Latest / Boring Science / The TERRIFYING Scale of the Virgo Supercluster
Transcript
- 0:00Speaker 1: There is a structure in space so large that if
- 0:03you shrank the entire Milky Way Galaxy down to the
- 0:06size of a single grain of sand, the Virgo Supercluster
- 0:10would still be several kilometers across. Sit with that for
- 0:14a moment, not as a fact to file away as
- 0:17a collision. The Milky Way contains somewhere between one hundred
- 0:21and four hundred billion stars. It stretches roughly one hundred
- 0:26thousand light years from edge to edge. By any measure
- 0:30available to human experience, it is incomprehensibly large, and it
- 0:35is a grain of sand. The structure surrounding it spans kilometers.
- 0:40If you find comfort in these gentle explorations of space
- 0:43and science, I'd be grateful if you'd consider subscribing and
- 0:47giving this video alike. I'd love to know where you're
- 0:50watching from and what time it is for you. Feel
- 0:53free to drop your location and time in the comets below.
- 1:03The number astronomers use is one hundred ten million light years.
- 1:08That is the diameter of the Virgo Supercluster, the vast
- 1:12cosmic structure that contains our galaxy, our neighborhood, everything we
- 1:17have ever called home. One hundred and ten million light years.
- 1:22A single light year is already about nine point five
- 1:25trillion kilometers. Multiply that by one hundred and ten million,
- 1:30and the number stops functioning as a number. It becomes noise.
- 1:35The human brain was built to navigate forests, calculate distances
- 1:40between villages, maybe stretch as far as continents in an atlas.
- 1:44It was not built for this. There is no failure
- 1:47of imagination happening when that number refuses to land. The
- 1:52number is simply outside the range that evolution prepared us for.
- 1:56Here is something worth holding alongside it. You live inside
- 2:01this structure right now. Every person alive, every person who
- 2:06has ever lived, every war and discovery and quiet Tuesday
- 2:10morning in recorded human history, all of it happened inside
- 2:14the Virgo Supercluster. It is not something out there. It
- 2:18is the thing we are embedded in, and almost nobody
- 2:21knows what it actually is. Ask someone on the street
- 2:25to name the galaxy they live in, and a reasonable
- 2:27number will say the Milky Way. Ask them what the
- 2:30Milky Way belongs to, and most will pause. Ask them
- 2:34what that belongs to, and the conversation tends to end.
- 2:38The Virgo Supercluster is the next frame out. It is
- 2:42the city our galaxy lives in, and it is essentially
- 2:45invisible to everyday awareness. It has a shape, It has
- 2:50a center of gravity. It has filaments and voids, and
- 2:53a beating heart fifty five million light years away that
- 2:57is quietly pulling everything toward it, including us right now,
- 3:02at roughly three hundred kilometers per second. That last part
- 3:06is not a metaphor. The Milky Way is in motion
- 3:10toward the core of the Virgo supercluster. The pull is real,
- 3:14the direction is specific. We are falling slowly and silently
- 3:19towards something enormous, and we cannot feel any of it.
- 3:24This is the problem the next several sections are going
- 3:27to take seriously. Not the problem of defining the Virgo supercluster,
- 3:32because definitions are easy. The problem is making it feel
- 3:35like something. Numbers this large have a way of producing
- 3:39a kind of cognitive static. You read one hundred and
- 3:42ten million light years, you nod, and nothing changes about
- 3:47how you understand your place in the universe. The goal
- 3:50here is different. The goal is to break that number open,
- 3:54walk through what lives inside it, and come out the
- 3:57other side with something closer to genuine comprehension than polite acknowledgment.
- 4:03We are going to start where we are the local group,
- 4:06our immediate cosmic neighborhood, then the larger structure it sits within,
- 4:12then the gravitational engine at the center of that structure,
- 4:15then the dark matter skeleton that holds it all together,
- 4:19invisible and enormous, without which none of the rest of
- 4:23it would exist in its current form. Then the discovery
- 4:26that even the Virgo supercluster turns out to be a
- 4:29small piece of something far larger, and then finally back
- 4:34to that number one hundred and ten million light years
- 4:38to see whether any of it made it feel more real.
- 4:41It probably will not feel completely real. That is an
- 4:45honest prediction. There are things in this universe that human
- 4:48intuition cannot fully contain, and the Virgo supercluster is almost
- 4:53certainly one of them. But there is a difference between
- 4:56a number that means nothing and a number that means
- 4:59something you can cannot quite hold. One is ignorance, the
- 5:03other is something closer to all and we are going
- 5:06to try to understand all of it. To understand what
- 5:09the Virgo supercluster is, you first have to understand how
- 5:13the universe organizes itself. Because it does organize itself in layers,
- 5:19each one almost incomprehensibly larger than the one below it.
- 5:23Start with stars. A star is a furnace of nuclear fire,
- 5:28a ball of plasma held together by its own gravity.
- 5:32Our Sun is one. There are roughly two trillion trillion
- 5:36of them in the observable universe. Stars, for the most part,
- 5:40don't drift alone through empty space. Gravity pulls them together.
- 5:45Hundreds of billions of stars orbiting a common center bound
- 5:49into a single rotating structure. That structure is a galaxy.
- 5:53The Milky Way is one Andromeda is another. There are
- 5:57roughly two trillion galaxies in the observable universe, which means
- 6:02galaxies are, in a certain sense, the basic unit of
- 6:06large scale cosmic structure. They are the buildings. But galaxies
- 6:10don't drift alone either. They gather. Gravity reaches across millions
- 6:15of light years and pulls galaxies toward each other, drawing
- 6:19them into loose associations called groups, or, when the numbers
- 6:23get larger and the gravitational binding tighter, clusters. A galaxy
- 6:29group might contain a few dozen members, a rich galaxy
- 6:32cluster can hold thousands. These are the city blocks. Dozens
- 6:37or hundreds of galaxies in a region of space, orbiting
- 6:41each other, interacting, sometimes colliding and merging over billions of years.
- 6:47Then comes the next level up. Groups and clusters are
- 6:50not randomly scattered across the universe. They are themselves gathered
- 6:54into larger structures. Loose associations of clusters and groups spread
- 6:59across tens or hundreds of millions of light years. These
- 7:03are superclusters the city itself. If a galaxy is one
- 7:08building and a cluster is a block of buildings, a
- 7:12supercluster is an entire metropolitan area, with neighbourhoods and arterials
- 7:18and dense downtown cores and thin suburban sprawl at the edges.
- 7:23That is what the Virgo Supercluster is. It is the
- 7:26city we live in. The numbers stated plainly are these.
- 7:32The Virgo Supercluster spans roughly one hundred ten million light
- 7:36years across its widest dimension, That is thirty three megaparsex
- 7:41if you prefer the unit astronomers use when light years
- 7:44start feeling small. It contains somewhere around forty seven thousand galaxies,
- 7:50not forty seven thousand stars. Forty seven thousand galaxies each
- 7:56one a structure of hundreds of billions of stars. A
- 8:00mass filling this volume is equivalent to roughly ten quintillian suns,
- 8:05and it is not a sphere. That is one of
- 8:07the first things that surprises people who encounter the actual shape.
- 8:12The Virgo supercluster is flattened. It is disc like roughly,
- 8:17though calling it a disc makes it sound neater than
- 8:20it is. Think of it more like a squashed irregular form,
- 8:23with a dense central region and thinner extensions reaching outward.
- 8:28About two thirds of its bright galaxies are concentrated near
- 8:32a central plane, a kind of equator pulled into alignment
- 8:37by the dominant gravitational forces at the heart of the structure.
- 8:41The remaining third are spread in a looser halo above
- 8:45and below that plane, like the sparse outer burroughs of
- 8:48a city. The overall impression, if you could somehow see
- 8:52it from far enough away, would be something like a
- 8:55flat and jelly bean, lumpy and asymmetric, with clear density
- 9:00variations running through it. The person who first proposed this
- 9:04structure existed was a French astronomer named Gerard de Vaucouleur.
- 9:10In the early nineteen fifties, he was studying the red
- 9:13shifts of galaxies, measuring how fast they appeared to be
- 9:17moving away from us. By looking at how much their
- 9:20light had shifted toward longer wavelengths, he noticed something. Galaxies
- 9:25in a particular broad region of sky seemed to share
- 9:28similar velocities, clustered too consistently to be coincidence. They seemed,
- 9:34in his word, dynamically related. They were moving together, responding
- 9:39to each other, behaving like members of a single structure.
- 9:43In nineteen fifty three, he named it the Local super galaxy.
- 9:48By nineteen fifty eight he had revised the name to
- 9:51the Local Supercluster. The astronomical community was not convinced. For decades,
- 9:57the idea sat in an uncomfortable middle ground between accepted
- 10:01fact and contested hypothesis. Some astronomers thought de Vauclur was
- 10:06seeing a real physical structure. Others thought he was finding
- 10:10patterns in noise, the kind of apparent clustering that emerges
- 10:14from any large, randomly distributed data set if you look
- 10:18at it with the right bias. The debate turned on
- 10:21a basic question with high stakes. Was the universe actually
- 10:26organized on these enormous scales, or were superclusters and illusion
- 10:31The answer came from the red shift surveys. Starting in
- 10:35the late nineteen seventies and accelerating through the early nineteen eighties,
- 10:39astronomers began mapping the positions and velocities of thousands of
- 10:43galaxies in three dimensions. For the first time, the Center
- 10:48for Astrophysics surveys led by teams at Harvard plotted galaxy
- 10:53after galaxy in the volume of space surrounding the Milky Way.
- 10:58The maps that emerged were unambiguit uk us Galaxies were
- 11:01not randomly distributed. They formed sheets, filaments, dense concentrations separated
- 11:09by enormous empty voids. The flattened concentration de Vaucouleur had
- 11:15described from his red shift measurements was real. It was
- 11:18therein the data, undeniable, a genuine physical structure stretching across
- 11:24one hundred million light years of space. For thirty years,
- 11:29people argued about whether this structure was real or whether
- 11:32astronomers were seeing patterns that weren't there, and the red
- 11:36shift surveys of the early nineteen eighties finally shut down
- 11:40the debate. Our immediate cosmic neighbourhood has a name, the
- 11:44local group. It is not a dramatic name. It sounds
- 11:48like something you would call a committee at a community center.
- 11:51But the local group spans roughly ten million light years,
- 11:55and that distance is already large enough to break the
- 11:57part of your brain that tries to picture things. Ten
- 12:01million light years light traveling at three hundred thousand kilometers
- 12:05every second needs ten million years to cross it. Not
- 12:09ten million kilometers, not ten million miles, ten million years
- 12:14of travel at the fastest speed anything in the universe
- 12:17is allowed to move. The local group is not a
- 12:20small place. It is simply small compared to what contains
- 12:24it within that volume. There are roughly eighty known galaxies.
- 12:28Most of them are dwarfs, small, faint, gravitationally dominated by
- 12:33the two giants that anchor the whole structure. Those two
- 12:36giants are the Milky Way and Andromeda. The Milky Way
- 12:40is our galaxy, a barred spiral containing somewhere between two
- 12:44hundred and four hundred billion stars roughly one hundred thousand
- 12:48light years across. Andromeda, also known as Messier thirty one,
- 12:52is larger still, perhaps a trillion stars, a disc that
- 12:56stretches wider than our own. These two galaxies hold the
- 13:00local group together. Everything else orbits one of them, drifts
- 13:04between them, or hangs loosely in the gravitational space. They
- 13:08share the dwarf galaxies, the Magellanic clouds visible from the
- 13:12southern hemisphere. The dozens of small irregular systems cataloged over
- 13:17the past century are satellites. They are buildings in the
- 13:21shadow of two much taller ones. Here is something worth
- 13:24sitting with. The Virgo supercluster is roughly seven thousand times
- 13:29larger than the local group, seven thousand times. If the
- 13:34local group were the size of a city block, the
- 13:36supercluster would be the size of a continent. If you
- 13:39handed someone a map of the local group and ask
- 13:42them to mark where the supercluster ended, they would need
- 13:46a map roughly seven thousand times bigger just to see
- 13:49the edge. The local group, for all its staggering size,
- 13:54is a single address on a street with thousands of
- 13:56other addresses, and our position within that address is not central,
- 14:01not even close. The Milky Way sits toward the outer
- 14:05edge of the local group. Andromeda is the slightly more
- 14:09dominant partner. It holds somewhat more mass, slightly more gravitational authority.
