Latest / Boring Science / How Big Is TON 618 Really
Transcript
- 0:00Speaker 1: Light from this object takes over ten billion years to
- 0:03reach us. When you look at Ton six one eight,
- 0:08you're seeing something from when the universe was barely three
- 0:11billion years old. That single fact should tell you this
- 0:16isn't an ordinary black hole. We're going to explore the
- 0:20actual size of Ton six one eight, and I need
- 0:24to be clear from the start. The numbers involved will
- 0:27challenge your ability to comprehend scale itself. This isn't hyperbole.
- 0:33The human brain didn't evolve to grasp distances measured in
- 0:38hundreds of billions of kilometers or masses equivalent to sixty
- 0:42six billion suns. But we're going to try anyway, using
- 0:47every comparison and perspective shift we can muster. By the
- 0:51end of this journey, you'll understand why Ton six one
- 0:55eight represents one of the most extreme objects physics allows
- 1:00to exist. You'll see why it shouldn't exist at all
- 1:04according to some theories, and you'll grasp why astronomers sometimes
- 1:09go quiet when they talk about it, as if they've
- 1:12stumbled onto something the universe forgot to keep hidden. If
- 1:16you find comfort in these gentle explorations of space and science,
- 1:21I'd be grateful if you'd consider subscribing and giving this
- 1:24video alike. Let's start with where this monster lives. Ton
- 1:35six one eight sits near the border between two constellations
- 1:40you've probably never heard of, Caine's Vanatiche and Coma Berenicis.
- 1:46The distance is staggering in two different ways. The light
- 1:50we see left Ton six one eight roughly ten point
- 1:54eight billion years ago. That's the light travel time. But
- 1:59because because the universe has been expanding while that light
- 2:03journeyed toward us, the actual comoving distance is approximately eighteen
- 2:08point two billion light years. Think about what that means
- 2:13for a moment. When the light currently hitting our telescopes
- 2:18began its journey, Earth didn't exist, our Sun didn't exist.
- 2:24The Milky Way looked completely different. Dinosaurs were still four
- 2:29billion years in the future. But distance is just the
- 2:33opening act. The real story is what Ton six' one
- 2:37eight actually is. Ton six' one eight is classified as a,
- 2:42quasar specifically a hyper luminous broad absorption line radio loud.
- 2:48Quasar that's a mouthful of technical terms that each reveals something.
- 2:53Crucial strip away the jargon and you're left with this
- 2:59TO n six one eight is a supermassive black. Hole
- 3:04actively feeding on an enormous accretion disk of superheated, matter
- 3:09releasing more energy than most galaxies, combined while simultaneously blasting
- 3:15radio waves across the cosmos and driving powerful winds of
- 3:19material away from itself at thousands of kilometers per. Second
- 3:25the black hole at the center is where things get
- 3:28genuinely uncomfortable for our sense of. Scale mass estimates vary
- 3:33depending on which measurement technique you. Trust the higher, estimate
- 3:38widely cited in popular sources Puts ton six hundred eighteen
- 3:44at sixty six billion solar. Masses that's sixty six billion
- 3:49times the mass of Our. SUN a more recent twenty
- 3:53nineteen measurement using different spectral lines suggests forty point seven
- 3:58billion solar. Masses either, way we're talking about a black
- 4:03hole that contains more mass than all the stars in
- 4:07the Entire Milky way galaxy, combined which clock in at
- 4:11around sixty four billion solar. Masses let that settle this single.
- 4:18Object this one black hole has more mass packed into
- 4:22it than our entire galaxy's worth of. Stars to put
- 4:26this in, perspective compare it To, sagittarius a. Star the
- 4:30supermassive black hole at the center of our Own Milky.
- 4:34Way sagetarius a star weighs in at four point three
- 4:38million solar. Masses it's not small by any. Standard its
- 4:43event horizon would fit Inside mercury's. Orbit But ton six
- 4:49one eight is roughly fifteen, thousand three hundred times more.
- 4:54Massive If sagittarius a star is a, Marble ton six
- 4:59one eight is a beach, ball the size of a.
- 5:02House now let's talk about the physical, size because this
- 5:06is where your intuition completely. FAILS a black hole's size
- 5:11is defined by its Schwartz child, radius the distance from
- 5:15the center to the event, horizon that point of no
- 5:19return where even light cannot. Escape For ton six one,
- 5:24eight this radius measures approximately one, thousand three hundred astronomical.
- 5:29Units one astronomical unit is the distance From earth to The,
- 5:34sun roughly one hundred fifty million, kilometers so we're talking
- 5:40about one, thousand three hundred times that. Distance the event horizon,
- 5:45diameter the full width across is roughly two, thousand six
- 5:51hundred astronomical, units or about three hundred ninety billion. Kilometers
- 5:58let me give you a reference point that m might Help,
- 6:00neptune the most distant planet in our solar system orbits
- 6:05The sun at an average distance of thirty astronomical. Units
- 6:10pluto out in The Kuiper belt averages about forty astronomical.
- 6:14Units The Kuiper belt itself extends to roughly fifty astronomical.
- 6:20Units ton six one eight's event horizon extends more than
- 6:25forty times farther Than neptune's. Orbit you could fit our
- 6:30entire solar system from The sun out to The Kuiper
- 6:34belt inside tons six one eighths event horizon more than
- 6:38forty times over line up forty complete solar systems side by,
- 6:43side and you just about span the diameter of this
- 6:47black hole's point of no. Return still having trouble visualizing,
- 6:51it let's try. This light travels at two hundred ninety nine,
- 6:57thousand seven hundred ninety two kilometers per. Second at that,
- 7:02speed light takes about eight minutes to travel from The
- 7:05sun To. Earth it takes light about four hours to Reach.
- 7:09Neptune but to cross from one side of tons six
- 7:13to one eight's event horizon to the other would take
- 7:16light moving at the fastest speed possible in our. Universe several,
- 7:22WEEKS nasa created a visualization comparing black holes And when
- 7:27they Reached ton six one eight at the, end they
- 7:31noted that its shadow is so enormous that a beam
- 7:34of light would take weeks to traverse. It compare that
- 7:39TO m eighty, seven the famous black hole photographed by
- 7:43the event horizon. TELESCOPE m eighty seven's black hole contains
- 7:49about five point four billion solar, masses and light would
- 7:53take roughly two and a half days to cross its.
- 7:56Shadow ton six one eight is in a completely different.
- 8:01Category the sheer scale creates a bizarre situation if you
- 8:06could somehow Observe ton six one eight up, close which
- 8:11you absolutely could not. Survive but let's pretend the event
- 8:15horizon would look more like a wall or barrier stretching
- 8:19infinitely in all directions than a spherical. Boundary your human
- 8:25field of view couldn't encompass enough of it to perceive the.
- 8:28Curve it would just be a flat black surface extending
- 8:33beyond your visual horizon in every, direction with space itself
- 8:39warping so severely near it that the laws of physics
- 8:43as you understand them would cease to make intuitive. Sense
- 8:48here's something that might disturb. You if you were falling
- 8:51Toward ton six one, eight you could cross the event
- 8:55horizon without immediately noticing anything. Wrong the gravitational, gradient the
- 9:01difference in gravitational pull between your head and feet would
- 9:05be relatively gentle compared to smaller black. Holes you'd pass
- 9:11the point of no return still, intact still, conscious with
- 9:16no immediate sensation that anything had. Changed only, later as
- 9:22you continued, falling would tidal forces eventually tear you, apart
- 9:27but the crossing itself almost. Peaceful smaller black holes rip
- 9:32you apart before you reach the event. Horizon ton six
- 9:37one eight is so large that its event horizon is almost. Gentle,
- 9:43now let's consider what surrounds this. Monster Because tons six
- 9:47to one eight doesn't sit in empty, space quietly, existing
- 9:51it's violently. Active as a, Quasar ton six one eight
- 9:58is actively feeding matter spirals inward through an accretion, disc
- 10:03a swirling disc of gas and dust being pulled toward
- 10:07the event. Horizon as this material accelerates and, compresses friction
- 10:13heats it to extreme. Temperatures we're talking about millions of.
- 10:17Degrees in some. Regions the accretion disc itself would extend
- 10:22for light days or even light. Weeks from the black,
- 10:26hole this superheated matter releases radiation across the entire electromagnetic
- 10:32spectrum radio, waves, microwaves, infrared visible, light, ULTRAVIOLET x, rays gamma.
- 10:40Rays the amount of energy being released is almost. Incomprehensible
- 10:46ton six one eight shines with the luminosity of approximately
- 10:51four times ten to the fortieth power. Watts to put
- 10:55that in more familiar, Terms ton six one eight is
- 11:00one hundred forty trillion times brighter than Our, sun one,
- 11:04object outputting more light and energy than one hundred forty
- 11:09trillion suns. Combined the host galaxy Surrounding ton six one,
- 11:14eight and there must be one because quasers sit at
- 11:17the centers of, galaxies is completely outshone by the central.
- 11:21Quaser despite potentially containing hundreds of billions of, stars the
- 11:28galaxy is invisible From. Earth the black hole's accretion disc
- 11:34is so bright that the entire galaxy is lost in the.
- 11:38Glare gas is falling Into ton six one eight at
- 11:43speeds approaching seven thousand kilometers per. Second that's roughly two
- 11:48point three percent the speed of. Light material is being
- 11:52consumed at an enormous, rate converting mass to energy with terrifying.
- 11:58Efficiency some of this infalling gas has been measured moving
- 12:03at speeds up to ten, thousand five hundred kilometers per
- 12:07second about three point five per cent light, speed demonstrating
- 12:11the immense gravitational. Pull but not everything falls. In ton
- 12:18six one eight also drives powerful. Outflows it's classified as
- 12:22a broad absorption line, quasar meaning its spectrum shows evidence
- 12:27of strong winds being driven away from the black. Hole
- 12:32radiation pressure from the accretion disk is so intense that
- 12:36it literally blows material outward at thousands of kilometers per.
- 12:40Second these winds carry away significant amounts of matter and,
- 12:45energy potentially affecting star formation across the entire host. Galaxy
- 12:51ton six one eight is also radio, loud producing significant
- 12:56radio emissions from relativistic. Jets these are streams of charged
- 13:02particles accelerated to near light, speed shooting outward perpendicular to
- 13:08the accretion. Disk the jets carry enormous energy and extend
- 13:13far beyond the black hole, itself potentially reaching across hundreds
- 13:18of thousands of light. Years in twenty twenty, one observations
- 13:23from The Atacama Large Millimeter array revealed something, remarkable an
- 13:29enormous nebula of gas Surrounding ton six hundred eighteen and
- 13:34its host. Galaxy This liman alpha, blob as it's, called
- 13:39has a diameter of at least one hundred kilo, parsex
- 13:43about three hundred thirty thousand light. Years that's twice the
- 13:48diameter of our Entire Milky way. Galaxy this nebula consists
- 13:53of two, parts an inner molecular outflow and an extensive
- 13:58cold molecular gas in the circumgalactic. Medium each part has
- 14:03a mass of approximately fifty billion solar masses. Combined that's
- 14:09one hundred billion solar masses of, gas more massive than
- 14:14the black hole. Itself both components are aligned with the radio,
- 14:20jets suggesting the black hole's activity has shaped the distribution
- 14:25of gas on truly galactic. Scales this gas represents an
- 14:30enormous reservoir that could potentially fuel future star formation or
- 14:34be consumed by the black. Hole the extreme radiation From
- 14:39ton six hundred eighteen excites hydrogen in the nebula so
- 14:43intensely that it glows brightly in The liman alpha, line
- 14:48an ultraviolet. Wavelength the nebula's existence and structure provide crucial
- 14:55insights into how galaxies formed in the early universe and
- 14:59how supermassive black holes influence their. Surroundings the temperatures Within
- 15:06ton six one eighth immediate environment reach approximately thirty eight
- 15:11thousand degrees celsius in some, regions with the innermost parts
- 15:16of the accretion disc potentially reaching millions of. Degrees at these,
- 15:22temperatures atoms are completely ionized and matter exists in a plasma,
- 15:29state emitting intense. Radiation so that's the basic picture Of
- 15:34ton six hundred. Eighteen an ultra massive black, hole possibly
- 15:40the most massive ever directly, measured surrounded by a vast accretion,
- 15:44disc releasing energy equivalent to one hundred forty trillion, suns
- 15:49driving powerful jets and, winds embedded in a nebula twice
- 15:53the size of our, galaxy existing at a time when
- 15:57the universe was barely three billion years. Old but understanding the,
- 16:02scale really grasping, it requires more than just. Numbers in
- 16:08the next, section we're going to break down exactly what
- 16:12those numbers mean by Comparing ton six hundred eighteen to
- 16:16objects you can actually. Visualize we'll work our way up
- 16:21from familiar scales to the truly, cosmic building a ladder
- 16:26of comprehension that might actually let you grasp what sixty
- 16:31six billion solar masses really means because right, now even
- 16:36armed with all these, facts you probably can't truly picture.
- 16:40It that's what we need to. Fix let's start with
- 16:44something you understand. Yourself you're about one point seven meters,
- 16:51tall maybe a bit more or. Less hold that image,
- 16:56Now picture standing next to a blue whale thirty meters,
- 17:00long the largest animal ever to exist On. Earth you'd
- 17:04barely reach its. Eye that's a scale jump your brain can.
- 17:08Handle now take another leap The International Space, station orbits
- 17:14four hundred kilometers Above. Earth you'd need to stack two
- 17:18hundred thirty five thousand blue whales end to end to reach.
- 17:22It that's starting to get difficult to, visualize but you
- 17:27can still sort of imagine it because you've seen pictures
- 17:30Of earth from. Space The moon sits three hundred eighty
- 17:35four thousand kilometers, away nearly a thousand times farther than the.
- 17:40Miss here's where most people's intuition. Breaks The sun is
- 17:45one hundred fifty million kilometers From earth one astronomical. Unit
- 17:51that's the standard measuring stick for Our solar. System, neptune
- 17:57the outermost, planet orbits at the thirty astronomical, Units pluto
- 18:03wanders out to about forty astronomical units at its farthest.
- 18:07Point the Entire solar system you learned about in, school
- 18:12everything from mercury to The Kuiper belt fits comfortably within
- 18:16fifty astronomical. Units ton six one eight's event horizon has
- 18:22a radius of thirteen hundred astronomical. Units read that. Again
- 18:27the edge of this black, hole not the accretion, disc
- 18:32not the surrounding, nebula just the point of no return
- 18:35where even light can't, escape extends twenty six times farther
- 18:41Than pluto's. Orbit if you Place ton six' one eight
- 18:45where Our sun, sits its event horizon would swallow every,
- 18:49planet every, asteroid every, comet every piece of rock and
- 18:55ice in our Entire solar system and still extend outward
- 18:59INTO mp space for another twelve hundred and fifty astronomical.
- 19:04Units but that's just the event. Horizon that's not even
- 19:09the full. Picture remember that accretion disk we, discussed the
- 19:14glowing mailstrom of superheated matter spiraling into the black. Hole
- 19:19it would extend significantly, farther possibly light days or even
- 19:24light weeks from the event horizon. Itself we're talking about
- 19:28a structure so vast that light traveling at three hundred
- 19:32thousand kilometers per second would take days to cross from
- 19:36one side to the. Other let's try another. Angle. Mass
- 19:42Our sun contains ninety nine point eight six percent of
- 19:46all the mass in Our solar, System, Jupiter, saturn all
- 19:51the other, planets the asteroid, belt, everything their rounding. Errors
- 19:56compared to The, sun The sun is basically The solar
- 20:00system's mass. Budget ton six one eight contains sixty six
- 20:06billion times more mass than. That the Entire Milky way
- 20:10galaxy two hundred billion to four hundred billion, stars all
- 20:15the gas, clouds all the, dust all the planets orbiting
- 20:18all those, stars the super massive black hole at our galactic.
- 20:23Center everything has a total stellar mass of roughly sixty
- 20:27four billion solar. Masses ton six one eight a single
- 20:32object out masses every star in our galaxy. Combined sagittarius a.
- 20:38Star the black hole at The Milky way's center weighs
- 20:42four point three million solar. Masses it's massive enough to
- 20:47hold our galaxy together to orchestrate the orbits of billions of.
