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10 times Webb telescope blew us away with images of universe

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10 times Webb telescope blew us away with images of universe

It is no exaggeration to say the James Webb Space Telescope (JWST) represents a new era for modern astronomy.

Launched on December 25 last year and fully operational since July, the telescope offers glimpses of the universe that were inaccessible to us before. Like the Hubble Space Telescope, the JWST is in space, so it can take pictures with stunning detail free from the distortions of Earth’s atmosphere.

However, while Hubble is in orbit around Earth at an altitude of 540km, the JWST is 1.5 million kilometres distant, far beyond the Moon. From this position, away from the interference of our planet’s reflected heat, it can collect light from across the universe far into the infrared portion of the electromagnetic spectrum.

This ability, when combined with the JWST’s larger mirror, state-of-the-art detectors, and many other technological advances, allows astronomers to look back to the universe’s earliest epochs.

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The Carina star-forming region imaged by the JWST. NASA

As the universe expands, it stretches the wavelength of light travelling towards us, making more distant objects appear redder. At great enough distances, the light from a galaxy is shifted entirely out of the visible part of the electromagnetic spectrum to the infrared. The JWST is able to probe such sources of light right back to the earliest times, nearly 14 billion years ago.

The Hubble telescope continues to be a great scientific instrument and can see at optical wavelengths where the JWST cannot. But the Webb telescope can see much further into the infrared with greater sensitivity and sharpness.

Let’s have a look at ten images that have demonstrated the staggering power of this new window to the universe.

1. Mirror alignment complete

A bright six-pointed orange star with text above it stating it's a telescope alignment evaluation image. Inset in the top right corner shows a red blob with two pointsA bright six-pointed orange star with text above it stating it's a telescope alignment evaluation image. Inset in the top right corner shows a red blob with two points
Left: The first publicly released alignment image from the JWST. Astronomers jumped on this image to compare it to previous images of the same part of sky like that on the right from the Dark Energy Camera on Earth. NASA/STScI/LegacySurvey/C. Jacobs

Despite years of testing on the ground, an observatory as complex as the JWST required extensive configuration and testing once deployed in the cold and dark of space.

One of the biggest tasks was getting the 18 hexagonal mirror segments unfolded and aligned to within a fraction of a wavelength of light. In March, NASA released the first image (centred on a star) from the fully aligned mirror. Although it was just a calibration image, astronomers immediately compared it to existing images of that patch of sky – with considerable excitement.

2. Spitzer vs MIRI

Two orange images showing a series of bright dots - the left one is much fuzzier than the right oneTwo orange images showing a series of bright dots - the left one is much fuzzier than the right one
This image shows a portion of the ‘Pillars of Creation’ in the infrared (see below); on the left taken with the Spitzer Space Telescope, and JWST on the right. The contrast in depth and resolution is dramatic. NASA/JPL-Caltech (left), NASA/ESA/CSA/STScI (right)

This early image, taken while all the cameras were being focused, clearly demonstrates the step change in data quality that JWST brings over its predecessors.

On the left is an image from the Spitzer telescope, a space-based infrared observatory with an 85cm mirror; the right, the same field from JWST’s mid-infrared MIRI camera and 6.5m mirror. The resolution and ability to detect much fainter sources is on show here, with hundreds of galaxies visible that were lost in the noise of the Spitzer image. This is what a bigger mirror situated out in the deepest, coldest dark can do.

3. The first galaxy cluster image

Two images of hundreds of dots of light on a dark background, with more visible on the right hand sideTwo images of hundreds of dots of light on a dark background, with more visible on the right hand side
SMACS 0723 galaxy cluster – from Hubble on the left, and JWST on the right. Hundreds more galaxies are visible in JWST’s infrared image. NASA/STSci

The galaxy cluster with the prosaic name of SMACS J0723.3–7327 was a good choice for the first colour images released to the public from the JWST.

The field is crowded with galaxies of all shapes and colours. The combined mass of this enormous galaxy cluster, over 4 billion light years away, bends space in such a way that light from distant sources in the background is stretched and magnified, an effect known as gravitational lensing.

These distorted background galaxies can be clearly seen as lines and arcs throughout this image. The field is already spectacular in Hubble images (left), but the JWST near-infrared image (right) reveals a wealth of extra detail, including hundreds of distant galaxies too faint or too red to be detected by its predecessor.