- 14:16The two galaxies are separated by about two point five
- 14:19million light years and between them and around them, the
- 14:24smaller members of the group orbit and drift. But we
- 14:27are not at the center of even this modest neighborhood.
- 14:31We are on the outskirts of a group that is
- 14:33itself on the outskirts of the supercluster. Picture it as
- 14:37layers of periphery, each one containing the next. The Milky
- 14:42Way is near the edge of the local group. The
- 14:45local group is near the edge of the Virgo Supercluster.
- 14:49Every frame you zoom out from we are closer to
- 14:52the boundary than to the mid delay. The center of
- 14:56the Virgo supercluster, roughly fifty to fifty five million in
- 15:00light years from US, is occupied by something enormous and
- 15:03gravitationally dominant. That structure is the Virgo Cluster, thousands of
- 15:08galaxies packed into a region that is still vast but
- 15:12far denser than the surrounding volume. The local group from
- 15:16the perspective of the Virgo cluster is a small collection
- 15:19of galaxies far out toward the edge of the supercluster,
- 15:23nothing particularly remarkable, one of more than one hundred groups
- 15:27scattered across this volume of space. But here is what
- 15:30makes our position more than just a footnote on a map.
- 15:34We are not sitting still. The local group is falling
- 15:37toward the Virgo cluster, slowly by everyday standards, quickly by
- 15:43any standard that involves tens of millions of light years.
- 15:47Measurements of galaxy velocities in our region show a clear
- 15:50in fall pattern, a systematic drift toward the supercluster's gravitational
- 15:56center at around three hundred kilometers per second. That motion
- 16:00is real. It is happening now. The center of the
- 16:04supercluster is pulling on us, and the local group is
- 16:07responding the way any mass responds to gravity over sufficient time.
- 16:12It moves three hundred kilometers per second. Sounds fast. It
- 16:17is fast. It is faster than any spacecraft humanity has
- 16:22ever launched. But the distance is so incomprehensibly large that
- 16:27even at that speed, the journey would take tens of
- 16:30billions of years. We are not falling toward the Virgo
- 16:34Cluster on any timescale that matters to anything alive. The
- 16:38infall is geological in its patients, cosmological in its indifference.
- 16:43It is not something you can watch unfold, not something
- 16:47any instrument can register. In a human lifetime. It is
- 16:51only visible when you stack decades of measurements, compare velocities
- 16:55across thousands of galaxies, and subtract out the background expansion
- 17:00of the universe to find the faint residual motion underneath.
- 17:05What remains when you do that subtraction is a current,
- 17:09a slow, enormous flow of matter toward the dense heart
- 17:13of the supercluster. The local group is caught in that current.
- 17:17The Milky Way is caught in it, and there is
- 17:20no mechanism that stops it, no counterforce strong enough to
- 17:24reverse it. On these scales, gravity is patient, and the
- 17:28Virgo Cluster has been accumulating mass and pulling on everything
- 17:32nearby since long before the Earth formed. This is our
- 17:35position in the universe, not at the center of a galaxy,
- 17:39not at the center of a group, not at the
- 17:42center of a supercluster, near the edge of all of them,
- 17:45drifting slowly inward, embedded in a structure so large that
- 17:50we spent most of human history not knowing it was
- 17:53there at all. Right now, as you read this, the
- 17:56Milky Way is moving toward the center of the Virgo
- 17:59Souper cluster at around three hundred kilometers per second, and
- 18:03we have no way to feel it. Here is the
- 18:06problem with a number like one hundred ten million light years.
- 18:11It is technically precise and completely meaningless at the same time.
- 18:15The brain hears it, the brain even repeats it, but
- 18:20nothing happens. There is no image, no weight, no feeling
- 18:24of distance. The number sits there like a locked door.
- 18:29So the only honest thing to do is try to
- 18:31break it open, comparison by comparison until something inside it
- 18:36starts to give. Start with a single light year light
- 18:40moves at roughly three hundred thousand kilometers per second. In
- 18:45one second, it crosses a distance so large that it
- 18:48would circle the entire Earth more than seven times. Keep
- 18:52that speed running for one full year without stopping, without
- 18:56slowing across the absolute silence of empty space. That distance
- 19:01is one light year. It works out to about nine
- 19:05point five trillion kilometers. That is already a number the
- 19:09human brain cannot hold. It is too large. It passes
- 19:13through comprehension without leaving a mark. Now multiply it by
- 19:17one hundred and ten million. That is the diameter of
- 19:21the Virgo supercluster, not the distance to the edge, the
- 19:25full width side to side through the middle. One hundred
- 19:30and ten million light years one hundred and ten million
- 19:34times nine point five trillion kilometers. The multiplication itself becomes
- 19:39meaningless almost immediately. You can do it on paper. The
- 19:43answer means nothing, So try a different door. The milky
- 19:47Way is not a small thing. It spans roughly one
- 19:50hundred thousand light years. That is already a number that
- 19:54defeats ordinary intuition. A galaxy so wide that light takes
- 19:58one hundred thousand year to cross it a structure containing
- 20:02somewhere between one hundred and four hundred billion stars. If
- 20:06you placed one thousand milky ways end to end, you
- 20:10would build something approximately one hundred million light years long.
- 20:14That is close to the diameter of the Virgo supercluster.
- 20:18One thousand galaxies, each one containing hundreds of billions of stars,
- 20:23each one vast enough to take one hundred thousand years
- 20:27to cross at the speed of light. Laid out in
- 20:30a line, and you still have not quite covered the
- 20:33full width. You need a few more. That door opens
- 20:37a little, but not all the way. Try a smaller scale.
- 20:41Shrink the milky Way down to the size of a
- 20:43single grain of sand, something you could lose between your fingers.
- 20:48At that scale, the Virgo supercluster would still stretch several
- 20:53kilometers across, not a room, not a building, several kilometers.
- 20:59You stand there holding your grain of sand, galaxy would
- 21:03need to walk for a significant stretch of time before
- 21:06reaching the other side of the structure. Your grain of
- 21:09sand belongs to that one lands differently. Something about the
- 21:13physical walk, something about having to move your body. There
- 21:18is a peculiar power in the act of imagining yourself
- 21:21moving through space, in replacing abstract mathematics with the concrete
- 21:26experience of distance traveled. Your feet know what a kilometer is.
- 21:31Your legs understand fatigue. Your mind can grasp the measure
- 21:35of time it takes to cover ground. When you can
- 21:38press the Virgo supercluster down to a size that requires
- 21:42your physical body to traverse it, When you give the
- 21:45number legs and breath and the weight of your own movement,
- 21:48something shifts. The scale suddenly has texture. It is no
- 21:53longer pure number. It becomes experience. Now try mass. The
- 21:59verse Ergo supercluster contains mass equivalent to roughly ten quintillion suns.
- 22:05A quintillion is a number most people have never had
- 22:08reason to say out loud. It is a billion billion
- 22:12a one, followed by eighteen zeros ten of those. If
- 22:17you try to count to ten quintillion at a rate
- 22:20of one number per second, without pausing, without sleeping, without
- 22:24stopping for any reason at all, the counting would take
- 22:28longer than the current age of the universe several times over.
- 22:32That is the mass packed into this one structure, ten
- 22:36quintillion solar masses, distributed across tens of thousands of galaxies,
- 22:42connected by filaments of gas and dark matter, all of
- 22:46it sitting inside a region of space one hundred ten
- 22:49million light years wide. And that is the whole supercluster.
- 22:54The central knot alone, the Virgo cluster at the heart
- 22:57of everything, contains roughly six txe hundred trillion solar masses
- 23:02packed into a volume that is still incomprehensibly large, but
- 23:06measurably smaller than the full supercluster six hundred trillion. That
- 23:10is six hundred followed by twelve zeros. A single region
- 23:14of the supercluster, the part we are slowly drifting toward,
- 23:18contains that much mass. It is the kind of number
- 23:22that should register is astonishing, and instead just sits there,
- 23:26too large to feel. Here is one that might work
- 23:29better think about time. Light takes about eight minutes to
- 23:33travel from the Sun to the Earth. It takes about
- 23:36four years to reach the nearest other star. It takes
- 23:39roughly one hundred thousand years to cross the Milky Way.
- 23:42To cross the Virgo Supercluster from one side to the other,
- 23:46light needs one hundred and ten million years. The universe
- 23:50itself is about thirteen point eight billion years old. That
- 23:55means a beam of light crossing this structure would consume
- 23:58nearly one full percent of the entire age of the
- 24:01universe just in the crossing. One percent sounds small, but
- 24:06the universe has existed for thirteen point eight billion years.
- 24:10One percent of that is one hundred and thirty eight
- 24:13million years. Light moving at the maximum possible speed in
- 24:17the universe, the speed nothing with mass can ever reach,
- 24:21would spend something close to that entire span just traveling
- 24:25through the structure we call home. When the light that
- 24:28is currently entering your eye from one edge of the
- 24:30Virgo Supercluster first began its journey, the dinosaurs had not
- 24:35yet appeared on Earth. The Permian Extinction, the largest mass
- 24:39die off in Earth's history, had not yet happened. The
- 24:42continents were still arranged differently. Complex life was crawling through
- 24:47shallow seas in configurations we would barely recognize that light
- 24:52was already in transit. It has been crossing space without
- 24:56stopping since before the world we know existed, and it
- 24:59is only now arriving that is one edge to somewhere nearby.
- 25:04The full crossing takes longer. Light that started crossing the
- 25:08Virgo Supercluster when the first complex animals were just beginning
- 25:12to appear on Earth has not finished crossing it yet.
- 25:15The Virgo Cluster is the reason the supercluster has its name.
- 25:20Everything in the previous section, the one hundred and ten
- 25:23million light years, the forty seven thousand galaxies, the flat
- 25:27and disc shape, all of it is organized around this
- 25:30one structure. The Virgo Cluster is the gravitational anchor. It
- 25:35is the reason the supercluster has a center at all.
- 25:39Without it, you would not have a supercluster. You would
- 25:42just have a diffuse scattering of galaxy groups with no
- 25:46particular relationship to each other. It sits roughly fifty five
- 25:50million light years away from us. That is already a
- 25:53number that should stop you. The previous section established that
- 25:57light crossing the full supercluster takes one hundred and ten
- 26:01million years. The Virgo Cluster is about half way across
- 26:06every photon of light you can detect from it. Tonight
- 26:09left the cluster when Earth was in the middle of
- 26:11the eocn epoch. Mammals had survived the extinction that killed
- 26:16the dinosaurs, but just barely Modern humans were still roughly
- 26:21fifty four million years away from existing. That light has
- 26:24been traveling since then, crossing empty space at three hundred
- 26:29thousand kilometers per second, and it is only now reaching
- 26:32your eyes. The cluster itself contained somewhere between one thousand,
- 26:37three hundred and two thousand galaxies. The range matters astronomers
- 26:42are not being vague. The uncertainty comes from the difficulty
- 26:45of defining the cluster's edges, which are not clean. Galaxies
- 26:50are still falling in from the surrounding region. Groups are
- 26:53mid infall. The boundary between cluster and supercluster is not
- 26:57a line, It is a gradient, and counting galaxies inside
- 27:02a gradient is harder than it sounds. What is not
- 27:05uncertain is the mass. The Virgo Cluster holds approximately one
- 27:10point two quadrillion solar masses. A quadrillion is a thousand
- 27:14trillion written out, it is a one followed by fifteen zeros.
- 27:19Our milky way contains roughly one point five trillion solar masses.
- 27:24That means the Virgo cluster is about eight hundred times
- 27:28more massive than our entire galaxy. Pack eight hundred milky
- 27:32Ways into one structure and you begin to approach the
- 27:35scale of what sits at the center of our supercluster,
- 27:39and roughly ninety percent of that mass is invisible. It
- 27:42is dark matter, detectable only through its gravitational effects on
- 27:47the light and motion of everything around it. The structure
- 27:50of the cluster is not what you might picture when
- 27:53you hear the word cluster. It is not a neat
- 27:56sphere of evenly distributed Galaxiesomers describe it as irregular, complex, multiicomponent.
- 28:04There are distinct subclusters within it, concentrations of galaxies that
- 28:09are themselves in the process of merging into the larger structure.
