Hey, everyone. In this video, we're going to start our journey down a path of organic chemistry that's very important called molecular orbital theory. Let's go ahead and get started. Guys, so first of all, I want to just give you a disclaimer. This topic is called the basics of molecular orbital theory, but to be honest, there's nothing basic about molecular orbital theory. It's one of the most widely misunderstood parts of organic chemistry and many students just avoid it entirely because they're so confused, and there are very few resources out there that provide very clear explanations that they just try to ignore it and try to get through organic chemistry without it. Unfortunately, there are some reactions that we're going to need to really understand molecular orbital theory so that we can learn those reactions. And without a good understanding of MO theory, you're just going to get lost. So what I'm going to try to do in the next 15 minutes or so is I'm going to try to tell you a really smooth story based on what you already know on how to understand molecular orbitals. And I actually worked really hard on this to try to build a good flow based on what I believe you already know and what you need to know by the end of this topic. So please let me know if this story made sense to you at the end. I'm totally down to redo this if it's confusing. But I'm going to try to just take my time. This isn't about getting through this quickly, it's about making sure that all of you guys get it at the end. So it seems like I'm going slow, that's on purpose because there are very few videos you can go to online that explain molecular orbital theory thoroughly and I'm going to try to build that video now. Okay? Cool. So let's start with what we know. As previously discussed, there's this idea called conjugation. You guys remember what conjugation means? Conjugation means that you have the ability to resonate. Okay? What does resonance mean? Resonance means that you're sharing electrons from one atom to another. You guys remember that? You can resonate electrons, etcetera. Well, one of the technical ways that you can talk about resonance is that resonance happens from nonbonding orbitals to adjacent nonbonding orbitals. What do I mean by nonbonding? That it's not making a bond to another atom. Now why are only nonbonding orbitals involved in resonance? Because if you're making a bond to an atom, it's stuck to that atom. And remember that resonance structures you can't move atoms around. Remember that? Remember the only thing you can move is bonds, like pi bonds and electrons. You can't move atoms. So when we're going to talk about the idea of conjugation, we're always going to talk about the nonbonding orbitals, meaning ones that don't have an atom attached to them. Okay? Cool. So now since we're going to be talking about nonbonding orbitals a lot today, I want to remind you that nonbonding only takes place in the outermost shell of an atom's electron configuration. So remember that you have like 1s orbitals, 2s orbitals, etcetera. You would only be dealing with the last shell, and since we're in organic chemistry, that last shell is usually going to be the 2nd shell, meaning that the electrons that are in the first shell, that one s, are not involved in any of the things we're going to talk about today. You can pretty much ignore the one s. What we're going to talk about is the 2s. Okay? So what I want to do is show you guys a very basic example of hybridization from organic chemistry 1. This is one of the first things you learned in organic chemistry 1, and I want to remind you how these electrons behave, how these valence electrons behave. Okay? So here is an alkene, and we know that we learned a long time ago that alkenes have 3 bonds, so an alkene carbon has 3 bonds attached to it, which would mean what we call them 3 groups or 3 bond sites. Remember, a bond site or a group is just anywhere that you have an atom attached or that you have a lone pair attached, okay. So if we were to look at this carbon right here that I already have circled, how many atoms does it have attached to it right now? It has a hydrogen, a hydrogen, and