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The NASA/ESA/CSA James Webb Space Telescope is widely referred to as the successor to the NASA/ESA Hubble Space Telescope. In reality, it is the successor to a lot more than that. With the inclusion of the Mid-InfraRed Instrument (MIRI), Webb also became a successor to infrared space telescopes such as ESA’s Infrared Space Observatory (ISO) and NASA’s Spitzer Space Telescope.
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The NASA/ESA/CSA James Webb Space Telescope has revealed two new views of the Pillars of Creation, which was made famous by the NASA/ESA Hubble Space Telescope in 1995, and again in 2014.
On the left is Webb’s Mid-Infrared Instrument (MIRI) image. Interstellar dust cloaks the scene. And while mid-infrared light specialises in detailing where dust is, the stars aren’t bright enough at these wavelengths to appear. Instead, these looming, leaden-hued pillars of gas and dust gleam at their edges, hinting at the activity within. Learn more about this image here.
On the right is Webb’s Near-Infrared Camera (NIRCam) image, where newly formed protostars are the scene-stealers. These are the bright red orbs that typically have diffraction spikes and lie outside one of the dusty pillars. Learn more about this image here.
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The NASA/ESA/CSA James Webb Space Telescope’s mid-infrared view of the Pillars of Creation strikes a chilling tone. Thousands of stars that exist in this region disappear from view — and seemingly endless layers of gas and dust become the centrepiece.
The detection of dust by Webb’s Mid-Infrared Instrument (MIRI) is extremely important — dust is a major ingredient for star formation. Many stars are actively forming in these dense blue-grey pillars. When knots of gas and dust with sufficient mass form in these regions, they begin to collapse under their own gravitational attraction, slowly heat up, and eventually form new stars.
Although the stars appear to be missing, they aren’t. Stars typically do not emit much mid-infrared light. Instead, they are easiest to detect in ultraviolet, visible, and near-infrared light. In this MIRI view, two types of stars can be identified. The stars at the end of the thick, dusty pillars have recently eroded most of the more distant material surrounding them but they can be seen in mid-infrared light because they are still surrounded by cloaks of dust. In contrast, blue tones indicate stars that are older and have shed most of their gas and dust.
Mid-infrared light also details dense regions of gas and dust. The red region toward the top, which forms a delicate V shape, is where the dust is both diffuse and cooler. And although it may seem like the scene clears toward the bottom left of this view, the darkest grey areas are where densest and coolest regions of dust lie. Notice that there are many fewer stars and no background galaxies popping into view.
Webb’s mid-infrared data will help researchers determine exactly how much dust is in this region — and what it’s made of. These details will make models of the Pillars of Creation far more precise. Over time, we will begin to understand more clearly how stars form and burst out of these dusty clouds over millions of years.
Contrast this view with Webb’s near-infrared light image.
MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.
Image Description: Semi-opaque layers of blue and grey gas and dust start at the bottom left and rise toward the top right. There are three prominent pillars. The left pillar is the largest and widest. The peaks of the second and third pillars are set off in darker shades of blue outlines. Few red stars appear within the pillars. Some blue and white stars dot the overall scene.
Download more versions of this image here.
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ESA spacecraft catch the brightest ever gamma-ray burst
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The Pillars of Creation are set off in a kaleidoscope of colour in the NASA/ESA/CSA James Webb Space Telescope’s near-infrared-light view. The pillars look like arches and spires rising out of a desert landscape, but are filled with semi-transparent gas and dust, and ever changing. This is a region where young stars are forming – or have barely burst from their dusty cocoons as they continue to form.
Protostars are the scene-stealers in this Near-Infrared Camera (NIRCam) image. These are the bright red orbs that sometimes appear with eight diffraction spikes. When knots with sufficient mass form within the pillars, they begin to collapse under their own gravity, slowly heat up, and eventually begin shining brightly.
Along the edges of the pillars are wavy lines that look like lava. These are ejections from stars that are still forming. Young stars periodically shoot out jets that can interact within clouds of material, like these thick pillars of gas and dust. This sometimes also results in bow shocks, which can form wavy patterns like a boat does as it moves through water. These young stars are estimated to be only a few hundred thousand years old, and will continue to form for millions of years.
Although it may appear that near-infrared light has allowed Webb to “pierce through” the background to reveal great cosmic distances beyond the pillars, the interstellar medium stands in the way, like a drawn curtain.
This is also the reason why there are no distant galaxies in this view. This translucent layer of gas blocks our view of the deeper universe. Plus, dust is lit up by the collective light from the packed “party” of stars that have burst free from the pillars. It’s like standing in a well-lit room looking out a window – the interior light reflects on the pane, obscuring the scene outside and, in turn, illuminating the activity at the party inside.
