Latest / Boring Science / Planet Nine May Be Real But It Doesn_t Make Sense
Transcript
- 0:00Speaker 1: Something is wrong at the edge of our Solar system.
- 0:03Not wrong in a subtle way, not wrong in a
- 0:06way that takes years of squinting at data to notice,
- 0:11wrong in a way that has forced some of the
- 0:13most careful planetary scientists alive to sit down, run the
- 0:17numbers twice, and then admit that something out there is
- 0:21pulling on things it should not be able to reach.
- 0:25Objects so far from the Sun that sunlight reaching them
- 0:29is barely a whisper, objects taking thousands of years just
- 0:34to complete a single orbit. Those objects are not behaving
- 0:40the way they should. Their paths through space are clustered, aligned,
- 0:46pointing in the same direction as if something enormous is
- 0:50standing just out of sight and tugging. No known planet
- 0:54can do this. Neptune, the farthest confirmed world in our
- 0:59Solar System, is not anywhere close to far enough out.
- 1:04Whatever is causing this is deeper in the dark than
- 1:07anything we have ever named. If you find comfort in
- 1:12these gentle explorations of space and science, I'd be grateful
- 1:16if you'd consider subscribing and giving this video alike. Here
- 1:26is the scale of what we are talking about. Earth
- 1:30orbits the Sun at roughly ninety three million miles out.
- 1:35Astronomers use that distance as a unit of measurement. One
- 1:40astronomical unit Neptune sits about thirty of those units out
- 1:45already unimaginably remote. The objects at the center of this
- 1:50mystery orbit at distances of two hundred fifty five hundred,
- 1:55even beyond one thousand astronomical units from the Sun. These
- 2:00are not planets. They are small icy bodies left over
- 2:05from the formation of the Solar System, drifting through a
- 2:09region so distant and so cold that the Sun looks
- 2:13like nothing more than a bright star from their surface.
- 2:17They should be scattered randomly, nothing should be organizing them,
- 2:22and yet when researchers mapped their orbits, they were not
- 2:27random at all. The idea that something is out there
- 2:31goes back further than most people realize. But the modern
- 2:35version of this story begins in earnest around two thy fourteen,
- 2:41when two astronomers noticed that a handful of these distant
- 2:45icy objects shared an orbital property that had no business
- 2:50being shared. The odds of this happening by chance were tiny,
- 2:56not impossible, but small enough to demand an explanation. That
- 3:01observation started a chain of events that ended with a
- 3:05formal scientific paper published in twenty sixteen proposing that a
- 3:11planet roughly five to ten times the mass of Earth
- 3:15is orbiting our Sun right now at a distance hundreds
- 3:19of times greater than Earth's. The paper named it Planet nine,
- 3:24and it came from two of the most credentialed planetary
- 3:28astronomers working today. This is not a fringe claim from
- 3:31someone posting to a forum at midnight. Mike Brown is
- 3:36the astronomer at Caltech who discovered so many large objects
- 3:40in the Outer Solar System that the scientific community was
- 3:44eventually forced to demote Pluto from planetary status. He is,
- 3:49in a real sense, the person most responsible for the
- 3:52Solar System having eight official planets instead of nine. His collaborator,
- 3:59constantine In Battigin, is a theoretical physicist and planetary scientist
- 4:05whose entire job is building mathematical models of how planets
- 4:10form and evolve. When these two say that the evidence
- 4:15points toward an undiscovered planet, the community listens. Not everyone agrees,
- 4:23but no one dismisses it. What makes this genuinely unsettling
- 4:28is that the evidence has not gone away. Every year
- 4:32since twenty sixteen, new objects have been found in the
- 4:36outer Solar System, and many of them fit the predicted pattern.
- 4:42The gravitational fingerprints keep showing up, the clustering keeps holding.
- 4:48Attempts to explain it away with observational bias have not
- 4:53fully worked. The mystery has only gotten more detailed, more specific,
- 4:59and harder to handwave out of existence. Brown himself has
- 5:04said he is extraordinarily confident the planet is real. Other
- 5:09researchers are more cautious, some are skeptical, but the question
- 5:14is alive in a way that legitimate scientific questions are alive,
- 5:19argued over at conferences, tested against new data, refined with
- 5:25every new discovery from the distant Solar System. There is
- 5:29also a candidate. In twenty twenty five, researchers digging through
- 5:35archival infrared survey images taken twenty three years apart, found
- 5:40an object that appears to have moved exactly the amount
- 5:44of planet at Planet nine's predicted distance would move. It
- 5:47has not been confirmed, it has not been given a name,
- 5:52but it exists as the best physical lead the search
- 5:56has ever produced. So here is where things stand. Either
- 6:01a significant subset of the most capable planetary scientists alive
- 6:06have been fooled by a statistical ghost for over a decade,
- 6:10or there is a world out there in the dark
- 6:13that nobody has directly seen yet, orbiting our Sun on
- 6:17a path so vast it takes between ten and twenty
- 6:21thousand years to complete a single loop. The question is
- 6:27not whether someone invented this story to fill a slow
- 6:30news cycle. The question is whether a world larger than
- 6:34Earth is sitting out there right now, invisible and we
- 6:39simply haven't looked in the right place yet. Before getting
- 6:43into what the evidence shows, it helps to understand what
- 6:47exactly researchers are talking about when they say planet nine.
- 6:52Planet nine is not a confirmed planet. It has not
- 6:55been photographed. No telescope has resolved it as a disc,
- 7:00tracked its motion across the sky, or measured its light.
- 7:05What it is at this point is a hypothesis, a
- 7:10predicted object whose existence would explain a set of observations
- 7:15that currently have no better explanation. That distinction matters. When
- 7:21astronomers talk about planet nine, they are describing something they
- 7:27believe is probably out there based on gravitational evidence, not
- 7:31something they have actually seen. So what do the predictions say?
- 7:36The leading models suggest Planet nine is somewhere between five
- 7:40and ten times the mass of Earth that puts it
- 7:44in a category planetary scientists call a super Earth, or,
- 7:48depending on its composition, a mini Neptune. These are not
- 7:53exotic categories. They are actually the most common type of
- 7:57planet found around other stars in the galaxy. Survey after
- 8:02survey of distant star systems has turned up planets in
- 8:06this size range more often than any other. What makes
- 8:11Planet nine strange is not what it is. It is
- 8:14where it is. Our Solar System, for a long time,
- 8:19appeared to have none of these mid sized worlds. Every
- 8:23planet here is either small and rocky like Earth or
- 8:26enormous like Jupiter. There is nothing in between, at least
- 8:31not anywhere close. Planet nine, if it exists, would fill
- 8:37that gap, it would just be doing it from an
- 8:40almost unimaginable distance. To understand how far out we are talking,
- 8:45you need a unit of measurement that makes the Solar
- 8:48System navigable. Astronomers use the astronomical unit abbreviated AU, which
- 8:56is simply the average distance from Earth to the Sun.
- 9:00That number is about ninety three million miles or one
- 9:05hundred fifty million kilometers. Neptune, the outermost confirmed planet orbits
- 9:11at roughly thirty astronomical units. In human terms, light takes
- 9:17about four hours to travel from the Sun to Neptune.
- 9:21A spacecraft moving at the speed of the New Horizon's
- 9:24probe that is currently the fastest human made object heading
- 9:29away from our Solar System, would take roughly twelve years
- 9:34just to reach Neptune. From Earth. Planet nine is predicted
- 9:38to orbits somewhere between two hundred ninety and five hundred
- 9:42astronomical units from the Sun. The estimates have shifted over
- 9:47time as new data and better models have come in,
- 9:51but even at the lower end of that range, you
- 9:53are looking at a distance nearly ten times farther than Neptune.
- 9:58Light that left the Sun this morning would take almost
- 10:02two days to reach Planet nine. At four hundred astronomical units.
- 10:08That same New Horizon spacecraft traveling at full speed would
- 10:13need over seventy years to get there. The planet sits
- 10:18in a region of the Solar System so remote that
- 10:22sunlight arriving at its surface is roughly one millionth the
- 10:26intensity of sunlight on Earth. It would be essentially dark
- 10:31out there. The orbit itself is not circular. Planet nine
- 10:36is predicted to follow a highly elongated path swinging from
- 10:41a closest approach of perhaps two hundred astronomical units out
- 10:45to a farthest point somewhere beyond six hundred astronomical units,
- 10:50before looping back in One complete orbit around the Sun
- 10:55at that distance would take somewhere between ten thousand and
- 10:59twenty thousand years. For context, ten thousand years ago, the
- 11:06last ice age was ending, humans were just beginning to
- 11:10settle into agricultural societies. Every civilization that has ever existed
- 11:16on this planet has risen and fallen within the span
- 11:20of less than one planet nine year. The orbital period
- 11:24is so long that in the entire history of recorded observation,
- 11:30the planet would have moved only a tiny fraction of
- 11:32the way around its track. This extreme orbit is part
- 11:36of why nobody has found it yet. A planet that
- 11:40spends most of its time at distances of four hundred
- 11:43or five hundred astronomical units from the Sun reflects almost
- 11:48no sunlight back toward Earth. It would appear as an
- 11:52extraordinarily faint point of light moving so slowly against the
- 11:58background stars that distinguishing its motion from noise requires comparing
- 12:04observations taken months or years apart. It is genuinely difficult
- 12:10to find. What researchers do have is a predicted mass range,
- 12:15a predicted orbital region, a predicted inclination, and a predicted distance.
- 12:23Recent models from twenty twenty five have actually tightened the
- 12:27estimate somewhat, pulling the likely orbit a bit closer than
- 12:32earlier calculations suggested somewhere around two hundred ninety to four
- 12:38hundred sixty astronomical units rather than the original four hundred
- 12:43to eight hundred. The mass estimate has also come down slightly.
- 12:49Earlier papers favored something closer to ten earth masses. More
- 12:54recent work suggests five or six earth masses is more likely.
- 13:00Some modeling points toward a composition that is rockier than
- 13:04the ice giant picture that dominated early descriptions of the object.
- 13:09None of these refinements change the fundamental picture. This is
- 13:14still a large world orbiting in the deep dark at
- 13:18a distance that dwarfs anything we have ever directly explored.
- 13:23What makes the hypothesis scientifically serious rather than speculative is
- 13:29precisely what it is not based on. It is not
- 13:33based on a single researcher's calculation or a mathematical anomaly
- 13:38in one data set. It is based on the orbital
- 13:41behavior of multiple independent objects in the Outer Solar System,
- 13:46objects whose paths cannot be explained by the gravity of
- 13:50any known planet. The gravitational fingerprint of something massive and
- 13:55distant is showing up across a range of observations by
- 14:00different teams using different instruments over more than a decade.
- 14:06Whether that fingerprint belongs to a real planet or has
- 14:09some other explanation is still an open question, but the
- 14:14fingerprint itself is not in dispute. Every single thing astronomers
- 14:20currently believe about Planet Nine, its mass, its orbit, its distance,
- 14:27even whether it exists at all, has been inferred from
- 14:30the behavior of other objects, none of which have ever
- 14:34been close enough to feel its gravity directly. The search
- 14:38for an undiscovered planet beyond Neptune is not a new idea.
- 14:43It is, in fact one of the oldest recurring obsessions
- 14:47in modern astronomy. Since Neptune was confirmed in eighteen forty six,
- 14:53at least thirty separate researchers have proposed that something larger,
- 14:58something unseen, was hiding even farther out. Every single one
- 15:04of them was eventually proven wrong. That streak matters. It
- 15:10is long enough and consistent enough that The first honest
- 15:14question anyone should ask about planet nine is a simple one.
- 15:19Why would this time be any different? To understand why
- 15:23the history is so embarrassing, you have to go back
- 15:27to how Neptune itself was found. That story is one
- 15:31of astronomy's genuine triumphs. Two mathematicians, Urbane Leverier in France
- 15:38and John couch Adams in England independently noticed that Uranus
- 15:43was not moving the way it should. Its orbit had
- 15:46small but measurable wobbles that Newton's laws could not explain
- 15:52if the known planets were all there was. Both men
- 15:56did the math. Both concluded something massive was pulling on
- 16:01Uranus from beyond. Leverier sent his predicted coordinates to an
- 16:07observatory in Berlin. They pointed their telescope and found Neptune
- 16:13within an hour. It was one of the most dramatic
- 16:16conformations in the history of science. That success planted an
- 16:22idea that would haunt astronomy for the next century. If
- 16:27you could predict Neptune from Uranus's wobbles, maybe you could
- 16:31predict something beyond Neptune the same way. And almost immediately
- 16:37people started trying. By the late eighteen hundreds, several astronomers
- 16:43had noticed that Neptune itself seemed to have small irregularities
- 16:48in its orbit. The conclusion felt obvious. There had to
- 16:54be another planet out there, something big, something tugging at Neptune,
- 16:59the way away, Neptune tugged at Uranus. The hunt was on.
- 17:05Nobody pursued it harder than Percival Lowell. He was wealthy,
- 17:10he was determined, and he was almost pathologically convinced that
- 17:14a trans Neptunian planet existed. He called it planet X,
- 17:20not because he didn't know what it was, but because
- 17:23X meant unknown. Starting around nineteen oh six, Lowell funded
- 17:28an observatory in Arizona specifically to find it. He ran calculations,
- 17:34he produced predicted positions, He searched the sky for years.
- 17:39He found nothing. Lowell died in nineteen sixteen without his planet.
- 17:46His observatory kept searching after his death, driven partly by
- 17:50institutional momentum and partly by genuine scientific interest. Then in
- 17:57nineteen thirty, a young assistant at lowell observatory named Clyde
- 18:02Tombaugh found something. He was blinking photographic plates comparing images
- 18:08of the same piece of sky taken on different nights
- 18:12looking for anything that moved. Something moved. It was faint, slow,
- 18:18and sat almost exactly where Lowell's calculations had suggested Planet
- 18:23X might be. The news spread around the world. Lowell's
- 18:28prediction seemed vindicated. The object was named Pluto, after the
- 18:33Roman god of the underworld, and for a few months
- 18:37it looked like the long hunt was finally over. It wasn't.
- 18:42Almost immediately, problems appeared. Pluto was too faint. Astronomers tried
- 18:50to calculate its mass from the way it was supposed
- 18:53to be influencing Neptune, and the numbers didn't add up.
- 18:57The more carefully they measured, the smaller Pluto seemed to get.
- 19:02It couldn't be responsible for the orbital wobbles that had
- 19:05motivated the search in the first place. By mid century,
- 19:10it was clear that Pluto was not Planet X. It
- 19:14was something much smaller, much stranger, and essentially coincidental. The
- 19:21apparent confirmation of Lowell's prediction turned out to be luck.
- 19:27The planet he was actually looking for was never found
- 19:30because it didn't exist. But that realization took a long
- 19:34time to sink in. Through the nineteen forties, fifties, and sixties,
- 19:41astronomers kept proposing additional planets. The orbital anomalies in Neptune
- 19:47and Uranus kept appearing in different data sets under different analyzes,
- 19:53interpreted in different ways by different researchers. Each new claim
- 19:58attracted attention, each eventually collapsed. The wobbles turned out to
- 20:04be measurement errors. When Voyager II flew past Neptune in
- 20:09nineteen eighty nine and gave astronomers precise mass measurements for
- 20:14the first time, scientists went back and recalculated Uranus's orbit
- 20:20using the corrected Neptunian mass. The wobbles disappeared entirely. There
- 20:26were no anomalies. There had never been anomalies. The whole
- 20:31foundation of a century of planet X searching evaporated in
- 20:35a single recalculation. What makes that particularly striking is the
- 20:40sheer number of very capable scientists who had built careers
- 20:45around something that wasn't there. This was not fringe science.
