All language subtitles for The.New.Frontier.S02E08.First.Light.1080p.NF.WEB-DL.DDP2.0.x264-NTb_track3_[eng]

For an instrument first
developed as recently as the 17th century,

the telescope has travelled a long way.

The latest version of the once humble
telescope will be going a lot farther.

Carrying us ever closer to the first light
that ever bathed the universe

in which we live.

Generational change
is part and parcel of our lives.

In terms of space exploration,

the Hubble Space Telescope
has been doing its extraordinary work

for a generation now.

And it's time to hand over the reins.

What we've reached is the limit
of Hubble's vision.

As amazing as Hubble has been,

we've come up against
the immutable reality

that Hubble can't,
in fact, see everything.

Galileo, Herschel, Hubble:

our knowledge of space
is marked by some of the greatest names

in the human history of stargazing.

But who was James Webb?

His name is attached
to the James Webb Space Telescope,

which will soon be helping us understand

what lies beyond
even the amazing reach of Hubble.

Originally called
the Next Generation Space Telescope,

Hubble's successor was renamed in 2002
to honor James E. Webb,

who ran NASA
from February 1961 to October 1968.

Those dates, of course, put Webb at
the heart of the American space program,

and the moon landing in particular.

But that was not
Webb's sole preoccupation.

Webb's energy
encompassed robotic spacecraft,

probes to Mars and Venus

and, in 1965,
his advocacy of a Large Space Telescope.

He was, in other words, a man of vision.

The James Webb Space Telescope
is nearing completion,

in readiness for a scheduled launch
in October 2018.

By a happy coincidence, exactly 50 years
since James Webb's tenure at NASA ended.

Its aim is modest: to study every
phase in the history of the universe.

Several major agencies have collaborated

in the creation of
the James Webb Space Telescope.

NASA's Goddard Space Flight Center
is at the hub.

ESA will provide the launch vehicle,
the ultra-reliable Ariane 5 rocket.

Canada's Space Agency is involved,

as is the Space Telescope
Science Institute,

while Northrop Grumman
is the chief contractor.

The Webb will be
wonderful for the astronomy community.

Not only will it give them the kinds
of wonderful resolution

we have with Hubble
that you can get above the atmosphere,

but it's gonna bring them access
to a wave length region

where many of them
have not worked before.

We have
a telescope that's far more powerful

than anything that we have had before,

working at infrared wavelengths,
which you can't see well from the ground.

And that will enable us to see things
from the most distant universe

that we can only guess at

to things at the outer solar system
that we can only guess at.

The Webb is gonna be
such a powerful telescope.

It's going to be like the Hubble

and, in the case of the Hubble,

probably more than half
of the greatest observations,

discoveries that the Hubble made,
were things that people didn't anticipate.

I expect the same for the Webb.

The James Webb Space
Telescope's mission duration

is a planned 10 years,

during which it has a number
of specific goals to accomplish.

It will search for the first galaxies,

determine how galaxies were formed, observe the formation of stars,

and measure the properties
of planetary systems,

both physical and chemical,
including our own Solar System.

Not least of all,
the Webb will carry on the task

that underlies so much
of humankind's activity in space:

investigating the potential
for life in other far-flung places.

The 6,200 kilogram space-based element
of the Webb will not orbit Earth,

as Hubble has been doing.

Instead it will orbit the Sun.

To do so it must first travel
1.5 million kilometers,

a 30-day journey to L2,

the Lagrangian point at which
the gravitational forces of Sun and Earth

are roughly equivalent.

Each orbit will take six months

and keep the JWST out of the shadow
of both Earth and Sun.

Its trajectory also makes
24/7 communications possible.

The Webb will stay in line with Earth
as it moves around the Sun.

And that is because,

while the James Webb Space Telescope
is looking for first light,

its first task is to find darkness:

the condition
in which it can operate at its best.

Three main component systems

make up the space-based
James Webb Space Telescope:

an Integrated Science Instrument Model,
ISM,

the Optical Telescope Element, OTE,

and the Spacecraft element.

The key to the JWST's enhanced vision
is its primary mirror,

which measures 6.5 meters across.

It comprises 18 segments
made of beryllium,

the lightest of the alkaline earth metals.

A five-layer sunshield
the size of a tennis court

will protect the JWST's
dazzling array of specialist technology.

As this orbiting infrared observatory
continues the work begun by Hubble.

On board are a near-infrared camera,
a near-infrared spectrograph,

a mid-infrared instrument,
a near-infrared imager,

and a slitless spectrograph.

The NIRSpec has microshutters

which will make it possible to observe
up to 100 objects simultaneously.

The Webb's cameras and spectrometers

are capable of detecting
extremely faint signals,

a crucial factor in its attempt
to see as far back as first light.

While NASA busies
itself with James Webb,

its European counterpart, ESA, is
hard at work on another, related mission

with a much more famous name
attached to it.

Euclid is named for the Alexandrian Greek
whose geometrical study, the elements,

formed the basis of our mathematical
thinking for almost two millennia.

What we want is, actually,
to continue our successful program

which is actually providing
the cutting edge space science,

meeting the challenges
of worldwide research.

But where the original
Euclid worked only with ruler and compass,

his namesake in space will have much more
sophisticated instruments in its locker.

Like the Webb,
Euclid boasts a modest mission:

to map the geometry
of the dark universe.

Over a period of some six years
it will look back over the entire time

in which dark energy has contributed
to the accelerating expansion

of the universe.

