NOVA Wonders Are We Alone?

Transcript

NOVA Wonders: Are We Alone?

PBS Airdate: May 9, 2018

TALITHIA WILLIAMS (Mathematician, Harvey Mudd College): What do you wonder about?

ERICH JARVIS (Rockefeller University): The unknown.

FLIP TANEDO (University of California, Riverside): What our place in the universe is?

TALITHIA WILLIAMS: Artificial intelligence.

ROBOT: Hello.

JARED TAGLIALATELA (Kennesaw State University): Look at this. What's this?

KRISTALA JONES PRATHER (Massachusetts Institute of Technology): Animals.

JARED TAGLIALATELA: An egg.

ANDRE FENTON (Neuroscientist, New York University): Your brain.

RANA EL KALIOUBY (Computer Scientist, Affectiva): Life on a faraway planet.

TALITHIA WILLIAMS: NOVA Wonders, investigating the biggest mysteries,…

JOHN ASHER JOHNSON (Harvard-Smithsonian Center for Astrophysics): We have no idea what's going on there.

JASON KALIRAI (Space Telescope Science Institute): These planets in the middle, we think are in the habitable zone.

TALITHIA WILLIAMS: …and making incredible discoveries.

CATHERINE HOBAITER (University of St Andrews): Trying to understand their behavior, their life, everything that goes on here.

DAVID COX (Harvard University): Building an artificial intelligence is going to be the crowning achievement of humanity.

TALITHIA WILLIAMS: We are three scientists, exploring the frontiers of human knowledge.

ANDRE FENTON: I'm a neuroscientist, and I study the biology of memory.

RANA EL KALIOUBY: I'm a computer scientist, and I build technology that can read human emotions.

TALITHIA WILLIAMS: And I'm a mathematician, using big data to understand our modern world. And we're tackling the biggest questions…

SCIENTISTS: Dark energy? Dark energy!

TALITHIA WILLIAMS: …of life…

DAVID T. PRIDE (University of Califormia, San Diego): There's all of these microbes, and we just don't know what they are.

TALITHIA WILLIAMS: …and the cosmos.

On this episode, the hunt for alien life is on, turning up mysterious clues…

TABETHA BOYAJIAN: This star loves attention, and it makes everybody crazy.

SETH SHOSTAK: That's not a planet. So what is it?

TALITHIA WILLIAMS: What are the odds?

SARA SEAGER (Massachusetts Institute of Technology): The ingredients for life are everywhere.

JASON KALIRAI: The universe has hundreds of billions of planets

TALITHIA WILLIAMS: But does anything live there?

JOHN ASHER JOHNSON: The chances of us finding life are very high.

TALITHIA WILLIAMS: Nova Wonders: Are We Alone? Right now.

The planet Earth, a ball of rock about 8,000 miles in diameter: we know there's a lot going on here.

ANDRE FENTON: Almost eight-billion people call it home, along with billions of other species.

RANA EL KALIOUBY: But is this the only place where the action is?

ANDRE FENTON: Our sun is just one of an estimated 300-billion stars in the Milky Way.

RANA EL KALIOUBY: And we think there are at least 100-billion other galaxies.

TALITHIA WILLIAMS: So, what are the chances that all the fun is only happening right here, in our tiny corner of the universe?

RANA EL KALIOUBY: Today, astronomers and engineers are building new tools to probe our solar system and our galaxy, hunting for clues of life beyond Earth.

TALITHIA WILLIAMS: What are they discovering?

RANA EL KALIOUBY: I'm Rana el Kaliouby.

ANDRE FENTON: I'm Andre Fenton.

TALITHIA WILLIAMS: I'm Talithia Williams.

And in this episode, Nova Wonders: Are We Alone? And what would it take to find out?

A few years ago, a group of amateur astronomers discovered a mysterious star. Located about 1,500 lightyears from Earth, the star flickers erratically, and no one knows why. If a star dims at regular intervals, chances are it's caused by an orbiting planet, and typically, it's only by a fraction of one percent. But the light from this star is dimming by more, much more.

SETH SHOSTAK: The thing about this star is the light dims every now and again, but it's being dimmed by 22 percent. So, that's not a planet. That's much too much, even for a Jupiter-sized planet. You don't get anywhere near that kind of dimming. So what is it?

TALITHIA WILLIAMS: Unlocking the star's secrets becomes the quest of Tabetha Boyajian, a stellar astrophysicist. Soon, people are calling it "Tabby's star."

TABETHA BOYAJIAN: I worked with dozens of other astronomers for several years, trying to figure out what could be causing these strange fluctuations in its light.

TALITHIA WILLIAMS: Is it caused by an asteroid belt? Or colliding planets?

TABETHA BOYAJIAN: So, we had this long list of ideas. None of them worked.

TALITHIA WILLIAMS: Then, one of Tabby's colleagues offers a possible idea, a bit outside the standard astronomy box…

TABETHA BOYAJIAN: When I showed him this star he said "Wow, this is really weird, and we don't have an explanation for it." He said, "These things all look like they could be caused by some artificial alien megastructure."

TALITHIA WILLIAMS: …an artificial alien megastructure, a giant structure built by a hypothetical alien civilization to harness the energy from its own sun.

When the word gets out…

REPORTER 1: Talk about the prospects of an alien megastructure…

REPORTER 2: …evidence of alien life.

REPORTER 3: The strange light pattern makes it seem more like a death star planet rather than a star.

TABETHA BOYAJIAN: This star loves attention, and it makes everybody crazy.

TALITHIA WILLIAMS: It is farfetched. To dim a star by so much, an alien megastructure would have to be at least half as big as the star itself. But, when the theory is first proposed, astronomers can't rule it out.

AVI LOEB (Harvard-Smithsonian Center for Astrophysics): The behavior of Tabby's star is quite weird.

JOHN ASHER JOHNSON: Given that we have no idea what's going there, I'm not too quick to throw out theories.

PAUL DAVIES (Arizona State University): Could this be some alien megastructure? We don't know.

TALITHIA WILLIAMS: Tabby and her team will continue to study the star, hoping to find more evidence.

For some people, the idea that there's a civilization out there, capable of building a giant structure around their sun, would be a dream come true.

It's the same dream that fuels our obsession with aliens…

Whether they charm us…

VIN DIESEL (as Groot, in Guardians of the Galaxy Vol. 2): I am groot.

