The Planets: Jupiter

Transcript

The Planets: Jupiter

PBS Airdate: July 31, 2019

NARRATOR: Half a billion miles from the sun, the giant of the planets…

HEIDI BECKER (Mission Scientist, Juno): It’s very violent and it’s very intimidating.

NARRATOR: …Jupiter. Of all the worlds in the solar system…

FRAN BAGENAL (University of Colorado): It’s the biggest planet. It, sort of, pushed a lot of the planets around. It is the bully of the solar system.

NARRATOR: …Jupiter’s immense size gives it incredible influence.

KONSTANTIN BATYGIN (California Institute of Technology): Jupiter is the most powerful gravitational object, second to the sun.

NARRATOR: And while Jupiter is at a safe distance from Earth today, in the past it drew much closer. Four-and-a-half-billion years ago, it embarked on a rampage across the solar system, leaving a trail of destruction in its wake.

LYNNAE QUICK (National Air and Space Museum): We can think of the asteroid belt as a planetary graveyard.

NARRATOR: Jupiter transformed the destiny of the planets and could even have changed the course of life on Earth.

KONSTANTIN BATYGIN: It is the most influential planet of our cosmic home.

NARRATOR: The Planets: Jupiter, right now, on NOVA.

NARRATOR: Beyond the edge of the inner solar system and the desolate wasteland of the asteroid belt, is the gas giant, Jupiter.

JUPITER

480 MILLION MILES FROM THE SUN

NARRATOR: Its serene marbled appearance disguises a planet in turmoil, where violent storms rage through clouds more than a thousand miles deep.

DERRICK H. PITTS (The Franklin Institute): When we look at Jupiter, we find one of the most amazing places we’ve seen in the solar system.

HEIDI BECKER: It’s very mysterious. It’s covered by clouds that hide what’s underneath.

NARRATOR: But Jupiter is a planet as influential as it is beautiful.

KONSTANTIN BATYGIN: Jupiter is by far the biggest planet. Its mass is greater than 300-times that of the earth, so it is the most powerful gravitational object, second to the sun.

NARRATOR: Four-and-a-half-billion years ago, Jupiter’s gravity had devastating consequences for the worlds around it.

DERRICK PITTS: Jupiter had this incredible effect that helped to shape the solar system overall.

NARRATOR: Clearing material from the inner solar system, Jupiter transformed the destiny of the planets, including our own.

KONSTANTIN BATYGIN: You’re looking at the crime scene—the structure of the solar system, what it is today—and trying to piece together what happened four-billion years ago. It is an amazingly intriguing problem.

NARRATOR: Jupiter is a world with a dark past. And you don’t have to look far to see the evidence.

In the Northern Arizona desert, this is Barringer Crater. It was formed 50,000 years ago when an iron nickel asteroid, 150 feet across, hit the earth, at 27,000 miles per hour, an asteroid that was, likely, thrown in our direction by Jupiter.

So what is it that enables Jupiter to influence the Earth from so far away? And how did it grow to such dominance? Only by seeing Jupiter close up, could we begin to answer those questions.

PIONEER 10

1972

NARRATOR: In 1972, Pioneer 10 becomes the first spacecraft to cross the asteroid belt.

DERRICK PITTS: Before Pioneer, we really had no idea whether or not a spacecraft would be able to survive all the hazards of a trip like that.

TAKES FIRST CLOSE UP IMAGES OF JUPITER

DERRICK PITTS: The images brought back to us really blew our minds, in terms of what we could see of Jupiter. To have the incredible detail about the dynamics of the atmosphere really was new and different to us.

ARCHIVE NEWS CLIP: Now the world wants to know; “what have we learned?”

NARRATOR: During its brief flyby, Pioneer observes Jupiter for four days, proving that missions to the outer solar system are possible.

VOYAGER MISSION CONTROL: We have ignition, and we have liftoff of the Titan Centaur, carrying the first of two Voyager spacecraft to extend man’s senses farther into the solar system than ever before.

VOYAGER 1 & 2 1977

FIRST JUPITER APPROACH JANUARY 1979

NARRATOR: The Voyager spacecraft see Jupiter’s Earth-sized red spot in unprecedented detail, discover the planet’s rings and capture the first detailed images of Jupiter’s moons.

