There’s a supermassive black hole at the
center of almost every galaxy in the Universe.
How did they get there?
What’s the relationship between these monster
black holes and the galaxies that surround
them?
Every time astronomers look farther out in
the Universe, they discover new mysteries.
These mysteries require all new tools and
techniques to understand.
These mysteries lead to more mysteries.
What I’m saying is that it’s mystery turtles
all the way down.
One of the most fascinating is the discovery
of quasars, understanding what they are, and
the unveiling of an even deeper mystery, where
do they come from?
As always, I’m getting ahead of myself,
so first, let’s go back and talk about the
discovery of quasars.
Back in the 1950s, astronomers scanned the
skies using radio telescopes, and found a
class of bizarre objects in the distant Universe.
They were very bright, and incredibly far
away; hundreds of millions or even billion
of light-years away.
The first ones were discovered in the radio
spectrum, but over time, astronomers found
even more blazing in the visible spectrum.
The astronomer Hong-Yee Chiu coined the term
“quasar”, which stood for quasi-stellar
object.
They were like stars, shining from a single
point source, but they clearly weren’t stars,
blazing with more radiation than an entire
galaxy.
Over the decades, astronomers puzzled out
the nature of quasars, learning that they
were actually black holes, actively feeding
and blasting out radiation, visible billions
of light-years away.
But they weren’t the stellar mass black
holes, which were known to be from the death
of giant stars.
These were supermassive black holes, with
millions or even billions of times the mass
of the Sun.
As far back as the 1970s, astronomers considered
the possibility that there might be these
supermassive black holes at the heart of many
other galaxies, even the Milky Way.
In 1974, astronomers discovered a radio source
at the center of the Milky Way emitting radiation.
It was titled Sagittarius A*, with an asterisk
that stands for “exciting”, well, in the
“excited atoms” perspective.
This would match the emissions of a supermassive
black hole that wasn’t actively feeding
on material.
Our own galaxy could have been a quasar in
the past, or in the future, but right now,
the black hole was mostly silent, apart from
this subtle radiation.
Astronomers needed to be certain, so they
performed a detailed survey of the very center
of the Milky Way in the infrared spectrum,
which allowed them to see through the gas
and dust that obscures the core in visible
light.
They discovered a group of stars orbiting
Sagittarius A-star, like comets orbiting the
Sun.
Only a black hole with millions of times the
mass of the Sun could provide the kind of
gravitational anchor to whip these stars around
in such bizarre orbits.
Further surveys found a supermassive black
hole at the heart of the Andromeda Galaxy,
in fact, it appears as if these monsters are
at the center of almost every galaxy in the
Universe.
But how did they form?
Where did they come from?
Did the galaxy form first, and cause the black
hole to form at the middle, or did the black
hole form, and build up a galaxy around them?
Until recently, this was actually still one
of the big unsolved mysteries in astronomy.
That said, astronomers have done plenty of
research, using more and more sensitive observatories,
worked out their theories, and now they’re
gathering evidence to help get to the bottom
of this mystery.
Astronomers have developed two models for
how the large scale structure of the Universe
came together: top down and bottom up.
In the top down model, an entire galactic
supercluster formed all at once out of a huge
cloud of primordial hydrogen left over from
the Big Bang.
A supercluster’s worth of stars.
As the cloud came together it, it spun up,
kicking out smaller spirals and dwarf galaxies.
These could have combined later on to form
the more complex structure we see today.
The supermassive black holes would have formed
as the dense cores of these galaxies as they
came together.
If you want to wrap your mind around this,
think of the stellar nursery that formed our
Sun and a bunch of other stars.
Imagine a single cloud of gas and dust forming
multiple stars systems within it.
Over time, the stars matured and drifted away
from each other.
That’s top down.
One big event that leads to the structure
we see today.
In the bottom up model, pockets of gas and
dust collected together into larger and larger
masses, eventually forming dwarf galaxies,
and even the clusters and superclusters we
see today.
The supermassive black holes at the heart
of galaxies were grown from collisions and
mergers between black holes over eons.
