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--------------------- 3792 - JAMES WEBB TELESCOPE
- SEEING FARTHER INTO THE PAST THAN EVER
BEFORE. To see the precious rare photons
from the most distant galaxies in the universe, the bigger the telescope, the
better. Space telescopes don't come
bigger than JWST, with its 21-foot (6.5 meters) primary mirror.
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- The farther a galaxy is from us, the faster
it is receding from us because of the expansion of the universe, so the more
its light becomes stretched, shifting the light toward redder wavelengths.
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- The most distant galaxies, which are also the
earliest galaxies we can see, emit light that is shifted all the way into
near-infrared wavelengths by the time it reaches Earth. It's this redshift that
prompted scientists to design JWST to specialize in near- and mid-infrared
light.
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- Prior to JWST's launch, the most distant
known galaxy was one called GN-z11. It has a redshift of 11.1, which
corresponds to seeing the galaxy as it was 13.4 billion years ago, just 400
million years after the Big Bang. That was the absolute limit of what
telescopes before JWST could detect.
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- Objects of great mass, such as galaxy
clusters, warp space with their gravity, creating a magnifying lens-like effect
that amplifies light from more distant objects. Astronomers began finding
faint, red smudges in the background of these lenses. These smudges have turned out to be the most
distant galaxies ever seen.
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First was a
galaxy at a redshift of 12.5, called GLASS-z12 (GLASS is the name of a specific
survey program, the "Grism Lens-Amplified Survey from Space"). We see
this galaxy as it existed 13.45 billion years ago, or 350 million years after
the Big Bang.
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- Galaxies with even greater redshifts soon
followed. One, nicknamed Maisie's Galaxy, is seen as it existed just 280
million years after the Big Bang, at a redshift of 14.3, while another, at
redshift 16.7, is seen just 250 million years after the Big Bang. There have
even been claims for a galaxy at an astounding redshift of 20, which if
confirmed would have existed just 200 million years after the Big Bang.
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- DISCOVERING WHAT LIT UP THE UNIVERSE. Following the Big Bang, but before stars and
galaxies had formed, the universe was dark and shrouded in a fog of neutral
hydrogen gas. Ultimately light, particularly ultraviolet radiation, ionized
that fog. But where did that light initially come from to end the cosmic dark
ages?
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- Astronomers believe that light came either
from young galaxies filled with stars, or from active supermassive black holes,
which are surrounded by accretion disks of brilliantly hot gas and shoot
powerful jets into space
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- This characteristic suggests that
fully-formed galaxies were on the scene quickly, but whether they already
contained supermassive black holes remains to be seen.
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- JWST MEASURES EXOPLANET ATMOSPHERE. Astronomers have now found more than 5,000
exoplanets and counting, but despite this remarkable haul, we still know next
to nothing about many of them.
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- When a planet passes in front of its star,
some of the star's light filters through the planet's atmosphere, and molecules
in the atmosphere can absorb some of that starlight, creating dark lines in the
star's spectrum, a barcode-like breakdown of light by wavelength. Knowing
what's in a planet's atmosphere, or even whether it has an atmosphere at all, can
teach astronomers about how a planet might have formed and evolved, what its
conditions are like and what chemical processes are taking place in that
atmosphere.
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- In August, 2022, astronomers announced
that JWST had made the first confirmed detection of carbon dioxide gas in the
atmosphere of an exoplanet, in this case WASP-39b, which is 700 light
years-away.
- Later, in November, astronomers released a
more complete spectrum showing the absorption lines of elements and molecules
in WASP-39b's atmosphere, including not only carbon dioxide but also carbon
monoxide, potassium, sodium, sulfur dioxide and water vapor.
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- The spectrum showed that there was a lot
more oxygen in the planet's atmosphere than carbon, as well as an abundance of
sulfur. Scientists think that sulfur must have come from numerous collisions
that WASP-39b experienced with smaller planetesimals when it was forming,
giving us clues to the planet's evolution that could also hint at how the gas
giants in our own solar system, Jupiter and Saturn, formed.