Webb’s new view of the Pillars of Creation will help researchers revamp models of star formation. By identifying far more precise star populations, along with the quantities of gas and dust in the region, they will begin to build a clearer understanding of how stars form and burst out of these clouds over millions of years.
The Pillars of Creation is a small region within the vast Eagle Nebula, which lies 6500 light-years away.
Webb’s NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.
Download the Hi-Res version of the video.
Credit:NASA, ESA, CSA, and STScI, ESO, NOIRLab/NSF/AURA, T.A.Rector, B.A.Wolpa, ESA/Hubble, J. DePasquale, A. Koekemoer, A. Pagan, N. Bartmann, M. Zamani
Music: Tonelabs – The Red North (www.tonelabs.com)
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Launched on 17 October 2002, ESA’s Integral mission is a world-class mission which has been observing the Universe’s violent explosions and powerful phenomena for 20 years, achieving many scientific firsts. The mission’s impressive lifetime is owed to responsibility and leadership on the side of ESA science and operations. This graphic highlights some of the mission’s impressive numbers to date.
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Lensed galaxies in VV 191 (Webb and Hubble composite image)
The Cartwheel Galaxy, a rare ring galaxy once shrouded in dust and mystery, has been unveiled by the imaging capabilities of the NASA/ESA/CSA James Webb Space Telescope. The galaxy, which formed as a result of a collision between a large spiral galaxy and another smaller galaxy, not only retained a lot of its spiral character, but has also experienced massive changes throughout its structure. Webb’s high-precision instruments resolved individual stars and star-forming regions within the Cartwheel, and revealed the behaviour of the black hole within its galactic centre. These new details provide a renewed understanding of a galaxy in the midst of a slow transformation.
Webb’s enormous mirror and precise instruments joined forces to capture the most detailed measurements of starlight filtering through the atmosphere of a planet outside our Solar System to date.
The spectrum of light – which contains information about the makeup of a planetary atmosphere 1,150 light-years away – reveals the distinct signature of water. The strength of the signal that Webb detected hints at the significant role the telescope will play in the search for potentially habitable planets in the coming years. Webb’s powerful new view also shows evidence of haze and clouds that previous studies of this planet did not detect.
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“After Euclid’s lifetime, it will just be floating in space. What if future beings found Euclid? How would they know anything about the humanity of the people?” – Tom Kitching, lead scientist of Euclid’s VIS instrument.
The team behind ESA’s Euclid mission has come together to create something special – a personal and collective galaxy-shaped fingerprint painting that has been attached to the spacecraft ready to launch into space. The collaborative nature of the artwork reflects the collaborative nature of the Euclid project overall; in both cases, people have come together to build something unique.
The Fingertip Galaxy was created by visual artist Lisa Pettibone and Euclid instrument scientist Tom Kitching. Since the very first fingerprint was pressed down in 2019, over 250 scientists and engineers have contributed to the piece of art.
So why a galaxy? Euclid is a galaxy-imaging machine that will observe billions of galaxies out to 10 billion light-years to make a 3D map of the Universe. The mission’s ultimate aim is to explore dark matter and dark energy.
“Although Euclid has always been beautiful in concept and materials, it didn’t really say anything about the people involved and humanity as a whole. We asked ourselves whether we could do something artistic that would speak to people,” says Lisa.
Scientists and engineers involved in Euclid were invited to dip their fingertips in paint and make their mark on a large piece of paper.
“We wanted something authentic, not perfect, and not shaped too much,” continues Lisa. “The result is a piece of art with a wonderful energy to it that captures all the energy of the people involved.”
The artwork was photographed and engraved onto a plaque using lasers at Mullard Space Science Laboratory – the same lasers that are used to etch parts for satellites. The plaque was fixed to Euclid and revealed at a ‘Goodbye Euclid’ event on 1 July 2022, when Euclid left Thales Alenia Space in Turin to head to Cannes for final testing as a complete system.
Euclid’s project scientist René Laureijs suggested adding text to the plaque to explain the thoughts behind it. Continuing the artistic nature of the project, poet Simon Barraclough wrote a dedicated poem, from which a short extract was chosen to be etched on to the plaque in a typewriter font that swirls around the galaxy of fingerprints. This video ends with Simon reading part of Since his poem.
Lisa summarises the Fingertip Galaxy: “It is adding an element of humanity to a dark, vast space, where as far as we can see there is no other intelligent life.”
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Filmmaker/composer: Sam Charlesworth
Fingertip Galaxy creators: Tom Kitching and Lisa Pettibone
Poet: Simon Barraclough – ‘Unextraordinary Light (For Euclid)’
Special thanks: ESA, Euclid mission team, Mullard Space Science Laboratory
Additional media: NASA, @jeremyperkins from unsplash.com
