Aug 19, 2025 Thanks to the invention of spaceflight, the drive to explore is leading us upward and outward - off of our own planet and out into the solar system where a host of alien worlds offers us vast new terrain to uncover. This visually breathtaking series offers a new perspective on our solar system. Through beautiful HD imagery, audiences will not only be taken to places they have never been, but they will get an immersive experience of places they could never go.
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For generations, our world has challenged explorers
to seek what lies beyond the horizon.
Now, the invention of spaceflight
is leading us outward to explore a host of alien worlds
with vast new territories.
Today, we see the sun, moon, and planets
with penetrating clarity through the eyes
of the intrepid machines blazing a trail for us
across the solar system.
Their cameras have become our windows
onto a bold new adventure.
Their discoveries have become our cosmic vistas.
To the human eye, our universe is all about light.
It's the sign that matter is present
in stars, in galaxies, and in great expanses of glowing gas.
But despite its beauty, this colorful realm
of gas and stars is not a place where life can exist.
Life as we know it is too fragile
to survive the searing temperatures that make
atoms of gas glow in space.
What life needs is a very different kind of place,
one not simply made of swirls of gas, but of something solid.
Life needs a rocky planet.
Without planets made of rock, there
would be no chance for life as we know it.
But simply having a solid place to stand
is no guarantee that life will gain a foothold.
We can see this in our own solar system,
where there are many different kinds of rocky worlds.
First in line is Mercury, a small and mysterious planet
that is alternately baked then frozen as it slowly
rotates in the sun's glare.
As the nearest planet to the sun,
Mercury's daytime surface temperature
can reach more than 420 degrees Celsius.
Yet on the planet's night side, where heat is quickly
radiated into space during long months of darkness,
the temperature can drop below minus 180.
For decades, Mercury's one and only visitor
was the Mariner 10 spacecraft, which
flew past the planet three times starting in 1974.
It gave us our first close-up look at Mercury's
baked and battered surface.
But Mariner 10's view was incomplete,
capturing less than half of the planet
during its few brief encounters.
So in 2004, NASA launched a new mission, Mercury Messenger,
whose goal is to orbit Mercury and provide
the first comprehensive survey of its geological features
and mineral composition.
At first glance, Messenger's images
seem to be showing us a desolate and moon-like world.
The surface is rough and heavily pockmarked
with craters from billions of years'
worth of meteorite impacts.
But first impressions can be deceiving.
Although Mercury is only slightly larger
than our own moon, its gravity is more than twice as strong,
which means Mercury is much more massive.
In fact, Mercury is so heavy it may be
almost entirely made of metal.
Some scientists have speculated Mercury began its existence
as a much larger planet whose exterior was mostly shattered
away in a giant collision, leaving behind
only a thin rocky mantle surrounding
a large metallic core.
Whatever happened, it's clear Mercury once
bubbled and rumbled with the internal heat
from a tumultuous formation.
Numerous features suggest a world
that was volcanically active in the distant past.
This view shows a landscape with multiple ripples underlying
the more recent impact craters.
The ripples, frozen in time, reveal
where vast pools of lava once flooded the planet's surface.
In this image, false colors help to highlight
Mercury's complex history.
Here, the bluish areas represent an ancient terrain
that was gradually buried by debris shown in orangey red.
The debris is made of material kicked up
by large crater-forming impacts blasted into Mercury's surface.
There are also giant cliffs and escarpments threading
their way among the craters.
These cliffs are a common feature on Mercury.
They may have formed when the planet's giant metal core
cooled and contracted, causing the overlying rock
to wrinkle like a planet-wide version of shrink wrap.
Messenger's first views of Mercury
reveal the bare bones of a rocky world.
There is nothing here but a solid surface
that hasn't changed very much over eons of geologic time.
While Mercury may provide the beginnings
of a stable platform, it is far too hot and barren
to be anything other than an empty stage.
To transform a dead planet into a living world,
more ingredients are needed.
First and foremost, an atmosphere.
Lack of atmosphere is not a problem for this planet.
Enigmatic Venus is the second rocky world from the sun.
Permanently shrouded under a dense, cloudy atmosphere,
Venus was hidden from astronomers for centuries,
despite being the nearest planet to Earth.
