Latest / Talking Science / States of Matter – Solid, Liquid, Gas and Beyond
Transcript
- 0:00Picture this. You're sitting outside on a patio.
- 0:03On a warm, lazy afternoon. Hopefully with a cold
- 0:06drink. Exactly. You've got a tall glass of water
- 0:09in your hand, and right in the middle of it is
- 0:11this single, solitary ice cube. Just floating
- 0:14there. Right. And if you watch it for a few minutes,
- 0:17it shrinks. The sharp edges get, you know, a
- 0:19little soft, a little round, and eventually it
- 0:21just completely vanishes into the liquid. Yeah.
- 0:24It just becomes part of the water. But then,
- 0:26say an hour later, you take some of that exact
- 0:28same water, you put it in a kettle on the stove.
- 0:31and it completely disappears again, but this
- 0:33time into the air as invisible steam. It is such
- 0:39an incredibly ordinary sequence of events. I
- 0:41mean, you see it every day. But today, our mission
- 0:44for this deep dive is to take that totally ordinary
- 0:46melting ice cube and that boiling kettle and
- 0:48basically completely shatter your understanding
- 0:50of what is actually happening. Because while
- 0:53we all learn about solid, liquid, and gas in
- 0:55school, you know, the classic three states of
- 0:57matter, those are really just the prologue to
- 1:00a much, much wilder story. They really are. So
- 1:02we are going to build our understanding from
- 1:04the ground up today. We're going to look at what
- 1:07happens at the microscopic level, why boiling
- 1:10points are actually kind of an illusion, and
- 1:15why the universe's most common state of matter
- 1:17is likely one you rarely even think about. Yeah,
- 1:19exactly. We're going to look way past the everyday
- 1:22surface and focus entirely on the fascinating
- 1:25why behind these things. By the time we finish,
- 1:28you will... You'll never look at a glass of ice
- 1:31water the same way again. Okay, let's unpack
- 1:33this. Because to understand the truly bizarre
- 1:37states of matter out in the far reaches of the
- 1:40universe, we really have to start right in front
- 1:42of it. Start with the basics, yeah. Right. We
- 1:44have to define what fundamentally makes a solid,
- 1:46a solid, and then liquid, a liquid. So if we
- 1:49stop looking at the ice cube itself and zoom
- 1:51way, way down to the microscopic level, what
- 1:54is actually going on? Well, right down at the
- 1:56bottom. Every substance is built from a huge
- 1:58number of tiny particles, either individual atoms
- 2:01or molecules, which are really just groups of
- 2:03atoms bonded together. And the key thing to realize
- 2:06is that these particles are never perfectly still.
- 2:09They're constantly vibrating, jostling, moving
- 2:12around. Even in a solid. Even in a solid. The
- 2:15state that a substance is in, whether it's solid,
- 2:18liquid, or gas, is entirely the result of this
- 2:21endless tug of war. A tug of war between... Explain
- 2:24kinetic energy and attractive forces. So the
- 2:27kinetic energy is the energy of motion. That's
- 2:30the energy pushing the particles to move around,
- 2:32to vibrate and spread apart from one another.
- 2:34Right. They want to move. Exactly. But working
- 2:37directly against that. you have attractive chemical
- 2:40forces pulling the particles together, trying
- 2:42to lock them in place. So in a solid, like our
- 2:45ice cube, I'm guessing the attractive forces
- 2:47are winning the tug -of -war. Oh, they're winning
- 2:49decisively. The attractive forces are so strong,
- 2:52and the kinetic energy is relatively low, so
- 2:55the particles are just locked into fixed positions.
- 2:58But you said they're not perfectly still. Right.
- 3:00They aren't frozen dead still. They are constantly
- 3:02jiggling and vibrating in place, but they just
- 3:05don't have enough energy to break free of that
- 3:07grip and swap places with their neighbors. Oh,
- 3:09okay. That locked -in grid is what scientists
- 3:12call a crystal lattice. Well, if it forms a perfect
- 3:15repeating pattern anyway. Or amorphous, if it's
- 3:18all jumbled together. But either way, they are
- 3:21locked tight. Which, I mean, that perfectly explains
- 3:24why a solid holds its shape. If I take an ice
- 3:26cube out of my glass and put it on the table,
- 3:28it stays an ice cube. Exactly. It has a fixed
- 3:30shape and a fixed volume because the molecules
- 3:33physically cannot leave their assigned seats.
