What Actually Happens If You Reach The Edge Of The Solar System — Transcript
Full transcript
- 0:00You are strapped into a seat that
- 0:01stopped being comfortable about 4 hours
- 0:03ago, and the engine behind you has just
- 0:05shut down. That silence is the important
- 0:07part. The burn is finished. The number
- 0:10on the screen in front of you says you
- 0:11are moving faster than any human being
- 0:13has ever moved, and nothing in front of
- 0:15you is going to slow you down for a very
- 0:17long time. You are heading for the edge
- 0:19of the solar system. The first thing
- 0:21that surprises you is how boring it
- 0:23looks.
- 0:24There is no tunnel of light, no sense of
- 0:26speed, no rushing. Out of the window,
- 0:29the stars sit exactly where they were
- 0:30yesterday. The only thing that tells you
- 0:32anything is happening at all is Earth,
- 0:35and Earth is already smaller than it
- 0:36should be. You watch it for a while,
- 0:39blue, white, unmistakable.
- 0:41Then a few days pass, and it is the size
- 0:43of a coin, then a marble, then it stops
- 0:46being a place and becomes a light.
- 0:48Somewhere around week two, you catch
- 0:50yourself looking for it and not finding
- 0:52it immediately. That is the moment the
- 0:54trip becomes real, not the launch, not
- 0:57the burn. The moment you have to search
- 0:59the sky for your entire species. You
- 1:01pass the orbit of Mars without seeing
- 1:03Mars. This disappoints you more than you
- 1:05expected. Space is mostly not where the
- 1:08things are, and the odds of a planet
- 1:10happening to be in the same neighborhood
- 1:11of its orbit as you are extremely poor.
- 1:14You cross one of the most famous lines
- 1:16in the solar system, and the view does
- 1:17not change at all. The asteroid belt is
- 1:20worse. You were braced for it. Everyone
- 1:23is braced for it. In your head, there
- 1:24was a wall of tumbling rock, and you
- 1:27weaving through it with your jaw
- 1:28clenched. What actually happens is that
- 1:31you cross the entire asteroid belt and
- 1:33never see a single asteroid. The rocks
- 1:35are there, millions of them, and they
- 1:37are separated by distances so absurd
- 1:40that missing them is not a skill, it is
- 1:42the default.
- 1:44This is your first proper lesson about
- 1:46the solar system. It is not a crowded
- 1:48place with dangerous gaps. It is an
- 1:50enormous emptiness with a few objects in
- 1:52it, and you are going to spend months
- 1:54being reminded of that. The next thing
- 1:56to change is not outside. It is the
- 1:58conversation.
- 2:00At first, talking to mission control was
- 2:02normal.
- 2:03Then there was a pause. Then the pause
- 2:05got long enough that you started
- 2:06planning your sentences around it. By
- 2:08the time you are past the belt, you say
- 2:10something and you wait, and you go and
- 2:12eat, and you come back, and the answer
- 2:15is there.
- 2:16Nobody is talking to you anymore. People
- 2:18are leaving you messages. There is a
- 2:20difference, and you feel it long before
- 2:22you admit it. Jupiter is the first place
- 2:25that actively tries to hurt you. You
- 2:27approach it from a distance that feels
- 2:29safe and is not. Jupiter has a magnetic
- 2:31field so violent that it traps charged
- 2:34particles into belts of radiation, and
- 2:36those belts extend far beyond anything
- 2:38you would sensibly call the surface.
- 2:40Your course is planned to keep you out
- 2:42of the worst of it. Plans and radiation
- 2:44have a complicated relationship.
- 2:47For a stretch of days, you live in the
- 2:48most shielded part of your ship, which
- 2:50is a space roughly the size of a
- 2:52wardrobe, surrounded by your own water
- 2:54supply. Because water is heavy, and
- 2:56heavy things stop particles. You sleep
- 2:59badly. You eat in there.
- 3:01You watch the dosimeter numbers climb in
- 3:03a way that is not immediately dangerous,
- 3:05but is absolutely being written down for
- 3:07later.
- 3:08Then you are past it, and the numbers
- 3:09settle, and you come out, and the sun
- 3:11looks wrong.
- 3:12It is still the brightest thing in the
- 3:14sky.