4. Stephan’s Quintet

Side-by-side images of four large, luminous circles with thousands of stars in the background and within; the left side has more brightness and sharpnessSide-by-side images of four large, luminous circles with thousands of stars in the background and within; the left side has more brightness and sharpness
Hubble (l) and JWST (r) images of the group of galaxies known as ‘Stephan’s Quintet’. The inset shows a zoom-in on a distant background galaxy. NASA/STScI

These images depict a spectacular group of galaxies known as Stephan’s Quintet, a group that has long been of interest to astronomers studying the way colliding galaxies interact with one another gravitationally.

On the left we see the Hubble view, and the right the JWST mid-infrared view. The inset shows the power of the new telescope, with a zoom in on a small background galaxy. In the Hubble image we see some bright star-forming regions, but only with the JWST does the full structure of this and surrounding galaxies reveal itself.

5. The Pillars of Creation

Two side-by-side images of finger-like protrusions on a multicoloured starry background, wth more detail visible on the rightTwo side-by-side images of finger-like protrusions on a multicoloured starry background, wth more detail visible on the right
The ‘Pillars of Creation’, a star-forming region of our galaxy, as captured by Hubble (left) and JWST (right). NASA, ESA, CSA, STScI; Joseph DePasquale (STScI), Anton M. Koekemoer (STScI), Alyssa Pagan (STScI)

The so-called Pillars of Creation is one of the most famous images in all of astronomy, taken by Hubble in 1995. It demonstrated the extraordinary reach of a space-based telescope.

It depicts a star-forming region in the Eagle Nebula, where interstellar gas and dust provide the backdrop to a stellar nursery teeming with new stars. The image on the right, taken with the JWST’s near-infrared camera (NIRCam), demonstrates a further advantage of infrared astronomy: the ability to peer through the shroud of dust and see what lies within and behind.

6. The ‘Hourglass’ Protostar

An orange-and-blue hourglass shape on a dark background, with a blurrier blue image of the same shape in the upper cornerAn orange-and-blue hourglass shape on a dark background, with a blurrier blue image of the same shape in the upper corner
The ‘hourglass protostar’, a star still in the process of accreting enough gas to begin fusing hydrogen. Inset: A much lower resolution view from Spitzer. NASA/STScI/JPL-Caltech/A. Tobin

This image depicts another act of galactic creation within the Milky Way. This hourglass-shaped structure is a cloud of dust and gas surrounding a star in the act of formation – a protostar called L1527.

Only visible in the infrared, an “accretion disk” of material falling in (the black band in the centre) will eventually enable the protostar to gather enough mass to start fusing hydrogen, and a new star will be born.

In the meantime, light from the still-forming star illuminates the gas above and below the disk, making the hourglass shape. Our previous view of this came from Spitzer; the amount of detail is once again an enormous leap ahead.

7. Jupiter in infrared

A turqoise and blue banded sphere with bright orange patches of light at both polesA turqoise and blue banded sphere with bright orange patches of light at both poles
An infrared view of Jupiter from the JWST. Note the auroral glow at the poles; this is caused by the interaction of charged particles from the sun with Jupiter’s magnetic field. NASA/STScI

The Webb telescope’s mission includes imaging the most distant galaxies from the beginning of the universe, but it can look a little closer to home as well.

Although JWST cannot look at Earth or the inner Solar System planets – as it must always face away from the Sun – it can look outward at the more distant parts of our Solar System. This near-infrared image of Jupiter is a beautiful example, as we gaze deep into the structure of the gas giant’s clouds and storms. The glow of auroras at both the northern and southern poles is haunting.

This image was extremely difficult to achieve due to the fast motion of Jupiter across the sky relative to the stars and because of its fast rotation. The success proved the Webb telescope’s ability to track difficult astronomical targets extremely well.

8. The Phantom Galaxy

Three similar images of spiral galaxy in different colours, with the middle one providing the most detailThree similar images of spiral galaxy in different colours, with the middle one providing the most detail
Hubble visible light (l), JWST infrared (r) and combined (middle) images of the ‘Phantom Galaxy’ M74. The ability to combine visible light information about stars with infrared images of gas and dust allow us to probe such galaxies in exquisite detail. ESA/NASA

These images of the so-called Phantom Galaxy or M74 reveal the power of JWST not only as the latest and greatest of astronomical instruments, but as a valuable complement to other great tools. The middle panel here combines visible light from Hubble with infrared from Webb, allowing us to see how starlight (via Hubble) and gas and dust (via JWST) together shape this remarkable galaxy.