- 20:52Stars ton six one eight is fifteen, thousand three hundred
- 20:58times more. Mass when astronomers calculated these, numbers they had
- 21:03to double check their. Math the figures seemed. Wrong they
- 21:09still seem, wrong even though we verified them through multiple independent.
- 21:14Methods here's what really breaks your, brain light speed. Comparisons
- 21:22you probably know that light from The sun takes eight
- 21:24minutes and twenty seconds to Reach. Earth that's the light
- 21:28travel distance across one astronomical. Unit light From neptune takes
- 21:34about four hours to reach. Us the edge of our solar,
- 21:38system light needs about seven hours to get. Here from
- 21:42that far, Out ton six one eighths event horizon is
- 21:46so enormous that a beam of light would take weeks
- 21:49to traverse its, diameter not hours. Weeks the exact same
- 21:55light that crosses our entire solar system in seven hours
- 21:59would need more multiple weeks to travel Across ton six
- 22:02one eight. Shadow compare that TO m eighty Seven, star
- 22:07the black hole we actually imaged with the Event horizon
- 22:11telescope in twenty, nineteen humanity's first direct photograph of a black.
- 22:17Hole that object made headlines. Worldwide it weighs five point
- 22:23four billion solar, masses making it one of the largest
- 22:27black holes in the relatively nearby. Universe its shadow is
- 22:32so large that light takes about two and a half
- 22:35days to cross. It ton six one eight is more
- 22:39than ten times. LARGER nasa created a visualization scaling up
- 22:44from small black holes to the largest known. Ones the
- 22:48animation starts with black holes a few times The sun's,
- 22:52mass then jumps to progressively larger. Objects it works through
- 22:58dozens of intermediate black, holes steadily increasing in. SCALE m
- 23:04eighty Seven star appears near the end of this, progression
- 23:08dwarfing everything that came before. It the animation treats it
- 23:13as one of the final boss battles of cosmic. Scale
- 23:17Then ton six one eight, appears AND m eighty Seven
- 23:21star looks. Small let's ground this in something. Tangible imagine
- 23:27you're an astronaut Approaching ton six one. Eight you're not falling,
- 23:32In you're just flying past at a safe, distance maybe
- 23:36a few light years. Away you point your spacecraft toward
- 23:40it and start your approach at light. Speed at that,
- 23:43Distance ton six one eight would appear as a point of,
- 23:47light brighter than anything in the, sky but still point.
- 23:52Like as you get, closer it starts to. Resolve, first
- 23:58you'd see the accretion, disc a glowing spiral larger than
- 24:02any galaxy you've ever. Observed the light isn't, white it's
- 24:07shifted across the spectrum from the intense gravitational. Effects space
- 24:13around the black hole is so severely warped that light
- 24:16from behind it bends around to the, front creating a halo.
- 24:21Effect you'd see multiple distorted images of the accretion discs
- 24:26simultaneously layered over each other in impossible. Geometry you're still
- 24:32weeks away at light, speed weeks and the structure keeps
- 24:37growing in your field of. View the accretion disc resolves
- 24:41into spiral, arms each one a river of plasma hot
- 24:45enough to vaporize anything that touches. It you'd see the
- 24:49jets if you looked perpendicular to the, disk columns of
- 24:53matter accelerated to ninety nine point nine percent light, speed
- 24:59shooting outward for hundreds of thousands of light. Years but
- 25:04the event horizon, itself you still couldn't see it. Directly it's, black,
- 25:10perfectly absolutely, black because no light escapes. It you'd only
- 25:17see its silhouette against the accretion. DISC a spherical absence
- 25:21where the universe simply. Stops that absence would span thousands
- 25:27of astronomical. Units your entire solar system could fit in
- 25:31the gap between where the accretion discs glow ends and
- 25:35where space itself becomes visible again on the other. Side
- 25:39now consider this from another. Perspective ton six one eight
- 25:44formed when the universe was only three billion years. Old
- 25:49that's less than a quarter of the universe's current. Age,
- 25:53somehow in that cosmically brief, period this object accumulated sixty
- 25:58six billion solar. Masses that's not just, impressive it's theoretically.
- 26:03Problematic Black holes grow by accreting. Matter material spirals, inward heats,
- 26:10up radiates, energy and eventually crosses the event. Horizon but
- 26:15there's a natural speed limit to this, process called The eddington.
- 26:19Limit when matter falls into a black, hole it releases enormous.
- 26:25Energy that energy creates radiation pressure that pushes away additional infalling.
- 26:31Matter the more massive the black, hole the higher Its eddington.
- 26:36Luminosity but the relationship is. Linear double the, mass double
- 26:42the maximum accretion. Rate For tons six hundred eighteen to
- 26:47reach sixty six billion solar masses in three billion, years
- 26:52it would need to accrete matter at rates that challenge
- 26:55or exceed The eddington limit for significant. Periods standard astrophysical
- 27:01models struggle to explain how this happens either the early
- 27:05universe had conditions that allowed Super eddington, accretion Or ton
- 27:11six hundred eighteen formed from an unusually massive seed black,
- 27:15hole or it grew through an improbable series of mergers
- 27:20with other massive black, holes possibly all. Three Professor Andrew
- 27:27king from The university Of leicester calculated theoretical maximum masses
- 27:32for black holes in two thoy. Fifteen his work suggested
- 27:37that non spinning black holes couldn't exceed fifty billion solar
- 27:41masses through accretion. Alone the physics become self. Limiting radiation
- 27:48pressure eventually prevents further. Growth spinning black holes can reach higher,
- 27:53masses potentially up to two hundred seventy billion solar masses
- 27:58if they're rotating extremely. Fast ton six to one eight
- 28:03sits at sixty six billion solar. Masses if it's not spinning,
- 28:08rapidly it's already exceeded theoretical. Predictions if it is spinning,
- 28:14rapidly it might still have room to, grow but it's
- 28:18approaching the upper limits of what physics. Allows we might
- 28:22be observing a black hole near the theoretical maximum, size
- 28:27a cosmic endpoint where growth becomes. Impossible that's surrounding. Nebula
- 28:33remember three hundred thirty thousand light years, across containing one
- 28:38hundred billion solar masses of. Gas that's not, decorative that's.
- 28:44Fuel that's material that could potentially feed the black hole
- 28:48for millions or billions of years to. Come but Whether
- 28:53ton six' one eight can actually consume it depends on
- 28:57complex feedback mechanisms we don't fully. Understand the Black hole's
- 29:03radiation might heat and disperse the gas before it can fall,
- 29:07in or the gas might cool and, collapse providing sustained.
- 29:12Feeding we're watching a cosmic drama whose ending we can't.
- 29:17Predict here's one more comparison that might. Help our sun
- 29:23will live for about ten billion years. Total it's currently
- 29:27halfway through that. Lifespan when it, dies it'll puff off
- 29:32its outer layers and leave behind a white dwarf with
- 29:36about sixty percent of its current mass roughly point six solar.
- 29:41Masses that white dwarf will then cool and fade for
- 29:46trillions of, years eventually becoming a black, dwarf a, cold
- 29:52dark cinder of carbon and. Oxygen ton six one eight
- 29:56could swallow one hundred ten billion of those dead stars
- 30:00and still have room for more inside its event. Horizon
- 30:03you can't actually picture. This your brain isn't built for.
- 30:08It we evolved to understand scales from centimeters to, kilometers
- 30:13from seconds to. Decades our intuitions work for objects we
- 30:18can see and time scales we can. Experience when you
- 30:23try to visualize sixty six billion solar masses or structures
- 30:27spanning thousands of astronomical, units you're using mental tools designed
- 30:33for an entirely different problem. Set but now you have the,
- 30:37scaffolding you understand the. Comparisons you know That ton six
- 30:44hundred and eighteen outmasses our galaxy stars, combined that its
- 30:48event horizon dwarfs our solar, system that light takes weeks
- 30:53to cross, it that it shouldn't exist according to some theoretical,
- 30:58models but does. Anyway the numbers might not create a
- 31:02picture in your, mind but they create something, else context
- 31:06for realizing just how far beyond normal cosmic scales this object.
- 31:12Sits and there's another element to this scale problem that
- 31:17Makes ton six one eight even stranger than the numbers alone.
- 31:22Suggest we've been talking about its, mass its, size its energy,
- 31:27output but we haven't talked about its, age or, rather
- 31:32when we're seeing. It the light reaching us From ton
- 31:36six one eight has been traveling for ten point eight billion.
- 31:40Years think about what that. Means when those photons left
- 31:45the vicinity of this, monster the universe was only three
- 31:49billion years, old barely a quarter of its current. Age
- 31:54The sun didn't exist, Yet earth didn't. Exist our entire
- 31:59solar system wouldn't form for another six billion. Years we're
- 32:04not Observing ton six one eight as it is. Now
- 32:08we're observing it as it was in the cosmic equivalent
- 32:12of early. Childhood and it was already this. Massive that
- 32:16shouldn't be, possible not according to our standard models of
- 32:20black hole formation and. Growth Black holes grow primarily through two,
- 32:25mechanisms accreting matter from their surroundings or merging with other black.
- 32:31Holes both processes take, time a lot of. Time starting
- 32:38from stellar mass black holes the kind formed when massive stars,
- 32:42collapse you'd need incredibly efficient growth over billions of years
- 32:48to reach even one billion solar. Masses reaching sixty six
- 32:53billion solar masses in only three billion years requires something
- 32:58far more. Extreme The eddington limit becomes crucial. Here it's
- 33:03the point where a black hole's radiation pressure from in
- 33:07falling matter exactly. Balances the gravitational pull bringing matter in
- 33:14push beyond this, limit and the radiation should blow away
- 33:18the very material trying to fall into the black, hole
- 33:22choking off further. Growth it's a self regulating mechanism that
- 33:26prevents black holes from growing too. Quickly But ton six
- 33:32one eight somehow bypass. This either it grew through Super eddington,
- 33:38accretion somehow pulling in matter faster than the radiation pressure should,
- 33:43allow or it formed from an unusually massive, seed or
- 33:48it represents an improbable chain of, mergers or all three happened.
- 33:53Simultaneously none of these explanations is particularly. Satisfying Super eddington
- 34:01accretion requires special. Conditions we don't fully understand massive seed
- 34:08black holes from direct collapse scenarios are theoretically possible but observationally,
- 34:14unconfirmed and the merger scenario requires an unlikely confluence of.
- 34:20Events yet here Sits ton six one, eight challenging our
- 34:24theories by simply. Existing the discovery history adds another layer
- 34:28to this. Puzzle ton six one eight wasn't found yesterday
- 34:34with cutting edge. Technology it was photographed in nineteen fifty
- 34:38seven at The Tonan Sintler observatory In mexico during a
- 34:43survey of faint blue. Stars on those photographic, plates it
- 34:47appeared decidedly, violate unusual enough to warrant catalog's entry number
- 34:54six hundred. Eighteen but quasars hadn't been recognized as a
- 34:59distinct class of objects. Yet that wouldn't happen until nineteen sixty.
- 35:04Three so for thirteen, Years ton six' one eight sat
- 35:09in a catalog as a mysterious violet, dot its true nature.
- 35:13Unknown in nineteen, seventy a radio survey In bologna detected
- 35:19radio emissions from its, location flagging it as potentially. Interesting
- 35:25Marie Helene ulrich then obtained optical spectra at The MacDonald,
- 35:29observatory revealing emission lines characteristic of. Quasers only then did
- 35:35astronomers realize what they were looking, at not a faint
- 35:39blue star in our, galaxy but a quasar billions of
- 35:43light years, away powered by a black hole of incomprehensible.
- 35:48Mass this delayed recognition isn't unusual in. Astronomy we often
- 35:54observe things before we understand, them but it's particularly striking
- 35:59WITH n six one eight because of what the delay,
- 36:03represents humanity's gradual realization that the universe contains objects operating
- 36:11at scales we hadn't. Imagined the brightness Makes ton six
- 36:16one eight simultaneously visible and. Invisible it shines with the
- 36:21luminosity of one hundred forty trillion suns with an absolute
- 36:27magnitude of negative thirty point. Seven it's one of the
- 36:31brightest objects in the known. Universe but that brilliance comes
- 36:37entirely from the accretion disc and surrounding, material not from
- 36:43stars in the host. Galaxy in, fact we can't see
- 36:47the host galaxy at. All it's completely outshone by the central,
- 36:51quasar potentially hundreds of billions of stars rendered invisible by
- 36:58the light from matter falling into the black. Hole the galaxy,
- 37:02exists it has, to as galaxies host these supermassive black,
- 37:08holes but it's lost in the. Glare that accretion disk
- 37:13deserves closer. Attention picture a structure extending light days or
- 37:19light weeks from the black, hole where matter spirals inward
- 37:23at velocities approaching seven thousand kilometers per. Second that's over
- 37:28two percent the speed of. Light the friction and compression
- 37:32heat this material to millions of. Degrees at those, temperatures
- 37:37atoms are completely. Ionized electrons are stripped, away leaving bare
- 37:43nuclei colliding at relativistic. Speeds the innermost regions reach the
- 37:49highest temperatures potentially tens of millions of, degrees near the event,
- 37:54horizon where orbital velocities. Peak this superheated plasma radiates across
- 38:01the entire electromagnetic, spectrum radio, waves, infrared visible, light, ULTRAVIOLET x,
- 38:11rays gamma. Rays every wavelength tells us something about the
- 38:17physical conditions at different locations in the. Disk the spectrum
- 38:22Of ton six hundred eighteen shows unusually wide emission. Lines
- 38:27these lines come from gas in what's called the broad line,
- 38:31region located beyond the accretion disc but still within the
- 38:36black hole's gravitational. Influence the width of these lines indicates.
- 38:41Velocity the faster the gas, moves the more the emission
- 38:45lines Are doppler, shifted creating broader features in the. Spectrum
- 38:51measurements show gas velocities reaching ten, thousand five hundred kilometers
- 38:57per second in some. Regions that's three point five per
- 39:01cent the speed of. Light this extreme velocity provides one
- 39:05of the key methods for estimating the black hole's. Mass
- 39:09the faster gas must orbit to avoid falling in the
- 39:13stronger the gravitational, force which directly relates to the central.
- 39:18Mass different research teams have used different spectral lines to
- 39:23Estimate ton six hundred eighteen s, mass yielding different. Results
- 39:29the original estimates using hydrogen beta emission lines suggested sixty
- 39:35six billion solar. Masses more recent measurements using carbon four
- 39:40emission lines produced a lower, estimate forty point seven billion solar.
- 39:46Masses both measurements use the same underlying, data but different
- 39:51calibration methods and. Assumptions this uncertainty. Matters If ton six
- 39:58hundred eighteen is only forty billion solar, Masses it's still extraordinarily,
- 40:04massive but falls within some theoretical. Predictions at sixty six
- 40:10billion solar, masses it exceeds certain theoretical limits for non
- 40:14spinning black, holes making it even more problematic for standard.
- 40:19Models the truth probably lies somewhere in that, range but
- 40:24the uncertainty reflects fundamental challenges in measuring black hole masses
- 40:30at such extreme. Distances we're not weighing these objects. Directly
- 40:36we're inferring their masses from the motion of surrounding, gas
- 40:40which requires assumptions about the, geometry viewing angle and dynamical
- 40:45state of the. System beyond the accretion disk and broad
- 40:50line region lies something even more, remarkable The lyman alpha,
- 40:56nebula discovered through observations with The ATTAKARMA a large millimeter
- 41:01array in twenty twenty. One this structure spans at least
- 41:07three hundred thirty thousand light, years twice the diameter of
- 41:11The Milky. Way it consists of two distinct, components an
- 41:16inner molecular, outflow likely driven by winds from the accretion
- 41:21disc and jets from near the black, hole and an
- 41:25extensive region of cold molecular gas in the circumgalactic, medium
- 41:31the diffuse halo of materials surrounding the. Galaxy each component
- 41:36contains roughly fifty billion solar masses of gas. Combined that's
- 41:42one hundred billion solar masses more than the black hole.
