To push beyond our boundaries, to see what lies beyond the horizon.

Now tens of billions of kilometers from Earth, two spacecraft are streaking out into the void.

What will we learn about the Galaxy, the Universe, and ourselves from Voyager’s epic Journey

to the stars?

December 19, 1972. The splashdown of the Apollo 17 crew capsule marked the end of the golden

age of manned spaceflight.

The Mercury, Gemini, and Apollo programs had proven that we could send people into space,

to orbit the Earth, fly out beyond our planet, then land on the moon and walk among its ancient

craters.

The collective will to send people beyond our planet faded in times of economic uncertainty,

war, and shifting priorities.

And yet, just five years after Apollo ended, scientists launched a new vision that was

just as profound and even more far-reaching.

We knew we were on a journey of discovery when we launched the Voyager spacecraft, but

we had no idea how much there was to discover.

We had a sense that we knew what it felt like to be Magellan or Columbus

It didn’t all go smoothly. Early computer problems threatened to doom Voyager 2. Then

its radio receiver failed, forcing engineers to use a back up.

Now, after more than three and a half decades of successful operations, the twin spacecraft

are sending back information on their flight into interstellar space.

Along the way, they have revealed a solar system rich beyond our imagining.

Time after time we were surprised by seeing things that we had not expected or even imagined:

volcanoes erupting from the moon, Io, the possibility of a liquid water ocean under

the icy crust of Europa, Titan, where we found an atmosphere, Uranus’ small moon, Miranda,

which had one of the most complex geologic surfaces we’ve seen. Even at Neptune, 40

degrees above absolute zero, even there, there were geysers erupting.

It’s the only spacecraft that has gone by Uranus. It’s the only spacecraft that has

gone by Neptune. Everything we know about those planets, we know from Voyager.

To see those first pictures coming in from the outer solar system, for the first time,

what had been a point of light in the sky was a place.

The journey was made possible by a rare alignment of the planets, a configuration that occurs

only once every 176 years.

That enabled the craft to go from planet to planet, accelerating as they entered the gravitational

field of one, then flying out to the next.

The Voyagers carried a battery of scientific equipment to collect data on the unknown worlds

in their path. That included a pair of vidicom cameras, and a data transfer rate slower than

a dialup modem.

They are primitive by today’s standards, but that didn’t stop them from returning

a flurry of discoveries. On Jupiter’s moon Io, Voyager’s cameras spotted nine erupting

volcanoes.

They documented volcanic plumes reaching 300 kilometers into the atmosphere, at velocities

of one kilometer every second.

Almost two years later, on November 12, 1980, Voyager 1 sailed down to within 124,000 kilometers

of Saturn’s cloud-tops. That’s one-third the distance between Earth and the moon.

It found that Saturn’s atmosphere is almost entirely hydrogen and helium. It is the only

planet in our solar system that is less dense than water.

One year earlier, Pioneer 11 had detected a thick, gaseous atmosphere on Saturn’s

large moon, Titan. Scientists decided to send Voyager 1 to follow up.

It sent back clues to one of the most fascinating bodies in the solar system.

Titan proved to be the only object in the solar system, other than Earth, with stable

bodies of surface liquid. Not water, but vast lakes of liquid methane.

Scientists could have chosen to send Voyager 1 out to Pluto. But Titan was more promising

scientifically.

But that meant its grand tour of the outer planets was over. Voyager 1 headed north,

above the plane of the solar system.

Five years later, and over a billion and a half kilometers beyond Saturn, Voyager 2 reached

Uranus.

Like all the other planets, Uranus spins like a top. But Voyager 2 found that it’s actually

tipped on its side. Its magnetic field reaches out in a bizarre corkscrew tail, millions

of kilometers into space.

Voyager 2 discovered two new rings; thin, dark bands of ice, rock, and dust with particles

the size of a fist.

Although the craft discovered 10 new Uranian moons, the most eagerly anticipated event

was a close encounter with Miranda, perhaps the most bizarre object in our solar system.

Close-ups revealed a strange and wondrous landscape including a canyon 19 kilometers

deep.

Miranda may have collided with another moon, shattered, and then by the force of its own

gravity, slowly reassembled into this chunk of rock and ice.

After 12 years on the road, Voyager 2 now sped toward its rendezvous with Neptune.

The planet appears blue because methane in its atmosphere absorbs most of the red in

the light spectrum.

Remarkably, Voyager 2 flew by Neptune only 35 kilometers off its charted course and only

1 second off its scheduled fly-by time.

Skimming only 5,000 kilometers above the planet’s north pole, Voyager found Neptune to be a

giant ball of melted rock and ice. Cloaked in hydrogen, helium, and methane gasses, its

atmosphere is whipped by winds of 1,000 kilometers per hour.

Flying in closer than any spacecraft has come to one of the outer planets, Voyager 2 discovered

at least four complete rings of ice and rock, six new moons, and a great dark spot; a hurricane

the size of Earth raging in Neptune’s southern hemisphere.

The storm circles the planet every 18 hours, and rotates around its own axis every 16 days.