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- In addition, the existence of sulfur dioxide
is the first example of a product of photochemistry on a planet beyond the
solar system, since the compound forms when a star's ultraviolet light reacts
with molecules in a planetary atmosphere.
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- WEBB SEARCHES FOR HINTS OF LIFE AND
HABITABILITY. The planets of the
TRAPPIST-1 system of seven rocky planets orbiting a red dwarf star located 40.7
light-years away from Earth. Four of these worlds lie in the star's putative
habitable zone, where temperatures would permit liquid water to persist on the
surface; given the right conditions they could potentially be habitable to
varying degrees.
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- Models predict that TRAPPIST-1c will have
an atmosphere similar to Venus, with lots of carbon dioxide. While TRAPPIST-1c
is likely too hot to be habitable, determining whether it has an atmosphere
and, if so, whether that atmosphere possesses carbon dioxide will be a big step
toward characterizing Earth-size worlds.
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- It will also be a big task, requiring 100
hours of observing time with JWST, which is tackling about 10,000 hours of
observations during its first year of science.
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- JWST is targeting the other worlds in the
TRAPPIST-1 system that are more likely to be habitable, as well as similar
worlds around other nearby stars. Astronomers will be on the lookout for
biosignatures, such as the presence of both methane and oxygen in an
atmosphere.
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- The discovery of photochemical reactions in
WASP-39b's atmosphere is also an important step, since photochemical reactions
drive the formation of the carbon-based molecular building blocks of life.
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- JWST STUDIES COSMIC CHEMISTRY & GALAXY
EVOLUTION. Some stars live for billions
upon billions of years, but others exist for just a short time before either
exploding in a supernova or expanding to become a red giant that then puffs off
its outer layers into deep space. In both situations, the stars disperse large
amounts of cosmic dust formed from elements heavier than hydrogen and helium
across space.
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- It turns out that there is a relationship
between a galaxy's mass, its star-formation rate and its chemical abundances.
Deviations from this relationship at high redshift might indicate that galaxies
evolved differently in the early universe.
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- Prior to JWST, astronomers could only
reliably measure the abundances of various elements in galaxies up to a
redshift of 3.3; in other words, galaxies that existed about 11.5 billion years
ago. But how abundant these heavy elements were in galaxies earlier than this
is a bit of a mystery.
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- Early results from JWST have shown that the
relationship between star formation and mass does hold for galaxies at
redshifts as high as 8, but that their abundance of heavier elements is three
times lower than expected. This discrepancy suggests that stars and galaxies
formed more quickly than we realized, before enough generations of stars had
the chance to die out and disperse their elements into the cosmos.
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- JWST SETS ITS SIGHTS ON THE SOLAR
SYSTEM. Brilliant Jupiter, its faint
rings and several of its small moons imaged by JWST.
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- Astronomers were not sure what to expect
when JWST pointed at Jupiter because of how fast it moves and how bright the
planet is compared to the faint distant galaxies JWST usually observes.
Scientists worried that Jupiter might overload JWST's sensitive detectors or
wipe out fainter features with its glare, but the results were better than
could be imagined.
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- JWST's images showed Jupiter's faint rings
and some of its small moons, as well as the planet's atmospheric bands and
auroras. By observing in near- and mid-infrared light, with the high resolution
that JWST's giant mirror provides, astronomers are able to peer deeper into
Jupiter's atmosphere to see what's going on beneath the cloud tops and learn
how deeply the clouds extend.
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- JWST has also imaged faraway Neptune,
Saturn's moon Titan and Mars. While JWST's portrait of the Red Planet shows
temperature variations on Mars' surface and absorption by carbon dioxide in its
atmosphere. In the future, JWST will observe Mars to track more tenuous gases,
such as mysterious seasonal plumes of methane that could originate in either
geological or biological activity.
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- One of the Hubble Space Telescope's most
iconic images was that of the Pillars of Creation, columns of molecular gas
many light-years long found in the Eagle Nebula. Those columns are cosmic
nurseries where stars are born. JWST has revisited the Pillars of Creation, and
the resulting images in near- and mid-infrared light are just as special as the
original.