- 28:13Galaxies are falling toward it from multiple directions along filaments
- 28:17that feed into it like rivers into a sea. In
- 28:21X ray images, the cluster glows with hot intergalactic gas
- 28:25that has been shocked and heated by the collision of
- 28:27infalling material. It is not a settled object. It is
- 28:32an ongoing event. The growth process involves complex gravitational interactions
- 28:38spanning hundreds of millions of years. As material falls inward,
- 28:43the cluster structure continuously reorganizes and reshapes itself. Smaller galaxy
- 28:49groups collide and merge, releasing enormous amounts of gravitational energy
- 28:54into space. This ongoing transformation means the cluster of today
- 28:59is measure beserably different from what it was ten million
- 29:02years ago. The cluster will continue to evolve, slowly, consuming
- 29:07more galaxies as long as there are galaxies within reach
- 29:11of its gravitational influence. At its heart sits Messia eighty seven.
- 29:17The next section will spend considerable time there, but it
- 29:20is worth establishing the basic fact here. M eighty seven
- 29:25is a giant elliptical galaxy estimated to contain around twelve
- 29:29trillion stars. Our Milky Way has somewhere between two hundred
- 29:34and four hundred billion. The difference is a factor of
- 29:37roughly thirty. M eighty seven grew that large by consuming
- 29:42other galaxies across billions of years, pulling them in with
- 29:45its gravity, stripping them apart, absorbing their stars into its
- 29:50own structure. It is the dominant gravitational object at the
- 29:54center of the dominant cluster. At the center of our supercluster.
- 29:59Everything curves toward it. Now Here is the part worth
- 30:03sitting with. The Virgo cluster is not static. It is
- 30:07actively accreting. More than a thousand galaxies have already fallen
- 30:12into it over the course of its history. They are
- 30:16inside it, now absorbed into the greater structure, and the
- 30:20accretion is continuing. Any galaxy currently within roughly forty million
- 30:26light years of the cluster's center is gravitationally bound to it.
- 30:31Those galaxies are already committed. Whatever they are doing right now,
- 30:35however fast they appear to be moving away in the
- 30:38hubb or flow, the Virgo Cluster's gravity has already won.
- 30:43They will fall in. It is a matter of time.
- 30:46Forty million light years that is the capture radius, the
- 30:51boundary inside which escape is no longer possible. The Milky
- 30:55Way is approximately fifty five million light years from the
- 30:59center of the Virgo cluster. The capture boundary is at
- 31:02forty million We are fifteen million light years outside the line.
- 31:07In supercluster terms. That is not a wide margin. The
- 31:11full supercluster spans one hundred and ten million light years.
- 31:15We are separated from the inescapable zone by a distance
- 31:18that is less than fifteen percent of the supercluster's total diameter.
- 31:23This is what astronomers mean when they say we sit
- 31:25on the periphery of the supercluster looking inward. We are
- 31:29outside the capture zone, but the gap between us and
- 31:32that zone is not comfortable in any cosmic sense. There
- 31:36is also the motion to consider. The local group is
- 31:39currently falling toward the Virgo cluster at approximately three hundred
- 31:43kilometers per second. We are getting closer, slowly by cosmic standards,
- 31:50but measurably. The cluster's gravity is working on us. Right
- 31:54now at this moment as you read this, we are
- 31:57not in free for toward it. Dark energy in the
- 32:01expansion of the universe complicate the trajectory, but the pull
- 32:05is real, and it has been real for billions of years.
- 32:09What the Virgo Cluster represents, more than anything else, is
- 32:13a demonstration of what gravity does. When you give it
- 32:16enough time and enough mass, it assembles things. Small things
- 32:21become large things, Large things become enormous things. A region
- 32:25of slightly higher density in the early Universe, a wrinkle
- 32:29smaller than anything you could see with the naked eye
- 32:32against the cosmic background, evolved over thirteen billion years into
- 32:36a structure holding one point two quadrillion solar masses and
- 32:40consuming its neighbors. The cluster is still growing. The process
- 32:45is not finished. The Milky Way sits just outside the
- 32:49boundary where the Virgo Cluster's gravity becomes inescapable, and how
- 32:53comfortable you find that fact probably depends on how you
- 32:56feel about the word just. Sitting at the center of
- 33:00the Virgo Cluster is one of the most extreme objects
- 33:03in our corner of the universe. It is a galaxy
- 33:06called Messia eighty seven, and almost every number attached to
- 33:10it requires a second read. Not because the numbers are complicated,
- 33:15but because they are so far outside the range of
- 33:18anything familiar that the brain keeps trying to file them
- 33:21away as typos M eighty seven is not simply a
- 33:25large galaxy sitting at the gravitational center of the Virgo cluster.
- 33:30It is a structure that has been consuming other galaxies
- 33:34for billions of years, growing more massive with each collision,
- 33:39each merger, each smaller system it has pulled apart, and
- 33:43absorbed into itself. The star count alone is enough to
- 33:47stop you. The Milky Way contains somewhere between two hundred
- 33:52and four hundred billion stars. That number is already difficult
- 33:57to hold. M eighty seven contains an estimated twelve trillion
- 34:02That is roughly thirty times as many stars as our
- 34:05entire galaxy. But raw star counts do not capture what M.
- 34:09Eighty seven actually is. This was because M eighty seven
- 34:13is not just bigger than the Milky Way in the
- 34:15way that a stadium is bigger than a house. It
- 34:18is a different category of object entirely. The Milky Way
- 34:21is a spiral galaxy, relatively flat, with defined arms and
- 34:26a disk STRUCTUREM eighty seven is an elliptical galaxy, a vast,
- 34:31roughly spherical cloud of stars sprawling outward in every direction,
- 34:35with no arms, no disk, no particular shape beyond sheer
- 34:40accumulated mass. Elliptical galaxies like M eighty seven are generally
- 34:44understood to be the end product of repeated galactic mergers.
- 34:48They are what you get after enough collisions have destroyed
- 34:51the original structure and left behind something enormous and featureless.
- 34:56At the center of M. Eighty seven, sits, something that
- 34:59may makes the galaxy itself feel like a backdrop. There
- 35:03is a supermassive black hole there. Its mass is measured
- 35:07at approximately six point five billion times the mass of
- 35:11our Sun. For comparison, the black hole at the center
- 35:15of the Milky Way, known as Sagittarius a star, has
- 35:19a mass of roughly four million solar masses. The black
- 35:23hole inside eight seven is more than a thousand times
- 35:27more massive than our own. It is one of the
- 35:29most massive black holes ever measured anywhere in the observable universe,
- 35:35and in twenty nineteen it became the first black hole
- 35:38ever directly photographed. That image is worth pausing on the
- 35:43event horizon telescope that is not a single telescope, but
- 35:48a coordinated network of radio observatories spread across multiple contiments,
- 35:54operating together as a single earth sized instrument turned its
- 35:58collective gaze toward eight seven and produced an image of
- 36:03the shadow of that black hole surrounded by a ring
- 36:05of glowing gas. The photograph showed an asymmetric orange ring
- 36:11brighter on one side than the other due to the
- 36:14rotation of the material around it. It was blurry by
- 36:17some standards. It was the most important astronomical photograph in decades.
- 36:23That object, the dark center of that orange ring is
- 36:27the supermassive black hole sitting at the heart of the
- 36:30dominant galaxy at the center of our supercluster. It is
- 36:34roughly fifty five million light years away, and we photographed it.
- 36:39The black hole does not sit quietly. M eighty seven
- 36:43has what astronomers call an active galactic nucleus, meaning the
- 36:48black hole is actively consuming surrounding material and releasing extraordinary
- 36:53amounts of energy in the process. The infalling gas forms
- 36:57a superheated disc from the poles of that DISM eighty
- 37:01seven launches jets of plasma outward into space. These jets
- 37:05travel at a significant fraction of the speed of light.
- 37:09One of them extends for roughly five thousand light years
- 37:12and is bright enough to have been observed for over
- 37:15a century. Karl Yansky detected the radio emissions from M
- 37:19eighty seven in the early twentieth century without fully understanding
- 37:23what he was looking at. The jet is not subtle.
- 37:26It is one of the most energetic continuous structures in
- 37:29the known universe, blasting through the surrounding gas of the
- 37:33Virgo cluster and depositing enormous amounts of energy into the
- 37:37cluster environment. That energy output affects the temperature and behavior
- 37:43of gas throughout the cluster. That MEANSM eighty seven's black
- 37:47hole is not just a local feature, but something that
- 37:50actively shapes the environment of the entire structure surrounding it.
- 37:54The sheer size of M eighty seven extends far beyond
- 37:57its visible core. The galaxy has a few stellar halo
- 38:01that reaches outward for hundreds of thousands of light years,
- 38:05filled with stars stripped from smaller galaxies during past merges.
- 38:10Some of the material at the edges of M eighty
- 38:12seven was almost certainly part of independent galaxies at some
- 38:17earlier pointing cosmic history, galaxies that wandered too close and
- 38:21were dismantled over time their stars scattered into the halo.
- 38:26This process is still ongoing. M eighty seven is still
- 38:29the gravitational dominant presence in the Virgo cluster, still pulling
- 38:34in material, still growing. One of the clearest ways to
- 38:37see how DIFFERENTM. Eighty seven is from the Milky Way
- 38:41is not through the star counts or the black hole mass,
- 38:45but through globular clusters. Globular clusters are dense ancient spherical
- 38:51groupings of stars, typically containing hundreds of thousands of stars
- 38:56bound tightly together. Most large galaxies host upon population of
- 39:00them in a halo around their center. They are among
- 39:04the oldest structures in the universe, some of them nearly
- 39:07as old as the universe itself. The Milky Way has
- 39:11approximately one hundred and fifty known globular clusters orbiting it.
- 39:16When astronomers surveyed the region around M eighty seven, they
- 39:20found something of a different order. M eighty seven is
- 39:24surrounded by a halo of approximately fifteen thousand globular clusters.
- 39:29Some of those clusters were likely captured along with the
- 39:32galaxies that M eighty seven absolute rebover billions of years.
- 39:38The number is not slightly larger than the Milky Ways count.
- 39:42It is one hundred times larger. The Milky Way has
- 39:45roughly one hundred and fifty globular clusters orbiting it. M
- 39:49eighty seven has around fifteen thousand. That tells you about
- 39:53as much as you need to know about the difference
- 39:56between these two galaxies. If you could step back far
- 40:00far enough to see the entire Virgo supercluster at once,
- 40:03the first thing you would notice is that it does
- 40:06not look like a cloud. It does not look like
- 40:09a sphere or a blob or any of the rounded
- 40:12shapes that the word cluster might suggest. What you would
- 40:16actually see is a web thin strands of galaxies stretching
- 40:20across enormous distances, connecting denser knots trailing off into near emptiness,
- 40:27sheets of galaxies arranged in flat planes, like the surface
- 40:31of a soap bubble, and between those strands and sheets
- 40:35vast regions of almost nothing. The structure looks less like
- 40:39a storm and more like the skeleton of one all
- 40:42framework and void, with the actual material pinned to the
- 40:46edges of the gaps. This is not unique to the
- 40:49Virgo Supercluster. It is the signature of how gravity has
- 40:53worked on matter across the entire history of the universe.
- 40:57But the Virgo Supercluster is close enough to study in detail,
- 41:01and what astronomers have found in its architecture is something
- 41:05that took decades to fully appreciate. The universe does not
- 41:09fill itself evenly. It builds highways, and then it builds nothing.
- 41:15Start with the galaxies themselves. Two thirds of the bright
- 41:19galaxies in the Virgo Supercluster are not scattered randomly across
- 41:23its full volume. They are concentrated near a central plane,
- 41:27a flattened disk running through the structure like the equatorial
- 41:31belt of some enormous slow spinning system. The remaining third
- 41:35spread outward into a looser halo, distributed more spherically around
- 41:40the central concentration, but still not evenly, still clumped and
- 41:45streaked rather than smooth. If you mapped only the bright
- 41:49galaxies and drew their positions in three dimensions, the result
- 41:53would look almost like a flattened lens with faint spray
- 41:56around it. This is the overall shape, but inside that
- 42:00shape the detail is stranger. There are two primary filaments
- 42:04threading through the supercluster, and they behave like rivers. One
- 42:09of them runs from the region near the URSA major group,
- 42:12passing through the IC three hundred and forty two group
- 42:16and continuing through them eighty one group, a chain of
- 42:19galaxy concentrations loosely strung along a common axis, separated by
- 42:25tens of millions of light years, but connected by their
- 42:28shared trajectory toward the gravitational center. The second filament runs
- 42:33in a different direction, entirely linking the Sculptor group into
- 42:38the broader network and eventually connecting toward the Virgo cluster itself.