a carbon, meaning that there are 3 bond sites, meaning that this mean that this equates to an sp2 hybridization. Remember that? That you're supposed to know that however many bond sites there are, that's how many, that's what your hybridization is. And 3 always means sp2. But let's go a little bit deeper into the electron configuration to remember how this hybridization works. And by the way, I have videos on all of this so far, but I'm just here to remind you. These are the highlights. So remember that carbon is in which, you know, is what's the atomic number of carbon? It's 6. Carbon has an atomic number of 6, which means that at its neutral state, how many protons does it have? 6. How many electrons does it have? 6. So when we build the electron configuration of carbon, we need to figure out where all those 6 electrons are going to go. Right? And remember that you always start with Aufbau principle from the lowest energy orbital. So you have to start filling your orbitals in ascending order of energy. So that means that out of the 6 electrons, where should those electrons go? Well, 2 of them should go into the 1s orbital because that's the lowest energy state orbital possible. Then another 2 of them should go into the 2s orbital because that's the next highest, right? And then we have Hund's rule. Remember that Hund's rule says that if you have, a bunch of seats on the bus, you need to fill them equally. You can't just have 2 kids on one seat and 0 kids on another seat. So in this case, notice that the p orbitals are all the same energy state, right? So that means that I would then get one electron in the 2px, one electron in the 2py, and now I ran out of electrons. I just put all my 6, meaning that there's no electrons for the 2pz. Does that make sense so far? So this is the way that we would fill these orbitals based on what we know from gen chem, based on what we know of just like, hey, there's 6 electrons and we need to put the put them into the electron configuration, this is what it should look like. But remember that in the first chapter of organic chemistry, what we learned is that this is not favored. And the reason is because guys, remember that carbon always wants to be able to make 4 bonds, right? But right now, the way that you have the carbon set up, the 2s already has a filled orbital, right? This is already filled. So can that orbital make a bond? No. And then we have, I'm just gonna use different colors, these 2 orbitals could make a bond because they could accept 1 electron. And then this one has no electrons, so it's not very good at making a bond because it would have to accept 2 electrons, not just 1. So that limits the amount of things that it can make bonds with. So what I'm trying to say is that it's not very favored to have these electrons scattered like this. What's more favored is to spread the electrons out evenly throughout all the orbitals, so that all the orbitals have a chance to make a bond, and this is the process that we call hybridization. Remember that when you have specifically 3 groups or 3 bond sites, what happens is that the 2s orbital blends with 2 of the p orbitals to give you an sp2 hybridized blended orbital. Okay? And that's what we have happening here in this gray box. Notice that, remember what you're supposed to memorize is that 3 bond sites equals sp2, which means that the 2s, the yellow from the 2s, blended with the 2 with the 2p orbitals, 2 of the p orbitals, to give us 3 new orbitals called sp2sp2, sp2. Okay. Now you might be wondering Johnny, why did you put 2 sp2? Well, because technically you can just call it sp2, but you can also call it 2 sp2 because they're in the second shell. And anything that's in the second shell can get a 2 behind it. Okay? So remember that sp3 means that there are 3 bonds and and they can all blend together in this way. Notice that now what happens is instead of getting 2 electrons in a lower energy orbital and then 2 electrons in higher, now we have is 3 electrons evenly spaced out between this, more averaged out energy level, okay. But there's also one more thing, which is that when you have sp 2 23 bond sites, that means that there's