- 41:46Itself this nebula isn't just, decoration its evidence of the
- 41:51black hole's influence extending across galactic. Scales the intense ultraviolet
- 41:57radiation from the quasar ionized hydrogen in the, nebula causing
- 42:02it to emit The lyman alpha, line a specific ultraviolet.
- 42:07Wavelength this emission is so strong that ton six one
- 42:12eight is classified as A lyman alpha, blob one of
- 42:16the largest such objects. Known the alignment of the nebula
- 42:20with the radio jets suggests a physical. Connection jets are
- 42:26narrow beams of charged particles accelerated to near light, speed
- 42:31shooting outward perpendicular to the accretion disc For ton six hundred.
- 42:37Eighteen these jets carry enormous energy and, momentum potentially shaping
- 42:42how gas is distributed across hundreds of thousands of light.
- 42:46Years this interaction between the black hole and its environment represents.
- 42:51Feedback the black hole affects its, surroundings which in turn
- 42:56affects how much matter can fall back into the black.
- 42:59Hole strong feedback can regulate or even halt black hole
- 43:04growth by heating and dispersing the gas that would otherwise feed.
- 43:08It Whether ton six one eight is currently in a
- 43:13feedback limited state or still growing actively remains. Unclear the
- 43:19surrounding nebula contains enough material to fuel continued growth for
- 43:24millions or billions of, years but whether that material can
- 43:28actually reach the black hole depends on complex processes we
- 43:33don't fully. Understand ton six one eight is also classified
- 43:37as radio, loud meaning it produces substantial radio emissions beyond
- 43:43what comes from the accretion disc. Alone this radio emission
- 43:48originates from the, jets where magnetic fields accelerate electrons to relativistic.
- 43:54Speeds as these electrons spiral around magnetic field, lines they
- 44:00emit synchrotron, radiation predominantly in radio, wavelengths but extending into
- 44:07other parts of the. Spectrum the jets themselves are poorly.
- 44:11Understood we know they exist because we detect their. Radiation
- 44:17we know they carry substantial energy because the radio emission
- 44:21is so, strong but the exact mechanism that launches them remains.
- 44:26Debated it involves the black hole's, spin magnetic fields threading
- 44:32the accretion, disc and the extraction of rotational energy from
- 44:36the black hole itself through a process called The Blanford xenogec.
- 44:41Mechanism For ton six hundred, eighteen the jets are aligned
- 44:46with the nebular, structure suggesting they've been active long enough
- 44:50to shape their environments. Significantly these outflows can suppress star
- 44:55formation by heating gas and preventing it from color aapsing into.
- 45:00Stars they can also trigger star formation in some regions
- 45:05by compressing gas. Clouds the net effect depends on local
- 45:10conditions and the jet's. Power ton six one eight also
- 45:16shows broad absorption lines in its, spectrum another classification. Tag
- 45:21these absorption features indicate high velocity winds flowing outward from the,
- 45:26quasar likely driven by radiation. Pressure these winds can reach
- 45:32thousands of kilometers per, second carrying away substantial amounts of
- 45:38matter and. Energy this outflow represents yet another feedback, mechanism
- 45:44as the black hole accretes matter and releases. Energy some
- 45:48of that energy drives winds that expel, material potentially limiting
- 45:54how much can fall in over cosmic. Time this feedback
- 45:59may be why s supermassive black holes and their host
- 46:02galaxies show correlated. Properties the black hole's growth and the
- 46:08galaxy's evolution are intimately linked through these feedback. Processes Studying
- 46:14ton six hundred eighteen in detail presents significant observational. Challenges
- 46:21its extreme distance makes it appear faint despite its intrinsic.
- 46:25Brightness the red shift stretches all. Wavelengths ultraviolet light is
- 46:31shifted into the visible, range visible light into, infrared and so.
- 46:37On this complicates, observations but also provides, opportunities as the
- 46:44red shift moves some spectral features that would normally be
- 46:48blocked By earth's atmosphere into observable. Wavelengths the host galaxy remains,
- 46:54invisible outshone by the. Quasar current technology g can't separate
- 47:01the galaxy's starlight from the overwhelming glare of the central.
- 47:05Engine future telescopes like The James Web Space telescope or
- 47:10planned extremely large telescopes may eventually resolve details about the
- 47:16host galaxy's stellar, population, mass and. Structure what we do
- 47:22know is That ton six' one eight represents a crucial
- 47:26window into the. Early universe quasers were much more common
- 47:31when the universe, was young during an era of rapid
- 47:35galaxy formation and black. Hole growth as the universe aged,
- 47:40and expanded galaxies consumed or dispersed much of, their gas reducing,
- 47:46Fuel availability quaser activity declined as. A result modern galaxies typically,
- 47:54have quiet supermassive, black holes, accreting slowly if. At all Our,
- 47:59own sagittarius, a star is, relatively inactive consuming matter at a.
- 48:04Modest rate But in ton six one, eight's era conditions favored.
- 48:10Active growth galaxies were forming and, Merging frequently gas, was
- 48:15abundant black holes, grew rapidly powering brilliant quasers visible across.
- 48:21The cosmos ton six one eight catches this process near,
- 48:26its peak showing us what the universe looked like during this.
- 48:30Transformative period the fact that such massive black holes existed
- 48:36so early constrains models of. Cosmic evolution it tells us
- 48:42about initial conditions in, the universe about how matter, was
- 48:46distributed about how quickly. Structures formed it tells us about
- 48:53the physics of black hole formation in conditions vastly different from.
- 48:58Today's universe something that doesn't quite Add up ton six
- 49:04one eight, shouldn't exist at least not according to some of.
- 49:09Our models the universe was only three billion years Old
- 49:14when ton six. One eight look the way we see,
- 49:17it now that's barely enough time for galaxies, to form
- 49:21let alone for a black hole to accumulate forty to
- 49:25sixty six billion. Solar masses standard accretion theory predicts growth
- 49:31rates that simply can't produce something this massive. This quickly
- 49:36the math. Doesn't work think about it. This way black
- 49:41holes grow by, consuming matter but there's a natural speed
- 49:45limit to, this process Called the. Eddington limit when matter
- 49:49falls toward a, black hole it heats up and. Releases
- 49:53radiation that radiation. Pushes outward at some point the outward
- 50:00radiation pressure equals the inward. Gravitational pull the system. Reaches
- 50:06equilibrium matter can't fall in faster than the radiation. Can
- 50:10escape this sets a maximum. Growth rate even starting from
- 50:15a stellar mass, black hole say one hundred, solar masses
- 50:20and accreting At the eddington limit continuously for three, billion
- 50:25years you'd only reach a few billion, solar masses not,
- 50:29forty billion not sixty. Six billion the timeline doesn't. Allow
- 50:34it so How did ton six hundred eighteen get so big?
- 50:39So fast several theories attempt to explain. This puzzle one
- 50:44possibility involves direct collapse instead of forming from a. Stellar
- 50:50remnant perhaps some primordial black holes formed when massive gas
- 50:54clouds in the early universe. Collapse directly bypassing the stellar,
- 51:00phase entirely these seeds would start, much heavier maybe ten
- 51:05thousand or even one hundred thousand. Solar masses that gives
- 51:10them a. Head start another idea Suggests super. Eddington accretion
- 51:15maybe under the, right conditions black holes can temporarily Exceed the.
- 51:20Eddington limit the early universe was dense. With Gas perhaps
- 51:26ton six one eight found itself in an environment so
- 51:30rich with fuel that it, gorged itself growing faster than
- 51:34the standard Limits predict some simulations show this might work
- 51:40if the accretion disc is geometrically thick and radiation escapes
- 51:45preferentially in certain directions rather than pushing. Uniformly outward there's
- 51:51also the. Merger scenario if multiple black holes formed early and,
- 51:56merged repeatedly they could build mass more quickly than a tcretion.
- 52:00Alone allows each merger adds the combined mass instantly without
- 52:06needing to wait for gas to spiral in a series of,
- 52:10such mergers combined with steady accretion, between events might produce
- 52:16an ultra massive black hole within the. Available time none
- 52:20of these explanations is. Entirely satisfying each. Has problems direct
- 52:27collapse requires very specific conditions that may not have. Been
- 52:31Common super eddington accretion faces theoretical challenges about stability and.
- 52:38Radiation escape mergers require an improbably high rate of collisions,
- 52:44Early On yet ton six one. Eight exists the universe
- 52:49doesn't care about our. Theoretical difficulties this brings us to
- 52:54another fascinating Aspect of ton six. Hundred eighteen it might
- 52:59be approaching its maximum. Possible mass in, twenty Fifteen Astrophysicist
- 53:05andrew king calculated theoretical mass limits for black holes based on.
- 53:10Accretion physics he found that for a non spinning, black
- 53:15hole the maximum mass achievable through accretion is roughly fifty billion.
- 53:21Solar masses if the black hole spins rapidly in the
- 53:25same direction as its, accretion disc this limit increases potentially
- 53:31to two hundred seventy billion. Solar masses the reason involves
- 53:35the innermost stable. Circular orbit as a black hole, gains
- 53:40mass this orbit. Moves outward eventually it reaches a point
- 53:47where the gravitational pull at the issco isn't strong enough
- 53:52to hold gas together against its own. Self gravity the
- 53:57disc becomes unstable and can't deliver mass to the black.
- 54:00Hole efficiently Growth stalls ton six, one eight with mass
- 54:06estimates ranging from forty point seven to sixty six billion,
- 54:10solar masses sits right at Or above king's limit for
- 54:15non spinning. Black holes if the higher mass estimate, Is
- 54:19correct ton six one eight might already be near its
- 54:23accretion based. Growth ceiling it could be one of the
- 54:26most massive black holes physically possible through, this mechanism but
- 54:31black holes can still grow. Through mergers when two black
- 54:36holes orbit each other and, eventually collide they combine. Their
- 54:41masses this process doesn't face the same radiation pressure constraints,
- 54:46as accretion so Even if ton six one eight has
- 54:53maxed out its, accretion potential it could continue growing by
- 54:58consuming other. Black hole, of course there's competition for the
- 55:02title of largest. Black HOLE, phoenix a another ultra massive,
- 55:07black hole has, been cited with mass estimates around one
- 55:12hundred billion. Solar, masses however that measurement carries. Significant uncertainty
- 55:20different techniques and assumptions produce. Different results the black hole
- 55:25at the center Of the phoenix cluster, is enormous but
- 55:29pinning down its exact mass. Remains challenging another contender is
- 55:34the black hole in the QUASAR sd ssj one four
- 55:38zero eight two one point six seven plus zero two
- 55:42five seven three three point two tri saying that three.
- 55:46Times fast its mass estimates also reach, extreme values though
- 55:52again with. Substantial uncertainty the competition for largest black hole
- 55:58depends heavily, on men, measurement techniques and which data sets. You,
- 56:03trust recently in twenty, twenty five astronomers discovered what they're
- 56:08calling The cosmic horseshoe, black hole weighing in at thirty
- 56:14six billion. Solar masses this discovery used a combination of
- 56:19gravitational lensing and, stellar kinematics a technique that provides more
- 56:25direct mass measurements than spectroscopic. Methods Alone The cosmic horseshoe
- 56:32ranks among the top ten most massive black, holes known possibly,
- 56:37top five but even at thirty six billion, solar masses
- 56:41it's still Smaller than ton six to one. Eight estimates
- 56:45the difficulties in precisely measuring black hole masses mean rankings.
- 56:50Can shift new, techniques emerge old measurements. Get revised what's
- 56:57clear Is that ton six one eight remains a, top
- 57:00contender consistently appearing in discussions of the universe's most massive.
- 57:06Black holes what about? Its size not, its mass but its.
- 57:11Physical dimensions the event horizon of a black hole scales with.
- 57:17Its Mass for ton six, one eight The schwarz, child
- 57:22radius the distance from the center to the event horizon
- 57:26is approximately, one thousand three hundred. Astronomical units REMEMBER one
- 57:34au is the Distance from earth To, the sun about
- 57:37one hundred fifty. Million kilometers ton six one eight event
- 57:43horizon extends, one thousand three hundred times. That distance to
- 57:48put it, another way the event horizon's diameter is roughly,
- 57:52two thousand six hundred. Astronomical units neptune Orbits the sun
- 57:58at about thirty. Astronomical units ton six one eight could
- 58:03swallow our entire solar system Out past neptune Past The
- 58:07kuiper belt more than forty. Times over its event horizon
- 58:12is larger than the orbits of all. Our planets combined
- 58:16with room, TO spare nasa created a visualization comparing black.
- 58:21Hole sizes it starts with stellar mass, black holes Moves,
- 58:26through sagittarius a star At The milky, way's center CONTINUES
- 58:30to m eighty seven's, black hole the one famously imaged
- 58:34by the event, horizon telescope and ends WITH t n six.
- 58:40ONE eight m eighty seven's black hole has an updated
- 58:45mass of five point four billion. Solar masses its shadow
- 58:50is so large that a beam of light traveling at
- 58:52three hundred thousand kilometers per second would take about two
- 58:56and a half days to. Cross It tom on six
- 59:00one eighth's shadow dwarfs even that light would take weeks to. Traverse.
- 59:05It weeks think about what that means Light circles earth's
- 59:12equator more than seven times in, one second yet it
- 59:16would need weeks To cross ton's six one. Eighth's shadow
- 59:20the scale. Defies comprehension, this shadow the apparent size of the,
- 59:25event horizon as seen by a, distant observer is actually
- 59:30larger than The schwarz child radius due to. Gravitational lensing
- 59:35the intense gravity bends light around the, black hole creating
- 59:40an optical illusion that makes the shadow appear Bigger for
- 59:45ton six. One eight this effect amplifies an already incomprehensible
- 59:51size into something even. More extreme standing on a Planet
- 59:56orbiting ton six, One eight if such a place it,
- 1:00:00could exist you'd see a region of absolute blackness dominating,
- 1:00:05the sky not just a, dark spot avoid. So vast
- 1:00:11it would cover a significant fraction of the, visible sky
- 1:00:15surrounded by a ring of tortured red shifted light from
- 1:00:19the accretion disk wrapping around the event. Horizon's curve, of
- 1:00:23course you couldn't actually. Stand there the tidal forces would
- 1:00:28tear you apart long before you. Got close the radiation would.
- 1:00:32Cook you the environment is utterly hostile to any conceivable form,
- 1:00:38of life but as a, thought experiment it illustrates the
- 1:00:42sheer presence such an object. Would have inside the, event
- 1:00:47horizon causality. Breaks down all paths. Lead inward you can
- 1:00:53no more avoid falling toward the singularity than you can
- 1:00:57avoid moving forward. In time the, singularity itself the point
- 1:01:03of infinite density at the black, hole's core remains hidden.
- 1:01:07From view shielded by the, event horizon we can't observe.
- 1:01:11It directly general relativity predicts, its existence but also suggests
- 1:01:17our equations break, down there requiring a theory of quantum
- 1:01:21gravity we don't. Yet have ton six one eight's temperature
- 1:01:26profile offers another window into. Its extremes the accretion discs
- 1:01:31emissions reveal temperatures around thirty eight thousand. Degrees celsius that's
- 1:01:36the temperature of gas in the outer regions of, the
- 1:01:39disk already hot enough to ionize atoms and produce intense.
- 1:01:44Ultraviolet radiation closer to the, black hole temperatures climb even
- 1:01:50higher millions. Of degrees at, those temperatures matter exist in a.
- 1:01:56Plasma state electrons are stripped, from atoms the GAS emits
- 1:02:01x rays and. Gamma rays this temperature gradient drives the
- 1:02:06luminosity hotter regions emit. More energy the, inner disk where,
- 1:02:11temperatures peak produces the most. Intense radiation as matter, spirals
- 1:02:18inward it releases gravitational. Potential Energy for ton six, hundred
- 1:02:24eighteen this process converts mass to energy with, extraordinary efficiency
- 1:02:31far better than. Nuclear fusion that's why quasers shine so
- 1:02:35brilliantly despite their. Compact size the Alignment of ton six
- 1:02:40hundred eighteens radio jets with its nebula suggests a long
- 1:02:44period of. Sustained activity jets don't. Form instantly they require
- 1:02:50stable accretion and a strong magnetic field maintained. Over time
- 1:02:56the fact that the nebula structure mirrors the jet orientation
- 1:03:00indicates these outflows have been shaping their environment, for millions
- 1:03:04possibly tens of millions. Of years ton six one eight
- 1:03:09isn't a. Brief flare it's, a persistent powerful engine that
- 1:03:14has been running for a significant fraction of. Cosmic history
- 1:03:18this persistence raises interesting questions about. Duty cycles quasars don't
- 1:03:24stay active forever fuel, supplies run low feedback mechanisms shut.
