Latest / Boring Science / LANIAKEA SUPERCLUSTER_ The Milky Way Is Just a Tiny Part of This
Transcript
- 0:00Speaker 1: Most people can tell you their street address, their city,
- 0:04their country, and if they are paying attention in school,
- 0:08maybe even the name of the galaxy they live in.
- 0:11But ask them to go one level higher, one step
- 0:15further out, and almost everyone goes quiet. There is a
- 0:20structure above the galaxy. There is a structure above the
- 0:24galaxy cluster. There is an address most people have never
- 0:28been given, and it belongs to a place so enormous
- 0:32that the number of galaxies inside it runs to roughly
- 0:36one hundred thousand. We live inside it right now. Most
- 0:41people have never heard its name. That silence matters. It
- 0:46is not a gap in trivia. It is a gap
- 0:48in something more basic, the question of where exactly you are.
- 0:55Humans have spent thousands of years getting better at answering
- 0:58that question. Apped the continents, we track the planets. We
- 1:03measured the distance to the Sun, to nearby stars, to
- 1:07the edge of our own galaxy. Every generation pushed the
- 1:12answer a little further out, and then for a long
- 1:15stretch the answer stalled. The galaxy was as far as
- 1:20most people got, and the Milky Way became the edge
- 1:23of the mental map beyond it. In this informal accounting
- 1:28was just space undifferentiated, unmapped vast. The truth is stranger
- 1:41and more structured than that. The universe at its largest
- 1:45scales is not a smooth, even fog of galaxies scattered
- 1:49randomly in every direction. It has bones, It has architecture.
- 1:55Galaxies cluster together, Clusters gather into super clusters. Superclusters are
- 2:02themselves embedded in a web of filaments and voids, stretching
- 2:06across hundreds of millions of light years. This structure exists,
- 2:12whether or not we know about it, and we are
- 2:14inside it. The question was never whether there was a
- 2:18larger address. The question was whether anyone would ever figure
- 2:24out what it was. In twenty fourteen, a team of
- 2:29astronomers did. What they published that year was not just
- 2:34a new measurement or a refined catalog. It was a
- 2:38map of something that had never been mapped before, the
- 2:42full supercluster that contains the Milky Way, defined for the
- 2:47first time with a clear boundary, a coherent shape, and
- 2:51a name. The structure stretches five hundred twenty million light
- 2:56years across. Its total mass runs to something like a
- 3:01hundred quadrillion suns. It holds roughly one hundred thousand large
- 3:06galaxies inside it, all of them flowing slowly and gravitationally
- 3:12toward a common center, and almost nobody outside of astronomy
- 3:17has heard of it. The name comes from Hawaiian. The
- 3:21team behind the discovery was based at the University of Hawaii,
- 3:26and when the time came to name the structure, they
- 3:29consulted with Hawaiian language experts rather than reaching for the
- 3:34usual Latin or Greek. The word they settled on is
- 3:38lania kia. Lani means heaven or sky, Akia means spacious, open, immeasurable.
- 3:48Together the phrase means something close to immense heaven. There
- 3:52is something right about that. Polynesian navigators once crossed the
- 3:56open Pacific with no instruments and no landmarks, reading the
- 4:00sky to find where they were in the world. The
- 4:04name given to our supercluster reaches back to those same navigators,
- 4:08and it carries that same orientation looking up to understand
- 4:13your place. Most people have a cosmic address they have
- 4:17never been told street, city, country, planet, solar system, galaxy, galaxy, cluster, supercluster.
- 4:27That last entry is the missing one. That is the
- 4:31level where the address has until recently been blank. For decades,
- 4:37astronomers thought the Virgo supercluster was the best answer, a
- 4:41structure about one hundred million light years across that the
- 4:45Milky Way sat on the edge of. But that picture
- 4:49was incomplete. The Virgo supercluster turned out to be a
- 4:54small piece of something much larger. What replaced it is deeper, wider, stranger,
- 5:02and harder to picture. It took a new way of
- 5:05thinking about the problem entirely, not just pointing telescopes, but
- 5:10rethinking what a supercluster even is before anyone could see
- 5:15it clearly. That discovery, how it was made, what it
- 5:20revealed about the structure we are embedded in, and what
- 5:24it means for the question of where you are. That
- 5:28is what the rest of this is about. The name
- 5:32is Lania Kia, and understanding what it is changes everything
- 5:37about how you think about where you are. For decades,
- 5:42if you asked an astronomer where the Milky Way sat
- 5:46in the largest known structure, the answer was the Virgo supercluster.
- 5:53That was the official answer. That was what the textbook said,
- 5:59and for a long time it felt like enough. To
- 6:03understand why that answer seemed satisfying, you have to walk
- 6:06through the hierarchy that astronomers had assembled, piece by piece
- 6:11over the twentieth century. Start at the bottom Earth orbits
- 6:16the Sun. The Sun is one star among several hundred
- 6:21billion in the Milky Way. The Milky Way, a barred
- 6:26spiral galaxy roughly one hundred thousand light years across, belongs
- 6:31to a small cluster of galaxies called the Local Group.
- 6:36The Local Group contains around eighty galaxies in total, most
- 6:41of them small and dim, gravitationally bound to each other
- 6:45and to the two dominant members, the Milky Way and
- 6:49the Andromeda galaxy. That cluster spans roughly ten million light years.
- 6:56Beyond the Local Group, things get larger much lower. The
- 7:01Virgo Supercluster was the next rung on that ladder. It
- 7:05stretched roughly one hundred million light years across an enormous
- 7:10region of space, containing thousands of galaxies organized into smaller
- 7:15clusters and groups, all loosely associated around a gravitational center.
- 7:21At that center sat the Virgo Cluster, itself, one of
- 7:25the nearest large galaxy clusters to us, holding several thousand
- 7:30galaxies packed into a region roughly eight million light years wide.
- 7:37The Local Group sat on the outer edge of this structure,
- 7:41a minor outpost well away from the dense central regions.
- 7:46That was the address, That was the picture. The man
- 7:51most responsible for assembling it was a French American astronomer
- 7:55named Gerard de Vaucouleur. Working in the nineteen fifteen es,
- 8:00Devoculur noticed something that had been hiding in plain sight.
- 8:05When he plotted the positions of nearby galaxies across the sky,
- 8:09they weren't scattered randomly. They clustered preferentially along a flattened plane,
- 8:16A great disk of galaxies tilted roughly six degrees relative
- 8:20to the celestial equator. He called this the local supercluster.
- 8:26Other astronomers were skeptical. The concept of superclusters enormous structures
- 8:33containing multiple clusters of galaxies, was not universally accepted at
- 8:38the time. Some researchers argued that what Devoculur was seeing
- 8:44was just a statistical accident, a coincidence in the distribution
- 8:48of nearby galaxies, rather than a genuine physical structure. The
- 8:54debate went on for decades. Gradually, as observations improved and
- 9:00galaxy catalogs grew larger, the reality of the local supercluster
- 9:05became harder to dismiss. By the nineteen eighties, most astronomers
- 9:10had accepted that Devoculur had been right. The Virgo Supercluster
- 9:15was real, and once it was accepted, the picture felt
- 9:19remarkably complete. You had a clean hierarchy. Planets orbited stars,
- 9:25Stars gathered in galaxies, Galaxies gathered in clusters, clusters gathered
- 9:31in superclusters. The universe was organized, nested, logical. The Virgo
- 9:38Supercluster was the top of that nesting, the largest box
- 9:42that contained our box, and it had a sensible size
- 9:46about one hundred million light years and a sensible shape.
- 9:51It was centered on a visible, well studied cluster of galaxies.
- 9:56You could point to it on a map. Cosmologic speaking,
- 10:01the address problem seemed solved. Then the data started behaving strangely.
- 10:07The universe is expanding. Edwin Hubble established this in nineteen
- 10:13twenty nine, and by the second half of the twentieth
- 10:17century it was one of the most thoroughly confirmed facts
- 10:21in all of science. Galaxies are receding from us and
- 10:26from each other at speeds proportional to their distances. The
- 10:31further away a galaxy is, the faster it appears to
- 10:35move away. This is not galaxies moving through space so
- 10:40much as space itself stretching, carrying galaxies along with it.
- 10:45If you know a galaxy's recession speed, you can calculate
- 10:49its distance. This relationship, called the Hubble flow, forms the
- 10:54backbone of how astronomers measure the large scale universe. The
- 10:58problem was that real galaxies didn't follow the Hubble flow exactly.
- 11:04When astronomers measured individual galaxy velocities carefully and compared them
- 11:09to what pure Hubble expansion predicted, there were systematic leftovers.
- 11:15Galaxies were moving at speeds and in directions that pure
- 11:19expansion could not account for. These deviations had a name
- 11:24peculiar velocities, and in small amounts, peculiar velocities were expected.
- 11:31Local gravity, the pull of a nearby galaxy cluster, the
- 11:35tug of a neighboring group would naturally push galaxies slightly
- 11:40off the smooth expansion baseline. That was normal. That was understood.
- 11:46What was not understood was the scale of what astronomers
- 11:50were beginning to see. By the nineteen seventies and into
- 11:55the nineteen eighties, galaxy surveys were growing large enough that
- 12:00a troubling pattern was becoming visible. Galaxies across an enormous
- 12:05volume of space, far larger than any individual cluster, far
- 12:11larger even than the Virgo supercluster, seemed to be drifting
- 12:15coherently in roughly the same direction. Not just a handful
- 12:20of galaxies, not just one cluster. Thousands of galaxies spread
- 12:25across hundreds of millions of light years were showing a
- 12:29systematic motion that pointed toward a particular region of the sky,
- 12:35somewhere in the direction of the constellations Centaurus and Norma.
- 12:41The motion was subtle, but it was measurable, and it
- 12:44was consistent. Something was pulling on a scale the existing
- 12:49maps see would not explain the Virgo supercluster alone, could
- 12:54not account for it. The gravitational influence of the Virgo
- 12:59cluster and d its surrounding structure was well understood, and yes,
- 13:04it tugged on the local group. But this new signal
- 13:08was different, larger, deeper, coming from a direction and on
- 13:13a scale that pointed to something much more massive, sitting
- 13:17further out, something that had never been properly identified or mapped.
- 13:23The clean hierarchy began to look incomplete. The top rung
- 13:28of the ladder seemed to be missing something, or rather,
- 13:32it seemed to be sitting on top of something larger
- 13:35that nobody had noticed. For a generation of astronomers, this
- 13:39was the uncomfortable feeling at the edge of the known map.
- 13:43The Virgo supercluster was real, The hierarchy was real, but
- 13:49the hierarchy wasn't the whole story. The galaxies weren't just
- 13:53expanding outward uniformly. They were being pulled subtly, but unmistakably
- 13:59towards something nobody had fully mapped. In the nineteen seventies,
- 14:04when astronomers first produced detailed maps of the cosmic microwave
- 14:08background radiation, something immediately looked wrong. The CMB is the
- 14:15oldest light in the universe, A faint glow left over
- 14:19from roughly three hundred eighty thousand years after the Big Bang,
- 14:24spread almost perfectly uniformly across the sky. Almost When scientists
- 14:31looked carefully at their new maps, they noticed that one
- 14:35side of the sky was slightly warmer than the other.
- 14:38Not dramatically, not in a way that leapt off the page.
- 14:44But the asymmetry was real, and it was consistent, and
- 14:48it meant something specific. The Milky Way was moving, not
- 14:53just spinning in place, not just orbiting the center of
- 14:56our galaxy. The entire local group was being carried in
- 15:01a direction at a speed of roughly six hundred kilometers
- 15:05per second toward a ragye on of the sky nobody
- 15:09had properly investigated. Six hundred kilometers per second is not
- 15:13a small number that is fast enough to cross the
- 15:17continental United States in under ten seconds. At that speed,
- 15:22something is doing the pulling. The simple model of cosmic
- 15:25expansion galaxies moving apart uniformly in all directions, like raisins
- 15:32in a rising loaf of bread, predicted no such drift.
- 15:37Everything should be moving outward from everything else, no preferred direction,
- 15:43no net flow toward any particular point. What the CMB
- 15:48maps were showing was a deviation from that picture. The
- 15:52local group had what astronomers call a peculiar velocity, meaning
- 15:58a velocity that cannot be counted for by the ordinary
- 16:02expansion of space alone. Something gravitational was adding an extra tug.
- 16:08Peculiar velocities are the fingerprints of structure. In a perfectly
- 16:13smooth universe, galaxies would have no peculiar velocities at all.
- 16:18They would simply ride the expansion of space outward evenly
- 16:23in all directions. But the universe is not smooth. Matter
- 16:28is clumped into galaxies, clusters filaments. Wherever mass concentrates, it
- 16:35pulls neighboring objects toward it, giving those objects a velocity
- 16:40component that points toward the mass rather than simply away
- 16:44from everything else. Measure enough peculiar velocities across a large
- 16:50enough volume of space, and you can reconstruct where the
- 16:53hidden mass is sitting. The CMB dipole was the first
- 16:58crude map of a percure peculiar velocity on the largest
- 17:02scale anyone had yet considered. It was telling astronomers that
- 17:07a significant mass concentration xi stead somewhere in the direction
- 17:12the local group was streaming toward, and that this concentration
- 17:16was large enough to accelerate thousands of galaxies simultaneously. Through
- 17:21the late nineteen seventies and into the nineteen eighties, several
- 17:26independent teams began measuring peculiar velocities for galaxies beyond the
- 17:31local group. What they found was alarming in its consistency.
- 17:37Galaxies in our general neighborhood were not just drifting outward
- 17:41with the hubble flow. They were streaming. Hundreds of galaxies
- 17:47spread across enormous distances were all showing a common component
- 17:52of motion pointed in roughly the same direction. This was
- 17:57not noise. This was a coherent bulk flow, a river
- 18:01of galaxies being carried together towards something. Astronomers called this
- 18:07the Great Attractor, and the name was chosen carefully. Whatever
- 18:12was out there was not a single object. It was
- 18:15a region, a concentration of matter so vast and so
- 18:20massive that its gravity was reaching hundreds of millions of
- 18:26light years in every direction and bending the trajectories of
- 18:30everything it touched. The nineteen eighty six paper that gave
- 18:34the Great Attractor its name came from a group of
- 18:37seven astronomers who would become known informally as the Seven Samurai.
- 18:43Donald Lynden Bell, Sandra Faber, and five colleagues had spent
- 18:48years building a catalog of elliptical galaxies with measured distances
- 18:54and velocities. When they analyzed the streaming motions in their data,
- 19:00they found that the bulk flow pointed toward a specific
- 19:03region of the sky, the direction of the constellation's normal
- 19:08and centaurous crux, roughly in the southern sky. Their best
- 19:14estimate placed the source of the gravitational pull at somewhere
- 19:18between one hundred fifty and two hundred fifty million light
- 19:23years away. The mass required to produce the observed streaming
- 19:28was staggering ten million billion solar masses that is a
- 19:35ten followed by fifteen zeros that is, tea and quadrillion
- 19:41suns concentrated into one region of space, exerting gravitational influence
- 19:47across a volume that makes our entire local group look
- 19:51like a single grain of sand on a beach. Stop
- 19:54and hold that number for a moment. Ten million billion
- 19:58solar masses. Our sun is already so large that a
- 20:02million earths would fit inside it. The Milky Way contained
- 20:07somewhere around two hundred to four hundred billion stars. The
- 20:12entire mass of everything in the local group, every star,
- 20:16every galaxy, all the dark matter, all the gas, is
- 20:21perhaps a few trillion solar masses. The Greater Tractor was
- 20:26something altogether different. It was not a cluster of galaxies
- 20:30in the ordinary sense. It was a concentration of mass
- 20:35that dwarfed entire superclusters, pulling the Milky Way and everything
- 20:40around it toward it at hundreds of kilometers per second,
- 20:45And it had apparently been doing this for billions of years,
- 20:49And yet for most of the nineteen eighties, nobody could
- 20:53see it properly. This is where the story gets genuinely strange.