- 20:51Some of the people proposing trans Neptunian planets were serious
- 20:55researchers at serious institutions, working with the best data available
- 21:01to them. The data was just wrong or incomplete, or
- 21:06being interpreted through assumptions that weren't valid. The pattern repeated
- 21:11itself so many times that by the nineteen nineties, healthy
- 21:16skepticism toward any new planet X claim was essentially the
- 21:21default position in the field, and that skepticism was earned.
- 21:27So when Battagin and Brown published their paper in twenty
- 21:31sixteen arguing for planet nine, they were walking into this history.
- 21:37Brown in particular knew exactly what it looked like. He
- 21:42had spent years studying the Outer Solar System and years
- 21:46watching speculative planet claims fall apart. He was not someone
- 21:52prone to wishful thinking about undiscovered worlds. When he and
- 21:57Battigin started working on the clustering problem, Brown's initial job
- 22:02was to find the conventional explanation, to identify the prosaic
- 22:07reason the data looked the way it did, and close
- 22:10the case without invoking anything new. The difference this time,
- 22:15and the reason serious researchers did not immediately file the
- 22:19claim alongside Lowell's notebooks and the corrected Neptune calculations, was
- 22:25the nature of the evidence itself. Every previous planet xclaim
- 22:30started with a theorist noticing a discrepancy and proposing a
- 22:35planet to explain it. The discrepancy always evaporated. When the
- 22:40data improved, the planet nine claims started differently. It started
- 22:47with actual objects in actual orbits, objects that had been
- 22:51measured carefully and repeatedly behaving in ways that nobody could explain.
- 22:58No measurement ex error makes a dozen objects point in
- 23:02the same direction. No instrument calibration issue creates a clustering
- 23:08signal across independent surveys. The track record is brutal, and
- 23:13any honest account of the planet nine hypothesis has to
- 23:17start by acknowledging it, because the only thing that makes
- 23:21this time feel different is that, for the first time,
- 23:24the evidence is not coming from one person's wishful calculations,
- 23:29but from objects in the actual sky that are doing
- 23:33something nobody can explain. To understand why anyone thinks there
- 23:38is a ninth planet, you have to start with the
- 23:42Kuiper belt. Most people learn the Solar System as eight
- 23:45planets and then empty space stretching out to infinity. That
- 23:50picture is wrong. Beyond Neptune, starting at roughly thirty astronomical
- 23:56units from the Sun, there is an enormous ring of material, icy, rocky, cold,
- 24:03and sprawling. It extends outward to somewhere around fifty astronomical
- 24:09units before thinning out. One astronomical unit is the distance
- 24:13from Earth to the Sun, about ninety three million miles,
- 24:18So the Kuiper Belt begins nearly three billion miles out
- 24:22and stretches billions of miles beyond that. Pluto lives there,
- 24:28so do hundreds of thousands of smaller bodies, maybe more.
- 24:33Short period comets, the ones that swing through the inner
- 24:37Solar System on cycles of less than two hundred years,
- 24:41almost certainly originate there, knocked inward by gravitational nudges over
- 24:47millions of yea. The Kuiper Belt is not chaos. It
- 24:52has structure. The objects inside it follow predictable rules, and
- 24:57the dominant force shaping those rules is Neptune. Neptune's gravity
- 25:03acts like a traffic warden for the outer Solar System,
- 25:07shepherding Kuiper Belt objects into stable orbital configurations, pushing some inward,
- 25:14flinging others outward, setting the boundaries of the belt itself.
- 25:19Most Kuiper Belt objects orbit on paths that are relatively
- 25:23flat compared to the plane of the Solar System, relatively circular,
- 25:28and never too far from Neptune's influence. When something does
- 25:33get knocked onto a wild, elongated orbit, Neptune's gravity eventually
- 25:38pulls it back into a more settled configuration. The system
- 25:43is messy in the details, but organized in the broad picture.
- 25:48Neptune runs the neighborhood. Then there are the objects that
- 25:53do not fit that picture at all. Scattered deep enough
- 25:57beyond the main belt, you find a popular of bodies
- 26:01on orbits so stretched and so distant that Neptune can
- 26:05barely reach them. These are the extreme trans Neptunian objects,
- 26:11sometimes called e TNOs. Their paths are not circular. They
- 26:17are long ellipses, dramatically elongated, that carry them out to
- 26:22hundreds of astronomical units from the Sun before swinging them
- 26:27back inward. Some reach five hundred astronomical units at their
- 26:32farthest point. A few go farther still. At those distances,
- 26:38the Sun's light takes days to arrive, the temperature drops
- 26:43close to absolute zero. These objects spend most of their
- 26:48orbital lives in a region so remote it barely registers
- 26:53on any map of the Solar System most people have
- 26:56ever seen. What makes Etno's particularly interesting is not just
- 27:01how far they go, It is what governs them when
- 27:05they get there. At two hundred, three hundred, five hundred
- 27:10astronomical units from the Sun, Neptune's gravitational reach is essentially zero.
- 27:17These objects have sailed far beyond the point where Neptune
- 27:21can do anything meaningful to their orbits. At those distances,
- 27:27the only force that should matter is the gravity of
- 27:30the Sun itself, pulling everything inward on long looping paths.
- 27:37The inner planets, the outer planets, even Jupiter, none of
- 27:42them have meaningful influence at these scales. The Sun dominates,
- 27:48and the Sun is symmetric, It pulls equally in every direction.
- 27:54Here is why that matters. If the Sun's gravity is
- 27:57the only thing shaping the orbits of excis extream trans
- 28:01Neptunian objects, and if the Sun pulls equally in every direction,
- 28:06then the orbits of those extreme objects should point in
- 28:10random directions. There is no reason for them to prefer
- 28:14one orientation over another. Some should be tilted this way,
- 28:19some that way. Their long axes should be scattered across
- 28:24the sky like compass needles with no north. That is
- 28:28what the math says. That is what every model of
- 28:32the outer Solar System predicted before anyone looked carefully. What
- 28:38actually showed up in the data was something else entirely.
- 28:43When researchers began cataloging enough extreme trans Neptunian objects to
- 28:48look for patterns, they found that the orbits were not
- 28:51scattered randomly. They were bunched. Multiple objects independently following their
- 28:59own long loan paths around the Sun seemed to be
- 29:02oriented in roughly the same direction. The long axes of
- 29:07their ellipses pointed in a similar region of sky. Their
- 29:12orbital planes tilted in similar ways. The alignment was not perfect,
- 29:18but it is far too consistent to look accidental, and
- 29:22the more objects research is found, the more the pattern held.
- 29:26Random processes do not produce this. If you flip a
- 29:30coin fifty times and it comes up heads forty times,
- 29:35you stop assuming the coin is fair. The Solar system
- 29:39was flipping the same way over and over. Something was
- 29:43biasing the outcome, organizing these objects, pulling their orbital orientations
- 29:49into rough agreement, and whatever it was, it was not Neptune.
- 29:55Neptune was too close, too weak at these distances. Who
- 30:00irrelevant to the extreme objects to be the cause. There
- 30:04was no obvious candidate in the known Solar system. Jupiter
- 30:09was too far in the known planets collectively could not
- 30:13account for it. The Sun, symmetric and indifferent, certainly was
- 30:19not doing it. This is the kind of signal that
- 30:22keeps researchers awake. Not a spectacular explosion, not a dramatic collision,
- 30:30just numbers that do not behave the way numbers are
- 30:33supposed to behave a quiet, stubborn pattern in the orbital
- 30:38data of objects most people have never heard of. It
- 30:43did not look like noise. It did not look like bias.
- 30:47It looked like something was out there, somewhere beyond the
- 30:51edge of the known Solar system, doing exactly what a massive,
- 30:56unseen planet would do. The orbits of the most distant
- 31:00objects in the Kuiper Belt were not scattered randomly across
- 31:04the sky the way they should be. They were clustering,
- 31:08pointing in the same general direction, as if something massive
- 31:13was standing just out of frame and pulling on all
- 31:16of them at once. In twenty fourteen, Chad Trujillo and
- 31:21Scott Shephard published a paper that most people outside astronomy
- 31:26never heard about. It did not make the front page,
- 31:30it did not trend online. A few dozen planetary scientists
- 31:34read it carefully, nodded, and filed it away, but buried
- 31:40inside that paper was a number that did not make sense,
- 31:44and numbers that don't make sense have a way of
- 31:47coming back. Trujillo had spent years doing exactly the kind
- 31:51of work that does not get you famous systematic surveys
- 31:56of the Outer Solar System, pointing telescope at faint, cold
- 32:01stretches of sky, running image stacking software for hours, looking
- 32:07for objects that barely moved. He had trained under Mike
- 32:11Brown at Caltech, one of the most productive planetary astronomers
- 32:16of his generation. Brown's group had found more distant Solar
- 32:20System objects than almost anyone alive. Truhio absorbed that approach,
- 32:26then took it further on his own. By twenty fourteen,
- 32:31he was running a dedicated survey program with Scott Shepherd
- 32:35at the Carnegie Institution, hunting for whatever was hiding in
- 32:39the deep outer Solar System. They were not looking for
- 32:43anything in particular, They were looking for everything. Then they
- 32:48found something they were not looking for at all. While
- 32:52compiling a new distant object called twenty twelve VP one
- 32:56point one three, Trujillo and Shepherd did what came careful
- 33:00astronomers always do with a new discovery. They compared it
- 33:04against everything else known in that orbital region, and they
- 33:09noticed something strange. Not just about twenty twelve VP one
- 33:14one three, about thirteen of the most extreme objects in
- 33:18the entire catalog. All of them shared a suspicious similarity
- 33:23in an obscure orbital parameter, the same number clustering around
- 33:28the same value across thirteen separate objects that were supposed
- 33:33to have nothing in common. The odds of that being
- 33:37random chance were extremely small. The parameter in question is
- 33:42called the argument of perihelion. That phrase sounds complicated, but
- 33:47the underlying idea is not. Every object orbiting the Sun
- 33:53has a closest point in its orbit called perihelion. The
- 33:58argument of perihelian describes the orientation of that closest point
- 34:03relative to the plane of the Solar System. Think of
- 34:07it this way. Imagine the Solar system as a flat
- 34:11clock face. Every orbit has a point where it swings
- 34:16closest to the center. The argument of perihelium tells you
- 34:21where on that clock face the closest approach happens. For
- 34:26a random collection of objects scattered by ancient gravitational encounters,
- 34:31those closest approach points should be aimed in all different
- 34:35directions twelve o'clock, six o'clock, three o'clock, everywhere, no particular
- 34:43direction should dominate. What Truehilo and Shepherd found was that
- 34:48the most extreme objects were not pointing in all different directions.
- 34:53They were clustered. The argument of perihelian values for those
- 34:58thirteen objects were all hovering near zero degrees, not scattered concentrated.
- 35:06Something was keeping those orbital orientations corralled into the same
- 35:11general region of space, and nothing in the standard model
- 35:15of the Solar System could explain it. Here is what
- 35:19makes that finding important. These were not ordinary Kuiper Belt
- 35:24objects sitting just beyond Neptune. These were the most extreme ones,
- 35:30objects with orbits so elongated and so distant that Neptune's
- 35:35gravity barely reaches them. At those distances, Neptune cannot hurt
- 35:41anything it does not have the gravitational muscle. Whatever was
- 35:46organizing those orbits had to be something else, something farther out,
- 35:53something not yet identified, or the clustering was a fluke
- 36:00statistical ghost in a small sample. Truhilo and Shepherd were
- 36:04careful they did not claim a planet existed that would
- 36:09have been a significant overreach from thirteen data points and
- 36:13one suspicious orbital parameter. What they wrote instead was more measured.
- 36:19They flagged the anomaly, calculated the probability that it was random,
- 36:25concluded the probability was low enough to warrant attention, and
- 36:30suggested that a distant, undiscovered body could plausibly explain what
- 36:35they were seeing. Then they published it and let the
- 36:39community decide what to do with it. This is how
- 36:43real scientific discoveries often begin, not with a dramatic announcement,
- 36:50with a footnote with a number that sits slightly off
- 36:54from where it should be, and a careful observer who
- 36:58decides to write it down wrote other than ignore it.
- 37:01The paper moved through the community at the speed of
- 37:04academic correspondents. Some researchers found it interesting but not compelling.
- 37:11Thirteen objects is a small sample. Small samples can fool you.
- 37:17Others thought the observational bias argument was strong enough to
- 37:22table the whole discussion. Since surveys tend to discover objects
- 37:27in places they've looked most and looked at places are
- 37:31not randomly distributed across the sky, the clustering might be real.
- 37:36It might be an artifact without more objects. It was
- 37:41genuinely hard to say, but some people read it differently.
- 37:46Some people looked at that concentration of arguments of perihelion
- 37:50near zero degrees and thought about what kind of object
- 37:54at what kind of distance, could produce exactly that pattern,
- 37:59not as vague possibility as a specific calculable gravitational problem.
- 38:06What mass would be required, what orbit would be required,
- 38:11whether the numbers could actually work. Those questions take a
- 38:15certain kind of mind to pursue. Someone comfortable with orbital
- 38:21mechanics at scales that make most calculations meaningless. Someone willing
- 38:26to spend months building simulations that might produce nothing, Someone
- 38:31with enough credibility to publish a result that would be
- 38:34scrutinized intensely, and enough stubbornness to defend it anyway. The
- 38:40paper landed on the desk of Mike Brown at Caltech,
- 38:44the same astronomer who had killed Pluto's planetary status nine
- 38:48years earlier, and this time he brought in a theorist
- 38:52named Constantine Battigin to figure out what was actually going on.
- 38:57For several months in twenty fifteen, Batagen and Brown worked
- 39:02in something close to secrecy, not because they were trying
- 39:06to scoop anyone because they were embarrassed by what they
- 39:10were finding. Mike Brown is not someone who believes easily
- 39:15in undiscovered planets. His career had gone almost exactly the
- 39:20opposite direction. He spent years in the early two thousands
- 39:25systematically hunting down objects in the Outer Solar System and
- 39:29proving that the things people had mistaken for giant, unseen
- 39:33worlds were actually just small, icy bodies that nobody had cataloged.
- 39:39Yet he was, by his own description, the person who
- 39:43killed Pluto. He had made a professional habit of deflating
- 39:48planet rumors. When the Trushillo and Shepherd paper crossed his
- 39:53desk in twoenty fourteen, pointing at that strange clustering in
- 39:58the argument of Perry Heally, his first instinct was not excitement.
- 40:04It was skepticism. His first instinct was to find out
- 40:08what everyone else was getting wrong. Constantine Bertigin came at
- 40:13the problem from a different angle. He is a theorist,
- 40:17the kind of researcher who builds mathematical models of how
- 40:21gravitational systems evolve over millions of years. Brown brought him
- 40:26in specifically to stress test the clustering signal to run
- 40:31the numbers and find the conventional explanation that would make
- 40:35the anomaly disappear. That was the plan. That was the assignment.
- 40:43Find the boring answer. They started with the six extreme
- 40:47trans Neptunian objects that had the best characterized orbits. These
- 40:53were not random selections. They were the objects with enough
- 40:57observational data that their orbit parameters could be trusted. The
- 41:03clustering those six objects showed was not subtle. Their orbits
- 41:08were not just pointing in roughly the same direction. They
- 41:12were aligned in three dimensions, tilted the same way, oriented
- 41:17the same way, behaving almost like they had been arranged deliberately.
- 41:23The probability of that happening by chance was somewhere around
- 41:27zero point zero zero seven percent, roughly one in fifteen thousand.