- 42:43These are not coincidences of position. Galaxies in filaments are
- 42:47moving along them. They are drifting, pulled by gravity, following
- 42:52the path of the strand toward whichever dense concentration lies
- 42:56at the far end. The filaments are not static structure,
- 43:00They are currents. Think of it like a water shed.
- 43:04Water on a hillside does not flow in random directions.
- 43:08It follows the contours of the landscape toward the lowest points.
- 43:12Galaxies do something similar, but the landscape is gravity itself,
- 43:17shaped by the distribution of matter and dark matter across
- 43:21hundreds of millions of light years. The filaments mark the
- 43:24low channels in that gravitational terrain. Groups of galaxies that
- 43:28formed in the filaments find themselves slowly accelerating along the strand,
- 43:33drawn toward the massive clusters that anchor the intersections. The
- 43:37Virgo cluster sits at one of those intersections, which is
- 43:41precisely why it has grown so dominant. It is not
- 43:45just massive. It is positioned where the floes converge between
- 43:49the filaments of the voids, and the voids deserve their
- 43:52own attention because it is easy to treat them as
- 43:55the absence of something interesting, rather than as something interesting
- 43:59in themselves. Avoid spanning thirty or forty million light years
- 44:04as a place where the large scale structure of the
- 44:06universe has essentially failed to form. In the early universe,
- 44:10matter was distributed nearly evenly. Tiny density fluctuations. Regions slightly
- 44:17more dense regions slightly less were the seeds of everything
- 44:21that came after. Where the density was slightly higher, gravity
- 44:25pulled more matter in, and those regions grew into filaments
- 44:29and clusters. Where the density was slightly lower, matter drained
- 44:33away into the surrounding over dense regions, and those regions
- 44:37became voids. The voids did not stay empty by accident.
- 44:41They were emptied actively, their matter flowing outward into the
- 44:46surrounding structure over billions of years. They are not completely empty.
- 44:51A careful survey of a large void will find occasional
- 44:55isolated galaxies, small groups that never fell into a filament,
- 45:00stragglers left behind by the general flow. But the contrast
- 45:04between a void and a filament is stark enough to
- 45:07register immediately in any map of the supercluster. Inside a filament,
- 45:13you might find dozens of galaxies within a few million
- 45:16light years of each other. Step into a void, and
- 45:20you could travel ten twenty thirty million light years and
- 45:25encounter almost nothing. The density drops by a factor that
- 45:29is difficult to express simply, if a filament is a
- 45:33busy street, a void is open ocean with one island
- 45:37every thousand kilometers. The overall structure filaments, sheets, clusters, voids
- 45:45is what astronomers call the cosmic web. The Virgo supercluster
- 45:50is not some exotic exception to the general pattern of
- 45:54the universe. It is a textbook example of it, close
- 45:58enough to study in fine detail, large enough to contain
- 46:01all of the major features. But knowing that it fits
- 46:04the pattern does not make the pattern less astonishing. The
- 46:08visible matter in this structure, all the stars and gas
- 46:11and dust that telescopes can detect, traces out something that
- 46:15looks almost designed, almost deliberate, long thin strands of galaxies
- 46:21arking across tens of millions of light years, dense nodes
- 46:25where strands intersect, enormous hollow regions where almost nothing has gathered.
- 46:32The universe built something that looks at this scale more
- 46:35like lace than like anything solid. The question of what
- 46:39actually holds this structure in the arrangement we observe is
- 46:43not fully answered by the galaxies alone. The visible matter
- 46:46follows the pattern, but it does not set the pattern.
- 46:50Something unseen is doing most of the gravitational work, and
- 46:54that is a problem that belongs to the next part
- 46:56of the picture. For now, the shape itself the thing
- 47:00worth holding. A supercluster one hundred and ten million light
- 47:04years across that is not a sphere, not a cloud,
- 47:08not a uniform distribution of anything, a web of strands
- 47:12and sheets built over billions of years by the slow
- 47:16arithmetic of gravity, with vast silent gaps between every thread.
- 47:21The voids between these filaments are real. They are not
- 47:24just gaps in our maps, and they can span tens
- 47:27of millions of light years with almost nothing in them.
- 47:31The Virgo cluster is not the only thing pulling on us.
- 47:34This took a while to figure out. For decades, the
- 47:37assumption was straightforward. The Virgo cluster sits at the gravitational
- 47:42center of the supercluster. Our local group sits near the edge.
- 47:46The cluster pulls us slowly inward. A clean picture, a
- 47:50sensible one. Then astronomers started measuring the actual velocities of
- 47:55galaxies across our region of space with more precision, the
- 47:59clean pure developed a problem. Everything was moving in the
- 48:03wrong direction. Not wrong in the sense of random or chaotic,
- 48:07but wrong in the sense that the motion did not
- 48:09point where the Virgo Cluster was. Galaxies across a vast
- 48:13stretch of the local universe were streaming toward a particular
- 48:17point in the sky, a point in the direction of
- 48:20the constellation Centaurus, roughly two hundred and fifty million light
- 48:24years away. The Virgo Cluster could not account for this.
- 48:29Something else was out there, something massive, and it was
- 48:33pulling on everything in the neighborhood. Astronomers named it the
- 48:36Great Attractor. The name sounds dramatic, and the reality earns
- 48:41that drama. The Great Attractor appears to be a concentration
- 48:46of mass so enormous that it is drawing not just
- 48:49our local group, but effectively our entire supercluster toward it.
- 48:54The infull velocity toward the Virgo cluster is roughly three
- 48:58hundred kilometers per second. The streaming motion toward the Greater
- 49:02Tractor runs at somewhere between six hundred and one thousand
- 49:05kilometers per second. Those are not small numbers. Light travels
- 49:10at three hundred thousand kilometers per second, so these are
- 49:14not relativistic speeds, but for the slow gravitational choreography of
- 49:18galaxy clusters drifting through space, these are remarkable velocities. Something
- 49:24very large is doing the pulling. The problem is seeing
- 49:27it directly. The Greater Tractor sits behind one of the
- 49:31most frustrating obstacles in observational astronomy. In that direction of sky,
- 49:36our line of sight passes straight through the densest part
- 49:40of the Milky Way zone, disc through the concentrated dust
- 49:44and gas of our galaxy's central plane. This region is
- 49:47called the zone of avoidance, and it does exactly what
- 49:50its name suggests. The disk of our own galaxy blocks
- 49:54the view. Optical telescopes cannot penetrate it. The light from
- 49:59whatever lies when that direction is absorbed or scattered before
- 50:02it reaches us. For years, the Great Attractor was essentially
- 50:07a gravitational rumor something inferred entirely from the motion of
- 50:11other things, rather than seen directly. Radio and X ray
- 50:16surveys eventually pierced the obscuring disk well enough to identify
- 50:20what is likely the primary culprit. The normal cluster, a
- 50:24rich concentration of galaxies sitting roughly at the position the
- 50:28greater attractor was predicted to occupy, has a mass consistent
- 50:32with much of the observed streaming motion. It became the
- 50:36leading candidate for what astronomers had been sensing through the
- 50:39motion of galaxies for years, but identifying the Normal cluster
- 50:44did not entirely close the case. When researchers ran the
- 50:48numbers carefully, the normal cluster alone was not quite heavy
- 50:52enough to account for everything that was observed the streaming
- 50:56motion suggested something more behind the normal A cluster farther
- 51:01along the same general direction sits, the Shapleigh Supercluster, at
- 51:06a distance of roughly six hundred fifty million light years.
- 51:10The Shapleigh Supercluster is one of the largest concentrations of
- 51:14matter in the nearby universe, a vast gathering of galaxy
- 51:19clusters containing mass that dwarfs the Virgo supercluster by a
- 51:23considerable margin. Current thinking places the Shapleigh Supercluster as a
- 51:28significant contributor to the overall streaming motion, working alongside the
- 51:34normal cluster region to produce the pool that shows up
- 51:37in galaxy velocity measurements across our neighborhood. The greater tractor,
- 51:41in other words, may not be a single thing at all.
- 51:45It may be a direction, a general zone of extreme
- 51:48mass density that combines several overlapping gravitational sources, each adding
- 51:54its weight to the total pool. What makes this genuinely
- 51:57strange is the scale involved. The Virgo cluster is fifty
- 52:01five million light years away, its gravitational influence on the
- 52:05local group is already difficult to absorb. The Shapleigh supercluster
- 52:10is more than ten times farther, yet its gravity reaches
- 52:14back across that distance and perceptibly nudges the motion of
- 52:17galaxies in our region. Gravity has no speed limit in
- 52:21the sense of influence. A mass concentration that formed billions
- 52:25of years ago began shaping the flow field around it,
- 52:29long before any astronomer existed to notice. The streaming motion
- 52:33we measure today is the accumulated product of billions of
- 52:37years of gravitational influence propagating outward from these massive concentrations. Then,
- 52:44in two thousand eight, a team of researchers published results
- 52:48suggesting something stranger still. Using data from the w MAP satellite,
- 52:54they reported that galaxy clusters at distances of several billion
- 52:58light years appear feared to be drifting coherently in a
- 53:02particular direction, a bulk flow that could not be explained
- 53:06by any known concentration of mass within the observable universe.
- 53:11They called this dark flow. The implication was unsettling. If
- 53:16the signal was real, something beyond the observable horizon structures
- 53:21so distant that their light has never reached us and
- 53:25never will. Given the expansion of the universe, might be
- 53:29exerting gravitational influence on matter inside our observable bubble. The
- 53:35universe we can see would be in a gravitational sense,
- 53:39not the whole story. Dark flow remains contested. Later analyzes
- 53:44using more sensitive CMB data have not consistently reproduced the
- 53:49original signal. The debate among cosmologists has not reached a
- 53:53clean resolution. Some researchers argue the original detection was a
- 53:58measurement artifact. Others maintain that the signal is real and
- 54:03that its explanation demands something genuinely new. The honest position
- 54:08is that the question is open, but the broader picture
- 54:11is not in doubt. The local group is embedded in
- 54:15a gravitational landscape far more complex than a simple infall
- 54:19toward the Virgo cluster. Multiple massive structures, some clearly identified,
- 54:24in some only partially visible, pull on us from different
- 54:28distances in different directions. The net motion we observe is
- 54:32the vector sum of all of these influences, tangled together
- 54:36across hundreds of millions of light years. Unpacking them requires
- 54:40measuring the velocities of thousands of galaxies and running those
- 54:44measurements through models that attempt to reconstruct the underlying mass distribution.
- 54:49It is an extraordinary thing to do. It is also
- 54:52not finished. Some researchers have raised the possibility that the
- 54:56pull comes from structures so large and so distant that
- 55:00they lie beyond the edge of what we can observe.
- 55:03That means we may never be able to see what
- 55:06is tugging on us. Everything discussed so far, the galaxies,
- 55:11the clusters, the filaments, the Virgo cluster M eighty seven
- 55:16represents only about ten percent of what is actually in
- 55:19the Virgo supercluster. The rest is dark matter, not dark energy,
- 55:25which is a separate concept entirely. Dark matter is matter,
- 55:30It is mass, It is gravity. It pulls on things.
- 55:34What it does not do is interact with light in
- 55:37any way that telescopes can detect. It does not emit light,
- 55:41It does not absorb light, it does not reflect light.
- 55:45It simply sits there, invisible and exerts gravitational force on
- 55:50everything around it. When astronomers calculate the total mass of
- 55:54the Virgo supercluster roughly one point four eight times ten
- 55:58to the fifteenth power solar massive, a number that is
- 56:01almost too large to write out, only about ten percent
- 56:05of that mass shows up in any telescope image ever taken.
- 56:09The galaxies you see in photographs of the supercluster, all
- 56:13forty seven thousand of them, every star in every one
- 56:16of those galaxies, all the gas clouds and dust lanes
- 56:20in glowing nebulae, that is the ten percent. The ninety
- 56:24percent is somewhere else, or rather everywhere, spread through the
- 56:29same space, invisible and unmeasured by any direct observation. This
- 56:34is not a fringe idea. It is one of the
- 56:37most well tested conclusions in modern cosmology, and the evidence
- 56:41comes from multiple independent directions at once. The first serious
- 56:46hints appeared in the nineteen thirties, when Swiss astronomer Fritz
- 56:50Swicky measured the velocities of galaxies inside the coma cluster
- 56:55and found something that did not add up. The galaxies
- 56:58were moving too fast. At those speeds, the cluster should
- 57:02have flown apart long ago. There was simply not enough
- 57:05visible mass to hold them together. Zwicki proposed that unseen
- 57:10matter was providing the extra gravity. For decades, most astronomers
- 57:14dismissed the idea. Then, in the nineteen seventies, VERA. Rubin
- 57:19and her colleagues measured the rotation curves of individual spiral
- 57:23galaxies and found the same problem at a different scale.
