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Saturday, October 26, 2024
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The James Webb Space Telescope (JWST), despite its relatively recent launch, has profoundly reshaped our understanding of the cosmos. It has observed planets, stars, galaxies, and black holes, revealing an array of celestial wonders. Though JWST may seem like a sudden marvel, its development has been the painstaking work of tens of thousands of scientists over decades. Among them, Maggie Aderin-Pocock downplays her own role, choosing instead to highlight the telescope's achievements. "The detail the telescope can capture, the remarkable resolution provided by its six-and-a-half-meter mirror, produces some truly magnificent images,"
URANUS
While the James Webb Space Telescope (JWST) frequently garners attention for its insights into the most distant corners of the universe, it's also ideally suited to capture stunningly detailed images of planets within our own solar system. “This image says it all,” notes Aderin-Pocock. “It’s a magnificent picture of Uranus. Many aren’t aware that Uranus has rings, yet all of the outer planets—Jupiter, Saturn, Uranus, and Neptune—do. Such detailed views are rare, and that’s because we’re observing infrared energy.”
The Carina nebula
Astronomers still have much to learn about the birth of stars, but the clues are found in nebulae—immense clouds of gas and dust that span distances far larger than our solar system. While stellar nurseries have been imaged for decades, the JWST allows us to observe details that were previously hidden. Shown above are the Carina and Ring nebulae. “With optical telescopes, not all visible light penetrates the dust and gas,” Aderin-Pocock explains. “But with an infrared telescope, we see these nebulae in an entirely new way—revealing details we’ve never seen before.”
The Pillars of Creation
One of the Hubble Space Telescope’s most iconic images is of the Pillars of Creation, a section of the Eagle Nebula—another region where stars are born within dense clouds of gas and dust. Yet, as Aderin-Pocock notes, astronomer John Charles Duncan first captured this image in the 1920s. Now, over a century later, JWST has provided a fresh perspective on these three pillars. “It highlights our technological advancement and progress. Each time we capture a more detailed image or use a new wavelength of light, we gain a deeper understanding,” she says.
The Rho Ophiuchi cloud complex
Beyond its scientific value, JWST’s infrared images of nearby stellar clouds, like Rho Ophiuchi, hold aesthetic appeal. “I love this image,” says Aderin-Pocock. “To me, it resembles a truly exotic bird.”
In the 1990s, astronomer Robert Williams directed Hubble at what seemed an empty patch of sky, allowing it to collect light over several days. The resulting image revealed a wealth of galaxies, many among the youngest and most distant we’d ever seen. “From this, astronomers estimated there are about 200 billion galaxies in the universe, which makes my head spin a bit,” Aderin-Pocock adds.
Galaxy cluster SMACS 0723
JWST has been actively capturing its own deep-field images, including one of the galaxy cluster SMACS 0723, allowing us to peer further back in time than Hubble ever could. “As the universe expands, wavelengths of light that start as visible gradually shift into the infrared,” explains Aderin-Pocock. “These galaxies existed so long ago and their light takes such immense time to reach us that viewing them in infrared offers a fresh perspective on how they originally appeared.”
The Cartwheel galaxy
In addition to observing distant galaxies, JWST can focus on nearby ones, offering clues about the formation of our own Milky Way. “Imagine you’re a T. rex trying to take a selfie—you might capture a close-up of your nose or ear, but it’s tough to fit your whole face in because you can’t move the camera far enough away,” says Aderin-Pocock. The Cartwheel Galaxy, formed by the collision of two smaller galaxies, could also offer insights into the Milky Way’s future, as it is expected to collide with the Andromeda galaxy in billions of years.
RS Puppis
A major puzzle in modern cosmology is the Hubble tension—a discrepancy in values when astronomers use different methods to measure the universe’s expansion rate. One method relies on Cepheid variable stars, like RS Puppis, which pulsate with remarkable regularity and were first extensively mapped by the Hubble telescope. Astronomers like Aderin-Pocock hope that JWST’s ability to capture these stars in greater detail could clarify whether the tension stems from limitations in past telescopes or suggests a deeper issue within our current model of the universe.
Galaxy cluster Abell 2744
For the first time, we are able to examine supermassive black holes and their host galaxies in the early universe with remarkable detail. Abell 2744, also known as Pandora’s Cluster, is a galaxy cluster located 4 billion light-years from Earth and contains at least one of these black holes. JWST’s capability to observe the gas and dust surrounding it enables us to gain insights into how these black holes form and operate. When combined with observations from X-ray telescopes, this data provides a comprehensive and detailed picture, according to Aderin-Pocock.
Barnard’s galaxy, also known as NGC 6822
Aderin-Pocock has dedicated much of her career to designing instruments for space, giving her unique insight into the remarkable precision and engineering of JWST. One impressive feature is its ability to focus on small areas of the sky, even amidst densely packed star fields, thanks to a microshutter array—tiny flaps roughly the width of a few human hairs that can block out unwanted light. The star field above includes Barnard’s star, one of our closest neighbors, which has recently been discovered to have its own planet. JWST will conduct further studies on this intriguing find.
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