- 41:34Battiggins started working through explanations. Maybe the clustering was an
- 41:39artifact of the way the Kuiper Belt forms, some kind
- 41:43of structural feature baked into the disk of debris left
- 41:47over from the early Solar System. The models said no,
- 41:52Maybe it was the gravitational influence of a passing star
- 41:56early in the Solar System's history, something that had left
- 42:00a long fingerprint on the distant debris possible in principle,
- 42:05but the geometry was wrong and the time scales didn't
- 42:08hold together. Maybe there was some interaction between these extreme
- 42:13objects themselves, a kind of collective gravitational effect that kept
- 42:18their orbits synchronized. He ran that model. It failed. The
- 42:24objects are too spread out and too light to gravitationally
- 42:28influence each other in any meaningful way. One by one,
- 42:33the conventional explanations broke down. What happened next is the
- 42:38part Brown has described publicly and with some obvious discomfort.
- 42:44After exhausting the standard options, Battagen ran a simulation with
- 42:49a hypothetical planet sitting on the opposite side of the
- 42:53Solar System from the clustered objects, an anti aligned orbit,
- 42:58a planet whose il jongated path pointed roughly away from
- 43:02the six extreme TNOs rather than toward them. This is counterintuitive.
- 43:09You might expect a planet to pull things toward it,
- 43:13not away, but orbital mechanics over millions of years don't
- 43:17work the way intuition suggests. Through a process involving mean
- 43:22motion resonances, where objects settle into stable gravitational relationships with
- 43:27each other based on their orbital periods. A planet in
- 43:31this anti aligned configuration would actually trap the extreme objects
- 43:37and keep their orbits locked in alignment on the opposite
- 43:40side of the sky. When Battergen plugged a planet into
- 43:45that configuration, the simulation reproduced the clustering almost perfectly. Brown
- 43:52looked at the results. He had spent years telling other
- 43:56astronomers they were wrong about outer planets. He had a
- 44:00reputation built on skepticism, and here was his own simulation
- 44:06telling him the same thing. Everyone he had dismissed had
- 44:09been saying that something was out there. He has said
- 44:14since that he found the result genuinely hard to accept.
- 44:18That he checked the math, checked it again, and kept
- 44:21looking for the floor. There was no flaw. What made
- 44:26Brown eventually willing to say it out loud was not
- 44:29just the simulation. It was Battign's point about the nature
- 44:34of the prediction. Previous planet X claims over the decades
- 44:39had a common flow. They started with a wobble in
- 44:43someone's data, proposed a planet to explain it, and stopped there.
- 44:49The planet was whatever size and distance you needed it
- 44:53to be to make the numbers work. There was no
- 44:56independent test. You couldn't go look look somewhere specific and
- 45:01either find it or not. Batigen's model was different in
- 45:06a specific way. It didn't just reproduce the clustering. It
- 45:11specified properties. The planet had to be in a roughly
- 45:15anti aligned orbit. It had to have a mass somewhere
- 45:18in the range of five to twenty Earth masses. It
- 45:22had to have a semi major axis in the hundreds
- 45:25of astronomical units. The model predicted what it had to be,
- 45:30not just that something had to exist. That specificity is
- 45:35what distinguishes a real scientific hypothesis from a pattern people
- 45:40talk themselves into. But Tigen has said that every planet
- 45:44ex proposal before this one was essentially a story. You
- 45:48could adjust the planet's parameters freely until the evidence fit,
- 45:53which means the evidence wasn't actually testing anything. This time,
- 45:57the math locked down the parameters independently. The planet had
- 46:02to fit in a particular region of orbital space, or
- 46:06the whole model broke. That is a prediction you can
- 46:10go test with the telescope. That is a prediction that
- 46:15can be falsified. Brown, for his part, described the experience
- 46:21of switching sides as something between uncomfortable and slightly surreal
- 46:27that after years of being the one who said these
- 46:30planets don't exist. He was now standing in front of
- 46:34a calculation he couldn't refute. The two wrote it up
- 46:38and submitted it to the Astronomical Journal. When the paper
- 46:42was published in January of twenty sixteen, it did not
- 46:46claim a discovery. It claimed a prediction, and the difference
- 46:51matters because a real prediction can be tested, and that
- 46:56was exactly what the community was about to try to do.
- 47:01The single most important question about the Planet nine hypothesis
- 47:06is whether the clustering of distant objects is real or
- 47:10whether it is an artifact of where telescopes happen to
- 47:14have been pointed. When Battergen and Brown published their twenty
- 47:18sixteen paper, they were working with six objects, six extreme
- 47:24trans Neptunian objects whose orbits all seemed to be pointing
- 47:29in roughly the same direction. Six sounds small, It sounds
- 47:34like the kind of number a skeptic could dismiss in
- 47:37an afternoon. But what made these six objects remarkable was
- 47:43not just that they were pointing the same way. It
- 47:46was the specific combination of properties they shared. Their orbits
- 47:51were aligned in the same direction. Yes, they were also
- 47:56bunched in terms of orbital tilt and the long axes
- 48:00of their ellipses. The lines that define the orientation of
- 48:04each orbit through space were clustered together in a way
- 48:09that defied easy explanation. You're not just seeing six arrows
- 48:14pointing the same way. You're seeing six arrows that are
- 48:18tilted at similar angles, spun to similar orientations, arranged as
- 48:24if something had reached in and organized them. The probability
- 48:29calculations that came out of the twoenty sixteen paper were
- 48:33striking Battergen and Brown estimated the odds of that particular
- 48:38configuration occurring by chance at around zero point zero zero
- 48:43seven percent. That's roughly one in fourteen thousand. Other researchers,
- 48:51using somewhat different statistical methods and slightly different object selections,
- 48:57put the number closer to one percent. One percent is
- 49:01not zero, but it is still the kind of number
- 49:05that demands explanation. If you shuffled a deck of cards
- 49:10and the first six cards were all aces, you wouldn't
- 49:14assume the deck was fair. Here is what anti alignment
- 49:18actually means, because it's one of the genuinely counterintuitive things
- 49:22about the whole hypothesis. Planet nine is not predicted to
- 49:28sit in the same direction as the objects It is
- 49:31influencing it's predicted to sit on the opposite side of
- 49:35the sky. The clustered objects are bunched in one region
- 49:39of their orbital orientation. Planet nine is expected to be
- 49:44bunched in the opposite region. This seems backwards at first.
- 49:50If a planet is pulling things toward it, why would
- 49:54the objects end up pointing away from it rather than
- 49:57toward it. The answer comes from orbit mechanics and the
- 50:01time scales involved over millions of years. As Planet nine
- 50:06and these distant objects slowly interact through gravity, the resonant
- 50:11dynamics of the system push the objects into configurations that
- 50:16are anti aligned with the planet's own orbit. Think of
- 50:20it less like a magnet pulling iron filings toward it
- 50:24and more like a slow gravitational game where the planet
- 50:29keeps nudging objects into a stable configuration on the far side.
- 50:35The objects aren't pointing toward Planet nine, They're pointing away
- 50:40from it, because that is where the long term stable
- 50:43configuration ends up. It's not intuitive, but the math is solid,
- 50:49and it's one of the features of the hypothesis that
- 50:52couldn't have been guessed without running the actual simulations. Now
- 50:56Here is where things get genuinely complicated because the anti
- 51:01alignment prediction runs directly into the observational bias problem. Most
- 51:07deep surveys of the Outer Solar System have been concentrated
- 51:11in specific regions of the sky. The reason is practical.
- 51:16Some regions are easier to observe from particular telescopes. Some
- 51:21regions are darker further from the galactic plane, less cluttered
- 51:26with background stars. If most of the searches have been
- 51:31conducted in certain patches of sky, then most of the
- 51:35objects found are going to be in those patches. And
- 51:38if most of the objects found are in those patches,
- 51:41they're going to appear clustered there, whether or not any
- 51:45planet is actually organizing them. It's the same logic as
- 51:49a net with big holes. What you catch tells you
- 51:52about the fish in the area, but it also tells
- 51:55you about where you threw the net. But Tigen and
- 51:58Brown knew this was a problem before anyone pointed it
- 52:02out to them. They knew the observational bias argument was
- 52:06the strongest objection to their work, and they spent considerable
- 52:10effort trying to address it. What they did was build
- 52:14a statistical model of where surveys had actually been looking,
- 52:19how deep those surveys went, and what population of objects
- 52:24they were realistically capable of detecting. They then asked whether
- 52:29a uniform, unclustered distribution of extreme trans Neptunian objects could
- 52:36produce the apparent clustering they were seeing, given the biases
- 52:41in where those objects had been found. The answer was
- 52:46that it couldn't. The bias was real, but it was
- 52:50not strong enough to produce the degree of clustering in
- 52:53the actual data. Were they right? That depends on who
- 52:58you ask. Some researchers accepted the bias correction and moved forward.
- 53:04Others argued the bias was harder to model than Battergen
- 53:08and Brown assumed that the searches were more concentrated than
- 53:12the analysis suggested that the sample was too small to
- 53:16draw firm conclusions from. Scott Shephard, one of the researchers
- 53:22who helped start the whole conversation in twenty fourteen, remained cautious.
- 53:28He believed the clustering was suggestive, but thought the sample
- 53:33needed to be larger before anyone could make strong statistical claims.
- 53:39His position wasn't that the planet doesn't exist, It was
- 53:43that the evidence wasn't yet ironclad. As more objects have
- 53:48been discovered, the picture has continued to look more consistent,
- 53:53with the clustering being real. The total number of objects
- 53:58showing the anomalous behavior has grown past six past a dozen,
- 54:04and each new addition either strengthens the pattern or weakens it.
- 54:10So far, the pattern has mostly held. What makes the
- 54:14clustering evidence compelling isn't any single number. It's the combination
- 54:20of the probability calculation, the anti alignment prediction, the multiple
- 54:26independent orbital parameters all pointing the same way, and the
- 54:30fact that the bias corrections, while imperfect, don't seem to
- 54:35make the signal disappear. After correcting for every known source
- 54:41of observational bias they could identify, Battagen and Brown found
- 54:46that the clustering remained statistically significant, not ironclad proof, but
- 54:52strong enough that explaining it without invoking a massive unseen
- 54:57planet required more special plea than most researchers were willing
- 55:02to do. The mechanism by which a single unseen planet
- 55:07could herd dozens of small objects into the same orbital
- 55:11orientation has a name that sounds technical but describes something
- 55:16almost elegant. It is called mean motion resonance, and once
- 55:21you understand what it actually does, the idea that one
- 55:26invisible planet could be quietly organizing the outer Solar System
- 55:31without anyone noticing for centuries starts to feel less like
- 55:35a science fiction premise and more like a straightforward consequence
- 55:40of how gravity works. Start with something familiar. Think about
- 55:46pushing a child on a swing. The swing has a
- 55:50natural rhythm, a period that is set by the length
- 55:53of the chain and nothing else. If you push at
- 55:57random moments, sometimes you add air energy and sometimes you
- 56:01take it away, the swing stays roughly the same. But
- 56:06if you push at exactly the right moment in the cycle,
- 56:09every single time the energy builds, the swing goes higher.
- 56:16The timing is everything. What you are doing, in the
- 56:19language of orbital mechanics is driving a resonance. You are
- 56:24not fighting the system. You are working with it at
- 56:28its own frequency. The result is something stable and controlled
- 56:33that no single random push could ever produce. Mean motion
- 56:38resonance between two orbiting bodies works the same way. When
- 56:43two objects orbit the same star and their orbital periods
- 56:47fall into a simple ratio two to one, three to two,
- 56:52four to nine, they complete their orbits in lockstep. They
- 56:57approach each other at regular, predictable intervals, always in the
- 57:01same configuration, always exchanging a small kick of gravitational energy
- 57:08at the same point in their paths. That regularity is
- 57:13what makes resonance different from a random gravitational nudge. The
- 57:18kicks are not scattered across the orbit. They are concentrated,
- 57:22and over millions of years, concentrated kicks in the same
- 57:26direction add up to something enormous. Jupiter's moons are the
- 57:31clearest example. In our own solar system, Eo, Europa and
- 57:36Ganymede orbit Jupiter in a four to two to one resonance.
- 57:41For every four times Io goes around, Europa goes around twice,
- 57:46and Ganymede once. They have been locked in that ratio
- 57:50for billions of years. The resonance is what keeps them there.
- 57:55Saturn's rings show the same physics from the other direction.
- 58:00A small moon's orbital period lines up with the period
- 58:03of ring particles. The repeated gravitational kicks clear the particles
- 58:08out the dark gaps that Cassini photographed so beautifully. The
- 58:15gaps in Saturn's rings are not accidents. They are the
- 58:19fingerprints of resonance. Places where the math said the kicks
- 58:23would always push outward over time, the particles left. Planet
- 58:30nine is predicted to do something structurally similar to the
- 58:33distant Kuiper Belt objects, just on a far longer time
- 58:38scale and across a vastly wider region of space. The
- 58:43objects in question have orbital periods of thousands of years.
- 58:48Planet nine, if it exists, has an orbital period somewhere
- 58:52between ten thousand and twenty thousand years. The ratios that
- 58:58emerge from those numbers produce resonant configurations, where a distant
- 59:03Kuiper Belt object and Planet nine return to the same
- 59:07relative geometry at regular intervals, separated by thousands of years
- 59:13between each encounter, but repeating with the same precision every time.
- 59:19Here is what happens when one of those objects falls
- 59:22into resonance with Planet Nine at each close approach, and
- 59:27close here means still enormously distant in human terms, but
- 59:33gravitationally significant. The object receives a small nudge. Because the
- 59:39nudge always arrives at the same point in the orbit,
- 59:43it always pushes in the same direction. Over millions of years,
- 59:48This relentless one directional pressure slowly rotates the object's orbital orientation.
- 59:56The long axis of the ellipse, the line that runs
- 59:59from the u s the object's closest approach to the
- 1:00:02Sun all the way out to its farthest point, gradually
- 1:00:06swings around and locks into a specific alignment relative to
- 1:00:10Planet nine. The object does not spiral in, it does
- 1:00:15not fly away. It settles into a configuration where the
- 1:00:20resonance itself becomes self reinforcing, where the kicks now work
- 1:00:25to keep the orbit in place rather than push it further.
- 1:00:30This is the counterintuitive part. The same mechanism that initially
- 1:00:35aligns the orbit then acts as a cage once the
- 1:00:39object is in resonance. The gravitational exchange at each encounter
- 1:00:45pushes back against any perturbation that tries to knock it
- 1:00:49out of alignment. The resonance is self correcting. You can
- 1:00:55think of it like a ball sitting in a bowl.
- 1:00:58Push it in any direction and the walls push back.
- 1:01:03Planet nine does not need to babysit each object individually.
- 1:01:08The orbital mechanics do the work automatically without any ongoing intervention,
- 1:01:15just the same repeating interaction playing out over geological time.
- 1:01:20What Batagen and Brown found when they ran simulations of
- 1:01:23this process was that Planet nine, in the orbit they predicted,
- 1:01:29would naturally produce exactly the clustering that is observed. Objects
- 1:01:34entering the resonance from various starting configurations would, over hundreds
- 1:01:39of millions of years, be steered into the anti aligned
- 1:01:44orientation that the surveys have actually detected. The clustering is
- 1:01:50not a snapshot of some brief coincidence. It is the
- 1:01:54steady state endpoint of a process that has been running
- 1:01:58since the early Solace System, and this matters because the
- 1:02:03number of objects that are supposed to be in this
- 1:02:05pattern is not small. The simulations suggest that over the
- 1:02:11age of the Solar System, planet nine could have shepherded
- 1:02:15a significant fraction of all extreme trans Neptunian objects into
- 1:02:20this configuration, not by touching them, not by coming anywhere
- 1:02:25near them in any meaningful sense, just by existing at
- 1:02:29the right distance, with the right orbital period and letting
- 1:02:33the mathematics of resonance do the rest. The orbital choreography
- 1:02:39is not a coincidence of physics. It is physics working
- 1:02:43exactly as it should. The fact that the distant Kuiper
- 1:02:47Belt objects fit the predicted resonance pattern so well, is
- 1:02:52one of the strongest arguments that something real is out
- 1:02:55there doing the shepherding. Mike Brown discovered Sedna in two
- 1:03:00thousand and three and immediately knew he had a problem.