Scientists tell us that what we can see

accounts for less than
5% of what is there.

The rest is made up of dark matter,
some 20%,

and the remainder, of dark energy.

They act in contradictory ways.

Dark matter acts through gravity
to play its role in forming galaxies

and slowing the rate of expansion
of the universe.

Dark energy, on the other hand,
defeats gravity

and thus encourages acceleration
of that expansion.

The Euclid Consortium,
part of ESA's "Cosmic Vision" program,

brings together 1,000 scientists
from 100 institutes in 14 countries,

with added input from NASA
in the United States.

In 2013 Italy's Thales Alenia Space group
was named as prime contractor,

with Airbus in France
responsible for the payload module.

On board Euclid's payload module

will be a telescope 1.2 meters
in diameter,

a visible light camera and a near-infrared
camera and spectrometer.

Euclid will undergo
its critical design review in 2017,

with its launch planned for December
2020 from Kourou in French Guiana.

Like the JWST,
it will orbit around the L2 point.

Channeling the thinker
whose name it bears,

Euclid will be looking for genuine insight
into the evolution of cosmic structures.

Investigating the nature of dark energy,
dark matter and gravity,

it will track their observational
signatures on the geometry of the universe

and on the cosmic history
of structure formation.

Euclid will deploy two key systems:

weak gravitational lensing, or WL,
and baryonic acoustic oscillations, BAO.

WL examines how background galaxies
are disturbed by foreground dark matter,

and measures modifications
in the shape of galaxies

brought on by
the gravitational lensing of dark matter.

BAO reveals the wiggle patterns

which help us gauge
the expansion of the universe,

revealing the three-dimensional
distribution of structures

by means of the spectroscopic redshifts
of galaxies and galaxy clusters.

Putting it more simply, perhaps,

Euclid's task, made easier by
its unprecedented accuracy and stability,

is to map the shape, position
and movements of two billion galaxies,

or one-third of the sky.

Even more excitingly,
JWST is not the only star performer,

pardon the pun, on the horizon.

In 2016 NASA confirmed
the decision to go ahead

with its Wide Field Infrared
Survey Telescope, or WFIRST for short.

WFIRST is a NASA
observatory that has the top ranking

of the National Academy of Sciences
to launch in the 2020's.

It has the same image precision
and power as the Hubble space telescope

but with 100 times
the area of sky that it views.

Looking at
a large fraction of the sky

allows you to get
a more complete accounting,

for example, the stars
in the Large Magellanic Cloud,

which is the nearest galaxy to us,

or the stars in the Galactic Bulge.

So, you can do
a much more complete accounting

in a much shorter amount of time.

This new observatory will offer
astrophysicists the best of both worlds

by casting its eye both wide and deep
as it seeks to shed light on dark energy,

exoplanets and cosmic acceleration.

Surveying large areas
in near-infrared light,

a single image from WFIRST
will have all the depth and sharpness

to which Hubble has accustomed us,

but will cover 100 times the area.

In fact a single image will encompass
as many as a million galaxies.

The new telescope's work
will slip into the groove

already made by Kepler,
the Sloan Digital Survey

and TESS,
the Transit Exoplanet Survey Satellite.

WFIRST will use microlensing rather
than the transit method of detection.

It will employ
a 2.4m diameter telescope

provided by
the National Reconnaissance Office,

but the best-of-both-worlds part
of the WFIRST story

comes with the coronagraph

which NASA has been able
to add to its instrumental array.

This is a means of dimming
the light from a so-called host star

in order to see better the planet
or planets orbiting it.

And that is highly significant
if we remember that the host star

may be up to a billion times brighter
than any exoplanet identified.

If successful, the coronagraph technique
will make it much easier

to determine the chemical composition
of planetary atmospheres.

WFIRST will be able to use
a unique deformable telescope

controlled by computer.

This first mission,
due for launch in the mid-2020's,

being what is called
a technology demonstration,

laying down a scientific marker

for future missions
to go in even more determined pursuit

of life beyond the confines
of our own Solar System.

While all of this is going on in space,

here on Earth another agency will be
tackling the question of dark matter

from yet another angle.

At CERN in Geneva,

the Large Hadron Collider is now running
at full power for the first time.

The very exciting
and intriguing possibility

that in addition to gravity
there might be a new force

between our visible matter and dark matter

which is transmitted
by a new photon-like particle,

which we call dark photons
or heavy photon or para-photons,

there are many different names
for this particle.

This experiment, its apparatus,
which is about 30 meters long,

and the main idea is that we search for
so-called invisible decay of dark photons,

and these particles could be quite light,
below 1 GeV.

And what is most important

that these particles could be searched
for at low energy experiment.

With fixed-target experiment.

So what you see here

is the beam pipe
where the beam is coming.

The electrons are deflected
by two magnets,

which are about 50 meters upstream.

The purpose of that
is really we need to be sure

that we get here are electron of 100 GeV.

So, in this magnet
when the electrons are deflected

you generate synchrotron radiation,

and this we detect
with this detector here.

So, the idea
is when the high energy electron

collide with the active target,
which is electro-magnetic colorimeter,

it creates, in this high energy collision
with a nuclei,

create dark photons
which carry away from the setup...

a significant fraction
of the primary energy.

So the experimental signature
of the existence of a prime

is an event with such missing energy,

and we search
for this event with this setup.

Might its scientists be able
to replicate dark matter itself?