- 20:58The Greater Tractor was not a subtle signal buried in
- 21:01noisy data. Its gravitational effect was measurable across hundreds of
- 21:07millions of light years. Thousands of galaxies were streaming toward it.
- 21:13The CMB dipole was pointing at it. And yet when
- 21:17astronomers turned their telescopes toward the region of Norma and
- 21:20Centaurus and tried to actually observe this gravitational engine directly,
- 21:26they ran into a wall, not a metaphorical wall, something
- 21:32physical sitting between us and the attractor, blocking the view
- 21:37the Milky Way itself. Our galaxy is a disc. We
- 21:42are embedded inside that disc, roughly two thirds of the
- 21:46way out from the center. When we look outward in
- 21:50the plane of the disc, toward what we see as
- 21:53the band of the Milky Way stretching across the night sky,
- 21:58we are looking through the maximum concentration of our own galaxy, stars, gas,
- 22:04and dust. There are hundreds of billions of stars between
- 22:09us and the edge of the galactic disk in that direction,
- 22:13along with enormous clouds of molecular gas and thick lanes
- 22:17of interstellar dust that absorb and scatter visible light almost completely.
- 22:24Anything sitting behind that disc invisible wavelengths is essentially invisible.
- 22:31Astronomers have a name for this region of the sky.
- 22:34They call it the zone of avoidance. The zone of
- 22:38avoidance covers a significant band across the entire sky. It
- 22:42is not a narrow slit. In some directions. It extends
- 22:46twenty to thirty degrees above and below the galactic plane.
- 22:51A substantial fraction of the entire sky, perhaps twenty percent
- 22:55or more of the observable universe as seen from Earth,
- 22:59is abs skewed or seriously compromised in optical wavelengths by
- 23:04our own galaxy's disc. This would be merely inconvenient if
- 23:08the objects behind it were distributed randomly, but they are not.
- 23:14The greater tractor sits squarely in this zone. The densest,
- 23:19most consequential structure in our corner of the universe happens
- 23:24to lie almost perfectly behind the thickest part of the
- 23:27galactic plane, as seen from our position within the Milky Way.
- 23:33You could not design a more effective obstacle if you tried.
- 23:37Astronomers throughout the nineteen eighties and into the nineteen nineties
- 23:42pushed hard against this limitation. They turned to radio telescopes,
- 23:47which can detect the twenty one centimeter emission line of
- 23:51neutral hydrogen through almost any amount of dust. They used
- 23:57X ray observatories, which can detect the hot gas in
- 24:00galaxy clusters even through substantial obscuration. They developed infrared surveys
- 24:07that could cut through dust far more effectively than optical light. Slowly, painfully,
- 24:15the picture behind the zone of avoidance began to clarify.
- 24:20The normal cluster emerged from the murk, a rich cluster
- 24:24of galaxies sitting right at the heart of the attractor region,
- 24:28dense with thousands of galaxies threaded through with hot gas.
- 24:34It was not the totality of the Great Attractor, but
- 24:38it was a confirmation that something mass sieve was genuinely there.
- 24:43The gravitational signal was real, the streaming was real, The
- 24:48thing causing it was real. What was almost absurd about
- 24:51the situation was the irony embedded in it. Here was
- 24:56the most gravitationally dominant structure within hundreds of millions of
- 25:01light years of the Milky Way, something pulling our entire
- 25:05galactic neighborhood toward it at enormous speed, something that had
- 25:10been shaping the large scale motion of galaxies in our
- 25:14region for billions of years. And the reason we could
- 25:18barely study it was not a technological limitation or a
- 25:22fundamental physical barrier. It was us. The very galaxy we
- 25:29live in was blocking our view of the gravitational engine
- 25:32at the center of our cosmic home. Imagine trying to
- 25:36map a city while standing in the middle of a
- 25:38thick forest that circles the entire downtown core. You can
- 25:42see what is directly around you. You can see patches
- 25:46of sky above, but the buildings at the center, the streets,
- 25:52the whole layout of the place you are trying to understand,
- 25:56all of it is blocked by the trees. That is
- 26:00roughly the situation astronomer's face when they try to observe
- 26:04the region of the universe sitting behind the plane of
- 26:07the Milky Way. The forest is our own galaxy, and
- 26:12it does not move. The problem has a name. Astronomers
- 26:17call it the zone of avoidance, which sounds like something
- 26:20you would find on a nautical chart warning ships away
- 26:24from shallow water. The name fits. It is a band
- 26:29running all the way around the sky, tracing the galactic plane,
- 26:34where the Milky Way's own stars, gas and dust absorb
- 26:39and scatter the light coming from anything beyond. In optical wavelengths,
- 26:45the kind of light human eyes can see. This band
- 26:49is essentially opaque. Galaxies that sit behind it are not dimmed,
- 26:54they are gone. Their light never makes it through. The
- 26:59zone of avoidance covers roughly twenty percent of the entire
- 27:03sky that is not a narrow strip you can work around.
- 27:08That is a fifth of everything running in a continuous
- 27:12band around the full equator of our celestial sphere. What
- 27:17makes this strange is that the obscuring material is not
- 27:21particularly thick by cosmic standards. The dust and gas clouds
- 27:26responsible for the blockage are relatively diffuse, but they are
- 27:31spread across tens of thousands of light years of galactic disk,
- 27:36and when you stack that much material between yourself and
- 27:40a distant galaxy, even thin stuff adds up. The total
- 27:45extinction in some parts of the galactic plane is enormous.
- 27:49Light from distant objects gets absorbed, scattered, and reddened into
- 27:54invisibility long before it reaches a telescope on Earth. Are
- 28:00not helpless. They found workarounds, and the workarounds are clever.
- 28:06Infrared light has longer wavelengths than visible light, and longer
- 28:12wavelengths cut through dust far more effectively. An infrared telescope
- 28:18can detect galaxies behind the galactic plane that are completely
- 28:23invisible to an optical instrument. X ray observations help as well.
- 28:30High energy X rays punch through interstellar dust with relatively
- 28:34little scattering, which is how some of the galaxy clusters
- 28:39lurking behind the zone of avoidance were first identified. Radio
- 28:44wavelengths work too. The twenty one centimeter emission line from
- 28:48neutral hydrogen passes straight through the galactic dust without any
- 28:53significant absorption, which means radio surveys can map hydrogen in
- 28:58distant galaxies even when those galaxies are sitting directly behind
- 29:03the Milky Way's thickest regions. These tools opened up parts
- 29:07of the zone of avoidance that had been completely dark before.
- 29:11The normal Cluster, one of the major structures near the
- 29:15Greater Tractor, was partly mapped through these techniques. Several previously
- 29:21unknown galaxy clusters were found hiding in the obscured region
- 29:26during the nineteen nineties and two thousands, when systematic infrared
- 29:31and radio surveys swept across the galactic plane for the
- 29:35first time. Each discovery reminded astronomers how much had been
- 29:41missed simply because of where they happened to be sitting.
- 29:45But here is the thing. Even with infrared, X ray
- 29:49and radio data combined, the zone of avoidance remains the
- 29:54worst characterized region of the nearby universe. The tools that
- 29:59cut through dust come with their own limitations. Infrared surveys
- 30:04still struggle with the bright emission from our own galaxy stars,
- 30:09which floods the detectors and makes faint background sources hard
- 30:14to extract. Radio surveys measure hydrogen, but mis galaxies with
- 30:19little neutral gas. X ray observations pick up hot cluster gas,
- 30:25but not the full picture of galaxy distribution. No single
- 30:29alternative method gives you what optical astronomy gives you. Everywhere else,
- 30:35the coverage is patchier, the catalogs are less complete, the
- 30:40distance measurements are harder to make and less reliable. When
- 30:44Brent Tully's team built the cosmic flows to catalog, the
- 30:48one that would eventually define Laniakia, the data thinned out
- 30:53and degraded precisely in the directions behind the galactic plane.
- 30:58The map had a whole in it, and the whole
- 31:01sat right over one of the most gravitationally significant regions
- 31:05in the local universe. There is a particular irony in
- 31:09all of this that is hard to ignore. The Milky
- 31:13Way is not a distant obstacle. It is not some
- 31:16intervening object that happens to lie in an unfortunate direction.
- 31:22It is the galaxy we live inside. The stars blocking
- 31:26our view of the Great Attractor are the same stars
- 31:29that make up the bright band of the Milky Way
- 31:33that humans have looked up at for all of recorded history.
- 31:38The dust blocking the light from thousands of background galaxies
- 31:42is the same dust that fills the spiral arms of
- 31:45our own home. We are embedded so deeply inside this
- 31:50structure that it wraps completely around us, and because of that,
- 31:55there is a ring around our entire sky where the
- 31:59universe versus functionally hidden. The very thing that makes us
- 32:04astronomers having a galaxy to stand in is the same
- 32:08day nung that blinds us to a fifth of what
- 32:12surrounds us. For years, the Greater Tractor sat squarely behind
- 32:17this veil, its true nature hidden behind the very structure
- 32:22that contains every star you can see on a clear night.
- 32:26The breakthrough that produced Laniaka was not a new telescope
- 32:30or a new piece of hardware. It was a new
- 32:33idea about what astronomers should be measuring. For most of
- 32:37the twentieth century, when astronomers tried to map the large
- 32:41scale structure of the universe, they did it by counting.
- 32:45They would survey a region of sky, catalog the galaxies
- 32:49they found, and draw boundaries around the densest concentrations. Where
- 32:55galaxies clumped together, that was a cluster. Where clusters grouped together,
- 33:01that was a supercluster. It was a logical approach. It
- 33:06was also, it turned out, incomplete. Density maps can tell
- 33:11you where matter piled up, but they cannot tell you
- 33:15what belongs together gravitationally. A city map that only shows
- 33:20population density misses the fact that commuters from far flung
- 33:25suburbs are functionally part of the same metropolitan system, even
- 33:30if they live in a sparse neighbourhood at the edge.
- 33:33Brent Tully understood this problem. Tully is an astronomer at
- 33:38the University of Hawaii's Institute for Astronomy, and by twenty
- 33:43fourteen he had spent decades building the most precise catalogs
- 33:48of galaxy distances and velocities that the field had ever produced.
- 33:53He had already made his name decades earlier, co developing
- 33:57the Tullyfisher relation, unique that links a spiral galaxy's rotation
- 34:03speed to its true brightness and allows astronomers to infer
- 34:07distances from observations alone. That earlier work was groundbreaking, but
- 34:14by the two thousands, Tully was working on something with
- 34:18even larger implications. He was thinking about what the motions
- 34:23of galaxies could reveal, not just their positions. Here is
- 34:27the key concept. When astronomers measure the velocity of a
- 34:31distant galaxy, they typically get two signals mixed together. One
- 34:37is the velocity from the expansion of the universe, the
- 34:41background hum of space itself stretching, which makes every galaxy
- 34:46appear to be moving away from us faster with distance.
- 34:52The second signal is something subtler. It is the galaxy's
- 34:57individual motion on top of that exten banshion caused by
- 35:01the gravitational tug of everything around it. Astronomers call this
- 35:06the peculiar velocity. It is the deviation from pure expansion
- 35:12and It is a direct fingerprint of the local gravitational field.
- 35:17If you could map the peculiar velocities of thousands of
- 35:21galaxies across hundreds of millions of light years, you would
- 35:25not be looking at where galaxies happen to be sitting
- 35:28right now. You would be looking at where gravity is
- 35:32pulling them. You would see the underlying skeleton of the
- 35:36mass distribution, not just its surface appearance. This is what
- 35:42Tully and his collaborators set out to do. The analogy
- 35:46that makes this clearest is a watershed stand somewhere in
- 35:51the rocky mountains, and the rain that falls on your
- 35:54left flows eventually toward the Pacific. The rain that falls
- 36:00on your right flows toward the Atlantic or the Gulf
- 36:04of Mexico. There is a dividing line running along the
- 36:07mountain ridges where these drainage basins meet. On either side
- 36:12of that line, water flows in fundamentally different directions. Neither
- 36:18side knows anything about the other. They belong to different systems. Now,
- 36:24imagine the same thing at cosmic scale. Galaxies are not
- 36:29sitting still. They are flowing very slowly by human standards,
- 36:34toward the nearest major gravitational concentration in one region, they
- 36:39flow toward one center of mass. In an adjacent region,
- 36:44they flow toward a different one. The boundary between those
- 36:48two regions, the cosmic equivalent of the continental divide, is
- 36:54where the peculiar velocities reverse direction. That boundary defines where
- 37:00one supercluster ends and another begins, not a density threshold,
- 37:06a water shed. This was the conceptual breakthrough. A supercluster,
- 37:12under Tully's definition, is not simply a region where galaxies
- 37:16are dense. It is a basin of attraction, a volume
- 37:20of space inside which all galaxy motions, once you subtract
- 37:25the background expansion, are directed inward toward the same gravitational center.
- 37:31The boundaries are determined not by how many galaxies you
- 37:35can count per cubic megaparsec, but by where the flow
- 37:39changes direction. The method required data, enormous amounts of it.
- 37:46To construct a meaningful map of peculiar velocities across hundreds
- 37:50of millions of light years. You need precise, independent distances
- 37:55for thousands of galaxies. Redshift alone does not work, because
- 38:00redshift conflates the expansion velocity with the peculiar velocity. You
- 38:07cannot separate them without an independent distance measurement. Tully and
- 38:13his colleagues had been building toward this for years. The
- 38:17result was the Cosmic Flows two catalog, containing measured distances
- 38:23for more than eight thousand, one hundred galaxies spread across
- 38:27a substantial volume of the nearby universe. Each distance was
- 38:33derived using one or more of the established techniques, primarily
- 38:37the Tullyfisher relation for spirals, along with other methods for
- 38:42other galaxy types. The CATA log represented the most complete
- 38:48and precise data set of its kind ever. Assembled. With
- 38:51those distances, the team could calculate each galaxy's peculiar velocity directly,
- 38:57subtract the expected expansion v velocity, and what remains is
- 39:02real motion gravitational flow. When you plot those flow vectors
- 39:08across thousands of galaxies, patterns emerge filaments of flow converging
- 39:14toward the same point boundaries where flow directions diverge, the
- 39:20invisible architecture of gravity made visible through the motion of light.
- 39:25The computation was not trivial. Converting raw distance and velocity
- 39:31measurements for thousands of galaxies into a coherent three dimensional
- 39:36flow map required sophisticated mathematical reconstruction. The team had to
- 39:43account for gaps in coverage, errors in individual distance measurements,
- 39:49and the contaminating effects of the zone of avoidance where
- 39:53peculiar velocity data was thin or absent. They developed techniques
- 39:58to smooth and reconstruc the flow field across poorly sampled regions,
- 40:03using the surrounding data to fill in the gaps as
- 40:06accurately as possible. It was as much mathematical craft as
- 40:12astronomical observation. When the paper landed in Nature on September four,
- 40:18twoenty fourteen, it presented not just a new structure, but
- 40:23a new framework. Every previous map of the local supercluster
- 40:29had drawn its borders based on galaxy density. Tulley's map
- 40:34drew borders based on gravitational coherence. The result was a
- 40:39structure vastly larger than anyone had previously outlined, one that
- 40:44absorbed the old Virgo supercluster as a single component, that
- 40:49stretched five hundred twenty million light years from one side
- 40:53to the other, and that contained roughly one hundred thousand
- 40:57large galaxies, all flowing, however slowly, toward a common gravitational center.
