Latest / Mechanical Engineering Made Simple / (#99) The Myth of the Perfect Burn
Transcript
- 0:00Welcome back to mechanical engineering made simple.
- 0:02It's great to be back. Today I want to start by asking
- 0:05everyone listening to do something for me.
- 0:08Picture the engine in your car, or maybe a massive gas turbine
- 0:13on a jet wing. When we think about what's
- 0:15happening inside, we usually have this very sanitized high
- 0:20school chemistry version of it. The textbook burn as we like to.
- 0:24Call. It's this neat little equation.
- 0:26You have fuel, you add air, you get a spark and poof, you get
- 0:29heat, carbon dioxide and water. It's, you know, linear clean.
- 0:33And it implies that if you just get that mixture right, you get
- 0:36100% energy release and totally harmless exhaust.
- 0:40Which is a lovely fiction. It really is.
- 0:42If combustion were that simple, my job and the jobs of thousands
- 0:46of combustion engineers, well, we just wouldn't exist because
- 0:49the. Reality is less of a polite
- 0:51handshake and more of a a riot. A battlefield, That's the word
- 0:55for it. If you can zoom into the
- 0:57molecular level inside that cylinder, you're not seeing a
- 1:00one way street where reactants just become products.
- 1:02No, you're seeing a chaotic state of what we call dynamic
- 1:07equilibrium. And that concept, dynamic
- 1:09equilibrium, that's really the heart of this deep dive, isn't?
- 1:13It is. We're going to walk through the
- 1:15story of a combustion reaction to answer some of the most
- 1:17popular questions we see online. Specifically, why don't engines
- 1:22get as hot as the math says they should?
- 1:25And the big one, Where do all these nasty pollutants actually
- 1:29come from if we're burning so-called clean fuel?
- 1:32The answers you're saying boil down to two invisible forces.
- 1:35Two invisible forces fighting against perfect efficiency.
- 1:38First, you've got dissociation, which acts like an energy thief.
- 1:41OK, the thief. And then you've got kinetics,
- 1:43which is basically a cosmic speed limit.
- 1:45All right, let's. Unpack this starting with the
- 1:47thief dissociation. To get this we have to look at
- 1:49equilibrium. Most of us remember the standard
- 1:52equation, right? Carbon monoxide, Co plus oxygen,
- 1:55O2. Makes carbon dioxide, CO2
- 1:58stable. Done.
- 2:00But that's the cold view. It implies that once CO2 forms,
- 2:03it just stays that way. But inside an engine, we're
- 2:06talking about temperatures pushing, you know, 2500, maybe
- 2:093000 Kelvin. That's incredibly hot.
- 2:11At those energy levels, the product molecules themselves are
- 2:13vibrating so violently that they start to shatter.
- 2:16What The exhaust is kind of unburning itself.
- 2:19In a way, yeah, that's a good way to put it.
- 2:21The reaction actually becomes reversible.
- 2:23CO2 splits back into carbon monoxide and oxygen, and water
- 2:28vapor rips apart into hydroxyl radicals and hydrogen.
- 2:32That process is dissociation, and it's all dictated by the
- 2:35absolute grandfather of thermodynamics, Gibbs energy.
- 2:39Right Gibbs, denoted by GI. Remember, the definition
- 2:43involves enthalpy minus the temperature times entropy.
- 2:45That's the one. And the key thing to remember is
- 2:48that the universe is fundamentally lazy.
- 2:50Any chemical system will always, always try to move toward the
- 2:53state with the lowest possible Gibbs energy.
- 2:56I always picture this is a ball rolling around a landscape of
- 2:58hills and valleys. That's a perfect analogy.
- 3:00The gas mixture is the ball and it's just looking for the
- 3:04deepest valley it can find. And the composition of the gas,
- 3:07how much fuel versus exhaust is the balls position?
- 3:09Exactly. And the depth of the valley is
- 3:11the energy state. So the mixture keeps reacting
- 3:14forward, then backward, shifting its composition until it finds
- 3:17the absolute bottom of that valley where the is 0.
- 3:21That's the point where DG the change in Gibbs energy is 0.