Now we know that Venus's atmosphere
is a toxic brew composed of carbon dioxide,
with clouds rich in sulfuric acid.
The carbon dioxide is brutally effective
at trapping the sun's energy, heating up
the planet to a staggering 460 degrees Celsius.
That's even hotter than Mercury, although Venus
is twice as far from the sun.
And Venus's atmosphere is incredibly dense.
The air pressure at the planet's surface
is so high it would easily crush a human astronaut to death.
These conditions are so extreme that to date,
we have only fleeting glimpses of Venus's surface taken
by a handful of Soviet landers, none of which
survived more than two hours.
With a planet so inhospitable to spacecraft,
scientists have had to come up with another way of exploring
Venus's hidden terrain from a safer distance.
Radar can penetrate the planet's thick blanket of clouds
and bounce off the rock below, providing a detailed look
at a bizarre and dramatic landscape.
What these images reveal is a world shaped by volcanoes,
and one that could still be volcanically active today.
The apparent lack of impact craters,
so different from what we see on Mercury,
is a strong indication that Venus's surface is young
and may be continually evolving.
Scientists now suspect that in the past,
Venus may have been much more like our own planet.
But as its atmosphere heated up, it
lost something vital that makes Earth
special in our solar system.
It's water.
Here on Earth, oceans have played a key role
in keeping our planet suitable for life.
Not only do oceans moderate the climate
and help keep the atmosphere stable,
they lubricate Earth's rocky surface,
so its internal heat is mainly channeled
into moving the continents slowly around the planet.
Without water, heat would build up and burst out
in vast and deadly lava flows, as may have occurred on Venus.
Most of all, oceans provide a liquid medium
where complex molecules can interact,
the preconditions scientists now believe
are necessary to turn mere chemistry into biology.
Earth is our best example of the true potential of rocky worlds.
It seems that when a planet has all three ingredients,
a solid surface, an atmosphere, and oceans of liquid water,
it can foster something new, the emergence and evolution
of life.
But while life has come to dominate Earth
with its richness and complexity,
it has also buried its tracks, making
it difficult to understand how our planet came
to be the way it is today.
That is one big reason why scientists
are so keen to explore the rest of the solar system,
now that the technology is available to do so.
It is here where we may find the clues that
will tell us what Earth was like before life appeared
and how it all happened.
It may be that only when we reach
across the ocean of space to distant rocky shores
can we truly understand our own identity.
In all of nature, there is perhaps
no view as haunting and beautiful as a full moon.
It is both familiar and mysterious,
a part of our world, yet a world unto itself.
Today, we look across at our nearest neighbor
and find not a mirror image, but an alter ego.
While Earth looks lush and colorful,
the moon is a study in black and white.
While Earth's surface is shaped by water and air
and abounds with the sounds of life,
the moon's is silent and still.
Here, no rivers run and no winds blow.
All that exists are memories of events long past,
memories of our solar system's violent beginnings,
and Earth's own tumultuous history.
For billions of years, the moon has
been the ultimate silent partner,
keeping watch over Earth from above
and keeping its secrets to itself.
That's not very satisfying to humans,
which explains why every civilization in history
has its own myth about how the moon came to exist.
But only after the invention of spaceflight
did we finally get the real story.
30 seconds.
What was it?
30 feet down, two and a half.
Picking up some dust.
Contact light.
OK, engine stop.
To date, over 50 spacecraft have now flown past, orbited,
or landed on the moon with eye-opening results.
At long last, our silent partner is beginning to reveal
its fascinating story.
When viewed up close, the moon's surface
is inundated with impact craters.
They form when small asteroids collide with the lunar surface
at high speed.
The energy from a large impact is enough
to liquefy and hollow out a crater many times
the size of the original impactor,
while throwing debris thousands of kilometers
in all directions.
Over billions of years, our planet
has experienced just as severe a beating.
But on Earth, impact craters are eroded away or buried
in sediment over time.
On the moon, they simply accumulate,
leaving a vivid and detailed record
of the hazardous nature of our solar system.
By carefully counting craters, it's
possible to tell which parts of the moon's surface
formed first and which came later.
For example, the dark patches on the moon,
we can see even from Earth, are clearly
younger than the surrounding bright areas.
In the past, astronomers named these dark patches
maria, Latin for seas.