- 41:05The Greater Tractor, which had mystified astronomers for decades, turned
- 41:11out to be the heart of this basin. It was
- 41:14not a strange anomaly in an otherwise simple universe. It
- 41:19was the gravitational flow of the largest structure any of
- 41:23us had ever lived inside. What made the work genuinely
- 41:27significant was not the size of what it found, though
- 41:31the size was staggering. It was the redefinition of the
- 41:35thing being measured. Tully's team did not discover that the
- 41:40universe was bigger than we thought. They changed the question.
- 41:44Instead of asking where the galaxies are, they asked where
- 41:48the galaxies are going. That shift in question produced a
- 41:53shift in structure, a new way of drawing the map
- 41:57of our cosmic address that nobody had managed before. When
- 42:02they applied it to over eight thousand galaxies with measured
- 42:06distances and velocities, the shape that emerged from the data
- 42:12was enormous, coherent, and unlike anything on the existing maps.
- 42:18The structure that emerged from Tully's maps was five hundred
- 42:22twenty million light years across. That number is easy to
- 42:27type and almost impossible to hold in your mind, but
- 42:31let's try the milky Way. Our galaxy, the one containing
- 42:37our sun and every star visible on a clear night,
- 42:41stretches roughly one hundred thousand light years from one edge
- 42:45to the other. That already sounds enormous. Light traveling at
- 42:51one hundred eighty six thousand miles per second, takes one
- 42:55hundred thousand years just to cross it. Yet, if you
- 42:59want to line up Milky Way sized galaxies end to
- 43:03end and span the full width of Lanyakia, you would
- 43:07need five thousand of them, not five, not fifty five
- 43:13thousand galaxies, each containing hundreds of billions of stars laid
- 43:18side by side, and you still haven't reached the other end.
- 43:23That is what five hundred twenty million light years means
- 43:26in practical terms. It is a number that defeats ordinary
- 43:31intuition entirely. The mass locked up inside this structure is
- 43:35just as staggering. Laniakia contains roughly one hundred thousand large galaxies.
- 43:42Each of those galaxies is, by any human measure, incomprehensibly large.
- 43:49But the total mass of Laniakia isn't just the mass
- 43:52of the stars inside those galaxies. It includes the dark
- 43:57matter halos wrapped around each one, the hot gas filling
- 44:02the space between galaxies, and the gravitational glue holding clusters together.
- 44:09Add it all up and you get something in the
- 44:11range of ten to the power of seventeen solar masses.
- 44:16That's a one, followed by seventeen zeros measured in suns
- 44:21one hundred quadrillion suns. Written out as a number, it
- 44:25has so many digits that the number itself becomes meaningless
- 44:29to read. The human brain simply doesn't have a reference
- 44:33frame for it. There is no analogy that fully survives
- 44:37contact with this scale. What does Laniakia actually look like?
- 44:42This is where it gets genuinely strange. It is not
- 44:46a sphere. It is not a uniform cloud. It does
- 44:49not have smooth edges or a clean center. If you
- 44:53could somehow generate an image of it in three dimensions
- 44:57and step back far enough to see the whole at once,
- 45:01what you would see look something like a crumpled, sprawling web,
- 45:07dense bright knots mark where massive galaxy clusters sit. Thin
- 45:13threads connect them, filaments made of galaxies and gas, stretching
- 45:19for hundreds of millions of light years Between the nodes
- 45:23and between those filaments, there is almost nothing vast regions
- 45:28of dark empty space where galaxies are rare or absent entirely.
- 45:34The structure has shape and anatomy. But nothing about that
- 45:38shape is neat or symmetrical. Think of it less like
- 45:42a ball and more like a handful of soap bubbles
- 45:45smashed together and stretched. The walls of the bubbles are
- 45:49the filaments, the places where galaxies concentrate the air. Inside
- 45:55each bubble is a void where multiple bubbles meet the
- 46:00concentration of matter is highest. Those are the clusters. Laniakia
- 46:06is the region defined by one connected system of these
- 46:10filaments and flows, all of it draining gravitationally toward a
- 46:15common center. That center is what astronomers call the Great Attractor,
- 46:21a region deep inside Laniakia where the gravitational pull is strongest.
- 46:28Galaxies across the full five hundred twenty million light year
- 46:33span of the structure are moving slowly in that direction,
- 46:38not because they are being pushed, but because gravity has
- 46:42been pulling on them for billions of years and they
- 46:45have built up a drift. This motion is subtle, you
- 46:50would not notice it over a human lifetime, but measured
- 46:54in kilometers per second, the infall toward the Great Attractor
- 46:58is real and detectable. It is what allowed Tully's team
- 47:03to define the structure in the first place. The watershed
- 47:07flows all run toward this gravitational basin. That's where the
- 47:12center of Laniakia is. Now Here is the part that
- 47:16changes how you think about where you are. The Milky
- 47:20Way does not sit anywhere near that center. It sits
- 47:24on the edge, the outskirts the rim, depending on how
- 47:30you measure it. Our local group is somewhere around one
- 47:34hundred fifty to two hundred fifty million light years from
- 47:38the greater tractor. That means we are not in the
- 47:41middle of Laniakia. We are roughly halfway to the edge,
- 47:45on the outer fringe, in a relatively sparse and quiet
- 47:49part of the structure. There are no major galaxy clusters nearby.
- 47:54There is no dramatic concentration of matter in our immediate vicinity.
- 48:00We are in the low density outer region of an
- 48:03enormous gravitational basin, and the heart of that basin is
- 48:08hundreds of millions of light years away. This should be
- 48:12a genuinely disorienting realization. For most of human history, humans
- 48:18assumed they occupied a special or central place in the cosmos.
- 48:23Copernicus moved the Earth away from the center of the
- 48:27Solar system. Later work moved the Sun away from the
- 48:31center of the galaxy. Now Laniakia moves us away from
- 48:36the center of our own supercluster. Whatever the center of
- 48:40things might be, we are not near it. We are peripheral.
- 48:44In every structure we have ever managed to identify, there
- 48:49is something worth sitting with there. The greater tractor is
- 48:53pulling us toward it. Our local group is drifting incredibly
- 48:58slowly in that dire, but we are not falling fast.
- 49:04The distance is so enormous and the drift so gradual
- 49:08that it will take billions of years to cover even
- 49:11a fraction of it, and dark energy, the force accelerating
- 49:16the expansion of the universe, will likely pull the outer
- 49:20regions of Laniakia apart before any dramatic convergence happens. We
- 49:27are moving toward the center of our supercluster, but the
- 49:31supercluster itself is dissolving as we go. It is not
- 49:36a destination we will ever reach. The overall architecture of
- 49:40Lania KaiA, when you map it out with the flows
- 49:43and the clusters and the filaments, divides into several major regions.
- 49:48There is the part containing the Virgo cluster and our
- 49:52local group, the part containing the hydra and Centaurus clusters,
- 49:57the region around the normal cluster near the Greater Tractor itself,
- 50:02and the Pavo Indus supercluster region further out. These are
- 50:08not cleanly separated neighbourhoods. They are connected by filaments blending
- 50:14into each other the way the suburbs of a city
- 50:17blend into its outskirts. But the rough anatomy is there,
- 50:22and it all connects into a single coherent gravitational basin.
- 50:29One thing that the three dimensional maps make very clear
- 50:33is how much empty space there is. The filaments are thin,
- 50:38the clusters are relatively compact. Most of the volume of
- 50:42Laniakir is void. If you were a traveler moving through
- 50:46this structure at random, you would spend the vast majority
- 50:50of your journey in near empty darkness, far from any galaxy.
- 50:55The bright connected web that shows up on the maps
- 50:59represents a t miny fraction of the total volume. Most
- 51:03of Laniakia is nothing. And yet, even knowing all that
- 51:08one hundred thousand large galaxies is not a small number
- 51:14spread across five hundred twenty million light years, they fill
- 51:18this structure with an almost uncountable number of stars, planets,
- 51:24and everything else. The Milky Way alone has somewhere between
- 51:29one hundred and four hundred billion stars. Multiply that by
- 51:34one hundred thousand galaxies, and even a rough estimate becomes
- 51:39a number that no human can meaningfully visualize. Whatever is
- 51:43out there in Laniakia, whatever is in those galaxies, on
- 51:48those planets, around those stars, it exists at a scale
- 51:53that makes the entire history of human civilization look like
- 51:58a footnote written in pens on the last page of
- 52:01a book inside a library that fills a continent. The
- 52:06structure is real. It is not a theoretical construct or
- 52:10a statistical artifact. It is a physical feature of the
- 52:14universe we live in, defined by the actual motions of
- 52:18actual galaxies across actual space. And the Milky Way, with
- 52:24all its hundreds of billions of stars, sits near the
- 52:28outer edge of this a small dot on the rim
- 52:31of something almost too large to picture. When the time
- 52:36came to name the structure, Brent Tully did not reach
- 52:40for Greek or Latin. Most astronomical discoveries get named after
- 52:44their discoverers, or after constellations, or after the catalogs they
- 52:49appeared in. Tully's team was working at the University of Hawaii.
- 52:55They were embedded in a place with its own deep language,
- 52:59its own history of navigating enormous and featureless expanses, and
- 53:05its own tradition of reading the sky. So Tully did
- 53:10something unusual. He consulted with Hawaiian language experts to find
- 53:15a name that fit what they had actually found. The
- 53:19word they landed on was Lani akaia. It comes from
- 53:22two Hawaiian roots. Lani means heaven or sky, or the
- 53:27celestial realm above, a KaiA means spacious, open, immeasurable. Together
- 53:34the phrase means something like immense heaven or the expansive sky,
- 53:39a realm of stars so vast it resists ordinary description.
- 53:45The name was suggested by Nawa'a Napoleon, an associate professor
- 53:49of Hawaiian language at Capiolani Community College. It were not
- 53:54a casual choice. It captured something real about the scale
- 53:59of the thing being named. A structure five hundred twenty
- 54:03million light years across containing one hundred thousand galaxies, bigger
- 54:09than anything our nearest ancestors could have conceived. Immense heaven
- 54:15is not an exaggeration. It is barely adequate. But there
- 54:19is something stranger and more interesting here than just a
- 54:23well chosen word. The name carries a cultural weight that
- 54:28runs directly parallel to the science behind it. Polynesian navigators
- 54:34cross the Pacific Ocean, the largest body of water on Earth,
- 54:39without compasses, without GPS, without charts in the modern sense.
- 54:45They crossed it by reading the sky. They memorized the
- 54:49rising and setting points of hundreds of stars. They understood
- 54:54how ocean swells move relative to wind and island chains.
- 54:58They track the color of the water, the flight paths
- 55:02of birds, the feeling of current against a hull. But
- 55:06above all, they read the heavens. The sky was their map.
- 55:11The sky told them where they were. These were not
- 55:15short journeys. The Pacific spans more than twelve thousand miles
- 55:19at its widest. Ancient Polynesian navigators reached Hawaii, New Zealand,
- 55:25Easter Island, and dozens of other island groups, separated by
- 55:30thousands of miles of open ocean, with no landmarks visible
- 55:34from the water. They did it by knowing the sky
- 55:38better than any civilization in history. The sky was not
- 55:42decoration to them, It was orientation. It told you which
- 55:47way was home. Now consider what Tully's team actually did.
- 55:52They spent years mapping how eight thousand galaxies moved through space.
- 55:57They tracked the floes, the cony urgencies, the divergences, the
- 56:03subtle gravitational currents running beneath the smooth expansion of the universe,
- 56:09and by reading those flows, they found our address, not
- 56:13our street address, not our galaxy, our supercluster. They used
- 56:19the motion of the cosmos to figure out where we
- 56:21are inside it. They navigated by reading the sky. The
- 56:26parallel is not decorative, it is exact. The navigators who
- 56:31crossed the Pacific were doing something that looks from the
- 56:34outside like it should be impossible. How do you find
- 56:39a small island in an ocean that wide using only
- 56:42the sky? The answer is that you know the sky
- 56:46well enough that it becomes a coordinate system, a live
- 56:51map of your position and heading. Tully's team was doing
- 56:55something that also looks from the outside like it should
- 56:59be impossible. How do you find the shape of a
- 57:02structure five hundred twenty million light years across when you
- 57:06are inside it and can only observe from a single point.
- 57:11The answer is that you read the flows well enough
- 57:15that they reveal the shape of the basin you are
- 57:18sitting in. There is something almost too fitting about this.
- 57:23The name Laniakia honors a tradition of navigation that solved
- 57:28the same fundamental problem at a completely different scale. Where
- 57:34are we? Which way is home? How do you find
- 57:38your position in a featureless expanse with no obvious landmarks.
- 57:43The Polynesian answer was the stars. Tully's answer was the
- 57:48motion of galaxies. Both are forms of reading the sky
- 57:52to find your place within it. Na Napoleon's suggestion was
- 57:57not just linguistically appropriate, it was philosophically accurate. The sky
- 58:03to Polynesian navigators was not a background. It was a
- 58:07location system. And that is precisely what lania Kia is.
- 58:12A location, a place in the cosmos that has a structure,
- 58:17a shape, a center, a set of flows defining its edges.
- 58:22For the first time in history, we have a name
- 58:25for the largest structure we belong to, and that name
- 58:29comes from a people whose entire civilization was built around
- 58:33the idea that the sky tells you where you are.
- 58:37That is a strange kind of symmetry. The navigators who
- 58:41crossed the Pacific by reading the heavens had no way
- 58:44of knowing what those heavens were embedded in. They knew
- 58:48the stars as guides. They did not know those stars
- 58:52were part of a galaxy, or that the galaxy was
- 58:55part of a supercluster, or that the supercluster had an aim.
- 59:01Now it does. The people who learned to cross the
- 59:04Pacific by reading the sky gave their language to the
- 59:08discovery of where that sky actually sits in the universe.
- 59:13The Virgo Supercluster did not disappear when Laniakir was defined.
- 59:19It simply shrank in significance. For decades, the Virgo Supercluster
- 59:24was the best answer astronomers had to the question of
- 59:28our large scale cosmic home. It was a genuine structure.
- 59:33It was real, roughly one hundred million light years across,
- 59:38centered on a dense knot of galaxies in the direction
- 59:42of the constellation Virgo. It had been identified in the
- 59:46nineteen fifties by astronomer Gerrard de Vaucouleur and refined by
- 59:52generations of researchers who followed him. If you had asked
- 59:56a cosmologist in nineteen ninety where the the Milky Way
- 1:00:00lived in the largest known structure, the answer was the
- 1:00:04Virgo Supercluster. And that answer felt solid, It felt complete.
- 1:00:11It had been tested and mapped and written into textbooks.
- 1:00:16When Lanyakir arrived in twenty fourteen, it did not invalidate
- 1:00:21any of that work. It just revealed that the work
- 1:00:25had been describing a neighborhood without realizing the city extended
- 1:00:30far beyond it. The Virgo Cluster itself sits near the
- 1:00:34heart of this older structure, and it is worth pausing
- 1:00:38on what that cluster actually is. Several thousand galaxies packed
- 1:00:44into a region roughly fifteen million light years across, not
- 1:00:49a loose scattering, but a genuine gravitational city, one of
- 1:00:54the richest concentrations of galaxies within several hundred million lights
- 1:01:00of Earth. It anchors the Virgo Supercluster the way a
- 1:01:05downtown core anchors a metropolitan region. Its mass pulls on
- 1:01:10everything around it. The local group, the small collection of
- 1:01:15roughly eighty galaxies that includes the Milky Way and Andromeda,
- 1:01:20is moving toward the Virgo Cluster right now, very slowly,
- 1:01:25tugged by its gravity across fifty to sixty million light
- 1:01:30years of intervening space. The Virgo Cluster is not abstract.