- 3:26That's equilibrium. Correct, but here's the catch
- 3:28that trips people up that landscape.
- 3:32It isn't static. The shape of the whole valley
- 3:35changes depending on pressure and temperature.
- 3:37So when you crank up the temperature in an engine, you're
- 3:40basically warping the landscape. You're completely reshaving it.
- 3:43The bottom of the valley moves, so at room temperature the
- 3:46bottom might be mostly CO2, but at 3000 Kelvin the bottom shifts
- 3:51to a mix of CO2, Co and oxygen. And what's the actual force
- 3:56pushing the ball around this landscape?
- 3:58That's something called chemical potential.
- 4:00You can think of it like chemical pressure.
- 4:02Just like air flows from high to low pressure, chemical species
- 4:05flow from high chemical potential to low chemical
- 4:08potential. The reactants are pushing to
- 4:10become products, but at these high temperatures, the.
- 4:13Products are pushing back. Precisely, and equilibrium is
- 4:17just the ceasefire line where the chemical potential of the
- 4:20reactants equals the chemical potential of the products.
- 4:23OK, that's the theory, but let's apply the So what factor?
- 4:27If I'm designing a Formula One engine, why do I care if 5 or
- 4:3110% of my molecules decide to break up?
- 4:33You care because it steals your power.
- 4:35This is why we call it the energy thief.
- 4:37Breaking those chemical bonds, turning CO2 back into Co and
- 4:41oxygen is endothermic. It absorbs heat.
- 4:44It absorbs huge amounts of it. It sucks thermal energy right
- 4:47out of the explosion. So let's say you do a quick
- 4:49calculation on a napkin. Assuming perfect combustion,
- 4:52your calculator says, congratulations, you're going to
- 4:55hit 2950 Kelvin. Which means a massive pressure
- 4:58spike, which means lots of torque on the crankshaft.
- 5:01Right, but then you run the actual engine and you only
- 5:05measure 2800 Kelvin. You've lost one 150° off the
- 5:09top. And that energy didn't just leak
- 5:11out through the cylinder walls. No, it was consumed internally
- 5:15by the molecules tearing themselves apart, and that's a
- 5:18direct loss in peak pressure, which is a direct loss in work
- 5:22output. That's a huge efficiency hit,
- 5:25and I see in the notes there's a metric for this alpha, the
- 5:28degree of dissociation. Yeah, alpha is just a fraction
- 5:31of the original molecule that's broken down.
- 5:34If alpha is 0, you've got a stable molecule.
- 5:36If alpha is 1, it's completely disintegrated.
- 5:39And engineers have some levers to pull here, right?
- 5:41We're not completely helpless. We have two main livers,
- 5:44pressure and temperature, and they work against each other.
- 5:48OK, walk us through the pressure side first.
- 5:50So think about what happens when things dissociate.
- 5:53Let's say 2CO2 molecules breakdown.
- 5:55They turn into two Co molecules plus one O 2 molecule.
- 5:58So you started with two particles and you end up with
- 6:01three. Exactly.
- 6:02Dissociation increases the total number of moles in the gas.
- 6:06It wants to take up more space. O applying Alicia Teles
- 6:09principle, if you squeeze the system, increase the pressure,
- 6:13it's going to fight back. It will try to relieve that
- 6:16stress by shifting toward the side with fewer molecules, which
- 6:20is the non dissociated side. So a high compression ratio in
- 6:24an engine actually helps suppress dissociation.
- 6:27It does high pressure kind of keeps the family together, but
- 6:30temperature does the complete opposite.
- 6:32It adds violent kinetic energy and encourages the breakup.
- 6:35That is such a cruel trade off, isn't it?
- 6:38The Carnot cycle tells us we want high temperatures for the
- 6:40best theoretical efficiency, but those same high temps trigger
- 6:44the dissociation that steals that very efficiency.
- 6:47Welcome to engineering. It's never just one variable,
- 6:50and there's a neat little nuance here in the data Water is
- 6:53tougher than carbon dioxide. Meaning H2O doesn't break down
- 6:57as easily. Right, in your typical
- 6:59hydrocarbon combustion, the water molecules dissociate a lot
- 7:02less than the CO2 molecules at the same temperature.