- 57:28Stars at the outer edges of galaxies were orbiting too fast.
- 57:32The visible mass of the galaxy could not account for it.
- 57:35Something invisible was adding gravity at the edges. The flat
- 57:39rotation curves that Reuben documented became one of the clearest
- 57:43pieces of evidence that dark matter was real and that
- 57:47it extended well beyond the visible boundaries of galaxies. The
- 57:51evidence kept piling up. When astronomers mapped how light from
- 57:56distant objects bends as it passes through galaxy clusters, a
- 58:00phenomenon called gravitational lensing, they could calculate how much mass
- 58:05was doing the bending. The number was consistently far higher
- 58:09than the mass of all the visible galaxies and gas
- 58:12in the cluster combined, the extra mass had to be
- 58:16there somewhere, in a form that telescopes could not see.
- 58:20Then came the large scale structure arguments. Cosmologists running simulations
- 58:26of how the universe evolved from the hot, nearly uniform
- 58:30state after the Big Bang found that ordinary matter alone
- 58:34could not produce the structures we observe. Galaxies, clusters, filaments, superclusters.
- 58:41None of it forms fast enough without something else. Dark
- 58:45matter clumps differently than ordinary matter because it does not
- 58:49interact with radiation. While the early universe was a dense,
- 58:53hot plasma of particles and light, all jostling and colliding,
- 58:58dark matter was already beginning to gather quietly into halos,
- 59:02building the gravitational scaffolding that ordinary matter would later collapse into.
- 59:07Without that head start, the universe should look almost smooth today. Instead,
- 59:13it looks like a web. Dark matter is why, within
- 59:17the Virgo supercluster, specifically, that web is what defines the
- 59:21shape of everything. The filaments are not random, The sheets
- 59:26of galaxies are not random. The concentration of galaxies in
- 59:30the Virgo cluster, rather than scattered evenly across the supercluster's
- 59:35volume is not random. All of it traces the underlying
- 59:39dark matter skeleton, which formed first and poured ordinary matter
- 59:43into the patterns we observe. Galaxies drift toward the densest
- 59:47nodes of the dark matter web, gas collects along its filaments,
- 59:52cools formed stars, and lights up what was already there. Structurally,
- 59:57in this sense, every galaxy photograph ever taken is really
- 1:00:01a map of dark matter. The glowing points are just
- 1:00:04the places where the dark matter density was high enough
- 1:00:08and the conditions right enough for ordinary matter to ignite.
- 1:00:12The Virgo Cluster itself sits at one of the deepest
- 1:00:15wells in the local dark matter distribution. Its gravitational pull
- 1:00:19on surrounding galaxies, the infowl we discussed the thousands of
- 1:00:24galaxies that have already been captured, is almost entirely a
- 1:00:28dark matter phenomenon. The visible mass of the cluster is
- 1:00:32enormous on its own terms, but the dark matter halo
- 1:00:35surrounding it extends far beyond the visible galaxies and accounts
- 1:00:40for roughly ten times as much mass as everything that
- 1:00:43lights up. What you see when you look at a
- 1:00:45photograph of the Virgo Cluster is a small bright signal
- 1:00:49riding on top of a vast, invisible structure that outweighs
- 1:00:53it by an order of magnitude. This creates a strange
- 1:00:56picture of what the Virgo supercluster actually is. Strip Away
- 1:01:00the dark matter and the supercluster would not exist as
- 1:01:03a recognizable structure. The galaxies would not be concentrated where
- 1:01:08they are, the filaments would not run the way they do.
- 1:01:11The clusters would not have formed at all, at least
- 1:01:14not in the time the universe has had available the
- 1:01:17entire architecture. Everything described in the previous sections, all the
- 1:01:22structure and motion and gravitational dynamics, is downstream of something
- 1:01:27we cannot see. The filamentary skeleton of dark matter came first,
- 1:01:32the galaxies followed. The supercluster is, in the deepest sense,
- 1:01:37a dark matter object that happens to have galaxies growing
- 1:01:40inside it. We have never directly detected a dark matter particle.
- 1:01:45Every attempt to catch one in a laboratory detector has
- 1:01:48come up empty. So far. Experiments buried deep underground, shielded
- 1:01:53from everything else, have been running for decades waiting for
- 1:01:56a dark matter particle to bump into an ordinary atom.
- 1:02:00Nothing confirmed yet. The evidence that dark matter exists is overwhelming.
- 1:02:05The evidence for what it actually is remains frustratingly incomplete.
- 1:02:10The galaxies are real, but they are the small bright
- 1:02:12things attached to a vast invisible structure, and the invisible
- 1:02:16structure is what actually holds everything in place. The Virgo
- 1:02:20supercluster is not a permanent feature of the universe. That
- 1:02:24fact sits uncomfortably alongside everything else in this story because
- 1:02:29the scale of the structure makes permanence feel like it
- 1:02:32should be guaranteed. Something one hundred ten million light years
- 1:02:36across should not be fragile, but it is, and the
- 1:02:40force undoing it has been at work since the beginning.
- 1:02:44Start with what happens first. In roughly five billion years,
- 1:02:48the Milky Way and Andromeda will collide. They are already
- 1:02:51moving toward each other, closing the gap at about one
- 1:02:54hundred and ten kilometers per second. When two galaxies merge,
- 1:02:58it is not a collision in the way two cars collide.
- 1:03:02The stars inside each galaxy are so far apart that
- 1:03:05almost none of them will actually strike another star. What
- 1:03:09happens instead is slower and stranger. The two galaxies will
- 1:03:13pass through each other, distort each other's shapes, swing around,
- 1:03:17pass through again, and over hundreds of millions of years,
- 1:03:21gradually spiral into a single combined structure. Astronomers have a
- 1:03:26name for what comes out the other side. They call
- 1:03:29it Milkomeda. It will be a large elliptical galaxy, rounder
- 1:03:34and less structured than either of the spirals that produced it,
- 1:03:37and it will contain the stars of both. The night
- 1:03:40sky viewed from any surviving planet during that merger will
- 1:03:45look nothing like what we see now. The Milky Way
- 1:03:48band will warp, Andromeda will fill enormous stretches of sky.
- 1:03:53Then slowly the two will become one. Milkomeda will still
- 1:03:57be part of the local group. The merger changes the
- 1:04:01dominant member, but not the group's membership or its trajectory.
- 1:04:05The local group, now organized around a single giant merged galaxy,
- 1:04:10will continue its slow fall toward the Virgo cluster that
- 1:04:14in four has been happening for billions of years already,
- 1:04:17and will not stop because the Milky Way and Andromeda
- 1:04:21decided to combine. Gravity does not pause for mergers. But
- 1:04:25here is where the story turns, because while gravity is
- 1:04:29pulling the local group inward, something else is pushing everything outward.
- 1:04:34Dark energy, the force responsible for the accelerating expansion of
- 1:04:39the universe, does not care about the gravitational hierarchy. It
- 1:04:44acts on all scales simultaneously. At small scales, gravity wins easily.
- 1:04:50The Earth stays bound to the Sun. The Sun stays
- 1:04:53bound to the Milky Way. Galaxy clusters hold themselves together
- 1:04:58against the expansion because the gravity inside them is strong
- 1:05:02enough to overpower it. But superclusters are a different situation. Entirely,
- 1:05:07the Virgo supercluster is not gravitationally bound. That is a
- 1:05:12precise statement with enormous consequences. A gravitationally bound system is
- 1:05:17one where the collective gravity of all its members is
- 1:05:20strong enough to hold the group together against the expansion
- 1:05:24of space. Galaxy clusters pass this test. The Virgo cluster
- 1:05:29itself is bound. Those thousands of galaxies are locked together
- 1:05:33and will not be pulled apart. The local group is bound,
- 1:05:37but the supercluster as a whole, the full one hundred
- 1:05:40and ten million light year structure, containing all of its
- 1:05:43clusters in groups and filaments, does not have enough internal
- 1:05:47gravity to hold itself together over the long run. Dark
- 1:05:51energy is winning at this scale. What that means, played
- 1:05:54out over tens of billions of years, is a gradual dissolution.
- 1:05:59The outer regions go first, the galaxies and group sitting
- 1:06:04in the looser periphery of the supercluster. The ones not
- 1:06:07tightly locked into dense clusters will find that the expansion
- 1:06:11of space slowly overcomes the weak gravitational threads connecting them
- 1:06:16to the rest of the structure. They will drift outward,
- 1:06:20not violently. There is no explosion, no sudden break. It
- 1:06:24is more like a crowd slowly dispersing after an event ends.
- 1:06:29One person leaves, then another, Then the edge is thin out,
- 1:06:33and eventually what was a gathering is just scattered individuals
- 1:06:36moving in different directions. The tightly bound clusters survive this.
- 1:06:42The Virgo cluster will remain intact. The local group once
- 1:06:46it has merged into Milkomeda and eventually fallen closer to
- 1:06:50the cluster may be drawn in and absorbed. What survives
- 1:06:54in the very long run is not the supercluster, but
- 1:06:57its gravitational cause. The dense, tightly packed clusters that gravity
- 1:07:02has held together strongly enough to resist the expansion. Everything
- 1:07:08between them will have drifted away. This is worth sitting
- 1:07:11with for a moment. The structure we have been describing,
- 1:07:15the filaments, the sheets, the vast, interconnected web of groups
- 1:07:20and clusters spanning one hundred ten million light years is
- 1:07:24a temporary arrangement. It formed because the early universe had
- 1:07:28density variations, small lumps in the distribution of matter and gravity.
- 1:07:33Spent billions of years amplifying those lumps into the structures
- 1:07:37we see today. But the expansion of the universe was
- 1:07:40always running in the other direction, and at supercluster scales,
- 1:07:44expansion is winning. What exists now is the peak, the
- 1:07:49moment of maximum structure at this scale. From here, the
- 1:07:53supercluster does not grow more organized. It begins slowly to
- 1:07:57come apart. There is a version of this that sounds
- 1:08:00like loss. A structure assembles itself over thirteen billion years,
- 1:08:06and then dark energy spends the next one hundred billion
- 1:08:09years quietly dismantling it. The galaxies that formed in the
- 1:08:13outer filaments, that spent their entire existence as part of
- 1:08:17this supercluster, will drift out into regions of space increasingly
- 1:08:22empty of neighbors. The filaments will thin, the sheets will fade.
- 1:08:28The cosmic web, at least locally, will unravel, but the
- 1:08:33time scales involved strip the word loss of most of
- 1:08:36its meaning. The complete dissociation of the supercluster happens over
- 1:08:40stretches of time so long that the Sun will have died,
- 1:08:44the Milky Way will have merged with Andromeda, and the
- 1:08:47stars formed in that merger will themselves have aged and faded. Life,
- 1:08:53if it still exists anywhere, will be operating on a
- 1:08:56fundamentally different set of physics problems than we are. The
- 1:09:00supercluster dissolving is not an event anyone will experience. It
- 1:09:04is a slow reversion to the mean of an expanding universe.
- 1:09:08What we are looking at from our vantage point near
- 1:09:11the edge is a structure in the process of being
- 1:09:14assembled and then slowly torn apart by the same expanding
- 1:09:19universe that created the conditions for it to form. In
- 1:09:22twenty fourteen, a team of astronomers published a paper that
- 1:09:26quietly moved the Virgo supercluster I leveled down in the hierarchy.
- 1:09:31No dramatic announcement, no press conference that made the evening news.
- 1:09:37A paper in the journal Nature, authored by R. Brent
- 1:09:41Tulley in his colleagues, and inside it was a map
- 1:09:44that changed our cosmic address. The Virgo Supercluster, one hundred
- 1:09:50ten million light years across, containing tens of thousands of galaxies,
- 1:09:55the structure that had anchored our sense of place in
- 1:09:58the universe for sixty years. It was not the top
- 1:10:01of the ladder. It was a branch, a single lobe
- 1:10:05of something vastly larger that nobody had fully seen before.