a 4th bond that's not being made. That means that there's an extra electron that is just going to be in an extra orbital and that extra orbital does not hybridize. So that is going to be here, my 2pz. Notice that this one didn't hybridize, so it's actually a little bit higher in energy because it didn't blend with the other ones. And it has one electron that's free to interact with, either to make a, potentially make a bond or to interact with other orbitals, okay? So this is gonna be what we keep, what we're gonna call our nonbonding orbital and this is gonna be the one that's gonna be the really interesting one for us for the rest of this section. We're gonna be talking about the nonbonding orbital a lot, okay? But let's put this on hold for a second because I want to go back to the 2 sp2s and talk about what they're doing. Okay? Well, remember that we said that it's making 3 bonds, right? So what we could do is we could show where those 3 bonds are happening. 1 of them is happening, I'm just going to use different colors for this, one of them is happening to an electron from a 1s orbital in the hydrogen. So that's this guy right here, I'm going to call him a and then this is a. What's happening is that the hydrogen has one electron, right? Hydrogens have an atomic number of 1, so it has one electron and it's sharing that electron with the one electron from the sp2, and what that's doing is it's making a bond. So when I drew this blue area here, this actually means that we're making a new bond between those 2 electrons that are now going to be shared in one orbital. Does that make sense so far? Cool. Notice that this is also happening on the bottom. I have another one. This is Hb let's say. This one is also overlapping with the electron from the sp2 and it's making a bond. Cool? And then lastly guys, notice that the carbon is also making a bond to another carbon, right? Let's call this c here. So it's making a bond to that carbon. Okay? But that carbon isn't just a 1s orbital because 1s is what you have if you just have a hydrogen. What it actually is, is it's another sp2 orbital, another sp2 hybridized orbital because notice that it has 3 bond sites. So you're going to have 1s and 2p's blend together and give you an sp2. And what's going to happen is that those 2 sp2's are going to overlap in one place and give us a new sigma bond and that's our new sigma bond. So by the way, all of these are sigma bonds. So this is sigma, oops, sigma and sigma because they're all overlapping in just one place. Basically like you could think of it like this, like this tip is going to overlap with this tip like this. Okay. They're all overlapping in one place, giving us 3 new sigma bonds. Okay. So now this brings us to the interesting part. What is happening with the nonbonding orbital? It's left over, but it has one electron left, so it's able to interact with something. But what is it going to do? What it actually looks like, guys, is it looks more like, just to show you, it looks more like this, okay, where you have your 3 sigma bonds, so sigma 1, sigma 2, sigma 3. We already talked about how that's happening, but then we have this extra electron that's just floating in an orbital waiting to do something. So what is it going to do? Well guys, it's going to be able to conjugate. If you can put an n If you can put another nonbonding orbital next to it, it will conjugate. And what conjugate means is that it can share its electrons between them freely, so the electrons can actually resonate or jump around from here to here, from here to here and they can blend together. Okay? Now the type of resonance that you get depends on what type of orbital is the second one that you're interacting it with. Okay? Now in a in when you make a pi bond, remember that a pi bond has to do with making a double bond, right? A pi bond would just mean that you have another nonbonding orbital that's exactly like the one that you started with, where it has one electron and basically it's overlapping with another, basically 2pz. Does that make sense? It's overlapping with... **[MESSAGE CUTS OFF]**
- 1. A Review of General Chemistry5h 5m
- Summary23m