- 1:03:30Down accretion the quasar, phase ends leaving behind, a dormant supermassive.
- 1:03:36Black hole how Long does ton six one eight. Have
- 1:03:40left is it near the end of its active phase
- 1:03:44or just. Getting started we can't say, for certain but
- 1:03:48given its enormous mass and the vast reservoir of gas
- 1:03:52in the, Surrounding nebula ton six one eight likely has
- 1:03:56fuel for continued activity for. Some, time Yet when tarn
- 1:04:01six hundred eighteen eventually runs out of easily, accessible fuel it,
- 1:04:06Will fade the accretion disk, will thin the jets will
- 1:04:11weaken and. Shut off the brilliant quasar, will dim revealing
- 1:04:16the host galaxy that currently remains hidden beneath. The glare
- 1:04:21at that POINT to n six one eight will resemble,
- 1:04:25the quiet supermassive black holes we see in, modern galaxies
- 1:04:30massive but dormant waiting for a fresh supply of gas.
- 1:04:33To reignite that future state represents the end point of.
- 1:04:38Quasar evolution all modern galaxies with super massive black holes
- 1:04:44likely went through quasar phases in. Their, youth sagittarius a
- 1:04:50star At The milky, way's center probably shone as a
- 1:04:54quasar billions of. Years ago now, it's quiet, accreting slowly
- 1:05:00reducing only. Faint emissions tons six one eight shows us
- 1:05:05what our galaxy's core might have looked like in, its
- 1:05:07prime a blazing beacon visible across. The universe this evolutionary
- 1:05:14Trajectory connects ton six one eight to every massive galaxy we.
- 1:05:19Observe today the correlation between black hole mass and galactic properties.
- 1:05:24Isn't coincidental supermassive black holes and their host galaxies grow
- 1:05:30together through a process. Called coevolution when a quasar blazes at,
- 1:05:36full power its radiation and jets heat, surrounding gas preventing
- 1:05:41it from cooling and. Forming stars this feedback mechanism regulates
- 1:05:47both star formation and black. Hole growth, without it galaxies
- 1:05:52would convert gas into stars, too quickly exhausting their fuel
- 1:05:57supply and looking nothing like the g galaxies. We observe
- 1:06:01ton six one eight exemplifies this process. In action its
- 1:06:06powerful jets inject energy into the. Surrounding Medium the lyman
- 1:06:11alpha nebula shows clear signs of. This interaction gas heated
- 1:06:16and ionized, by radiation structures aligned with, jet directions velocities consistent.
- 1:06:23Without flows the black hole isn't just, consuming gas it's
- 1:06:29reshaping its, entire environment determining what gas cools and, form
- 1:06:35stars what gas gets heated, and dispersed what structures emerge
- 1:06:40from the cosmic. Raw materials this feedback operates on multiple.
- 1:06:46Scales simultaneously close to the. Black hole within the, accretion
- 1:06:51disc temperatures reach millions, of degrees radiation pressure becomes so
- 1:06:57intense it can reverse, the inflow creating winds that blow
- 1:07:02material away. Farther out jets deposit energy across hundreds of
- 1:07:08thousands of, light years even farther at. Megaparsec scales the
- 1:07:14cumulative effect of many quasars heats the, intergalactic medium affecting
- 1:07:20cosmic structure. Formation itself the efficiency of this process depends
- 1:07:25critically On the, eddington limit the balance point between gravity
- 1:07:30pulling matter inward and radiation pressure pushing. It outward for
- 1:07:35a black hole of ton six hundred, eighteen's Mass the
- 1:07:39eddington luminosity, is enormous roughly ten to the power of.
- 1:07:44Forty watts ton six one eight shines at approximately four times,
- 1:07:49that value Suggesting super. Eddington accretion how does it? Manage
- 1:07:55this several mechanisms might Enable super. Eddington rate if the
- 1:08:01accretion disc is geometrically thick rather, than thin radiation can
- 1:08:06escape along the poles while matter continues flowing in along.
- 1:08:11The equator if the accretion flow is clumpy rather, than
- 1:08:16smooth dense clumps can shield material behind them from. Radiation
- 1:08:21pressure if the black hole is, spinning rapidly frame dragging
- 1:08:27effects near the event horizon can extract, rotational energy supplementing
- 1:08:32the luminosity without requiring more accretion ton six one. Eight
- 1:08:38s spin. Remains unknown measuring black hole spin requires observing
- 1:08:44features near the, event horizon the innermost stable, circular orbit relativistic,
- 1:08:51line profiles or spin dependent efficiency. Of accretion for an
- 1:08:57object ten point eight billion, light away these measurements exceed.
- 1:09:02Current capabilities we can only infer spin indirectly from luminosity and,
- 1:09:09accretion signatures but spin matters enormously for. Maximum Mass andrew
- 1:09:16king's theoretical work showed that a non spinning black hole
- 1:09:20growing through accretion should max out around fifty billion. Solar
- 1:09:25masses beyond, that mass the innermost stable circular orbit moves
- 1:09:30outward past the point where gas self gravity can hold.
- 1:09:34It together the accretion disc fragments. Growth, stalls however a
- 1:09:41rapidly spinning black hole aligned with its accretion disc can
- 1:09:46reach masses up to two hundred seventy billion solar masses
- 1:09:51before hitting. This limit ton six hundred, eighteen's mass whether
- 1:09:57forty point seven billion or s sixty six billion, solar
- 1:10:01masses depending on, the measurement places it near or potentially
- 1:10:06above the non. Spinning limit if the higher mass estimate,
- 1:10:10Is correct ton six one eight must be. Spinning significantly
- 1:10:16if the lower, estimate holds it might be approaching its.
- 1:10:20Maximum size regardless. Of spin, Either way ton six one
- 1:10:26eight likely won't grow much larger through. Accretion alone mergers
- 1:10:31offer an alternative. Growth path when two black holes orbit,
- 1:10:35each other they lose energy to gravitational waves and. Eventually
- 1:10:40merge the resulting black hole has mass equal to the
- 1:10:44sum of the original masses minus the energy radiated as,
- 1:10:48gravitational waves typically a few percent for supermassive black holes
- 1:10:55like Those in ton six one eight's, mass range mergers
- 1:10:59could add tens of billions of solar masses in a.
- 1:11:02Single event the, early Universe when ton six one eight,
- 1:11:07was active experienced higher galaxy merger rates. Than today galaxies were,
- 1:11:13closer together dark matter halos were. Still assembling major mergers.
- 1:11:19Happened frequently each merger brought gas to fuel the quasar
- 1:11:25and potentially delivered another supermassive black hole to merge with the.
- 1:11:29Central one this environment favoured rapid black hole growth through
- 1:11:35both accretion, and mergers but mergers also. Pose challenges when
- 1:11:40two supermassive black holes enter the, same galaxy they don't.
- 1:11:44Immediately merge they must first sync to the galactic center
- 1:11:49through dynamical friction interactions with stars and gas that extract
- 1:11:55energy and. Angular momentum this process works, well initially but
- 1:12:01slows as the black holes form a. Bound binary getting
- 1:12:05from a wide binary separation down to merger requires, additional
- 1:12:10mechanisms interactions with a third, black hole a dense, stellar
- 1:12:15cusp or a circumbinary. Gas disc this final parsec problem
- 1:12:22has puzzled theorists. For decades some massive black hole binaries
- 1:12:28might stall at separations of about, a parsec never merging
- 1:12:32on time scales shorter than the age of. The universe,
- 1:12:36if true this would limit how quickly black holes can grow. Through,
- 1:12:40mergers however recent simulations suggest that in gas rich early,
- 1:12:46universe conditions circumbinary discs provide sufficient torque to. Drive mergers
- 1:12:52ton six hundred eighteen might have grown partly through. Such
- 1:12:57mergers the broader absorption line Features in ton's six hundred
- 1:13:03eighteen spectrum hint at. Powerful outflows these absorption lines appear
- 1:13:09blue shifted shifted to, shorter wavelengths indicating material MOVING. Toward
- 1:13:16us at, high velocities the gas absorbs specific wavelengths from the,
- 1:13:22quasar's light creating dark lines in. The spectrum the width
- 1:13:28and velocity of these lines reveal outflow speeds reaching thousands
- 1:13:34of kilometers. Per second these outflows aren't accretion disc. Winds
- 1:13:39alone their large scale, galactic winds driven, by radiation pressure.
- 1:13:44And jets gas accelerated to these velocities carries enormous, kinetic
- 1:13:50energy enough to heat the surrounding medium and potentially expel
- 1:13:54it from the. Galaxy entirely this represents the feedback mechanism
- 1:14:00in its most, direct form the black hole literally blowing
- 1:14:04away its own. Fuel supply the mass outflow rate can
- 1:14:08be estimated from the absorption. Line Properties for ton six,
- 1:14:13hundred eighteen outflows likely carry away hundreds to thousands of
- 1:14:18solar masses. Per year compare this to the accretion rate
- 1:14:23needed to power the quasar several hundred solar masses. Per
- 1:14:28year based, on luminosity the outflow and accretion rates. Are
- 1:14:33comparable for every bit of matter the black, hole consumes
- 1:14:37roughly an equal amount. Gets expelled this balance determines the.
- 1:14:42System's evolution if outflows exceed accretion, too much the quasar
- 1:14:47starves and. Shuts down if, accretion dominates the black hole grows.
- 1:14:53Without limit the fact that We observe ton six one
- 1:14:57eight in a roughly balanced state suggests. Self regulation the
- 1:15:03quasar adjusts its own fuel supply, through feedback maintaining conditions
- 1:15:10where it can shine brightly without either exhausting its gas
- 1:15:14reservoir too quickly or. Growing uncontrollably the radio loud classification
- 1:15:20indicates significant. Jet power only about ten percent of quasers
- 1:15:25produce powerful. Radio jets the distinction correlates with black hole
- 1:15:30spin and magnetic. Field configuration jets require strong magnetic fields
- 1:15:36threading the accretion disc and. Event horizon as the black,
- 1:15:40hole spins it drags these, fields around extracting rotational energy
- 1:15:46and launch in plasma along the spin axis at. Relativistic
- 1:15:50speeds ton six one eight jets punch through the accretion
- 1:15:56disc and, continue outward eventually creating radio lobes millions of
- 1:16:02light Years across these lobes aren't visible in current observations
- 1:16:06Due to ton six one, eighth distance but they must
- 1:16:11exist based on the. Radio spectrum the jets deposit energy
- 1:16:15in the, intergalactic medium heating it and potentially triggering or suppressing.
- 1:16:21Star formation in smaller galaxies. They encounter jet speeds approach
- 1:16:27the speed. Of light particles accelerated to such velocities produce
- 1:16:32synchrotron radiation emission from charged particles spiraling in. Magnetic fields
- 1:16:40this produces the radio signature. We detect the total power
- 1:16:45in the jets can be estimated from, radio luminosity typically
- 1:16:50a few percent of the quaser's. Total Luminosity for ton six,
- 1:16:55hundred eighteen jet power might reach ten to the power
- 1:16:59of third thirty, nine watts, or more enough to power
- 1:17:02a trillion sun's worth of energy output in. Mechanical form
- 1:17:06the alignment between jets And the liman alpha nebula structure
- 1:17:11suggests these outflows have been stable for millions. Of years
- 1:17:16jets can, be intermittent turning on and off as accretion,
- 1:17:20rates vary but producing the observed nebula structure requires sustained.
- 1:17:26Jet activity the gas didn't just get blown. Away randomly
- 1:17:31it was shaped and sculpted by persistent. Directed outflows this
- 1:17:36stability implies a stable. Accretion geometry the accretion disc maintains
- 1:17:43its orientation over. Long periods the black hole's spin axis
- 1:17:47stays aligned with. A disc major disturbances like galaxy mergers
- 1:17:53or sudden gas infoll from unusual directions would disrupt this
- 1:17:58alignment and pertendly shut down the. Jets temporarily the fact
- 1:18:03that we see stable Jets suggests ton six one eight
- 1:18:08has had a relatively undisturbed, recent history at least on
- 1:18:13timescales of millions. Of years the nebula's mass one hundred
- 1:18:18billion solar, masses total exceeds the black hole's. Mass significantly
- 1:18:24this gas represents the building material for future stars or
- 1:18:29future black. Hole accretion if, conditions allow the nebula could
- 1:18:34form thousands of massive star clusters over the next few. Billion,
- 1:18:39years alternatively if the quaser, remains active it might gradually
- 1:18:45consume much of. This material the fate depends on. Cooling
- 1:18:50times hot gas must cool before it can collapse and.
- 1:18:56Form stars cooling depends on deby density and temperature in the,
- 1:19:02inner regions where the quasar's radiation keeps the gas ionized.
- 1:19:07And hot cooling times exceed the age of, the universe
- 1:19:12this gas won't form stars. Anytime soon in, outer regions
- 1:19:17where radiation, is weaker cooling, times shorten star formation might,
- 1:19:23proceed there building the stellar halo of the. Host galaxy
- 1:19:28this process mirrors what we see in. Modern galaxies massive
- 1:19:33elliptical galaxies contain old stellar populations with little ongoing. Star
- 1:19:37formation their gas is hot, and diffuse kept that way
- 1:19:42by past quasar activity and ongoing heating from. Old stars
- 1:19:47the quasar phase ended billions of, years ago but its.
- 1:19:51Effects persist ton six one eight shows us this process
- 1:19:57in progress the moment when a quas is actively suppressing
- 1:20:01star formation. Through Feedback the lyman alpha emission itself provides a.
- 1:20:07Diagnostic tool this ultraviolet line occurs when electrons in hydrogen
- 1:20:12atoms transition from the first excited state to the. Ground
- 1:20:17state the photon energy corresponds to ten point two, electron
- 1:20:22vaults placing it IN. The uv ton six one eight's
- 1:20:27extreme luminosity PRODUCES copious uv radiation that ionizes the. Surrounding
- 1:20:34hydrogen when, electrons recombine they cascade down through, energy Levels
- 1:20:39producing lyman. Alpha photons the nebula glows brightly in this
- 1:20:45line because the quasar provides the. Energy source turn off
- 1:20:49the quasar and the nebula would fade on time scales
- 1:20:53of thousands to millions, of years the time needed for
- 1:20:57electrons to recombine And for lyman alpha photons to scatter
- 1:21:02out of. The nebula the current brightness tells us the
- 1:21:06quasar has been, active recently within the past few. Million years,
- 1:21:11at most scattering. Matters here lyman alpha photons don't. Escape
- 1:21:18directly they scatter off neutral hydrogen many times before. Finally
- 1:21:23escaping this resonant scattering can trap photons for, extended periods
- 1:21:29creating a diffuse glow around. The source the nebula's extended
- 1:21:35structure partially results from this. Scattering process photons produced near
- 1:21:41the quasar random walk outward, through scattering eventually emerging at.
- 1:21:47Large distances the velocity structure of the nebula encodes. Its
- 1:21:52history different regions show different velocities relative to. The quasar
- 1:21:59some gas gas moves, toward us, some away some orbits the.
- 1:22:04Black hole by mapping these velocities, using spectroscopy astronomers reconstruct
- 1:22:11the three dimensional structure. And Dynamics the alma observations that
- 1:22:16revealed the molecular gas component provided precisely this information velocity
- 1:22:23maps showing how gas flows through. The system these observations
- 1:22:28showed two. Distinct components the inner molecular outflow moves at
- 1:22:34hundreds of kilometers, per second directly driven by the quaser's jets.
- 1:22:39And radiation the extensive circumgalactic medium moves, more slowly representing
- 1:22:45gas that's been affected by the quasar but not. Directly
- 1:22:49expelled both components contain MOLECULAR hydrogen h two rather than just.