- 7:05The water is just more stable. OK, so we can't just guess at
- 7:08this. If I'm building a simulation, I
- 7:10need a number. How do we calculate where this
- 7:13balance point actually is? For that we use the equilibrium
- 7:17constant, which we call K sub P It's a value that tells us the
- 7:21exact ratio of products to reactants at a specific
- 7:24temperature based on their partial pressures.
- 7:27And the sources mentioned the Van Hoff equation here.
- 7:30The Van Hoff equation is just a beautiful way to show how that
- 7:33case of P constant changes with temperature.
- 7:36It linearizes the problem. If you plot the natural log of
- 7:40case of P against one over temperature, you get a straight
- 7:43line. That sounds great for a chart,
- 7:45but looking at the actual math, this seems really hard to
- 7:48calculate by hand. You're ending up with cubic
- 7:50equations and systems of non linear equations.
- 7:53It's a total nightmare to do by hand.
- 7:54It looks like the method is basically guess and check.
- 7:56That's essentially what it is. It's an iterative loop.
- 8:00You see, you can't solve for the final temperature directly
- 8:03because the final composition depends on the temperature.
- 8:06But the temperature depends on the heat release, which depends
- 8:08on the composition. It's a circular reference.
- 8:11Exactly. So you have to guess a final
- 8:13temperature. Then you calculate K sub P for
- 8:16that temperature. Find the composition.
- 8:18Then you check the energy balance.
- 8:20Did the heat released match your guess?
- 8:23And it probably didn't. Almost never in the first try.
- 8:26So you adjust your guess and you do the whole loop again and
- 8:29again until it converges. I'm very glad we have software
- 8:32like Matlab or Python to handle that iterative part now.
- 8:35We are too, but you have to understand the logics to set it
- 8:38up. But here's the thing.
- 8:40Even with a perfect computer model, equilibrium has one fatal
- 8:45flaw, which is it assumes you have infinite time.
- 8:49It assumes the molecules can just hang out, bump into each
- 8:51other, and comfortably settle into that lowest energy state.
- 8:54And inside an engine cylinder, Comfortable is the last word I'd
- 8:57use, right? Let's think about the clock.
- 8:59If your engine is running at 6000 RPM, that's 100 revolutions
- 9:03a second. The entire 4 stroke cycle
- 9:05happens in 10 milliseconds. And the actual combustion event
- 9:08maybe? Two to three milliseconds.
- 9:10That is just insanely fast. It's faster than the chemistry
- 9:14can keep up with sometimes. And that brings us to our second
- 9:17invisible force, chemical kinetics.
- 9:21The speed limit. Exactly.
- 9:23Equilibrium tells you what would happen if you waited forever.
- 9:26Kinetics tells you what actually happens in the three
- 9:28milliseconds you've got. So thermodynamics is the
- 9:31destination, but kinetics is the rush hour traffic.
- 9:34I like that. That's good.
- 9:36Reactions are a contact sport. They only happen when molecules
- 9:40physically collide. So first you need a crowded
- 9:43room. We call that molar
- 9:45concentration. The higher the density, the more
- 9:47collisions. But just bumping into each other
- 9:49isn't enough, is it? No.
- 9:51If they just gently bump, they bounce off.
- 9:54Nothing happens. They need to smash into each
- 9:56other with enough force to actually shatter their existing
- 9:59bonds so new ones can form. And that minimum energy
- 10:02threshold is the activation energy E.
- 10:05Right, and this is all governed by the Arrhenius equation.
- 10:07It is the famous rate constant K = a times E to the power of
- 10:12negative E over RT. It looks scary, but you're
- 10:15right, it tells a simple story. The A part is just how often
- 10:18they collide. And the exponential term is the
- 10:20gatekeeper. It tells you what fraction of
- 10:23those collisions actually have enough energy to get over that
- 10:26activation hurdle. And if the temperature T drops,
- 10:30that exponential term crashes towards 0 incredibly fast.
- 10:35And this the speed limit. This is where the story gets
- 10:38darker, isn't it? Because this lack of time is the
- 10:40origin story for most of our pollutants.
