New Telescope Pictures 2023 – Our naked eye can never see what a telescope sees: by traveling through light and space, James Webb can see the origin of the universe – something that our minds find difficult to understand.
Acting like a time machine, the first images released by this powerful telescope on July 12 showed us distant galaxies, dying stars and the atmospheres of planets outside our solar system.
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Now, more than a year after its launch, James Webb has given scientists and humanity alike some stunning new images from space, this time giving us a look at how stars are born.
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A new image released by NASA on January 11 shows NGC 346, a young star cluster located in a nebula about 200,000 light-years from our planet.
Scientists are particularly interested in this group of stars because they believe it can give us a glimpse of what the universe looked like three billion years after the Big Bang, the so-called “cosmic day,” the period of galaxy formation that followed . the end of the “cosmic dawn”.
A high-resolution image taken by the James Webb Space Telescope revealed more clumps than previously expected, “including stars and planets as clouds of dust and hydrogen,” according to NASA.
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This means that in this latest stunning image, we can see the formation of planets, not just stars.
The James Webb Telescope has produced a highly detailed description of the iconic formation pillars, first made famous by images taken by NASA’s Hubble Space Telescope in 1995, where new stars form in dense clouds of gas and dust.
3D towers look like rock formations, but are more permeable. These pillars are made up of cold interstellar gas and dust that sometimes appear translucent in the near infrared.
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Based on images taken in 1995 and 2014, Webb’s new look at the constellations will help researchers refine their star formation models by determining more precisely the number of newly formed stars and the amount of gas and dust in the region.
Over time, they begin to better understand how stars form and explode in these dust clouds over millions of years.
This composite image provided by NASA shows formation poles (left) taken by the Hubble Space Telescope in 2014 and NASA’s James Webb Telescope in 2022. Space Telescope Science Institute Office of Public Affairs/Public
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On October 28, NASA released the second Webb Mid-Infrared (MIRI) image of the formation’s towers. It’s haunting—according to NASA, this exclusive dusty rendering makes it look dark and “cool.”
That’s because the mid-infrared light is meant to describe where the dust is, and at those wavelengths, many nearby stars aren’t bright enough to see.
“Instead, these plumes of lead-colored gas and dust glow around the edges, suggesting its activity,” NASA explained.
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Mid-infrared view of the Pillars of Creation from the James Webb Space Telescope. Contributed by NASA, ESA, CSA, STScI, Joseph De Pasquale (STScI), Alyssa Pagan (STScI)
In images released by NASA in September, the 30 Doradus Nebula can be seen in all its glory.
Nicknamed the Tarantula Nebula, it is a favorite of star-forming astronomers, being the largest and brightest star-forming region in the nearest galaxies to the Milky Way.
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The Tarantula Nebula is located 161,000 light-years away in the Large Magellanic Cloud galaxy. It got its name because of the long, dusty threads that resemble the legs of spiders in ancient drawings.
However, the James Webb telescope captured the stellar nursery with a new level of clarity, showing tens of thousands of young stars previously shrouded in cosmic dust.
This image released by NASA on September 6, 2022 shows a star-forming region in the Tarantula Nebula taken by the James Webb Space Telescope. NASA, ESA, CSA, STScl and Webb ERO production team via AP
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This stunning image is the so-called Galaxy Phantom (M74). Webb’s ability to capture longer wavelengths of light allows scientists to identify star-forming regions in these galaxies.
The image shows masses of gas and dust in the galaxy’s arms and a dense cluster of stars in its core.
James Webb Telescope view of the ghost galaxy ESA/Webb, NASA and KSA, J. Lee and the PHANGS-JWST team
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NASA also published unprecedented observations of a planet outside our solar system, using the powerful infrared vision of the James Webb Space Telescope to reveal new details that ground-based telescopes could not detect.
The image of exoplanet HIP 65426 b, a gas giant six to twelve times the mass of Jupiter, is the first time a web telescope has taken a direct image of a planet outside the solar system.
This image shows the exoplanet HIP 65426 b in different infrared bands as seen by the James Webb Space Telescope. NASA/ESA/CSA, A. Carter (UCSC), ERS 1386 team, and A. Pagan (STScI)
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“This is a transformative moment not only for Webb, but for astronomy in general,” said Sasha Hinckley, associate professor of physics and astronomy at the University of Exeter in the UK, who led the observations.
HIP 65426 b, located 355 light-years from Earth, is 15 to 20 million years old compared to our 4.5 billion-year-old Earth.
It is 100 times farther from its host star than Earth is from the Sun, so Webb can easily separate the planet from the star in the image because it is far enough from the star. But it is more than 10,000 times fainter than its star in the near-infrared and hundreds of thousands of times fainter in the mid-infrared.
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“Getting this image is like hunting for space treasure,” said Arin Carter, a researcher at the University of California, Santa Cruz, who led the analysis of the images.
“At first, I could only see the light from the star, but with careful image processing, I was able to remove that light and reveal the planet.”
NASA scientists also released new photos of the solar system’s largest planet, calling the results “pretty incredible.”
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The James Webb Telescope returned images in July, capturing unprecedented views of Jupiter’s northern and southern lights and swirling polar nebulae. Jupiter’s Great Red Spot, a storm big enough to engulf Earth, stands out brightly from countless smaller storms.
A wide-angle image is particularly dramatic, showing faint rings around the planet as well as two small moons against a bright background of galaxies.
“I’ve never seen Jupiter like this. It’s all incredible,” said planetary astronomer Imke de Pater of the University of California, Berkeley, who helped make the observations.
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According to an American-French research team, the infrared images were artificially colored in blue, white, green, yellow and orange to bring out the details.
The latest images come just weeks after another series of images by James Webb’s team showed us the Cartwheel Galaxy in greater depth, taking our understanding of the universe a step further by showing what happens after two galaxies collide.
Looking through the cosmic dust created by the collision with its infrared cameras, the telescope gave us a glimpse of how the Cartwheel galaxy is changing after it collided with another, smaller galaxy billions of years ago.
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A large, pink, dotted galaxy looks like a wheel with a small inner oval, and to the right are dusty blue and two smaller spiral galaxies of the same size. NASA via AP
Scientists believe that the Cartwheel Galaxy, a ring galaxy more than 500 million light-years away from our planet, owes its name to the bright inner ring and colorful outer ring that were part of a larger spiral similar to the Milky Way before to be broken by another spiral. . . galaxy.
NASA reports that the high-speed collision reminded scientists of the general image of the galaxy as a wagon wheel. From the center of the collision, the galaxy’s two rings expanded outward, creating this rare ring shape.
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Never before have scientists been able to clearly see and understand the chaos of the Cartwheel galaxy.
Mid-infrared light captured by Webb’s MIRI infrared camera reveals fine details of dusty regions and young stars in the Cartwheel Galaxy. NASA, ESA, CSA, STScI, Webb ERO Production Group
The Hubble Space Telescope has already surveyed the galaxy, but due to the large amount of dust surrounding the Cartwheel galaxy, the telescope could not observe the phenomena taking place inside the galaxy.
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But now, thanks to the infrared cameras of the James Webb Telescope, scientists have been able to look at the bright center of the galaxy.
To do this, an image was created by combining a Webb Near Infrared Camera (NIRCam) and a Mid-Infrared Instrument (MIRI), which are able to see through dust and detect wavelengths of light that cannot be observed under visible light conditions.
The resulting image shows the formation of stars after galaxies collide – a process that is not yet fully understood.
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This image from the James Webb Telescope shows the edge of a nearby young star.