- 1:22:56Atomic hydrogen this indicates sufficient densasnsity and shielding for molecules
- 1:23:01to survive despite the intense. Radiation environment molecular gas is star.
- 1:23:08Formation fuel under the, right conditions it collapses to. Form
- 1:23:12stars the presence of one hundred billion solar masses of
- 1:23:17molecular Gas around ton six one eight suggests enormous star,
- 1:23:22Formation potential yet current observations show the gas remains. Mostly
- 1:23:27diffuse why isn't it forming? Stars now turbulence provides. One
- 1:23:33answer gas must be relatively calm to collapse under its.
- 1:23:37Own gravity turbulence random motions on various scales provides support.
- 1:23:43Against collapse similar to. Thermal pressure the jets and Outflows
- 1:23:48from ton six one eight inject, turbulent energy stirring the
- 1:23:54gas and. Preventing collapse only once the quasar shuts down
- 1:23:59and turnmbulance dissipates can star formation. Proceed efficiently temperature offers.
- 1:24:05Another factor molecular gas must cool to about ten kelvin to.
- 1:24:10Form stars warmer gas has too much. Thermal pressure the
- 1:24:16quasar's radiation heats the gas directly through photoionization and INDIRECTLY
- 1:24:22through uv photons that dissociate molecules and free atoms that,
- 1:24:28then recombine. Releasing heat this heating maintains temperatures too high for.
- 1:24:34Star formation magnetic fields add. Additional complexity molecular gas contains
- 1:24:42embedded magnetic fields that provide extra support against. Gravitational collapse
- 1:24:49field strengths and geometries remain poorly constrained FOR t n six,
- 1:24:54one eight but analogy with other systems suggests fields player
- 1:24:59a set. Significant role turbulence can amplify fields through. Dynamo
- 1:25:05action strong fields, resist compression further suppressing. Star formation all
- 1:25:13these factors combine To keep ton six to one eight
- 1:25:16nebula in a state of, suspended potential vast amounts of
- 1:25:20gas capable of forming stars but prevented from doing so
- 1:25:25by the quasar's. Ongoing activity this state won't. Last forever
- 1:25:31eventually the gas supply, runs low, accretion slows the, quasar
- 1:25:37dims and. Conditions shift then the nebula, can cool fragment
- 1:25:44and form the next generation of stars that will comprise the.
- 1:25:49Mature galaxy this suspended state represents a pivotal moment in.
- 1:25:54Cosmic history we're witnessing the transition between violent quasar drips
- 1:26:00an activity and the mature galaxy that will. Emerge afterward
- 1:26:04other systems at lower redshifts show us snapshots of later
- 1:26:09stages in. This process quasers, dimming, gas cooling star FORMATION
- 1:26:16igniting tn six one eight catches the system at peak
- 1:26:22activity maximum energy input before the inevitable. Decline begins how
- 1:26:29long does this? Phase last quasers don't. Shine forever their
- 1:26:34lifetimes depend on fuel supply and. Feeding efficiency for Systems
- 1:26:39like ton six, one eight typical quasar lifetimes range from
- 1:26:43tens to hundreds of millions, of years brief by, cosmic
- 1:26:48standards but long enough to profoundly reshape. Their environments the
- 1:26:54current bright phase might persist for another fifty million years
- 1:26:59before fuel depletion forces the black hole. Into dormancy what
- 1:27:04signals the transition from active. To dormant the accretion rate
- 1:27:09provides the. Key metric as long as sufficient gas reaches the,
- 1:27:13black hole the quaser. Continues shining once the, supply diminishes whether, through,
- 1:27:20consumption expulsion or changes in the, galactic environment the accretion,
- 1:27:26rate drops the, disk cools the, jets weaken the radiation.
- 1:27:32Field dims this happens gradually over millions, of years. Not
- 1:27:38suddenly during, this transition the nebula's fate. Becomes sealed without
- 1:27:44the quasar's, energy input, turbulence dissipates, heating stops magnetic. Fields
- 1:27:51decay the gas begins cooling, through radiation losing energy. To
- 1:27:56space molecular hydrogen excels. At cooling its rotation and vibration
- 1:28:02states efficiently radiate away. Thermal energy over several tens of millions,
- 1:28:08of years temperatures drop from hundreds of kelvin to the
- 1:28:13critical ten, kelvin threshold where gravitational collapse. Becomes inevitable once cooling,
- 1:28:20proceeds sufficiently, fragmentation begins the once uniform nebula breaks. Into
- 1:28:26clumps each clump contracts under its. Own gravity as, contraction continues,
- 1:28:32densities rise triggering. Further, collapse eventually these fragments become dense
- 1:28:39enough and hot enough at their cause to ignite. Nuclear
- 1:28:42fusion stars. Are born the process transforms the diffuse nebula
- 1:28:49into a, stellar population converting one hundred billion solar masses
- 1:28:54of gas into perhaps ten to twenty. Billion stars this
- 1:28:59star oh formation won't happen uniformly throughout. The nebula different
- 1:29:04regions will form stars at different times. And rates the
- 1:29:09densest regions, Collapse first the most turbulent regions. Resist collapse
- 1:29:15longest regions with stronger magnetic fields form stars. More slowly
- 1:29:21the result is, a complex extended period of star formation
- 1:29:26lasting hundreds of millions. Of years what kind of galaxy
- 1:29:31emerges from. This process the answer depends on, many factors
- 1:29:36the nebula's, angular momentum its, density distribution the history of
- 1:29:41mergers with. Other galaxies the massive black hole at the
- 1:29:45center suggests a massive elliptical. Galaxy. Forms eventually ellipticals contain old,
- 1:29:52stellar populations, little gas and limited ongoing star formation consistent
- 1:29:59with the cism that consumed or expelled most of its
- 1:30:02gas during an earlier. Active phase the host galaxy likely
- 1:30:07already contains some older stars Formed before ton six one
- 1:30:12eight became. A quasar these stars are invisible, to us
- 1:30:17now outshone by the, quasar's brilliance but they exist orbiting the,
- 1:30:22black hole contributing to the galaxy's. Total mass the nebula
- 1:30:27will add to this, existing population creating multiple generations of
- 1:30:33stars with different ages. And compositions can we see examples
- 1:30:38of this process at. Later. Stages yes astronomers study post,
- 1:30:43starburst galaxies systems that recently ceased forming stars after an.
- 1:30:48Intense burst these objects show strong absorption lines from massive
- 1:30:54stars that formed within the past, billion years but lack
- 1:30:58the emission lines in dating ongoing. Star formation they Represent
- 1:31:04what tons six hundred eighteen's host might look like a
- 1:31:08few billion years. From now we also study massive elliptical
- 1:31:13galaxies in the, nearby universe the descendants of systems LIKE
- 1:31:18t n six. One eight these contain ancient, stellar populations
- 1:31:24dormant super massive, black holes and. Little gas their star's
- 1:31:29orbit in random directions rather than in, organized discs suggesting
- 1:31:34formation through violent processes involving mergers. And Feedback The milky
- 1:31:41WAY'S neighbour m eighty seven provides, an example a massive
- 1:31:45elliptical with a five point four billion solar mass, black
- 1:31:50hole now quiet after its quaser phase ended. Long ago
- 1:31:55tons six one eight's nebula encodes the galaxy's future in its.
- 1:31:59Present structure the total gas mass determines the final. Stellar
- 1:32:05mass the velocity structure determines the. Galaxy's rotation the density
- 1:32:11distribution determines where. Stars form reading this information requires detailed
- 1:32:18observations that push current instruments to. Their limits the alignment
- 1:32:23between the nebula and the radio jets reveals something crucial
- 1:32:28about the. System's geometry jets emerge perpendicular to the accretion
- 1:32:34disc following the black hole's. Spin axis the fact that
- 1:32:40the molecular outflow and circumgalactic medium both align with this
- 1:32:44axis indicates the jets have shaped the gas distribution on
- 1:32:49scales from thousands to hundreds of thousands of. Light years
- 1:32:55this shaping happens through. Momentum transfer jets carrying no enormous.
- 1:33:00Kinetic energy when they collide with, surrounding gas they transfer
- 1:33:05momentum pushing gas outward. And sideways the collision, creates shocks
- 1:33:12abrupt increases in pressure and temperature that heat and compress.
- 1:33:17The gas these shocks drive the, molecular outflow launching gas
- 1:33:23at hundreds of kilometers per second away from the. Galaxy's
- 1:33:27centre but jets do more than push. Gas around they
- 1:33:31also inject energy throughout. The nebula high energy particles streaming
- 1:33:36along the jets interact with surrounding matter through collisions and.
- 1:33:41Electromagnetic interactions this heats the gas and generates radiation across.
- 1:33:48The spectrum, the process called jet, driven heating helps maintain
- 1:33:54the nebula's elevated temperature and prevents premature. Star formation magnetic
- 1:34:01fields play a critical but poorly. Understood role the jets
- 1:34:06themselves contain strong magnetic fields field lines wound up by
- 1:34:12the rotating accretion disc and carried outward by. Flowing plasma
- 1:34:17these fields extend into, the nebula threading through. The gas
- 1:34:23field pressure provides additional support against. Gravitational collapse field tension
- 1:34:29can accelerate gas perpendicular to. Field lines understanding the magnetic
- 1:34:35field structure remains a major. Observational challenge different regions of
- 1:34:40the nebula likely have different magnetic field strengths. And geometries near,
- 1:34:46the jets fields are strong and, well organized aligned with the.
- 1:34:50Jet direction farther out fields weaken and become more tangled due.
- 1:34:56To turbulence in the densest clump fields may be compressed.
- 1:35:02And amplified this complexity makes modeling the system. Extremely difficult
- 1:35:09the circumgalactic medium represents the nebula's, outer, envelope gas extending
- 1:35:15to hundreds of, kilo parsex but not directly expelled by jets.
- 1:35:19Or winds this gas has a different origin than the.
- 1:35:23Inner outflow it might be primordial material that never fell into.
- 1:35:28The galaxy it might be gas expelled by earlier. Feedback
- 1:35:33episodes it might be material tidily stripped from smaller galaxies
- 1:35:39merging with. The host its presence indicates a complex history
- 1:35:43of gas flows into and out of. The galaxy this
- 1:35:48outer gas reservoir serves another function beyond future. Star formation
- 1:35:53it regulates the. System's evolution as the quasar expels gas
- 1:35:59from the, inner regions this outer reservoir can flow, back
- 1:36:03inward potentially reigniting accretion and restarting. The quasar this creates
- 1:36:10a feedback cycle where active and dormant phases alternate over
- 1:36:15hundreds of millions. Of years where the ton six one
- 1:36:19eight has experienced previous cycles. Remains unknown the mass budget provides.
- 1:36:25Important constraints the black hole contains forty to sixty six billion,
- 1:36:31solar masses depending on. The measurement the nebula contains one
- 1:36:36hundred billion solar masses. Of gas the existing stellar population
- 1:36:42likely contains several hundred billion, solar masses though we can't observe.
- 1:36:48It directly the total baryonic mass in the system exceeds
- 1:36:53five hundred billion, solar masses comparable to the most massive
- 1:36:57galaxies in. Today's universe dark matter dominates the. Total mass
- 1:37:04the galaxy sits within a dark matter halo containing perhaps
- 1:37:08several trillion. Solar masses this dark matter provides the gravitational
- 1:37:14potential well that holds the. System together, without it the
- 1:37:20violent feedback from the quaser would have dispersed the. Nebula
- 1:37:24entirely dark matter's gravity keeps everything bound despite the intense.
- 1:37:30Radiation pressure the interplay between baryonic matter and dark matter
- 1:37:35shapes the. Galaxy structure baryons cool and concentrate toward, the
- 1:37:41center where they form stars and feed the. Black hole
- 1:37:45dark matter remains distributed more broadly in a roughly. Spherical
- 1:37:49halo the ratio between baryonic and dark matter mass in
- 1:37:54the central regions exceeds the cosmic average because baryons have
- 1:37:59concentrated things through, dissipative processes while dark. Matter cannot chemical
- 1:38:05composition adds another layer. Of complexity the Gas in ton
- 1:38:10six hundred eighteen's nebula isn't pure hydrogen. And helium it,
- 1:38:15contains metals elements heavier than helium produced by. Stellar nucleosynthesis,
- 1:38:22these metals though comprising only a small fraction, by mass
- 1:38:27profoundly affect the. Gas's behavior they enhance cooling through, Emission
- 1:38:32lines they, provide opacity affecting. Radiation transfer they eventually become
- 1:38:40incorporated into planets. And life where do these metals? Come
- 1:38:45from stars that formed earlier in the host galaxy or
- 1:38:50in smaller galaxies that merged. With it these stars lived
- 1:38:55their lives fused lighter elements into, heavier ones and expect
- 1:39:00old material through stellar winds or supernova explosions that enriched
- 1:39:05material mixed with, primordial gas raising. The metallicity the current
- 1:39:12Metallicity in ton six hundred eighteen's nebula likely reaches twenty
- 1:39:16to fifty percent of the, solar value not pristine but
- 1:39:21not fully. Enriched either this intermediate metallicity tells us about the.
- 1:39:27Galaxy's history it formed stars before becoming. A quasar those
- 1:39:32stars produce the metals we, now observe but the majority
- 1:39:37of star formation hasn't. Happened yet that awaits the. Nebula's
- 1:39:42collapse after the quasar, shuts down the final stellar population
- 1:39:48will have higher metallicity than the current nebula because ongoing
- 1:39:53star formation will continue enriching the gas or the spatial
- 1:39:58distribution of Metals within when the nebula likely, isn't uniform
- 1:40:03regions closer to the black hole experienced more intense radiation,
- 1:40:08and heating possibly affecting. Chemical processes regions where jets interact
- 1:40:14with gas might show different compositions due to. Shock chemistry
- 1:40:21mapping metallicity variations requires spectroscopic observations at, multiple positions observations
- 1:40:28that challenge current. Instrumental capabilities dust adds. FURTHER complications a
- 1:40:35small fraction of metals condenses into. Solid grains dust particles
- 1:40:40typically smaller than. A micron these grains affect radiation transfer
- 1:40:46by absorbing and. Scattering light they also catalyze molecule formation
- 1:40:52by providing surfaces where atoms can meet. And bond the
- 1:40:56amount and distribution of Dust in tons six hundred eighteen's
- 1:41:01nebula remain, poorly constrained but certainly affect the. System's evolution
- 1:41:07observing dust directly requires. Infrared observations dust absorbs ultraviolet and
- 1:41:14optical light from, the quasar, heats up and re radiates in.
- 1:41:18The infrared the resulting infrared emission provides information about, dust,
- 1:41:24mass temperature and Distribution for ton six. One eight such
- 1:41:31observations require space based. Infrared telescopes ground based instruments can't
- 1:41:38access the relevant wavelengths due to. Atmospheric absorption future observations
- 1:41:44will revolutionize. Our Understanding The James Web space telescope's infrared
- 1:41:50capabilities can probe the dusty Regions around ton six. One
- 1:41:55eight the extremely, large telescope once, oper rational will provide
- 1:42:01unprecedented spatial resolution in optical and. Infrared light next generation
- 1:42:08radio arrays will map molecular gas with. Exquisite detail these
- 1:42:13facilities Will transform ton six' one eight from a distant
- 1:42:18curiosity into a detailed laboratory for. Studying galaxy evolution what
- 1:42:24Questions remain unanswered many we don't know the precise three
- 1:42:29dimensional geometry. Of the nebula current observations provide projections, on
- 1:42:35the sky but. Not depth information we don't know the
- 1:42:40detailed velocity field throughout. The entire structure we don't know
- 1:42:44how magnetic. Fields vary spatially we don't know. The metallicity
- 1:42:49distribution we don't know. The dust content we don't know
- 1:42:54whether the host galaxy has experienced. Previous active phases answering
- 1:43:00these questions requires coordinated observing campaigns using multiple telescopes across.