But when explored up close, it's clear
there's never been any water on these alien shores.
Rather, the maria are vast, low-lying plains
of volcanic rock.
Long ago, these plains were covered
in hot lava that spilled out from the moon's interior
and flooded over an older landscape.
Because they are richer in iron than other parts of the moon,
they appear darker in contrast.
One of the big achievements of lunar exploration
has been the complete mapping of both sides of the moon's
surface.
The moon rotates in perfect time with its orbital period,
with one side constantly facing Earth.
Surprisingly, the two sides of the moon
turn out to be quite different from one another.
While the side that faces Earth is covered with maria,
the moon's far side exhibits much less contrast.
It's an ancient, rugged terrain interrupted only
by a few larger impact sites.
This peculiar two-sidedness has to do
with the moon's crust, which is substantially
thicker on the far side.
Scientists now suspect that billions of years ago,
when the moon's internal heat forced lava upward,
it found a shorter route to the surface on the moon's near side.
But how and when did those circular plains
form in the first place?
The surprising answer comes from the lunar samples
that were brought back by Apollo astronauts.
The samples show the lunar maria were once
the sites of enormous impacts, many of which date back
roughly 3.9 billion years.
This is very early in the solar system's history,
when space was more crowded with debris than it is today.
Nevertheless, the evidence now suggests
something exceptional happened 3.9 billion years ago,
as though a storm of asteroids suddenly swept
through the inner solar system, pummeling all of the planets
as well as our own moon.
The devastating barrage left the moon plastered
with giant circular scars.
On Earth, it was much worse.
The impacts would have vaporized oceans
and liquefied large sections of our planet's crust.
Though no animal or plant was living on Earth at the time,
it is possible microbial life had already made its debut.
When the bombardment came, perhaps only those microbes
that were dwelling far down near deep sea vents
survived to repopulate the ancient Earth
and become our distant ancestors.
The idea that the moon and Earth were both heavily bombarded
is one of the big results to come out of the samples
that astronauts returned to Earth.
An even bigger one is the astonishing revelation
that the moon itself may have once been the product
of a giant collision.
This theory is that early in our solar system's history,
an object as large as Mars once collided with Earth
and dealt our planet a staggering blow.
The collision immediately spewed out vast amounts of debris.
Much of this material found itself in orbit around Earth,
where it eventually coalesced to form a single large moon.
As incredible as it seems, this giant impact scenario
offers the best explanation for some of the moon's
more puzzling features, including its apparent lack
of an iron core.
Ironically, the moon's destructive birth
may have also been crucial to maintaining
Earth as a cradle of life, unique in our solar system.
The moon's presence helps to stabilize
the tilt of Earth's axis, preventing
climate swings that would be devastating to life
and civilization.
Because of the way it formed, the moon's past
is intimately linked with our own.
Without it, the evolution of life
may have taken a very different course.
In fact, if it weren't for the moon,
we might not even be here at all.
We've been, uh, we've landed.
That's one small step, one giant leap for mankind.
Exploring the moon has given us a remarkable window
into the past.
But the moon may also be our gateway
to a long-term future in space.
In the US, China, and elsewhere, efforts
are now underway to return humans to the lunar surface.
It is an ambitious goal, but it's also
a stepping stone along the road to more distant destinations.
Exactly where the next human mission will land
is still an open question.
But one thing is certain, there is
no shortage of interesting places on the moon
where scientists would love to visit.
The lunar South Pole would surely
be at the top of their wish list.
Here, the sun never shines on the floors of some craters.
Forever in shadow, these dark craters
should be cold enough to trap water vapor
and maybe even form lunar ice.
Although the moon is dry, the water vapor
could come from comets colliding with its surface.
Scientists have now confirmed the presence
of hydrogen in many South Polar craters, strong evidence
for the presence of ice.
If there is enough ice, it could provide lunar explorers
with much-needed water.
But finding and retrieving the ice
will be a challenging task, as it
would involve venturing into perpetually dark places.
Today, the moon presents us with an intriguing and exciting
destination in space, and a staging ground
for even more daring explorations on Mars and beyond.
Perhaps more than any other location in the solar system,
it is the moon that tells us we live
on just one world among many.
And if we are determined enough, we can one day visit them all.