TALITHIA WILLIAMS: …frighten us…

ADRIANNE PALICKI (as Cmdr. Kelly Grayson in The Orville): Oh no…

TALITHIA WILLIAMS: …seduce us…

TOM CRUISE (as Cage in Edge of Tomorrow): Aargh.

TALITHIA WILLIAMS: …or try to kill Tom Cruise.

TOM CRUISE (as Cage in Edge of Tomorrow): Oh, man, my god.

TALITHIA WILLIAMS: And it's not just the movies. Even the Pentagon recently admitted that it secretly investigated U.F.O. sightings for years. But what's the reality?

Right now, as far as technologically advanced life goes, we have a sample size of one: us.

In fact, when it comes to any form of life, whether it looks like this or this or this, the only examples we know of are right here on Earth.

And the truth is, if we found even one other example of this kind of life, it would be the biggest scientific discovery in our lifetimes.

So where do we start to look?

In 2009, NASA took a major step in the hunt for life beyond Earth, launching the Kepler Space Telescope, to track down signs of Earthlike planets beyond our solar system.

Up until then, astronomers had found about 300 exoplanets, but few were anything like Earth. Small, rocky planets like ours are not easy to spot.

NATALIE BATALHA (NASA Ames Research Center): Planets are literally lost in the glare of their parent stars. The brightness difference, the contrast between a star like our sun and the earth that's right next to it is 10-billion to one.

TALITHIA WILLIAMS: So, instead of hunting for light reflecting off a planet's surface, the telescope focuses on starlight.

JASON KALIRAI: What Kepler did was it looked in a part of the Milky Way galaxy where we had lots of stars in a small field. And it just took pictures over and over again. And occasionally, if those stars have planets, then sometimes those planets would come in front of the star.

JOHN ASHER JOHNSON: As the planet comes around, it's going to block part of the star, and that light won't get to you. And so, that constant level that you see from the star suddenly goes down just a bit.

NATALIE BATALHA: So, these momentary dimmings of light that repeat once every orbit are indicative of a planet orbiting a star.

TALITHIA WILLIAMS: Astrophysicists, like John Asher Johnson and his team at Harvard, use Kepler data to estimate an orbiting planet's size and distance from its star.

JOHN'S STUDENT #1: The dips are pretty deep, so it must be a fairly large planet.

TALITHIA WILLIAMS: Deep dips in the star's light mean the planet is really big or the star is really small.

JOHN'S STUDENT #2: The spacing between them, what is that, like a day or two?

TALITHIA WILLIAMS: And frequent dimming means gravity has drawn it close to the star, making the planet really hot.

JOHN ASHER JOHNSON: Feels pretty much like a classic hot Jupiter.

TALITHIA WILLIAMS: A giant broiling ball of gas like this would not be a great spot for life, so the team looks for signals that are more subtle.

AMBER (John A. Johnson's student): Looking at this, it doesn't look like much, but it looks like there is some sort of periodic signal there.

JOHN ASHER JOHNSON: So, what do we know? We know this is small?

AMBER: It's blocking out less than a percent of the light that we're receiving from…

TALITHIA WILLIAMS: Something is causing the star to dim ever so slightly and at longer intervals.

Could this be a small planet, closer to Earth's size? And the distance from its sun suggests temperatures potentially comfortable for life.

JOHN ASHER JOHNSON: This is really interesting. I mean, this is exactly the kind of thing we are looking for. This could be a rocky planet somewhere near the habitable zone.

JOHN'S STUDENT: Yeah, this is really exciting.

JOHN ASHER JOHNSON: Yeah.

TALITHIA WILLIAMS: The discoveries coming from Kepler have been astounding: nearly 3,000 confirmed planets so far.

JASON KALIRAI: The Kepler Space Telescope blew open our understanding of planets.

NATALIE BATALHA: We have found lava worlds. We've got planets that are orbiting, not one, but two stars. We have found planets that may be covered entirely in liquid water.

TALITHIA WILLIAMS: And some of these planets are Earth-sized, with temperatures potentially ripe for life.

JOHN ASHER JOHNSON: Kepler allowed us to see the sheer numbers and the absolute commonness of Earth-sized planets throughout the galaxy. And so, the chances of us finding life elsewhere, in my view, is very high.

TALITHIA WILLIAMS: In fact, using the small sample of sky observed by Kepler, astronomers now estimate that there are tens of billions of planets in our galaxy the same size and temperature as Earth. These planets could have liquid water on their surfaces; their rocky cores could hold the building blocks of life; and their stars should provide plenty of energy, but does that mean that life would thrive there?

Turns out, that could depend a lot on the star itself.

JASON KALIRAI: Planets are really at the mercy of what happens to the stars that they're orbiting around.

JASON KALIRAI'S DAUGHTER SURIYA: Dad, can you walk slower, maybe?

TALITHIA WILLIAMS: Jason Kalirai is a stellar astrophysicist.

JASON KALIRAI: What are you guys excited about seeing tonight?

JASON KALIRAI'S DAUGHTER MIRA: I'm excited about seeing Saturn.

JASON KALIRAI: Saturn should look amazing tonight.

TALITHIA WILLIAMS: An expert in the behavior of stars, he knows the profound influence they have on orbiting planets.

JASON KALIRAI: So, by studying those stars, we can figure out what kind of planets might be most suitable for finding life.

All right, so here's our main mirror. Do you guys remember what this is called?

JASON KALIRAI'S DAUGHTERS: First mirror?

JASON KALIRAI: Primary mirror.

JASON KALIRAI'S DAUGHTERS: Oh, primary.

TALITHIA WILLIAMS: Jason's curiosity about the cosmos started early.

JASON KALIRAI: As a young kid, one of the things that I found most exciting was trying to figure out how the universe works. And countless times, I would be in our backyard looking up at the night sky, wondering what part of the universe I'm seeing.

TALITHIA WILLIAMS: Jason had clear views of the sky in British Columbia, where he grew up. His parents moved there from Punjab, India, in the 1970s.

JASON KALIRAI: If they had stayed in India, I would not be an astronomer. That's just the way the system is. But in Canada, I could take a liking to whatever I liked. And as a very young kid, I liked astronomy, and when I wanted to become an astronomer and see that through, there was nothing stopping me.