- 1:43:06The electromagnetic spectrum radio observations. Map molecular gas infrared observations
- 1:43:14probe dust and. Obscured star formation optical observations. TRACE ionized
- 1:43:20gas x ray observations reveal the hottest material near. The
- 1:43:25black hole each wavelength provides complementary information about different. Components
- 1:43:31and processes the challenge lies in combining these diverse observations
- 1:43:37into a. Coherent physical model different observations sample, different, physical,
- 1:43:43conditions temperatures. Densities ionization states connecting them requires detailed modeling, of,
- 1:43:52radiative transfer. Chemistry and dynamics computational simulations help by predicting
- 1:44:00what observations should show for, different model parameters allowing comparison between.
- 1:44:06Theory and observation ton six one eight represents more than.
- 1:44:12An individual object it's a window, into cosmic dawn showing
- 1:44:18us galaxy. Formation in action by studying it and similar systems,
- 1:44:23at high redshift we reconstruct the processes that. Built today's
- 1:44:28galaxies we learn how black holes and. Galaxies co evolve
- 1:44:34we understand how feedback. Regulates star formation we trace the
- 1:44:39chemical enrichment. Of the universe each distant quasar adds another
- 1:44:43piece to. This cosmic puzzle the broader implications extend. Beyond
- 1:44:48individual systems ton six hundred eighteen's existence constrains theoretical models of.
- 1:44:55The early universe how common we was such. Massive black
- 1:44:59holes current surveys suggest ultramassive black holes are rare. But
- 1:45:05not unique several candidates exist. With comparable masses their scarcity
- 1:45:12indicate special conditions were needed. For their formation perhaps they
- 1:45:17required unusually dense environments where gas. Could collapse rapidly perhaps
- 1:45:23they formed from direct collapse scenarios rather. Than stalar remnants
- 1:45:29perhaps they grew through exceptionally efficient accretion or. Rapid merger
- 1:45:34sequences population. Studies matter here by cataloging all known ultramassive
- 1:45:40black holes and analyzing, their properties statistically astronomers can infer
- 1:45:47the conditions. That produce them do they preferentially appear in?
- 1:45:52Certain cosmic environments do they show correlations with? Particular galaxy
- 1:45:58types do their host galaxies? Share common characteristics these questions
- 1:46:06guide searches for additional examples and inform simulations of. Early
- 1:46:11structure formation the theoretical framework. Faces genuine challenges standard accretion models.
- 1:46:19PREDICT growth timescales a stellar mass black hole of ten
- 1:46:24solar masses Accreting at the eddington limit would require hundreds
- 1:46:29of millions of years to reach a, million solar masses
- 1:46:33reaching forty billion solar masses within. Three billion years the
- 1:46:39Time available given ton six one eighths redshift pushes these models.
- 1:46:44To Their limits super eddington accretion. Provides one solution if
- 1:46:50black holes Temporarily exceeded the eddington limit during particularly, gas
- 1:46:54rich phases they could grow faster than. Conventional models allow
- 1:47:00another possibility involves massive seed black holes instead of starting
- 1:47:06from stellar remnants of tens. Of solar masses perhaps some
- 1:47:11black holes began with thousands or even millions. Of solar
- 1:47:15masses direct collapse, scenarios propose that, under certain conditions massive
- 1:47:22gas clouds could collapse directly into black holes without. Forming
- 1:47:27stars first these scenarios require specific circumstances pristine gas lacking
- 1:47:35metals that would enable, cooling and fragmentation intense radiation fields preventing,
- 1:47:41normal star formation rapid infall preventing feedback from. Disrupting the
- 1:47:46collapse whether such conditions existed in the early. Universe remains
- 1:47:51debated merger driven growth offers. Yet another pathway if multiple
- 1:47:58smaller black holes merged repeatedly in, dense galactic environments the
- 1:48:03combined mass. Could grow rapidly each merger would release gravitational
- 1:48:08waves and potentially kick the remnant black, hole through recoil
- 1:48:14but in sufficiently massive, dark matter halos the black hole
- 1:48:18would remain gravitationally bound and continue growing through subsequent. Mergers
- 1:48:24and accretion numerical simulations, explore these scenarios calculating expected growth
- 1:48:31rates and comparing them to observations The physics near ton
- 1:48:36six one eight's event horizon. Defies everyday intuition, at one
- 1:48:42thousand three, hundred astronomical Units the schwarz child radius exceeds
- 1:48:47the size of our entire solar system Forty times over
- 1:48:52light itself would take weeks to cross from one side.
- 1:48:55To the other a beam of light traveling at three
- 1:48:58hundred thousand, kilometers per second traversing a distance so vast
- 1:49:04that our planetary system becomes. Insignificant by comparison matter approaching
- 1:49:10this boundary experiences gravitational forces strong enough to tear apart
- 1:49:17stars long before crossing. The event horizon tidal forces scale
- 1:49:23inversely with black hole mass for equal distances. From, the
- 1:49:26center paradoxically this means crossing the event horizon of an
- 1:49:32ultra massive Black hole like ton six one eight would
- 1:49:36be less violent than crossing into a stellar. Mass black hole,
- 1:49:41the tidal gradient the difference in gravitational force across, an
- 1:49:45object's extent decreases for. Larger black holes an Astronaut falling
- 1:49:50into ton six one eight could theoretically cross the event horizon.
- 1:49:55Without immediate spaghettification the fatal tidal forource would manifest closer
- 1:50:01to the singularity deep within the. Event horizon's interior this
- 1:50:07counterintuitive result highlights. General relativity subtleties the event horizon isn't.
- 1:50:13A physical surface nothing marks. Its location locally an in
- 1:50:18falling observer would notice nothing, special upon, crossing no, wall
- 1:50:24no barrier. No sudden, change only later, attempting to escape
- 1:50:30would they discover the impossibility. Of their situation all future directed.
- 1:50:36Paths lead inward no amount of thrust. Could reverse course
- 1:50:43the event horizon represents a one way membrane in. Space
- 1:50:47time itself hawking radiation. Introduces quantum effects even black holes
- 1:50:54emit thermal radiation due to quantum fluctuations near. The event
- 1:50:58horizon the temperature depends. Inversely on mass stellar mass black
- 1:51:04holes have temperatures of millionths of a kelvin ton six
- 1:51:10one eight temperature would be proportionally lower trillionths, of a
- 1:51:15kelvin far colder than the. Cosmic microwave background such black
- 1:51:19holes gain mass from background radiation faster than they Lose mass.
- 1:51:24To hawking radiation they grow. Rather than evaporate only in,
- 1:51:31the distant future after stars cease forming and the universe
- 1:51:35cools below Even the, minuscule hawking temperature would ultra massive black.
- 1:51:41Holes begin evaporating the time scale for complete evaporation scales
- 1:51:47as the cube of the mass for ton, Six hundred
- 1:51:51eighteen this exceeds ten to the one, hundredth power years
- 1:51:56a number so large it dwarfs the current age. Of
- 1:51:59the unit, by unimaginable factors the black hole would outlast,
- 1:52:05not just stars but the very concept of conventional time in.
- 1:52:09Any recognizable sense the information. Paradox lurks here what happens
- 1:52:16to information that falls into? A black hole does it
- 1:52:20disappear violating quantum? Mechanics unitarity principle does it Somehow escape?
- 1:52:27Through hawking radiation does it remain encoded on. The event
- 1:52:31horizon these questions remain unresolved despite decades of THEORETICAL work
- 1:52:40to n. Six one eight like, all black holes embodies
- 1:52:45this fundamental tension between general relativity, and quantum, mechanics string
- 1:52:51theory and other. Quantum gravity. Approaches proposed solutions perhaps black holes,
- 1:52:57aren't truly black but rather fuzzballs quantum objects. Without event
- 1:53:03horizons perhaps the interior connects to other universes through. Wormhole
- 1:53:09like structures perhaps information is preserved, through holographic principles where
- 1:53:15the event horizons surface encodes. The volume's information none of
- 1:53:20these ideas, have achieved consensus and experimental tests remain far.
- 1:53:26Beyond current capabilities Gravitational waves from ton six hundred eighteen's
- 1:53:31formation and growth Might carry information when, black holes merge
- 1:53:37they produce gravitational waves ripples in, space time itself propagating.
- 1:53:42At light Speed detectors Like ligo and virgo observe mergers
- 1:53:48as stellar. Mass black holes future space Based detectors like
- 1:53:53lisa will access lower frequencies corresponding to supermassive. Black hole
- 1:53:59mergers detecting gravitational waves from ultramassive black hole mergers would
- 1:54:06require even, more ambitious instruments but the scientific payoff. Would
- 1:54:11be enormous such detections would reveal, black, hole spins masses
- 1:54:17and orbital parameters with precision impossible. Through electromagnetic observations they
- 1:54:24would test general relativity in the strong field regime where
- 1:54:28spacetime curvature. Reaches extreme values they would provide independent mass
- 1:54:34measurements to compare. With spectroscopic estimates they would probe the
- 1:54:40merger history of massive galaxies. Across cosmic time the challenge
- 1:54:46lies in. The time scales gravitational wave signals from ultramassive
- 1:54:51black holes have periods of. Days to years detecting them
- 1:54:57requires continuous monitoring over, its extended periods correlating data from
- 1:55:03multiple spacecraft to. Achieve sufficient sensitivity the signals. Would be
- 1:55:09weak even the most massive mergers produce only tiny strains
- 1:55:13in space time by the time, waves reach us but
- 1:55:17the scientific returns justify. The technological investment ton six one
- 1:55:24eight jets. Deserve closer examination radio observations reveal powerful outflows
- 1:55:30carrying enormous energy into. The surrounding medium the jet launching
- 1:55:36mechanism involves complex magnetohydrodynamics near. The event horizon magnetic fields
- 1:55:43threading the accretion disc become twisted and amplified. By differential
- 1:55:48rotation the fields extract rotational energy from the black hole
- 1:55:53Itself through the, blandford's nagic process channeling it. Into collimated
- 1:55:59outflows traveling at, Near light speeds these relativistic jets interact,
- 1:56:05with ambient gas creating shock. Waves and turbulence they inflate
- 1:56:11enormous radio emitting bubbles visible in. Low frequency observations they
- 1:56:17deposit energy, across vast regions heating gas and preventing. It
- 1:56:22from cooling. And forming stars this feedback mechanism helps explain
- 1:56:28why the most massive galaxies today contain relatively little cold
- 1:56:32gas despite. Their enormous masses their central black holes expelled
- 1:56:37or heated the gas during. Previous Active phases for ton,
- 1:56:42six hundred eighteen the jets Align with the lyman alpha.
- 1:56:47Nebula's major axis this. Alignment isn't coincidental the jets shape
- 1:56:54gas distribution by pushing material perpendicular to. Their propagation direction
- 1:57:01gas swept into the jet's, path, gets accelerated. Heated or
- 1:57:06dispersed gas lying perpendicular to the jets experiences, less direct
- 1:57:12interaction allowing it to accumulate into the. Observed nebula structures
- 1:57:18the jet power, must be substantial perhaps ten to the
- 1:57:22power of forty six, ergs per second equivalent to the
- 1:57:26luminosity of. A trillion suns magnetic fields throughout the system.
- 1:57:31Remain poorly constrained theory predicts strong fields near the black
- 1:57:36hole where. They drive jets fields in the, accretion, disk
- 1:57:41channel plasma and affect angular momentum transport fields in the
- 1:57:46nebula might influence gas dynamics, and star formation but observing
- 1:57:53these fields. Directly proves difficult polarization measurements provide indirect evidence
- 1:58:00showing that radiation has interacted. With magnetic fields future radiopolarimetry
- 1:58:07could map field. Structures in detail the host galaxy's stellar population,
- 1:58:12remains essentially invisible overwhelmed. By the quasars brilliance estimates suggest
- 1:58:19it likely contains hundreds of, billions of stars based on
- 1:58:24the black hole galaxy mass relationship observed. In nearby, systems
- 1:58:30THIS Relationship the, m sigma relation correlates black hole mass
- 1:58:36with the velocity dispersion of stars in. The galactic Bulge
- 1:58:42extrapolating to ton six one eight suggests a galaxy mass
- 1:58:48exceeding a. Trillion solar masses such a galaxy would rank
- 1:58:52among the most. Massive ever formed its dark matter halo would,
- 1:58:57be correspondingly enormous perhaps containing ten trillion solar. Masses or
- 1:59:03more the halo provides the gravitational well within, which gas
- 1:59:07accumulates galaxies merge. And structure grows understanding the halo's properties requires.
- 1:59:16Gravitational lensing observations if a background galaxy Fortuitously aligns with ton,
- 1:59:23six one eight its light would be, bent and magnified
- 1:59:27revealing the. Foreground mass distribution such, alignments are rare. But
- 1:59:33not impossible the cosmic. Web context matters large scale structure
- 1:59:39simulations show that the most massive halos form at the.
- 1:59:44Intersections of filaments the nodes where cosmic structure IS densest
- 1:59:50to n six one eight likely occupies such a node
- 1:59:54positioned where. Multiple filaments meet gas flowing along filaments converges,
- 2:00:00at these locations providing abundant fuel for black hole growth.
- 2:00:06And star formation the system's environment probably included, numerous companion
- 2:00:12galaxies some of which may have merged with the. Host
- 2:00:15over time simulations help interpret observations by predicting what structures
- 2:00:21should look like. Under different assumptions cosmological simulations follow the
- 2:00:27evolution of dark matter from early density fluctuations to. Present
- 2:00:32day structures, adding gas, physics star formation and black hole
- 2:00:38feedback allows comparison. With observed galaxies the simulations that best
- 2:00:45match observations constrain physical processes. And parameter values refining our
- 2:00:52understanding of. How galaxies form ton six hundred eighteen provides
- 2:00:57a particularly stringent test. Its extreme properties, ultramassive black, hole
- 2:01:04enormous nebula powerful jets must all emerge naturally from physical
- 2:01:09processes operating in. The early universe Simulations that produce ton
- 2:01:15six one eight like systems reveal which conditions and. Mechanisms
- 2:01:20were necessary they guide observers toward key measurements that would distinguish.
- 2:01:26Between competing models they suggest what future telescopes should look
- 2:01:31for when studying similar. High redshift quasers future telescopes will.
- 2:01:36Transform Our Understanding The James, web space, telescope already operational
- 2:01:44can detect Infrared light from ton six one, eight's host
- 2:01:48galaxy piercing through dust that. Obscures optical observations web sensitivity
- 2:01:54allows imaging of structures near the quasa that, were previously
- 2:01:58invisible potentially revealing, star formation, regions galactic morphology. And companion
- 2:02:06objects the, extremely large telescope scheduled for completion in the,
- 2:02:12late twenty twenties will provide unprecedented angular resolution. From the
- 2:02:18ground its thirty nine metre mirror will resolve features ten
- 2:02:23times smaller than current, telescopes can achieve possibly distinguishing Different
- 2:02:29regions within ton six one eighths accretion disc or detecting
- 2:02:35individual star clusters in. The host galaxy square kilometer array
- 2:02:41radio observations will map the jets and magnetic fields. With
- 2:02:46exquisite detail this instrument's collecting area equivalent to a square kilometer,
- 2:02:53of radio antennas will detect faint emissions from outflows and
- 2:02:58trace gas dynamics. Throughout the system combined with alma's, MOLECULAR
- 2:03:04line observations ska data will reveal how jets shape the
- 2:03:09circumgalactic medium and regulate star formation across hundreds of thousands.
- 2:03:15OF light years x Ray observatories like athena planned for
- 2:03:20the twenty thirties will probe the high Energy physics near
- 2:03:24ton six one. EIGHTS event horizon x rays trace the
- 2:03:29hottest gas in the accretion disks inner regions where temperatures reach.
- 2:03:35Millions of degrees SPECTROSCOPY of these x rays, reveals chemical,
- 2:03:40abundances ionization, states and velocities constraining accretion physics and testing
- 2:03:47general relativity in. Extreme gravitational FIELDS time resolved x ray
- 2:03:53observations could detect variability caused by orbiting hotspots or. Magnetic
- 2:03:59reconnection events gravitational wave detectors Might eventually sense ton six.
