Sherlock & Co.

Introducing: The Rest Is Science

12 min
Dec 4, 20255 months ago
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Summary

Michael Stevens and Professor Hannah Fry introduce their new science podcast 'The Rest is Science,' exploring gravity through multiple theoretical frameworks. They discuss Newton's gravitational model, Einstein's revolutionary spacetime curvature theory, and practical implications like how time passes at different altitudes.

Insights
  • Einstein's spacetime curvature model solved longstanding problems with Newtonian gravity, particularly Mercury's orbital precession, by reconceptualizing gravity as geometry rather than force
  • Gravity operates at the speed of light, not instantaneously, which has profound implications for how we understand celestial mechanics and the propagation of gravitational effects
  • Gravitational effects vary measurably across Earth's surface due to altitude differences, causing time to pass at different rates in different locations (5.6 microseconds/year difference between Boulder and Greenwich)
  • Complex scientific concepts require analogies and accessible language to communicate abstract ideas like spacetime curvature to general audiences
  • The progression from Newton to Einstein represents a paradigm shift from force-based to geometry-based physics, fundamentally changing how we model reality
Trends
Science communication moving toward narrative-driven exploration of fundamental concepts rather than answer-focused educationIncreased focus on making abstract physics accessible through relatable analogies and thought experimentsGrowing audience interest in understanding the historical evolution and competing theories within scientific fieldsPodcast format enabling deep-dive discussions of complex scientific topics with expert co-hostsEmphasis on curiosity-driven inquiry as the engine of scientific progress
Topics
Gravitational Theory and Newton's LawsEinstein's General Relativity and Spacetime CurvatureMercury's Orbital PrecessionSpeed of Light as Universal Speed LimitGravitational Attraction Between ObjectsTime Dilation and Altitude EffectsSpacetime as Geometric CanvasInverse Square LawGravitational Force PropagationComparative Physics TheoriesScience Communication and AnalogiesAstrology vs. PhysicsVacuum and Free FallMass and Gravitational EffectsThought Experiments in Physics
Companies
Gohanger
Production company hosting the new podcast series 'The Rest is Science' featuring Stevens and Fry.
People
Michael Stevens
Co-host of 'The Rest is Science' podcast, introducing the new show and discussing gravity theories.
Professor Hannah Fry
Co-host of 'The Rest is Science' podcast, expert discussing Einstein's relativity and gravitational theory.
Isaac Newton
Historical physicist whose gravitational force model is discussed as foundational but incomplete theory.
Albert Einstein
Physicist whose spacetime curvature theory revolutionized understanding of gravity and solved Mercury's orbital problem.
Quotes
"Because that's what moves science forward, not the polishing of answers but the sharpening of questions."
Michael Stevens
"The simplest way to think of it is that in our universe objects are attracted to each other."
Professor Hannah Fry
"We are gravitationally attracted to each other right now. It cannot overcome the air."
Professor Hannah Fry
"What if it's the shape of the canvas that we are on?"
Michael Stevens
"Time travels slower in Greenwich than it does in Boulder. The difference is about 5.6 microseconds a year."