TALITHIA WILLIAMS: Today, he shares his love of astronomy with his twin daughters, Suriya and Mira.

JASON KALIRAI'S DAUGHTER MIRA: Are there any people on different planets?

JASON KALIRAI: So, there's lots of stars in the universe, and all of those stars have planets around them. So, on one of those planets, right now, there might be a dad with his two daughters, on a farm, looking up at the night sky, asking the same question.

JASON KALIRAI'S DAUGHTER MIRA: O.M.G!

JASON KALIRAI: I love showing my daughters the night sky through a telescope,…

JASON KALIRAI'S DAUGHTER SURIYA: Is that Saturn?

JASON KALIRAI: That's Saturn. Can you see the rings?

JASON KALIRAI'S DAUGHTER SURIYA: Whoa!

JASON KALIRAI: …because you see so much more out there that's otherwise invisible to us…

Is that cool?

JASON KALIRAI'S DAUGHTER SURIYA: Yeah.

JASON KALIRAI: …that it instills that curiosity to want to go and find out those answers.

And with astronomy, they'll never be satisfied, 'cause it'll always just throw more questions at you.

TALITHIA WILLIAMS: Jason pursues his questions about the cosmos at the Space Telescope Science Institute, in Maryland. And when it comes to the search for alien worlds, he focuses on the kinds of stars that might be friendliest for life, because not all stars are created equal.

JASON KALIRAI: When we look up at the night sky, we're seeing just the brightest beacons of light. It's not representative of the true distribution of stars, which contains many more lower-mass stars, stars much smaller than the sun.

TALITHIA WILLIAMS: These low-mass stars, sometimes called "red dwarfs," are smaller and cooler than our sun. And while our own sun will burn out in about five-billion years, red dwarfs could burn for trillions of years.

Across the Milky Way galaxy, red dwarfs probably host billions of planets, many of them small and rocky, like Earth. So, how likely is it these planets host life?

One group of planets, just 40 lightyears away, has enticed scientists like Jason, the TRAPPIST-1 system.

JASON KALIRAI: One of the biggest discoveries in the last few years was the discovery of the TRAPPIST-1 system. This is an incredible star.

TALITHIA WILLIAMS: TRAPPIST-1's seven planets are all close to Earth's size and circle it in tight orbits, like a condensed version of our own solar system.

JASON KALIRAI: These planets take a few days to go around their star, and they're only located a couple million miles from their star.

TALITHIA WILLIAMS: TRAPPIST-1's innermost planet orbits its host star every one-and-a-half days.

JASON KALIRAI: It's 90 times closer to the TRAPPIST-1 star than our Earth is to the sun, and so, it's going to be very hot on that planet.

TALITHIA WILLIAMS: Though not a lava world, it's too hot for liquid water or for life as we know it.

JASON KALIRAI: The other end of extreme, we've got Planet H, which is going to take about 20 days going around the TRAPPIST-1 system, which is a huge amount of time, given how faint the TRAPPIST-1 star is. And so it's going to be very cold.

TALITHIA WILLIAMS: Any water here is likely frozen solid.

But a few TRAPPIST-1 planets seem to orbit in the "Goldilocks" zone, just right, with temperatures that could be similar to those on Earth.

JASON KALIRAI: We think these planets in the middle are in the habitable zone—conditions are going to be just right—where liquid water could exist.

TALITHIA WILLIAMS: When the discovery was first announced, hopes were high that some of these planets might harbor life.

But Jason is more skeptical, not because of the planets, but because of the star. Red dwarfs may be small and cool, but they are also more violent and volatile than our sun.

JASON KALIRAI: These are generally pretty active stars. These exhibit a number of solar flares, where there's material that can impact the planet.

TALITHIA WILLIAMS: This material carries enormous amounts of radiation, many billions of hydrogen bombs' worth, enough to destroy the cells of any living thing on a nearby planet.

Jason fears these radioactive solar flares could wipe out any life that might arise in the TRAPPIST-1 system.

JASON KALIRAI: It's actually unclear whether or not the conditions necessary to sustain life and the time that life needs to develop are going to be stable on these planets.

TALITHIA WILLIAMS: Jason isn't giving up on planets that orbit red dwarfs, but he does worry that life there might be so different from our own, we might never recognize it.

JASON KALIRAI: I have no doubt that planets that are very different from Earth and stars that are very different from the sun will still lead to different types of life. But we don't know what we're looking for.

So, the simplest experiment is to try and find life that resembles the life that we understand well on Earth.

TALITHIA WILLIAMS: So, can we find a twin, an Earthlike planet orbiting a sun-like star?

Kepler tracked down a few, but they're more than a thousand lightyears away. How can we find more? And closer? Luckily, a new detective is joining the hunt, NASA's Transiting Exoplanet Survey Satellite, called TESS.

DAVID CHARBONNEAU (Harvard-Smithsonian Center for Astrophysics): TESS will now do a survey of all the nearby stars, so that we can find the very closest planetary systems to us.

TALITHIA WILLIAMS: The telescope's four cameras will observe some 200,000 stars, many big and bright like our sun.

DAVID CHARBONNEAU: TESS will take a snapshot, and it will image all the stars along the strip of the sky. Then it'll move on and do the next set of stars and the next set of stars. That's when there's going to be this firehose that's going to turn on. All of a sudden, we're going to get data from all the closest stars.

TALITHIA WILLIAMS: …data that could translate into thousands of nearby planets, including a lot like our own.

We could soon find ourselves surrounded by potentially habitable neighbors. But then what? If we find a nearby twin, could we ever know if life exists there?

RANA EL KALIOUBY: The very closest potentially habitable planets are a few lightyears away. That's about 25-trillion miles.

Even if we built a spacecraft that could travel a million miles an hour, it would take about 3,000 years to get there. But even if we can't go there, it might be possible to find evidence of life on a faraway plane, in effect, by sniffing its atmosphere.

SARA SEAGER: I mean, we'd all love to find an alien. We'll just be lucky to find anything at all. So, at this point, it doesn't matter what it is, we just want to find some sign of life.

TALITHIA WILLIAMS: M.I.T. astronomer Sara Seager thinks that sign will come in the form of gases in a planet's atmosphere, called "biosignatures."

SARA SEAGER: We call a gas a biosignature gas, if it's a gas that's produced by life that accumulates in the planet atmosphere.