- 3:15It is no longer a disk that hurts to
- 3:16look at. It has become small, hard, a
- 3:19brilliant point rather than a face.
- 3:22Out here, sunlight is roughly a 25th of
- 3:25what it is at Earth. Your solar panels,
- 3:27which were the obvious and elegant
- 3:28solution for the first stretch of the
- 3:30journey, are now decorative.
- 3:32You switch fully to the nuclear source
- 3:34that has been sitting quietly in the
- 3:35back of the ship, and from this point
- 3:37on, every watt of power and every degree
- 3:39of warmth you have comes from a lump of
- 3:41decaying material and a very old idea.
- 3:45Cold is the background condition now.
- 3:47Not the cold of space, which is a
- 3:49misleading phrase, but the simple fact
- 3:51that nothing is warming you except your
- 3:52own machine, heat becomes something you
- 3:55budget. You notice which parts of the
- 3:56cabin your hands avoid. Your body has
- 3:59been keeping its own notes. Months
- 4:01without weight do measurable things.
- 4:04Fluid shifts upward, so your face looks
- 4:06puffy in a way you have stopped
- 4:07noticing, and your legs look like
- 4:09someone let the air out of them. Muscles
- 4:11that are not asked to fight gravity stop
- 4:13pretending they need to be strong. Bone
- 4:15density can fall, and it does not fall
- 4:18evenly, and it does not always come back
- 4:20the way you want it to.
- 4:21Your eyesight can change, and for some
- 4:23people that change does not fully
- 4:25reverse.
- 4:26You exercise because the schedule says
- 4:28so. 2 hours a day strapped to a machine
- 4:31going nowhere at high effort, which is
- 4:33the most accurate description of your
- 4:35entire life at the moment.
- 4:37And underneath all of that, the
- 4:38radiation continues. Not the dramatic
- 4:41Jupiter kind, the steady kind. Out here
- 4:44you are outside the magnetic shield that
- 4:46Earth quietly held over you for your
- 4:47entire existence, and high-energy
- 4:50particles from the rest of the galaxy
- 4:51pass through the hull and through the
- 4:53water and through you constantly. One
- 4:56particle is nothing. The dose is a
- 4:59number that only becomes meaningful
- 5:00across years, and that is exactly the
- 5:02problem, because years is what you have.
- 5:05If you're enjoying this video, please
- 5:07hit the subscribe button. It genuinely
- 5:09helps keep the channel alive.
- 5:11Saturn comes and goes. Then Uranus. Then
- 5:14Neptune, and with Neptune something
- 5:16changes that you were not prepared for.
- 5:18The sun stops being the sun. At
- 5:21Neptune's distance, it is a thousand
- 5:22times fainter than it is at home.
- 5:25It is still the brightest star in your
- 5:26sky by an enormous margin, but that is
- 5:28the word your brain reaches for now, a
- 5:30star.
- 5:32Noon does not exist here. There is no
- 5:34day. There is a permanent, gorgeous,
- 5:36freezing twilight, and you are living in
- 5:38it. You start leaving a light on.
- 5:41Past Neptune, you enter the Kuiper Belt,
- 5:43and it does to you exactly what the
- 5:44asteroid belt did, only slower and
- 5:47colder.
- 5:48Billions of icy bodies, Pluto among
- 5:50them, and you sail through the entire
- 5:52region without seeing one of them with
- 5:54your own eyes. The instruments log
- 5:56things, you do not.
- 5:58This is where the trip stops having
- 6:00landmarks.
- 6:01Everything up to now had a name, a
- 6:03planet, a belt, a moment. From here, the
- 6:06only thing that changes is the number on
- 6:08the distance display, and that number
- 6:09becomes so large that it stops meaning
- 6:11anything emotionally. You look at it, it
- 6:14has gone up, you feel nothing. Your
- 6:16messages home now take hours in each
- 6:18direction. You ask a question at
- 6:20breakfast and the answer arrives after
- 6:21dinner, and by then the question has
- 6:23stopped mattering. People stop sending
- 6:25you news because news is stale before it
- 6:27lands. They send you recordings of
- 6:29ordinary things instead, a kitchen, a
- 6:32dog, weather. You watch them more than
- 6:35you should. And then, quietly, far
- 6:37beyond anything with a name, you hit the
- 6:39first real boundary. The sun does not
- 6:42just make light.