Oddly, the largest of Neptune’s 8 moons, Triton, orbits in the opposite direction to

the planet’s spin.

Triton was likely an independent object in orbit around the sun, until it was captured

by Neptune’s gravity.

Pocked with impact craters and glazed with methane and nitrogen ice, Triton is the coldest

known object in the Solar System, at minus 240 degrees Celsius.

On its surface, scientists saw jagged mountains, high cliffs, and frozen lakes.

The most bizarre discovery was the presence of icy geysers with plumes reaching 160 kilometers

downwind.

Leaving Neptune, Voyager 2 snapped one of the most remarkable pictures ever taken.

Neptune and its cold moon Triton, framed by the dim light of the Sun.

Several years earlier, the Pioneer spacecraft carried a plaque illustrating the spin state

of a hydrogen atom, a man and woman set against an outline of the spacecraft, and the position

of the Sun relative to 14 prominent pulsars.

The Voyagers brought their own message in a bottle: a disk encoded with images of life

on Earth, greetings in 55 languages, a selection of music, messages, and natural sounds.

And here was this Noah’s Ark of human culture that was being sent to the outer planets,

and then beyond to wander in the interstellar darkness for a billion years. On Valentine’s Day 1990,

Voyager 1 looked homeward. And what did it find? Not the frame-filling Apollo Earth,

but instead, that one-pixel Earth. That’s here. That’s home.

Thirteen years after launch, the Voyager craft finally began their journey into the galaxy

at large.

They run on plutonium-powered Radioisotope Thermoelectric Generators, a standard set

up for NASA deep space missions. Because even these systems don’t last forever, scientists

have had to shut down Voyager’s instruments one by one.

Among the most valuable remaining sensors are magnetometers that can read magnetic fields

that constantly sculpt the outer solar system.

This region is the outer edge of a bubble formed by the sun’s magnetic field and the

solar wind.

Tonight we’re going to be getting the data back from a magnetometer roll calibration

maneuver, and that maneuver actually happened on the Voyager 1 spacecraft over 16 hours

ago, and the data is finally making it back to the earth. What we’re doing is a roll

about this high-gain antenna, and so if the high-gain antenna here is pointed out toward

earth we’re going to be rolling the spacecraft along that high-gain antenna. That roll is

done so that we can calibrate the instrument so that we know what magnetic field belongs

to the sun and what component belongs to the actual spacecraft.

They’re very near the edge of the bubble the sun creates around itself called the Heliosphere.

We’re getting very close to the boundary. We don’t know how close because no spacecraft

has ever been there before, but it could be another few months, it could be another few

years, but it’s probably not much longer than that. We travel a billion miles every

three years.

You can’t see the bubble the sun creates around itself because it’s invisible, but

we can see an analog of it in a sink. If we turn the water on very fast and look at the

bottom of the sink, we see that near where the water hits the bottom of the sink, it’s

flowing very fast radially outward in all directions, and getting thinner until it abruptly

slows down in this thick region, and turns around and flows down the drain. The two Voyager

spacecraft are both in this thick region in our heliosphere where the wind has slowed

down and is starting to go down the tail of the heliosphere. And eventually, in hopefully

not too many more years, Voyager 1 will leave this thick region and enter interstellar space.

We have a 20-watt transmitter on the spacecraft transmitting over 11 billion miles away, and

so it comes in very slowly. But every bit left that spacecraft over 16 hours ago and

every bit is telling us something new that we haven’t known before.

As the solar wind travels out from the sun, it pushes against the galactic medium and

abruptly slows down in a region called the Termination shock. Outside this is the Heliosheath,

where the sun’s magnetic field is bent back by the interstellar wind.

The sun’s magnetic field spins in opposite directions on the north and south poles, creating

a sheet where the two spins meet. This sheet gently ripples as it travels outward. When

this sheet reaches the termination shock, it starts to compress like water waves hitting

a wall.

The voyager spacecraft have now found that these stacked up ripples of magnetic field

form smaller bubbles, shown here as a computer simulation.

The discovery of this frothy character changes our understanding of how extremely fast moving

particles, called cosmic rays, enter our solar system.

When they arrive at this region, they slowly move from bubble to bubble until they can

reach smooth magnetic field lines and follow them toward the sun.

Recently, the twin Voyagers began their transition into interstellar space.

Voyager today is headed for the edge of interstellar space. That’s the space between stars and

it’s filled with material that has been injected by the explosion of stars, matter

which came from a particular direction, creating a wind which has shaped the bubble in which

the solar system is surrounded.

Since July of 2012, the solar wind has decreased, while the galactic wind has sped up.

That places the craft in what scientists call the “magnetic highway,” where the alignment

of magnetic fields allows particles from the sun to escape, and particles from the galaxy

to pour in.

When either one reports a complete change in the direction of the magnetic field, that’s

when scientists will know that it has finally exited the solar system.

Meanwhile, they are delivering a whole new view of the galaxy in ultraviolet light. From

Earth, this light is normally blocked by the haze of particles at the edge of the solar

system.

Scientists are able to capture this light from other galaxies because their wavelength