHYSICS - 104
The MoonA look at our nearestneighbor in Space!Free powerpoints at http:/www.worldofteaching.comWhat is the Moon? A natural satellite One of more than 96 moons inour Solar System The only moon of the planetEarthLocation, location, location! Abo
Boise State - PHYSICS - 104
OUR SOLAR SYSTEMTHE MILKY WAYTHE SUNMERCURYVENUSEARTHMARSJUPITERSATURNURANUSNEPTUNEPLUTOThis powerpoint was kindly donated towww.worldofteaching.comhttp:/www.worldofteaching.com is home to over athousand powerpoints submitted by teachers. T
Boise State - PHYSICS - 104
OuterSpaceObjectsOuterSpaceObjectsCenterofMilkyWayCenterofMilkyWayCOMETSCOMETSPhotographsprovidedonthewebbyNASASeriesof7slidesHalleysCometHalleysComet13May1910overFlagstaff,ArizonaHalleyCometHalleyCometfromGiotto1986GiottoGiottoCometBrad
Boise State - PHYSICS - 104
SpectrafromRetinaNebula:Green=hydrogenBlue=oxygenRed=nitrogenTarantulaNebulaintheLargeMagellanicCloudStellarStellarformationinPapillonNebulainLargeMagellanicCloudLagoonNebulaOrionOrionNebulafromHubble1,500 light yearsfrom earthS
Boise State - PHYSICS - 104
Our Solar SystemOurThese photographs are taken from the NASAspace missions.spacehttp:/nssdc.gsfc.nasa.gov/photo_gallery/Our SunOurMicrosoft Clip ArtSolar Eclipse 2001SolarTransittime:3hoursinLusaka,ZambiaTotaleclipse:2sec.shortof3minutesPhoto
Boise State - PHYSICS - 104
Part 2 of Solar SystemPartMars GlobalSurveyor (MGS)1996 to 20061996240,000 photos240,000Marsphotographphotograph4viewsofsurfaceMarsMars19June1976SngiViktrafcecpaMars surfaceMarsOlympus MonsOlympuslargest volcano in solar system
Boise State - PHYSICS - 104
Celestial Objects to scaleOuter Space 4czones of the Solar system: inner solar system, asteroidbelt, giant planets (Jovians) and Kuiper belt.Sizes and orbits not to scale.Sizes are to scale.Arp147 imageHeres what NASA thinks.www.nasa.gov/multimed
Boise State - PHYSICS - 104
Space The Final FrontierSpaceEarly astronomersEarly Astronomer - Astronomers use the principles of physics and mathematicsAstronomer Astronomersto learn about the fundamental nature of the universe, including the sun, moon,planets, stars, ..Nicho
Boise State - PHYSICS - 104
Space Science UnitQuick overview:GalaxiesMultiple Star SystemsConstellationsSpectroscope LabToilet Paper SolarSystem LabCharacteristics of StarsH-R DiagramMeasuring Star distances(parallax)The Sun: Our special StarActivities of the SunIntrod
Boise State - PHYSICS - 104
The solar systemWhat is the solar system?The Sun, its planets and other objectsin orbit are all together known as thesolar system.The nine planets(starting with the closest to the Sun)MercuryVenusEarthMarsJupiterSaturnUranusNeptunePlutoHow
Boise State - PHYSICS - 104
Threats to EarthP2g part 1 & 2ObjectivesIn this lesson we should learn: about the properties of asteroids how asteroids have affected Earth in thepastOutcomesFoundation PaperYou should now be able to. State that large asteroids have collided wit
FSU - MAC - 1130
1 Right Triangle TrigonometryTrigonometry is the study of the relations between the sides and angles of triangles. Theword trigonometry is derived from the Greek words trigono (o), meaning triangle,and metro (), meaning measure. Though the ancient Gree