TALITHIA WILLIAMS: About two-and-a-half-billion years ago, life on Earth began pumping out a powerful biosignature. Colonies of bacteria, like these stromatolites, started producing oxygen, like plants do today.

Now our atmosphere is roughly 20 percent oxygen, a telltale sign of life. But how could we ever study a distant planet's atmosphere and detect what gases it holds?

SARA SEAGER: If the planet and star are fortuitously aligned, that starlight can shine through the planet atmosphere.

TALITHIA WILLIAMS: Different gases will absorb starlight in different ways.

SARA SEAGER: It turns out that each gas has its own specific way of interacting with light.

TALITHIA WILLIAMS: We're all familiar with glowing colored gases; they're what lights up the neon signs of cities.

SARA SEAGER: In this tube, for example, there's mercury, showing up as a blue. I can change that out for another gas. This one is helium, it looks orange.

TALITHIA WILLIAMS: When Sara splits the light, she can see even more detail: each gas has a unique light signature.

These signatures could tell Sara about the gases in a planet's atmosphere, gases that could be signs of life. But to see them, she'll need a very powerful telescope.

In 2020, NASA plans to launch the James Webb Space Telescope, the most powerful space-borne telescope to date.

JASON KALIRAI: The James Webb Space Telescope has a 21-foot gold mirror, so it can make exquisitely sensitive measurements of the atmospheric composition of other planets.

TALITHIA WILLIAMS: It makes those measurements with the help of a device called a spectrometer, which, like a prism, divides light into constituent colors.

This helps scientists like Sara identify gases surrounding a planet.

SARA SEAGER: We hope to see gases like water vapor on a small rocky planet, which would indicate liquid water oceans. We'd like to see methane and other gases. And some of these, on their own or together, would help make the case for life on another planet.

TALITHIA WILLIAMS: But even with those gases, the case might be missing a crucial piece of evidence.

MERCEDES LÓPEZ-MORALES (Harvard-Smithsonian Center for Astrophysics): Those are pieces of the puzzle, but that puzzle will be incomplete until we detect oxygen.

TALITHIA WILLIAMS: Astrophysicist Mercedes López-Morales wants to find oxygen in another planet's atmosphere. Remember, Earth got most of its atmospheric oxygen only after living creatures started pumping it out.

But oxygen has a faint signal, and might be difficult for the James Webb Space Telescope to spot on distant planets, so Mercedes is pinning her hopes for finding oxygen on a new telescope, being constructed in a unlikely place.

Underneath the football stadium at the University of Arizona, scientists are turning seven massive slabs of glass into gigantic mirrors.

MERCEDES LÓPEZ-MORALES: This is an 8.4-meter-in-diameter mirror that is today the largest one piece mirror that humans can build.

TALITHIA WILLIAMS: When completed, the mirrors, each weighing 20 tons, will travel to a mountain in Chile, where they will be assembled into the Giant Magellan Telescope, a mega-telescope expected to be 10 times stronger than the Hubble Space Telescope.

That power will come from the near-perfect shaping and polishing of seven mirrors joined into one.

MERCEDES LÓPEZ-MORALES: We need to polish this mirror very, very finely.

TALITHIA WILLIAMS: Each mirror takes more than three years to polish to within 20 nanometers. That's at least 1,000 times smaller than the width of a human hair.

MERCEDES LÓPEZ-MORALES: Every time I see one of these mirrors, I see this big bucket that is collecting light for me. And the bigger the bucket, the more light I can collect, and the easier it will be to detect oxygen in an Earthlike planet.

The Giant Magellan Telescope is going to be a game changer for us.

TALITHIA WILLIAMS: The G.M.T. is scheduled to start hunting for oxygen on other planets within the decade.

JASON KALIRAI: Technology moves very quickly. I think we will find life on another world. We will find a signature that's a smoking gun for life on a nearby planet.

TALITHIA WILLIAMS: But could we find more than a smoking gun?

While some alien-hunters set their hopes on the next generation of telescopes to spot life from afar, some explorers are searching for "E.T." much closer to home.

Astrobiologist Kevin Hand is hunting for life in our own solar system, but the aliens he dreams of are very different from the ones in the movies.

He's looking for a kind of life that could thrive in some of the harshest places on Earth.

KEVIN HAND (NASA Jet Propulsion Laboratory): So, here we are, sitting on a red-hot blister on planet Earth, a volcano.

TALITHIA WILLIAMS: At Lassen Volcanic National Park, in California, temperatures in these springs rise to nearly 200 degrees Fahrenheit, deadly to most forms of life.

KEVIN HAND: This particular bubbling hot spring, of course, does not look like a good place for life. It's not a good place for, for me, this tree or any large creature.

TALITHIA WILLIAMS: And yet, if you look closely, the pools are literally teeming with life. It's just very tiny microbes.

KEVIN HAND: What's amazing about microbes is that they can survive in a variety of different harsh and extreme conditions. For example, all of the green that you see here, these are microbes that are doing photosynthesis, thriving off of energy from the sun.

TALITHIA WILLIAMS: But not all microbes need sunlight.

KEVIN HAND: In this stream that's coming from one of the hot springs, we've got microbes that are surviving on all the compounds dissolved in the water. These microbes don't need sunlight.

TALITHIA WILLIAMS: Kevin thinks he might find creatures like these lurking not too far from Earth.

KEVIN HAND: These are the kinds of lifeforms that we think could potentially inhabit the deep, dark oceans of other worlds.

TALITHIA WILLIAMS: But what oceans? None of the other planets in our solar system have liquid water oceans on their surfaces.

So, astrobiologists like Kevin are laying their bets on two balls of ice that aren't planets at all, but moons: Enceladus, a moon of Saturn, and Europa, a moon of Jupiter. At first glance, both appear to be barren, but cracks on the surface reveal activity below.

Extreme gravitational forces created by their massive parent planets could be causing the moons' rocky cores to heat up. And when you put together heat and ice…

MARY VOYTEK (NASA Senior Astrobiologist): Because of frictional heating of the ice against the solid core, you get the formation of subsurface oceans.

TALITHIA WILLIAMS: Scientists now believe that the ice on both moons covers hidden oceans below, with Europa holding more water than all of Earth's oceans combined. And here, deep in the oceans of these tiny moons, could lie all the fundamental ingredients of life.