- 1:01:37It is a real gravitati onal presence, something our entire
- 1:01:42galactic neighborhood feels, but the local group's position in all
- 1:01:46of this is worth examining closely roughly eighty galaxies, most
- 1:01:52of them small satellites orbiting either the Milky Way or Andromeda.
- 1:01:57The two dominant members, our galaxy and its large neighbour
- 1:02:02are themselves unremarkable spiral galaxies by the standards of the
- 1:02:07broader universe. The local group sits in the outer regions
- 1:02:12of the Virgo supercluster, not near its center. Then the
- 1:02:17Virgo supercluster itself, as Laniakia revealed, occupies an outer region
- 1:02:22of Laniakia. Stack these positions together and a clear picture forms.
- 1:02:29We are not near the center of our galaxy cluster.
- 1:02:33Our cluster is not near the center of the Virgo supercluster.
- 1:02:38The Virgo supercluster is not near the center of Lania KaiA.
- 1:02:43At every level of the hierarchy, we are somewhere on
- 1:02:47the periphery, a pattern that seems almost deliberate, but is
- 1:02:51simply what the data shows. The conceptual demotion this represents
- 1:02:57is worth sitting with every level of our cosmic address
- 1:03:02that had felt like a meaningful designation. Virgo Supercluster home
- 1:03:08the largest structure we belonged to turned out to be
- 1:03:12a subdivision of something larger. It is like being told
- 1:03:17that the city you have lived in your whole life,
- 1:03:20the city whose name you gave when people asked where
- 1:03:24you were from, is not a city at all. It
- 1:03:28is a district, and the actual city is five times bigger,
- 1:03:34extends in directions you were not looking, and contains structures
- 1:03:39in its other districts you have never seen. The name
- 1:03:42on your driver's license did not change, You did not move,
- 1:03:47but your sense of where you are shifted completely. This
- 1:03:52kind of conceptual reshuffling has happened before. In astronomy. Earth
- 1:03:57was not the center of the Solar System, the Sun
- 1:04:00was not the center of the galaxy. The Milky Way
- 1:04:04was not the only galaxy. Each revision followed the same pattern.
- 1:04:10A structure that seemed like the largest relevant frame turned
- 1:04:13out to be a component of something larger. The Virgo
- 1:04:18supercluster joining this list was not a shock to anyone
- 1:04:22paying attention to the history of the field, but it
- 1:04:25was still a genuine revision of the scientific record. Every
- 1:04:30textbook that had listed the Virgo supercluster as our supercluster
- 1:04:35needed an asterisk, if not a rewrite. What Laniakia absorbed
- 1:04:41was not just a name on a map. The Virgo
- 1:04:44Supercluster had been associated with a specific picture of cosmic structure,
- 1:04:49a set of boundaries, a hierarchy. That picture was not
- 1:04:54wrong exactly. The galaxies are still where they were, the
- 1:04:59flows are rear. The Virgo Cluster still dominates its local
- 1:05:03region of space. But the boundaries that defined the Virgo
- 1:05:08Supercluster as an independent entity were revealed to be permeable,
- 1:05:13artificial in a certain sense, drawn around a density peak
- 1:05:18rather than around a true gravitational basin. When Tully's team
- 1:05:24redrew those boundaries using flow patterns instead of density, the
- 1:05:29Virgo Supercluster was absorbed. It became one region in a
- 1:05:33much larger structure, like a borough absorbed into a growing
- 1:05:37metropolis that had expanded far beyond its original limits. There
- 1:05:43is something almost vertiginous about this if you follow it
- 1:05:46all the way down. The Milky Way is one of
- 1:05:50roughly eighty galaxies in the Local Group. The Local Group
- 1:05:55is one of perhaps a thousand groups and clusters in
- 1:05:58the Virgo Supercluster. The Virgo Supercluster is one of several
- 1:06:04major components within Laniakia. Laniakia contains something on the order
- 1:06:10of one hundred thousand large galaxies spread across five hundred
- 1:06:15twenty million light years. At each step, the scale multiplies
- 1:06:21and the previous frame of reference shrinks. Our galaxy, which
- 1:06:26contains hundreds of billions of stars, is a minor entry
- 1:06:30in a minor cluster on the outer edge of a
- 1:06:34supercluster component that is, itself an outer region of the
- 1:06:39structure we actually live in. None of this diminishes what
- 1:06:43the Vergo Supercluster is. It is still a real and
- 1:06:48massive structure. The gravitational influence of the Virgo Cluster on
- 1:06:53our local group is real and measurable. But calling the
- 1:06:58Virgo Supercluster our home supercluster, the way astronomers did for
- 1:07:04half a century was like calling a suburb the city.
- 1:07:09What we had called home for half a century turned
- 1:07:12out to be one small corner of a much larger room.
- 1:07:16Laniaka is not a smooth, uniform cloud of galaxies. It
- 1:07:20has bones. If you could somehow pull back far enough
- 1:07:24to see the whole structure at once, the way you
- 1:07:27might look down at a city from altitude on a
- 1:07:30clear night, what you would see is not a featureless glow.
- 1:07:35You would see something more like a nervous system, bright
- 1:07:39knots of light where clusters sit, long faint threads connecting them,
- 1:07:45and between those threads enormous darkness, not empty by accident,
- 1:07:52but empty because gravity spent billions of years pulling matter
- 1:07:56away from those regions and piling it somewhere else. The
- 1:08:01voids are not gaps in the data. They are real features,
- 1:08:05as much a part of the structure as the clusters themselves.
- 1:08:10The major galaxy clusters inside Laniakia red like a catalog
- 1:08:15of the southern and equatorial sky. Virgo is the closest
- 1:08:20significant one to us. Hydra and Centaurus sit deeper in
- 1:08:25part of a dense complex that blends into the gravitational
- 1:08:28center of the whole structure. The normal cluster lies close
- 1:08:32to the greater tractor itself, embedded in the most crowded
- 1:08:36region of Laniakia's interior. Ophiucus is one of the most
- 1:08:41massive clusters in the entire supercluster, holding an enormous concentration
- 1:08:46of hot gas and hundreds of galaxies bound tightly together.
- 1:08:52Fornax and Eridanus anchor a separate region of the structure,
- 1:08:57part of the southern extension of the film entry Web.
- 1:09:01These are not just names on a list. Each one
- 1:09:05represents a gravitational knot that has been accumulating matter for
- 1:09:10most of the age of the universe. A galaxy cluster
- 1:09:14forms because the universe was never perfectly smooth. In the
- 1:09:19earliest moments after the Big Bang, there were tiny variations
- 1:09:24in density. Some regions had slightly more matter, some slightly less.
- 1:09:30Those differences were almost imperceptibly small, but gravity is patient.
- 1:09:37Over hundreds of millions of years, the slightly denser regions
- 1:09:42pulled more matter toward themselves that made them denser. Still,
- 1:09:47other matter fell in from surrounding areas. Eventually those regions
- 1:09:53collapsed into the first galaxies. Galaxies fell toward each other,
- 1:09:59grouping into clusterters, and clusters gathered into superclusters. What you
- 1:10:05see in Laniakia now is the result of that process,
- 1:10:08running for roughly thirteen billion years. The clusters are where
- 1:10:13gravity won most decisively. The voids are where it why
- 1:10:18it's too thinly spread to win at all. The assembly
- 1:10:22process did not stop once the initial clusters formed. Smaller
- 1:10:27clusters and galaxy groups continued falling into larger ones throughout
- 1:10:31cosmic history. Their mergers, releasing tremendous energy. A massive cluster
- 1:10:38like Virgo or Centaurus did not reach its present configuration
- 1:10:43until relatively recently. On cosmic time scales, clusters continue to
- 1:10:49grow and evolve, incorporating isolated galaxies that venture too close
- 1:10:55to their gravitational influence. The largest clusters have been aque,
- 1:11:00cumulating matter steadily for billions of years, and some are
- 1:11:04still in the process of merging with neighboring structures today.
- 1:11:09This ongoing accretion gradually reshapes the cluster environment and increases
- 1:11:15total mass. The clusters visible in Laniakia are not static
- 1:11:20monuments to ancient gravity b up dynamic systems, still assembling
- 1:11:26and growing, drawing matter inward through the cosmic web. Inside
- 1:11:30a cluster like Virgo or Norma, individual galaxies are not
- 1:11:35sitting still. They move at speeds of hundreds or even
- 1:11:39thousands of kilometers per second, orbiting the cluster's center of
- 1:11:44mass the way bees circle a hive. The space between
- 1:11:48them is filled with extremely hot diffuse gas so hot
- 1:11:53it emits X rays, and all of it is held
- 1:11:56together by the combined gravity of the galaxies. The gas
- 1:12:01the dark matter that makes up the majority of the
- 1:12:04cluster's total mass. A rich cluster can contain anywhere from
- 1:12:09hundreds to several thousand galaxies. The Virgo cluster alone holds
- 1:12:15several thousand. That kind of density is genuinely strange when
- 1:12:21you think about what galaxies are. Each one of those
- 1:12:25is a structure containing hundreds of billions of stars. They
- 1:12:30are packed together tightly enough to interact, distort each other,
- 1:12:34and occasionally merge. The filaments that connect these clusters are
- 1:12:39harder to see, but just as real. They are elongated
- 1:12:43structures rivers of galaxies flowing between the dense nodes of
- 1:12:48the web. A single filament inside Laniakia might stretch for
- 1:12:53one hundred million light years or more, containing thousands of
- 1:12:58galaxies arranged loosely along its length. These are not solid structures.
- 1:13:04There is enormous space between the galaxies inside a filament,
- 1:13:09but statistically the galaxy density along a filament is meaningfully
- 1:13:15higher than in the surrounding voids. Gravity draws matter toward
- 1:13:20the filaments, and the filaments drain toward the clusters at
- 1:13:24their ends. The whole thing flows slowly toward the densest concentrations.
- 1:13:32Then there are the voids. Cosmological voids are among the
- 1:13:37strangest objects in the universe, if you can call an
- 1:13:41absence an object. They range in diameter from about thirty
- 1:13:45million light years on the small end to three hundred
- 1:13:49million light years for the largest known examples. Inside a void,
- 1:13:54the mean density of matter is less than a tenth
- 1:13:58of the cosmic average. Galaxies are not absent entirely. There
- 1:14:03are isolated galaxies and small groups scattered through void regions,
- 1:14:08but they are so sparse that the void is, on
- 1:14:12cosmic terms, essentially empty. If you lived in a galaxy
- 1:14:18inside one of the large voids bordering Laniakaia, your view
- 1:14:22of the night sky would be far lonelier than ours.
- 1:14:26The nearest large galaxy cluster might be a hundred million
- 1:14:31light years away. The universe would look far emptier than
- 1:14:35it do as from our position. What makes this architecture
- 1:14:40striking is that it is not unique to Laniakia. The
- 1:14:44same pattern clusters at the nodes, filaments connecting them, voids
- 1:14:51filling the space between, appears everywhere in the observable universe.
- 1:14:56At these scales, cosmologists call it the cosmic It is
- 1:15:01the large scale structure of the universe, and it was
- 1:15:05not designed. It emerged naturally from gravity acting on the
- 1:15:10tiny density fluctuations left over from the earliest moments of
- 1:15:15cosmic history. Simulations that start from the conditions of the
- 1:15:20early universe and run the physics forward reproduce this filamentary
- 1:15:25structure automatically. The web was always going to form this
- 1:15:30way given those initial conditions. Laniakia is one node in
- 1:15:36that larger web, surrounded by neighboring superclusters that have the
- 1:15:41same e internal architecture of clusters filaments voids, each one
- 1:15:48connected to others across distances that dwarf even Laniakia itself.
- 1:15:53This matters for how you think about what Laniakia is.
- 1:15:57It is not a bounded object floating in empty space.
- 1:16:01It is a region of the cosmic web that has
- 1:16:04a coherent gravitational basin, a region where galaxy motions converge
- 1:16:10toward a common center, but its edges blend into surrounding
- 1:16:14structures that are themselves organized the same way. The filaments
- 1:16:20inside Laniakia connect outward to filaments in neighboring superclusters. The
- 1:16:26voids inside Laniakia open onto voids that extend far beyond
- 1:16:31its defined boundary. The structure has no sharp walls. It fades,
- 1:16:37bleeds outward, continues from inside. Living in a galaxy on
- 1:16:43the outer edge of one of the smaller filamentary extensions,
- 1:16:48you see almost none of this. You see a sky
- 1:16:51full of stars that all belong to your galaxy. You
- 1:16:56see a handful of nearby galaxies with a telescope. If
- 1:17:01you look at the distribution of distant galaxies across the
- 1:17:04whole sky with a powerful enough survey, you start to
- 1:17:09see hints of the filamentary structure over dense regions in
- 1:17:13some directions, under dense regions in others. But the full
- 1:17:19three dimensional picture the bones of Laniakia only becomes visible
- 1:17:25when you map thousands of galaxies across hundreds of millions
- 1:17:29of light years and trace how they are moving. This
- 1:17:33is not a structure you would recognize from the inside.
- 1:17:38That is exactly why it took until two thy fourteen
- 1:17:42for anyone to draw its full outline. Here is the
- 1:17:45strange part Laniakia is not actually held together. There is
- 1:17:50a difference between a gravitationally bound structure and a basin
- 1:17:54of attraction. A gravitationally bound structure is one where gravity
- 1:18:00he wins, where the objects inside it are locked together
- 1:18:04tightly enough that expansion cannot pull them apart. Galaxy clusters
- 1:18:10are bound. The Virgo cluster, sitting near the center of
- 1:18:14our local corner of Laniakia, holds thousands of galaxies in
- 1:18:19a gravitational grip. They will never escape. Those galaxies are
- 1:18:24not going anywhere. They will continue orbiting, colliding, eventually merging
- 1:18:31over tens of billions of years into something unrecognizable. But
- 1:18:35they will stay together. Our own local group is bound.
- 1:18:41The Milky Way and the Andromeda galaxy are falling toward
- 1:18:45each other right now, closing the gap at roughly one
- 1:18:49hundred ten kilometers per second. In about four point five
- 1:18:54billion years, they will collide. That is a gravitationally bound
- 1:18:59system behavior exactly as bound systems do. Laniakia is something different.
- 1:19:05Its galaxies are not locked to each other. They are
- 1:19:09simply flowing in the same direction, pulled toward the greater tractor,
- 1:19:14the way water flows toward the lowest point in a valley.
- 1:19:18The structure has coherence because the flows are real and measurable,
- 1:19:24but coherence is not the same as a bond. A
- 1:19:27river has coherence the water moves together in a shared
- 1:19:33direction following the same gradient. But the river does not
- 1:19:37hold itself together. It flows because the landscape underneath it
- 1:19:42slopes a certain way. Remove the slope and the river stops.
- 1:19:49Laniakia is similar. Its structure exists because the gravitational landscape
- 1:19:54of this region of space slopes inward toward the greater tractor.
- 1:20:00The galaxies follow that slope right now in this epoch
- 1:20:05of cosmic history. T hat slope is real enough to
- 1:20:09define an enormous coherent supercluster. But there is something else
- 1:20:14shaping that landscape. Dark energy is real. It is the
- 1:20:19dominant energy component of the universe, and it is working
- 1:20:23against gravity at every scale large enough for the expansion
- 1:20:28of space to matter. On the scale of galaxy clusters,
- 1:20:33gravity wins. On the scale of superclusters, the contest is
- 1:20:38closer on the scale of Laniakia. Dark energy is already winning.