- 6:43It blows a wind, a thin stream of
- 6:45charged particles racing outward in
- 6:47every direction, and that wind carves a
- 6:49bubble in the galaxy. For your entire
- 6:51journey, you have been inside that
- 6:53bubble, and now you are near the place
- 6:55where the wind finally slows down and
- 6:56piles up against everything outside.
- 6:59This is called the termination shock,
- 7:01and it is one of the strangest
- 7:02experiences available to a human being
- 7:05because crossing it feels like
- 7:06absolutely nothing. There is no wall, no
- 7:09shutter, no view.
- 7:10The only way you know it happened is
- 7:12that your instruments tell you the
- 7:13particles around you have changed their
- 7:15behavior. The solar wind has stopped
- 7:17rushing and started crowding. You sit
- 7:19there, perfectly still, having crossed
- 7:22one of the great frontiers of the solar
- 7:23system, holding a cup.
- 7:25Beyond it, the region is messier. The
- 7:28magnetic field out here is tangled and
- 7:30unsettled, and the protection the sun
- 7:32was still weakly offering you begins to
- 7:34thin out. The galactic radiation
- 7:36creeping into your ship ticks upward
- 7:38again.
- 7:39And then comes the one that counts.
- 7:41The heliopause, the place where the
- 7:43sun's influence finally loses to the
- 7:45rest of the galaxy. Inside it, the
- 7:47particles around you mostly came from
- 7:49your own star. Outside it, they mostly
- 7:51did not. You cross it, nothing happens.
- 7:55There is no edge.
- 7:56That is the thing nobody tells you. You
- 7:58have traveled for years to reach a
- 8:00boundary that turns out to be a slow
- 8:01gradient in a plasma you cannot see.
- 8:04Detectable only because a machine says
- 8:05so. You expected a threshold. You got a
- 8:08change in a graph. Behind you, the sun
- 8:11is a single bright star among many. If
- 8:13you did not know which one it was, you
- 8:15could lose it.
- 8:16And here is the part that actually
- 8:17breaks you.
- 8:18You have not reached the edge of the
- 8:20solar system.
- 8:21Because the sun's light gave up long
- 8:23ago, but the sun's gravity did not.
- 8:26Somewhere far out beyond you, wrapped
- 8:27around everything, is the Oort Cloud, a
- 8:30vast shell of icy bodies still loosely
- 8:32held by your star. That is the true
- 8:34gravitational edge. To reach the
- 8:35beginning of it at your speed would take
- 8:37you something in the order of centuries.
- 8:39To pass through the whole thing and be
- 8:41genuinely free of the sun would take
- 8:43tens of thousands of years.
- 8:45You are traveling faster than any human
- 8:47has ever traveled, and you will die of
- 8:49old age having crossed only a rounding
- 8:51error of the distance.
- 8:53So, you do the only thing left to do.
- 8:55You keep going. Your supplies are
- 8:57finite, and your course is fixed.
- 9:00Because turning around out here is not a
- 9:02decision, it is a fuel budget you do not
- 9:04have. The ship keeps its own quiet
- 9:06routine. The power source keeps
- 9:08decaying, a little weaker every year.
- 9:10And one day, the heaters will be running
- 9:12on less than you would like, and you
- 9:13will start closing off sections of the
- 9:15ship to keep one room warm. You will
- 9:17keep sending messages. The delay will
- 9:19grow into days.
- 9:21And eventually, you will send one, and
- 9:22nobody will answer, and you will never
- 9:24find out whether that is because
- 9:26something happened to them, or because
- 9:27something happened to your antenna.
- 9:29That is what actually happens if you
- 9:31reach the edge of the solar system. You
- 9:33do not arrive anywhere. You do not break
- 9:35through anything. You get the most
- 9:37extraordinary view in human history. You
- 9:39cross an invisible line that behaves
- 9:41like weather, and you discover that the
- 9:42solar system does not end. It just gets
- 9:45quieter, and colder, and emptier, and it
- 9:48keeps holding on to you long after it
- 9:49has stopped giving you any light.
- 9:52You wanted to find out where the sun
- 9:53lets go. It does not.
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