Science Simplified Weekly · Episode 21 · 6 min · English audio · 11 September 2026
Black Holes Explained: The Sun, Sucked Small as an Airport
What happens if you crush the Sun into a black hole? A wild space story for curious minds of any age.
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Podcast · 26 episodes · Latest 23 October 2026 · English audio
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What this episode covers
In this engaging episode, we explore the fascinating world of black holes by comparing them to a sun being squeezed down to the size of an airport. We break down what black holes are, how they form, and why they are some of the most mysterious objects in the universe. Whether you're a curious kid or a seasoned physicist, you'll gain a clearer understanding of these cosmic giants and why they matter in understanding our universe.
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Transcript
926 words · Script-based transcript; wording may differ from the recording.
Okay, get this. If you could somehow crush our Sun down until it became a black hole, it would be less than three kilometers across. Wait, what? Three kilometers? That’s like... the size of a small airport. The whole SUN? The WHOLE sun! And you know, at its very center would be a singularity—a point of infinite density. It's almost the same problem we talked about last week with the Big Bang, just... inverted! Okay, so you’ve got my attention. What even IS a black hole? Beyond, you know, a scary thing in sci-fi movies. Right! It’s actually so much cooler than that. A black hole is a place in space where gravity is so strong that nothing—and I mean NOTHING, not even light—can escape.
It’s the ultimate one-way street. So that’s why they’re black. Because light can’t get out. Exactly! And that boundary, that line you cross where escape becomes impossible? That’s called the event horizon. It’s the point of no return. So it's like a cosmic vacuum cleaner, just sucking everything in? If one came near our solar system, we'd be toast? Ah, I am SO glad you said that. That is the biggest misconception! They are absolutely NOT cosmic vacuum cleaners. Seriously. Gravity outside the event horizon works just like it does for any other object. You could orbit a black hole just like we orbit the Sun. Really?
You could fly by one? Totally! As long as you stay outside that event horizon, you're fine. But the second you cross it... you can never come back. Okay, so how do you even make one of these things? You said crushing the Sun, but I assume that’s not the usual method. No, not quite. The most common way is just... the death of a truly enormous star. We’re talking a star at least twenty times more massive than our Sun. Twenty. Okay. So, its whole life, the star is in this perfect balance between gravity trying to crush it and the nuclear fusion in its core pushing out. But when it runs out of fuel... gravity wins.
And it wins BIG. The core just collapses. It collapses catastrophically. The outer layers get blasted away in a supernova explosion, but if the core left behind is heavy enough—more than about three times our sun’s mass—nothing can stop the collapse. It just keeps crushing itself down, and down, and down... until it forms that singularity. A point of basically infinite density. And the event horizon forms around it. How big is that? You said the Sun's would be tiny. It's all about mass! The rule is roughly three kilometers of radius for every solar mass. So a black hole with the mass of ten suns would have an event horizon about thirty kilometers across.
The size of a city, basically. A city-sized object with the mass of TEN suns. That is... that's a lot to wrap your head around. And that's just a baby one! The supermassive black hole at the center of our own Milky Way galaxy, Sagittarius A, is about four MILLION times the mass of the sun. Okay, never mind. My brain just blue-screened. But here's the part that REALLY gets me. You want to know what happens if you fall in? I'm almost afraid to ask. Is it just... instant darkness? A quick end? Well, the tidal forces would be insane. Gravity would pull on your feet so much more strongly than your head that you'd be stretched out like spaghetti.
Spaghettification. I've heard that. It sounds... unpleasant. Oh, it would be! But here is the absolute wildest part. As you actually cross the event horizon—the point of no return itself—you wouldn't feel a thing. Hold on. What? No bump. No sign. No "Welcome to the Black Hole" banner. To you, falling in, it would just be another point in spacetime. You'd float right across it without even knowing you’d just passed the point where escape became physically impossible. That is... that's terrifying. The idea that the point of no return is completely unnoticeable. Isn't it just the most mind-bending thing? Your fate is sealed, the laws of physics say you can ONLY move toward the singularity, but you have no idea.
So we’ve got these stellar-mass ones, and then the supermassive ones like the one in our galaxy. And we've even seen a picture of one, right? The one from 2019? Yes! The Event Horizon Telescope! They took a picture of the monster at the center of the M87 galaxy—a black hole with the mass of 6.5 BILLION suns. And it looked exactly like the theories predicted: a black shadow surrounded by a glowing ring of superheated gas. It was one of the most beautiful moments in modern science. So we know they're there. We know how they work, mostly. But what about the very center? That singularity. Ahhh, yes. The big question.
You said it’s a point of infinite density, but... that can't be real, can it? Physics isn't supposed to have infinities. You are asking the EXACT question that keeps physicists up at night. The singularity is where our best theory of gravity, Einstein’s general relativity, just breaks. It gives us an impossible answer. Most physicists think it’s a sign that we need a better theory—a theory of quantum gravity—to explain what’s really going on in there. So the biggest, most powerful objects in the universe... end in a question mark we can't answer yet. Exactly. They are the ultimate cosmic mystery. And that’s why I love them.
Sources for this episode
- Black Holes for Kids | Whizbee
- M87* One Year Later: Proof of a Persistent Black Hole Shadow
- M87* One Year Later: Catching the Black Hole's Turbulent Accretion Flow
- Wobbling Shadow of the M87* Black Hole - Event Horizon Telescope
- New EHT Images Reveal Unexpected Polarization Flips at M87*
- What Happens When Something Gets ‘Too Close' to a Black Hole? - NASA Science
- Astronomers Reveal First Image of the Black Hole at the Heart of Our Galaxy | Event Horizon Telescope
- New Event Horizon Telescope Results Trace M87 Jet Back to Its Black Hole - National Radio Astronomy Observatory
- What is a black hole event horizon (and what happens there)? | Space
- Supermassive Black Hole Spin Constraints from Polarimetry in ...
- [1906.11238] First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- Spatially resolved spectral properties of M87* on event ...
Made with AI. AI may assist this episode’s research, and it writes and voices the episode. Neither the transcript nor this page is an editorial fact check. To report an error, email hi@lissin.com with the episode URL and timestamp. See our editorial standards.
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About Science Simplified Weekly
One scientific idea each week, explained in an AI-generated podcast for anyone from curious kids to physicists.