MARY VOYTEK: If you have ocean water coming into contact with rock at elevated temperatures, you'll get energy for life that's not coming from the sun, but from chemical reactions.

KEVIN HAND: Worlds like Europa and Enceladus, where we've got good evidence for vast, global, liquid-water oceans, could be where a second origin of life occurred.

TALITHIA WILLIAMS: Kevin thinks there's a strong chance that life could exist on Europa, the larger of the two moons. But how could you ever find it?

KEVIN HAND: You wouldn't want to go to Europa. It'd be a beautiful view of Jupiter, but as soon as you stepped out of your spacecraft, you'd die. It's minus-280 degrees Fahrenheit, there's no atmosphere, and then the radiation that would rain down onto you would kill you within a matter of tens of minutes.

TALITHIA WILLIAMS: Astronauts won't be attempting to skate across Europa's icy surface anytime soon, so NASA is studying ways to send a robotic probe nearly 400-million miles to the bright moon to hunt for traces of life, but not before we know what to look for.

If Europan sea creatures, even microbes, existed and made their way to the surface of the ice, their cells and anything resembling D.N.A. would be heavily altered by radiation. But Kevin thinks we can hunt for remnants of life in the form of amino acids, the building blocks of proteins.

KEVIN HAND: So, if we found amino acids in ice, that could be a pretty strong sign of life within that ocean.

TALITHIA WILLIAMS: But how likely is it that traces, in the form of amino acids, could survive on the surface and be detected by our spacecraft?

To figure that out, Kevin and his team are replicating some of the conditions on the icy moon, right here at NASA's Jet Propulsion Laboratory, in Pasadena.

In this latest test, Kevin's molecular guinea pig is glycine, the simplest amino acid, found in every living thing on Earth.

KEVIN HAND: We're mixing glycine in with water to, kind of, replicate what could be in Europa's ocean, were it to have life.

TALITHIA WILLIAMS: The mixture goes into a stockpot, a witch's brew of water and salts.

Over three weeks, Kevin pummels the glycine with the sub-zero temperatures and dangerously low pressure you'd experience on Europa's surface. Finally, it's time to find out if any glycine survived the ordeal.

KEVIN HAND: Okay, well, we've definitely cooked up something interesting in here.

TALITHIA WILLIAMS: If the amino acid is completely destroyed, the odds of finding some sign of life on Europa's surface are slim to none.

KEVIN HAND: It doesn't look like ice; it looks like a solid but soft surface. This is almost like a crème brûlée, I think.

Going in. Oooh, interesting. Okay.

LAB TECHNICIAN: Do you feel like there was a tough crust?

KEVIN HAND: No, no. It's very powdery. Oh, look at that.

TALITHIA WILLIAMS: Kevin was expecting a hard icy shell, but he's surprised to see that the ingredients have frozen into a thick powder.

KEVIN HAND: You can…it's almost like a layered, feathered material.

TALITHIA WILLIAMS: Now for the real test: Kevin probes the ice with a spectrometer, using light to seek out and measure glycine's unique signature.

Can a simple amino acid, a single building block of life, withstand the harsh environment of Europa's surface and be detectable?

KEVIN HAND: Get in nice and close, and we'll get the maximum signal.

TALITHIA WILLIAMS: And like a beacon, it appears: a small but clear signal of glycine. It means that if there is microbial life in the oceans of Europa, we might be able to find some of its building blocks on the moon's icy surface.

KEVIN HAND: Is that what the signal of life on a distant world might look like? We just don't know. The next thing to do is launch a spacecraft and go look for it out there in the solar system.

ANDRE FENTON: Finding amino acids on Europa's surface would be encouraging, but what we really want to know is what might be swimming around in Europa's vast oceans. Could there be microbes? Like the ones that dominated Earth's own oceans for billions of years?

Or something more complex? If we want to find out, then we need to send a mission much deeper, down through the ice and into the pitch black oceans below.

But how do you prepare for such an ambitious trip to a place unlike anywhere on Earth? Engineer Bill Stone believes he has the answer.

WILLIAM "BILL" STONE (Stone Aerospace): If you ask me, "What is exploration?" It is the process of putting your boot in a place where no one has ever been before.

TALITHIA WILLIAMS: Bill's "boot" is an underwater vehicle named "Sunfish," his prototype for an ocean-exploring robot. It might not look like much, but if there's something swimming around on Europa, a miniature version of this robot could be the first to spot it.

BILL STONE: It will be one of the greatest intellectual feats of humankind, if we pull this off.

TALITHIA WILLIAMS: NASA is studying how to get to Europa's surface in about 15 years. Bill is planning for a much more ambitious journey: fly a robotic lander 400-million miles to Europa and land on the surface, bore through an icecap some 10- to 15-miles-thick, then release an autonomous underwater vehicle to explore the mysterious ocean below.

BILL STONE: Once you get through the ice, Sunfish will go out and map, explore and look for life.

TALITHIA WILLIAMS: This wouldn't be the first robotic mission in our solar system. Mars rovers have explored the red planet by following commands that come from Earth, 34-million miles away.

That's not possible on Europa, which is roughly three times as distant as Mars.

BILL STONE: The problem is there's a two-hour delay light travel time between Europa and Earth, so we can't sit there and joystick something.

TALITHIA WILLIAMS: This robot must be able to think and explore all on its own, or else it won't be able to see much of the European ocean, and the mission to Jupiter's moon could be a wasted opportunity.

MAN ON WALKIE TALKIE: Where would you like us to position the robot?

TALITHIA WILLIAMS: To do that, it needs practice.

ROBOT OPERATOR: Okay, here we go; heading east.

BILL STONE: We're at Peacock Springs State Park in northern Florida, because there is an underwater labyrinth, a maze.

TALITHIA WILLIAMS: The ground in this part of Florida is riddled with winding, water-filled caves. Can Bill's robot negotiate this confusing environment on its own?

A team of experienced cave divers tags along, in case the robot breaks down. Other than that, the robot is virtually alone, using sonar to explore and map its surroundings, inch by inch.

BILL STONE: The robot doesn't know anything about this cave, and so, it is learning to explore as it goes.

ENGINEER #1: So, we're at 21.

ENGINEER #2: So, 240 points us down the tunnel.