- 3:35Right. But then you leave that ice cube on the
- 3:38patio, you add heat energy from the sun, and
- 3:42that heat translates directly into kinetic energy.
- 3:45So they start jiggling faster. The particles
- 3:47start vibrating harder and faster, and eventually...
- 3:50They gain enough kinetic energy that those attractive
- 3:53forces just can't hold them rigidly in place
- 3:55anymore. The grip finally loosens. And it becomes
- 3:58a liquid. Yes. In a liquid, the particles stay
- 4:02close together. They're literally touching their
- 4:04neighbors, which is why a liquid still takes
- 4:06up a fixed volume. I mean, you can't compress
- 4:08water easily. Right, right. But because the rigid
- 4:11bonds are broken, the particles can now slide
- 4:13past one another. the exact shape of the bottom
- 4:21of its container. And then if we move from the
- 4:23patio to the stove and just keep adding more
- 4:25and more heat energy, the kinetic energy completely
- 4:29overpowers the attractive forces entirely. Complete
- 4:32domination. The particles just fly apart, moving
- 4:35totally independently as a gas. They fill whatever
- 4:37shape and volume is available. If I release a
- 4:40gas in a room, it spreads out evenly to fill
- 4:43every corner. Yeah, a really great way to visualize
- 4:45this whole sequence is to imagine a crowded dance
- 4:48floor. Oh, I like this. Imagine a solid as a
- 4:51dance floor where everyone is standing in a highly
- 4:53ordered fixed formation. You're holding hands
- 4:56with the people next to you. You can sway to
- 4:58the music. You can rock back and forth. That's
- 5:00the kinetic vibration. Exactly. That's the vibration.
- 5:04But you aren't changing your exact spot on the
- 5:06floor. So if a solid is like a synchronized line
- 5:09dance and a gas is where everyone has just left
- 5:12the building and they're spread out across the
- 5:13sprawling outdoor festival grounds, moving totally
- 5:17freely, is a liquid essentially just a really
- 5:20polite mosh pit? Yes, that is perfect. In that
- 5:24liquid mosh pit, you are still packed in tightly.
- 5:27You're bumping shoulders with everyone, taking
- 5:29up the same amount of total floor space as the
- 5:31line dancers did. But you're moving around. Right.
- 5:34You're wandering around, squeezing past people,
- 5:36swapping neighbors constantly. You don't have
- 5:39a fixed arrangement anymore. So changing states
- 5:41is fundamentally all about pumping energy into
- 5:44the system to change the dynamic on the dance
- 5:46floor. But there is a deeply surprising secret
- 5:49about what happens to temperature during that
- 5:52process, right? There really is. But first, we
- 5:55probably need to define what temperature actually
- 5:57is. Okay, lay it on me. It's not some mysterious
- 5:59invisible quality. Temperature is simply a direct
- 6:03measurement of the average kinetic energy of
- 6:05the particles in a system. It is literally just
- 6:08a measure of how fast those microscopic things
- 6:10are moving. Right. Okay, so let's trace the sequence
- 6:13on the stove. I put a block of ice in a pan and
- 6:16turn on the heat. I'm pumping energy into it.
- 6:19The particles vibrate more violently, so the
- 6:21temperature goes up. Yep. Eventually, they break
- 6:23free, sliding past each other. That's melting.
- 6:26I keep heating that newly formed liquid water.
- 6:28The molecules move faster and faster. The temperature
- 6:30goes up until they break the grip entirely and
- 6:33fly off as steam, boiling. But here is the crazy
- 6:36part. During the exact moment of a phase change...
- 6:40Like while the ice is in the process of melting,
- 6:42where the liquid water is in the actual process
- 6:44of boiling, the temperature stops rising entirely.