- 1:20:44At the outer edges. The expansion of the universe is
- 1:20:48not uniform in its effects. Galaxies that are gravitationally bound
- 1:20:53to each other are immune. The expansion of space does
- 1:20:57not reach in and tear apart structures the are already
- 1:21:00gravitationally locked, But galaxies on the outer fringes of Laniakia,
- 1:21:06where the gravitational pull from the center is weaker and
- 1:21:10the distances are greater, are in a different situation. For
- 1:21:15those galaxies, the outward push of cosmic expansion is already
- 1:21:20comparable too or greater than the inward pull of gravity.
- 1:21:26Over time, that balance tips further toward expansion. The outer
- 1:21:32galaxies drift, then they accelerate away. The boundary of the
- 1:21:38structure does not hold. Think about what this means practically.
- 1:21:43Right now, a galaxy near the edge of Laniakia is
- 1:21:47technically part of the supercluster. Its motion if you subtract
- 1:21:52out the general expansion of the universe points inward. It
- 1:21:57is part of the flow. Over hundreds of billions of years,
- 1:22:02the expansion rate increases relative to the gravitational attraction, and
- 1:22:08at some point that galaxy's peculiar velocity, the inward drift
- 1:22:14that makes it part of Laniakia, gets overwhelmed by the
- 1:22:18expanding universe, carrying it away. The galaxy tips over the
- 1:22:23watershed divide and effectively leaves the supercluster, not dramatically, not suddenly,
- 1:22:31just gradually, inexorably, as cosmic expansion stretches the space between
- 1:22:37it and the Greater Tractor until gravity can no longer
- 1:22:41bridge the gap. This happens first at the edges and
- 1:22:46works inward. The filaments connecting distant clusters weaken and eventually dissolve.
- 1:22:54The clusters themselves remain intact. They are bound, but the
- 1:22:59threads thinking them across hundreds of millions of light years
- 1:23:03slowly break. The supercluster's architecture. That web of bright nodes
- 1:23:09connected by strands of galaxies gradually loses its connections. The
- 1:23:16nodes persist, the web does not. The Greater Tractor does
- 1:23:21not switch off. It remains a massive concentration of matter,
- 1:23:26and it continues pulling nearby galaxies toward it. But its
- 1:23:30gravitational reach has a limit, and that limit gets shorter
- 1:23:34as dark energy drives space to expand faster. Currently, the
- 1:23:40Greater Tractor's influence extends across the full scale of Laniakia,
- 1:23:45roughly two hundred and fifty million light years in all
- 1:23:48directions over hundreds of billions of years. The region where
- 1:23:54its gravity beats out expansion contracts. More and more of
- 1:23:58the supercluster's outer volume crosses over into territory where expansion wins.
- 1:24:04What you are left with Eventually is not Laniakia. You
- 1:24:09are left with a collection of bound galaxy clusters, each isolated,
- 1:24:14each intact within itself, but separated from all the others
- 1:24:19by expanding voids too large for gravity to bridge. The
- 1:24:24greater tractor's neighbourhood survives as a dense core. The outlying
- 1:24:30regions drift away into the darkness. Nothing remains to show
- 1:24:35that these clusters were ever connected, that galaxies across five
- 1:24:40hundred twenty million light years once all flowed toward the
- 1:24:44same gravitational basin. This is the strange status Laniakia holds.
- 1:24:51It is real, the flows that define it are measurable.
- 1:24:55The structure that Brent Tully's team drew in twenty fourteen
- 1:24:59is coherent and meaningful, and yet it is not permanent
- 1:25:03in the way that a galaxy is permanent, or a
- 1:25:06star or a planet. It exists as a structure only
- 1:25:10because we happen to be living in an epoch when
- 1:25:13its coherence is intact, when the gravitational flows are strong
- 1:25:18enough relative to expansion to give it definable shape and
- 1:25:23definable borders. In a universe older than ours by a
- 1:25:27factor of ten or one hundred, there would be no
- 1:25:31Laniarka to find, there would be no flow to map.
- 1:25:37We mapped it just in time, in a sense, a
- 1:25:40structure coherent enough to define today but destined to dissolve
- 1:25:45over time scales longer than the current age of the universe.
- 1:25:49To define a structure by how galaxies move, you first
- 1:25:53have to know where those galaxies actually are. That sounds obvious,
- 1:25:58it is in practice one of the hardest problems in
- 1:26:02observational astronomy, and solving it took the better part of
- 1:26:06five decades. Here is the core difficulty. You cannot lay
- 1:26:11a measuring tape across space. You cannot bounce a signal
- 1:26:15off a galaxy one hundred million light years away, and
- 1:26:18time the echo. Every method astronomers have for measuring cosmic
- 1:26:23distances is indirect. Each one rests on a physical relationship
- 1:26:29something that connects a property you can observe to a
- 1:26:32property you cannot directly measure, and each one carries error.
- 1:26:38Small errors in distance, when converted into peculiar velocities, produce
- 1:26:43large errors in the flow maps. The flow maps are
- 1:26:48only as clean as the distances underneath them. Everything that
- 1:26:52makes Laniakir real and mappable and coherent traces back to
- 1:26:57this unglamorous problem of actually pinning down where things are.
- 1:27:01The way astronomers approach this is through what they call
- 1:27:05the distance ladder. The idea is to build outward in steps.
- 1:27:11Each step uses a method that works reliably over a
- 1:27:14certain range of distances but fails beyond it. Each new
- 1:27:19method gets calibrated against the previous one before you trust
- 1:27:23it at greater distances. The bottom rungs of the ladder
- 1:27:28are close enough that geometry alone can do the work. Parallax,
- 1:27:34the tiny apparent shift in a nearby star's position, as
- 1:27:38Earth orbits the Sun, works out to a few thousand
- 1:27:42light years above that. You switch to a different technique
- 1:27:47at each transition. You are trusting that the calibration between
- 1:27:51methods is solid, because any error there propagates upward through
- 1:27:56every measurement you make at greater distances. To reach galaxies
- 1:28:01hundreds of millions of light years away, you need methods
- 1:28:05that work at truly enormous scales. Two of the most
- 1:28:10important are the Tullyfisher relation and the fundamental plane, and
- 1:28:15together they are responsible for most of the data that
- 1:28:19went into defining Laniakia. The Tullyfisher relation applies to spiral galaxies.
- 1:28:27It was noticed in nineteen seventy seven by Brent Tully
- 1:28:32and J. Richard Fisher, and the same Tully would later
- 1:28:36lead the Laniakia team. What they found was a tight
- 1:28:40correlation between how fast a spiral galaxy rotates and how
- 1:28:44intrinsically luminous it is. A galaxy spinning faster is more massive,
- 1:28:51and more massive galaxies are brighter. If you measure a
- 1:28:55spiral galaxy's rotation speed, you can infer how bright it
- 1:28:59truly is. Then you compare that true brightness to how
- 1:29:04bright it appears in the sky. The difference tells you
- 1:29:08how far away the light must have traveled to look
- 1:29:11as faint as it does. It's the same logic as
- 1:29:15knowing how powerful a light bulb is and using its
- 1:29:18apparent dimness to estimate how far down the street it sits.
- 1:29:23The challenge is precision. Small uncertainties in the rotation speed
- 1:29:29measurement translate into distance errors. Calibrating the relation required extensive
- 1:29:35work across nearby galaxies, where independent checks were possible. For
- 1:29:41elliptical galaxies, which don't rotate the same way, a different
- 1:29:46method applies elliptical galaxies follow what astronomers call the fundamental plane,
- 1:29:54a relationship involving three observable quantities the galaxy size, its
- 1:30:00surface brightness, and the velocity dispersion of its stars, basically
- 1:30:06how fast the stars are moving relative to each other. Internally,
- 1:30:11these three properties are not independent. They are linked by
- 1:30:16the underlying physics of how elliptical galaxies form and evolve.
- 1:30:21If you measure two of them, you can infer the third,
- 1:30:25and from the inferred properties you can extract the true luminosity,
- 1:30:30which again gives you distance. The fundamental plane is messier
- 1:30:34than Tullyfisher in some respects, with more scatter in the relationship,
- 1:30:39but it extends the distance ladder to galaxy types that
- 1:30:42Tullyfisher cannot reach. The Cosmic Flows project, led by tully
- 1:30:48in his team, was built to gather these measurements in
- 1:30:51systematic large numbers. The Cosmic Flows two catalog, which fed
- 1:30:58directly into the two thousand, five fourteen Laniakia paper, contained
- 1:31:02distances for more than eight thousand, one hundred galaxies. That
- 1:31:08number sounds large until you realize how vast the volume
- 1:31:12of space being mapped actually is. At the outer edges
- 1:31:16of the survey, the coverage was thin. Individual galaxies were
- 1:31:21separated by gaps where no measurements existed. The flow maps
- 1:31:27in those regions were smooth interpolations between real data points.
- 1:31:32Every boundary on the Laniakia map is only as sharp
- 1:31:36as the data density behind it allows. What cosmic flows
- 1:31:41for released years later brought was scale nearly fifty six
- 1:31:46thousand galaxy distances, gathered using eight separate methodologies cross checked
- 1:31:52against each other. The expanded catalog allowed the flow maps
- 1:31:57to extend further and resolve structure more finely. It also
- 1:32:02allowed genuine tests of whether the twoenty fourteen boundaries held
- 1:32:08up under scrutiny from a data set seven times larger.
- 1:32:13Mostly they did, which is itself a statement about how
- 1:32:18solid the original analysis was despite the sparse coverage. It
- 1:32:24is worth being specific about how much human effort this represents.
- 1:32:28Measuring rotation curves for thousands of spiral galaxies requires deep
- 1:32:34spectroscopic observations, long nights at large telescopes, careful sky subtraction,
- 1:32:41and painstaking reduction of the raw data. It requires doing
- 1:32:46this for galaxies that appear as faint smudges in the sky.
- 1:32:51It requires going back and remeasuring, checking for systematic errors,
- 1:32:57updating calibrations as better nearby act INCA points become available.
- 1:33:02The Cosmic flows catalogs reflect observational campaigns stretching back to
- 1:33:08the nineteen seventies, accumulated across hundreds of telescope nights at
- 1:33:14facilities from Hawaii to the Canary Islands to Chile. Nobody
- 1:33:20did this in a single coordinated push. It accumulated peace
- 1:33:25by piece, researcher by researcher over four decades, until the
- 1:33:31database was large enough and reliable enough to trace the
- 1:33:35floes that outlined Laniakia. The map of Laniakia is only
- 1:33:40as reliable as the distances that went into building it,
- 1:33:44which means it rests on decades of unglamorous observational work
- 1:33:50that most people never hear about. If Laniakia had a neighbourhood,
- 1:33:55the Shapleigh Supercluster would be its nearest significant neighbour, and
- 1:34:01the relationship between them is not simple. The Shapleigh Supercluster
- 1:34:07sits roughly six hundred fifty million light years away, That
- 1:34:13is several hundred million light years further out than the
- 1:34:16Greater Tractor, which already sits one hundred fifty to two
- 1:34:21hundred fifty million light years from the Milky Way. By
- 1:34:26any measure, Shapley is distant, but distant does not mean irrelevant.
- 1:34:33Shapley is one of the most massive concentrations of matter
- 1:34:37in the observable universe, and its gravitational influence reaches far
- 1:34:42beyond its own boundaries. When astronomers began measuring the peculiar
- 1:34:48velocities of galaxies throughout and around Laniakia, something strange kept
- 1:34:54showing up in the data. The greater tractor was not
- 1:34:58just pulling nearby galaxy toward itself, it was also moving.
- 1:35:04The entire gravitational center of Laniakia was drifting, being pulled
- 1:35:09in Shapley's direction. This is where the picture gets complicated.
- 1:35:15Laniakia was defined as a basin of attraction, a region
- 1:35:19where galaxy motions converge inward toward a shared gravitational center.
- 1:35:25That definition worked cleanly within its mapped boundaries. But the
- 1:35:30greater tractor at Laniakia's core is itself part of a
- 1:35:34larger flow. Something with even more mass is pulling on
- 1:35:39it from further out. The Shapley concentration, as astronomers sometimes
- 1:35:45call it, generates a gravitational pull strong enough to tug
- 1:35:50on a structure containing one hundred quadrillion solar masses, which
- 1:35:55raises a real question. Is Laniakia truly an independent basin
- 1:36:01or is it a smaller valley inside a larger one,
- 1:36:04one that drains ultimately towards Shapley. There is no clean
- 1:36:09answer yet. Some analyzes suggest Laniakia and the off Yucus
- 1:36:14cluster region form a combined basin that flows towards Shapleigh,
- 1:36:19which would make Laniakia a sub basin rather than a
- 1:36:23top level structure. Others maintain that the flow patterns are
- 1:36:27distinct enough to treat them separately. The boundary is fuzzy.
- 1:36:33That fuzziness is not a failure of science. It reflects
- 1:36:38the fact that the universe does not organize itself into
- 1:36:41tidy boxes. Gravity does not stop at the edges of
- 1:36:46whatever structure we choose to name. Then something else turned
- 1:36:50up entirely. In twenty twenty, a team of astronomers announced
- 1:36:55the discovery of a massive structure lying just beyond Laniakia's boundary.
- 1:37:01They called it the South Pole Wall. The name comes
- 1:37:05from its orientation in the sky, concentrated near the south
- 1:37:09celestial pole and extending outward in a great sweeping arc.
- 1:37:15The scale of it is hard to take in. The
- 1:37:18south Pole Wall stretches across roughly two hundred degrees of sky,
- 1:37:23more than a semicircle. It wraps around Laniakia like an arm.
- 1:37:29The densest part of the structure sits about five hundred
- 1:37:32million light years from the Milky Way, but following the
- 1:37:36arc northward, it curves inward to within three hundred million
- 1:37:40light years of us. It is not some distant background feature,
- 1:37:46it is immediately adjacent. What makes the south Pole Wall
- 1:37:50particularly striking is how long it went unnoticed. Part of
- 1:37:55the answer is the zone of avoidance. A significant porsche
- 1:38:00of this structure lies behind the galactic plane, hidden behind
- 1:38:04the dust and gas of the Milky Way. The tools
- 1:38:08that revealed it, the same peculiar velocity mapping technique used
- 1:38:13to define lania KaiA, are better at seeing through that
- 1:38:16obstruction than optical surveys. The South Pole Wall is a
- 1:38:22reminder that Laniakia does not float in empty space. It
- 1:38:27sits within a rich, dense cosmic environment, bordered by enormous
- 1:38:32structures that we are still in the process of cataloging.
- 1:38:36In twenty twenty three, a study using the Cosmic Flow's
- 1:38:40four catalog pushed this work further. Cosmic Flows four contains
- 1:38:46distances for nearly fifty six thousand galaxies compared to the
- 1:38:50eight thousand, one hundred used in the original two thy
- 1:38:54fourteen Laniakia paper. With that much more data, the wa
- 1:39:00watershed technique could be applied at larger scales and with
- 1:39:04better precision. The result was a map that confirmed Laniakia's
- 1:39:09size and shape and simultaneously identified five neighbouring superclusters using
- 1:39:15the same method. Those neighbours are Shapley, Perseus Pisces, Hercules, Leapus,
- 1:39:22and APUs. Each one is a distinct gravitational basin in
- 1:39:27its own right, a region where galaxy motions converge inward,
- 1:39:32just as they do within Laniakia. Each one is enormous,
- 1:39:36and each one sits adjacent to Laniakia in a way
- 1:39:40that makes the entire local region of the universe feel
- 1:39:44increasingly crowded and interconnected. Perseus Pisces is one of the
- 1:39:50largest concentrations of matter in the nearby universe, a long,
- 1:39:56filamentary structure stretching across hundreds of millions of light years
- 1:40:01in a completely different direction from Shapley Hercules sits further out,
- 1:40:08a less concentrated but still massive structure. Lepus and APUs
- 1:40:13are less studied, less well characterized, identified primarily through the
- 1:40:19flow signatures in the cosmic flows for data, rather than
- 1:40:23through dense optical surveys. These are not minor footnotes. They
- 1:40:29are superclusters, and Laniakia sits among them, not at the
- 1:40:34edge of organized structure, but deep inside a web of it.