TALITHIA WILLIAMS: Things seem to be going well, until, in one narrow cave, Sunfish stops. It suddenly seems confused.

ENGINEER #1: It's drifting a lot. Whoa.

BILL STONE: What do you do if something goes wrong? What's your procedure? All that has to go into the code.

ENGINEER #1: Zero, zero, 240-D.

TALITHIA WILLIAMS: A few lines of code outline a new strategy: backup and remap from a different angle. This time, the robot succeeds.

BILL STONE: It's achieved the goal; turning back.

TALITHIA WILLIAMS: This is a small step that could one day lead to a giant leap in the search for life beyond Earth.

BILL STONE: If there's going to be life on Europa, there is no reason why we can't have life somewhere else in the universe…be the first validation that we aren't the only ones, so, from that standpoint, it's going to shake a lot of ground.

TALITHIA WILLIAMS: If we found evidence of life on Europa, even if it were just a teeny tiny microbe, that would be huge.

PAUL DAVIES: All it needs is for one microbe that is life-but-not-as-we-know-it, to make the point that it can't be that hard to get going, just one microbe.

SETH SHOSTAK: The importance of that is to say, "Guess what? Biology's not very hard." It's an infection in the universe, right? It's all over the place.

TALITHIA WILLIAMS: If a galaxy oozing with pond scum doesn't seem too exciting, then remember, over a few billions years, these tiny creatures evolved into all the plants and animals that swim, crawl and fly around our planet, including us. So, could the same thing happen somewhere else?

What do we think aliens that evolved on another planet would be like?

EARTH VS. THE FLYING SAUCERS: Flying saucers have invaded our planet.

TALITHIA WILLIAMS: In lots of movies, aliens look remarkably like us, with two arms and legs…

THE MYSTERIANS: Only you of Earth, you and your women, can give us life.

CHARACTER IN THE MYSTERIANS: Get back or I'll fire.

TALITHIA WILLIAMS: And of course, those eyes.

ALIEN IN "THE UNNATURAL," THE X-FILES: Aaar.

FREDRIC LEHNE (as Young Arthur Dales in "The Unnatural," X-Files): Aaar.

SETH SHOSTAK: From the standpoint of Hollywood, the aliens tend to be these little gray guys with big eyeballs, and, you know, and no sense of humor, and no clothes, by the way. They seem very dispassionate. They don't seem to get angry, they don't seem to have a lot of fun, either.

JUDGE (in Mars Attacks!): Come on down, Mr. Ambassador.

TALITHIA WILLIAMS: Science fiction aliens usually have something else in common with us: intelligence. But what are the chances that life, if it did arise elsewhere, would evolve into creatures with big brains?

After all, aren't we the only smart ones on this planet? Some biologists would say, "no."

JARED TAGLIALATELA: Good job, buddy.

TALITHIA WILLIAMS: And they're not just talking about our closest relatives. From dolphins, to birds, to even the octopus—a creature more closely related to snails and clams than to us, but smart enough to use tools and open jars—we're not the only animals who've evolved impressive brains.

Of course, none of these creatures will build a spaceship anytime soon. But for many scientists, the idea that we're the only technologically advanced creatures in the universe seems a bit, well, presumptuous.

SETH SHOSTAK: We used to think the earth was the center of the universe; that was wrong. Then we thought the sun was the center of the universe; and that was wrong. Then we thought our galaxy was the center of the universe; and that was wrong. Every time we thought we were really special, we were wrong. And so, the idea that we're somehow special in terms of being alive or being intelligent, I mean, that's probably wrong too.

JOHN ASHER JOHNSON: I find it extremely hard to believe that, in the vastness of our universe, that a rocky planet that harbors intelligent, sentient life happened just once.

TALITHIA WILLIAMS: Some scientists have spent their entire careers hunting the vast emptiness of space, trying to pick up a signal.

JILL TARTER (SETI Institute): I always just took for granted that there would be other stars that would be suns for other creatures, and that just seemed to me the natural way of the world.

TALITHIA WILLIAMS: More than three decades ago, astronomer Jill Tarter co-founded the SETI Institute, dedicated to the search for extraterrestrial intelligence.

JILL TARTER: It's been amazing to be able to spend a career on a question that I'm fascinated with and a question that everybody else out there is curious to know the answer to.

TALITHIA WILLIAMS: She was the inspiration for the character Dr. Ellie Arroway in Carl Sagan's book, Contact, which was adapted to a feature film, in 1997.

Today, SETI conducts searches with the Allen Telescope Array, a network of 42 radio telescopes in Hat Creek, California.

The telescopes comb the skies for radio waves, which can carry signals and information across the great distances of space.

DOUG VAKOCH (Messaging Extraterrestrial Intelligence): Radio waves are an excellent way to communicate, because they cut through the atmosphere of our earth and also cut through the space between the stars.

TALITHIA WILLIAMS: In fact, we've been sending out our own radio waves since the dawn of broadcasting, about a century ago.

DICK VAN DYKE (As Rob Petrie, The Dick Van Dyke Show): Morning, honey.

TALITHIA WILLIAMS: If any aliens are listening, their ideas about Earthlings could be based on The Dick Van Dyke Show.

DICK VAN DYKE (As Rob Petrie, The Dick Van Dyke Show): I said, "How's my old lady?"

MARY TYLER MOORE (As Laura Petrie, The Dick Van Dyke Show): Well, I don't know. I haven't spoken to your mother lately. But I'm fine.

TALITHIA WILLIAMS: The hope of SETI is that some aliens might also be broadcasting.

SETH SHOSTAK: The idea is that, if life has sprung up on some other worlds and, and it's technological life, in other words, they've you know, they've learned a little bit of physics, they built some equipment, this, that and the other, they could build radio transmitters that are sending signals into space that we could pick up here.

TALITHIA WILLIAMS: At Hat Creek, the telescopes listen in on millions of radio channels, at a time, looking for unique patterns that could be alien transmissions.

JILL TARTER: When something shows up that we don't think is interference, something that we've not seen before, immediately we follow up on that signal to try and figure out what it is, and whether it's, in fact, our technology or potentially someone else's.

TALITHIA WILLIAMS: But unique signals are rare, just one or two a year. And so far, even the most promising ones have turned out to be human interference. Still, the event that SETI is waiting for could happen any day.