- 2:04:05One eight's influence CURRENT detectors like ligo and virgo aren't
- 2:04:11sensitive enough to detect gravitational waves from individual, supermassive black
- 2:04:17holes but future space based DETECTORS concepts like lisa will
- 2:04:23observe lower frequency waves produced by merging. Supermassive Black holes
- 2:04:29if ton six one eight's black hole, formed through mergers as,
- 2:04:34some theories suggest similar events occurring today would. Generate detectable
- 2:04:39signals these observations would reveal, black, hole spins masses and.
- 2:04:45Merger histories directly multi messenger astronomy combines electromagnetic observations with gravitational.
- 2:04:52Waves And neutrinos if ton six one eight jets accelerate
- 2:04:59part of to, ultra high energies neutrino detectors might register
- 2:05:04signals from nuclear interactions in. The jet plasma neutrinos travel,
- 2:05:10unimpeded through space arriving simultaneously with photons from, the same
- 2:05:15event despite. Traversing different paths Detecting neutrinos from ton six
- 2:05:22one eight would confirm hadronic acceleration mechanisms and. Constrain jet
- 2:05:28composition statistical studies of similar. Objects provide context ton six one.
- 2:05:36Eight isn't unique it's the most massive example of a
- 2:05:40population surveys identifying hundreds of high redshift quasers enable statistical analyzes,
- 2:05:47of their properties. Clustering and evolution the distribution of, black hole,
- 2:05:53masses accretion rates and host galaxy properties reveals patterns that individual.
- 2:05:59Objects Can't show comparing ton six hundred eighteen to its
- 2:06:05peers highlights what makes it exceptional and what characteristics are
- 2:06:10typical for. Ultra massive systems quasar luminosity functions track the
- 2:06:16number density of quasars at different. Luminosities and redshifts these
- 2:06:22functions show that luminous quasars were more common in, the
- 2:06:26early universe peaking around redshift two to three when the
- 2:06:30universe was two to three. Billion years old ton six
- 2:06:36one eight at redshift two point two formed during. This
- 2:06:40peak epoch the decline in quaser activity at later times
- 2:06:45suggests that black hole growth rates decreased as gas supplies
- 2:06:50dwindled and feedback mechanisms became more effective. At regulating accretion
- 2:06:56clustering analyzes measure how quasers are distributed in space relative
- 2:07:01to the. Large scale structure quasers occupy the most massive,
- 2:07:06dark matter halos clustered in over dense regions where galaxy formation.
- 2:07:11Is most active ton six hundred eighteen's position within, the
- 2:07:17cosmic web determines its environment and. Influences its evolution if
- 2:07:22located at, a filament intersection it would have access to
- 2:07:26copious gas supplies flowing. Along multiple filaments if isolated in,
- 2:07:32a massive halo its fuel supply would depend more on
- 2:07:36internal processes. Like galaxy mergers chemical evolution studies trace element abundances.
- 2:07:44Through cosmic history early generation stars produce, light, elements, Carbon
- 2:07:50oxygen nitrogen later generation synthesized, heavier, elements. Iron silicon magnesium
- 2:07:58the spectrum of ton n six one eight s broad
- 2:08:01line region show strong emission, lines, from carbon, nitrogen and
- 2:08:06oxygen indicating that significant stellar nucleosynthesis had already occurred by
- 2:08:12the time. The quasar formed the gas fueling the black
- 2:08:16hole had been enriched by previous, generations of stars constraining
- 2:08:22the timeline of star formation in. The host galaxy metallicity
- 2:08:26measurements quantify these abundances. Relative to hydrogen solar metallicity refers
- 2:08:34to the chemical Composition. Of our sun about two per
- 2:08:38cent of its mass consists of elements. Heavier than helium
- 2:08:43measurements of ton six hundred eighteen s broad line region
- 2:08:47suggest metallicities approaching or, exceeding solar values implying substantial. Prior
- 2:08:53star formation this enrichment occurred within the first billion years of,
- 2:08:58the galaxy's existence requiring rapid star formation rates and efficient
- 2:09:04mixing of stellar rejector throughout. The interstellar medium dust observations.
- 2:09:10Provide additional constraints dust grains form when heavy elements condense
- 2:09:16in the cool outflows. From dying stars infrared observations detect
- 2:09:22thermal emission from dust heated by starlight. Or quasar radiation
- 2:09:28the infrared luminosity indicates the dust, mass and temperature revealing
- 2:09:33the star formation history and the balance between dust. Production
- 2:09:38And destruction for ton, six one eight infrared observations show
- 2:09:45substantial dust consistent with, vigorous star formation either currently ongoing
- 2:09:51or in. The Recent past star formation rates in the
- 2:09:55host galaxy remain uncertain due to contamination. From quasar lfe
- 2:10:01typical estimates for luminous quasars at similar redshifts suggest rates
- 2:10:06of hundreds to thousands of solar. Masses Per year if
- 2:10:11ton six one eights host galaxy form stars, at this
- 2:10:14pace it would build a stellar mass exceeding a trillion
- 2:10:18solar masses within. A billion years consistent with the implied
- 2:10:23galaxy mass from the black. Hole galaxy correlation such rapid
- 2:10:27star formation requires enormous gas reservoirs and efficient conversion of.
- 2:10:32Gas into stars stellar initial mass. Function affects predictions this
- 2:10:39function describes the relative numbers of stars formed. AT different
- 2:10:43MASSES a standard imf produces mostly low mass stars with.
- 2:10:49Fewer massive stars alternative IMFs with more massive stars would
- 2:10:54yield different, chemical, enrichment patterns luminosities. And feedback effects observations
- 2:11:01of stellar populations in distant galaxies SUGGEST that the imf
- 2:11:06may vary with, redshift or environment complicating interpretations of star
- 2:11:12formation rates. And chemical evolution supernova feedback influences both star
- 2:11:18formation and. Black hole growth massive stars explode as supernovae
- 2:11:24after only a, few million years injecting energy and momentum.
- 2:11:28Into surrounding gas this feedback heats, and disperses gas potentially suppressing.
- 2:11:34Subsequent star formation, in dense environments supernova might trigger star
- 2:11:41formation by compressing. Nearby gas clouds the balance between suppression
- 2:11:47and triggering determines the overall star formation efficiency and the
- 2:11:52time scale over which galaxies build. Their stellar populations active
- 2:11:58galactic nucleus pias feedback operates. On, larger, scales, radiation pressure
- 2:12:04jets and winds driven by the central black hole affect
- 2:12:09the entire galaxy and. Its circumgalactic medium this feedback can
- 2:12:14quench star formation by heating, or expelling gas explaining why
- 2:12:20the most massive galaxies observed today have relatively low star
- 2:12:24formation rates despite their. Large gas reservoirs ton six one
- 2:12:29eighth's powerful feedback likely regulate star formation, in its host
- 2:12:35potentially transitioning the galaxy from an active star forming phase
- 2:12:40to a. Quiescent passive phase observations of other massive galaxies
- 2:12:47suggest this transition occurred in the past. Several billion years
- 2:12:52massive elliptical galaxies in the nearby universe contain old stellar
- 2:12:57populations with little. Ongoing star formation these galaxies likely experienced
- 2:13:04intense starburst phases, at high redshift then quenched due to
- 2:13:09agn feedback or exhaustion. Of gas supplies ton six one
- 2:13:16eight may represent an earlier stage in, this evolutionary sequence
- 2:13:21captured during the peak of both black hole growth, and
- 2:13:24star formation before feedback mechanisms shut. Down both processes merger.
- 2:13:30Histories affect structure hierarchical structure formation predicts that massive galaxies
- 2:13:36assembled through numerous mergers. Of smaller galaxies each merger brings
- 2:13:41gas that can fuel starbursts and. Black hole accretion the
- 2:13:45stellar populations formed during different merger events have distinct, ages
- 2:13:50and metallicities creating complex distributions that Observations CAN potentially disentanglen
- 2:14:00n six one eight's host likely experienced, multiple major mergers
- 2:14:05each contributing to its current mass and triggering episodes. Of
- 2:14:10quaser activity dynamical modeling. Reconstructs these histories simulations that reproduce
- 2:14:17observed properties reveal. Plausible Formation pathways for ton, six hundred
- 2:14:22eighteen models must explain how the black hole grew so
- 2:14:27massive so quickly while simultaneously building the host. Galaxy's stellar
- 2:14:32population successful models typically invoke either continuous rapid accretion from
- 2:14:39dense gas streams or episodic bursts of accretion. Triggered by
- 2:14:44mergers both scenarios require specific initial conditions and environmental factors that,
- 2:14:52may be rare explaining why ultra massive Black holes like
- 2:14:57ton six hundred. Eighteen are uncommon observational biases. Affect discovery
- 2:15:03rates luminous quasers are easier to detect, than faint ones
- 2:15:08so surveys naturally find, the brightest examples like to n.
- 2:15:13Six one eight fainter quasers with smaller black holes might
- 2:15:17outnumber the ultra massive ones but remain undetected due to.
- 2:15:22Instrumental sensitivity limits correcting for these biases requires careful statistical
- 2:15:29analysis of, survey selection functions allowing astronomers to infer the
- 2:15:35true number density of black holes. At different masses variability
- 2:15:40studies track changes over time quasers vary in brightness due
- 2:15:45to fluctuations in accretion rate or. Changes In obscuration monitoring
- 2:15:51ton six one eight over months or years could reveal
- 2:15:56variability patterns that constrain the accretion disc. Side and structure
- 2:16:01shorter timescale variations probe smaller spatial regions closer to, the
- 2:16:06black hole while longer term trends reflect changes in the
- 2:16:10overall fuel supply. Or feedback processes spectroscopic monitoring detects changes in.
- 2:16:18Emission line profiles if the broad line, regions structure evolves
- 2:16:23line widths and. Intensities shift accordingly reverberation mapping exploits these
- 2:16:31changes to measure the region's size by timing the delay
- 2:16:35between continuum variations and Line response for ton. Six hundred
- 2:16:41eighteen such measurements would refine black hole mass estimates and
- 2:16:46test whether the broad line region's properties differ from those in.
- 2:16:50Less extreme systems polarization measurements reveal magnetic field geometries. And
- 2:16:57scattering processes light from the accretion disc becomes polarized through
- 2:17:04scattering off electrons or alignment of dust grains. By magnetic
- 2:17:08fields the degree and direction of polarization in code information, about,
- 2:17:15field strength orientation and the distribution. Of Scattering material for ton,
- 2:17:24six one eight polarization data, would constrain, jet magnetic fields and.
- 2:17:30Accretion disc structure complementing spectroscopic, and photometric observations the broader.
- 2:17:38Cosmological context matters ton six one eight formed during an
- 2:17:44epoch when the universe's structure. Was rapidly evolving the cosmic
- 2:17:48star formation rate peaked, around redshift two then declined as
- 2:17:53gas was consumed and feedback mechanisms. Became more efficient understanding
- 2:17:59why this transransition occurred requires Studying objects like ton six
- 2:18:04one eight that exemplify. The peak phase their properties constrain models,
- 2:18:11of gas, accretion star formation and feedback that. Govern galaxy
- 2:18:16evolution dark energy's influence becomes relevant on. The largest scales
- 2:18:22the accelerated expansion of the universe affects structure growth by.
- 2:18:26Counteracting gravitational collapse in, the distant future dark energy will
- 2:18:32prevent new structures from forming and eventually tear apart. Gravitationally
- 2:18:37bound Systems but during ton six, one eight's epoch dark energy's,
- 2:18:45effects were minimal allowing structures to grow rapidly. Through gravitational
- 2:18:50instability the current dominance of dark energy marks a transition point,
- 2:18:56in cosmic history after which structure. Formation slows dramatically ton
- 2:19:03six hundred eighteen offers a window into processes that. Shaped
- 2:19:08the universe its extreme properties ultra, massive black, hole intense,
- 2:19:13luminosity enormous nebula powerful jets reflect conditions in the early
- 2:19:20universe that. No longer prevail studying this system reveals how
- 2:19:25galaxies formed, from primordial gas how black holes grew to,
- 2:19:30dominate galactic centers and how feedback regulated the transformation from
- 2:19:36actively star forming systems. To passive ellipticals every observation adds
- 2:19:43another piece to. This cosmic puzzle the system's fate remains
- 2:19:48uncertain over. Cosmic time scales will the black hole continue,
- 2:19:53growing through mergers eventually exceeding. Theoretical mass limits will feed
- 2:19:59back mechanisms shut, down accretion permanently leaving. A quiescent remnant
- 2:20:06will the host galaxy, merge with neighbours triggering new? Episodes
- 2:20:11of activity these questions await answers that observations overcoming Decades
- 2:20:17will provide what we know today represents a beginning to
- 2:20:23n six' one eight challenges our understanding and pushes theoretical.
- 2:20:28Models to their limits it exemplifies the, universe's capacity for,
- 2:20:33extremes objects, so massive, so luminous so energetic that they redefine.
- 2:20:41What we consider possible in, studying this cosmic giant we
- 2:20:46confront fundamental questions about growth limits and the processes that
- 2:20:51govern the. Larger structures in existence, the numbers don't lie
- 2:20:56but they don't. Quite capture it either You now know
- 2:21:00that ton six hundred eighteen's event, horizon spans two thousand.
- 2:21:04Six hundred astronomical units you understand that light takes weeks.
- 2:21:09To cross its shadow you've grasped that it outmasses every star.
- 2:21:15In our galaxy combined but knowing these facts and truly
- 2:21:19comprehending them. Remain different things entirely your brain isn't. Wired
- 2:21:24for this scale evolution shaped your intuitions for, objects measured
- 2:21:29in meters, distances covered in hours, masses you can lift or.
- 2:21:34At least imagine lifting ton six hundred eighteen exists so
- 2:21:40far outside, this comfortable range that even armed with precise,
- 2:21:45measurements and careful comparisons you. Can't really picture it the
- 2:21:51best you can do is understand the relationships how it
- 2:21:56compares to, things slightly less incomprehensible building a ladder of
- 2:22:01analogies that points to ward but never. Quite reaches The
- 2:22:06truth what makes ton six hundred eighteen genuinely remarkable. Isn't
- 2:22:11just its size plenty of things in. The universe are
- 2:22:15large galaxy clusters span, Millions of light years cosmic voids stretch.
- 2:22:22Across hundreds of millions the observable universe itself measures ninety three.
- 2:22:29Billion light years across size alone. Doesn't make something special the.
- 2:22:34Remarkable aspect is concentration sixty six billion solar masses packed
- 2:22:40into a region you could traverse at light speed. In
- 2:22:43a few weeks that concentration creates gravitational fields so intense
- 2:22:49they warp space time into shapes that. Break your intuitive
- 2:22:52understanding it creates energy densities that shouldn't exist according. To
- 2:22:58some theoretical limits it produces feedback effects that reshape entire
- 2:23:04galaxies across hundreds of. Thousands of light years ton six
- 2:23:10one eight represents physics operating at the. Edge Of what's
- 2:23:14possible black holes can't grow arbitrarily large through accretion radiation pressure.
- 2:23:21Eventually prevents further growth theoretical calculations put this limit around
- 2:23:28fifty billion solar masses for, non spinning black holes potentially higher.
- 2:23:34For rapidly spinning ones ton six one eight sits, right
- 2:23:39at this boundary possibly already at its. Maximum accretion based mass,
- 2:23:44it's not just big it's as big as a black
- 2:23:47hole can get through. The standard growth mechanism the. Timeline
- 2:23:51makes it worse this object assembled its mass within three
- 2:23:56Billion Years. Of the big bang standard growth models. Struggle
- 2:24:01to explain this you can't simply start with a stellar
- 2:24:05mass black hole and grow it to sixty six billion
- 2:24:09solar masses in that time. Frame using conventional accretion. The
- 2:24:14math doesn't work. Something unusual happened either the seed black
- 2:24:21hole started much more massive than, stellar remnants typically provide
- 2:24:26or accretion preceded faster, than theoretical limits suggest or multiple
- 2:24:32massive black holes, merged in rapid succession or. All three
- 2:24:37occurred simultaneously we don't know. Which explanation is. Correct each
- 2:24:42has problems direct collapse scenarios require special conditions that may.