- 10:43It is. Let's talk about thermal and
- 10:45onitric oxide. OK, so in the air all around us,
- 10:48nitrogen and oxygen are like strangers on a subway.
- 10:50They're in the same space, but they totally ignore each other.
- 10:53At room temperature, yes, the activation entity to break that
- 10:57triple bonded nitrogen molecule is just massive.
- 11:00But inside the engine at those peak flame temperatures, 3000
- 11:04Kelvin. We have enough energy.
- 11:06The Arrhenius gatekeeper opens the door.
- 11:08Right, the Zeldovich mechanism kicks in.
- 11:10It's a chain reaction where free nitrogen atoms start attacking
- 11:13oxygen molecules and suddenly you're making NO.
- 11:16But wait. Following our equilibrium logic,
- 11:19as the piston moves down, the gas expands and cools.
- 11:22The energy valley should shift back.
- 11:24The NO should want to break up and go back to being harmless N2
- 11:28and O2. It wants to.
- 11:30Thermodynamics says it absolutely should, but kinetics
- 11:33says sorry, you're too slow. The expansion happens too
- 11:37quickly. Way too quickly as the
- 11:39temperature plummets during that expansion stroke.
- 11:41Look at the Arrhenius equation again.
- 11:43The rate for the reverse reaction breaking down NO, just
- 11:46hits a wall. The rate goes to effectively 0.
- 11:49So the NO gets trapped. It's frozen in the mixture.
- 11:51We call it frozen equilibrium. The chemical composition is
- 11:54literally frozen in its high temperature state even though
- 11:57the gas itself is cooled down. The NO is a fossil of the
- 12:01combustion peak. And it gets pumped out the
- 12:03tailpipe before it ever has time to decompose.
- 12:06That's a really powerful image. The pollution is a snapshot of
- 12:09the chaos that didn't have time to clean itself up.
- 12:11Exactly. And it's not just no think about
- 12:14soot or particulates. This happens in rich zones of
- 12:18the chamber. Rich meaning too much fuel, not
- 12:20enough air, right? Like in a diesel engine near the
- 12:23surface of an injected fuel droplet, it's super rich,
- 12:27there's not enough oxygen to go around, so the carbon atoms,
- 12:29they just start bonding with each other.
- 12:31Forming chains and then sheets and clumps, creating those
- 12:35little sip particles. And once those solid particles
- 12:38form, burning them back up takes even more time and heat.
- 12:41If the cycle ends before that can happen, you get black smoke.
- 12:46And sulfur dioxide SO2. That was a simpler villain.
- 12:49It's just an impurity in the fuel.
- 12:51If there's sulfur in your diesel or gasoline, it burns and
- 12:54becomes SO2, which leads to acid rain.
- 12:57The only fix there is to clean the fuel at the refinery.
- 12:59And then there's the big one, carbon dioxide.
- 13:02The one that's unavoidable. That one is the fundamental
- 13:04product. It's not a mistake of kinetics.
- 13:07If you burn a hydrocarbon you are going to get CO2.
- 13:09The only way to stop making it is to burn less fuel or burn a
- 13:13fuel with no carbon, like hydrogen.
- 13:15So this all comes together into what we call the engineer's
- 13:17dilemma. It's a nasty optimization
- 13:19problem. To get maximum power and
- 13:21efficiency, thermodynamics demands high temperatures.
- 13:24But high temperatures cause dissociation which steals your
- 13:27energy, and high temperatures activate the Zelda Vich
- 13:30mechanism which creates smog. You're fighting physics on 2
- 13:34fronts. You push for efficiency, you get
- 13:36pollution, you lower the temperature to cut pollution,
- 13:39you lose efficiency, and you burn more fuel.
- 13:42It's a vicious cycle. So what's the fix?
- 13:45How have we been cheating the system?
- 13:47For the last 40 years, the main answer has been to clean up the
- 13:49mess afterwards. That's the catalytic converter.
- 13:52The Magic Platinum box and the exhaust.
- 13:54It's a little chemical factory. It takes the unburned fuel, the
- 13:57Co and the NO, and it forces them to finish the reactions
- 14:01that kinetics froze inside the engine.
- 14:03But I've heard they're incredibly fussy.