Much JWST science is designed to be combined with Hubble’s optical views and other imaging to leverage this principle.

9. A super-distant galaxy

Side by side images of a black background with many small galaxies of various shapes glowing faintlySide by side images of a black background with many small galaxies of various shapes glowing faintly
A ‘zoom in’ on a galaxy from one of the universe’s earliest epochs, when the universe was only about 300 million years old (the small red source visible in the centre of the right panel). Galaxies at this distance are impossible to detect in visible light as their emitted radiation has been ‘redshifted’ far into the infrared. NASA/STScI/C. Jacobs

Although this galaxy – the small, red blob in the right image – is not among the most spectacularly picturesque our universe has to offer, it is just as interesting scientifically.

This snapshot is from when the universe was a mere 350 million years old, making this among the very first galaxies ever to have formed. Understanding the details of how such galaxies grow and merge to create galaxies like our own Milky Way 13 billion years later is a key question, and one with many remaining mysteries, making discoveries like this highly sought after.

It is also a view only the JWST can achieve. Astronomers did not know quite what to expect; an image of this galaxy taken with Hubble would appear blank, as the light of the galaxy is stretched far into the infrared by the expansion of the universe.

10. This giant mosaic of Abell 2744

An irregularly shaped image of hundreds of glowing dots on a dark backgroundAn irregularly shaped image of hundreds of glowing dots on a dark background
An image of the galaxy cluster Abell 2744 created by combining many different JWST exposures. In this tiny part of the sky (a fraction of a full Moon) almost every one of the thousands of objects shown is a distant galaxy. Lukas Furtak (Ben-Gurion University of the Negev) from images from the GLASS/UNCOVER teams

This image (click here for full view) is a mosaic (many individual images stitched together) centred on the giant Abell 2744 galaxy cluster, colloquially known as “Pandora’s Cluster”. The sheer number and variety of sources that the JWST can detect is mind boggling; with the exception of a handful of foreground stars, every spot of light represents an entire galaxy.

In a patch of dark sky no larger than a fraction of the full Moon there are umpteen thousands of galaxies, really bringing home the sheer scale of the universe we inhabit. Professional and amateur astronomers alike can spend hours scouring this image for oddities and mysteries.

Over the coming years, JWST’s ability to look so deep and far back into the universe will allow us to answer many questions about how we came to be. Just as exciting are the discoveries and questions we can not yet foresee. When you peel back the veil of time as only this new telescope can, these unknown unknowns are certain to be fascinating.

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Marine plankton could act as alert in mass extinction event: UVic researcher – Saanich News

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A University of Victoria micropaleontologist found that marine plankton may act as an early alert system before a mass extinction occurs.

With help from collaborators at the University of Bristol and Harvard, Andy Fraass’ newest paper in the Nature journal shows that after an analysis of fossil records showed that plankton community structures change before a mass extinction event.

“One of the major findings of the paper was how communities respond to climate events in the past depends on the previous climate,” Fraass said in a news release. “That means that we need to spend a lot more effort understanding recent communities, prior to industrialization. We need to work out what community structure looked like before human-caused climate change, and what has happened since, to do a better job at predicting what will happen in the future.”

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According to the release, the fossil record is the most complete and extensive archive of biological changes available to science and by applying advanced computational analyses to the archive, researchers were able to detail the global community structure of the oceans dating back millions of years.

A key finding of the study was that during the “early eocene climatic optimum,” a geological era with sustained high global temperatures equivalent to today’s worst case global warming scenarios, marine plankton communities moved to higher latitudes and only the most specialized plankton remained near the equator, suggesting that the tropical temperatures prevented higher amounts of biodiversity.

“Considering that three billion people live in the tropics, the lack of biodiversity at higher temperatures is not great news,” paper co-leader Adam Woodhouse said in the release.

Next, the team plans to apply similar research methods to other marine plankton groups.