- 1:03:04Not the good kind of problem, where you find something
- 1:03:07unexpected and the explanation is obvious once you look. The
- 1:03:12bad kind, the kind where you stare at the numbers,
- 1:03:16run them again and realize that what you are looking
- 1:03:19at should not exist under any version of how the
- 1:03:22Solar system is supposed to work. Sedna was not a
- 1:03:27mystery waiting for a clever answer. It was a flat
- 1:03:30contradiction of the standard model, sitting out there in the
- 1:03:34dark at roughly seventy six astronomical units from the Sun,
- 1:03:39following an orbit so stretched and so distant that at
- 1:03:43its farthest point it swings out to around nine hundred
- 1:03:47astronomical units before slowly, over thousands of years, drifting back in.
- 1:03:54And here is the thing that broke the model. At
- 1:03:58its closest approach to the Sun, Sedna still never gets
- 1:04:02anywhere near Neptune. Its perihelion sits at about seventy six
- 1:04:07astronomical units Neptune orbits at roughly thirty that gap matters enormously.
- 1:04:15To understand why, you have to know how normal Kuiper
- 1:04:19Belt objects get their orbits. The standard picture is straightforward.
- 1:04:25Neptune is the great sculptor of the outer Solar System.
- 1:04:29Objects that stray too close to it get gravitationally kicked
- 1:04:33outward into elongated orbits, sometimes extremely elongated ones, stretching hundreds
- 1:04:41of astronomical units from the Sun. But those kicks work
- 1:04:45in both directions. The same gravitational interaction that flings an
- 1:04:51object outward will eventually, over many passes, pull it back.
- 1:04:57Normal scattered disc objects return to netl Tune's neighborhood. They
- 1:05:02cross Neptune's orbit on the way in and on the
- 1:05:04way out. Every interaction leaves a trace. Neptune is the mechanism,
- 1:05:11and the mechanism requires contact. Sedna never makes contact. Its
- 1:05:17orbit does not cross Neptune's Neptune cannot have scattered Sedna
- 1:05:22into its current path because Neptune cannot reach it. Whatever
- 1:05:27puts Sedna where it is, it was not the planet.
- 1:05:30We can see. That is the problem. It is not subtle.
- 1:05:36It is not a statistical anomaly that shows up only
- 1:05:40in refined data. It is a fundamental impossibility under the
- 1:05:45standard model, sitting out there at seventy six astronomical units
- 1:05:50announcing itself every time you run the orbital calculation, So
- 1:05:54what else could explain it? Astronomers came up with three
- 1:05:59serious possibilities. The first was a close stellar encounter. Early
- 1:06:04in the Solar System's history, the Sun formed inside a
- 1:06:08dense stellar nursery, surrounded by thousands of other young stars
- 1:06:13before those stars dispersed over tens of millions of years.
- 1:06:18If one of those stars passed close enough, its gravity
- 1:06:22could have pulled Kuiper Belt objects outward, detaching them from
- 1:06:26Neptune's influence and depositing them in distant orbits with high perihelia.
- 1:06:32The math works roughly a star passing at around eight
- 1:06:37hundred astronomical units could produce objects with Sedna like orbits.
- 1:06:44The problem is that such an encounter would need to
- 1:06:47have happened within the first few hundred million years, and
- 1:06:52it would need to have been a fairly specific kind
- 1:06:54of pass Not impossible, but it requires a piece of
- 1:06:59early sears Solar System history that no one has directly confirmed.
- 1:07:04The second idea was even more dramatic. What if sedna
- 1:07:09was not originally part of our Solar system at all.
- 1:07:13Some models suggested that the Sun could have captured small
- 1:07:16bodies from neighboring stars during the crowded early period in
- 1:07:20the Berth cluster. A passing star brings its own Kuiper
- 1:07:25Belt objects into the neighborhood. The Sun's gravity snags a few,
- 1:07:30and those captured bodies end up in exactly the kinds
- 1:07:34of detached high Perihelian orbits that Sedna occupies. It is
- 1:07:39a legitimate mechanism. Several papers worked out the orbital dynamics
- 1:07:44in reasonable detail, but it is also a difficult idea
- 1:07:48to test, and it still leaves open the question of
- 1:07:52why these orbits look the way they do. The third
- 1:07:55option was quieter, more uncomfortable. What if something is out
- 1:08:01there right now, not a star that passed billions of
- 1:08:05years ago, not a capture from another system, A massive
- 1:08:10body still present, still exerting a gravitational pull on the
- 1:08:15outer Solar system, something that pushed Sedna out and is
- 1:08:19still pushing for years. This idea sat at the edges
- 1:08:23of the conversation because there was only one Sedna. One
- 1:08:28object can be a fluke. One object does not prove
- 1:08:32a pattern. Then, in twenty fourteen, Trujilo and Shepherd found
- 1:08:38two Thy twelve VP one one three. The name is
- 1:08:43not memorable, the orbit is. This object had a perihelion
- 1:08:48of around eighty astronomical units, never approaching Neptune, tracing a
- 1:08:54path through the Outer Solar System with no connection to
- 1:08:58any known planet. A second detached object, a second impossibility,
- 1:09:05the same kind of orbit, the same detachment from Neptune's reach,
- 1:09:10showing up again in the same general region of the sky.
- 1:09:15The chance of two such objects appearing by coincidence with
- 1:09:20no underlying cause started to look very small. What had
- 1:09:25been a mystery doubled overnight. This is the part where
- 1:09:29Battigen and Brown's models become important in a specific way.
- 1:09:34When they ran simulations of the Outer Solar System with
- 1:09:37Planet nine included, something interesting happened. The planet did not
- 1:09:43just shepherd the orbital orientations of extreme trans Neptunian objects.
- 1:09:48Over time, it actively produced Sedna like bodies. Standard Kuiper
- 1:09:55Belt objects interacting with Planet Nine's gravity through the resonance
- 1:10:00mechanism described earlier, got slowly pulled away from Neptune's gravitational reach.
- 1:10:08Their Perihelia lifted over millions of years. Objects that started
- 1:10:14as ordinary scattered disc members ended up detached, tracing high
- 1:10:20Perihelian orbits with no connection to Neptune. The model generated
- 1:10:25Sedna like objects naturally without any special conditions, as a
- 1:10:30direct consequence of planet nine's existence. That is a meaningful result.
- 1:10:37It does not just explain the clustering of orbital orientations.
- 1:10:42It explains why these detached objects exist at all. It
- 1:10:47turns two separate mysteries into one answer, and the answer
- 1:10:51points the same direction. Every other piece of evidence points
- 1:10:56Sedna was not supposed to exist, and finding a second
- 1:11:00one in twenty fourteen only made the problem harder. Two
- 1:11:06objects that cannot be where they are according to any
- 1:11:10model that does not include something massive and unseen sitting
- 1:11:15far out in the dark. One of the tests that
- 1:11:18distinguishes a real scientific hypothesis from a just so story
- 1:11:23is whether it produces unexpected predictions things nobody asked it
- 1:11:28to explain, which turn out to be true anyway. When
- 1:11:32Batttergen and Brown published their twenty sixteen paper, the core
- 1:11:37argument was about clustering. Six extreme trans Neptunian objects were
- 1:11:43bunched together in a way that looked almost impossible by chance,
- 1:11:48and a massive planet in an anti aligned orbit could
- 1:11:52explain the pattern. That was the claim. That was what
- 1:11:57they set out to prove. But the math did not
- 1:12:01stop there. When you run a simulation of how planet
- 1:12:05nine's gravity works on distant objects over hundreds of millions
- 1:12:09of years, something unexpected falls out of the equations. A
- 1:12:15second population of objects should exist, not clustered in the
- 1:12:19same plane as Planet nine, but tilted almost perpendicular to it,
- 1:12:25nearly at right angles to the entire flat disc of
- 1:12:28the Solar System. Nobody asked for this prediction. It just appeared.
- 1:12:34To understand why this happens, you have to think about
- 1:12:38what planet nine is doing two objects over deep time.
- 1:12:43It is not nudging things gently in one direction. It
- 1:12:47is running a slow gravitational campaign across geological time scales,
- 1:12:52pulling orbital orientations into specific configurations. Through resonance. Get locked
- 1:13:01into the anti aligned clustering that started the whole conversation.
- 1:13:05But some objects, depending on where they start and how
- 1:13:09their orbits interact with Planet Nine's influence, get pushed in
- 1:13:14a completely different direction. The math shows that their orbital
- 1:13:18planes get tilted steeper and steeper over millions of years,
- 1:13:23until they are orbiting almost vertically compared to everything else
- 1:13:27in the Solar system. These would be high inclination objects,
- 1:13:33strange ones, the kind that if you found one, you
- 1:13:38might write off as an oddity from some ancient gravitational
- 1:13:42encounter and move on. And that is exactly what astronomers
- 1:13:46had been doing. High inclination trans Neptunian objects were known
- 1:13:52before twenty sixteen. They were considered curiosities. There was no
- 1:13:58unified explanation for why some distant objects followed orbits tilted
- 1:14:03so steeply out of the Solar plane, while most did not.
- 1:14:08Some researchers had noted them, catalogued them, and essentially filed
- 1:14:13them away under unexplained phenomena. There were bigger puzzles to
- 1:14:18work on. Then Battagen and Brown's paper arrived, and the
- 1:14:23prediction was right there in the appendix, Planet nine should
- 1:14:27be producing a population of objects in roughly perpendicular orbits.
- 1:14:32Here is what those orbits should look like. Here is
- 1:14:36the range of inclinations to expect. And observers went back
- 1:14:40through existing survey catalogs with fresh eyes and started checking.
- 1:14:46What they found was striking, There were already objects in
- 1:14:50the data that matched the prediction almost exactly. High inclination,
- 1:14:56extreme trans Neptunian objects sitting in all orbits tilted between
- 1:15:01roughly fifty and one hundred thirty degrees relative to the
- 1:15:05solar plane, clustered along specific orientations that the planet nine
- 1:15:11model had predicted in advance. Not one object, not two,
- 1:15:18several of them, distributed across the sky in a pattern
- 1:15:22consistent with what the simulation had produced. Objects that had
- 1:15:26seemed like isolated anomalies were suddenly part of a coherent picture.
- 1:15:32In the last few years before this writing, observers identified
- 1:15:36at least four objects tracing orbits along one perpendicular line
- 1:15:41from Neptune and one object along another. These are small numbers,
- 1:15:47but the point is not the count. The point is
- 1:15:50the match. These objects were not discovered in order to
- 1:15:54confirm the prediction. They are already sitting in survey archives
- 1:16:00cataloged before the planet nine hypothesis existed. The prediction was published,
- 1:16:06and then someone checked whether reality had already done the experiment.
- 1:16:12This is how scientific confidence actually builds. It is not
- 1:16:17about finding more examples of the thing your theory was
- 1:16:20designed to explain Any sufficiently flexible model can be tuned
- 1:16:25to fit its target data. What you cannot fake is
- 1:16:29a prediction that goes somewhere. The theory was not aimed. Planet
- 1:16:34nine was proposed to explain orbital clustering in one specific plane.
- 1:16:39The perpendicular population prediction was a byproduct of the mathematics,
- 1:16:45not the goal. When a theory wanders into territory, it
- 1:16:50was never pointed at and still describes what is actually there.
- 1:16:55That is a different kind of evidence. Think about what
- 1:16:59it would take for this to be a coincidence. You
- 1:17:03would need the high inclination objects to be distributed roughly randomly.
- 1:17:09You would need the specific orientations Battagen and Brown calculated
- 1:17:14to have no particular meaning, and you would need all
- 1:17:19of this to line up with the survey archives. By chance,
- 1:17:23the probability gets uncomfortable quickly, not impossible, but uncomfortable in
- 1:17:29exactly the way that makes researchers lean forward in their chairs.
- 1:17:33There are still legitimate questions. The sample is small. A
- 1:17:38handful of objects is not a statistical avalanche. Each new
- 1:17:43discovery of a high inclination extreme tno either fits the
- 1:17:48pattern or introduces a complication, and the community is still
- 1:17:53working through what the full distribution actually looks like. High
- 1:17:58inclination objects are harder to find than low inclination ones
- 1:18:02because surveys tend to be concentrated near the solar plane.
- 1:18:07That bias means the known population is almost certainly incomplete,
- 1:18:12and the real distribution could look different once a deeper,
- 1:18:16wider survey fills in the gaps, but the core fact
- 1:18:20does not go away. Before twenty sixteen, nobody knew why
- 1:18:25certain distant objects followed nearly vertical orbits. After twenty sixteen,
- 1:18:32there was a specific model that said those objects should exist,
- 1:18:36described roughly where they should be concentrated, and explain the
- 1:18:40mechanism producing them. The mechanism is the same long period
- 1:18:45resonance that drives the clustering Planet nine as a gravitational
- 1:18:51shepherd creates two populations at once, one aligned, one perpendicular,
- 1:18:58and both seemed to be real. Observers found the perpendicular
- 1:19:03objects they were already in the data, waiting to be
- 1:19:07recognized for what they were, and that fact alone moved
- 1:19:12Planet nine from an interesting speculation to something that looks
- 1:19:16increasingly like a real prediction about the actual structure of
- 1:19:21the Solar System. The predicted orbit of planet nine has
- 1:19:24been moving around as more data comes in, and tracking
- 1:19:28how it has changed actually tells you a lot about
- 1:19:31how the hypothesis has matured. When Battagen and Brown published
- 1:19:36their original twenty sixteen paper, the numbers were wide. They
- 1:19:42estimated Planet nine sat somewhere between four hundred and eight
- 1:19:46hundred astronomical units from the Sun. One astronomical unit is
- 1:19:52the distance from the Earth to the Sun about ninety
- 1:19:56three million miles. Neptune, the outermost known planet, orbits at
- 1:20:02roughly thirty astronomical units, So even the closest end of
- 1:20:06that early estimate put Planet nine more than thirteen times
- 1:20:10farther out than Neptune. The far end put it almost
- 1:20:15twenty seven times farther. That is not a tight constraint.
- 1:20:20That is a search area the size of a continent
- 1:20:22when you are looking for something the size of a house.
- 1:20:26The reason the range was so wide comes down to
- 1:20:29how the orbit gets inferred in the first place. Researchers
- 1:20:33are not measuring Planet nine directly. They are working backwards
- 1:20:38from the motion of small objects. It is presumably pushing
- 1:20:41around the more extreme trans Neptunian objects. You have well
- 1:20:46characterized orbits for the tighter your model gets. In twenty sixteen,
- 1:20:53the data set was thin, six objects good enough to
- 1:20:58identify the cluster pattern, not good enough to pin down
- 1:21:02the planet's exact position with any precision. Every new object
- 1:21:07added to the catalog since then has acted like a
- 1:21:10new data point, tightening the picture. By twenty twenty one,
- 1:21:15the estimate had sharpened considerably. The semi major axis, which
- 1:21:20is the average distance across the full length of the orbit,
- 1:21:24came down to roughly three hundred eighty astronomical units, with
- 1:21:29an uncertainty range that had narrowed significantly compared to the
- 1:21:33original proposal. That number shifted again shortly after landing closer
- 1:21:40to four hundred sixty astronomical units. Then, in twenty twenty five,
- 1:21:47with better modeling and more objects in the data set,
- 1:21:50researchers pushed it down further to around two hundred ninety
- 1:21:55astronomical units, with an uncertainty of plus or minus about
- 1:22:00thirty astronomical units. That is a meaningful compression. The search
- 1:22:08area has gone from a sprawling range spanning hundreds of
- 1:22:11astronomical units to something researchers can actually start pointing telescopes
- 1:22:17at systematically, what does an orbit at two hundred ninety
- 1:22:21astronomical units actually look like. Planet nine is not in
- 1:22:27a circular orbit. That much has been clear from the beginning.