- 1:10:09They called it lania KaiA. The name comes from Hawaiian
- 1:10:13meaning immeasurable heaven, and the people who chose it were
- 1:10:16not being poetic, They were being accurate. Lania KaiA spans
- 1:10:21roughly five hundred and twenty million light years. It contains
- 1:10:25around one hundred thousand galaxies. Its mass is approximately ten
- 1:10:30to the power of seventeen solar masses. If you stacked
- 1:10:33that number out in suns, you would run out of
- 1:10:36ways to describe it before you got close. The Virgo Supercluster,
- 1:10:41for all its scale, accounts for only a fraction of
- 1:10:44what lanier KaiA actually is. To understand why this discovery
- 1:10:48was possible in twenty fourteen and not earlier, you have
- 1:10:52to understand what Tully's team did differently. Previous maps of
- 1:10:55the large scale universe were built on positions you measure
- 1:10:59a game. Galaxies redshift, you calculate its distance, You plot
- 1:11:04it on a map. Do that for enough galaxies, and
- 1:11:07patterns emerge, clusters, filaments, voids. That approach built everything we
- 1:11:13knew about the Virgo supercluster. It was good science, but
- 1:11:17it had a blind spot. It could tell you where
- 1:11:20galaxies were, it could not easily tell you which way
- 1:11:23they were falling. Tully's team mapped velocities, not just how
- 1:11:27fast galaxies were moving away from us due to cosmic expansion,
- 1:11:32but how fast they were moving relative to that expansion.
- 1:11:35Their peculiar velocities the component of motion driven by local
- 1:11:40gravity rather than the universe's overall stretching. If you can
- 1:11:44measure that for hundreds of thousands of galaxies, something remarkable
- 1:11:49becomes visible. You can see the flow. Galaxies are like
- 1:11:53water running downhill. They drift toward gravitational concentrations. Map enough
- 1:11:59of those drift vectors and you can trace the basins,
- 1:12:03the regions of space where everything is flowing toward a
- 1:12:06common point, where one basin ends and another begins. That
- 1:12:10is a boundary. That boundary defines a supercluster. This was
- 1:12:15the conceptual shift. A supercluster is not just a dense
- 1:12:19region of galaxies. It is a gravitational watershed. Everything within
- 1:12:24it is flowing inward toward a common attractor, and nothing
- 1:12:28crosses the ridge line into the next basin. By that definition,
- 1:12:32the Virgo Supercluster was not its own watershed. It was
- 1:12:36a tributary. All of its galaxies, including our own Milky Way,
- 1:12:40are flowing not just toward the Virgo Cluster, but towards
- 1:12:44something deeper inside Lanikaea. That's something is the greater attractor,
- 1:12:49the mysterious gravitational concentration that astronomers had been puzzling over
- 1:12:54for decades, partially hidden behind the plane of our own galaxy.
- 1:12:58It sits near the center of Lanikaea, in the region
- 1:13:01of the Norma cluster, and it is the point toward
- 1:13:04which the entire flow of our supercluse tear ultimately drains.
- 1:13:10Lania Kaya is not just the Virgo Supercluster scaled up.
- 1:13:14It is a different kind of object. It contains the
- 1:13:17Virgo Supercluster as one component, but also the Hydra Centaurus Supercluster,
- 1:13:23the Normal Supercluster, the pavo Inda Supercluster, and several other
- 1:13:28large concentrations of galaxies that were previously considered separate structures,
- 1:13:34all of them, it turns out, a part of the
- 1:13:36same gravitational basin. All of them are flowing toward the
- 1:13:40same attractor. The boundaries that astronomers had drawn between them
- 1:13:44were real in a positional sense, they were not real
- 1:13:47in a dynamical one. The numbers require a moment. The
- 1:13:51Virgo supercluster is one hundred and ten million light years across,
- 1:13:56Lania KaiA is five hundred and twenty million light years across.
- 1:13:59That is not a modest expansion of the neighborhood. It
- 1:14:02is nearly five times the diameter, which means roughly one
- 1:14:06hundred times the volume. Lanier Kia contains about one hundred
- 1:14:10thousand galaxies. To the Virgo superclusters forty seven thousand, its
- 1:14:15mass is one hundred times greater. Every measure of it
- 1:14:18is overwhelming. In a different direction. Here is something worth
- 1:14:23sitting with the greater tractor. That object at the heart
- 1:14:27of Lanier KaiA, toward which we are all slowly falling,
- 1:14:31was discovered because astronomers noticed an unexplained tug on galaxies
- 1:14:35throughout our region of space. For years, they could not
- 1:14:39identify the source clearly because the milky way's own disc
- 1:14:43blocked the view. They knew something massive was there, they
- 1:14:47couldn't see it directly, And when Tully's team mapped the
- 1:14:51flow patterns across hundreds of thousands of galaxies, the shape
- 1:14:56of that hidden center finally came into focus, not as
- 1:15:00a visible object, as a pattern in motion. The attractor
- 1:15:05revealed itself through what everything around it was doing. That
- 1:15:09is an almost strange way to discover the center of
- 1:15:12your home, not by looking at it, but by watching
- 1:15:15which way everything falls. Lania kaya is almost certainly not
- 1:15:20gravitationally bound in the way a galaxy cluster is the
- 1:15:23same dark energy pulling apart. The Virgo supercluster at its
- 1:15:27periphery is doing the same thing at lania Kaia's scale,
- 1:15:31only more so. What Tully's team identified is a structure
- 1:15:35defined by present day flow patterns, not a permanent gravitational cage.
- 1:15:40Over billions of years, as cosmic expansion continues to accelerate,
- 1:15:46the flow will weaken, the water shared boundaries will dissolve,
- 1:15:50and lanikaere as a coherent structure, will fade. What we
- 1:15:54are mapping now is real, but temporary, in the way
- 1:15:58that all things that superclusters gales are temporary. None of
- 1:16:01this was apparent in twenty thirteen. In twenty thirteen, the
- 1:16:06Virgo Supercluster was the answer to the question of what
- 1:16:09our largest local structure was called. One year later, it
- 1:16:14was a lobe, a single tendril flowing into something five
- 1:16:18times its size, anchored to a gravitational center that had
- 1:16:22been partially hidden from us the entire time. Every time
- 1:16:26the map gets redrawn, we end up living somewhere slightly smaller.
- 1:16:30Our galaxy shrank when we measured it against others. Our
- 1:16:34supercluster shrank when we found Lania Kea and Lania KaiA.
- 1:16:38Itself is embedded in a larger structure called the piscey
- 1:16:42Setu supercluster complex, which suggests the hierarchy may not end
- 1:16:47bear either. The Virgo supercluster is not unusual. That is
- 1:16:51perhaps the strangest thing about it. After everything, the one
- 1:16:56hundred ten million light years, the forty seven thousand galaxy,
- 1:17:00the gravitational pull of eighty seven, the dark matter skeleton
- 1:17:05holding it all together, the Virgo supercluster is by cosmic
- 1:17:09standards ordinary. The observable universe contains roughly ten million structures
- 1:17:15like it. Ten million each one spanning hundreds of millions
- 1:17:19of light years, each one containing tens of thousands of galaxies,
- 1:17:24each one anchored by its own massive central cluster, threaded
- 1:17:28by its own filaments, carved out by its own voids.
- 1:17:33The Virgo supercluster is not a landmark. It is a
- 1:17:36data point. To understand what that means, you have to
- 1:17:40zoom out past Lania KaiA, entirely past the five hundred
- 1:17:44and twenty million light years of that larger structure, past
- 1:17:47everything we have covered so far. At the scale where
- 1:17:51individual superclusters become visible as objects, the universe reveals its
- 1:17:56true architecture. It is not a uniform fog of galaxies.
- 1:18:00It is not a random scatter. It is a web.
- 1:18:04Astronomers call it the cosmic web, and it is the
- 1:18:07largest confirmed organizational structure in existence. Superclusters form the nodes
- 1:18:13connecting them of filaments, enormous strands of galaxies and dark matters,
- 1:18:18stretching across hundreds of millions of light years, sometimes more.
- 1:18:23Between the filaments of voids, vast mostly empty regions where
- 1:18:27almost nothing lives. The filaments themselves are staggering objects. A
- 1:18:32typical filament runs somewhere between fifty and five hundred million
- 1:18:36light years in length and maybe one or two megaparsecs thick.
- 1:18:41They are not solid structures. They are rivers of galaxies,
- 1:18:45loosely aligned, drifting toward the denser concentrations at their ends.
- 1:18:50The Virgo supercluster sits at one such node. The filaments
- 1:18:54feeding into it are part of a network that connects
- 1:18:57to other superclusters, other nodes, other gravitational anchors spread across
- 1:19:03the observable cosmos. Then there are the walls. If filaments
- 1:19:07are rivers, walls are something closer to continents. In two
- 1:19:11thousand three, astronomers mapping the Sloane Digital Sky Survey identified
- 1:19:17an enormous concentration of galaxies stretching nearly one point four
- 1:19:22billion light years across. They called it the Sloane Great War.
- 1:19:26At the time, it was the largest known structure in
- 1:19:29the universe. It held that title for about a decade.
- 1:19:33Then a team examining gamma ray burst distributions identified something else,
- 1:19:38the Hercules Corona Borealis Great Wall, roughly ten billion light
- 1:19:43years across. To call that a war is almost a
- 1:19:47category error. It spans nearly ten percent of the diameter
- 1:19:51of the entire observable universe. It is so large that
- 1:19:55some cosmologists debate whether it qualifies as a coherent structure
- 1:19:59at all, or whether it is simply a statistical density enhancement.
- 1:20:05So enormous it blurs the line between structure and background.
- 1:20:09This is where the definitions start to strain. There is
- 1:20:12a principle in cosmology called the cosmological principle. It holds
- 1:20:17that on large enough scales, the universe is roughly the
- 1:20:20same everywhere, homogeneous and isotropic, the same in every direction,
- 1:20:27the same in every region. The cosmic microwave background supports this.
- 1:20:32The after glow of the Big Bang is almost perfectly uniform,
- 1:20:36with tiny temperature fluctuations of only about one part in
- 1:20:40one hundred thousand. Those fluctuations grew into everything we see,
- 1:20:45but at scales above roughly three hundred million light years,
- 1:20:49the lumps and filaments should average out, the universe should
- 1:20:53look smooth. Structures like the Hercules, Corona Borealis Great Wall
- 1:20:59are so large they push against this expectation. They are
- 1:21:03either a genuine challenge to the cosmological pre enciple, or
- 1:21:08they are a reminder that our maps and our statistics
- 1:21:11have limits. Below that smoothing scale. Though the web is
- 1:21:15real and it is everywhere. Every supercluster we can identify
- 1:21:19sits within it. Every filament connects to something larger. Every
- 1:21:24void is bounded by walls that contain galaxies drifting along
- 1:21:28the edges. The structure repeats. It is not identical everywhere,
- 1:21:33but the pattern nodes, filaments, voids shows up across the
- 1:21:39entire observable universe with something close to regularity. Run a
- 1:21:44simulation of how the universe should have evolved from those
- 1:21:47tiny early fluctuations, applying known physics and the measured amounts
- 1:21:52of dark matter and dark energy, and you get a
- 1:21:55cosmic web that looks almost exactly like the one we observe.
- 1:22:00Yeb is not a surprise. It was predicted. It emerged
- 1:22:04from conditions set in the first fraction of a second
- 1:22:07after the Big Bang, encoded in the physics of how
- 1:22:10matter clumps under gravity when dark matter provides the scaffold.
- 1:22:15There are about ten million superclusters in the observable universe.
- 1:22:19The observable universe itself spans roughly ninety three billion light
- 1:22:24years in diameter. Inside that volume, there are an estimated
- 1:22:28two trillion galaxies two trillion, the Virgo supercluster holds perhaps
- 1:22:34forty seven thousand of them. That is not even close
- 1:22:37to a rounding error. Pull back to the scale where
- 1:22:40all ten million superclusters are simultaneously visible, and the Virgo
- 1:22:45supercluster is simply one bright spot among millions in a
- 1:22:49glowing web, indistinguishable, unremarkable, a predictable feature at a predictable location,
- 1:22:57in a pattern that repeats across the cosmos. Striking about
- 1:23:00this is not the size. The size stopped being graspable
- 1:23:04several sections ago. What is striking is the regularity. The
- 1:23:09universe at its largest scale is doing something almost mechanical.