- 6:47Wait, really? So if I'm boiling water for pasta
- 6:49and I turn the burner all the way to maximum,
- 6:51the water itself doesn't actually get any hotter.
- 6:54The thermometer just stalls. What's fascinating
- 6:56here is that the thermometer absolutely stalls.
- 6:59At sea level, a pot of boiling water hits 100
- 7:02degrees Celsius, and it stays exactly there.
- 7:06Wow. No matter how much fire you put under that
- 7:08pot, The liquid water will not get hotter than
- 7:11100 degrees. But I'm actively pumping intense
- 7:14heat into it. If the temperature is a measure
- 7:17of kinetic energy and I'm adding energy, where's
- 7:20it going if it's not speeding up the molecules?
- 7:22It is going into what physicists call latent
- 7:25heat. Latent comes from the Latin word for hidden.
- 7:27Hidden heat. Think back to our tug of war. That
- 7:30extra heat energy from your stove isn't speeding
- 7:33up the particles anymore. Instead, it is doing
- 7:36the heavy lifting, the actual mechanical work
- 7:38of ripping those attractive bonds apart so the
- 7:41molecules can finally separate and fly away as
- 7:43a gas. So it's essentially paying the toll to
- 7:46let the particles leave the mosh pit. Precisely.
- 7:49You are physically stretching and breaking the
- 7:51electromagnetic bonds between the molecules.
- 7:53And that requires a massive amount of energy.
- 7:55I can imagine. Turning boiling water into steam?
- 7:59takes several times more energy than heating
- 8:01that same water all the way from freezing up
- 8:03to boiling in the first place. All that energy
- 8:06from your stove gets stored in the steam as hidden
- 8:09latent heat. Which honestly explains why steam
- 8:12causes much more severe burns than boiling water.
- 8:15I've always heard that, but the mechanics of
- 8:17it are wild. It's completely counterintuitive
- 8:20until you know the physics. Right. Like if boiling
- 8:22water hits your skin, it burns you with this
- 8:25100 degree temperature. But if steam hits your
- 8:28skin, it doesn't just burn you with temperature.
- 8:30It hits your cooler skin, condenses back into
- 8:32a liquid. And in that instant, it releases all
- 8:35of that massive, hidden, latent heat. All the
- 8:38energy it used to break its bonds. Exactly. Directly
- 8:40into your tissue. It is a phenomenal amount of
- 8:42energy transfer. Completely invisible to a thermometer.
- 8:45thermometer until it changes state. But this
- 8:48actually brings us to another assumption we need
- 8:50to break. OK, what's that? We just talked about
- 8:51water boiling at 100 degrees Celsius. But heat
- 8:55isn't the only variable in this molecular tug
- 8:58of war. There is an invisible hand. constantly
- 9:01pressing down on everything around us. Atmospheric
- 9:04pressure, the literal weight of the sky pushing
- 9:06down on us. Exactly. And it fundamentally alters
- 9:10the rules of boiling. Boiling point is not a
- 9:13fixed universal number. It's not. No. Let's look
- 9:16closely at how a bubble forms. When you heat
- 9:18a pot of water, a molecule at the bottom gets
- 9:21enough energy that it wants to become a gas.
- 9:23It tries to expand into a microscopic vapor bubble.
- 9:26Okay. But the entire weight of the Earth's atmosphere
- 9:29is pressing down on the surface of the water,
- 9:31crushing that little bubble before it can grow.
- 9:34Boiling only happens when the vapor pressure
- 9:36inside those bubbles is strong enough to push
- 9:38back against and overcome the atmospheric pressure
- 9:41sitting on top of the liquid. Here's where it
- 9:44gets really interesting. So atmospheric pressure
- 9:46is basically a heavy lid on a jack -in -the -box.
- 9:49That's a great way to put it. At sea level, the
- 9:51lid is pretty heavy so the little vapor springs
- 9:53inside the water need a lot of force, like a
- 9:56full 100 degrees of heat energy to pop the lid
- 9:59open and escape as bubbles. Right. But what happens
- 10:02if we take our pot of water up Mount Everest?