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- JWST's infrared vision is able to penetrate
through the dust in the Pillars to gain a better view of the star formation
going on inside, showing knots of molecular gas on the verge of collapsing into
nascent stars. When those stars are just a few hundred thousand years old, they
begin to shoot out jets that erode the edges of the Pillars.
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- JWST CHANGED HOW SPACE TELESCOPES ARE
BUILT. JWST's massive, golden primary
mirror, formed by unfolding 18 hexagonal segment, was brand-new engineering to
permit a telescope of such great size to be launched into space.
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- JWST was launched on December 25, 2021, the
$10 billion infrared observatory was designed
to learn how galaxies form and grow, to peer far back into the universe to the
era of the first galaxies, to watch stars be born inside their nebulous embryos
in unprecedented detail, and to probe the atmospheres of exoplanets and
characterize some of the closest rocky worlds.
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- However, the complexity of the James Webb
Space Telescope (Webb or JWST), including its fold-out, segmented 21-foot (6.5
meters) mirror and its delicate sun-shield the size of a tennis court.
- The James Webb Space Telescope launched atop
an Ariane 5 rocket from French Guiana on Dec. 25, 2021.
The main reason
that JWST is performing so well is because of its superlative optics, which are
able to achieve their maximum potential resolution for the majority of infrared
wavelengths that the telescope observes in. This success means that JWST's
images have a clarity to them that were unobtainable by the likes of the Hubble
Space Telescope and NASA's retired Spitzer Space Telescope, or larger
telescopes on the ground such as those at the Keck Observatory in Hawaii, whose
vision is blurred by Earth's atmosphere.
But with JWST,
individual stars so close together they were once indistinguishable can now be
resolved; the structures of very distant galaxies are now discernible; and even
something close by such as the rings of Neptune pop with the most detail seen
in decades.
The James Webb
Space Telescope's stunning view of Neptune, with its rings clearly visible.
The James Webb
Space Telescope's stunning view of Neptune, with its rings clearly visible.
(Image credit: NASA/ESA/CSA/STScI)
"When the
JWST's images of Neptune first came out, both Heidi [Hammel, an
interdisciplinary scientist on JWST and an expert on the outer planets of the
solar system] and myself looked at them, and then at each other, and asked,
'are we really looking at Neptune'?" Naomi Rowe-Gurney, an astronomer at
NASA Goddard Space Flight Center in Maryland, told Space.com.
Although the Keck
Observatory has imaged Neptune's rings, our most impressive view before JWST
came from Voyager 2's flyby in 1989. "Heidi had not seen the rings [this
well] since Voyager 2, and I had never seen the rings like this because Voyager
was before I was born!" Rowe-Gurney said.
Normally, faint
details or features around a bright object, such as the dark and tenuous rings
around blue Neptune, are difficult to see against the glare of the bright
object. To counteract this, an instrument is required to have the
characteristic of "high dynamic range" to take in both the faint and
the bright at the same time.
"We didn't
realize that JWST would have this amazing dynamic range and be able to resolve
really faint things like the rings of Neptune and the small moons and rings of
Jupiter," Rowe-Gurney said.
Alien atmospheres
It's not only the
planets of our solar system that JWST is scrutinizing. A key aim of the
telescope is to detect the composition of exoplanets' atmospheres using a
technique called transmission spectroscopy. As a planet transits its star, the
star's light shines through the planet's atmosphere, but atoms and molecules
within that atmosphere can block some of the light at characteristic
wavelengths, which gives away the composition of the atmosphere.
The first
exoplanet result released from JWST was the transmission spectrum of WASP-39b,
which is a "hot Jupiter" exoplanet orbiting a sun-like star located
700 light-years away. JWST detected carbon dioxide in WASP-39b's atmosphere,
the first time the gas has ever been detected on an exoplanet. Other gases present
included carbon monoxide, potassium, sodium, water vapor and sulfur dioxide,
the last of which can only be created through photochemistry when atmospheric
gases react with the ultraviolet light from the planet's star — another
exoplanet first.