FRAN BAGENAL: It wasn’t until Voyager went up close and personal and took amazing pictures of the moons, that we really began to get a sense of just how complex and the variety of the worlds around Jupiter.

EUROPA

FRAN BAGENAL: The icy surfaces of Europa, so different, so dynamic…

IO

…the volcanoes on Io…

GANYMEDE

FRAN BAGENAL: …Ganymede all broken up; and then…

CALLISTO

FRAN BAGENAL: …Callisto was just this big icy surface covered in impact craters.

NARRATOR: We now know the giant planet has more than 79 moons. Jupiter is a world so large its immense gravity has assembled a solar system in miniature. So, how did it grow to such incredible size?

JUNO MISSION CONTROL: T-ten, nine, eight, seven, six…

NARRATOR: In 2011, the Juno spacecraft launches from Cape Canaveral…

JUNO MISSION CONTROL: …one, ignition and liftoff of the Atlas V with Juno, on a trek to Jupiter.

NARRATOR: …its mission: to uncover the secrets of Jupiter’s formation.

JUNO

2011

FRAN BAGENAL: When we launched the Juno spacecraft away from the Earth, out towards Jupiter, we didn’t have enough speed to get away out of the gravity of the sun. So, we actually had to come back to Earth, get a gravity assist from Earth, and then go out to Jupiter.

NARRATOR: After travelling for five years, on July 4th, 2016, the spacecraft finally arrives. It’s an incredible moment for the science team.

FRAN BAGENAL: You see all these swirls, you see all sorts of spots coming up, you see all these vortices, you see dramatic storm systems interacting. It’s mind-blowingly beautiful pictures that this little camera has been taking.

HEIDI BECKER: “JunoCam” was able to see the “Great Red Spot” from up close. We can see height to the clouds, we can see features that look like storms. Maybe it’s hailing or snowing ammonia on Jupiter. And the most startling thing that we saw from JunoCam’s imagery was that the poles of Jupiter are actually blue.

Juno’s objective is to look as close at Jupiter and as deep inside as we possibly can, to understand as best as we can: what is it made of? What is its interior structure like? Because the answers to those questions help to tell us where and how Jupiter might have formed.

By analyzing the planet’s magnetic and gravitational fields, Juno is able to look deep into Jupiter’s interior.

FRAN BAGENAL: And what we found is that there is a lot of mass inside. That mass is the core of the planet, around which the hydrogen was pulled in in those early stages of solar system formation.

NARRATOR: By discovering the planet’s core, Juno is helping us to reconstruct Jupiter’s first moments, a story that begins very early in the solar system’s history.

5 BILLION YEARS AGO

NARRATOR: Nearly five-billion years ago, a distant exploding star sends a shockwave across the galaxy, causing the cloud of gas and dust that would become our solar system to collapse, forming the sun. Farther out, Jupiter’s core is already beginning to grow, gathering in vast clouds of gas. After 50-million years, the sun’s nuclear furnace ignites, the light of its first dawn revealing Jupiter.

While the terrestrial worlds are little more than rubble, Jupiter is fully formed, allowing it to shape everything that follows.

KONSTANTIN BATYGIN: So, when it comes to setting the stage, setting the structure of how the solar system is going to evolve, Jupiter plays the biggest role. It is the most influential planet of our cosmic home.

NARRATOR: Over the next hundred-million years, the four rocky planets of the inner solar system form, in their familiar positions: Mercury, Venus, Earth, then Mars. And while this layout is familiar to us, it might be extremely rare.

KONSTANTIN BATYGIN: The more we’ve looked around, the more we’ve found that the typical solar system is unlike that of our own.

NARRATOR: Our sun is just one of three-hundred-billion stars in our galaxy, and almost every one of those stars is likely home to its own system of planets.

LEIGH FLETCHER (University of Leicester): When we look out into the rest of our galaxy, we’re starting to discover worlds around other stars. We call them “exoplanets.” The planets that we’re seeing, they’re not all Earth-like objects, they’re not all big objects, like Jupiter. The vast majority of them have sizes and masses that are similar to Uranus and Neptune.

