🔥 Supermassive Black Holes: The Cosmic Engines That Shouldn’t Exist 🔥

🌌 The Biggest Cosmic Mystery Supermassive black holes—some billions of times the mass of the Sun—exist at the centers of galaxies, shaping the universe as we know it. But here’s the problem: some of these giants formed incredibly early, just a few hundred million years after the Big Bang. That shouldn’t be possible based on our current understanding of black hole growth.

🔭 In This Episode, We Explore: 🕳️ The Engine Black Holes – How they act as galactic powerhouses, fueling everything from star formation to galaxy evolution. ❓ The Mystery of Their Origins – How did they grow so fast in the early universe? 💡 The Leading Theories – From primordial black holes to direct collapse models, we break down the possibilities. 🚀 The James Webb Telescope’s Latest Discoveries – Did JWST find evidence that early black holes broke the laws of physics? 🌠 The Future of Black Holes – What will happen to these cosmic monsters in the far future? 🔥 Hawking Radiation & the End of Time – How black holes may eventually evaporate, leaving behind a cold, dark universe.

💡 Why This Episode Matters: Black holes are among the most extreme and mysterious objects in the cosmos. Understanding them could unlock new physics—perhaps even answering questions about the nature of space and time itself.

📌 Links & Resources:

• 🌌 More deep space discoveries on Cosmos in a Pod: https://rss.com/podcasts/cosmos-in-a-pod/

Hashtags: #BlackHoles #SupermassiveBlackHole #JWST #SpaceMysteries #Astrophysics #Cosmos #DarkEnergy #GalacticEngines #HawkingRadiation

Episode Transcript

(00:00):
Imagine you're in a spaceship,

(00:03):
and you're going back in time, back to the early universe,
like a few hundred million years after the Big Bang,
and you come across this huge galaxy,
blazing with light from new stars forming.
But as you get closer to the center,
there's this incredible gravitational pull.

(00:25):
It's like something you've never encountered before.
It's an engine black hole,
a black hole billions of times the mass of our sun.
But here's the thing,
those black holes shouldn't even exist yet.
Welcome to Cosmos and applaud the Space and Astronomy series.
Please like, comment, share, and subscribe.
Absolutely.
So the question is, how did these giant black holes form
so early in the universe?

(00:46):
Yeah, that's a really great question,
and it's a mystery that's been puzzling astronomers
for decades.
The usual way we think black holes form
is from a dying star collapsing in on itself.
But that takes a really long time, billions of years.
And the universe just wasn't old enough back then
for stars to die and create black holes that big.
Okay, so we're saying that the standard model

(01:08):
of how black holes form isn't wrong.
It just doesn't explain these supermassive ones.
Exactly, it works fine for the smaller black holes,
but for these supermassive ones,
especially the ones we see in the early universe,
it just doesn't quite add up.
Yeah, so what are some of the other ideas
about how they formed?
Well, one idea is something called primordial black holes.

(01:30):
Primordial black holes.
Yeah.
Those are the ones that formed right after the Big Bang.
Exactly.
Imagine the conditions back then,
so much energy and density, everything packed together.
Yeah.
Some scientists think that little puppets
and all that chaos could have collapsed
and formed black holes right away, no stars needed.
Wow, so like seeds of black holes
scattered through the early universe.

(01:51):
Right, and that would give them a huge head start
to grow into those supermassive ones.
But we haven't actually found any
of these primordial black holes.
Not yet.
It's a cool idea, but we need more evidence.
OK, so we've got the standard model, which might be too slow,
and the primordial black hole idea,
which we haven't proven.
What else is there?
Well, the most likely explanation right now
is something called direct collapse.

(02:13):
Direct collapse.
Yeah, instead of a single star collapsing,
you have a massive cloud of gas, millions
of times the mass of the sun, collapsing directly
into a black hole.
So they skip the whole star phase altogether.
Exactly, and this could explain how
those supermassive black holes form so fast.
OK, but even with direct collapse,
wouldn't they still need to grow incredibly quickly?

(02:35):
That's the next part of the puzzle.
We have to look at some extreme processes,
like super-Eddington accretion and the role of galaxy mergers.
OK, I'm hooked.
Let's talk about that.
Great, so we know these black holes
would have to grow super fast, even with that direct collapse
start.
Yeah, how does that happen?
Well, it comes down to something called accretion.
I know that black holes suck in stuff, anything
that gets too close.

(02:55):
Right, but it's not as simple as just falling straight in.
All that gas and dust spirals inward around the black hole,
and it forms this swirling disk.
Oh yeah, I've seen pictures of those accretion disks.
And they get incredibly hot because of all the friction,
and that releases a ton of energy.
So it's not just a silent, invisible process.
They're blazing with energy.