- 1:40:39This brings in the Pisces Setus supercluster complex. This is
- 1:40:43an even larger organizational level, a structure that contains Laniakia, Perseus,
- 1:40:49Pisces Cetus, and several other components in a single elongated
- 1:40:55complex stretching across roughly a billion light years. The Pisce's
- 1:41:00Cetus complex is among the largest known structures in the
- 1:41:04observable universe. Laniakia is its inner component, its central region,
- 1:41:11which means the structure we spent so much effort defining,
- 1:41:15the one that took decades of observational work to map,
- 1:41:19is itself a neighborhood inside something far larger. There is
- 1:41:24a pattern here. Before twenty fourteen, our largest named home
- 1:41:30was the Virgo supercluster. Then Lanyakia absorbed it and grew
- 1:41:35the answer by a factor of five in diameter. Now,
- 1:41:39Laniakia sits inside the Pisce's Cetus complex and flows towards Shapley.
- 1:41:45Each time astronomers step back and look at a larger volume,
- 1:41:49The structure does not end. It continues. New walls, new clusters,
- 1:41:56new basins of attraction keep appearing at the edges of
- 1:41:59whatever app was just completed. This is not a coincidence.
- 1:42:04It is what the physics predicts. Gravity has been operating
- 1:42:08on matter for thirteen billion years, pulling density enhancements into
- 1:42:13galaxy clusters, pulling clusters toward each other along filaments, pulling
- 1:42:19superclusters into still larger flows. There is no obvious scale
- 1:42:25at which this process terminates. The cosmic web extends across
- 1:42:30the entire observable universe ninety three billion light years in diameter,
- 1:42:36and on that scale, the largest structures observable are only
- 1:42:41a small fraction of the whole. Laniakia, at five hundred
- 1:42:46twenty million light years, is enormous by human standards and
- 1:42:50unremarkable by universal ones. What lies beyond Laniakia, then, is
- 1:42:56not emptiness. It is more structure, more flow, more mass
- 1:43:01concentrations pulling on each other across distances that make Laniakir
- 1:43:06itself look modest. The south pole wall wraps around it shaply,
- 1:43:12pulls on it from one direction. Perseus Pisces anchors a
- 1:43:17different gravitational basin nearby. The cosmic Flows four catalog has
- 1:43:22already pushed the frontier outward, and the catalogs that follow
- 1:43:26will push it further still. Every boundary we draw around
- 1:43:31our cosmic home turns out to have something larger just
- 1:43:35outside it. From far enough out, the universe looks like
- 1:43:39a net, not a metaphor, not a poetic approximation. When
- 1:43:46astronomers map the distribution of galaxies across hundreds of millions
- 1:43:50of light years, the actual image that comes back looks
- 1:43:55like a three dimensional mesh, bright filaments running between dens
- 1:44:00its nodes, with vast dark holes where almost nothing lives.
- 1:44:05Superclusters sit at the intersections, filaments run between them, and
- 1:44:11the space in between. Most of the volume of the
- 1:44:15universe is nearly empty. This is the cosmic web, and
- 1:44:20Laniakia is one small piece of it. The scale of
- 1:44:25the observable universe is roughly ninety three billion light years
- 1:44:29across Laniakia spans about five hundred twenty million light years
- 1:44:36do the math our entire supercluster, with its one hundred
- 1:44:41thousand galaxies and mass equivalent to one hundred quadrillion suns,
- 1:44:46occupies less than one percent of the observable universe's diameter.
- 1:44:51Drop it into the full cosmic map, and it becomes
- 1:44:55difficult to find. The web extends in every direction, repeating
- 1:45:00its pattern of filaments and voids and dense nodes all
- 1:45:04the way to the edge of what we can see.
- 1:45:07Laniakia is one node in that pattern. Nothing about its
- 1:45:12location is obviously special, nothing marks it as unusual among
- 1:45:17the thousands of similar structures scattered across the cosmic map.
- 1:45:22The voids are the part that most people don't expect.
- 1:45:26When you picture the universe packed with galaxies, you are
- 1:45:30picturing the bright parts, the filaments and clusters. But the voids,
- 1:45:36those enormous dark regions between the filaments, are not exceptions
- 1:45:41to the rule. They are the rule. The voids dominate.
- 1:45:47A single void can stretch one hundred to three hundred
- 1:45:50million light years across some of the largest the supervoids
- 1:45:56are even bigger. The density inside them is less than
- 1:46:00a tenth of the average density of the universe. Galaxy
- 1:46:04after galaxy, cluster after cluster, essentially nothing for hundreds of
- 1:46:10millions of light years in any direction. The universe, by volume,
- 1:46:15is mostly darkness. The bright web we trace is a
- 1:46:20thin skeleton stretched across an enormous emptiness. What makes this
- 1:46:25structure strange is that it was predictable. Scientists did not
- 1:46:30discover the cosmic web by looking at the sky and
- 1:46:33then scrambling to explain what they saw. They predicted it
- 1:46:37first from the mathematics of gravity and the initial conditions
- 1:46:42of the early universe, and then confirmed it through observation.
- 1:46:47The Millennium simulation, run in two thousand five by a
- 1:46:51team including Folka, Springle and hundreds of collaborators, started with
- 1:46:57conditions matching the early universe and ran gravity forward across
- 1:47:02thirteen billion years of simulated time. The result was a
- 1:47:07filamentary web of structure that matched the observed distribution of
- 1:47:12galaxies with uncomfortable precision. Uncomfortable because nothing about the early
- 1:47:19universe looked like it was headed toward this. The early
- 1:47:23universe was almost perfectly smooth, almost not quite The temperature
- 1:47:29variations in the cosmic microwave background are tiny one part
- 1:47:34in one hundred thousand, but they were there baked into
- 1:47:38the universe by quantum fluctuations in the first fraction of
- 1:47:41a second. After the Big Bang. Inflation stretched those quantum
- 1:47:46variations to macroscopic scales. Gravity did the rest. Regions that
- 1:47:53were slightly denser than average pulled in more matter. Regions
- 1:47:58that were slightly less dense long lost matter to their neighbours.
- 1:48:02Over hundreds of millions of years, the slight variations grew,
- 1:48:07dense regions became filaments, The densest intersections of filaments became
- 1:48:13clusters and superclusters. The under dense regions became voids. The
- 1:48:19same process, operating on the same initial conditions produces the
- 1:48:24same web pattern every time you run the simulation. The
- 1:48:27cosmic web is not accidental. It is the inevitable output
- 1:48:32of simple physics applied to a nearly uniform starting state.
- 1:48:37The Illustrious simulation and its successor Illustrious TNNG pushed this further.
- 1:48:45These models incorporated not just gravity, but gas dynamics, star formation,
- 1:48:51black hole feedback, and the influence of dark energy. The
- 1:48:56resulting simulated universes looked at large scale almost indistinguishable from
- 1:49:02what we observe. Filaments in the right places, voids of
- 1:49:07roughly the right size, clusters of roughly the right mass.
- 1:49:13The match is not perfect. There are still open questions
- 1:49:17about the precise distribution of matter on small scales, but
- 1:49:22the broad architecture of the cosmic web has been reproduced
- 1:49:26repeatedly from first principles. This is one of the more
- 1:49:30remarkable facts in all of modern cosmology. The largest structures
- 1:49:35we can observe were written into the universe before the
- 1:49:39first star ever formed. Laniakia sits in this web the
- 1:49:44way any other supercluster does. It is a gravitational basin,
- 1:49:49a node where filaments converge and matter has pooled over
- 1:49:54billions of years. On the full cosmic map, at the
- 1:49:58scale where lania Kaya becomes a recognizable object, dozens of
- 1:50:03similar structures are visible in every direction. The Shaply supercluster,
- 1:50:08the Perseus Pisces chain, the Hercules supercluster, each one a
- 1:50:14basin like Laniakia, each one pulling its local collection of
- 1:50:18galaxies inward, each one connected to its neighbours by filaments
- 1:50:23and separated by voids. The cosmic web at this scale
- 1:50:28looks almost biological dense nodes connected by thin, bright threads
- 1:50:34vast dark cavities in between. If you have ever seen
- 1:50:39an image of neurons under a microscope, or a leaf's
- 1:50:42vein structure, or the foam that forms when soap bubbles
- 1:50:46crowd together, those images all resemble the cosmic web for
- 1:50:52the same mathematical reason that different physical systems driven by
- 1:50:57similar branching processes tend to produce similar geometric patterns. There
- 1:51:03is nothing cosmologically remarkable about Laniakir's position in this web.
- 1:51:08It is not at the center of anything. It is
- 1:51:11not the most massive node within reach. It is one
- 1:51:15of many similar structures spread across a universe that extends
- 1:51:19unimaginably far beyond what any current telescope can probe. The
- 1:51:25only thing that makes Laniyakir unusual is our location inside it.
- 1:51:30Because we are here, we can study it in detail
- 1:51:33that is impossible for any other supercluster. We know its shape,
- 1:51:38its mass, its internal flows, the positions of its major clusters,
- 1:51:44the behavior of its filaments. We have mapped it at
- 1:51:48a resolution no other supercluster will achieve in any telescope
- 1:51:53that currently exists. That is the advantage of being inside
- 1:51:58something rather than looking at it from across the universe.
- 1:52:03Laniakia is one knot in that net, not special in
- 1:52:07any obvious cosmological sense, but the knot we happen to
- 1:52:11be able to examine from the inside. One of the
- 1:52:15earliest clues that something was pulling our region of the
- 1:52:19universe came not from counting galaxies, but from measuring temperature.
- 1:52:25In the nineteen seventies, when physicists first mapped the cosmic
- 1:52:30microwave background in fine detail, they expected to find something
- 1:52:35close to uniform. The CMB is the afterglow of the
- 1:52:39Big Bang light released roughly three hundred eighty thousand years
- 1:52:45after the universe began, now cool to just a few
- 1:52:49degrees above absolute zero, arriving at our detectors from every
- 1:52:55direction in the sky. If the universe were perfectly smooth,
- 1:53:00and we were sitting still relative to that background, the
- 1:53:04temperature would be essentially the same in every direction. It
- 1:53:08is not. One side of the sky runs slightly warmer,
- 1:53:12the opposite side runs slightly cooler. The difference is tiny,
- 1:53:18on the order of a thousandth of a degree, but
- 1:53:21it is real, clean and impossible to ignore that asymmetry
- 1:53:26is called the CMB dipole, and what it tells you
- 1:53:30is motion. When you move toward a source of light,
- 1:53:33the waves compress slightly and shift toward higher energy, higher temperature,
- 1:53:39move away, and they stretch, cooling down. The dipole in
- 1:53:44the CMB is a Doppless signature. Our entire region of
- 1:53:49the universe is moving, moving fast, roughly six hundred kilometers
- 1:53:54per second relative to the background radiation that fills all
- 1:53:58of space. That the number raised an immediate question. Six
- 1:54:02hundred kilometers per second is not slow. It is not
- 1:54:06something you can attribute to the gravity of a nearby
- 1:54:09galaxy cluster or even a modest supercluster. Something with enormous
- 1:54:15gravitational pull had to be responsible, and when astronomers tried
- 1:54:20to account for all the known mass in the local universe,
- 1:54:24all the visible galaxy clusters within a few hundred million
- 1:54:28light years, they could not explain it. The pull of
- 1:54:33known structures was not enough. There was a missing source.
- 1:54:38That gap was one of the first signs pointing toward
- 1:54:42what would eventually be called the Greater tractor, the gravitational
- 1:54:48engine sitting near the center of Laniakir, pulling our local
- 1:54:52group and thousands of other galaxies toward a common point
- 1:54:57hundreds of millions of light years away. What made this
- 1:55:01early evidence particularly strange was that the bulk flow was
- 1:55:05not just ours. Individual galaxies near by were showing anomalous
- 1:55:10velocities in the same general direction. Galaxy clusters across a
- 1:55:16wide region of space were all drifting toward the same
- 1:55:19part of the sky, faster than the cosmic expansion alone
- 1:55:24could explain. This is what peculiar velocities look like in practice,
- 1:55:30not random noise scattered in all directions, but a coherent
- 1:55:35drift a tide millions of galaxies all leaning the same way.
- 1:55:41The CMB dipole was the loudest signal, but the galaxy
- 1:55:46velocities were the conformation that the effect was real and widespread.
- 1:55:52The problem with early peculiar velocity data was that it
- 1:55:56depended entirely on galaxy distance measurements that carry their own uncertainties.
- 1:56:02If your distances are slightly wrong, your inferred velocities are wrong.
- 1:56:08A pattern that looks coherent might dissolve under better measurements.
- 1:56:13Astronomers needed a way to check the velocity field independently,
- 1:56:18using a completely different physical process that check eventually arrived
- 1:56:23in the form of a phenomenon called the kinetic Sunyayev
- 1:56:26Zeldevich effect. Here is the basic picture. Galaxy clusters contain
- 1:56:32enormous clouds of hot gas plasma at tens of millions
- 1:56:36of degrees, threaded through the space between individual galaxies. When
- 1:56:42CMB photons travel through this hot gas, they interact with
- 1:56:47the fast moving electrons. If the cluster itself is moving
- 1:56:51relative to the CMB rest frame, this interaction leaves a
- 1:56:55subtle imprint on those photons moving toward us. The cluster
- 1:57:01slightly boosts the energy of passing photons moving away, it
- 1:57:06slightly reduces it. The effect is extraordinarily small. Detecting it
- 1:57:13requires precise microwave observations, careful subtraction of other signals, and
- 1:57:19large statistical samples of clusters. But it is physically distinct
- 1:57:24from anything in the galaxy distance measurements, no Tully fissure relations,
- 1:57:30no fundamental pe Lane corrections, no distance ladder, just microwave
- 1:57:37photons and hot gas and the Doppler shift of a
- 1:57:40moving cluster read directly from the sky. When researchers began
- 1:57:45applying kinetic sunya of Zeldevich measurements to galaxy clusters across
- 1:57:49the local universe. The results were striking. The clusters showed
- 1:57:54bulk motion, not random velocities pointing in scattered directions, but
- 1:58:00a coherent flow in roughly the direction of the greater tractor,
- 1:58:05consistent with what the peculiar velocity surveys had been showing
- 1:58:09for decades. This was not a marginal overlap. The independent probe,
- 1:58:16built on entirely different physics, pointed toward the same gravitational
- 1:58:21basin that Tully's watershed analysis had defined using galaxy flows.
- 1:58:26What this convergence means is important. A recurring concern whenever
- 1:58:32a large scale structure gets mapped from peculiar velocities is
- 1:58:37that the result might be an artifact, a product of
- 1:58:41which galaxies happened to be measured, that surveys covered, which
- 1:58:46parts of the sky, which distance methods were applied. Lanyakir
- 1:58:51was defined using a specific catalog of roughly eight thousand galaxies,
- 1:58:57that is, a finite sample with finite coverage. If the
- 1:59:01pattern were statistical noise, independent probes using different physics on
- 1:59:07different objects should produce a different picture. They do not.