- 1:22:31A circular orbit at two hundred ninety astronomical units would
- 1:22:35be strange enough on its own, but the orbit is
- 1:22:39highly eccentric, stretched out in an elongated ellipse rather than
- 1:22:44a round loop. That means the planet swings relatively close
- 1:22:48at one end its perihelion, and then arcs out to
- 1:22:53a much farther distance at the other end its ophelion.
- 1:22:58Current models put the perry Heels somewhere in the range
- 1:23:01of three hundred astronomical units, and the Aphelian outpassed five
- 1:23:07hundred astronomical units, possibly farther. The planet spends most of
- 1:23:13its time near the far end of that arc, which
- 1:23:16is part of why it is so hard to find.
- 1:23:20It moves slowly out there, it reflects almost no sunlight,
- 1:23:25and it is pointed away from the parts of the
- 1:23:28sky that most survey have covered most thoroughly. The orbital
- 1:23:32period follows from those numbers. At a semi major axis
- 1:23:37near two hundred ninety astronomical units, Planet nine would take
- 1:23:42somewhere between ten thousand and twenty thousand years to complete
- 1:23:46a single orbit around the Sun. To put that in perspective,
- 1:23:51ten thousand years ago, humans were just beginning to farm.
- 1:23:56The planet has not completed a single full loop in
- 1:24:00all of recorded human history. We are watching one frame
- 1:24:04of a very slow film. The orbital inclination, the angle
- 1:24:09at which Planet nine's orbit tilts relative to the flat
- 1:24:13plane of the Solar System, adds another layer of complexity
- 1:24:18to the search. The best current models suggest an inclination
- 1:24:22of somewhere around fifteen to twenty degrees that is tilted
- 1:24:27enough to push the planet out of the narrow band
- 1:24:29of sky where most planetary surveys are concentrated, but not
- 1:24:34so extreme that it would be invisible to wide field
- 1:24:37surveys designed to cover large areas. Now Here is the
- 1:24:42part that matters practically. The twoenty twenty five refinement, pushing
- 1:24:48the semi major axis estimate down toward two hundred ninety
- 1:24:52astronomical units, has a direct consequence for detectability. The closer
- 1:24:59something is, the more sunlight reaches it. Sunlight falls off
- 1:25:04with the square of the distance an object at two
- 1:25:08hundred ninety astronomical units receives more than twice as much
- 1:25:13light as the same object sitting at four hundred sixty
- 1:25:17astronomical units. That makes it brighter in the sky, not
- 1:25:23dramatically brighter. We are still talking about an extraordinarily faint
- 1:25:28object against a field of millions of background stars, but
- 1:25:32the margin matters when you are building a survey strategy
- 1:25:36around barely detectable signals. The mass estimate has moved two.
- 1:25:42The original twenty sixteen paper put Planet nine at roughly
- 1:25:47ten Earth masses. That number has been revised downward. Current
- 1:25:53estimates lean toward five to six Earth masses. That puts
- 1:25:57it firmly in the category researchers a super Earth or
- 1:26:01sub Neptune, smaller than the original proposal, but still massive
- 1:26:07enough to explain the gravitational effects on the Outer Solar System.
- 1:26:12Whether it is closer in character to a scaled up
- 1:26:15rocky planet or a stripped down ice giant is still
- 1:26:19an open question. A twenty twenty five study suggested the
- 1:26:24composition might skew rocky rather than icy, which would affect
- 1:26:29its reflectivity and therefore how bright it appears. All of
- 1:26:34these refinements, the shrinking semi major axis. The updated mass
- 1:26:40the tighter inclination range feed directly into where astronomers point
- 1:26:45their telescopes next. A hypothesis that can only say somewhere
- 1:26:51between four hundred and eight hundred astronomical units in some
- 1:26:55direction is nearly impossible to test in any reasonable timeframe.
- 1:27:02A hypothesis that says roughly two hundred and ninety astronomical
- 1:27:06units inclined about fifteen degrees currently near a particular region
- 1:27:11of sky is a search target. That shift from vague
- 1:27:16to specific is how a theoretical idea becomes something you
- 1:27:20can actually go look for. The latest models suggest Planet
- 1:27:24nine is somewhat closer and somewhat smaller than originally thought,
- 1:27:29which sounds like bad news for a dramatic discovery, but
- 1:27:32is actually good news for finding it. A closer still
- 1:27:37massive planet means that if the right survey points at
- 1:27:40the right piece of sky at the right moment, the
- 1:27:44discovery could happen very soon. The question every skeptic asks
- 1:27:49first is the obvious one. If there is a planet
- 1:27:53out there, why hasn't anyone seen it? It is a
- 1:27:57fair question. We have craters on Mars, photographed storms on
- 1:28:03Jupiter's moons, and tracked asteroids no bigger than a house.
- 1:28:09The idea that an entire planet, something five or six
- 1:28:13times the mass of Earth could be sitting in our
- 1:28:16own Solar system without anyone noticing seems almost absurd. But
- 1:28:20the answer comes down to a few brutal physical realities,
- 1:28:25and once you understand them, the mystery of why we
- 1:28:28haven't found it starts to feel less like a failure
- 1:28:32and more like an inevitability. Start with light. Everything we
- 1:28:37see in the sky, from distant galaxies to the faint
- 1:28:41smudge of a comet, is visible because it reflects or
- 1:28:45emits light that reaches our instruments. Planet nine reflects sunlight,
- 1:28:51just like every other planet. The problem is how much
- 1:28:55sunlight reaches it in the first place. Light from the
- 1:28:59Sun weaken with distance, following what physicists call the inverse
- 1:29:04square law. Double the distance, reduce the brightness by a
- 1:29:08factor of four. At Neptune, roughly thirty astronomical units from
- 1:29:15the Sun, sunlight is already about nine hundred times fainter
- 1:29:19than what hits Earth. Planet nine is predicted to sit
- 1:29:24somewhere between three hundred and five hundred astronomical units out
- 1:29:29at five hundred astronomical units. Sunlight arrives at roughly one
- 1:29:35millionth the intensity we experience here. The planet reflects that
- 1:29:40already feeble l et back toward us, and by the
- 1:29:45time those photons travel hundreds of astronomical units back to Earth,
- 1:29:50the signal is extraordinary. Small Planet nine would be so
- 1:29:54dim that even our most sensitive instruments struggle to pick
- 1:29:58it out against the back ground darkness of space. Then
- 1:30:02there is the sky itself. People underestimate how enormous it is.
- 1:30:08The whole celestial sphere covers roughly forty one thousand square
- 1:30:12degrees planet nine's predicted orbit based on the latest models,
- 1:30:18sweeps across a significant fraction of that area, and pinpointing
- 1:30:22exactly where along that orbit the planet sits right now
- 1:30:26is still an open problem. Surveys don't just point at
- 1:30:30one place and stare. They work in strips and patches,
- 1:30:34accumulating coverage over years. Even the largest modern sky surveys
- 1:30:40have covered the full sky only a handful of times,
- 1:30:43and most of those sweeps were not deep enough or
- 1:30:46sensitive enough to detect something as faint as Planet nine
- 1:30:50at the distances being discussed. Wise is a good example.
- 1:30:55The wide field Infrared Survey Explorer was launched in two
- 1:30:59thousand nine and mapped the entire sky in infrared light,
- 1:31:04exactly the kind of observation you would want for detecting
- 1:31:07a cold, dark, distant world. Astronomers searched its data specifically
- 1:31:14for planet nine candidates. They found nothing that held up,
- 1:31:19but wise was optimized for a different kind of science,
- 1:31:23detecting warm objects like brown dwarfs and nearby stars. Its
- 1:31:29sensitivity at the wavelengths and distances relevant to Planet nine
- 1:31:33was limited, not ruled out, just not found pan stars.
- 1:31:40A Hawaii based optical survey that has imaged huge portions
- 1:31:44of the sky repeatedly over the past decade also came
- 1:31:47up empty. Again, not because the planet isn't there, but
- 1:31:53because optical surveys looking invisible light faced the s aim
- 1:31:57fundamental problem. A planet reflecting one millionth of already weak
- 1:32:02sunlight produces almost no signal at visible wavelengths. These were serious,
- 1:32:08rigorous searches. They just weren't quite the right tool at
- 1:32:12the right depth. Here is the specific challenge that makes
- 1:32:16this search so technically brutal. Planet nine, if it exists,
- 1:32:22would appear in a single image as a point of light.
- 1:32:26That is it, no disk, no fuzzy glow, no distinguishing feature,
- 1:32:32just a dot identical in appearance to the billions of
- 1:32:36stars and galaxies captured in any wide field survey image.
- 1:32:41There is no way to identify it from a single observation.
- 1:32:46The only way to know you are looking at a
- 1:32:48planet rather than a star is to see it move.
- 1:32:52Stars are so far away that they appear fixed in
- 1:32:56the sky over any human timescale, A planet, even a
- 1:33:01very distant and slow moving one, drifts visibly against the
- 1:33:06stellar background if you compare observations taken months or years apart.
- 1:33:11But Planet nine moves slowly at five hundred astronomical units,
- 1:33:18tracing an orbit that takes somewhere between ten thousand and
- 1:33:22twenty thousand years to complete. The planet barely crawls across
- 1:33:26the sky from our perspective. In a single year, it
- 1:33:31would shift by roughly a fraction of a degree detectable,
- 1:33:36but only if you know where to look and have
- 1:33:39images taken at the right spacing to catch that tiny drift.
- 1:33:45Running that kind of comparison automatically across billions of objects
- 1:33:49in archived survey data is a genuinely hard computational problem,
- 1:33:56most surveys weren't designed to do it. What this means
- 1:33:59in practice is that the relevant archived data is enormous
- 1:34:04and still only partially searched in the systematic way needed
- 1:34:09to catch slow moving faint objects. Survey images pile up
- 1:34:14over years. Each one contains millions of sources matching the
- 1:34:20same patch of sky across observations taken months or years apart,
- 1:34:25filtering out artifacts, handling gaps in coverage, and then flagging
- 1:34:31anything that has shifted by the tiny amount expected for
- 1:34:35a five hundred astronomical unit object. That is the work,
- 1:34:40and it is painstaking. Some of it has been done,
- 1:34:44most of it has not. There is also the coverage
- 1:34:48problem to consider. Honestly, the parts of sky that have
- 1:34:52been searched most deeply are not uniformly distributed. Some regions
- 1:34:58have been imaged many times. Others, particularly in the southern
- 1:35:02hemisphere and in areas obscured by the dense star fields
- 1:35:06near the galactic plane, have sparse coverage or none at all.
- 1:35:12Planet nine's predicted orbital path crosses some of those poorly
- 1:35:16surveyed regions. The absence of a detection in well covered
- 1:35:21sky doesn't tell you much about what might be sitting
- 1:35:25in the gaps. It is genuinely possible that planet nine
- 1:35:29has already appeared in existing survey images multiple times without
- 1:35:34being recognized, a faint moving dot, dismissed as noise, or
- 1:35:40simply unexamined because no one knew to compare two images
- 1:35:44taken years apart at the right coordinates. In twenty twenty five,
- 1:35:50a team of researchers searching through archival infrared survey data
- 1:35:55announced they had found something, not a planet, not a
- 1:36:00confirmed discovery, something a faint point of infrared light, sitting
- 1:36:06in two different positions in two different surveys taken twenty
- 1:36:10three years apart. The object had moved, and the distance
- 1:36:15it covered in those twenty three years was exactly what
- 1:36:19you would expect from planet nine moving along its predicted orbit.
- 1:36:24That is not nothing. That is, in fact the most
- 1:36:29promising lead the search has ever produced. Here is what
- 1:36:33the data actually shows. In nineteen eighty three, a space
- 1:36:38telescope called IRAS, the Infrared Astronomical Satellite, swept the sky
- 1:36:44in infrared wavelengths and catalogued hundreds of millions of objects.
- 1:36:50It was the first all sky infrared survey ever completed,
- 1:36:55and the images have been sitting in archives ever since. Later,
- 1:37:01a Japanese satellite called Akari conducted its own infrared survey
- 1:37:06of the same sky. When researchers laid the two data
- 1:37:10sets side by side and looked carefully at the region
- 1:37:14where planet nine is predicted to be, they found something odd.
- 1:37:19A faint source appears in the IRS data at one position.
- 1:37:25That same source does not appear in the Akari data
- 1:37:28at that position but roughly forty seven arc minutes away,
- 1:37:34a small but measurable shift against the background stars. There
- 1:37:39is an object in the Akari images that was not
- 1:37:42there in iras. The two detections are separated by twenty
- 1:37:48three years and about forty seven arc minutes of sky.
- 1:37:53That angular movement matches the expected drift of a planet
- 1:37:57sitting somewhere around seven hundred hundred astronomical units from the
- 1:38:02Sun tracing a slow arc across the background field of
- 1:38:06distant stars. Seven hundred astronomical units is farther out than
- 1:38:11the orbital models most researchers have been working with. Recently,
- 1:38:15The twoenty twenty five refinements pushed planet nines likely location
- 1:38:20closer somewhere between two hundred ninety and four hundred sixty
- 1:38:25astronomical units. An object at seven hundred astronomical units would
- 1:38:31be even slower, moving, even colder, even dimmer than those
- 1:38:36estimates suggest, But orbital models carry real uncertainty, and the
- 1:38:42predictions are ranges, not exact values. A seven hundred astronomical
- 1:38:48units detection would be on the outer edge of those ranges,
- 1:38:53but not outside the realm of what the hypothesis actually allows.
- 1:38:57The object, if it is real, would be large. The
- 1:39:01infrared brightness suggests something with a mass greater than Neptune
- 1:39:06that fits. Planet nine was never supposed to be small
- 1:39:11five to ten Earth masses, roughly Neptune class in size.
- 1:39:16That is the target range. An object detectable in the
- 1:39:20IRAS data at that distance would have to be emitting
- 1:39:25faint heat of its own, a slow thermal glow from
- 1:39:28a world that formed billions of years ago and has
- 1:39:32been cooling in the dark ever since. At seven hundred
- 1:39:36astronomical units from the Sun, there is almost no solar
- 1:39:41heating to speak of. The planet's own internal warmth is
- 1:39:46essentially all it has left. So why isn't this a discovery?
- 1:39:50Because two data points do not make an orbit. You
- 1:39:54need a trajectory. You need to see the object in
- 1:39:57at least three positions, ideally more to calculate where it
- 1:40:01has been and where it is going. Iras and Akari
- 1:40:06give two positions twenty three years apart. That is a
- 1:40:11starting direction. It is not a confirmed path. The object
- 1:40:17could theoretically be something closer and faster that happened to
- 1:40:21land in those two positions by coincidence. The probability of
- 1:40:26that is low, but it is not zero. Before anyone
- 1:40:30can say this is planet nine, the object needs to
- 1:40:33be found in a third data set, preferably a modern
- 1:40:37one with enough depth and resolution to pin down its
- 1:40:40location precisely. Then the orbit can be calculated, then the
- 1:40:46claim can be made. The researchers who published the Candidate
- 1:40:49were careful about all of this. They described exactly what
- 1:40:54they had found, exactly why it was interesting, and exactly
- 1:40:59what would be needed to confirm it. That kind of
- 1:41:02precision matters. The history of planet nine claims, and really
- 1:41:08the history of trans Neptunian planet claims going back over
- 1:41:12a century, is littered with detections that did not survive scrutiny.
- 1:41:18Being careful is not timidity. It is the whole point.