NARRATOR: In most other systems, the region of space where our planet orbits is empty. Instead, close to the star we see “super Earths”…

PLANET: 40 ERIDANI A B

CONSTELLATION: ERIDANUS

MASS: 8.5 X EARTH

NARRATOR: …vast rocky planets between two- and 10-times more massive than Earth.

PLANET: JANSSEN

CONSTELLATION: CANCER

ATMOSPHERE: HYDROGEN & HELIUM

NARRATOR: But these worlds are thought to have thick, suffocating atmospheres that render them completely inhospitable to life as we know it, so what is it that makes our system so different?

KONSTANTIN BATYGIN: Some sequence of events must have happened that made our solar system special.

NARRATOR: As we’ve explored the planets, we discovered strange anomalies that hint at a catastrophic upheaval that shaped the solar system. Our missions to Venus found that it once had far more water than you’d expect for a planet so close to the sun, just as Earth has today.

The spacecraft we’ve sent to Mars, touched down on a world that is, curiously, just half the size of her sister planets Earth and Venus. But it was in the region of space closest to Jupiter that our probes discovered the most astonishing evidence.

KONSTANTIN BATYGIN: The asteroid belt actually holds a remarkable amount of information about the solar system’s dynamic and dramatic evolution.

THE ASTEROID BELT

PRESENT DAY

LYNNAE QUICK: The asteroid belt sits in between Mars and Jupiter, and it separates the inner solar system from the outer solar system. People think that the asteroid belt is very densely packed, but the asteroids there are actually very widely separated. They’re spread over this huge volume.

KONSTANTIN BATYGIN: So, if you stand on top of one asteroid, you won’t be able to see another one. It’s nothing like what you would imagine in science fiction.

BETHANY EHLMANN (California Institute of Technology): When we send spacecraft outward into the solar system, through the asteroid belt, we double check that there’s not going to be a large asteroid in the way, but we really don’t need to make any kind of course correction, because the asteroid belt is largely empty space.

NARRATOR: But it hasn’t always been like this. It’s thought the asteroid belt once contained enough material to build a planet the size of the Mars, so why is it so empty today?

DAWN 2007

DELTA II MISSION CONTROL: …five, four, three, two, main engine start, one, zero and liftoff of the Delta II rocket with Dawn, using ion propulsion to reach the catalysts of our solar system.

BETHANY EHLMANN: Dawn’s mission is to investigate the two largest asteroids in the asteroid belt, Vesta and Ceres.

NARRATOR: After a year in orbit around Vesta, In March, 2015, Dawn makes its final approach on Ceres, a body that makes up over a third of the mass of the entire belt.

BETHANY EHLMANN: It was really exciting, because an object that had been sort of grainy and mysterious, was suddenly there, revealed before us, ready for exploration.

NARRATOR: On approach, the first images Dawn sends back to Earth reveal something unexpected.

DAWN IMAGING

BETHANY EHLMANN: As Ceres came into view, we would see these amazing bright spots on the surface, pockmarking it here and there, nothing like we’d ever seen before. And the most outstanding ones were found in Occator Crater. Occator Crater is one of the larger but younger craters on Ceres. The most intriguing thing though, is what we see in the center, which is a central pit and then a bright dome of, of this intriguing, super bright material.

NARRATOR: Now the mission team’s challenge is to identify what the mysterious substance actually is.

BETHANY EHLMANN: With the instruments on the Dawn mission, we’re looking at the chemical fingerprints of the bright materials. And, actually, we see that they’re salts. All this points to the fact that there were once brines, salty waters that rose near the surface of Ceres to create these deposits.

NARRATOR: Dawn goes on to discover over 300 bright spots, clues to Ceres’ former life.

BETHANY EHLMANN: If we were to peel away the dark surface of Ceres, what we’d find underneath is a mixture of rock and ice. Ceres is not just the largest asteroid; it’s a dwarf planet in its, in its own right. It’s spherical, and it has differentiated into layers. We know from Dawn data that there is an ice-rich layer on the outer, comprising the outer crust, tens of kilometers thick.

NARRATOR: But it hasn’t always been this way.

BETHANY EHLMANN: Ceres is frozen today, but early in its history, radioactive elements in its interior would have provided heat that melted the liquid water that’s currently ice. And so, we think that during the early portions of Ceres’ history, it had a global ocean.

