Clearly I need to learn to be more specific
when I do these episodes.
Everything time I open my mouth, I need to
prepare for the collective imagination of
the viewers.
We did a whole video about the biggest things
in the Universe, and identified superclusters
of galaxies as the best candidate.
Well, the part of superclusters actually gravitationally
bound enough to eventually merge together
in the future.
But you had other ideas, including dark energy,
or the Universe itself as the biggest thing.
Even love?
Aww.
One intriguing suggestion, though, is the
idea of the vast cosmic voids between galaxies.
Hmm, is the absence of something a thing?
Whoa, time to go to art school and talk about
negative space.
Ah well, who cares?
It’s a super interesting topic, so let’s
go ahead and talk about voids.
When most people imagine the expansion of
the Universe after the Big Bang, they probably
envision an equally spaced smattering of galaxies
zipping away from one another.
And that’s pretty accurate at the smallest
scales.
But at the largest scales, like when you can
see billions of light-years in a cube that
fits on your computer screen, then a larger
structure starts to take shape.
It looks less like an explosion, and more
like a tasty tasty sponge cake, with huge
filaments, walls, and the vast gaps in between.
The gaps, the voids, the supervoids, are the
point of today’s video, but to understand
the gaps, we’ve got to understand why the
Universe is clumped up the way it is.
Run the Universe clock backwards, all the
way to the beginning, to a fraction of a second
after the Big Bang.
When the entire cosmos was compressed down
into a tiny region of superheated plasma.
Although it was mostly uniform in density,
there were slight variations - quantum fluctuations
in spacetime itself.
And as the Universe expanded, those differences
were magnified.
What started out as tiny differences in the
density of matter at the smallest scale, turned
into regions of higher and lower density of
matter in the Universe.
Here we are, 13.8 billion years after the
Big Bang, and we can see how the microscopic
variations at the beginning of time were magnified
to the largest scales.
Instead of individual galaxies, we see huge
walls containing thousands of galaxies; filaments
of galaxies connect in nodes.
These structures are huge; hundreds of millions
of light-years across, containing thousands
of galaxies.
But the gaps, the voids, between these clusters
can be even larger.
Astronomers first started thinking about these
voids back in the 1970s, when the first large-scale
surveys of the Universe were made.
By measuring the redshift of galaxies, and
determining how fast they were speeding away
from us, astronomers started to realize that
the distribution of galaxies wasn’t even.
Some galaxies were relatively close, but then
there were huge gaps in distance, and then
another cluster of galaxies collected together.
Over the last few decades, astronomers have
built sophisticated 3-dimensional models that
map out the Universe in the largest scales.
The Sloan Digital Sky Survey, updated in 2009,
has provided the most accurate map so far.
The Large Synoptic Survey Telescope, destined
for first light in a few years will take this
to the next level.
The largest void that we currently know of
is known as the Giant Void (original, I know),
and it’s located about 1.5 billion light-year
away.
It has a diameter of 1 billion to 1.3 billion
light-years across.
To be fair, these regions aren’t really
completely empty.
They just have less density than the regions
with galaxies.
In general, they’ve got about a tenth the
density of matter that’s average for the
Universe.
Which means that there’s still gas and dust
in these regions, as well as dark matter.
There will still be stars and galaxies out
in the middle of those voids.
Even the Giant Void has 17 separate galaxy
clusters inside it.
You might imagine continuing to scale outward.
Maybe you’re wondering if the this spongy
distribution of matter is actually just the
next step to an even larger structure, and
so on, and so on.
But it isn’t.
In fact, astronomers call this “the End
of Greatness”, because it doesn’t seem
like there’s any larger structure to the
Universe.
As the expansion of the Universe continues,
these voids are going to get even larger.
The walls and filaments connecting clusters
of galaxies will stretch and break.
The voids will merge with each other, and
only gravitationally bound galaxy clusters
will remain as islands, adrift in the expanding
emptiness.
The full scale of the observable Universe
is truly mind boggling.
We’re here in this tiny corner of the Local
Group, which is part of the Virgo Supercluster,
which is perched on the precipice of vast
cosmic voids.
So much to explore, so let’s get to work.
We’ve talked about supervoids, but that’s
really scratching the surface of the large
scale structure of the Universe.
What else fascinates you?
Let me know and I’ll turn them into future
episodes.
We’ve talked so much about supernovae, but
never regular novae.
What’s the difference?
Find out in our next episode.
Oh, and make sure you stick around for the
blooper.
A big thanks to Sergio Botero, Mingyen Chang,
Mathew Anderson, and the rest of our 624 patrons
for their generous support.
If you love what we’re doing and want to
help out, head over to patreon.com/universetoday.