- Intro to Organic Chemistry5m
- Atomic Structure16m
- Wave Function9m
- Molecular Orbitals17m
- Sigma and Pi Bonds9m
- Octet Rule12m
- Bonding Preferences12m
- Formal Charges6m
- Skeletal Structure14m
- Lewis Structure20m
- Condensed Structural Formula15m
- Degrees of Unsaturation15m
- Constitutional Isomers14m
- Resonance Structures46m
- Hybridization23m
- Molecular Geometry16m
- Electronegativity22m
- 2. Molecular Representations1h 14m
- 3. Acids and Bases2h 46m
- 4. Alkanes and Cycloalkanes4h 19m
- IUPAC Naming29m
- Alkyl Groups13m
- Naming Cycloalkanes10m
- Naming Bicyclic Compounds10m
- Naming Alkyl Halides7m
- Naming Alkenes3m
- Naming Alcohols8m
- Naming Amines15m
- Cis vs Trans21m
- Conformational Isomers13m
- Newman Projections14m
- Drawing Newman Projections16m
- Barrier To Rotation7m
- Ring Strain8m
- Axial vs Equatorial7m
- Cis vs Trans Conformations4m
- Equatorial Preference14m
- Chair Flip9m
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- A-Values17m
- Decalin7m
- 5. Chirality3h 39m
- Constitutional Isomers vs. Stereoisomers9m
- Chirality12m
- Test 1:Plane of Symmetry7m
- Test 2:Stereocenter Test17m
- R and S Configuration43m
- Enantiomers vs. Diastereomers13m
- Atropisomers9m
- Meso Compound12m
- Test 3:Disubstituted Cycloalkanes13m
- What is the Relationship Between Isomers?16m
- Fischer Projection10m
- R and S of Fischer Projections7m
- Optical Activity5m
- Enantiomeric Excess20m
- Calculations with Enantiomeric Percentages11m
- Non-Carbon Chiral Centers8m
- 6. Thermodynamics and Kinetics1h 22m
- 7. Substitution Reactions1h 48m
- 8. Elimination Reactions2h 30m
- 9. Alkenes and Alkynes2h 9m
- 10. Addition Reactions3h 18m
- Addition Reaction6m
- Markovnikov5m
- Hydrohalogenation6m
- Acid-Catalyzed Hydration17m
- Oxymercuration15m
- Hydroboration26m
- Hydrogenation6m
- Halogenation6m
- Halohydrin12m
- Carbene12m
- Epoxidation8m
- Epoxide Reactions9m
- Dihydroxylation8m
- Ozonolysis7m
- Ozonolysis Full Mechanism24m
- Oxidative Cleavage3m
- Alkyne Oxidative Cleavage6m
- Alkyne Hydrohalogenation3m
- Alkyne Halogenation2m
- Alkyne Hydration6m
- Alkyne Hydroboration2m
- 11. Radical Reactions1h 58m
- 12. Alcohols, Ethers, Epoxides and Thiols2h 42m
- Alcohol Nomenclature4m
- Naming Ethers6m
- Naming Epoxides18m
- Naming Thiols11m
- Alcohol Synthesis7m
- Leaving Group Conversions - Using HX11m
- Leaving Group Conversions - SOCl2 and PBr313m
- Leaving Group Conversions - Sulfonyl Chlorides7m
- Leaving Group Conversions Summary4m
- Williamson Ether Synthesis3m
- Making Ethers - Alkoxymercuration4m
- Making Ethers - Alcohol Condensation4m
- Making Ethers - Acid-Catalyzed Alkoxylation4m
- Making Ethers - Cumulative Practice10m
- Ether Cleavage8m
- Alcohol Protecting Groups3m
- t-Butyl Ether Protecting Groups5m
- Silyl Ether Protecting Groups10m
- Sharpless Epoxidation9m
- Thiol Reactions6m
- Sulfide Oxidation4m
- 13. Alcohols and Carbonyl Compounds2h 17m
- 14. Synthetic Techniques1h 26m
- 15. Analytical Techniques:IR, NMR, Mass Spect6h 50m
- Purpose of Analytical Techniques5m
- Infrared Spectroscopy16m
- Infrared Spectroscopy Table31m
- IR Spect:Drawing Spectra40m
- IR Spect:Extra Practice26m
- NMR Spectroscopy10m
- 1H NMR:Number of Signals26m
- 1H NMR:Q-Test26m
- 1H NMR:E/Z Diastereoisomerism8m
- H NMR Table21m
- 1H NMR:Spin-Splitting (N + 1) Rule17m
- 1H NMR:Spin-Splitting Simple Tree Diagrams11m
- 1H NMR:Spin-Splitting Complex Tree Diagrams8m
- 1H NMR:Spin-Splitting Patterns8m
- NMR Integration18m
- NMR Practice14m
- Carbon NMR4m
- Structure Determination without Mass Spect47m
- Mass Spectrometry12m
- Mass Spect:Fragmentation28m
- Mass Spect:Isotopes27m
- 16. Conjugated Systems6h 13m
- Conjugation Chemistry13m
- Stability of Conjugated Intermediates4m
- Allylic Halogenation12m
- Reactions at the Allylic Position39m
- Conjugated Hydrohalogenation (1,2 vs 1,4 addition)26m
- Diels-Alder Reaction9m
- Diels-Alder Forming Bridged Products11m
- Diels-Alder Retrosynthesis8m
- Molecular Orbital Theory9m
- Drawing Atomic Orbitals6m
- Drawing Molecular Orbitals17m
- HOMO LUMO4m
- Orbital Diagram:3-atoms- Allylic Ions13m
- Orbital Diagram:4-atoms- 1,3-butadiene11m
- Orbital Diagram:5-atoms- Allylic Ions10m