CERES

4.5 BILLION YEARS AGO

NARRATOR: In infancy, Ceres was well on its way to becoming a fully-fledged world. The water that now lies frozen within its interior was once liquid. Protected beneath a thin layer of ice, ancient Ceres is covered by a deep saltwater ocean. But then something happens to cut its development short.

As the young Jupiter circles the sun, it clears a path through the gas cloud that envelops the early solar system. But that process causes it to do something alarming. Jupiter begins to spiral inwards, plowing straight through the region of space that would become the asteroid belt.

KONSTANTIN BATYGIN: When the young Jupiter moves through the primordial asteroid belt, things get scattered around, things get gravitationally deflected. And, as a consequence of all of this gravitational interaction, more than 99 percent of the original mass that was there is basically now gone.

BETHANY EHLMANN: The asteroid belt has been disrupted, over time, by the movement of the giant planets. And this has acted to throw material from the asteroid belt out of the asteroid belt, into the outer solar system.

KONSTANTIN BATYGIN: These proto-planetary cores, like Ceres, were never able to graduate to full-fledged planets, because there was just not enough material in the orbital neighborhood.

NARRATOR: When Jupiter passed through the primordial asteroid belt, it starved Ceres of material, halting its growth, and the dwarf planet was condemned to spend eternity as a cold, barren rock.

But Ceres isn’t the only world in our solar system whose development was cut short; Mars would share a similar fate.

THE INNER SOLAR SYSTEM

4.5 BILLION YEARS AGO

NARRATOR: After marauding through what would become the asteroid belt, Jupiter enters the region of space where Mars is forming, continuing its journey, spiraling towards the sun. As Jupiter bulldozes inwards, its immense gravity scatters material in all directions. Some is sent careening into the sun, and some is thrown out into interstellar space.

KONSTANTIN BATYGIN: It is because of the gravitational clearing of this neighborhood by Jupiter that Mars was unable to grow to more than 10 percent of that of the Earth. This is why Mars is small.

NARRATOR: And by clearing material out of the inner solar system, the giant planet may also have prevented the formation of the super-Earths we see in other systems. And if it had continued moving inwards, our planet, too, might never have formed.

But then, just as it looks like Jupiter will sweep everything away, the giant planet stops in its tracks, because in the far reaches of the outer solar system another planet is forming: the solar system’s second gas giant, Saturn. And its arrival changes everything.

KONSTANTIN BATYGIN: As Jupiter moved inwards, Saturn moved inwards and caught up to Jupiter’s orbit. When this happened, the two locked into a special configuration known as a “mean motion resonance.” This is where the planets begin to interact gravitationally in a very coherent manner. And now, locked as a unit, the two reversed their migration course and moved back out.

THE SOLAR SYSTEM PRESENT DAY

NARRATOR: Saturn caused Jupiter to retreat, leaving behind just enough material from which the inner planets could form: Mercury, Venus and our home.

DERRICK PITTS: Earth is in exactly the right location to provide the environment for life to develop, so if Jupiter had moved around even more, who knows? Maybe life never would have developed in this solar system, as we know it.

NARRATOR: And as its voyage across the solar system draws to a close, Jupiter helps to provide our living world with its most precious ingredient. Today, two thirds of our planet’s surface is covered by ocean, more than 320-million cubic miles of water, each drop teeming with life.

DERRICK PITTS: One of the big questions about the evolution of our solar system is how did we get water here, on this planet?

EDGARD RIVERA-VALENTÍN (Lunar and Planetary Institute): So, we think that the inner planets didn’t naturally form with a lot of water. Water is primarily in the outer solar system. But if you end up having Jupiter and Saturn moving outwards, then that is able to suddenly deliver more water into the inner solar system.

NARRATOR: Locked in a gravitational dance with Saturn, Jupiter moves back through the asteroid belt. And, as it does so, water-rich material is flung inward, where it is incorporated into the growing terrestrial worlds.

BETHANY EHLMANN: So, the movement of the giant planets have actually played an important role in the delivery of water to the inner solar system.

KONSTANTIN BATYGIN: In a sense, it is Jupiter’s outwards motion through the asteroid belt that we have to thank for the delivery of water to surface of the earth. The earth would be quite a different planet, if not for Jupiter’s primordial dance.