- 1:23:13Matter fell into the gravitational well seeded by dark matter.
- 1:23:18It flowed along filaments, It pooled in clusters, It left
- 1:23:23voids behind. That process happened here, and it happened in
- 1:23:27ten million other locations spread across the observable universe, all
- 1:23:32following the same physics, all producing versions of the same structure.
- 1:23:37Our supercluster is not the result of some special set
- 1:23:40of conditions. It is what happens when you leave gravity
- 1:23:44running for thirteen billion years. It happened everywhere at the
- 1:23:49very largest scales. Our supercluster disappears into the average one
- 1:23:53node inner web, so vast and so regular that the
- 1:23:57universe doesn't particularly care whether it's there. The Virgo supercluster
- 1:24:02was not discovered by pointing a telescope at the sky
- 1:24:05and seeing a giant structure. There is no image of it,
- 1:24:10no photograph captures its shape. It was discovered the way
- 1:24:14most things at cosmic scales are discovered, through numbers, patterns,
- 1:24:19and a French astronomer in the nineteen fifties who notice
- 1:24:22something strange in the data. Gerard de Vaucouleur was measuring
- 1:24:27the velocities of galaxies. The tool for this is redshift.
- 1:24:32When a galaxy moves away from us, the light it
- 1:24:35emits gets stretched, the wavelengths grow longer on the spectrum,
- 1:24:40they shift toward the red end. The faster the galaxy
- 1:24:44is receding, the more the light stretches. Measure the stretch
- 1:24:48and you know the velocity. Combine the velocity with Hubble's law,
- 1:24:53the relationship between recession speed and distance, and you get
- 1:24:57how far away the galaxy is. Devocolurs was running these
- 1:25:02measurements on hundreds of galaxies across a wide region of sky,
- 1:25:06and he noticed something that wasn't supposed to be there.
- 1:25:10A large number of galaxies in one particular region of
- 1:25:13sky were sharing velocities that were too similar to be coincidental.
- 1:25:18They weren't just neighbours on the sky. There were neighbours
- 1:25:21in three dimensional space, moving together, dynamically connected. In nineteen
- 1:25:27fifty three, he called the structure the local super galaxy.
- 1:25:32A few years later he renamed it the Local Supercluster.
- 1:25:36The astronomy community, for the most part, was skeptical. Seeing
- 1:25:41a pattern in a data set is not the same
- 1:25:44as proving the pattern is real. The argument ran for
- 1:25:48three decades. Critics pointed out that Devocolur was selecting which
- 1:25:52galaxies to include, that the boundaries of the proposed structure
- 1:25:56were fuzzy, that the signal could be noise or bias
- 1:25:59in the Sun. This is how science is supposed to work.
- 1:26:03An observation gets challenged, the challenger demands better data. The
- 1:26:08data improves. In the late nineteen seventies and into the
- 1:26:12nineteen eighties, it finally did. The Center for Astrophysics Redshift surveys,
- 1:26:18built at Harvard was something different in scale from anything
- 1:26:21done before. Astronomers mapped thousands of galaxies in three dimensions,
- 1:26:26measuring redshifts systematically across large patches of sky, rather than
- 1:26:31cherry picking individual targets. The results were not subtle. The
- 1:26:36three D maps showed enormous structures, sheets of galaxies, filaments
- 1:26:42connecting clusters, vast empty voids between them. The supercluster was
- 1:26:47not a statistical artifact. It was a feature of the universe.
- 1:26:52The debate closed. What Devoculure had seen in the nineteen
- 1:26:56fifties was real, and it was larger than even he
- 1:26:59had described. Here is how the mapping actually works, because
- 1:27:04the process matters. You take a galaxy, you measure its spectrum,
- 1:27:10the rainbow of light it emits, and you find the
- 1:27:13characteristic fingerprint of hydrogen or calcium or other elements. Those
- 1:27:19fingerprints appear at known wavelengths in a laboratory. In the
- 1:27:23galaxy spectrum, those same fingerprints are shifted. You measure how
- 1:27:28far they shifted. That gives you the galaxy's recession velocity.
- 1:27:33You apply Hubble's law and convert velocity into distance. Now
- 1:27:38you have three numbers, two coordinates for the galaxy's position
- 1:27:43on the sky and one for how far away it is.
- 1:27:46Three numbers give you a point in three dimensional space.
- 1:27:50Do that for ten thousand galaxies, do it for a million,
- 1:27:54then clot the points the structure appears. The Sloan Digital
- 1:28:00Sky Survey pushed this to a scale that devoculurs could
- 1:28:04not have imagined. Launched in the year two thousand and
- 1:28:08running in phases ever since, it eventually measured redshifts for
- 1:28:13millions of galaxies across a substantial fraction of the visible sky.
- 1:28:17The maps it produced showed the cosmic web in extraordinary detail,
- 1:28:22filaments stretching hundreds of millions of light years, enormous voids,
- 1:28:27walls of galaxies billions of light years long. The Virgo
- 1:28:31supercluster appeared in those maps, not as something exceptional, but
- 1:28:36as one node among many in a much larger network.
- 1:28:39It was the Sloane data, combined with other surveys, that
- 1:28:43gave the Tully team in twenty fourteen, the raw material
- 1:28:47to define laniar KaiA. But the technique has a hard limit,
- 1:28:51and the limit is embarrassingly close to home. The Milky
- 1:28:54Way is a disc galaxy. We sit inside the disc
- 1:28:58roughly two thirds of the way out the center. When
- 1:29:01we look in the direction of the disc's plane, which
- 1:29:04is the bright band of the Milky Way visible in
- 1:29:06the night sky. We are looking through the densest concentration
- 1:29:10of stars, gas, and dust in the galaxy. This material
- 1:29:15absorbs light. Galaxies behind it are invisible or nearly so.
- 1:29:20Astronomers call this the zone of avoidance, which is a
- 1:29:23precise name for a frustrating problem. Roughly twenty percent of
- 1:29:28the sky is obscured by our own galaxy's disc Everything
- 1:29:32behind that curtain is either invisible to optical telescopes or
- 1:29:36severely degraded. Radio telescopes and X ray observatories can push
- 1:29:41through some of it, but significant regions remain mapped only
- 1:29:45poorly or not at all. The zone of avoidance falls
- 1:29:49squarely across a region of sky that includes the direction
- 1:29:52of the Great Attractor. This is not a coincidence of
- 1:29:55bad luck. The Greater Tractor sits roughly in the plane
- 1:29:59of the galaxy from our perspective, which is precisely where
- 1:30:02we can see the least. The gravitational anomaly was detected
- 1:30:06through its effects on the motions of galaxies around it
- 1:30:10before anyone could clearly see what was causing it. Decades
- 1:30:14of work with radio and near infrared surveys have partially
- 1:30:17lifted the curtain. The normal cluster and related structures have
- 1:30:21been identified, but the full picture of what lies behind
- 1:30:24the zone of avoidance and how much mass is hidden there,
- 1:30:28is still being assembled. What this means is that our
- 1:30:31map of the Virgo supercluster is not finished. Forty seven
- 1:30:36thousand cataloged galaxies is account of what we've been able
- 1:30:39to see, not a census of what is there. The
- 1:30:43structures hidden by the Milky Way's disc are real. They
- 1:30:47influence the motion of everything around them, but we cannot
- 1:30:51directly observe them from our current position, embedded as we
- 1:30:55are in the very galaxy doing the blocking parts of
- 1:30:59our our own supercluster remain hidden behind the disk of
- 1:31:03the Milky Way, which is a strange thing to have
- 1:31:06to say about something we live inside. Every human who
- 1:31:10has ever lived has spent their entire existence inside the
- 1:31:13Virgo supercluster, not metaphorically, not in some abstract cosmological sense,
- 1:31:21literally inside it, Embedded in a structure one hundred ten
- 1:31:25million light years across with no possibility of exit and
- 1:31:29no way to feel the walls. Every person who was
- 1:31:33ever born, lived and died did so inside this thing,
- 1:31:38every war ever fought, every city ever built, every quiet
- 1:31:44morning anyone ever sat through with a cup of coffee
- 1:31:47and nowhere pressing to be. All of it happened here
- 1:31:51inside the Virgo Supercluster, and almost none of those people
- 1:31:56had any idea. That is a strange fact to sit with.
- 1:32:00We have spent most of human history trying to understand
- 1:32:03where we are. We mapped continents, We charted coast lines.
- 1:32:08We tracked the movements of planets and stars, and worked
- 1:32:11out the geometry of the Solar System. We discovered that
- 1:32:15the Sun was a star, that the stars were distant suns,
- 1:32:19that the Milky Way was a galaxy among billions. Each
- 1:32:22expansion of the map was a shock. Each one reset
- 1:32:26our sense of how large the context was. And even now,
- 1:32:30with all of that knowledge accumulated, most people walk around
- 1:32:34with the working picture of the universe that stops somewhere
- 1:32:38around the Solar System. The supercluster barely registers. It does
- 1:32:43not feel like anything from inside. That is the deepest
- 1:32:47strangeness about living inside a structure this size. There is
- 1:32:51nothing to press against. When you are inside a room.
- 1:32:55You know you are inside a room because there are walls.
- 1:32:59When you you are inside a city, you know roughly
- 1:33:02where the city ends, because eventually the buildings thin out
- 1:33:06and the fields begin. The Virgo supercluster has no edge
- 1:33:10you can point to, no boundary you could cross and
- 1:33:14know you had crossed it. The density of galaxies simply
- 1:33:18decreases as you move outward, gradually over tens of millions
- 1:33:22of light years. You could travel in any direction for
- 1:33:26millions of years and never experience a threshold, never feel
- 1:33:30a change. The structure that contains everything we have ever
- 1:33:34known does not announce itself. Carl Sagan's pale blue dot
- 1:33:38image gave a generation of people a visceral sense of
- 1:33:42scale at one particular level, Earth photographed from four billion
- 1:33:47miles away, reduced to a speck of light suspended in
- 1:33:50a beam of sunlight. The image worked because it connected
- 1:33:54something visible to something almost too large to hold. But
- 1:33:58the pale blue dot is inside a solar system. The
- 1:34:02solar system is inside the Milky Way. The Milky Way
- 1:34:06is inside the local group. The local group is inside
- 1:34:09the Virgo supercluster. The Virgo supercluster is inside Lanakare. Each
- 1:34:15of those frames shrinks the dot further. Each one adds
- 1:34:19another layer of context that makes the blue speck smaller,
- 1:34:23more improbable, more isolated. By the time you reach the
- 1:34:27supercluster level, the dot is not just pale, It is
- 1:34:31essentially undetectable. It is a single atoman a building, and
- 1:34:36the building is on a continent, and the consonant is
- 1:34:39on a planet, and the planet is not the largest
- 1:34:42thing in the room. The question worth asking is what
- 1:34:46this actually does to anything. The scale is staggering. That
- 1:34:51part is easy to say. But does it change what
- 1:34:54happens on the dot? Does it reduce the weight of
- 1:34:58any particular moment A child being born, a species going extinct,
- 1:35:06a civilization collapsing or rising. Does any of that register
- 1:35:10differently once you know the supercluster is out there, enormous
- 1:35:15and silent, indifferent to all of it. The honest answer
- 1:35:19is probably no, and probably yes. The facts of human
- 1:35:23experience operate at human scales. Pain is pain at the
- 1:35:27same intensity, regardless of what is behind the night sky.
- 1:35:32The supercluster is not competing with any of that. It
- 1:35:36is simply the context the outermost known frame, and frames
- 1:35:40do not usually change what they contain. A painting is
- 1:35:44the same painting in a large room as in a
- 1:35:46small one. But something does shift when you genuinely try
- 1:35:50to hold the scale, not the numbers, because the numbers
- 1:35:53defeat you. Something else, the knowledge that this structure has
- 1:35:58been here for billions of years and will continue long
- 1:36:01after the Earth is gone. That everything we consider permanent,
- 1:36:05every mountain range, every ocean, every civilization we are capable
- 1:36:10of imagining, is temporary in a way that the Supercluster
- 1:36:13is not. We are not the reference point. We are
- 1:36:16the variable. The supercluster is the constant, at least on
- 1:36:21the time scales that matter to anything that has ever
- 1:36:24lived here. There is something almost clarifying about that. The
- 1:36:28supercluster does not need us to understand it to exist.