JODIE FOSTER (as Eleanor Arroway in Contact): Okay. Point source confirmed. Whatever it is, it ain't local.

TALITHIA WILLIAMS: While Hollywood has fantasized about this moment of discovery, it's harder than it looks. The Allen Telescope Array can only listen to a few hundred million, out of billions of possible radio frequencies, at a time.

JILL TARTER: We haven't yet figured out how to look at all the sky, all the time, at all frequencies, but that's ultimately what we want to do.

TALITHIA WILLIAMS: In fact, we've been listening for nearly 60 years, and so far, crickets.

But the fraction of stars we've searched carefully and the time for which we've been listening are still both quite small. So, plenty of people remain hopeful that technologically advanced civilizations are out there.

And that's why the mysterious dimming of one particular star was, for some, so tantalizing.

In 2015, astronomer Tabetha Boyajian and her colleagues published their findings about a very weird star.

According to data from the Kepler Space Telescope, Tabby's star was dimming at strange, irregular intervals, sparking theories about an enormous structure, built by a hypothetical advanced alien civilization. The buzz spurred more research. Today, a worldwide network of powerful ground-based telescopes stare at Tabby's star around the clock.

TABETHA BOYAJIAN: We can actually process the data in near-real time, and when we see something start to happen, we can trigger more intense observations of what is passing in front of the star at that time.

TALITHIA WILLIAMS: For a while, the star was silent. Then suddenly, it started dimming erratically again. The ground-based telescopes provide information about the star that Kepler couldn't see, not just the dimming of the star, but how those dips in brightness appear in different colored wavelengths.

TABETHA BOYAJIAN: Something is happening with our star here.

We sent off alerts via Twitter, and data of all sorts started coming our way. At this point, it's like we're swimming in data.

TALITHIA WILLIAMS: Tabby and her team at Louisiana State are looking for patterns in the color data that could tell them what kind of material is passing in front of the star.

TABETHA BOYAJIAN: Blue light and red light will react differently to material that's passing in front of the star, and you'll have a different signature in how far down these dips go.

TALITHIA WILLIAMS: Whatever is passing in front of Tabby's star appears to be blocking more blue light than red and orange light. But what would block out more blue light?

Tabetha has a theory: space dust.

TABETHA BOYAJIAN: Dust scatters blue light more than it does red light. And so, that indicates that there's some sort of dusty semi-opaque, you know, material that's crossing in front of the star and blocking out its light.

EMILY (Louisiana State University): It's got the signatures of being dust, rather than, it's…can't be some sort of opaque object, like a planet or an alien megastructure?

TABETHA BOYAJIAN: That's right.

TALITHIA WILLIAMS: The culprit is likely scattered dust, and not a solid alien megastructure.

But the mystery is hardly solved. What created this giant cloud of dust? Why is it centered around Tabby's star? Astronomers will need more data if they're ever going to crack this one.

TABETHA BOYAJIAN: Nature is a lot more creative than we are, and you know, we're just going to have to, you know, really buckle down and try and, and figure this one out.

TALITHIA WILLIAMS: Tabby's star is just one in a long line of mysteries that, at first, raised hopes for finding E.T., but later were revealed to have solutions unrelated to life. For some, the lack of firm evidence is troubling.

In 1950, physicist Enrico Fermi went to lunch with some colleagues and asked a simple question: "Where is everybody?"

ANDRE FENTON: If there are billions of habitable planets out there, and life is common…

RANA EL KALIOUBY: …why haven't a bunch of aliens already showed up on our doorstep?

What could explain the silence?

TALITHIA WILLIAMS: For some, the quietness of the cosmos is evidence that we really could be alone, but many astronomers disagree.

JASON KALIRAI: The idea that there's intelligent life out there that has never interacted with us or that we've never seen it, that, to me, is not confusing at all. I mean, I think that's perfectly consistent.

It's no different than a child looking at an ant farm, right? The child is not going to be compelled to interact with an individual ant, and more so, the ants probably don't even know that the child is analyzing the ant farm.

And so, there's very likely intelligent civilizations out there that may be looking at us, but what do they have to gain from interacting with us? We might be very basic and insignificant compared to them.

TALITHIA WILLIAMS: Or perhaps interstellar travel is too challenging, even for super-smart aliens. Or maybe they did exist but ended up destroying themselves.

For many, the universe is simply too large, too many stars with too many planets, too many potential homes for creatures that might start small but could, like us, thrive and grow.

JOHN ASHER JOHNSON: The universe is mind-boggling. It's bigger than what we humans can actually wrap our consciousness around.

JASON KALIRAI: The universe has hundreds of billions of planets and hundreds of billions of galaxies.

SARA SEAGER: So, it just seems like, when you roll the dice many, many times, one of them is going to luck out.

MERCEDES LÓPEZ-MORALES: We live in a groundbreaking era. We might be the first generation in human history that will be able to say that there is life elsewhere in the universe.

JILL TARTER: Our young people have a much greater opportunity to see themselves as Earthlings.

DAVID CHARBONNEAU: But we also could find out that, to the best of our ability to measure, we really are alone.

PAUL DAVIES: If it turns out that Earth is rare, then that's all the more reason to look after what we've got, because if we destroy ourselves, the flame of mind and the flame of culture will be snuffed out for good.

TABETHA BOYAJIAN: I hope that we aren't the only things out there. There's got to be something else.

SETH SHOSTAK: You know there's, there's a lot of room up there. It's hard to believe that everything interesting is down here. It just never struck me as a very reasonable point of view.

BILL STONE: Are we alone in the universe? Not a chance.