- 1:59:12The CMB dipole. The bulk flow studies of the nineteen
- 1:59:17eighties and nineteen nineties, the kinetic Sunyayev Zeldovich measurements from
- 1:59:23large microwave surveys all describe the same motion across the
- 1:59:28same enormous volume of space. Multiple independent methods of measuring
- 1:59:33motion at cosmic scales now point toward the same picture,
- 1:59:38a coherent flow of galaxies across hundreds of millions of
- 1:59:43light years converging on the same gravitational basin. We do
- 1:59:48not live near the heart of Lanyakir. The Milky Way
- 1:59:53sits out near the edge, somewhere on the outer rim
- 1:59:57of a structure five hundred twenty million light years across,
- 2:00:01pulled slowly but measurably toward the gravitational center. Slowly is
- 2:00:07the key word. The distance between us and the greater
- 2:00:12tractor is somewhere between one hundred fifty and two hundred
- 2:00:16fifty million light years at our current in full velocity,
- 2:00:21reaching it would take far longer than the current age
- 2:00:24of the universe, and dark energy will almost certainly intervene
- 2:00:30before any arrival is possible. So we are falling inward technically,
- 2:00:35but we are never going to get there we are
- 2:00:38permanent residents of the outskirts. What would it look like
- 2:00:42to live somewhere else. Imagine the Milky Way had formed
- 2:00:47closer to the dense core of Lania Ka, near one
- 2:00:51of the major clusters at the heart of the structure.
- 2:00:55The sky would look different in ways that are hard
- 2:00:57to fully picture. Galaxy density near the center is dramatically higher.
- 2:01:04Neighboring galaxies would be closer. Interactions and mergers between galaxies
- 2:01:11happen far more frequently in dense environments, and those collisions
- 2:01:16drive bursts of star formation, reshape spiral arms, heat the
- 2:01:21surrounding gas, and feed supermassive black holes into periods of
- 2:01:25intense activity. A galaxy in that environment would be a
- 2:01:30different kind of place, noisier, more active, more frequently disrupted.
- 2:01:37The quiet spiral structure of the Milky Way, which has
- 2:01:40remained relatively undisturbed for billions of years, is partly a
- 2:01:45product of where we ended up. The outskirts are calm
- 2:01:49out here, the galaxy density drops in some directions. The
- 2:01:55voids open up regions tens of millions or hundreds of
- 2:01:59million millions of light years across where almost nothing lives.
- 2:02:04These are not empty in an absolute sense, but the
- 2:02:07density of matter is less than a tenth of the
- 2:02:10universe's average, and galaxies in voids are rare and isolated things.
- 2:02:17We have voids opening up around us in certain directions
- 2:02:20right now. The local group is not completely alone, but
- 2:02:25it is a small association of galaxies in a relatively
- 2:02:29sparse region far from the nearest major cluster. That is
- 2:02:34just the reality of living on the periphery of a supercluster.
- 2:02:39The closest large cluster to us, the Virgo cluster, is
- 2:02:44still fifty to sixty million light years away. In cosmic terms,
- 2:02:50that is a neighbour. In any other terms, it is
- 2:02:54an almost meaningless distance. There is something worth sitting with here.
- 2:03:00The fact that we ended up in this particular location,
- 2:03:03on the quiet edge rather than the turbulent core, is
- 2:03:07not a coincidence in the way luck is a coincidence.
- 2:03:12It is the outcome of processes that were set in
- 2:03:15motion almost fourteen billion years ago, and this is where
- 2:03:20the story gets genuinely strange. The structure of Laniakia, the
- 2:03:25reason the Greater Tractor exists where it does, the reason
- 2:03:30the Milky Way formed in the specific region of space
- 2:03:33it occupies. All of it traces back to conditions in
- 2:03:37the first fractions of a second after the Big Bang.
- 2:03:41The early universe was almost perfectly uniform. Almost There were
- 2:03:47tiny fluctuations in density, variations so small that the temperature
- 2:03:53difference they created in the cosmic microwave background is measured
- 2:03:57in hundred thousandths of a degree. These fluctuations were not
- 2:04:02random in the classical sense. They were quantum mechanical. At
- 2:04:07the smallest scales, imaginable quantum uncertainty produces unavoidable variations in
- 2:04:14energy density in the very early universe. During the period
- 2:04:19cosmologists call inflation, space expanded so violently and so fast
- 2:04:26that those microscopic quantum fluctuations were stretched to cosmic scales.
- 2:04:32A variation that existed across a distance smaller than a
- 2:04:35proton became after inflation, a variation spread across what would
- 2:04:41eventually be millions of light years. T He universe locked
- 2:04:46those fluctuations in as it expanded. Gravity did the rest.
- 2:04:51Over billions of years. Regions that were even slightly denser
- 2:04:55than average pulled in surrounding matter. The denser they got,
- 2:05:00the more they pulled, the emptier regions got emptier. As
- 2:05:05matter drained away toward the denser ones, What started as
- 2:05:09a near uniform gas of hydrogen and helium slowly organized
- 2:05:14itself into the cosmic web filaments and clusters and voids
- 2:05:19over time, scales measured in billions of years. The greater Tractor,
- 2:05:25the dense concentration of mass at the heart of Laniaka,
- 2:05:29formed because gravity amplified a slight over density that had
- 2:05:34its origin in a quantum event that happened before a
- 2:05:37single atom existed. That is not a small claim. The
- 2:05:42reason the Milky Way is where it is, the reason
- 2:05:46we are on the outskirts of this particular structure rather
- 2:05:49than somewhere else, traces back to a quantum fluctuation that
- 2:05:55was inflated to cosmic scales before the universe was a
- 2:05:59second old. There was no inevitability to the specific location.
- 2:06:05If the fluctuations had been arranged slightly differently, the large
- 2:06:10scale structure would have assembled differently. The Greater Tractor would
- 2:06:15be somewhere else, the Milky Way would be somewhere else.
- 2:06:21The whole map changes with tiny differences in those initial conditions.
- 2:06:27We are here because of randomness that occurred at the
- 2:06:30very bottom of physical reality. And was then enlarged to
- 2:06:35a scale of hundreds of millions of light years. This
- 2:06:38is not philosophy drifting away from the science. It is
- 2:06:42the science. Cosmologists can take the measured fluctuations in the
- 2:06:47cosmic microwave background, run them forward through simulations using known physics,
- 2:06:54and reproduce structures that look like the cosmic web we
- 2:06:57actually observe. Emulations produce filaments, voids, clusters, and superclusters in
- 2:07:06roughly the right proportions and at roughly the right scales.
- 2:07:10The structure is predictable. The specific arrangement is not. The
- 2:07:17quantum randomness of the earliest moments of the universe, amplified
- 2:07:22by gravity over thirteen billion years is what put us
- 2:07:26where we are, on the quiet edge of an immense heaven.
- 2:07:32If you wanted to write out where you live in
- 2:07:34the most complete way possible, the address would be longer
- 2:07:38than most people expect. Start with the obvious part. Earth
- 2:07:44a rocky planet about eight thousand miles across, orbiting an
- 2:07:49average star roughly ninety three million miles away. That star
- 2:07:54is the Sun, and the Sun sits inside a solar
- 2:07:57system that stretches roughly foa to five light hours out
- 2:08:01to Neptune, and considerably further if you count the loose
- 2:08:06halo of comets at its outer edge. That whole region,
- 2:08:11every planet, every moon, every chunk of rock and ice
- 2:08:16that gravitationally belongs to our star fits inside a bubble
- 2:08:21perhaps two light years across at its most generous estimate.
- 2:08:26That is your street address, a two light year bubble
- 2:08:30in a cosmos ninety three billion light years wide. Step outward,
- 2:08:37the Sun is one of somewhere between two hundred and
- 2:08:39four hundred billion stars in the Milky Way galaxy. The
- 2:08:44Milky Way is a barred spiral, a flat rotating disc
- 2:08:49about one hundred thousand light years across and roughly one
- 2:08:53thousand light years thick through much of its disk. The
- 2:08:57Sun sits about twenty six thousand light years from the
- 2:09:01galactic centre, out in one of the spiral arms, in
- 2:09:06a fairly quiet and unremarkable neighbourhood. The Solar System is
- 2:09:11so small compared to the Milky Way that if you
- 2:09:15shrunk the galaxy to the size of North America, the
- 2:09:19entire Solar system would be smaller than a dime. The
- 2:09:23Milky Way is your city, and it is already almost
- 2:09:28incomprehensibly large, but the Milky Way is not alone. It
- 2:09:33belongs to a collection of galaxies called the Local Group,
- 2:09:37a gravitationally bound cluster of roughly eighty known galaxies spread
- 2:09:43across approximately ten million light years. Most of these eighty
- 2:09:48galaxies are small. The dominant members are the Milky Way
- 2:09:53and Andromeda, two large spirals falling toward each other at
- 2:09:57several hundred kilometers per second and expected to collide in
- 2:10:02about four billion years. The Local Group is your region,
- 2:10:08your county. If you're keeping the metaphor, running ten million
- 2:10:12light years is one hundred times the width of the
- 2:10:15Milky Way, hold that ratio in your head, because it
- 2:10:20is about to repeat itself. The Local Group is one
- 2:10:25small cluster among many in the Virgo Supercluster. This structure,
- 2:10:30which astronomers had considered our home supercluster for decades before
- 2:10:35twenty fourteen, stretches roughly one hundred million light years across.
- 2:10:42It contains something on the order of one hundred galaxy
- 2:10:46groups and clusters. The Virgo Cluster itself a dense concentration
- 2:10:52of several thousand galaxies, sitting roughly fifty to sixty million
- 2:10:57light years from the Milky Way anchors the structure. The
- 2:11:03Virgo supercluster is ten times wider than the local group.
- 2:11:08Each step outward in this address multiplies the scale by
- 2:11:12a factor that should feel staggering, but somehow keeps arriving
- 2:11:16as a routine number in the equations. This is part
- 2:11:20of what makes cosmic scales genuinely difficult. The jumps are
- 2:11:25not gradual, they are sudden and enormous. And then there
- 2:11:30is Laniakia. The Virgo supercluster, it turns out, is not
- 2:11:35a standalone structure. It is one subdivision, one lobe of Laniakia,
- 2:11:42the supercluster defined in twenty fourteen by tracing the gravitational
- 2:11:47flow of galaxies rather than just their density. Laniakia stretches
- 2:11:53five hundred twenty million light years across. It contains roughly
- 2:11:58one hundred thousand and large galaxies. Its total mass is
- 2:12:03something in the neighborhood of ten to the power of
- 2:12:06seventeen solar masses, which is one hundred quadrillion suns, a
- 2:12:11number that stops being a number and becomes a symbol.
- 2:12:16The Virgo supercluster, which felt enormous when it was considered
- 2:12:20the top of the hierarchy, is approximately one fifth the
- 2:12:25width of Laniakia. What we called the largest structure we
- 2:12:30belonged to was a suburb, a small neighbourhood in something
- 2:12:35vastly larger that nobody had successfully outlined until fairly recently.
- 2:12:41Beyond Laniakia, the address continues. The greater tractor at Laniakia's
- 2:12:47center is itself moving toward the Shapleigh Supercluster, several hundred
- 2:12:52million light years further out. Laniakia is likely part of
- 2:12:56the pissy Seatus supercluster complex, a structure so large it
- 2:13:01dwarfs even Laniakia. The south Pole wall wraps around Laniakia's
- 2:13:07edge like an arm. These structures together form part of
- 2:13:12the cosmic web, the large scale architecture of the observable universe,
- 2:13:18filaments of galaxies hundreds of millions of light years long,
- 2:13:23connecting nodes like Laniakia, surrounding voids up to three hundred
- 2:13:28million light years across, where almost nothing lives. The full
- 2:13:34observable universe spans roughly ninety three billion light years. Laniakia,
- 2:13:41at five hundred twenty million light years, represents less than
- 2:13:46one percent of that diameter. The challenge of communicating all
- 2:13:50of this is real. The human mind handles a few
- 2:13:53orders of magnitude comfortably. It can picture a city being
- 2:13:58larger than a neighbourhood, a country being larger than a city.
- 2:14:02But the jump from the Solar system to the Milky
- 2:14:05Way is a factor of roughly a billion in linear scale.
- 2:14:10The jump from there to Lania Kia is another factor
- 2:14:14of five million. These are not differences in degree. They
- 2:14:19are differences that exhaust the imagination. It is the same
- 2:14:24problem physicists face when trying to hold atoms and solar
- 2:14:28systems in the same mental picture simultaneously. The scale range
- 2:14:34is simply too large for intuition to carry without breaking.
- 2:14:39What astronomers mean when they talk about a cosmic address
- 2:14:43is something genuinely new in human history. For most of
- 2:14:47our existence as a species, the question of where exactly
- 2:14:51we sat in the universe had no real answer. The
- 2:14:55sky was overhead. Beyond that, the answers we stories. Even
- 2:15:02one hundred years ago, astronomers were still debating whether the
- 2:15:06Milky Way was the entire universe or just one of
- 2:15:10many island galaxies. The idea that those galaxies organized into groups, clusters,
- 2:15:17and superclusters came later. The idea that those superclusters were
- 2:15:23themselves components of even larger basins of gravitational attraction. Came
- 2:15:29later still, in twenty fourteen, in a paper in Nature,
- 2:15:34each generation has extended the address by one more line.
- 2:15:40This is not trivia. It is the most complete answer
- 2:15:43to the question of where we are that any human
- 2:15:46civilization has ever been able to give. Dark energy is
- 2:15:51the reason Laniakia will not survive. That sentence sounds dramatic,
- 2:15:56but it is just physics. To understand what it means,
- 2:16:01you have to understand what dark energy actually is. And
- 2:16:04the honest answer is that nobody fully does. What astronomers
- 2:16:10know is this. Dark energy is the dominant energy component
- 2:16:14of the universe, accounting for roughly sixty eight percent of everything.
- 2:16:20It does not clump, It does not interact with light
- 2:16:24or matter in any detectable way. It is invisible, massless,
- 2:16:29and spread perfectly uniformly across all of space. The only
- 2:16:35thing it appears to do is cause space itself to expand,
- 2:16:39and it does this with a persistence that nothing in
- 2:16:42the universe can overcome at large enough scales. For most
- 2:16:46of the twentieth century, physicists assumed the expansion of the
- 2:16:50universe was slowing down. This made intuitive sense. The Big
- 2:16:55Bang flung matter outward, gravity pulls matter together. Over time,
- 2:17:01gravity should gradually win, decelerating the expansion, the way a
- 2:17:06ball thrown upward gradually loses speed. The only real question
- 2:17:13was whether gravity would win completely, stopping the expansion and
- 2:17:18reversing it into an eventual collapse, or whether the universe
- 2:17:22would expand forever at a diminishing rate. Both options assumed
- 2:17:28the same direction, expansion slowing over time. Then, in nineteen
- 2:17:34ninety eight, two independent teams of astronomers studying distant Type
- 2:17:39one A supernova published results that were almost impossible to believe.
- 2:17:46The supernovae were fainter than they should have been. They
- 2:17:49were farther away than the models predicted. The expansion was
- 2:17:54not slowing down, It was speeding up. Space was not
- 2:17:59fighting groundvity to a standstill. Something was actively pushing it
- 2:18:03apart faster with every passing era. That discovery earned its
- 2:18:09lead researchers the Nobel Prize in Physics in twenty eleven,
- 2:18:14and it rewrote cosmology in a single year. The force
- 2:18:19responsible for this acceleration is what physicists called dark energy,
- 2:18:25a label that carries a lot of honesty in it.
- 2:18:28The word dark here means unknown. It is not dark matter,
- 2:18:33which at least has well understood gravitational effects. Dark energy
- 2:18:39is stranger than that. It behaves like a property of
- 2:18:42empty space itself, a baseline energy that the vacuum carries,
- 2:18:48sometimes called the cosmological constant, a term Einstein introduced and
- 2:18:54then famously abandoned, and then turned out to be correct
- 2:18:57about after all. As space expands, a new volume of
- 2:19:02empty space is created, the total amount of dark energy
- 2:19:06grows with it. This is why the expansion accelerates over time,
- 2:19:12rather than settling into a constant rate. More space means
- 2:19:16more dark energy, which drives more expansion, which creates more space.