Read More: Global study, UVic researcher analyze how mammals responded during pandemic

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The largest marine reptile ever could match blue whales in size – Ars Technica

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Blue whales have been considered the largest creatures to ever live on Earth. With a maximum length of nearly 30 meters and weighing nearly 200 tons, they are the all-time undisputed heavyweight champions of the animal kingdom.

Now, digging on a beach in Somerset, UK, a team of British paleontologists found the remains of an ichthyosaur, a marine reptile that could give the whales some competition. “It is quite remarkable to think that gigantic, blue-whale-sized ichthyosaurs were swimming in the oceans around what was the UK during the Triassic Period,” said Dean Lomax, a paleontologist at the University of Manchester who led the study.

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Giant jawbones

Ichthyosaurs were found in the seas through much of the Mesozoic era, appearing as early as 250 million years ago. They had four limbs that looked like paddles, vertical tail fins that extended downward in most species, and generally looked like large, reptilian dolphins with elongated narrow jaws lined with teeth. And some of them were really huge. The largest ichthyosaur skeleton so far was found in British Columbia, Canada, measured 21 meters, and belonged to a particularly massive ichthyosaur called Shonisaurus sikanniensis. But it seems they could get even larger than that.

What Lomax’s team found in Somerset was a surangular, a long, curved bone that all reptiles have at the top of the lower jaw, behind the teeth. The bone measured 2.3 meters—compared to the surangular found in the Shonisaurus sikanniensis skeleton, it was 25 percent larger. Using simple scaling and assuming the same body proportions, Lomax’s team estimated the size of this newly found ichthyosaur at somewhere between 22 and 26 meters, which would make it the largest marine reptile ever. But there was one more thing.

Examining the surangular, the team did not find signs of the external fundamental system (EFS), which is a band of tissue present in the outermost cortex of the bone. Its formation marks a slowdown in bone growth, indicating skeletal maturity. In other words, the giant ichthyosaur was most likely young and still growing when it died.

Correcting the past

In 1846, five large bones were found at the Aust Cliff near Bristol in southwestern England. Dug out from the upper Triassic rock formation, they were dubbed “dinosaurian limb bone shafts” and were exhibited in the Bristol Museum, where one of them was destroyed by bombing during World War II.

But in 2005, Peter M. Galton, a British paleontologist then working at the University of Bridgeport, noticed something strange in one of the remaining Aust Cliff bones. He described it as an “unusual foramen” and suggested it was a nutrient passage. Later studies generally kept attributing those bones to dinosaurs but pointed out things like an unusual microstructure that was difficult to explain.

According to Lomax, all this confusion was because the Aust Cliff bones did not belong to dinosaurs and were not parts of limbs. He pointed out that the nutrient foramen morphology, shape, and microstructure matched with the ichthyosaur’s bone found in Somerset. The difference was that the EFS—the mark of mature bones—was present on the Aust Cliff bones. If Lomax is correct and they really were parts of ichthyosaurs’ surangular, they belonged to a grown individual.

And using the same scaling technique applied to the Somerset surangular, Lomax estimated this grown individual to be over 30 meters long—slightly larger than the biggest confirmed blue whale.

Looming extinction

“Late Triassic ichthyosaurs likely reached the known biological limits of vertebrates in terms of size. So much about these giants is still shrouded by mystery, but one fossil at a time, we will be able to unravel their secrets,” said Marcello Perillo, a member of the Lomax team responsible for examining the internal structure of the bones.

This mystery beast didn’t last long, though. The surangular bone found in Somerset was buried just beneath a layer full of seismite and tsunamite rocks that indicate the onset of the end-Triassic mass extinction event, one of the five mass extinctions in Earth’s history. The Ichthyotian severnensis, as Lomax and his team named the species, probably managed to reach an unbelievable size but was wiped out soon after.

The end-Triassic mass extinction was not the end of all ichthyosaurs, though. They survived but never reached similar sizes again. They faced competition from plesiosaurs and sharks that were more agile and swam much faster, and they likely competed for the same habitats and food sources. The last known ichthyosaurs went extinct roughly 90 million years ago.