- 10:04Well, on Mount Everest, you have far less atmosphere
- 10:07above you. The air is thinner. The pressure pushing
- 10:10down is much weaker. So your jack -in -the -box
- 10:13lid is incredibly light. So they pop open easier.
- 10:16Exactly. Because of that, the water molecules
- 10:19don't need nearly as much energy. to push back
- 10:22and form bubbles. They don't have to fight as
- 10:24hard. So water boils at a noticeably lower temperature
- 10:27on a mountain than it does at sea level. Which
- 10:29completely ruins cooking. I mean, if you try
- 10:31to boil an egg or cook rice on Everest, the water
- 10:34boils away before it actually gets hot enough
- 10:36to cook the food. Yep, it just evaporates. The
- 10:39water is actively rolling and bubbling, but the
- 10:41liquid itself is physically cooler than a pot
- 10:44of simmering water in a kitchen at sea level.
- 10:46That's why mountaineers often complain that their
- 10:48tea tastes strangely weak at high altitudes.
- 10:50Really? I never thought about that. Yeah. The
- 10:54boiling water they pour over the leaves simply
- 10:55isn't hot enough to extract the flavor compounds
- 10:58efficiently. The mechanical action of boiling
- 11:01is happening, but the thermal energy just isn't
- 11:03there. And we use this exact same physics in
- 11:06reverse in the kitchen, right? The pressure cooker.
- 11:08We do. In a pressure cooker, you clamp a heavy
- 11:11lid on the pot and seal it tight. As the water
- 11:15heats up, steam tries to expand. but it's trapped.
- 11:18So it builds up inside. Because it can't escape,
- 11:21it pushes down on the liquid water. The pressure
- 11:24inside the pot builds up far beyond normal atmospheric
- 11:27pressure. Now, your jack -in -the -box lid is
- 11:29incredibly heavy. Ah, so the water molecules
- 11:32need a massive amount of energy to form bubbles
- 11:35against that crushing pressure. Exactly, which
- 11:37means the water is forced to reach a much higher
- 11:40temperature before it can finally boil. You get
- 11:42genuinely hotter liquid and hotter scheme, which
- 11:45drastically cuts the cooking time for tough meats
- 11:47or dried beans. Okay, so if we can manipulate
- 11:50the boiling point just by changing the pressure,
- 11:53what happens if we push both pressure and temperature
- 11:56to absolute unnatural extremes? Beyond heavy
- 12:00cooking pots, beyond mountains, do the rules
- 12:03just break? They don't just break, they vanish.
- 12:05Every substance has something called a critical
- 12:08point. This is a highly specific, extreme combination
- 12:12of temperature and pressure. And when you force
- 12:15a substance past its critical point, the ordinary
- 12:18distinction between a liquid and a gas... completely
- 12:21breaks down. Wait, how does that even look? Normally,
- 12:24if I have a half -empty water bottle, I can see
- 12:26the liquid water at the bottom and the air and
- 12:28water vapor at the top. There's a clear line,
- 12:31a physical surface boundary between them. Below
- 12:33the critical point, yes, that surface boundary
- 12:36is always there. But if you take a sealed, incredibly
- 12:39strong glass tube of liquid and gas and you start
- 12:42cranking up the heat and the pressure simultaneously,
- 12:44something bizarre happens. I'm listening. The
- 12:46liquid expands and becomes less dense. The gas
- 12:49gets compressed and becomes more dense. And right
- 12:52at the critical point, their densities perfectly
- 12:54match. You watch that visible boundary literally
- 12:57fade away and disappear into a fog. And what's
- 13:00left behind? The substance merges into a single
- 13:03phase called a supercritical fluid. A supercritical
- 13:06fluid? Yeah. It is a true physical hybrid. It
- 13:09acts like a liquid because it's dense enough
- 13:11to dissolve. other substances efficiently. But
- 13:14it acts like a gas because it has no surface
- 13:16tension. It can spread and diffuse deeply into
- 13:18tiny microscopic pores of solid materials in
- 13:21a way a liquid just can't. Are we talking about
- 13:24a ghost liquid? It sounds like it shouldn't exist.