- Orbital Diagram:6-atoms- 1,3,5-hexatriene13m
- Orbital Diagram:Excited States4m
- Pericyclic Reaction10m
- Thermal Cycloaddition Reactions26m
- Photochemical Cycloaddition Reactions26m
- Thermal Electrocyclic Reactions14m
- Photochemical Electrocyclic Reactions10m
- Cumulative Electrocyclic Problems25m
- Sigmatropic Rearrangement17m
- Cope Rearrangement9m
- Claisen Rearrangement15m
- 17. Ultraviolet Spectroscopy51m
- 18. Aromaticity2h 31m
- 19. Reactions of Aromatics: EAS and Beyond5h 1m
- Electrophilic Aromatic Substitution9m
- Benzene Reactions11m
- EAS:Halogenation Mechanism6m
- EAS:Nitration Mechanism9m
- EAS:Friedel-Crafts Alkylation Mechanism6m
- EAS:Friedel-Crafts Acylation Mechanism5m
- EAS:Any Carbocation Mechanism7m
- Electron Withdrawing Groups22m
- EAS:Ortho vs. Para Positions4m
- Acylation of Aniline9m
- Limitations of Friedel-Crafts Alkyation19m
- Advantages of Friedel-Crafts Acylation6m
- Blocking Groups - Sulfonic Acid12m
- EAS:Synergistic and Competitive Groups13m
- Side-Chain Halogenation6m
- Side-Chain Oxidation4m
- Reactions at Benzylic Positions31m
- Birch Reduction10m
- EAS:Sequence Groups4m
- EAS:Retrosynthesis29m
- Diazo Replacement Reactions6m
- Diazo Sequence Groups5m
- Diazo Retrosynthesis13m
- Nucleophilic Aromatic Substitution28m
- Benzyne16m
- 20. Phenols55m
- 21. Aldehydes and Ketones: Nucleophilic Addition4h 56m
- Naming Aldehydes8m
- Naming Ketones7m
- Oxidizing and Reducing Agents9m
- Oxidation of Alcohols28m
- Ozonolysis7m
- DIBAL5m
- Alkyne Hydration9m
- Nucleophilic Addition8m
- Cyanohydrin11m
- Organometallics on Ketones19m
- Overview of Nucleophilic Addition of Solvents13m
- Hydrates6m
- Hemiacetal9m
- Acetal12m
- Acetal Protecting Group16m
- Thioacetal6m
- Imine vs Enamine15m
- Addition of Amine Derivatives5m
- Wolff Kishner Reduction7m
- Baeyer-Villiger Oxidation39m
- Acid Chloride to Ketone7m
- Nitrile to Ketone9m
- Wittig Reaction18m
- Ketone and Aldehyde Synthesis Reactions14m
- 22. Carboxylic Acid Derivatives: NAS2h 51m
- Carboxylic Acid Derivatives7m
- Naming Carboxylic Acids9m
- Diacid Nomenclature6m
- Naming Esters5m
- Naming Nitriles3m
- Acid Chloride Nomenclature5m
- Naming Anhydrides7m
- Naming Amides5m
- Nucleophilic Acyl Substitution18m
- Carboxylic Acid to Acid Chloride6m
- Fischer Esterification5m
- Acid-Catalyzed Ester Hydrolysis4m
- Saponification3m
- Transesterification5m
- Lactones, Lactams and Cyclization Reactions10m
- Carboxylation5m
- Decarboxylation Mechanism14m
- Review of Nitriles46m
- 23. The Chemistry of Thioesters, Phophate Ester and Phosphate Anhydrides1h 10m
- 24. Enolate Chemistry: Reactions at the Alpha-Carbon1h 53m
- Tautomerization9m
- Tautomers of Dicarbonyl Compounds6m
- Enolate4m
- Acid-Catalyzed Alpha-Halogentation4m
- Base-Catalyzed Alpha-Halogentation3m
- Haloform Reaction8m
- Hell-Volhard-Zelinski Reaction3m
- Overview of Alpha-Alkylations and Acylations5m
- Enolate Alkylation and Acylation12m
- Enamine Alkylation and Acylation16m
- Beta-Dicarbonyl Synthesis Pathway7m
- Acetoacetic Ester Synthesis13m
- Malonic Ester Synthesis15m
- 25. Condensation Chemistry2h 9m
- 26. Amines1h 43m
- 27. Heterocycles2h 0m
- Nomenclature of Heterocycles15m
- Acid-Base Properties of Nitrogen Heterocycles10m
- Reactions of Pyrrole, Furan, and Thiophene13m
- Directing Effects in Substituted Pyrroles, Furans, and Thiophenes16m
- Addition Reactions of Furan8m
- EAS Reactions of Pyridine17m
- SNAr Reactions of Pyridine18m
- Side-Chain Reactions of Substituted Pyridines20m
- 28. Carbohydrates5h 53m
- Monosaccharide20m
- Monosaccharides - D and L Isomerism9m
- Monosaccharides - Drawing Fischer Projections18m
- Monosaccharides - Common Structures6m
- Monosaccharides - Forming Cyclic Hemiacetals12m
- Monosaccharides - Cyclization18m
- Monosaccharides - Haworth Projections13m
- Mutarotation11m
- Epimerization9m
- Monosaccharides - Aldose-Ketose Rearrangement8m
- Monosaccharides - Alkylation10m
- Monosaccharides - Acylation7m
- Glycoside6m
- Monosaccharides - N-Glycosides18m
- Monosaccharides - Reduction (Alditols)12m
- Monosaccharides - Weak Oxidation (Aldonic Acid)7m
- Reducing Sugars23m
- Monosaccharides - Strong Oxidation (Aldaric Acid)11m
- Monosaccharides - Oxidative Cleavage27m