(03:16):
Exactly, but there's a limit to how fast a black hole
can grow this way.
As it pulls in more matter, all that energy from the disk
can actually start pushing away incoming gas.
So it's like a back pressure.
Exactly, and that limit on how fast it can grow
is called the Eddington limit.
But you said these early black holes had to grow super fast.

(03:36):
So how do they get around that limit?
Right, well, some black holes might
have gone through periods of super Eddington accretion.
Super Eddington accretion?
Yeah, basically they were breaking the speed limit.
Whoa, is there any proof of that?
Actually, yes.
The James Webb SACE telescope saw a black hole
growing 40 times faster than the Eddington limit.
40 times?
That's insane.

(03:57):
What could make them grow that fast?
One idea is that those powerful jets
we see coming from black holes could be playing a role.
Those beams of energy.
Right, they blast out from the black holes poles,
and they might be diverting some of the energy away
from the accretion disk.
So more material can fall in.
Yeah, it's a complex process, but the JWST
is giving us a closer look.

(04:17):
OK, so super Eddington accretion is part of it,
but where does all that material even
come from in the first place?
It's not like there's an endless buffet out there.
That's a great question, and that leads us to galaxy mergers.
When galaxies crash into each other.
Exactly, and when that happens, the black holes
at their centers get pulled together by gravity.

(04:39):
Oh, wow.
They start orbiting each other, getting closer and closer.
It's a spectacular dance.
So it's not just a one-time meal.
It's like a constant feast fueled by these mergers.
Exactly, and these mergers are amazing.
They can trigger bursts of star formation,
creating these beautiful cosmic fireworks.
It's mind-blowing to think about,
but even black holes can't keep growing forever, right?
You're right.

(05:00):
They do have a lifespan.
They eventually run out of fuel as the universe expands
and everything spreads out.
So what happens then?
What's the final act?
It involves something called Hawking radiation.
OK, I've heard of that, but I don't really get it.
It's based on quantum mechanics.
You see, even the empty space around a black hole
is full of these things called virtual particles.
Virtual particles.
Yeah, it's like pairs of particles constantly popping

(05:22):
in and out of existence.
They borrow energy from the vacuum of space,
and they usually destroy each other almost instantly.
But near a black hole, something weird can happen.
What happens?
Sometimes one particle falls into the black hole,
and the other one escapes.
And that escaping particle takes some of the black hole's energy
with it.
So even though nothing can escape from inside the black hole,

(05:45):
it's still losing energy.
Exactly.
And over a really, really long time,
this energy leak called Hawking radiation
makes the black hole shrink.
And then what happens in the end?
So we were talking about Hawking radiation
and how black holes lose a tiny bit of energy over time.
Right.
But what happens when it's all gone, when there's
no more black hole left?

(06:05):
Well, it's not exactly an explosion,
but it's kind of like one.
OK.
All that energy trapped inside has to go somewhere.
So it releases this huge burst of energy and particles.
So the black hole disappears in a burst of energy.
Yeah, you could say that.
It's more like an evaporation, though.
So no more black hole, just a little echo of radiation.
Right, and that radiation just spreads out into the universe.

(06:27):
It's kind of sad in a way, these giant black holes just
fading away.
I guess so.
But remember, this takes an incredibly long time,
much longer than the current age of the universe.
Yeah, that's true.
And it brings us to this idea of the heat death
of the universe.
Heat death.
That sounds ominous.
It's just a theory, but it fits with what

(06:47):
we know about physics.
OK.
Imagine a universe where everything has run out of fuel.
All the stars are dead.
All the black holes have evaporated.
So just a cold, empty universe.
Pretty much, just a faint sea of particles
spread out over unimaginable distances.
No more stars, no more galaxies, just darkness and silence.
It's the ultimate end state of the universe,

(07:08):
according to thermodynamic.
Oh, wow.
It's kind of amazing to think about.
It is.
It makes you realize how precious our time
in the universe is.
We're lucky to be here when things are still happening.
Exactly.
We get to see stars being born, galaxies colliding,
black holes growing.
It's a pretty special time.
I agree.
Well, this has been a fascinating deep dive

(07:28):
into the world of supermassive black holes.
It has.
And who knows what new discoveries
await us in the future.
That's right.
There's always more to learn.
Absolutely.
Thanks for joining us on Cosmos in a Pod.
It was my pleasure.
And to all our listeners, don't forget
to subscribe to our YouTube channel
for more explorations of the universe.
And keep looking up at the stars.

(07:49):
Until next time.