- 13:27How can something behave like an expanding gas
- 13:29but clean like a liquid? If we connect this to
- 13:32the bigger picture, this ghost liquid is actually
- 13:35incredibly practical. The prime example is decaffeinating
- 13:38coffee. Wait, my morning decaf is made with extreme
- 13:41hybrid physics. It is. Industrially, they load
- 13:43unroasted coffee beans into a massive chamber
- 13:46and pump in supercritical carbon dioxide. Oh,
- 13:49what? Because it has gas -like diffusion, the
- 13:51supercritical CO2 penetrates deep inside the
- 13:54cellular structure of the raw coffee beans. But
- 13:57because it has liquid -like dissolving power,
- 13:59it acts as a solvent. It selectively grabs the
- 14:03caffeine molecules and pulls them out. And it
- 14:05doesn't ruin the coffee. No, because supercritical
- 14:08CO2 is highly selective. It grabs the caffeine
- 14:11but leaves the delicate flavor compounds behind,
- 14:13avoiding the harsh chemical solvents they used
- 14:16to use in the past. That's amazing. And the best
- 14:18part. When they're done, they just open a valve
- 14:20and release the pressure. The supercritical fluid
- 14:22instantly reverts back into ordinary CO2 gas.
- 14:25It just floats away, leaving absolutely zero
- 14:28chemical residue on your coffee beans. That is
- 14:30wild. Okay, so we manipulated pressure and temperature
- 14:34to get supercritical fluids. Let's look at another
- 14:36extreme. What if we just take temperature and
- 14:38push it as far as it can possibly go? What happens
- 14:41when a gas gets so hot that the kinetic energy
- 14:43just goes off the charts? Does it just get hotter
- 14:45forever? No, it eventually hits a breaking point.
- 14:48When you heat a gas to extreme temperatures,
- 14:51the particles are moving so incredibly fast and
- 14:54colliding with each other so violently that the
- 14:57atoms themselves literally begin to tear apart.
- 15:00They break. Yeah, the collisions are so forceful,
- 15:03they knock the negative electrons completely
- 15:05loose from their orbits around the atoms. Leaving
- 15:07the pieces floating around. Exactly. You are
- 15:09left with a churning soup. of free -floating
- 15:12negative electrons and the positively charged
- 15:15atomic cores they left behind. Those positively
- 15:18charged cores are called ions. So you basically
- 15:21have a highly energized ionized gas. And this
- 15:25is the fourth state of matter, plasma. And because
- 15:27the particles in this soup carry electrical charges,
- 15:30unlike ordinary neutral gas atoms, it behaves
- 15:33completely differently, right? Very differently.
- 15:35Because of all those free -floating charges.
- 15:37Plasma conducts electricity incredibly well,
- 15:40and it responds very strongly to magnetic fields.
- 15:43Ordinary gases don't care about magnets. Plasma
- 15:46does. So what does this all mean? Is this just
- 15:48something that happens inside a fusion reactor?
- 15:51Not at all. You actually see plasma on Earth
- 15:53all the time. Really? Where? If you look at a
- 15:56glowing neon sign, the gas inside that glass
- 15:59tube is being energized by a high voltage electrical
- 16:02current until electrons are knocked loose and
- 16:05it becomes a glowing plasma. Oh, I had no idea.
- 16:07Yeah. A lightning bolt is a brief, violent tube
- 16:11of plasma superheating the air. Even the very
- 16:14tip of a candle flame has a tiny bit of plasma
- 16:17dancing in it. But Earth is kind of the exception
- 16:19here, right? Yes, very much so. To really appreciate
- 16:22plasma, you have to look up. Out in the cosmos,
- 16:25plasma is king. The sun, and virtually every
- 16:28single star in the night sky, is an unfathomably
- 16:31massive ball of plasma. That makes sense given
- 16:34the heat. The heat and pressure is so intense
- 16:36that atoms just cannot hold on to their electrons.