- 14:05They are. They need an almost perfectly
- 14:07balanced or a stoichiometric mixture of air and fuel to work.
- 14:11We call it Lambda equals 1. Why is that?
- 14:14If you're too rich, there's no oxygen left to burn the leftover
- 14:17fuel in the catalyst. If you're too lean, there's too
- 14:20much oxygen and you can't chemically reduce the NO back to
- 14:24nitrogen. Which explains why cars have
- 14:26oxygen sensors and computers constantly adjusting the fuel
- 14:29injection. They're trying to walk that
- 14:32razor's edge. Thousands of times a second.
- 14:35There are other strategies like lean burn where you run with
- 14:38lots of excess air. Which lowers the peak
- 14:40temperature. Right, it acts like a heat sink.
- 14:42Lower temp means almost no NO formation, which is great and
- 14:46it's sufficient, but your standard three-way catalyst
- 14:49stops working in that oxygen rich exhaust.
- 14:52So then you have to invent whole new complex catalyst systems.
- 14:57It's a never ending game of whack a mole.
- 14:59It feels like we're just bound by the limits of a heat engine.
- 15:02We are. We're trapped by the second law
- 15:03of thermodynamics. As long as we're making heat to
- 15:06push a piston, we're stuck in this cycle of dissociation and
- 15:09frozen kinetics. So is.
- 15:11There a way to just flip the table to exit this game
- 15:14completely? There is, and it brings us right
- 15:17back to Gibbs Energy, the fuel cell.
- 15:19Now a fuel cell isn't a heat engine at all.
- 15:22Not at all. It's an electrochemical device
- 15:24doesn't burn the fuel. It takes the chemical energy,
- 15:26the Gibbs free energy, and converts it directly into
- 15:28electricity. So it completely skips the fire
- 15:31step. Which means it skips the Carnot
- 15:32efficiency limit, and because it runs at much lower temperatures,
- 15:35you don't have dissociation stealing energy, and you
- 15:37certainly don't have the Zeldovich mechanism creating
- 15:41thermal NO. So in theory, it solves both of
- 15:43the invisible villain problems we started with.
- 15:46In theory, yes. Now they have their own huge
- 15:48engineering challenges, cost, durability, hydrogen storage.
- 15:53But from a pure thermodynamic standpoint, they're a much more
- 15:56elegant way to get the energy out of a molecule.
- 15:58It really changes your perspective.
- 16:00You think you're just pressing A pedal to go faster?
- 16:02But what you're really doing is orchestrating a high speed
- 16:06molecular war, trying to manage a chaotic explosion, freeze time
- 16:12to capture the work, and then scrub the casualties out of the
- 16:15exhaust. It gives you a lot of respect
- 16:17for the engineers who make that happen seamlessly for hundreds
- 16:20of thousands of miles. It's a miracle of control
- 16:22engineering that it works at all.
- 16:24So to recap, the perfect burn is a myth.
- 16:27Real combustion is a balancing act between the energy stolen by
- 16:31dissociation and the ticking clock of kinetics.
- 16:34And while we've gotten very good at masking those imperfections,
- 16:37the underlying physics hasn't changed.
- 16:39Which leaves us with a final thought to Mull over.
- 16:43We're in this massive push for 0 emission vehicles like EVs, but
- 16:47we have to remember the whole system if the electricity for
- 16:50that EV comes from a natural gas power plant.
- 16:53You haven't eliminated the dissociation or the kinetics
- 16:56problems, you've just moved them from your tailpipe to a
- 17:00smokestack 100 miles away. The chemistry doesn't disappear,
- 17:03it just relocates. The only way to truly beat the
- 17:06limits of the heat engine is to stop using heat engines all
- 17:10together. Whether that's solar wind or
- 17:13electrochemical cells, yeah, you have to step out of the cylinder
- 17:16entirely. That's the only way to win the
- 17:18game. A heavy thought to end on if you
- 17:20haven't already, get over to our YouTube channel Mechanical
- 17:22Engineering Made Simple, where we post hands on how to videos,
- 17:25visual breakdowns, and practical engineering walkthroughs you can
- 17:28actually use. A family that solves together
- 17:31stays together.