- 1:41:23The reaction from the broader Planet nine community was what
- 1:41:27you might expect from people who have been hunting something
- 1:41:30for a decade and suddenly have the best lead they
- 1:41:33have ever seen. Cautious, genuinely excited, careful about what the
- 1:41:39data does and does not say. Mike Brown called it interesting.
- 1:41:45Constantine Battigin acknowledged the candidate, but noted that recovery in
- 1:41:50a third observation is the essential next step. The phrasing
- 1:41:55from most researchers was some version of this is promise,
- 1:42:00and we need more data. And this is exactly the
- 1:42:04kind of thing that could turn into a real discovery
- 1:42:07or could turn into another false alarm, and right now
- 1:42:12we cannot tell which. What makes this particular candidate harder
- 1:42:16to resolve quickly is the age of the source data.
- 1:42:21IRIS observed in nineteen eighty three, Akari's relevant survey was
- 1:42:26conducted in the mid two thousands. Neither instrument exists in
- 1:42:31a form that can take new observations. The follow up
- 1:42:35has to come from completely different telescopes aimed at a
- 1:42:39specific patch of sky, going deep enough in infrared wavelengths
- 1:42:44to pick up a faint cold, distant object that most
- 1:42:49surveys were never designed to detect. Some of that follow
- 1:42:54up is already underway. Whether it produces a recovery or
- 1:42:58a non detection, the answer will come from painstaking work
- 1:43:03comparing new deep images against the predicted position, looking for
- 1:43:09a faint source that has crept a little further along
- 1:43:12its arc since the last time anyone looked. There is
- 1:43:17also the question of what a non detection would mean.
- 1:43:20If the object cannot be found in current imaging at
- 1:43:23the predicted position, that does not automatically mean the twenty
- 1:43:27twenty five candidate was wrong. It might mean the orbital
- 1:43:31estimate is off. It might mean the object is fainter
- 1:43:35than expected. It might mean the follow up surveys were
- 1:43:39not deep enough. This is the frustrating reality of hunting
- 1:43:44something at the edge of the Solar System. Absence of
- 1:43:47detection is not the same as proof of absence, but
- 1:43:51a positive recovery would be unambiguous. You find it moving,
- 1:43:57you calculate the orbit, You check whether where it matches
- 1:44:00the planet nine prediction. That is the moment everything changes
- 1:44:06until the object is recovered in a third independent observation
- 1:44:10and an actual orbit can be calculated the twoenty twenty
- 1:44:14five candidate. Sits where most things in science sit before
- 1:44:18they become discoveries, in the space between a compelling lead
- 1:44:23and a confirmed result, which is a genuinely uncomfortable place
- 1:44:27to be. In late twenty twenty five, the most powerful
- 1:44:32survey telescope ever built began scanning the Southern Sky from
- 1:44:37a mountaintop in Chile. The timing was not accidental. The
- 1:44:43planet nine search had reached the point where the next
- 1:44:46step required an instrument that did not yet exist, and
- 1:44:50then suddenly it did. The Vera Sea Reuben Observatory sits
- 1:44:55at an elevation of nearly two thousand, seven hundred meters
- 1:44:59on Sero pachon, a peak in the Chilean andes chosen
- 1:45:04specifically for its stable atmosphere and exceptional darkness. What it
- 1:45:10does is straightforward in concept and almost absurd in scale.
- 1:45:15Every few nights it photographs the entire Southern Sky, then
- 1:45:20it does it again, then again. Over ten years, it
- 1:45:25will image roughly ten billion individual objects, and its computers
- 1:45:30will compare every new image against the archive, flaging anything
- 1:45:35that has moved. That last part is the whole game.
- 1:45:41Finding Planet nine is not a matter of pointing a
- 1:45:44telescope at one location and waiting for something to appear.
- 1:45:49The planet, if it exists, would look like a point
- 1:45:52of light, indistinguishable from millions of background stars. At first glance.
- 1:45:58Stars don't move, at least not perceptibly on human timescales.
- 1:46:03A planet does. Catch the same piece of sky twice,
- 1:46:08separated by months, and a planet will have shifted position.
- 1:46:13Catch it a third time and you have a trajectory
- 1:46:17at Planet nine's predicted distance of somewhere between three hundred
- 1:46:21and six hundred astronomical units. That motion is extremely slow.
- 1:46:28We're talking about a world moving at a pace that
- 1:46:31would take it ten to twenty thousand years just to
- 1:46:35complete one full lap around the Sun. But slow is
- 1:46:40not the same as undetectable. The Reuben Observatory's ten year
- 1:46:45baseline is long enough to watch it creep. The numbers
- 1:46:49behind the telescope are worth sitting with for a moment.
- 1:46:53Its primary mirror is eight point four meters across. Its camera,
- 1:46:58called l S s ST Cam, is the largest digital camera
- 1:47:03ever built for astronomy, collecting images across a three point
- 1:47:07two billion pixel detector. Each single exposure covers an area
- 1:47:13of sky, roughly fifty times larger than the full moon.
- 1:47:17The system can scan the entire accessible southern sky every
- 1:47:21three to four nights. No telescope with this combination of depth, speed,
- 1:47:27and coverage has ever existed. Previous surveys like pan Stars
- 1:47:32and WYS had pieces of what was needed, neither had
- 1:47:36all of it at once. The Ruben Observatory has all
- 1:47:40of it. Mike Brown has been asked many times what
- 1:47:44instrument he would build if the goal was specifically to
- 1:47:48find planet nine. His answer is always the same. He
- 1:47:52would build the Ruben Observatory, not a variation of it,
- 1:47:57not something inspired by it, exactly that telescope. It is,
- 1:48:03in his framing, the perfect machine for this particular problem,
- 1:48:07not because it was designed with Planet nine in mind,
- 1:48:10but because the requirements for conducting the deepest, most comprehensive
- 1:48:15survey of the time varying southern sky happen to align
- 1:48:19almost perfectly with what the planet nine search demands. The
- 1:48:25fact that it exists and is operational right now is,
- 1:48:30depending on how you look at it, either very good
- 1:48:33luck or the inevitable result of planetary science reaching the
- 1:48:38point where this kind of instrument was necessary. Here is
- 1:48:43how the detection would actually work. The Reuben Observatory's software pipeline,
- 1:48:48running continuously as new images come in, subtracts each fresh
- 1:48:53exposure from the stored archive. Anything that has stayed in
- 1:48:57the same position drops out of the comparaison. Anything that
- 1:49:01has moved stays in the system then catalogs the moving
- 1:49:06objects and attempts to link detections across multiple nights into
- 1:49:11coherent orbital tracks. For known populations like asteroids and comets,
- 1:49:18this is routine. For something at Planet nine's distance, the
- 1:49:23motion between exposures taken a few nights apart would be tiny,
- 1:49:28smaller than many expected signals, but over months and years,
- 1:49:33the accumulated drift becomes unambiguous. The pipeline is designed specifically
- 1:49:40to find this kind of slow, faint, distant motion. There
- 1:49:45is a practical constraint worth mentioning. The Reuben Observatory surveys
- 1:49:49the southern sky, not the whole sky. Planet nine's predicted
- 1:49:54orbit does not confine it to the southern hemisphere, and
- 1:49:57current models place it somewhere in a broad arc that
- 1:50:01spans both hemispheres. If Planet nine happens to be sitting
- 1:50:05in the northern portion of its orbit right now. The
- 1:50:09Reuben Observatory will not find it directly. What it will
- 1:50:13do is eliminate the southern portion of the predicted parameter
- 1:50:18space with a thoroughness that no previous survey has approached.
- 1:50:24That alone would reshape the search significantly. A non detection
- 1:50:29in the southern sky after ten years of deep coverage
- 1:50:33would push the orbital models toward northern solutions and tell
- 1:50:38northern sky observatories exactly where to concentrate. But the optimistic
- 1:50:43reading of the timeline is more exciting. Brown and Battigan's
- 1:50:47most recent orbital estimates in twenty twenty five placed Planet
- 1:50:52nine at roughly two hundred ninety to four hundred sixty
- 1:50:56astronomical units, somewhat closer than earlier pricretions had suggested. Closer
- 1:51:02means brighter. Brighter means the Ruben observatory has a better
- 1:51:07chance of catching it in fewer years rather than more.
- 1:51:12Some researchers think the detection, if it happens, could come
- 1:51:16early in the survey window rather than at the end.
- 1:51:20The telescope has been running for months now, the data
- 1:51:24is accumulating, the comparison pipeline is running every night. What
- 1:51:30makes this moment different from every previous phase of the
- 1:51:34Planet nine search is that the waiting is no longer passive.
- 1:51:39Earlier researchers could only analyze the objects already known and
- 1:51:45run orbital simulations. Now there is an active machine specifically
- 1:51:51configured to catch the thing they have been looking for.
- 1:51:55Each night the Ruben Observatory runs adds another leg of
- 1:52:00data to the archive. Each new comparison narrows the space
- 1:52:04where Planet nine can hide. The search has a clock
- 1:52:07on it now, and the clock is running. Brown's prediction
- 1:52:11is specific. If something starts moving across the survey images
- 1:52:16at around five hundred to six hundred astronomical units from
- 1:52:20the Sun, following the predicted orbital path, it will be
- 1:52:25planet nine, and the Reuben Observatory is essentially built to
- 1:52:30catch exactly that kind of slow, faint, distant motion. Not
- 1:52:36everyone is convinced the vera Reuben Observatory may be perfectly
- 1:52:41positioned to find Planet nine, but a meaningful portion of
- 1:52:45the scientific community is not yet willing to accept that
- 1:52:50there is something out there to find. These are not
- 1:52:54fringe voices. They are working astronomers with serious objections. Their
- 1:53:01arguments deserve the same attention as the evidence. On the
- 1:53:05other side, The loudest challenge to the planet nine hypothesis
- 1:53:10is not about the planet itself, It is about the
- 1:53:13data being used to justify it. Samantha Lawla, an astronomer
- 1:53:19at the University of Regina, has argued that the apparent
- 1:53:24clustering of extreme trans Neptunian objects is not a real signal.
- 1:53:30It is a ghost. When astronomers go looking for faint
- 1:53:34distant objects in the Outer Solar System, they do not
- 1:53:37scan the entire sky Equally, Surveys concentrate on certain regions.
- 1:53:44Some parts of the sky get studied again and again,
- 1:53:48others go almost completely unexamined. If your catalog of known
- 1:53:54extreme TNOs is drawn primarily from the regions where telescopes
- 1:53:59have pointed more often, the objects in that catalog will
- 1:54:03cluster in those regions almost automatically, not because something is
- 1:54:08pulling them there, b because nobody looked anywhere else. This
- 1:54:14is observational bias. It is a genuine problem for any
- 1:54:19argument built on the positions of a small, carefully selected
- 1:54:23sample of objects. Lawla and her colleagues have run simulations
- 1:54:27of this effect. They modeled what the known distribution of
- 1:54:31extreme TNOs would look like if the actual underlying population
- 1:54:37were spread randomly across the sky, but surveys had only
- 1:54:41covered certain portions of it. The result looked remarkably similar
- 1:54:47to the clustering that Battagen and Brown pointed to as
- 1:54:50evidence for planet nine. If Lawla is right, the Solar
- 1:54:55system's distant edge may be perfectly ordinary. A pattern is
- 1:55:00a systematic artifact of incomplete data. This is a hard
- 1:55:05argument to dismiss. The sample of known extreme trans Neptunian
- 1:55:10objects is small, depending on how you define the category
- 1:55:15you are talking about, somewhere between a dozen and a
- 1:55:19few dozen objects. Statisticians will tell you that drawing strong
- 1:55:24conclusions from a sample that size is risky, even under
- 1:55:28ideal conditions. When the sample itself is collected through an
- 1:55:34inherently biased process, those conclusions get shakier still. Batagen and
- 1:55:41Brown have pushed back on this. They have argued that
- 1:55:45their analysis accounts for known observational biases, that the clustering
- 1:55:50persists even when they correct for the regions of sky
- 1:55:54that have been searched most heavily. The probability of the
- 1:55:58observed alignment occurring by chance after correction, They estimate it
- 1:56:04somewhere between roughly one percent and a fraction of a percent.
- 1:56:09Those are not certainty level numbers, but they are not nothing.
- 1:56:14Where you fall on this argument depends significantly on how
- 1:56:18much you trust the bias corrections. That is a judgment
- 1:56:23call that reasonable scientists are making. Differently. Then there are
- 1:56:28the alternative explanations that do not involve a planet at all.
- 1:56:34One class of models invokes dark matter. The idea is
- 1:56:39that the gravitational influence attributed to planet nine might instead
- 1:56:44be coming from a concentration of dark matter somewhere in
- 1:56:48the outer Solar System, or from the overall large scale
- 1:56:52distribution of dark matter in the galaxy affecting the orbits
- 1:56:56of very distant objects. Most recves find this explanation more
- 1:57:01complicated than it needs to be. The specific predictions it
- 1:57:06makes are harder to test, but it is a legitimate
- 1:57:10scientific position that cannot simply be ruled out. Modified gravity
- 1:57:16is another alternative. Some researchers have proposed that our understanding
- 1:57:22of how gravity works at extremely large scales may be incomplete,
- 1:57:28that the anomalous orbits of distant Kuiper Belt objects are
- 1:57:32a signature of that incompleteness, rather than evidence of a
- 1:57:36hidden mass. These are serious theoretical proposals, not idle speculation,
- 1:57:44though most planetary scientists consider them less economical than the
- 1:57:48planet nine hypothesis. Scott Shepherd sits in a different category
- 1:57:53from the outright skeptics. He was one of the original
- 1:57:56researchers who notice the clustering problem. He co authored the
- 1:58:01twoenty fourteen paper with Truhilo that first raised the alarm.
- 1:58:06He is not arguing that the signal is definitely fake.
- 1:58:10He is arguing that the statistics are not yet strong
- 1:58:13enough to say it is definitely real. His position is
- 1:58:18essentially that the current sample size cannot carry the weight
- 1:58:21being placed on it. More extreme trans Neptunian objects need
- 1:58:26to be found and their orbits need to be characterized
- 1:58:30before the clustering argument becomes truly compelling. The statistical case
- 1:58:36for planet nine, in his view, is not closed. It
- 1:58:41is open, and it will remain open until the data
- 1:58:45set is substantially larger. This matters because Shepherd knows the
- 1:58:50data better than almost anyone. He has spent years surveying
- 1:58:55the Outer Solar System. When he says the evidence is
- 1:58:59not efficient, he is not speaking from ignorance of what
- 1:59:03the evidence says. He is speaking from a deep familiarity
- 1:59:08with how fragile the sample still is. The community as
- 1:59:12a whole reflects this spread of positions. Brown describes himself
- 1:59:17as extraordinarily confident. Batagen has said that unlike every previous
- 1:59:23planet exclaim, this hypothesis comes with a specific, testable prediction.
- 1:59:30Others are more measured, a few are genuinely skeptical in
- 1:59:35the lawless sense, believing the whole pattern dissolves once you
- 1:59:40account properly for where the surveys have pointed. There is
- 1:59:44no consensus here in any useful meaning of the word.
- 1:59:48What makes this uncomfortable is that both sides are using
- 1:59:52the same underlying data set and reaching fundamentally different conclusions
- 1:59:58about what it means. That is a sign that the
- 2:00:02data set is not yet good enough to settle the argument.
- 2:00:06That is precisely what Shepherd has been saying. More surveys,
- 2:00:11more objects, better bias corrections, an independent detection from a
- 2:00:17telescope like the Reuben observatory. That is what it will
- 2:00:21take to move from a contested claim to a resolved one.