- 16:39Even the vast, seemingly empty space between
- 16:41stars and galaxies is filled with a very thin,
- 16:45invisible mist of plasma. Wait, if the stars
- 16:47are plasma and the space between the stars is
- 16:50plasma, does that mean solid, liquid, and gas?
- 16:52The things we think of as the normal states of
- 16:54matter are actually the weird... rare exceptions
- 16:57in the universe. It really does. Physicists joke
- 17:00about it, but it's factually true. By volume,
- 17:04plasma makes up the overwhelming majority of
- 17:06all ordinary matter in the observable universe.
- 17:09Solid, liquid, and gas only really exist on relatively
- 17:13cool dense little rocks like Earth. That completely
- 17:16flips my perspective. The default state of the
- 17:18universe is a glowing, electrically charged soup.
- 17:21Okay, so extreme heat rips atoms apart into plasma.
- 17:25What about the exact opposite? What if we remove
- 17:27almost all the energy? What happens when we approach
- 17:29absolute zero? Absolute zero is the coldest temperature
- 17:32theoretically possible. It's minus 273 .15 degrees
- 17:36Celsius. It is the absolute floor of physics,
- 17:39the point where kinetic energy is almost entirely
- 17:41gone. The motion just stops. Exactly. In 1995,
- 17:44scientists decided to see what would happen if
- 17:46they pushed matter right up to that edge. They
- 17:48used a complex setup of lasers and powerful magnets
- 17:51to cool a small cloud of atoms down to just a
- 17:54tiny fraction of a degree above absolute zero.
- 17:56Wait, lasers? Lasers are intense beams of light.
- 17:59They burn things. How on earth do you use a laser
- 18:01to cool something down to absolute zero? It sounds
- 18:04totally counterintuitive, I know. But remember...
- 18:07Cooling something down just means slowing the
- 18:09atoms down. Right, kinetic energy. Atoms are
- 18:12flying around wildly. Yeah. If you tune a laser
- 18:14perfectly, you can fire a stream of photons,
- 18:17particles of light, directly at an atom that
- 18:20is moving toward the laser. When the atom absorbs
- 18:22that photon, the impact pushes back against it,
- 18:25slowing its momentum just a tiny bit. Ah, like
- 18:28a head -on collision. Yes. It's like throwing
- 18:31millions of ping -pong balls at a rolling bowling
- 18:33ball. Eventually, the bowling ball slows to a
- 18:36halt. Okay, that makes sense. So they trap this
- 18:38little cloud of atoms, they bombard it with lasers
- 18:40from all sides until the atoms basically stop
- 18:42moving. And what happened? Did it just become
- 18:45the hardest, most brittle solid ever? No, it
- 18:48did something far stranger. At that incredibly
- 18:50low temperature, everyday classical physics completely
- 18:53breaks down and the bizarre rules of quantum
- 18:56mechanics take over. Things get weird. Very weird.
- 18:59You see, in quantum mechanics, particles also
- 19:01act like waves. Normally, those waves are incredibly
- 19:05tiny. But as the atoms got colder and colder
- 19:08and slower and slower, their quantum waves began
- 19:11to stretch out and expand. And since they were
- 19:13trapped in a tight magnetic field, their expanding
- 19:16waves began to overlap. And when they overlapped,
- 19:18the individual atoms actually lost their separate
- 19:21identities. They stopped being a collection of
- 19:23distinct individual particles and merged into
- 19:26a single unified quantum wave. They acted as
- 19:29one single giant entity. So if we take our dance
- 19:32floor analogy down to absolute zero, is it like
- 19:35the music completely stops, the temperature drops,
- 19:38and everyone freezes so perfectly still that
- 19:40their physical bodies literally blur together
- 19:42and become one giant singular dancer? Yes. From
- 19:45a quantum perspective, the dancers lose their
- 19:48individuality entirely. You can no longer point
- 19:50to an atom and say, oh, that one is atom and
- 19:52that one is atom B. They're all everywhere at
- 19:54once within that trap. That's terrifying and
- 19:56amazing. This state is called a Bose -Einstein
- 19:59condensate. It was predicted mathematically by
- 20:02Albert Einstein and Satyendra Nath Bose in the
- 20:051920s, decades before we had the laser technology
- 20:08to actually create it. Wow. They just knew the
- 20:10math worked out. Yeah. When scientists finally
- 20:13achieved it in 1995, it won the Nobel Prize because
- 20:17it gave scientists a way to observe quantum behavior,
- 20:20which is normally invisibly small, on a macro
- 20:22scale that we can actually look at. That is incredible.