- 1:36:32It was assembling its filaments and drawing galaxies toward its
- 1:36:36center long before there were eyes to see any of it.
- 1:36:39The Virgo Cluster was pulling galaxies into itself before the
- 1:36:44Earth had cooled eighty seven, was consuming smaller galaxies, while
- 1:36:49single celled organisms were the most complex life this planet
- 1:36:52had managed to produce. The supercluster does not require witnesses.
- 1:36:58It simply is, and yet here we are inside it,
- 1:37:02trying to take its measure. We built the instruments, we
- 1:37:06developed the mathematics. We learned to read the red shift
- 1:37:09of light and turn it into a distance, turn that
- 1:37:13distance into a map, turn the map into a structure.
- 1:37:17We found the filaments, we named the clusters. We identified
- 1:37:21our own position within the supercluster and confirmed that we
- 1:37:25are falling toward its center at three hundred kilometers per second.
- 1:37:29That is not nothing. The structure may not require witnesses,
- 1:37:33but it has them, improbable ones. Sitting on a pale
- 1:37:37blue dot near the edge of the local group looking
- 1:37:41in the scale doesn't make the dot smaller in any
- 1:37:44way that matters to the things living on it, but
- 1:37:47it does change what it means to ask where home is.
- 1:37:50For all of the measurements and maps and redshift surveys,
- 1:37:54there is a long list of things astronomers genuinely do
- 1:37:57not know about the Virgo supercluster. Start with the great attractor.
- 1:38:02Something is pulling on us, pulling on the entire local group,
- 1:38:06pulling on the Virgo cluster itself, pulling on hundreds of
- 1:38:10thousands of galaxies across an enormous volume of space. Astronomers
- 1:38:15can measure the pull. They can see it in the
- 1:38:17peculiar velocities of galaxy streaming in a specific direction. What
- 1:38:22they cannot fully see is the thing doing the pulling.
- 1:38:26The normal cluster sits in roughly the right place, and
- 1:38:30for a while it seemed like the answer. Then better
- 1:38:33measurements suggested the normal cluster wasn't quite massive enough behind
- 1:38:38it partially obscured, something larger might lurk. The Shapleigh supercluster,
- 1:38:44roughly six hundred fifty million light years away, is one candidate,
- 1:38:49but even Shaply may not account for the full magnitude
- 1:38:52of the streaming motion. The honest answer right now is
- 1:38:56that nobody knows exactly what the Great Attractor is. And
- 1:39:00part of the reason nobody knows is that our own
- 1:39:03galaxy is in the way. The Milky Way's disc is
- 1:39:06thick with gas and dust. In certain directions on the sky.
- 1:39:10This material absorbs so much light that distant galaxies become
- 1:39:14invisible to optical telescopes. This region is called the zone
- 1:39:19of avoidance. It cuts a wide band across the sky,
- 1:39:23and it is not a minor inconvenience. It hides a
- 1:39:26significant portion of our cosmic neighborhood. The Greater Tractor sits
- 1:39:31almost precisely behind it. Radio telescopes and X ray observatories
- 1:39:36can peer through the disc somewhat, and researchers have used
- 1:39:40these tools to identify galaxy clusters hiding in the zone,
- 1:39:44but the picture remains incomplete. There are structures in our
- 1:39:48own supercluster that we have not cataloged because we cannot
- 1:39:52see them clearly. We live inside this thing, and pieces
- 1:39:56of it are still hidden from us by our own
- 1:39:58front yard. They seven thousand galaxy figure for the supercluster's
- 1:40:02total population is a catalog number. It reflects what has
- 1:40:07been found and measured and recorded. It is not a census.
- 1:40:11Galaxies come in a vast range of sizes, and the
- 1:40:14faint dwarf galaxies at the small end of that range
- 1:40:17are genuinely difficult to detect at supercluster distances. Studies of
- 1:40:21the local group alone keep revising the count upward as
- 1:40:25new instruments pick out fainter objects that previous surveys missed.
- 1:40:29The same thing is almost certainly true across the full
- 1:40:32extent of the Virgo supercluster. The true number of galaxies
- 1:40:37inside it is larger than forty seven thousand. How much
- 1:40:41larger is an open question. Some estimates push the real
- 1:40:44count considerably higher once you account for everything too dim
- 1:40:48to have been cataloged. Yet then there is the boundary problem.
- 1:40:52Where does the Virgo supercluster actually end. The twenty fourteen
- 1:40:57lanier Kea paper drew boundaries by mapping the flow patterns
- 1:41:00of galaxies, the idea being that any galaxy whose motion
- 1:41:04is ultimately directed toward the same gravitational basin belongs to
- 1:41:09the same supercluster. It was a genuinely clever approach, and
- 1:41:13it produced a striking result, but not everyone agrees with
- 1:41:17the methodology. Some astronomers argue that defining a supercluster by
- 1:41:22flow convergence rather than by gravitational binding, creates boundaries that
- 1:41:27are somewhat arbitrary, dependent on the precision of velocity measurements
- 1:41:32and the assumptions built into the flow models. The edges
- 1:41:36of lanie KaiA, and therefore the edges of the Virgo
- 1:41:39supercluster within it, are not hard lines. They are regions
- 1:41:43of lania KaiA, and therefore the edges of the Virgo
- 1:41:47supercluster within it are not hard lines. They are regions
- 1:41:51of f uncertainty, where the answer changes depending on which
- 1:41:55team's method you trust. Dark matter is perhaps the deepest
- 1:41:59open question. We know it is there. The gravitational evidence
- 1:42:04is consistent and overwhelming, But knowing something exists and understanding
- 1:42:09how it behaves in detail are different things. The filamentary
- 1:42:13structure of the Virgo supercluster, the sheets and strands of
- 1:42:17galaxies connecting the clusters, is thought to trace the skeleton
- 1:42:21of the underlying dark matter distribution. The galaxies are, in
- 1:42:25a sense just the lit portions of a much larger
- 1:42:29invisible web, but that web has never been directly observed.
- 1:42:33It is inferred. The models that describe how dark matter
- 1:42:37clumps and flows and shapes the cosmic web are sophisticated,
- 1:42:41and they match the observations well. They are still models.
- 1:42:45The specific three dimensional arrangement of dark matter throughout the
- 1:42:49Virgo supercluster is not something anyone has mapped. It is
- 1:42:54something people have calculated. The future of the supercluster is
- 1:42:58similarly uncertain in its details. The broad picture dark energy
- 1:43:03eventually pulling apart the looser outer regions while the tightly
- 1:43:06bound inner clusters hold together depends on the precise value
- 1:43:10of the cosmological constant, the number that describes how fast
- 1:43:15the universe's expansion is accelerating. That number has been measured,
- 1:43:20it has also been argued over for decades, and attension
- 1:43:23in the measurements remains unresolved. Different methods of measuring the
- 1:43:27expansion rate produce slightly different answers, and astronomers have not
- 1:43:32agreed on why. Until that tension is resolved, Precise predictions
- 1:43:37about when and how structures at supercluster scales begin to
- 1:43:40dissolve are difficult to make with confidence. The direction is clear,
- 1:43:46the timeline is not. What makes all of this strange
- 1:43:49is that the Virgo supercluster is our home. This is
- 1:43:53not some distant, exotic object at the edge of the
- 1:43:56observable universe. It is the structure. We are embedded in,
- 1:44:00the thing that contains everything we have ever called a neighborhood,
- 1:44:04and we are still filling in the map. The Greater
- 1:44:07Tractor remains partly concealed. The galaxy count is provisional, the
- 1:44:13boundaries are contested, The dark matter skeleton is inferred but unseen.
- 1:44:19The future depends on a number still being argued over.
- 1:44:23For something this close, this fundamental to our cosmic address.
- 1:44:27The list of uncertainties is almost too long to take seriously,
- 1:44:32and yet there it is. Every time astronomers have thought
- 1:44:35they had the largest structure nailed down. The next generation
- 1:44:39of surveys has handed them some inmed bigger, and there
- 1:44:43is no particular reason to think that pattern has stopped.
- 1:44:47After all of that, the number is still one hundred
- 1:44:50ten million light years, and it still does not mean anything.
- 1:44:54Your brain can actually feel. Walk through every comparison, every analogy,
- 1:45:00every carefully constructed scale model, and when you arrive at
- 1:45:03the end, the number sits there, unchanged, unmoved, a grain
- 1:45:08of sand stretched across several kilometers light that has been
- 1:45:13traveling since before complex animals existed and still has not
- 1:45:17crossed the whole thing. These images land for a moment,
- 1:45:21then they slip. The brain accepts them as facts and
- 1:45:24refuses them as feelings. That is not a failure of attention.
- 1:45:29That is just the honest limit of what human intuition
- 1:45:32was built to do. But something else is true. You
- 1:45:36now know things about where you are that most people
- 1:45:38who have ever lived did not know. The local group
- 1:45:42ten million light years of bound galaxies is still just
- 1:45:46a small corner of this structure, the Virgo cluster one thousand,
- 1:45:50three hundred to two thousand galaxies packed into the gravitational
- 1:45:54heart of the supercluster sits roughly fifty five million light
- 1:45:58years away, and it is on you right now, not metaphorically.
- 1:46:03The Milky Way is falling toward it at around three
- 1:46:06hundred kilometers per second. Every second the gap closes by
- 1:46:10three hundred kilometers. You cannot feel it. Nothing in your
- 1:46:14life changes because of it, and yet it is happening
- 1:46:17constantly in the background of everything. M eighty seven is
- 1:46:21out there, twelve trillion stars organized around a black hole.
- 1:46:26We actually photographed. The image exists. The orange ring is real.
- 1:46:32That black hole anchors the dominant galaxy in the dominant
- 1:46:35cluster of the structure you live inside. And the filaments
- 1:46:39connecting everything, those long invisible threads of dark matter with
- 1:46:43galaxies strung along them like lights, those are real too,
- 1:46:48not visible, not something you can point to from a backyard,
- 1:46:52but real, structurally real, the actual skeleton of your cosmic address.
- 1:46:58Here is the strange part. Knowing all of this does
- 1:47:01not make the sky look crowded. It still looks exactly
- 1:47:05the same, the same quiet scatter of points in the dark.
- 1:47:09Oryon still has his shoulder, The Virgo constellation still sits
- 1:47:14in the spring sky, unremarkable to anyone not looking for it.
- 1:47:19Somewhere behind those faint stars fifty five million light years back,
- 1:47:23the Virgo cluster churns enormous and indifferent. You are aimed
- 1:47:29at it, moving toward it, part of a structure that
- 1:47:33is simultaneously being assembled by gravity and pulled apart by
- 1:47:37dark energy, two forces running in opposite directions, across scales
- 1:47:42too large for any single lifetime to register, And Lanikaea
- 1:47:47is above all of it. The structure that swallowed the
- 1:47:50supercluster hole five hundred and twenty million light years. Our
- 1:47:55supercluster is one tendril of it, one lobe reaching outward
- 1:47:59from a center we cannot easily see because the Milky
- 1:48:03Way's own disc is in the way. The Greater Tractor
- 1:48:06sits somewhere in that direction, massive and partially hidden, tugging
- 1:48:11on everything around it, including us. Some of those questions
- 1:48:15are still open, Some of the map is still blank.
- 1:48:19The zone of avoidance is a genuine gap in our knowledge,
- 1:48:22hidden behind the plane of our own galaxy. This structure
- 1:48:26is temporary, not on any timescale that matters to a
- 1:48:30human life, not on any timescale that matters to human civilization,
- 1:48:35but on the timescale of the universe, the supercluster is
- 1:48:39a passing arrangement. Dark energy is winning at this scale.
- 1:48:43The outer galaxies will eventually drift away. What looks like
- 1:48:47a coherent structure today is something the universe will disassemble
- 1:48:52over the next tens of billions of years. But one
- 1:48:55hundred ten million light years will become a memory in
- 1:48:58the geometry of an older colts. The number never got smaller.
- 1:49:02It was never going to. But the structure behind it
- 1:49:06is real, and our position inside it is real, and
- 1:49:10the motion is real, and the dark matter holding it
- 1:49:13together is real. The sky looks the same as it
- 1:49:17always did. The supercluster keeps doing what it has been
- 1:49:20doing since before the Earth existed, slowly assembling itself, slowly
- 1:49:26being pulled apart, enormous and silent and indifferent, And we
- 1:49:31are inside it, looking out