- Monosaccharides - Osazones10m
- Monosaccharides - Kiliani-Fischer23m
- Monosaccharides - Wohl Degradation12m
- Monosaccharides - Ruff Degradation12m
- Disaccharide30m
- Polysaccharide11m
- 29. Amino Acids3h 20m
- Proteins and Amino Acids19m
- L and D Amino Acids14m
- Polar Amino Acids14m
- Amino Acid Chart18m
- Acid-Base Properties of Amino Acids33m
- Isoelectric Point14m
- Amino Acid Synthesis: HVZ Method12m
- Synthesis of Amino Acids: Acetamidomalonic Ester Synthesis16m
- Synthesis of Amino Acids: N-Phthalimidomalonic Ester Synthesis13m
- Synthesis of Amino Acids: Strecker Synthesis13m
- Reactions of Amino Acids: Esterification7m
- Reactions of Amino Acids: Acylation3m
- Reactions of Amino Acids: Hydrogenolysis6m
- Reactions of Amino Acids: Ninhydrin Test11m
- 30. Peptides and Proteins2h 42m
- Peptides12m
- Primary Protein Structure4m
- Secondary Protein Structure17m
- Tertiary Protein Structure11m
- Disulfide Bonds17m
- Quaternary Protein Structure10m
- Summary of Protein Structure7m
- Intro to Peptide Sequencing2m
- Peptide Sequencing: Partial Hydrolysis25m
- Peptide Sequencing: Partial Hydrolysis with Cyanogen Bromide7m
- Peptide Sequencing: Edman Degradation28m
- Merrifield Solid-Phase Peptide Synthesis18m
- 32. Lipids 2h 50m
- 34. Nucleic Acids1h 32m
- 35. Transition Metals5h 33m
- Electron Configuration of Elements45m
- Coordination Complexes20m
- Ligands24m
- Electron Counting10m
- The 18 and 16 Electron Rule13m
- Cross-Coupling General Reactions40m
- Heck Reaction40m
- Stille Reaction13m
- Suzuki Reaction25m
- Sonogashira Coupling Reaction17m
- Fukuyama Coupling Reaction15m
- Kumada Coupling Reaction13m
- Negishi Coupling Reaction16m
- Buchwald-Hartwig Amination Reaction19m
- Eglinton Reaction17m
Molecular Orbital Theory - Online Tutor, Practice Problems & Exam Prep
Molecular orbital theory explains how atomic orbitals combine to form molecular orbitals, influencing bonding and stability in compounds like alkenes. Constructive interference leads to bonding molecular orbitals, enhancing electron density between atoms, while destructive interference results in antibonding molecular orbitals, reducing stability. Understanding hybridization, such as sp2, is crucial for predicting molecular behavior and reactivity, particularly in reactions involving conjugation and resonance. This foundational knowledge is essential for grasping complex organic reactions and mechanisms.
In these videos we will discuss the basics of the Molecular Orbital Theory, beginning with the idea of non-bonding orbitals.
Review of Atomic Orbitals
Video transcript
Review of Molecular Orbitals
Video transcript
When adjacent non-bonded atomic orbitals overlap with each other or are next to each other, they create more favorable molecular orbitals. A molecular orbital is simply the overlap of a few atomic orbitals. If you want to know what the molecular orbital is going to look like, we can use a system very common in organic chemistry called the linear combination of atomic orbitals (LCAO), which helps you predict what the molecular orbital will look like.
Now that I've hopefully convinced you that atomic orbitals like to share electrons, I want to talk about what those electrons look like after they share. We're going to take the example of ethene. Recall that one orbital has one electron, another orbital has another electron—these are the atomic orbitals, and this is typically how we represent them. Each of the conjugated atoms will receive one atomic orbital. Notice that I have 2 conjugated atoms, so I draw 1, 2 atomic orbitals next to each other and place however many free electrons there are into those orbitals. Atom 1 is donating one electron, which is why I put one electron there. Atom 2 is donating another, which is why I add another electron.
Remember, an orbital is just a region of space that is statistically probable to have electrons. It's like a cloud of electron density where there's a high chance we'll find electrons, but it's not actually a particle. When you bring atomic orbitals close together, they don't collide; they interfere with each other like waves, not like particles. This interference can be constructive or destructive.