- 2:00:26The honest state of the field is that if you
- 2:00:29walked into a room of twenty planetary scientists and asked
- 2:00:33for a show of hands, you would get a spread
- 2:00:37of answers. The researchers who think Planet nine probably exists
- 2:00:43are not uniformly confident. The ones who doubt it are
- 2:00:47not uniformly dismissive. It is exactly the kind of contested
- 2:00:52leave question that makes planetary science worth following. Right now,
- 2:00:58in twenty twenty five, research has announced a new object
- 2:01:02in the Outer Solar System, and it immediately made things
- 2:01:06more complicated. The object has a name that only an
- 2:01:10astronomer could love, twoenty seventeen o F two zero one.
- 2:01:17It's roughly seven hundred kilometers across, which puts it in
- 2:01:21the range of a dwarf planet candidate. That's about the
- 2:01:25distance from New York to Chicago, end to end, rolled
- 2:01:29into a ball of ice and rock, sitting billions of
- 2:01:32miles from the Sun. By any normal measure, it's a
- 2:01:36small thing, but its orbit is not small at all.
- 2:01:41The path this object traces around the Sun is one
- 2:01:44of the most elongated ever recorded for a body this size.
- 2:01:49It swings out to enormous distances far beyond Neptune, far
- 2:01:54beyond the bulk of the Kuiper Belt into the same
- 2:01:58cold territory where Planet nine is predicted to rome. When
- 2:02:03the team first announced it, the natural reaction from the
- 2:02:07Planet nine community was something close to excitement. Here was
- 2:02:13another object on an extreme orbit that conventional Solar system
- 2:02:17physics struggles to explain. Something had to push it out there,
- 2:02:23something had to give it that elongated path. Planet nine
- 2:02:27was the obvious candidate. So far, so good. Then the
- 2:02:32modeling started. When researchers ran the numbers on twenty seventeen
- 2:02:37F two zero one, in detail, a problem surfaced. The
- 2:02:42clustering that sits at the heart of the planet nine
- 2:02:45hypothesis is not just about objects having extreme orbits. It's
- 2:02:51about those extreme orbits all pointing in roughly the same direction.
- 2:02:56The argument of perihelion, the longitude of ascending none, the
- 2:03:01orientation of the orbital plane. These parameters cluster together among
- 2:03:06the known extreme trans Neptunian objects in a way that
- 2:03:10screams gravitational influence from a single massive source. That clustering
- 2:03:17is the evidence, that's what the whole case rests on.
- 2:03:21And twoenty seventeen O F two zero one did not
- 2:03:25cluster with the others. Its orbits sat outside the predicted pattern,
- 2:03:31not wildly outside, not in some completely different region of
- 2:03:35parameter space, but outside enough to notice, outside enough to
- 2:03:41create a real scientific tension. What does that actually mean.
- 2:03:46There are two ways to read it, and they point
- 2:03:49in opposite different directions. The first reading is that twoenty
- 2:03:54seventeen o F two zero one supports the planet nine picture.
- 2:04:00The hypothesis predicts that a massive outer planet would scatter
- 2:04:04objects across a range of extreme orbits over millions of years.
- 2:04:10Not every object gets nudged into the same clustered configuration.
- 2:04:15Some get pulled into the clustering, some get pushed into
- 2:04:19perpendicular orbits, and some end up in less ordered paths
- 2:04:24that still reflect the chaotic gravitational history of the outer
- 2:04:29Solar System. Under this reading, twoenty seventeen o F two
- 2:04:35zero one is exactly the kind of outlier you'd expect.
- 2:04:40Its unusual orbit is consistent with the general influence of
- 2:04:43a large unseen planet, even if it doesn't contribute to
- 2:04:47the specific clustering signal. The second reading is less comfortable
- 2:04:52for the hypothesis. If Planet nine is real and its
- 2:04:56gravity is shepherding distant objects into coherent orbital families, then
- 2:05:01why is this object not part of the family. Every
- 2:05:05nonconforming object is a data point that doesn't fit the model.
- 2:05:10One nonconforming object is easy to dismiss. But the concern
- 2:05:16is what happens as more surveys come in and more
- 2:05:19objects are discovered. If the outer Solar system turns out
- 2:05:24to be full of extreme TNOs that don't cluster, the
- 2:05:28statistical case weakens. The researchers behind the twenty seventeen o
- 2:05:34F two zero one paper were careful. They didn't claim
- 2:05:38the discovery broke planet nine. They said more data is needed.
- 2:05:44That phrase appears constantly in this field, and it is
- 2:05:48not a deflection. It is a genuine statement about where
- 2:05:52the science is. Here's the underlying issue. The total number
- 2:05:57of known extreme trans Neptunian object is still remarkably small.
- 2:06:03Astronomers are making a statistical argument about the structure of
- 2:06:07a vast dark region of space based on a sample
- 2:06:11that most statisticians would call uncomfortably thin. Adding one object
- 2:06:18that doesn't fit the pattern doesn't destroy the statistics, but
- 2:06:23it does shift them slightly in the wrong direction, and
- 2:06:28it raises a question that the skeptics have been asking
- 2:06:31from the beginning. Is the clustering signal in the existing
- 2:06:36sample real or is it a reflection of where the
- 2:06:39surveys happen to look. What made twenty seventeen F two
- 2:06:44zero one particularly interesting was the question of how it
- 2:06:49got to where it is. Its highly elliptical orbit is
- 2:06:53not something that forms easily from standard Solar System dynamics.
- 2:06:58Something gave it that part. The researchers noted that planet
- 2:07:03nine could explain it, but so could a close stellar
- 2:07:07encounter early in the Solar System's history, or dynamics that
- 2:07:11don't require any undiscovered planet at all. The orbit taken
- 2:07:17alone doesn't confirm anything. It's consistent with several scenarios at once.
- 2:07:24That ambiguity is exhausting in the best possible way, because
- 2:07:28it means the outer Solar System is still generating genuine
- 2:07:32puzzles faster than existing models can resolve them. The Vera
- 2:07:36Reuben Observatory is expected to find dozens, possibly hundreds of
- 2:07:41new extreme trans Neptunian objects over the next decade. Each
- 2:07:47one will either strengthen the clustering signal or dilute it.
- 2:07:52Twenty seventeen F two zero one was a preview of
- 2:07:57what that process is going to feel like. A new
- 2:08:00object announced, the community examines the orbit, the orbit doesn't
- 2:08:06behave exactly as predicted, and everyone updates their confidence levels
- 2:08:11slightly while agreeing that the question is still open. The
- 2:08:16Outer Solar System has a way of producing exactly the
- 2:08:20kind of ambiguous evidence that keeps a question open just
- 2:08:25when it seems like it might be closing. And two
- 2:08:29thy seventeen o F two zero one was a perfect
- 2:08:33example of that. If Planet nine is real, the next
- 2:08:38question is obvious. Where did it come from? This is
- 2:08:42not a simple question. An object five or six times
- 2:08:46the mass of Earth sitting somewhere between three hundred and
- 2:08:50five hundred astronomical units from the Sun on an orbit
- 2:08:55so elongated it takes ten thousand to twenty thousand years
- 2:08:59to comple single loop that is not where planets are
- 2:09:03supposed to end up. Normal planet formation does not produce this.
- 2:09:09Something had to put it there. The leading candidates for
- 2:09:14how that happened are genuinely different from each other in
- 2:09:18ways that matter. The theory that Battagen and Brown consider
- 2:09:23most plausible starts about four and a half billion years ago.
- 2:09:27In the first few million years of the Solar System's existence.
- 2:09:32The early Solar System was nothing like the orderly arrangement
- 2:09:35we see today. It was a chaotic, dense environment, a
- 2:09:41disk of gas, dust, rocky debris swirling around a young Sun,
- 2:09:47with planetary embryos forming and colliding and being flung around
- 2:09:52by gravitational interactions that played out over millions of years.
- 2:09:57The four giant planets Jupiter, Saturn, Uranus, and Neptune were
- 2:10:03not sitting where they are now. They were closer in
- 2:10:08and they were moving. In this picture, Planet nine started
- 2:10:12out as the core of what might have become a
- 2:10:15fifth giant planet. It was growing in the inner part
- 2:10:19of the outer disc, accumulating mass, heading toward the threshold
- 2:10:24where it would have started pulling in hydrogen and helium
- 2:10:27gas and becoming something like Jupiter. It never got there.
- 2:10:33Before it could cross that threshold, it wandered too close
- 2:10:37to one of the giants, most likely Jupiter, possibly Saturn.
- 2:10:43What followed was a gravitational slingshot. The planet's close approach
- 2:10:48gave Jupiter or Saturn a tiny nudge inward while flinging
- 2:10:53the smaller body outward at enormous speed. One encounter, one pass,
- 2:10:59and a planet sized object that had been forming in
- 2:11:02a relatively normal part of the Solar System was suddenly
- 2:11:06launched into a wildly elongated orbit that carried it far
- 2:11:11beyond anything we would call the Solar System today. At
- 2:11:16this point, the ejected core would have been on an
- 2:11:19orbit that carried it almost all the way out of
- 2:11:23the Solar System, entirely its ophelion. The farthest point of
- 2:11:28its orbit would have been extraordinarily distant, possibly thousands of
- 2:11:34astronomical units from the Sun. But it didn't escape, and
- 2:11:39this is where the story gets interesting. The early Sun
- 2:11:43was not alone. It formed inside a stellar nursery, a
- 2:11:47dense cluster of young stars, all born from the same
- 2:11:51collapsing cloud of gas. Hundreds of stars packed into a
- 2:11:56relatively small region of space, all moving around each other,
- 2:12:01all exerting gravitational influences on everything nearby. The gravity of
- 2:12:07those passing stars, combined with drag from the leftover gas
- 2:12:11of the solar nebula, slowly worked on Planet nine's orbit.
- 2:12:17Each close stellar pass nudged the orbit slightly, the gas
- 2:12:22drag pulled energy out of the most extreme part of
- 2:12:25the trajectory. Over millions of years, this gradually raised the
- 2:12:30closest point of the orbit the perihelion, and reduced the
- 2:12:35farthest point. What started as a nearly escape velocity trajectory
- 2:12:40slowly settled into something more stable. By the time the
- 2:12:45Sun's berth cluster dispersed, planet nine was locked into a
- 2:12:49distant but permanent orbit around our star. The odds of
- 2:12:54this scenario playing out exactly right have been estimated at
- 2:12:58a few percent. That sounds low, but a few percent
- 2:13:03is not zero. Over the violent, chaotic timescales of early
- 2:13:08planetary formation, a few percent is actually a reasonable outcome.
- 2:13:13The Solar System built four giant planets and had extra
- 2:13:18material left over, something plausibly could have started forming a fifth.
- 2:13:23There are other theories. One is that planet nine did
- 2:13:27not form in our Solar System at all. The Sun's
- 2:13:31berth cluster was crowded enough that two young stars could
- 2:13:35have passed within gravitational capture range of each other. In
- 2:13:39this scenario, planet nine was originally orbiting a different star.
- 2:13:45During a close encounter, the gravitational tug of war between
- 2:13:49the two stars pulled Planet nine free from its original
- 2:13:53host and left it bound to the Sun instead. Capture
- 2:13:58is actually a known Mesha mechanism. We think the outer
- 2:14:02aut cloud may contain objects that were gravitationally borrowed from
- 2:14:06neighboring stars during exactly this kind of early cluster interaction.
- 2:14:12Whether a planet sized object could survive capture in a
- 2:14:16stable orbit is a more complicated question, but the physics
- 2:14:21does not rule it out. A third possibility is that
- 2:14:25planet nine formed where it currently lives, or somewhere close
- 2:14:30to it. The outer disc of the early Solar System
- 2:14:34extended a long way out and there was material available.
- 2:14:39The problem with in place formation at extreme distances is
- 2:14:43that the material in the outer disc would have been
- 2:14:46spread too thinly to efficiently accumulate into a planet sized
- 2:14:51object in any reasonable timeframe. The disc was too sparse,
- 2:14:57the collision rates too low, the formation window too short.
- 2:15:03Most researchers find this scenario the least convincing of the three,
- 2:15:08though it is not impossible if there was a local
- 2:15:10concentration of material driven by some disk instability. The rogue
- 2:15:15planet capture scenario is a fourth option. Planet nine as
- 2:15:20a free floating world ejected from some other star system,
- 2:15:24entirely drifting through interstellar space until the Sun's gravity caught
- 2:15:29it at just the right moment. The window for this
- 2:15:33kind of capture is extremely narrow. It requires a very
- 2:15:38specific geometry, a very specific relative velocity. The probability is
- 2:15:45low enough that most researchers do not treat it as
- 2:15:48a serious front runner, though it cannot be fully dismissed.
- 2:15:52What most researchers keep coming back to is the ejection story.
- 2:15:57It fits the predicted orbital characteristics better than the alternatives.
- 2:16:03It is consistent with what the Niece model tells us
- 2:16:06about the early Solar System's dynamical history. It requires no
- 2:16:11exotic physics, no unusual stellar encounters, no improbable capture geometry,
- 2:16:19just a young Solar system doing what young Solar systems
- 2:16:23apparently do, throwing pieces of itself into the dark. Whatever
- 2:16:28mechanism put Planet nine in its current orbit. The Solar
- 2:16:32System's early history was violent enough that a few percent
- 2:16:36probability is not a long shot. It is the kind
- 2:16:40of thing that, given enough time and enough gravitational encounters,
- 2:16:46you would expect to happen at least once. If Planet
- 2:16:50nine is out there, it is nothing like any planet
- 2:16:54that has ever had a name, not like Earth, not
- 2:16:57like Neptune, not like anything in the life lineup of
- 2:17:00eight worlds most people learned in school. It belongs to
- 2:17:04a category that astronomers have named, But our solar system
- 2:17:09until now has never clearly displayed five to six times
- 2:17:14the mass of Earth that puts it in a range
- 2:17:18researchers call a super Earth or sub Neptune, and it
- 2:17:22is worth pausing on what that actually means, because the
- 2:17:25name is doing a lot of work. A super Earth
- 2:17:29is not just a bigger version of our planet. At
- 2:17:33five or six Earth masses, the gravity pulling on the
- 2:17:36surface would be significantly stronger. The internal pressure at the
- 2:17:42core would be far beyond anything Earth experiences. The planet
- 2:17:48would be a fundamentally different kind of object, sitting in
- 2:17:52a size class that turns out to be the most
- 2:17:54common type of Powell and It in the galaxy. We
- 2:17:58just don't have one nearby to study. What does the
- 2:18:00interior look like? That depends on which model you trust,
- 2:18:05and the models have shifted recently. The earlier picture was
- 2:18:10something close to a mini Neptune, a dense, rocky core
- 2:18:14buried under a thick shell of water and ice, possibly
- 2:18:18capped by a deep hydrogen helium atmosphere. Something in the
- 2:18:22same family as Uranus or Neptune, just smaller. More recent
- 2:18:28work has pushed back on that. Some researchers now think
- 2:18:31planet nine's composition skews rocky, more like a massive terrestrial
- 2:18:36planet than an icy giant. The distinction matters for detection
- 2:18:41because a rockier planet reflects light differently than an icy one,
- 2:18:46and the predicted brightness used by search teams is built
- 2:18:50on assumptions about what the surface is actually made of.
- 2:18:54If those assumptions are wrong, the planet could be dimmer
- 2:18:58than expected or brighter. Right now, nobody knows. What is
- 2:19:03not in question is the temperature. At five hundred astronomical
- 2:19:09units from the Sun, planet nine would be extraordinarily cold,
- 2:19:14the kind of cold that makes the outer planets look tropical.