In fact, this is actually how astronomers
think the planets in the Solar System formed.
By pieces of dust attracting one another into
larger and larger grains until the planet-sized
objects formed over millions of years.
Bottom up, small parts coming together.
So which is it?
Astronomers think they know the answer now,
and we’ll get to it in a second, but first
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Shortly after the Big Bang, the entire Universe
was incredibly dense.
But it wasn’t the same density everywhere.
Tiny quantum fluctuations in density at the
beginning evolved over billions of years of
expansion into the galactic superclusters
we see today.
I want to stop and let this sink into your
brain for a second.
There were microscopic variations in density
in the early Universe.
And these variations became the structures
hundreds of millions of light-years across
we see today.
Imagine the two forces at play as the expansion
of the Universe happened.
On the one hand, you’ve got the mutual gravity
of the particles pulling one another together.
And on the other hand, you’ve got the expansion
of the Universe separating the particles from
one another.
The size of the galaxies, clusters and superclusters
were decided by the balance point of those
opposing forces.
If small pieces came together, then you’d
get that bottom up formation.
If large pieces came together, you’d get
that top down formation.
When astronomers look out into the Universe
at the largest scales, they observe clusters
and superclusters as far as they can see - which
supports the top down model.
On the other hand, observations show that
the first stars formed just a few hundred
million years after the Big Bang, which supports
bottom up.
So the answer is both?
No, the most modern observations give the
edge to the bottom up processes.
The key is that gravity moves at the speed
of light, which means that the gravitational
interactions between particles spreading away
from each other needed to catch up, going
the speed of light.
In other words, you wouldn’t get a supercluster’s
worth of material coming together, only a
star’s worth of material.
But these first stars were made of pure hydrogen
and helium, and could grow much more massive
than the stars we have today.
They would live fast and die in supernova
explosions, creating much more massive black
holes than we get today.
The first protogalaxies came together, collecting
together these first monster black holes and
the massive stars surrounding them.
And then, over millions and billions of years,
these black holes merged again and again,
accumulating millions and even billions of
times the mass of the Sun.
This was how we got the modern galaxies we
see today.
There was a recent observation that supports
this conclusion.
Earlier this year, astronomers announced the
discovery of supermassive black holes at the
center of relatively tiny galaxies.
In our own Milky Way, the supermassive black
hole is 4.1 million times the mass of the
Sun, but accounts for only .01% of the galaxy’s
total mass.
But astronomers from the University of Utah
found two ultra compact galaxies with black
holes of 4.4 million and 5.8 million times
the mass of the Sun respectively.
And yet, the black holes account for 13 and
18 percent of the mass of their host galaxies.
The thinking is that these galaxies were once
normal, but collided with other galaxies earlier
on in the history of the Universe, were stripped
of their stars and then were spat out to roam
the cosmos.
They’re the victims of those early merging
events, evidence of the carnage that happened
in the early Universe when the mergers were
happening.
We always talk about the unsolved mysteries
in the Universe, but this is one that astronomers
are starting to puzzle out.
It seems most likely that the structure of
the Universe we see today formed bottom up.
The first stars came together into protogalaxies,
dying as supernova to form the first black
holes.
The structure of the Universe we see today
is the end result of billions of years of
formation and destruction.
With the supermassive black holes coming together
over time.
Once telescopes like James Webb get to work,
we should be able to see these pieces coming
together, at the very edge of the observable
Universe.
This was a fun episode, and I know you’re
fascinated by black holes.
Were there any other topics that you’d like
me to dig into?
Let me know your thoughts in the comments.
In our next episode we look at the Deep Space
Gateway, NASA’s plans to put a space station
out at the Moon, which will serve as a stepping
stone to the rest of the Solar System.
It’s time for a playlist, all about supermassive
black holes.
First, I’d like to direct you to an interview
I did with Dr. Andrea Ghez, who found the
supermassive black hole at the heart of the
Milky Way.
Followed by a TED talk she gave.
A response from Michio Kaku about this puzzling
mystery.
SciShow Space video about the black hole.
Finally, a public lecture about supermassive
black holes.