NARRATOR: Today, Jupiter has settled into a regular orbit, back beyond the far edge of the asteroid belt, its days of marauding through the solar system at an end. But its gravity remains a constant threat, and nowhere is that more apparent than on the closest of Jupiter’s large moons.

IO

PRESENT DAY

NARRATOR: Io is the most volcanic world in the solar system.

LYNNAE QUICK: If you were to send a spacecraft to Io and take a picture, you would see hundreds of volcanoes erupting at one time.

FRAN BAGENAL: Active volcanoes, lava spewing out; hot, hot, hot lava.

NARRATOR: The biggest lava lake on Io is Loki Patera. At more than 120 miles in diameter, it’s a million times the area of any lava lake on Earth, its surface constantly churned by waves of molten rock. But Io is the same size as our moon, so why isn’t it just as cold and dead?

STEVE DESCH (Arizona State University): Jupiter is a massive planet. It’s 318-times the mass of the earth. And this poor little moon has to orbit near this giant, and meanwhile the other moons are in an orbital resonance with it, and they keep tugging it out of a circular orbit.

ED RIVERA: When things are in resonances, that means they’re meeting each other up at the same point in space constantly, so that means that there’s a constant tug coming in from all of these moons.

CASSINI IMAGES

LYNNAE QUICK: This tugging creates friction. And this friction becomes heat, very much in the same way as if you were to rub your hands together on a cold day, that friction would create heat. And this is what we call “tidal heating.”

CASSINI IMAGES

STEVE DESCH: When you take a moon like Io, and you stretch it this way and then let it relax and stretch it this way and let it relax, the friction inside is constantly heating up the rock, until you reach the melting point.

NARRATOR: This process raises the temperature in Io’s interior to more than 2,000 degrees Fahrenheit, creating its lava lakes and powering immense volcanic plumes that rise up to 200 miles from the moon’s surface and out into space.

Because of Jupiter’s great size, the gravitational field that drives Io’s volcanism, extends far beyond its moons, even as far as Earth, where there’s evidence it’s done far more than create the occasional crater.

BRUCE SCHUMACHER (U.S. Forest Service Paleontologist): Preserved in the limestone layers along this stretch of river are several thousand dinosaur tracks, dating back to the Jurassic period, some 150-million years ago.

NARRATOR: Etched into the banks of the Purgatoire River are the final traces of a lost world.

BRUCE SCHUMACHER: Some of these tracks are from a large herbivorous dinosaur, a sauropod, big hind footfalls moving through the area, and right near those are three-toed prints of a meat-eating animal, something like Allosaurus. And all of those tracks being together tell a story, and the easiest story that one might imagine is that of a predator pursuing prey on this ancient lakeshore.

NARRATOR: But today, the dinosaurs are gone. The course of evolution was dramatically changed, and it’s likely Jupiter was responsible.

KONSTANTIN BATYGIN: Jupiter has been profoundly implicated in periodic extinctions of life on Earth. And, indeed, it’s quite likely that the asteroid which wiped out the dinosaurs, almost 70-million years ago was launched from the asteroid belt by Jupiter’s gravitational influence.

People often think of the asteroid belt as this unstructured, unchanging population of debris, but as you can see here, there’s quite a bit of structure to the asteroid belt. In green, what we have are the so-called Trojan asteroids, objects that occupy the same orbit as Jupiter. In red, what we have are the Hilda asteroids. They form this triangular shape, because of the resonance that they’re in with Jupiter.

The asteroid belt as a whole is, kind of, dancing to Jupiter’s tune.

NARRATOR: But it’s a delicate balance that can change at any time.

KONSTANTIN BATYGIN: Because Jupiter exerts such tight control over the long-term changes of the asteroid orbits, if an asteroid comes off its well-defined, orbital track, so to speak, then Jupiter will just fling it out of the asteroid belt and, potentially, even send it towards the earth.

NARRATOR: Dislodged from its orbit by Jupiter’s gravity, an asteroid six miles across tumbles out of the asteroid belt. It is now on a collision course with Earth. When it strikes, the impact generates a fireball so hot, anything within a 600-mile radius dies instantly. The impact throws some 300-billion tons of sulfur up into the atmosphere. And during the “nuclear winter” that follows, 75 percent of species, plant and animal, are wiped from the face of the earth, including the largest creatures ever to walk on its surface.