- 2:24:49Not Have been common super eddington. Accretion faces stability issues
- 2:24:55rapid merger. Sequences Seem statistically unlikely yet ton six,' one
- 2:25:01eight exists anyway. Indifferent to our theoretical difficulties the surrounding
- 2:25:08nebula adds, another layer to this puzzle one hundred billion
- 2:25:12solar masses of gas extending three hundred thirty Thousand Light years.
- 2:25:18Twice the milky way's diameter this, isn't just decoration its
- 2:25:24fuel it's the raw material for future star formation. Or
- 2:25:29continued black, hole growth the nebula structure aligned with the
- 2:25:34radio jets shows how the black hole has already shaped.
- 2:25:39Its environment on galactic scales radiation, and outflows have redistributed,
- 2:25:45gas heated it ionized it preventing it from. Cooling and
- 2:25:50collapsing into stars this feedback mechanism explains why massive galaxies today,
- 2:25:57contain relatively little cold, gas despite their enormous masses their
- 2:26:03central black holes expelled or heated most of. It during
- 2:26:07earlier active phases ton six one eight shows, us this
- 2:26:12process in action the moment when a quasar is actively
- 2:26:17regulating its own fuel supply and suppressing star. Formation throughout
- 2:26:22its host galaxy, eventually the fuel, runs out the quasar
- 2:26:26dims and the heated gas cools over hundreds of millions
- 2:26:30of years before forming. The next generation of stars that
- 2:26:35future state represents what astronomers call, a red and dead
- 2:26:39galaxy massive elliptical containing old stellar populations. With little ongoing
- 2:26:46star formation our observations suggest most massive ellipticals in the
- 2:26:52nearby universe went through quasar. Phases BILLIONS of years ago
- 2:26:56to n six one eight provides a, window into that
- 2:27:00earlier epoch showing us what these systems look. Like during
- 2:27:05their violent. Youth the jets deserve emphasis streams of plasma
- 2:27:12accelerated to ninety nine, point nine percent light speed carrying
- 2:27:17power equivalent to a trillion suns extending across hundreds. Of
- 2:27:22thousands of light, years these aren't side effects they're integral
- 2:27:27to how supermassive. Black holes influence their environments the jets inject,
- 2:27:33energy throughout the circumgalactic medium heating gas and maintaining it
- 2:27:38at temperatures. Too high for star formation they shape the
- 2:27:42distribution of gas on scales far larger than the accretion
- 2:27:46disk or. Even the host galaxy itself magnetic fields, thread
- 2:27:52through the entire system though. We can't observe them directly
- 2:27:58theory predicts strong, feels near the event horizon where they
- 2:28:02extract rotational energy from the spinning black hole and. Channel
- 2:28:07it into the jets fields in the accretion disk. Affect
- 2:28:13how matter spirals inward fields in the nebula might influence gas.
- 2:28:19Dynamics and future star formation understanding these fields requires polarization
- 2:28:26measurements and radio observations that push. Current instruments to their
- 2:28:32limits the, host galaxy remains essentially invisible, outshone by the
- 2:28:37central quasar despite potentially containing. Hundreds of billions of stars
- 2:28:43we can infer its properties from the black hole galaxy mass,
- 2:28:47relationship observed in nearby systems but. We can't observe IT
- 2:28:52directly future Telescopes Like Jwst or the extremely large, telescope
- 2:28:59might evently, resolve details but for now the galaxy is
- 2:29:04lost in the glare. Of the accretion discs brilliance this
- 2:29:08creates an odd situation where we know, more about the
- 2:29:12black hole an, object we can't see directly than, about
- 2:29:16the galaxy surrounding it which should. Be far easier to
- 2:29:21observe the black hole's mass comes from measuring velocities of
- 2:29:26orbiting gas. In the broad line region the, galaxy's stellar
- 2:29:30population remains hidden revealed only through gravitational effects and. Statistical
- 2:29:36relationships with other systems discovery histories often. Reveal something about
- 2:29:43scientific progress ton six' one eight was, photographed in nineteen
- 2:29:48fifty seven catalogued, as a mysterious violet object then sat
- 2:29:54in records for thirteen years before. Anyone realized what it
- 2:29:59was after quasars were recognized as a distinct class of,
- 2:30:03objects in nineteen sixty three and after radio observations flagged
- 2:30:08it as unusual in nineteen seventy did. Spectroscopy reveal its
- 2:30:12true nature we observed. It decades before understanding it. This
- 2:30:19pattern repeats, throughout astronomy, we detect, signals catalog objects, take
- 2:30:25images and, only later sometimes much later. Do we grasp
- 2:30:30their significance the delay reflects both. Technological limitations and conceptual
- 2:30:36ones sometimes we lack instruments sensitive. Enough to observe crucial
- 2:30:42details sometimes we lack the theoretical framework. To interpret what we're
- 2:30:48seeing progress requires both, better observations and better theories. Each
- 2:30:54In forming the, other, for ton six one. Eight key
- 2:30:59questions remain unanswered we don't know. Its precise three dimensional
- 2:31:04structure observations, provide projections on the. Sky but not depth
- 2:31:09information we don't know the detailed. Velocity field throughout the
- 2:31:14nebula we don't know. How magnetic fields vary spatially we
- 2:31:20don't know the. Metallicity distribution in different regions we don't
- 2:31:25know whether previous active phases occurred. Before the one we
- 2:31:29observe future observations will. Address SOME of these gaps j
- 2:31:35wst can probe dusty. Regions invisible at optical wavelengths the
- 2:31:41extremely large telescope will resolve structures ten times. Smaller than
- 2:31:46current observations achieve the square kilometer array will map molecular
- 2:31:52gas and. Magnetic fields with unprecedented detail gravitational wave detectors
- 2:31:59might eventually sense mergers, involving similarly massive black holes revealing.
- 2:32:04Formation pathways and growth histories but some. Questions may Remain
- 2:32:10permanently unanswerable we observed ton six hundred eighteen as it
- 2:32:16was ten. Point eight billion years ago the light we
- 2:32:21see has been traveling since the universe was. Only three
- 2:32:25billion years old we have no information. About what's happened
- 2:32:29since then the system has evolved for ten point eight
- 2:32:34billion years. In ways we can't observe the, quasar might
- 2:32:39still be active or it might have shut. Down billions
- 2:32:43of years ago the, nebula might have formed stars. Or
- 2:32:47it might remain. Diffuse we simply don't know this limitation applies.
- 2:32:53To all high redshift observations we see distant objects, as
- 2:32:58they were long ago frozen in time at. Whatever epoch
- 2:33:02their light departed, the universe has continued evolving but that,
- 2:33:07evolution remains hidden from us blocked by. The finite speed
- 2:33:12of light only by observing many similar systems at different
- 2:33:17redshifts can, we reconstruct the evolutionary sequence piecing together cosmic history.
- 2:33:24From snapshots at different epochs ton six hundred eighteen occupies a.
- 2:33:29Crucial position in that sequence it formed during, the peak
- 2:33:34of quaser activity when black hole growth rates and star
- 2:33:38formation rates. Both reached their cosmic maxima understanding this epoch
- 2:33:44reveals how galaxies transitioned from gas rich actively forming systems.
- 2:33:50To gas pore passive ones it shows us when and
- 2:33:54how feedback mechanisms. Became effective at regulating growth it constrains
- 2:34:01models of cosmic evolution that predict the properties. Of galaxies
- 2:34:05we observe today the broader. Implications extend beyond individual objects
- 2:34:11Ultra massive black holes like ton six hundred eighteen provide
- 2:34:16tests of. Fundamental physics in extreme conditions general relativity predicts
- 2:34:22how space time should, curve near such massive objects but
- 2:34:26we've never tested those. Predictions in regimes this extreme the
- 2:34:30event horizon, should behave in specific ways tidal, forces should
- 2:34:35follow predictable patterns time. Dilation should match theoretical calculations confirming
- 2:34:43these predictions. Validates our understanding, of gravity where it matters.
- 2:34:47Most quantum effects remain mysterious hawking radiation suggests black holes emit,
- 2:34:55thermal radiation and eventually evaporate but The time scar scale
- 2:35:00for ton six hundred eighteen exceeds ten to the, power
- 2:35:04of one hundred years so long that the concept. Of
- 2:35:07time itself becomes questionable the information paradox asks what happens
- 2:35:13to information that, falls into a black hole and no
- 2:35:17consensus answer exists. Despite decades of theoretical work ton six
- 2:35:24one eight embodies this paradox as. Dramatically as any object
- 2:35:28can string theory and, quantum gravity approaches proposed solutions. But
- 2:35:35experimental tests. Remain impossible with current technology we Can't probe,
- 2:35:41physics at the plank scale where quantum. Effects should modify
- 2:35:45general relativity we can't observe, the interior of event. Horizons
- 2:35:51where singularities supposedly lurk we are left with mathematics and
- 2:35:56theoretical arguments. Unable to test prediction directly ton six one
- 2:36:02eight reminds us that the universe contains regimes where our
- 2:36:06best theories break down and. New physics must eventually emerge the.
- 2:36:12Scale still doesn't quite register you can, recite the numbers one,
- 2:36:16Thousand three, hundred astronomical units schwarzchild radius, sixty six billion
- 2:36:22solar masses one hundred. Forty trillion times solar luminosity you
- 2:36:28can Follow the comparisons forty times neptune's Orbit More massive
- 2:36:33than the milky way's stars combined light takes, weeks to
- 2:36:37cross its, shadow but actually visualizing it actually grasping what
- 2:36:42those numbers mean in any visceral sense. That remains beyond
- 2:36:48human capability your brain. Compresses THE information into abstractions to
- 2:36:54n six one eight becomes a category ultra massive black.
- 2:36:59Hole rather than. A thing you can imagine the nebula
- 2:37:03becomes a number one hundred billion solar masses. Rather than a.
- 2:37:08Physical structure you can picture the jets become a concept
- 2:37:13relativistic outflows rather. Than actual streams of plasma you can
- 2:37:19visualize the translation from measurement to. Understanding its fundamental cognitive
- 2:37:25limits this limitation isn't. Failure its recognition of scope the
- 2:37:32universe operates at scales both far smaller and. Far, Larger
- 2:37:36than human experience spans quarks and electrons inhabit realms trillions
- 2:37:43of times smaller. Than anything you can see galaxy superclusters
- 2:37:48and cosmic voids extend billions of light years beyond. Anything you,
- 2:37:53can travel to your intuitions shaped by evolution to navigate
- 2:37:58a world of medium size objects moving at moderate speeds
- 2:38:03simply weren't designed. For extremes in either direction what you can.
- 2:38:08Grasp is relationship and context ton six. Hundred eighteen isn't
- 2:38:15just large it's among. The largest black holes, known it
- 2:38:19isn't just distant it's one of the most distant. Quasas
- 2:38:23we've studied in, detail it isn't just massive it's at
- 2:38:28or near the theoretical. Maximum mass achievable through accretion these,
- 2:38:35relationships place it in context showing where it fits in the.
- 2:38:40Cosmic hierarchy of extreme objects. You can also grasp implication
- 2:38:46tons six hundred eighteen's existence tells us something about the
- 2:38:51early universe that conditions allowed such massive black holes to.
- 2:38:56Form within three billion years its property these constrain theoretical
- 2:39:01models of black. Hole growth and galaxy evolution its feedback
- 2:39:06effects demonstrate how black holes influence their environments on scales.
- 2:39:11Far exceeding their Physical size these implications connect ton six
- 2:39:18hundred eighteen to broader questions. About cosmic structure and evolution
- 2:39:23the human tendency to seek. Meaning in observations Runs deep
- 2:39:28you look at ton six one eight and want, to
- 2:39:31know what it means what significance it holds beyond. Just
- 2:39:35being large and distant the scientific answer focuses on what we,
- 2:39:40learn constraints on accretion, physics tests of general, relativity insights into,
- 2:39:48galaxy formation but, there's another meaning less. Precise but perhaps
- 2:39:55more profound ton six one eight represents. The universe's capacity
- 2:40:00for extremes physics. Allows black holes to exist the laws
- 2:40:06of nature permit matter to collapse into regions so dense
- 2:40:10that space. Time itself warps beyond recognition the same forces that,
- 2:40:16shape ordinary stars and, planets scaled up and concentrated produce
- 2:40:22objects that. Challenge our ability to understand the universe isn't
- 2:40:27obligated to operate at scales. We find comfortable or comprehensible
- 2:40:33it simply, operates according to its laws. Producing whatever those
- 2:40:37laws allow this indifference to. Human comprehension is itself significant
- 2:40:44the universe doesn't. Care whether we understand it ton six
- 2:40:49one eight, existed long before humans evolved will continue existing long,
- 2:40:55after our species is gone and would remain exactly as
- 2:40:59it is even if no. Conscious observers ever studied it
- 2:41:05our attempts to measure and, understand it reflect our curiosity
- 2:41:10not any. Intrinsic meaning the object. Possesses yet that Curiosity
- 2:41:15matters humans are the, universe's way of studying itself matter
- 2:41:21arranged in such a way that it can contemplate. Its
- 2:41:24own existence and Origins when you think, about ton six
- 2:41:28hundred eighteen when you grapple with its scale and, try
- 2:41:32to understand its properties. You're participating in something remarkable atoms
- 2:41:39forged in ancient stars now, arranged into a human brain
- 2:41:45considering the nature of an ultra massive black hole, billions
- 2:41:49of light years away the universe examining itself. Through the
- 2:41:54medium of. Consciousness that's the real story. Ton six one
- 2:41:58eight tells not just facts about, mass and size and,
- 2:42:03Luminosity though those are important not just implications, for cosmology
- 2:42:09and galaxy. Evolution though those matter too the deeper story
- 2:42:14is about the relationship between the universe and the minds.
- 2:42:18That try to understand it how we push, against the
- 2:42:22limits of comprehension developing mathematics and observations and theories to
- 2:42:28grasp phenomena. That exceed our intuitive capabilities the effort itself
- 2:42:34is valuable regardless of. How complete our understanding becomes we'll
- 2:42:40never Stand on a planet, orbiting ton six one eight never,
- 2:42:45directly observe its event horizon never witness its eventual fate.
- 2:42:50Billions of years from now but, we can measure, its
- 2:42:54properties model its evolution connect it to theoretical frameworks that
- 2:42:59explod how. Such objects form and grow we, can place it,
- 2:43:04in context understand its significance and use it to test.
- 2:43:09Our theories about the, cosmos that's what, science offers not
- 2:43:13complete understanding but. Progressive refinement of incomplete, understanding each observation adds,
- 2:43:21Detail each measurement constrains theories each new. Instrument reveals previously
- 2:43:28hidden aspects the, process continues building knowledge incrementally occasionally making
- 2:43:36dramatic leaps when new. Technologies OR insights become available t
- 2:43:41n six one eight will continue revealing. SECRETS as our
- 2:43:45capabilities improve jwst observations might. Resolve the host galaxy's structure
- 2:43:54gravitational wave detectors might. Sense mergers involving similar objects advanced
- 2:44:00simulations might explain how it. Grew so massive so quickly
- 2:44:05future generations of astronomers will study it with, instruments we
- 2:44:09haven't yet imagined asking. Questions we, haven't yet formulated for
- 2:44:14now you know what can. Be known from current observations
- 2:44:19you understand the scale even if. You can't truly visualize
- 2:44:22it you grasp the implications even if. The full picture
- 2:44:27remains incomplete you've confronted one of the most extreme objects
- 2:44:32in the universe and emerged. With, some measure of understanding
- 2:44:37however limited human comprehension must be when faced with phenomena.
- 2:44:43This far beyond everyday experience the universe, contains to n
- 2:44:48six one, eight, and countless other wonders objects and phenomena
- 2:44:54that push the. Boundaries of what physics allows some we've.
- 2:44:58Discovered many more awight detection each one challenges, us to
- 2:45:04expand our understanding to develop new, ways, of, thinking about.
- 2:45:08Matter energy space and time each one reminds us that
- 2:45:14reality is richer and. Stranger than we Might imagine that's
- 2:45:19how big ton, six hundred eighteen really is not just in,
- 2:45:23astronomical units or solar masses but in the space it
- 2:45:27occupies in our, attempts to understand the cosmos a landmark
- 2:45:31at the edge of comprehension pointing toward. Mysteries that still
- 2:45:35await resolution