The James Webb
Space Telescope's analysis of the atmospheric composition of WASP-39b.
The James Webb
Space Telescope's analysis of the atmospheric composition of WASP-39b. (Image
credit: NASA/ESA/CSA/J. Olmsted (STScI))
"I keep
being amazed by what we're able to do with the exoplanet data, like the carbon
dioxide and the photochemistry that was found in the atmosphere of
WASP-39b," Mullally said. "That was really cool, and I don't remember
people talking about [detecting photochemistry] ahead of time. I'm really
looking forward to seeing what we can do with the terrestrial exoplanets
orbiting the cool M-dwarfs and seeing what their atmospheres are made of."
In particular,
the TRAPPIST-1 planetary system of seven worlds orbiting an M-dwarf 40
light-years away is a key target of the JWST. Preliminary results, which failed
to detect thick blankets of hydrogen surrounding some of the TRAPPIST-1 worlds,
were released during a conference held at STScI in December, but we'll have to
be patient for more comprehensive results from these planets, of which up to
four could reside in their star's habitable zone.
WASP-39b was an
easy first target because its star is bright and the planet's signal is strong.
M-dwarfs like TRAPPIST-1 are much fainter, despite being closer.
"We have to
wait until we can get enough transits of these guys to build up the
signal-to-noise, because you can't do it with just one or two transits,"
Mullally said. "I think we're going to have to wait until at least the end
of the cycle 1 observations [summer 2023] before anybody is going to be in a
position to say if they've found anything really spectacular."
Star formation
near and far
Another aspect of
JWST's mission is to not only observe exoplanets, but to better understand how
they, and their stars, form. Star formation in particular is a crucial process
to understand it because it connects so many things in the universe both near
and far.
Longmore is
leading a study to use JWST to observe frantic star formation in a region at
the center of our own Milky Way galaxy, called the central molecular zone, some
26,000 light-years from us. The center of our galaxy hosts the highest
concentration of stars, and at our distance they all appear packed in —
indistinguishable to the likes of the Hubble Space Telescope — while copious
amounts of dust shroud most of them from view in optical light. Look with a
large-aperture infrared telescope like JWST, however, and those two concerns
are shoved aside.
"These are
the JWST's two capabilities that are going to blow my field apart,"
Longmore said. The telescope's superb optics are able to resolve individual
baby stars in the center of the galaxy, and infrared light will pass right
through the dust to reach the observatory.
"Ordinarily,
with Hubble, it's like trying to point your telescope at a brick wall and see
through it," he added, "But the JWST is looking through a window in
that wall and can count individual stars."
The star-forming
Pillars of Creation, imaged in mid-infrared by the JWST in what will surely
become an iconic picture.
The star-forming
Pillars of Creation, imaged in mid-infrared by the JWST in what will surely
become an iconic picture. (Image credit: NASA/ESA/CSA/STScI/J. DePasquale
(STScI)/A. Pagan (STScI))
It's taking
longer to gather all the data from the center of the galaxy, but that's because
it's such a complex environment, with bright, diffuse emission everywhere, and
all that has to be disentangled from the relevant signal of star formation via
determined and careful data processing.
"On all the
projects I'm on, people are still fighting with calibration and things, but
hopefully in the next six months that will change," Longmore said. He
added an amusing story of how one of his team's observations had been blighted
by a mysterious circle on the image. After deeper investigation, it turned out
that this wasn't some mysterious new phenomenon, but that JWST had previously
been looking at bright Jupiter, and the giant planet's after-image had not yet
been properly flushed out of the instrument's electronic sensors!
Longmore and his
colleagues are targeting the central molecular zone because it is the region in
our galaxy that most resembles star-forming conditions in the early universe,
when the star-formation rate was high and dense clusters of stars formed. In
the Central Molecular Zone, the astronomers intend to measure a property called
the initial mass function (IMF), which describes the range of stellar masses in
a star-forming nebula.
Currently,
astronomers do not understand what determines why stars form with the masses
that they have, only that low-mass stars are much more common than luminous
high-mass stars, at least in the local universe. Was this still the case over
13 billion years ago in the first galaxies? Answering that question could help
explain both how galaxies formed and what ended the universe's dark ages.