By driving the dinosaurs to extinction, Jupiter cleared the way for us to inherit the planet. And, although it still occasionally flings asteroids our way, Jupiter also protects us.

For objects heading towards Earth from the far reaches of the solar system, the giant planet’s immense gravity acts as a shield. Around 100 years ago, a lump of rock and ice two-and-a-half miles across is hurtling toward the inner solar system, but Jupiter stands in its way.

ATLANTIS MISSION CONTROL: Five, four, three, two, one, we have ignition and liftoff of Atlantis and the Galileo spacecraft, bound for Jupiter.

NARRATOR: Seventy years later, a mission launches that will witness just how effective a shield Jupiter can be.

ATLANTIS 1989

NARRATOR: On board the space shuttle Atlantis, the Galileo Orbiter.

COMET SHOEMAKER-LEVY 9

NARRATOR: Three years after Galileo launches, comet Shoemaker-Levy 9 has been captured by Jupiter’s gravity. And now, locked in the giant planet’s deadly embrace, tidal forces begin to tear the comet apart, its journey into the inner solar system cut short. What happens next presents the Galileo scientists with a unique opportunity.

ANDREW INGERSOLL (Mission Scientist, Galileo): So, everyone was observing it and they realized two things. One is that it had just passed very close to Jupiter and probably had gotten pulled apart by Jupiter’s tides, and the other was that it was going to crash into Jupiter two years later.

FRAN BAGENAL: The discovery that a comet was about to hit Jupiter was a huge surprise and very exciting.

JULY 1994

150 MILLION MILES FROM JUPITER

NARRATOR: After crossing the inner solar system, Galileo is approaching the spot where it will witness the comet’s final moments.

ANDY INGERSOLL: We knew Galileo would be able to see the flashes directly. We knew that the impacts were going to occur on the night side and that Galileo was going to be able to see them.

GALILEO IMAGES

NARRATOR: On July 16th, Galileo sees the first fragments of the comet enter Jupiter’s southern hemisphere.

ANDY INGERSOLL: At 60 kilometers per second, the fragments really heated the atmosphere red hot, almost to the temperatures of the sun.

FRAN BAGENAL: And the pieces hit the planet one after the other.

NARRATOR: Pieces of comet Shoemaker-Levy 9 strike Jupiter over the course of six days.

ANDY INGERSOLL: They looked like big flashes on Jupiter. The pictures of the impact were fantastic.

GALILEO IMAGES

NARRATOR: These powerful pulses of light, captured from 150-million miles away are the only time we have ever witnessed a comet strike. The most destructive impact releases energy equivalent to 6,000,000 megatons of T.N.T., leaving behind a giant dark cloud 7,500 miles across.

By capturing objects and incinerating them on impact, Jupiter protects us from bodies that might otherwise threaten Earth.

Galileo would go on to study Jupiter for another eight years.

ARCHIVE NEWS CLIP: The spacecraft will orbit Jupiter at least 11 times, making a close flyby of one of the Galilean satellites on each orbit. As the probe samples the Jovian atmosphere, scientific results will be relayed to the orbiter.

NARRATOR: Galileo records 400-mile-per-hour winds in Jupiter’s clouds and measures lightning strikes many times more powerful than those on Earth.

ARCHIVE NEWS CLIP: The spacecraft will sweep within 200 kilometers of the surface of Europa, yielding high resolution images. Galileo’s Europa encounters will give us our first detailed look at this moon’s mysteriously fractured surface.

NARRATOR: Galileo’s images confirm Europa is an ice moon. Analysis of its magnetic field reveals Europa’s cracked surface floats above an ocean 60 miles deep, which contains more water than all the oceans on Earth.

Then, on September 21, 2003, Galileo meets the same fate as the comet that had greeted its arrival.

ANDY INGERSOLL: At the end of the mission the spacecraft was low on fuel and it had suffered a lot of radiation damage, and we had to dispose of it.