- 2:19:22The feedback loop is slow by human standards, but relentless
- 2:19:26on cosmological time scales. Now Here is where Lania KaiA
- 2:19:31enters the picture. Gravity and dark energy are in a
- 2:19:35continuous contest, and which one wins depends on scale. On
- 2:19:41small scales, gravity wins easily. The atoms in your body
- 2:19:46are not being pulled apart by dark energy. Planets, solar systems, galaxies,
- 2:19:53even galaxy clusters. These are all gravitationally bound. The matter
- 2:19:59in them is low together tightly enough that the gentle
- 2:20:02outward pressure of dark energy is irrelevant. But as you
- 2:20:07move to larger and larger scales, gravity becomes weaker and
- 2:20:12dark energy becomes more significant. Superclusters occupy exactly the zone
- 2:20:18where this contest becomes interesting. Laniakia is not gravitationally bound.
- 2:20:25This was established when it was first defined in twenty fourteen,
- 2:20:30and it is worth sitting with. The structure is real,
- 2:20:34the galaxy flows are real, The inward motion toward the
- 2:20:38Greater Tractor is real. The basin of attraction exists, but
- 2:20:43the outer regions of Laniakia do not have enough gravitational
- 2:20:47connection to the center to resist the expansion of space indefinitely.
- 2:20:53The Greater Tractor exerts a genuine gravitational pull estimated at
- 2:20:59roughly ten mins, billion billion solar masses of influence that
- 2:21:03sounds enormous against dark energy operating across five hundred million
- 2:21:09light years. It is not enough. The outer galaxies of
- 2:21:14Laniakia are already in a kind of slow tug of
- 2:21:17war right now for our epoch of cosmic history. The
- 2:21:22gravity of the Greater Tractor remains strong enough to draw
- 2:21:26our local group and billions of nearby galaxies toward its basin.
- 2:21:32This infall will continue for billions of years, but the
- 2:21:37boundary of that influence is not fixed. As the universe
- 2:21:41expans and the distances between outer regions of Laniakia and
- 2:21:46its gravitational center grow, the gravitational force between them weakens.
- 2:21:53Dark energy's push does not weaken with distance the way
- 2:21:57gravity does, so the balance tip. Galaxies near Laniakia's periphery
- 2:22:03will eventually cross a threshold where expansion carries them away
- 2:22:08faster than gravity can draw them back. The filaments at
- 2:22:12the edges will thin, the outer clusters will drift. The
- 2:22:17structure will not collapse or explode. It will simply dissolve
- 2:22:22gradually and quietly over time scales that are hard to
- 2:22:27write down meaningfully. What does the far future universe actually
- 2:22:32look like? Astronomers have modeled this, and the picture is
- 2:22:37striking in its emptiness. The local group itself, the Milky
- 2:22:42Way Andromeda, and roughly eighty smaller companions, is bound. In
- 2:22:48several billion years, the Milky Way and Andromeda will merge
- 2:22:53into a single massive galaxy. That merge structure will remain
- 2:22:58gravitationally locked, but beyond the local group, the rest of
- 2:23:03Laniakir will gradually recede. The Virgo cluster will eventually pass
- 2:23:09beyond the boundary where gravitational connection is possible. The Hydra
- 2:23:15and Centaurus clusters, the Normer Cluster, the hundreds of groups
- 2:23:20that today participate in the infall toward the greater tractor,
- 2:23:25all of them will drift beyond reach on time scales
- 2:23:29of hundreds of billions of years. What remains will be
- 2:23:32isolated islands of gravitationally bound matter, separated from each other
- 2:23:38by expanding voids that grow wider with every passing eon.
- 2:23:43The universe will still exist, stars will still burn for
- 2:23:48a while. But the large scale structure we can see today,
- 2:23:52the filaments, the clusters, the flowing basins of attraction, the
- 2:23:58shape that Brent Tully's team apped in twoenty fourteen, none
- 2:24:03of that will be visible. An observer in that far
- 2:24:07future universe, looking outward from whatever remains of our local
- 2:24:11group would see nothing but darkness in all directions, no
- 2:24:17neighboring galaxies close enough to identify, no structure at all.
- 2:24:23The cosmic web will have stretched beyond any possible detection.
- 2:24:28Whatever civilization existed then would have no way of knowing
- 2:24:32that a supercluster had once surrounded them half a billion
- 2:24:37light years of galaxies flowing together in a coherent structure,
- 2:24:42with a name that meant immense heaven. In the far future,
- 2:24:47nothing observable will remain to show that hundreds of thousands
- 2:24:52of gala zis once flowed together toward a common center
- 2:24:56across half a billion light years of space. The five
- 2:25:00fourteen paper that named Laniakia was not the end of
- 2:25:03the story. It was more like the first reliable map
- 2:25:07of a territory that had previously been described only in rumours.
- 2:25:12Tully's team had used a catalog of roughly eight thousand,
- 2:25:15one hundred galaxies with measured distances and velocities. That number
- 2:25:20sounds large for a structure five hundred twenty million light
- 2:25:25years across, it is actually quite thin coverage, like trying
- 2:25:30to map an entire continent from a few hundred survey
- 2:25:33points scattered unevenly across it. The researchers knew this. The
- 2:25:39paper itself acknowledged the gaps. What they had produced was
- 2:25:44a framework, a first outline, and the work of filling
- 2:25:48it in had barely started. Cosmic Flows three came next,
- 2:25:54released in twenty sixteen. It pushed the galaxy count to
- 2:25:57around eighteen thousand. More galaxies meant denser sampling, which meant
- 2:26:03the flow patterns could be traced with finer resolution. The
- 2:26:07boundaries of Laniakia didn't collapse under the new data. The
- 2:26:12basic shape held, but the details shifted. Some filaments resolved
- 2:26:18more clearly. Some previously ambiguous regions near the edges snapped
- 2:26:23into focus. The watershed boundaries, which in the original paper
- 2:26:28had been somewhat blurry in certain directions, tightened in some
- 2:26:33places and softened in others. This is how science actually works,
- 2:26:40not a single revelation, but a slow accumulation of better measurements,
- 2:26:45each one adjusting the picture slightly. The twoenty fourteen map
- 2:26:51wasn't wrong, it was coarse then Cosmic flows four arrived
- 2:26:57in twenty twenty three, and the number jumped to nearly
- 2:27:01fifty six thousand galaxies, that is roughly seven times the
- 2:27:06original data set. Eight different distance measurement techniques fed into
- 2:27:10the catalog. The Tullyfisher relation for spiral galaxies, the fundamental
- 2:27:16plane for ellipticals, and several others all cross checked against
- 2:27:21each other. The result was a peculiar velocity map of
- 2:27:26the local universe with a level of detail that would
- 2:27:29have been unthinkable in twenty fourteen. The twoenty twenty three
- 2:27:35analysis confirmed Laniakia's overall size and shape five hundred twenty
- 2:27:42million light years across roughly one hundred thousand large galaxies mass,
- 2:27:48sitting around ten to the seventeenth solar masses. The original
- 2:27:53outline held, but the same watershed technique that had defined
- 2:27:58Laniakia in two twenty fourteen now revealed five neighboring superclusters
- 2:28:04incomparable detail, shaply, Perseus, Pisces, Hercules, Leapus, and APIs, each
- 2:28:12one its own basin of gravitational attraction, each one adjacent
- 2:28:17to Laniakia in the larger cosmic web. The local universe
- 2:28:22suddenly had neighbours with names and borders. There are debates,
- 2:28:26though not everyone agrees that Laniakia's boundaries are drawn in
- 2:28:30exactly the right places. Some researchers argue that the edges
- 2:28:35of the structure are sensitive to which galaxies are included
- 2:28:39in the catalog and how distances are weighted. At large radii,
- 2:28:45the zone of avoidance still creates real gaps in the data.
- 2:28:49Galaxies behind the Milky Way's disc are underrepresented in every
- 2:28:53version of cosmic flows, which means the flow maps in
- 2:28:57those directions are less reliable. If significant structures are hidden
- 2:29:03in those gaps, the boundary of Laniakia in that region
- 2:29:07of sky could shift when better data eventually fills the
- 2:29:10blind spot. These are not fatal objections. They are exactly
- 2:29:16the kind of edge case uncertainties you expect at the
- 2:29:19frontier of a measurement campaign. The core of the structure
- 2:29:24is solid, the edges are still being negotiated. What comes
- 2:29:29next is more data orders of magnitude. More spectroscopic surveys
- 2:29:36now underway or in planning will measure galaxy redshifts for
- 2:29:40tens of millions of objects. The Dark Energy Spectroscopic Instrument
- 2:29:46already operating in Arizona is accumulating galaxy spectra at a
- 2:29:51rate that would have seemed impossible a decade ago. Surveys
- 2:29:56like these won't just extend the cosmic flows approach, they
- 2:30:00will transform it. Peculiar velocity maps derived from millions of
- 2:30:05galaxies instead of tens of thousands will resolve structures that
- 2:30:10currently appear as vague suggestions in the data. The flow
- 2:30:15patterns around Laniakia's edges, where the supercluster's influence fades and
- 2:30:21the influence of neighboring structures takes over, will become far clearer.
- 2:30:26The extremely large telescope currently under construction in Chile's Attacama
- 2:30:31Desert will add something different. Its light gathering power is
- 2:30:36so far beyond existing instruments that it will be able
- 2:30:40to measure distances and velocities for galaxies that are simply
- 2:30:45too faint for current surveys to handle reliably. This reaches
- 2:30:51further out and fills in the picture at larger scales.
- 2:30:55Whether structures like the South Pole Wall, the enormous arc
- 2:31:00discovered in twenty twenty just beyond Laniakia connect to Lania
- 2:31:06Kia's flow patterns, or belong to entirely separate basins is
- 2:31:11exactly the kind of question that next generation instruments are
- 2:31:16positioned to answer. The map of our cosmic neighborhood is
- 2:31:21not finished. That might sound like a limitation, but it
- 2:31:25is also the honest state of things, and it means
- 2:31:29the most interesting results may not be the ones already published.
- 2:31:34Every time the catalog has expanded, something unexpected has appeared
- 2:31:39at the new resolution. More galaxies revealed cleaner filaments. Better
- 2:31:45coverage revealed neighboring superclusters that the original data could only
- 2:31:51hint at. There is no obvious reason to expect that
- 2:31:55pattern to stop. The outline that Tully's team drew in
- 2:31:59two thousand and four has held up, but the details
- 2:32:02inside it are still being filled in, and the territory
- 2:32:06just outside it keeps turning out to be larger than
- 2:32:08anyone expected. Every civilization that ever looked up at the
- 2:32:12sky had some answer to the question of where they
- 2:32:15were in it. The Babylonians placed themselves beneath the Dome
- 2:32:20of Gods. Medieval astronomers put Earth at the center of
- 2:32:24nested crystalline spheres. Polynesian navigators read the sky not as theology,
- 2:32:31but as a map, and they used it to cross
- 2:32:34the largest ocean on the planet, without instruments, without landmarks,
- 2:32:40without anything except an extraordinarily precise knowledge of the heavens
- 2:32:45above them. Every one of those civilizations had an answer.
- 2:32:51None of them had the right one. We are the
- 2:32:55first generation in human history that does. That answer is
- 2:33:00strange enough to stop you cold. If you sit with it,
- 2:33:04you are not at the center of your galaxy. You
- 2:33:07are not at the center of your galaxy cluster. You
- 2:33:10are not at the center of your supercluster. The Milky
- 2:33:15Way sits near the outer edge of Laniakia, in a
- 2:33:19relatively quiet, relatively sparse region, far from the dense clusters
- 2:33:24where galaxy interactions are frequent and the cosmic environment is violent.
- 2:33:31We are on the rim. We are in the suburbs
- 2:33:34of an immense structure that stretches five hundred and twenty
- 2:33:38million light years from one side to the other, and
- 2:33:42we are being slowly pulled toward its heart by a
- 2:33:46gravitational concentration so massive it took decades just to find it.
- 2:33:53That pool will never complete. Dark energy will likely win
- 2:33:58before we get anywhere near the center. We are drifting outward,
- 2:34:03even a as we fall inward, passengers in a structure
- 2:34:07that is quietly dissolving at its edges. And yet this
- 2:34:11unremarkable outpost is the only place, as far as anyone knows,
- 2:34:16where the question has ever been asked that asymmetry is strange.
- 2:34:22The Greater Tractor sits at the gravitational heart of lania KaiA,
- 2:34:27surrounded by some of the densest concentrations of galaxies in
- 2:34:32our cosmic neighborhood. Nobody there is asking anything. The rich
- 2:34:38clusters of the normous supercluster region, the dense nodes where
- 2:34:43filaments converge, silent, The vast empty voids that occupy most
- 2:34:49of Laniakia's volume silent. One minor spiral galaxy, far from
- 2:34:55anything particularly remarkable, produce the only observed us in the
- 2:35:00known universe who looked outward and wanted to understand the
- 2:35:04structure they were part of. That is not an answer
- 2:35:08to anything. It is just the fact, and the fact
- 2:35:13is strange. Think about what Tully's team actually did. The
- 2:35:17Polynesian navigators used the sky to find their place in
- 2:35:21the ocean. They read the stars, the swells, the flight
- 2:35:26paths of birds, and they triangulated themselves into a location.
- 2:35:31Tully's team did something that rhymes with that, but runs deeper.
- 2:35:35They didn't use the sky to find their place in
- 2:35:38the world. They used the motion of one hundred thousand
- 2:35:41galaxies to find their place within the structure that contains
- 2:35:45the sky itself. The navigators crossed the Pacific. The astronomers
- 2:35:51mapped the Pacific and discovered it was part of a
- 2:35:54continent they hadn't known existed. The Hawaiian name connects those
- 2:35:59two as across centuries, the same language, the same sky,
- 2:36:05an entirely different scale of understanding. What that understanding gives
- 2:36:11us is a complete address not just Earth, not just
- 2:36:15the Solar System, not just the Milky Way or the
- 2:36:19local group, but the full hierarchy extending outward to Laniakia
- 2:36:24and beyond. For most of human history, that address was
- 2:36:28unknown past the level of a few nearby stars. A
- 2:36:32century ago, we didn't know other galaxies existed. Fifty years ago,
- 2:36:38we didn't know what was pulling our region of the
- 2:36:40universe off course. Ten years ago, we didn't have a
- 2:36:44name for the supercluster we live in. The discovery is
- 2:36:48genuinely recent. The picture is genuinely incomplete. There are structures
- 2:36:54beyond Laniakia still being traced, boundaries still being debated, being
- 2:37:00extended from eight thousand galaxies to fifty six thousand, and
- 2:37:06eventually further still. The twoenty fourteen paper was a door opening,
- 2:37:13not a door closing. What sits on the other side
- 2:37:16of that door is uncomfortable and astonishing in equal measure.
- 2:37:22We are peripheral. We are temporary in the sense that
- 2:37:26the structure we belong to will not survive on cosmological
- 2:37:30time scales. The outer filaments of Laniakia are already losing
- 2:37:36coherence to dark energy. In hundreds of billions of years,
- 2:37:41the flows that define our cosmic home will disperse into
- 2:37:45an expanding void. Laniakia will not exist in any meaningful sense.
- 2:37:51The immense heaven will dissolve. This is not a reason
- 2:37:56for distress. It is just the physics. The structure was real,
- 2:38:01the flows were real. The answer to where we are
- 2:38:05is real, even if the structure itself is temporary. Somewhere
- 2:38:10on the outer rim of an immense heaven there is
- 2:38:13a small spiral galaxy, and on one of its unremarkable arms,
- 2:38:18something learned to ask where it was, and is only
- 2:38:22now beginning to find out