Professor Hannah Fry
Full Transcript
Hello Sherlock listeners, I'm Michael Stevens. And I'm Professor Hannah Fry. Well thank you John and Sherlock for letting us take over the channel. We are here to tell you about our new show for Gohanger, The Rest is Science. Every week we take a fresh look at the familiar, we're going to be exploring the forces, the theories and the phenomena that shape how we live in, think about and see the world. We are going to pull apart what we take for granted to reveal the unexpected patterns and hidden logic just beneath the surface. Because that's what moves science forward, not the polishing of answers but the sharpening of questions. It's curiosity that sparks those. Hey wait, how does that actually work kind of a moment that changes the way we see the world? So okay here is a little glimpse of what has to come from our focus and if it sparks something unexplainable for you, then you can join us every Tuesday and Thursday for new episodes of The Rest is Science. I will figure it out together. How would you describe gravity to an alien from another universe that had never experienced gravity? The simplest way to think of it is that in our universe objects are attracted to each other. And if you, without any interfering from outside, if you just have two objects near each other, they will come together. That's it. I mean that's it really. The alien goes, what? That is so odd. Right. And what do you mean by an object? Anything with mass. Anything with mass. Because I think that we sort of imagine gravity as though it's like the earth is pulling us down. But the thing is, is that we're also pulling the earth up. Right? And if you get much smaller objects than planets and you put them in space, they're pulling each other and we'll come together. That's right. And we calculated the two baseballs placed in intergalactic space. A meter apart would very slowly collapse in towards each other until they touched. It would take three days for that to happen, but it would be because of their gravitational attraction to each other. We are gravitationally attracted to each other right now. It cannot overcome the air. It would have to push out of the way, the friction between our butts and the seats, but yet we are attracted. In fact, when you're born, right, you've got some zodiac constellation that's like, I don't know, it's, how does astrology work? Something, something, something, Pisces. Right. Okay. You're a Pisces if you're born in a particular time of the year. But yet the gravitational influence of Pisces on you is less than the gravitational influence of the doctor who delivered you on you. Because otherwise, but thank you for working. That's why people are like, oh, you're an Aquarius. And I'm like, no, I'm a schnit cookie. Because Dr. Schnit cookie was there influencing me at a physical level. Yeah. Not just the catching, not just the physical touch, but the gravitational attraction to his mass. Right. We've been talking a lot about very like fundamental things in this really abstract way to just explain that things fall down. Because here on earth, they're attracted to the earth. And you were talking about how it's not just the earth pulling things in. Things pull the earth as well. But the earth is so much bigger than everything else we work with that equal attraction they have affects other stuff, like a pen, a lot more than it does the earth. But I once calculated that if you dropped a pen from six feet up, it actually pulls the earth up towards it, nine trillions, the width of a proton. Oh, which is by my calculation, small, it's very small. So the pen falls the remainder of that distance, which is still pretty much six feet, but they all coming to meet each other. But they're coming to meet each other somewhere in between. Yeah. It just happens to be a much longer trip for the pen. And there you've got both of those senses of mass happening together, the gravitational attraction, but then also that force moves each object with very different accelerations. I mean, that pen though is particularly light. If you take an object that is heavier, denser, I mean, heavy, actually, there's sort of an implication of gravity in that statement itself, right? But if you take something that has more matter, the amount that the earth would move would change too. That's right. That's right. So when people say a feather in a hammer dropped in a vacuum, so there's no air to move out of the way, they will fall at the same rate. They'll hit the ground at the same time. I tell you what, why don't we just clear up the question of what is gravity according to what different people thought at different times? Yeah. Because everything you're describing so far is essentially like a Newtonian view of gravity. So Newton has this idea that actually gravity is all about objects accelerating towards each other, right? Like forces, mass times acceleration was one of his, was one of his laws. And he was saying that we are accelerating towards the earth, which is the reason why when you chuck an apple or any object, your baseball, if you like, when you chuck it, it accelerates towards the earth and follows this curved path. And everyone for, you know, many hundreds of years was like, that guy Newton, he's, he's got it made. He's done it for us. That's perfect. But there were still some lingering question, some little things that didn't quite make sense. So, for instance, where is this, how is this force sort of acting? Like let's say you took the sun and you had like a magic wand that made the sun disappear instantaneously. It would take eight, nine minutes for the light to hit us. But according to Newton's