FRAN BAGENAL: And the best way to do that is to send it into the planet so it burns up. You don’t want the spacecraft to hit one of the moons, especially a moon like Europa that may have life, because the spacecraft may be carrying life from Earth.

ANDY INGERSOLL: When you have to say goodbye, it’s a sad moment, but on the other hand, if you look back and say, “What a successful life the spacecraft had!” And I think that’s the way we all felt.

NARRATOR: Jupiter, the oldest and largest of the planets is the giant of our solar system. In youth, it went on a rampage. For some young planets, that spelled disaster. But for others, like our own world, it cleared the way for their formation. And so Earth and all of humanity owe Jupiter a great debt.

But the fate of the dinosaurs is a reminder that it’s a debt that could be recalled at any time.

STEVE DESCH: Solar system evolution is never really done, and the orbits of the planets are just not going to stay stable.

KONSTANTIN BATYGIN: Over million-year time scales, the orbits of the planets are quite predictable; over much longer time scales, however, they act in a fundamentally chaotic manner.

NARRATOR: Which means the story of Jupiter may have one final twist.

KONSTANTIN BATYGIN: Among our calculations of long-term evolution of the solar system, we find that about one percent of the time, Mercury’s orbit can become exceedingly elliptical as a result of gravitational interactions with Jupiter.

NARRATOR: This would have dire consequences for the inner solar system. Mercury could be thrown into the sun, flung out into interstellar space, or even set on a collision course with the earth.

KONSTANTIN BATYGIN: In every one of these situations, however, the orbits of the other planets, Earth included, get messed up. So, the solar system, the inner solar system, becomes an unlivable place, if this occurs.

NARRATOR: And so Jupiter, the giant that shaped the birth of our world might one day bring about its demise.

Credits

PRODUCED AND DIRECTED BY

Stephen Cooter

SERIES PRODUCERS

Zoe Heron

Gideon Bradshaw

EXECUTIVE PRODUCER FOR BBC STUDIOS

Andrew Cohen

NARRATED BY

Zachary Quinto

ASSISTANT PRODUCER & ADDITIONAL DIRECTING

Katy Savage

DIRECTOR OF PHOTOGRAPHY

Julius Brighton

EDITED BY

Paul Crosby

Graeme Dawson

ANIMATION

Lola Post Production

MUSIC

Anže Rozman for Bleeding Fingers Music

SCORE PRODUCER

Russell Emanuel

SCORE SUPERVISOR

Christopher J. King

MUSIC EDITOR

Jake Schaefer

TITLE MUSIC

Muse

VFX SUPERVISOR

Rob Harvey

VFX PRODUCER

Rebecca Kelly

CG SUPERVISOR

Rasik Gorecha

2D SUPERVISOR

Joe Cork

DEVELOPMENT

Nicola Cook

Nik Sopwith

Josh Green

PRODUCTION MANAGER

Evih Efue

POST PRODUCTION COORDINATOR

Kate Moore

PRODUCTION COORDINATOR

Toby Keeley

JUNIOR PRODUCTION MANAGER

Emma Chapman

SOUND

Andy Paddon

AERIAL PHOTOGRAPHY

Olly Meacock

Tim Browning

STORYBOARD ARTIST

John Kennedy

EDIT ASSISTANT

Miguel Arnott Muzaly

ONLINE EDITOR

Scott Hinchcliffe

COLORIST

Paul Koren

AUDIO MIX

Richard Addis

SOUND DESIGNER

Jay Price

Junior Researcher

Sarah Houlton

ARCHIVE PRODUCER

Maggie Oakley

ARCHIVE

BBC Motion Gallery

Caltech

NASA

NASA / Ames Research Center / Ted Stryk

NASA/JPL/Cornell University

NASA/JPL/DLR

NASA/JPL/Space Science Institute

NASA/JPL/University of Arizona

NASA / JPL-Caltech

NASA/JPL-Caltech/Kevin M. Gill

NASA/JPL-Caltech/SETI Institute

NASA/JPL-Caltech/SSI/CICLOPS/Kevin M. Gill

NASA / JPL-Caltech / SSI / SwRI / MSSS / ASI / INAF / JIRAM / Björn Jónsson

NASA/JPL-Caltech/SwRI/MSSS/Kevin M. Gill

NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI

NASA / Kennedy Space Center

NASA Ames Research Center

NASA Johnson Space Center

NASA / NSSDC

Petr Scheirich

Pond5

ACADEMIC CONSULTANTS FOR THE OPEN UNIVERSITY

Stephen R Lewis

David A Rothery

SCIENTIFIC ADVISOR

Emily Lackdawalla

----

For BBC Studios

PRODUCTION EXECUTIVE

Laura Davey

BBC COMMISSIONING EDITOR

Tom McDonald

-----

NOVA SERIES GRAPHICS

yU + co.