Deep fields and
the first galaxies
After she saw
President Joe Biden reveal the first deep-field image from the JWST, of the
galaxy cluster SMACS 0723, a "gravitational lens" whose massive
gravity magnifies objects behind it, Frye and her student, Massimo Pascale at
the University of California, Berkeley, raced to analyze the image.
"We didn't
sleep for three-and-a-half days, and our paper was one of the first two papers
submitted on JWST data," Frye said.
Together, they
found 42 new gravitationally lensed images of 14 different high-redshift
galaxies, galaxies located so far away that the expanding universe has
stretched their light, making them appear redder. Further studies and more deep
fields followed, and a host of high-redshift candidates were discovered by
Frye's team and others, including some galaxies at record-breaking redshifts of
12, 13 and above; these redshifts mean that we see the galaxies as they existed
less than 300 million years after the Big Bang.
These
high-redshift galaxies have proven something of a surprise, in that they appear
more luminous than models of galaxy formation predicted they should be.
"One
possible explanation is that they're producing too many high-mass stars, that
they have a top-heavy IMF," Longmore said, noting the importance of
measuring the IMF in the central molecular zone to understand stellar masses in
young neighborhoods.
Why the IMF would
be different over 13.5 billion years ago is not understood, but then again the
early universe seems to have been a far more intense place than it is today.
"In the present day, galaxies in general are not forming stars so
actively, but many galaxies formed stars more actively in the early
universe," Frye said.
Frye is a member
of the PEARLS (Prime Extragalactic Area for Reionization and Lensing Science)
team. PEARLS is a JWST project to image a variety of deep fields, including two
apparently sparse regions of sky and a number of galaxy clusters and
proto-clusters, to observe the first few billion years of galaxy formation.
The PEARLS field
looking toward the North Celestial Pole. Inset are numerous types of galaxy,
from interacting galaxies to ruby-red dusty star-forming galaxies.
The PEARLS field
looking toward the North Celestial Pole. Inset are numerous types of galaxy,
from interacting galaxies to ruby-red dusty star-forming galaxies. (Image
credit: NASA/ESA/CSA/Rolf A. Jansen, Jake Summers, Rosalia O'Brien, Rogier
Windhorst (ASU)/Aaron Robotham (UWA)/Anton M. Koekemoer (STScI)/Christopher
Willmer (University of Arizona)/JWST PEARLS Team)
In December, the
PEARLs team released their first dataset, of an extraordinary field of distant
galaxies close to the North Ecliptic Pole. This region is directly above the
main plane of the Milky Way and so is constantly visible to JWST, and it's also
high above interfering features such as zodiacal dust.
Within the image
are a whole host of galaxies. Some interact and some show a clear spiral
structure; the collection exhibits a whole range of colors, from cobalt blue to
ruby red. The latter are of great interest to Frye.
"We can now
observe [in the PEARLS image] an abundance of red disk galaxies, which we think
might be red spirals," Frye said. "This type of galaxy is very
interesting because they are analogs of what the Milky Way might have looked
like when it was younger."
The reddening is
caused by huge amounts of dust in these galaxies; the dust is the result of
rapid formation of massive stars that quickly die in supernova explosions and
spill vast amounts of dust into space. Such galaxies are completely hidden from
Hubble, but infrared light can pass through the dust and make the galaxies
visible to JWST.
"The analogy
is a New Year's Eve fireworks display," Frye said. "If you have a lot
of fireworks going off then eventually they are obscured by dusty smoke."
RELATED STORIES:
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— James Webb
Space Telescope's iconic image reveals a stellar surprise
The JWST has
impressed scientists in the six months that it has been gathering data since
becoming fully operational in June, but the real fireworks are still to come
with major discoveries awaiting us.
It's slow going,
requiring patience, Frye said. "There's too much for any one person to be
able to study or understand on really short timescales, it's going to take us a
long time to process all the data."
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December 24,
2022 3797
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--- Thursday, December 29,
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