Credits

HOSTED BY Talithia Williams CO-HOSTED BY Rana el Kaliouby
André Fenton PRODUCED AND DIRECTED BY Jane Teeling and Phil Bertelsen WRITTEN BY Phil Bertelsen EXECUTIVE PRODUCER Julia Cort SERIES PRODUCERS Michael Bicks & Anna Lee Strachan EDITED BY Ben Howard DIRECTORS OF PHOTOGRAPHY Jason Longo
John Behrens ANIMATION Edgeworx Studios LLC
Ekin Akalin ORIGINAL MUSIC BY Christopher Rife ADDITIONAL MUSIC BY Scorekeeper's Music SUPERVISING PRODUCER Kevin Young COORDINATING PRODUCER Elizabeth Benjes ADDITIONAL CAMERA Lincoln Else
Glenn Evans
Ben Howard
Jill Heinerth SOUND RECORDISTS Adriano Bravo
Rodrigo Salvatierra
Jason Longo
John Behrens
Steve Bores
Marshall Potter
Jason Cotton
Chris Hall
---
Clint Bramesco
Derek Hanson
Eric Laws
David Strayer ASSISTANT CAMERA Rachel Behrmann
Theodore Caleb Haas
Jason Allread ADDITIONAL EDITING Jenna Bliss
Bruce Shaw
Michael H. Amundson
Jaro Savol ASSISTANT EDITORS Julio Ramirez
Allison Corcoran
Yoni Turkienicz PRODUCTION ASSISTANTS Rachel Behrmann
Lauren Vernea
Rob Picciano
Theodore Caleb Haas
Jason Allread
Zach Baum
Christian Jones STUDIO PRODUCTION ASSOCIATE PRODUCER Diane Knox HAIR AND MAKEUP Phoebe Ramler GAFFER Mike Lee PRODUCTION ASSISTANT Harlem Logan ONLINE EDITOR AND COLORIST David Bigelow AUDIO MIX Heart Punch Studio POST SUPERVISORS Stephen Altobello
Todd Goings LINE PRODUCERS Dorin Razam-Grunfeld
Stef Gordan RESEARCH Lauren Vernea
Nurit Chinn ARCHIVAL MATERIAL Giant Magellan Telescope – GMTO Corporation
Internet Archive
NASA/Ames/J. Jenkins
NASA Goddard Space Flight Center
NASA Goddard Space Flight Center/SDO/Genna Duberstein
NASA Goddard Space Flight Center/Michael McClare
NASA/Kepler mission
NASA, ESA, and J. Lotz and the HFF Team (STScI)
NASA/ESA/STScI
R. Kilgard et al. / Wesleyan U. / NASA / CXC / STScI
SDO/NASA Goddard's Scientific Visualization Studio
NASA/GSFC/SDO
NASA/Chris Chamberland
NASA/JPL-Caltech/MSSS
Earth Science and Remote Sensing Unit, NASA Johnson Space Center
NASA, Dana Berry/SkyWorks Digital, Northrop Grumman, STScI
Las Cumbres Observatory
National Geographic Creative
NASA/JPL/Caltech
NASA/JPL-Caltech/SETI Institute
NASA/JPL/University of Arizona/University of Colorado
NASA & ESA, Jesús Maíz Apellániz (Centro de Astrobiología, CSIC-INTA, Spain)
Wolfgang Baumeister / Science Photo Library
T. Stevens & P. McKinley, Pacific Northwest Laboratory / Science Photo Library
Dennis Kunkel Microscopy / Science Photo Library SPECIAL THANKS Jennifer Burt
Eliza Kempton
Laura Kreidberg
Andrew Vanderburg
Lawrence Ziegler
Jacob Bean
Andrei Tokmakoff
Jason Wright
Angelle Tanner
Eva Bodman
Alyssa Rhoden
David Kipping
Jon Fortney
Reilly Talbot
Katherine Talbot
Sarah Ballard
Pete Worden
Jane and Jerry Conlon
The Kalirai family
The Boyajian-Mazingue family
Druid Circle
Clifton Ragsdale
Carolyn Albertin
Yan Wang
Stone Aerospace
PondView Systems SCIENCE ADVISOR David Grinspoon NOVA WONDERS PACKAGING GRAPHICS Michael H. Amundson CLOSED CAPTIONING The Caption Center POST PRODUCTION ONLINE EDITOR Lindsey Rundell Denault DIGITAL PRODUCTION ASSISTANT Ana Aceves DIGITAL ASSOCIATE PRODUCERS Michael Rivera
Arlo Perez DIGITAL MANAGING PRODUCER Kristine Allington SENIOR DIGITAL EDITOR Tim De Chant SENIOR DIGITAL PRODUCER Ari Daniel DIRECTOR OF NATIONAL AUDIENCE RESEARCH Cory Allen PUBLICITY Eileen Campion
Eddie Ward DIRECTOR OF PUBLIC RELATIONS Jennifer Welsh DIRECTOR AUDIENCE DEVELOPMENT Dante Graves PRODUCTION ASSISTANT Lindsey Chou PRODUCTION COORDINATOR Linda Callahan UNIT MANAGER Vanessa Ly BUSINESS MANAGER Ariam McCrary PARALEGAL Sarah Erlandson TALENT RELATIONS Janice Flood LEGAL COUNSEL Susan Rosen RIGHTS MANAGER Lauren Miller ASSOCIATE RESEARCHER Brian Kantor POST PRODUCTION ASSISTANT Jay Colamaria SENIOR PROMOTIONS PRODUCER AND EDITOR Michael H. Amundson BROADCAST MANAGER Nathan Gunner SCIENCE EDITOR Caitlin Saks DEVELOPMENT PRODUCER David Condon PROJECT DIRECTOR Pamela Rosenstein SENIOR SCIENCE EDITOR Evan Hadingham SENIOR PRODUCER Chris Schmidt SENIOR SERIES PRODUCER Melanie Wallace DIRECTOR, BUSINESS OPERATIONS & FINANCE Laurie Cahalane SENIOR EXECUTIVE PRODUCER Paula S. Apsell

A NOVA Production by Ark Media for WGBH Boston

© 2018 WGBH Educational Foundation

All rights reserved

This program was produced by WGBH, which is solely responsible for its content. Some funders of NOVA Wonders 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 the National Science Foundation, the Gordon and Betty Moore Foundation, the Alfred P. Sloan Foundation and the John Templeton Foundation.

This material is based upon work supported by the National Science Foundation under Grant No. DRL-1420749. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.

IMAGE: Image credit (Deep Space Radio Telescopes) © Neo Edmund/Shutterstock

Participants

Natalie Batalha, Tabetha Boyajian, David Charbonneau, Paul Davies, Rana el Kaliouby, André Fenton, Kevin Hand, John Johnson, Jason Kalirai, Avi Loeb, Mercedes López-Morales, Sara Seager, Seth Shostak, William Stone, Jill Tarter, Doug Vakoch, Mary Voytek, Talithia Williams

More Ways to Watch