version of gravity, we would immediately stop accelerating towards the sun, which means that the earth should immediately spin off into the blackness of space. It doesn't really make any sense, right? Because isn't it that nothing can travel faster than the speed of light? So how can it be that we would feel the loss of the gravitational pull of the sun before the light switched out? Right. Yeah. And so we know for a fact today that gravity travels how fast speed of light, speed of light, no faster. Work is, it's a, the universal speed limit. Yeah. Certainly, it's not instantaneous. Absolutely. Which means that if the sun suddenly vanished, we wouldn't know about it at all. But was that a problem for Newton? Newton, no. But as the time went on, people were like, let's say a bit fishy going on. Sorry, a bit weird. I'm not sure I like this. Yeah. The other one that was a bit weird that people just couldn't quite work out is Mercury's orbit. The thing about Mercury, closest planet to the sun, it has this elliptical orbit. But that elliptical orbit is itself spinning around. It's affected by the other planets. So, so the, it doesn't trace out the same ellipse every single time it orbits the sun, that ellipse is moving around. Yeah. It's called the perihillian of Mercury's orbit. Okay. Which sort of makes sense, right? Helian meaning sun. And everyone was cool with that. Everyone was absolutely fine with that. That they knew that, you know, the orbit was going to change because of where different planets were. But when they ran the calculations, according to Newton's version of gravity, that it's essentially just to accelerate objects, accelerating towards each other, something was off, right? It's like the number of arc seconds of Mercury's orbit just didn't totally make sense. And for a long time, you know, the telescopes won that accurate. People were like, maybe we've just made a miscalculation and sort of a bit, I don't know. This is for a long time. Like hundreds of hundreds of years. And then when Einstein came along and he was like, I think there's something else going on here. Einstein has this great intuition that it's not just that objects are magically accelerating towards each other. But that space time itself has this curvature to it. So the sun, for instance, this giant gravitational force is literally bending and warping space time between us and it. And so if you got a magical wand and you made the sun disappear immediately, there would be this ripple that was sent out from the absence of that sun. Imagine taking a bowling ball on a rubber sheet and then removing it. That rubber sheet is going to kind of bounce up and down and ripple as you remove the weight. And that that ripple would reach us at the speed of light. You had this great intuition, worked out all the calculations for it. And that one of the very first things that he turned his equations to was the Prahillian of Mercury's orbit to see if his new theory came up with a more accurate prediction than Newton's. And he absolutely nailed it. Like, level of precision. I mean, he said that he was happy for days after he looked at those calculations, was like, I've absolutely got it. I found the missing piece to the puzzle. So two things. First, that leap from there's a force acting on things. Maybe it's mediated by some particle or whatever. To leap from there to actually maybe gravity is just a change in the shape of space time. Is really gigantic. Because space time is such a bizarrely abstract thing. It's the canvas that we are on. If we were to to mention all this would be easier. We could say, you know, a two dimensional creature could be painted onto this curtain. And if I crumpled the curtain up, they're still stuck on it and they're going over all of these crinkles, but they don't even know it. I can bring them together and push them apart. If it gets crumpled up or curved, you're just going to follow along that curve. You cannot leave it. And so, yeah, Einstein is like, but what if it's the shape of the canvas that we are on? Exactly. Even the shape of time and how quickly time runs for you, if we allow that to change, then Mercury's orbit makes sense. Exactly right. It's that crumbling in the curtain. That's a really nice way to do it. Yeah, I think you need analogies because we're just talking about things that are so outside of our normal day to day activities. Totally. We understand forces. We understand pushes and poles. But to see that space and time themselves push and pull, it's kind of more like, you're just in them. But here's the thing, right? The implications of this idea that space time is like a crumpled curtain. It means that across the surface of the earth, even, the gravitational effects are slightly different. So I did some calculations, bolder in Colorado, right? Which of course is like a very high altitude compared to Greenwich in London, where I am. The gravitational effect in bolder is 9.796 meters per second. What is it in Greenwich? 9.812. Wow. I've got high gravitational effect than you. Yeah. So you are more attracted to the center of earth than I am in order because I'm further away. And the inverse square law says, exactly, further away, gravitational effect is diminishes. And the fact that what that means, given Einstein's version of gravity, is that the way that time changes in bolder is different to the way that time changes in Greenwich, because what gravity is doing is it's bending and warping space time. So what this means is that time travels slower in Greenwich than it does in bolder. And the difference is about 5.6 microseconds a year. So what I will say is that you are aging faster than me.