Constructive interference means that the waves of those atomic orbitals build on each other, increasing their amplitude and the chances of finding electrons between them. This is called an in-phase overlap, forming a bonding interaction, which means that the chances of finding electrons between these two atoms is unusually high.
On the other hand, destructive interference occurs when atomic orbitals are out of phase, causing the waves to cancel each other out, creating a node where there is no mathematical chance of finding electrons. This leads to an antibonding interaction, making the atoms unstable and likely to repel each other.
It is important to note that the positive and negative lobes of an atomic orbital do not relate to electrical charges; it's just a way to think about orbitals. During constructive overlap, the whites (or positives) and grays (or negatives) are on the same side, aligning properly; during destructive overlap, they are opposite each other.
According to the Pauli exclusion principle, you can only put two electrons in each orbital. When we make our new molecular orbitals, molecular orbital pi 1 and molecular orbital pi 2, based on the overlapping atomic orbitals, both electrons can fill the lowest energy orbital, creating a bonding interaction with no electrons in the antibonding region. If we had an extra electron, it would go into the higher energy, antibonding orbital, destabilizing the bond.
In conclusion, the reason alkenes can form such good double bonds is that they have exactly two electrons to share constructively in one molecular orbital, effectively making it look like a single, low-energy molecular orbital that promotes bonding between the two. I hope this is a good start to understanding molecular orbital theory, and I will follow up with more videos explaining exactly what you need to know so you can apply this theory to solve problems.
Do you want more practice?
More setsHere’s what students ask on this topic:
What is molecular orbital theory in organic chemistry?
Molecular orbital theory (MO theory) in organic chemistry explains how atomic orbitals combine to form molecular orbitals, which are spread over the entire molecule. These molecular orbitals can be bonding, antibonding, or nonbonding. Bonding molecular orbitals result from constructive interference of atomic orbitals, increasing electron density between atoms and stabilizing the molecule. Antibonding molecular orbitals result from destructive interference, decreasing electron density between atoms and destabilizing the molecule. Understanding MO theory is crucial for predicting molecular behavior, stability, and reactivity, especially in reactions involving conjugation and resonance.
How do atomic orbitals combine to form molecular orbitals?
Atomic orbitals combine to form molecular orbitals through the process of linear combination of atomic orbitals (LCAO). When two atomic orbitals overlap, they can interfere constructively or destructively. Constructive interference leads to bonding molecular orbitals, where electron density between the nuclei increases, stabilizing the molecule. Destructive interference leads to antibonding molecular orbitals, where electron density between the nuclei decreases, creating a node and destabilizing the molecule. The resulting molecular orbitals can accommodate electrons from the combining atomic orbitals, influencing the molecule's overall stability and reactivity.
What is the difference between bonding and antibonding molecular orbitals?
Bonding molecular orbitals result from constructive interference of atomic orbitals, where the electron density between the nuclei increases, leading to a stable interaction. These orbitals are lower in energy compared to the original atomic orbitals. Antibonding molecular orbitals result from destructive interference, where the electron density between the nuclei decreases, creating a node with zero electron probability. This interaction is unstable and higher in energy compared to the original atomic orbitals. Electrons in bonding orbitals stabilize the molecule, while electrons in antibonding orbitals destabilize it.
What is the significance of hybridization in molecular orbital theory?
Hybridization is significant in molecular orbital theory as it explains the mixing of atomic orbitals to form new hybrid orbitals, which can then combine to form molecular orbitals. For example, in sp2 hybridization, one s orbital and two p orbitals mix to form three sp2 hybrid orbitals. These hybrid orbitals can overlap with other atomic or hybrid orbitals to form sigma bonds, while the remaining unhybridized p orbital can form pi bonds. Understanding hybridization helps predict the geometry, bonding, and reactivity of molecules, particularly in organic compounds like alkenes.
How does molecular orbital theory explain the stability of alkenes?
Molecular orbital theory explains the stability of alkenes through the formation of bonding and antibonding molecular orbitals. In alkenes, the sp2 hybridized carbons form sigma bonds, while the unhybridized p orbitals overlap to form a pi bond. The pi bond results from the constructive interference of the p orbitals, creating a bonding molecular orbital with increased electron density between the carbons, stabilizing the molecule. The absence of electrons in the antibonding molecular orbital further enhances stability. This delocalization of electrons in the pi bond contributes to the overall stability and reactivity of alkenes.
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