- 20:25And this raises an important question, you know,
- 20:27about how limited our everyday perception of
- 20:30the universe actually is. Because the deeper
- 20:32physicists look, the more exotic states they
- 20:34find. Have you ever heard of a super solid? I've
- 20:37heard the term, but I have no idea what it actually
- 20:40is. If you cool certain liquids, like liquid
- 20:42helium, down close to absolute zero, they undergo
- 20:45quantum phase change and become a superfluid.
- 20:48In a superfluid, the liquid has absolutely zero
- 20:50internal friction. None. Its viscosity is zero.
- 20:54How does that even work? Well, if you stir a
- 20:56cup of coffee, it eventually stops spinning because
- 20:59the fluid rubs against itself and the cup. If
- 21:01you stir a cup of superfluid helium, it will
- 21:04spin forever. No way. Seriously. In fact, because
- 21:07it has zero friction, a superfluid will literally
- 21:10creep up and over the walls of its container.
- 21:13defying gravity just to find a lower energy state.
- 21:16Wait, it just crawls out of the bowl? It crawls
- 21:18right out of the bowl. And on the other end of
- 21:20the extreme, beyond plasma, you have something
- 21:22called quark -gluon plasma. If you smash atoms
- 21:24together in a particle accelerator with enough
- 21:27unbelievable heat and force, you don't just knock
- 21:30the electrons loose. What happens? You literally
- 21:32shatter the protons and neutrons themselves into
- 21:35their fundamental building blocks, quarks and
- 21:36gluons. It's a state of matter that hasn't existed
- 21:40naturally since the first fractions of a second
- 21:42after the Big Bang. It completely humbles you.
- 21:45I mean, our whole lives are built around solid,
- 21:47liquid and gas, the ice cube, the water, the
- 21:49steam. But they are just a tiny, fragile sliver
- 21:53of reality dictated by the very specific, very
- 21:57moderate temperature and pressure we happen to
- 21:59live in on the surface of the Earth. They are
- 22:01definitely the exception, not the rule. So the
- 22:04next time you are sitting on the patio and you
- 22:05watch that ice cube melt in your glass, I hope
- 22:08you look at it with a newfound respect. It's
- 22:11not just water warming up. Not at all. It is
- 22:14a quiet, microscopic demonstration of latent
- 22:17heat. It's the eternal tug of war between kinetic
- 22:21energy and attractive bonds. It is the exact
- 22:24same foundational physics that dictates how a
- 22:26pressure cooker traps steam, why neon signs glow,
- 22:30what powers the blazing heart of the sun, and
- 22:32what happens when atoms blur together into a
- 22:34single quantum dancer in the coldest high -tech
- 22:37laboratories on Earth. And I'll leave you with
- 22:39this one final thought to ponder. All right,
- 22:42what is it? We only discover things like supercritical
- 22:44fluids and boson sine condensates because human
- 22:47beings invented incredibly complex machines to
- 22:50force matter into artificial extremes of temperature
- 22:53and pressure. But the universe has natural extremes
- 22:55we can barely fathom. What completely unknown,
- 22:58unimaginable states of matter might currently
- 23:01exist naturally inside the crushing gravity of
- 23:04a black hole or deep within the unimaginably
- 23:07dense core of a neutron star just waiting for
- 23:10us to figure out they are there. Man, it makes
- 23:12the universe feel a lot bigger and a lot stranger.
- 23:15Thank you so much for joining us on this deep
- 23:17dive. We'll catch you next time.