NOVA THEME MUSIC

Walter Werzowa

John Luker

Musikvergnuegen, Inc.

ADDITIONAL NOVA THEME MUSIC

Ray Loring

Rob Morsberger

CLOSED CAPTIONING

The Caption Center

POST PRODUCTION ONLINE EDITOR

Lindsey Rundell Denault

DIGITAL EDITORS

Allison Eck

Katherine Wu

DIGITAL ASSOCIATE PRODUCERS

Arlo Perez

Ana Aceves

DIGITAL PRODUCER

Emily Zendt

DIGITAL MANAGING PRODUCER

Kristine Allington

SENIOR DIGITAL PRODUCER

Ari Daniel

PROGRAM MANAGER, NOVA SCIENCE STUDIO

Tenijah Hamilton

OUTREACH COORDINATOR

Gina Varamo

DIRECTOR OF EDUCATION AND OUTREACH

Ralph Bouquet

DIRECTOR OF NATIONAL AUDIENCE RESEARCH

Cory Allen

PUBLICITY

Eileen Campion

Eddie Ward

AUDIENCE ENGAGEMENT EDITOR

Sukee Bennett

DIRECTOR OF AUDIENCE DEVELOPMENT

Dante Graves

DIRECTOR OF PUBLIC RELATIONS

Jennifer Welsh

PRODUCTION ASSISTANT

Angelica Coleman

PRODUCTION COORDINATOR

Linda Callahan

RESEARCHERS

Brian Kantor

Robin Kazmier

TALENT RELATIONS

Janice Flood

PARALEGAL

Sarah Erlandson

RIGHTS MANAGERS

Lauren Miller

Hannah Gotwals

BUSINESS MANAGERS

Ariam McCrary

Elisabeth Frele

LEGAL AND BUSINESS AFFAIRS

Susan Rosen

POST PRODUCTION ASSISTANT

Jay Colamaria

SENIOR PROMOTIONS PRODUCER AND EDITOR

Michael H. Amundson

SUPERVISING PRODUCER

Kevin Young

BROADCAST MANAGER

Nathan Gunner

SENIOR EXECUTIVE PRODUCER, EMERITA

Paula S. Apsell

SCIENCE EDITOR

Caitlin Saks

DEVELOPMENT PRODUCER

David Condon

PROJECT DIRECTOR

Pamela Rosenstein

COORDINATING PRODUCER

Elizabeth Benjes

SENIOR SCIENCE EDITOR

Evan Hadingham

SENIOR SERIES PRODUCER

Melanie Wallace

DIRECTOR, BUSINESS OPERATIONS & FINANCE

Laurie Cahalane

EXECUTIVE PRODUCERS

Julia Cort Chris Schmidt

A BBC Studios Production with NOVA and WGBH Boston for PBS [logo] and BBC Earth [logo]co-produced by Tencent Penguin Pictures and The Open University.

© 2019 BBC

The Planets Additional Material © 2019 PBS

All rights reserved

Additional Material © 2019 WGBH Educational Foundation

All rights reserved

This program was produced by WGBH, which is solely responsible for its content. Some funders of NOVA also fund basic science research. Experts featured in this film may have received support from funders of this program.

Original funding for this program was provided by Draper, the David H. Koch Fund for Science and the Corporation for Public Broadcasting

Image: (CG illustration of Jupiter)

Created by Lola Post Production/© BBC Studios

Participants

Fran Bagenal, Konstantin Batygin, Heidi Becker, Steve Desch, Bethany Ehlmann, Leigh Fletcher, Andrew Ingersoll, Derrick Pitts, Lynnae Quick, Edgard Rivera-Valentín, Bruce Schumacher

More Ways to Watch