PLOS ONE, 2024.  DOI: 10.1371/journal.pone.0300289

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Jeremy Hansen – The Canadian Encyclopedia

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Early Life and Education

Jeremy Hansen grew up on a farm near the community of Ailsa Craig, Ontario, where he attended elementary school. His family moved to Ingersoll,
Ontario, where he attended Ingersoll District Collegiate Institute. At age 12 he joined the 614 Royal Canadian Air Cadet Squadron in London, Ontario. At 16 he earned his Air Cadet
glider pilot wings and at 17 he earned his private pilot licence and wings. After graduating from high school and Air Cadets, Hansen was accepted for officer training in the Canadian Armed Forces (CAF). He was trained at Chilliwack, British Columbia, and the Royal Military College at Saint-Jean-sur-Richelieu,
Quebec. Hansen then enrolled in the Royal Military College of Canada in Kingston,
Ontario. In 1999, he completed a Bachelor of Science in space science with First Class Honours and was a Top Air Force Graduate from the Royal Military College. In 2000, he completed his Master of Science in physics with a focus on wide field of view satellite tracking.   

CAF Pilot

In 2003, Jeremy Hansen completed training as a CF-18 fighter pilot with the 410 Tactical Fighter Operational Training Squadron at Cold Lake, Alberta.
From 2004 to 2009, he served by flying CF-18s with the 441 Tactical Fighter Squadron and the 409 Tactical Fighter Squadron. He also flew as Combat Operations Officer at 4 Wing Cold Lake. Hansen’s responsibilities included NORAD operations effectiveness,
Arctic flying operations and deployed exercises. He was promoted to the rank of colonel in 2017. (See also Royal Canadian Air Force.)

Career as an Astronaut

In May 2009, Jeremy Hansen and David Saint-Jacques were chosen out of 5,351 applicants in the Canadian Space Agency’s
(CSA) third Canadian Astronaut Recruitment Campaign. He graduated from Astronaut Candidate Training in 2011 and began working at the Mission Control Center in Houston, Texas, as capsule communicator (capcom, the person in Mission Control who speaks directly
to the astronauts in space.

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David Saint-Jacques (left) and Jeremy Hansen (right) during a robotics familiarization session, 25 July 2009.

As a CSA astronaut, Hansen continues to develop his skills. In 2013, he underwent training in the High Arctic and learned how to conduct geological fieldwork (see Arctic Archipelago;
Geology). That same year, he participated in the European Space Agency’s CAVES program in Sardinia, Italy. In that human performance experiment Hansen lived underground for six days.
In 2014, Hansen was a member of the crew of NASA Extreme Environment Mission Operations (NEEMO) 19. He spent seven days off Key Largo, Florida, living in the Aquarius habitat on the ocean floor, which is used to simulate conditions of the International
Space Station and different gravity fields. In 2017, Hansen became the first Canadian to lead a NASA astronaut class, in which he trained astronaut candidates from Canada and the United States.  

Did you know?

Hansen has been instrumental in encouraging young people to become part of the STEM (Science, Technology,
Engineering, Mathematics) workforce with the aim of encouraging future generations of space explorers.
His inspirational work in Canada includes flying a historical “Hawk One” F-86 Sabre jet.

Artemis II

In April 2023, Hansen was chosen along with Americans Christina Koch, Victor Glover and Reid Wiseman to crew NASA’s Artemis II mission to the moon. The mission, scheduled for no earlier
than September 2025 after a delay due to technical problems, marks NASA’s first manned moon voyage since Apollo 17 in 1972. The Artemis II astronauts will not land on the lunar
surface, but will orbit the moon in an Orion spacecraft. They will conduct tests in preparation for future manned moon landings, the establishment of an orbiting space station called Lunar Gateway, or Gateway, and a base on the moon’s surface where astronauts
can live and work for extended periods. The path taken by Orion will carry the astronauts farther from Earth than any humans have previously travelled. Hansen’s participation in Artemis II is a direct result of Canada’s contribution of Canadarm3
to Lunar Gateway. (See also Canadarm; Canadian Space Agency.)

“Being part of the Artemis II crew is both exciting and humbling. I’m excited to leverage my experience, training and knowledge to take on this challenging mission on behalf of Canada. I’m humbled by the incredible contributions and hard work of so many
Canadians that have made this opportunity a reality. I am proud and honoured to represent my country on this historic mission.” – Jeremy Hansen (Canadian Space Agency, 2023)

Did you know?

On his Artemis II trip, Hansen will wear an Indigenous-designed mission patch created for him by Anishinaabe artist Henry Guimond.

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Honours and Awards

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