- 2:19:18By comparison, Neptune, sitting at about thirty astronomical units, already
- 2:19:25reaches surface temperatures around negative two hundred degrees celsius. Planet
- 2:19:31nine is more than fifteen times farther out. At that distance,
- 2:19:37the Sun's heat is essentially irrelevant. Surface temperatures would sit
- 2:19:42close to absolute zero, somewhere around negative two hundred twenty
- 2:19:47to negative two hundred thirty degrees celsius, possibly colder there
- 2:19:53is no process delivering meaningful warmth from outside. Any heat
- 2:19:58coming from the planet itself would be left over energy
- 2:20:02from its formation, slowly leaking out over billions of years.
- 2:20:08The planet is, in every practical sense frozen. The darkness
- 2:20:14is harder to comprehend than the cold. Sunlight at planet
- 2:20:18nine's distance is one millionth as bright as it is
- 2:20:21here on Earth, not one percent, not one thousandth one
- 2:20:26millionth On Earth on a clear day, sunlight is roughly
- 2:20:31one thousand, three hundred watts per square meter. At planet nine.
- 2:20:37That number drops to something in the range of a
- 2:20:39thousandth of a watt. A single household candle produces more
- 2:20:44light than the sun delivers to Planet nine's surface. This
- 2:20:49is why the planet is so difficult to detect. It
- 2:20:53does not glow on its own and barely reflects anything
- 2:20:58from Earth. It would appear as an extraordinarily faint point
- 2:21:03of light, dimmer than thousands of objects we have already catalogued,
- 2:21:08indistinguishable from background stars, unless you catch it moving across
- 2:21:13the sky over months or years. Now, imagine standing there,
- 2:21:19not in any practical sense, just as a thought experiment.
- 2:21:23You are on the surface of planet nine or whatever
- 2:21:26passes for a surface, and you look up. The sky
- 2:21:30is black, completely black. There are no nearby planets catching
- 2:21:35the Sun's light, no moon overhead, nothing bright enough to
- 2:21:39illuminate the ground beneath your feet. The stars are there,
- 2:21:44the same stars visible from Earth, but they shed nothing useful.
- 2:21:50Then you find the Sun. It is not hard to locate,
- 2:21:54because it is the brightest thing in the sky by
- 2:21:57an enormous margin. The other star in the night sky
- 2:22:01seen from Earth, tops out at a certain brightness. The
- 2:22:06sun from Planet nine would blow past all of them.
- 2:22:10It would look like an intensely brilliant point of light,
- 2:22:14far out shining anything else in the sky, the kind
- 2:22:18of brightness that would be painful to look at directly,
- 2:22:21even from that distance. But it would be a star,
- 2:22:26not a disk. No warmth, no colour spread across the horizon,
- 2:22:33no sense of a nearby star, just a hard, blinding
- 2:22:38pea ooint against an otherwise featureless black sky. The surface itself,
- 2:22:44if the planet has one, would be completely dark, no shadows,
- 2:22:50no texture visible to human eyes. Whatever geological features exist,
- 2:22:56craters or ridges or frozen planes of compressed ice and rock,
- 2:23:01they would be invisible without artificial light. The gravity would
- 2:23:05pull noticeably harder than Earth's. The atmosphere, if there is one,
- 2:23:11might be a thin shell of frozen gases clinging to
- 2:23:14the surface, or nothing at all. If the light elements
- 2:23:18have long since escaped. It would be a world that
- 2:23:22has been sitting in near perfect isolation for billions of years,
- 2:23:27untouched by sunlight, unvisited, unknown, standing on the surface of
- 2:23:34Planet nine, if it has a surface in any meaningful sense,
- 2:23:38the Sun would be nothing more than the brightest star
- 2:23:41in an otherwise pitch black sky, shedding no warmth, casting
- 2:23:46no shadows, giving no light that a human eye could use.
- 2:23:52That is not a problem for scientists. That is the
- 2:23:55kind of problem that energizes astronomers. Throughout the history of astronomy,
- 2:24:02observations have repeatedly challenged prevailing models of how planets form
- 2:24:07and evolve. This is not viewed as a setback, but
- 2:24:11as an opportunity. When telescopes reveal unexpected features in distant
- 2:24:16solar systems, or when laboratory analysis of meteorites produces surprising
- 2:24:22isotopic signatures, researchers recognize these moments as gateways to deeper understanding.
- 2:24:31The scientific process thrives on such contradictions. They force researchers
- 2:24:37to examine their assumptions more carefully. They demand more rigorous
- 2:24:42testing of existing theories. They open new avenues of investigation
- 2:24:48that might never have been pursued otherwise. Consider how our
- 2:24:53models of planetary formation have evolved over decades. Early models
- 2:24:59were relatively simple, proposing that planets coalesced from cosmic dust
- 2:25:04in straightforward patterns. As observations accumulated, the picture became more complex.
- 2:25:12Astronomers discovered planetary systems arranged in ways that seemed to
- 2:25:16violate the assumptions built into older models. Some planets orbited
- 2:25:22far closer to their stars than theory predicted. Others occupied
- 2:25:27orbits that crossed the paths of neighboring worlds. These observations
- 2:25:32sparked intense scientific discussion. Researchers began proposing new mechanisms to
- 2:25:39explain the data. They suggested that planets could migrate across
- 2:25:44vast distances. They proposed that gravitational interactions between young planets
- 2:25:51could reshape orbital configurations dramatically. Each new observation refined the
- 2:25:58model further. The same principle applies to understanding the early
- 2:26:03Solar systems, specifically, For many years, scientists relied on a
- 2:26:09relatively static model of how our system formed. It was
- 2:26:13assumed that planets settled into their current orbits relatively quickly
- 2:26:18and remained there. Then came observations of exoplanetary systems that
- 2:26:24showed far greater dynamism and chaos than anyone had anticipated.
- 2:26:30These observations, combined with new theoretical work, led to the
- 2:26:35development of the NIS model and other sophisticated frameworks. These
- 2:26:41frameworks proposed that the Young Solar System was far more
- 2:26:45turbulent than previously imagined. Planets that formed in one region
- 2:26:51migrated to different orbital zones. Gravitational interactions between multiple planetary
- 2:26:58bodies created how some smaller bodies were ejected from the
- 2:27:03system entirely, others were scattered into different regions. These revised
- 2:27:10models explained previously puzzling observations about asteroid and comet distribution patterns.
- 2:27:16The study of the Moon's formation history provides an excellent
- 2:27:20illustration of how observations transform understanding. For decades, scientists debated
- 2:27:28the origin of the Moon. Multiple competing models existed. Some
- 2:27:33propose that the Moon had condensed from the same material
- 2:27:37as Earth, forming as a coplanetary body. Others suggested that
- 2:27:43Earth had captured the Moon gravitationally from elsewhere in the
- 2:27:47Solar System. Still others argued for different mechanisms entirely. The
- 2:27:53ambiguity persisted because direct evidence was limited. Then came the
- 2:27:59Apollo Miss. Astronauts brought back hundreds of kilograms of lunar samples.
- 2:28:06Scientists analyzed these rocks with increasingly sophisticated techniques. The isotopic
- 2:28:12composition revealed crucial information. The samples showed that the Moon's
- 2:28:18m aterial was not identical to Earth's material, yet too
- 2:28:23similar to be a captured body from elsewhere. This observation
- 2:28:28effectively eliminated several competing models. It pointed toward a different
- 2:28:34mechanism entirely, a giant impact. The giant impact hypothesis proposed
- 2:28:40that a Mars sized body collided with the early Earth.
- 2:28:45The immense energy from this collision vaporized material from both bodies.
- 2:28:51Debris from the impact disc coalesced into the Moon. This
- 2:28:56model could explain the isotopic similarities between Earth than Moon
- 2:29:01while accounting for their differences. It accounted for the Moon's
- 2:29:05relatively large size compared to Earth. It explained the Moon's
- 2:29:10unusual orbital characteristics. When observations of other planetary systems revealed
- 2:29:16that giant impacts might be relatively common during planetary formation,
- 2:29:22the hypothesis gained additional credibility. What had once seemed like
- 2:29:27a radical and controversial idea became the mainstream scientific view.
- 2:29:32Yet even this refined model continues to evolve. New observations
- 2:29:38raise new questions. Precise measurements of the Moon's composition have
- 2:29:44revealed subtle variations in different samples. Some concentrations of elements
- 2:29:50differ slightly from what the original giant impact model predicted.
- 2:29:56Researchers continue to refine their understanding of the collision and
- 2:30:00specific characteristics. Did multiple impacts occur rather than one single event,
- 2:30:08What was the exact size and composition of the impacting body?
- 2:30:13At what velocity did the collision occur? How much of
- 2:30:17the Moon's material came from Earth versus the impact. Scientists
- 2:30:22cannot yet answer all these questions definitively, but the process
- 2:30:28of attempting to answer them drives research forward. This pattern
- 2:30:32repeats throughout astronomical science. Models serve a crucial function. They
- 2:30:39organize our understanding and make predictions that can be tested.
- 2:30:44When observations confirm predictions, confidence in the model increases when
- 2:30:51observations contradict the model. That contradiction is valuable data. It
- 2:30:58signals that something important remains misunderstood. It indicates whether the
- 2:31:03model's simplifications or assumptions break down. Rather than viewing this
- 2:31:09as failure, the scientific community embraces it as progress. The
- 2:31:15process of questioning and refining models is not separate from science.
- 2:31:20It is the essence of science. When a confirmed observation
- 2:31:25breaks a good model, the model gets better, the understanding
- 2:31:30of what happened four billion years ago gets sharper. By
- 2:31:34most estimates, the wait is not long. Fred Adams at
- 2:31:38the University of Michigan has looked at the current rate
- 2:31:42of new trans Neptunian object discoveries run the numbers concluded
- 2:31:48that somewhere around twenty thirty five, the data pool will
- 2:31:52be large enough to either confirm planet nine or force
- 2:31:56the field to abandon the hypothesis entirely. That is not
- 2:32:01a long time. Most people reading this will be alive
- 2:32:05to see that answer arrive. The question is whether the
- 2:32:09answer will be yes or no, And right now nobody
- 2:32:13can tell you. The instrument at the center of that
- 2:32:16timeline is the Vera Sea Reuben Observatory in Chile, which
- 2:32:21began its survey of the Southern Sky in twenty twenty five.
- 2:32:26Over the next ten years, it will image roughly ten
- 2:32:29billion objects, comparing new observations against old ones, continuously flagging
- 2:32:36anything that moves. Planet nine, if it sits in the
- 2:32:40Southern Sky at the predicted distance, will move slowly at
- 2:32:45five hundred astronomical units. The orbital speed is glacial from
- 2:32:49our perspective, but it will move. The Reuben Observatory is
- 2:32:55precisely the kind of machine designed to catch that kind
- 2:32:58of feint low drift. Mike Brown, the Caltech astronomer who
- 2:33:05co authored the original twenty sixteen prediction, has said that
- 2:33:10if someone handed him unlimited funds and told him to
- 2:33:14build the perfect Planet nine telescope, he would build exactly
- 2:33:18what Rubinli ready is. That is not a casual endorsement.
- 2:33:24That is a researcher saying the right tool finally exists.
- 2:33:28So what happens if the Reuben Observatory finds it. The
- 2:33:32answer is not simply that a new planet gets added
- 2:33:35to the list. The discovery would mean the early Solar
- 2:33:39System was far more violent than current formation models describe.
- 2:33:44It would mean a planetary core formed close to the
- 2:33:47Sun was flung outward by a gravitational encounter with Jupiter
- 2:33:53or Saturn survived the ejection has been orbiting in the
- 2:33:58dark at extreme distance from billions of years. No planet
- 2:34:03has ever been confirmed to have done this. The NIE model,
- 2:34:07which describes how the giant planets migrated early in the
- 2:34:11Solar System's history, would need revision. The broad architecture of
- 2:34:16our Solar System, long assumed to be the product of
- 2:34:19a relatively orderly formation process, would turn out to be
- 2:34:24the survivor of something messier, and our Solar System, long
- 2:34:29thought to be unusual for lacking super earths and sub neptunes,
- 2:34:34the most common planet type found around other stars, would
- 2:34:38turn out to have one all along, just hiding. What
- 2:34:43does non detection mean? This is where the picture gets
- 2:34:47more complicated. If the Ruben Observatory completes its survey and
- 2:34:53finds nothing matching the predicted orbital parameters, that does not
- 2:34:58prove Planet nine is app The southern sky covers most
- 2:35:03but not all, of the predicted search zone. A planet
- 2:35:07in the right orbital configuration could still be sitting in
- 2:35:10a part of the sky the survey could not reach
- 2:35:13deeply enough, but non detection would be significant. It would
- 2:35:19force researchers back to the clustering evidence and ask harder
- 2:35:23questions about whether that evidence was ever as strong as
- 2:35:27it looked. The observational bias problem, the concern that extreme
- 2:35:34trans Neptunian objects have been discovered in concentrated patches of
- 2:35:39sky rather than uniformly. An illusion of clustering would move
- 2:35:45from a minority objection to the main explanation on the table.
- 2:35:51The field would have to either find a new explanation
- 2:35:54for the clustering or accept that the sample was never
- 2:35:58large enough to draw concs pcllusions from. The clustering itself
- 2:36:03has been the backbone of the hypothesis since two thy
- 2:36:07sixteen six objects became a dozen. The statistics tightened. The
- 2:36:13probability of a random arrangement producing what was observed dropped
- 2:36:18well below one percent by most calculations, But statistics are
- 2:36:23only as reliable as the sample they are drawn from.
- 2:36:27The extreme outer Solar system is not uniformly surveyed. Every
- 2:36:32new object discovered carries the potential to either reinforce the
- 2:36:37pattern or break it. The twoenty twenty five discovery of
- 2:36:42twenty twenty three KQ fourteen, a sedna like object whose
- 2:36:47perihelion points in the opposite direction from other known sednoids,
- 2:36:53has already pushed the predicted orbital distance for planet nine
- 2:36:57farther out. The picture keeps shifting. That is not a
- 2:37:02weakness in the hypothesis. That is how science works when
- 2:37:07the data is still coming. In the twenty twenty five
- 2:37:11infrared candidate, the faint source that appeared in one position
- 2:37:15in the nineteen eighty three IRS data and a shifted
- 2:37:20position in later Akari imaging sits in the background of
- 2:37:24all of this like an unresolved note. The movement is
- 2:37:29consistent with planet nine at roughly seven hundred astronomical units.
- 2:37:35The signal is real, but one recovery in archival data
- 2:37:39does not make a confirmed orbit. A confirmed orbit is
- 2:37:44what the field requires before anything gets announced as a discovery.
- 2:37:50Astronomers are currently trying to locate the object in more
- 2:37:53recent survey images. If they find it, and if the
- 2:37:58trajectory matches, the timeline to resolution could compress dramatically. The
- 2:38:04answer might not take until twenty thirty five. It might
- 2:38:09come sooner that is the thing about this search that
- 2:38:13is genuinely unusual compared to most open questions in planetary science.
- 2:38:18The window is defined, the instrument is running, the orbital
- 2:38:23models are specific enough to tell observers where to look.
- 2:38:28The candidate in the archival infrared data is already being chased.
- 2:38:33At some point in the next decade, the Reuben Observatory's
- 2:38:37computers will compare two images separated by months identify a
- 2:38:43point of light that has drifted against the background stars.
- 2:38:48Either that drift will match a planet nine orbit, or
- 2:38:52it will not. The answer is coming. The question is
- 2:38:57just which answer it will be. Right now, somewhere in
- 2:39:01a vast stretch of sky that the surveys have not
- 2:39:04yet covered deeply enough, there may be a frozen world
- 2:39:08larger than Earth, tracing a slow arc around a Sun
- 2:39:12that barely illuminates it. And either it is there waiting
- 2:39:16to be found, or it is not. The Solar System
- 2:39:21is stranger and emptier than we thought. Either answer is
- 2:39:26going to change something fundamental about the picture we have
- 2:39:29been building for the last four hundred years.