The James Webb Space Telescope is expected to provide vital information about TOI-1075 b's composition and atmosphere, as well as the temperatures and conditions on its surface. The telescope’s advanced instruments can detect the composition of exoplanet atmospheres by analyzing the light that passes through them as they transit in front of their stars. Read more here
Betelgeuse, the red supergiant star nestled within the Orion constellation, has captured the attention and curiosity of astronomers and stargazers alike due to its peculiar behavior of fluctuating brightness. This enigmatic phenomenon has sparked numerous theories and speculations in the scientific community, aiming to unravel the secrets behind Betelgeuse's captivating light variations. In this article, we delve into some of the most intriguing theories that shed light on this astronomical puzzle. Read full article here
Wolf-Rayet stars are among the most fascinating objects in the universe, characterized by their intense luminosity, high temperatures, and strong stellar winds. These massive stars are in the later stages of their lives and are known for their complex and varied spectra, which provide astronomers with a wealth of information about their physical properties and evolution. In this article, we will explore the remarkable WR 124 star photographed by the James Webb Space Telescope. WR 124 is located 15000 light years away in the constellation Sagittarius. Read more here
NASA's James Webb Space Telescope has begun the study of one of the most renowned supernovae, SN 1987A (Supernova 1987A). Located 168,000 light-years away in the Large Magellanic Cloud, SN 1987A has been a target of intense observations at wavelengths ranging from gamma rays to radio for nearly 40 years, since its discovery in February of 1987. New observations by Webb's NIRCam (Near-Infrared Camera) provide a crucial clue to our understanding of how a supernova develops over time to shape its remnant.
This image reveals a central structure like a keyhole. This center is packed with clumpy gas and dust ejected by the supernova explosion. The dust is so dense that even near-infrared light that Webb detects can't penetrate it, shaping the dark "hole" in the keyhole.
A bright, equatorial ring surrounds the inner keyhole, forming a band around the waist that connects two faint arms of hourglass-shaped outer rings. The equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots, which appeared as the supernova's shock wave hit the ring. Now spots are found even exterior to the ring, with diffuse emission surrounding it. These are the locations of supernova shocks hitting more exterior material.
While these structures have been observed to varying degrees by NASA's Hubble and Spitzer Space Telescopes and Chandra X-ray Observatory, the unparalleled sensitivity and spatial resolution of Webb revealed a new feature in this supernova remnant—small crescent-like structures.
These crescents are thought to be a part of the outer layers of gas shot out from the supernova explosion. Their brightness may be an indication of limb brightening, an optical phenomenon that results from viewing the expanding material in three dimensions. In other words, our viewing angle makes it appear that there is more material in these two crescents than there actually may be.
The high resolution of these images is also noteworthy. Before Webb, the now-retired Spitzer telescope observed this supernova in infrared throughout its entire lifespan, yielding key data about how its emissions evolved over time. However, it was never able to observe the supernova with such clarity and detail.
Despite the decades of study since the supernova's initial discovery, there are several mysteries that remain, particularly surrounding the neutron star that should have been formed in the aftermath of the supernova explosion. Like Spitzer, Webb will continue to observe the supernova over time.
Its NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) instruments will offer astronomers the ability to capture new, high-fidelity infrared data over time and gain new insights into the newly identified crescent structures. Further, Webb will continue to collaborate with Hubble, Chandra, and other observatories to provide new insights into the past and future of this legendary supernova.
TOP IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A). At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
LOWER IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A), which has been annotated to highlight key structures. At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
🚀 India's Chandrayaan-3 Triumphs: Lunar Orbit Conquest! 🌕
🌠 A Giant Leap for India's Space Exploration! 🌠
We're thrilled to share the incredible news of Chandrayaan-3's latest achievement! 🎉 India's lunar mission is soaring to new heights as it successfully enters Lunar orbit, paving the way for an extraordinary soft landing near the Moon's enigmatic south pole! 🌌
🛰️ Chandrayaan-3, with its cutting-edge orbiter, lander, and rover, is now on a thrilling journey towards uncovering the Moon's mysteries. 🌑 The health of the spacecraft is impeccable, monitored carefully from the Mission Operations Complex at ISRO Telemetry, Tracking and Command Network in Bengaluru. 💻
🗓️ Next on the mission's agenda? The Lunar bound orbit maneuver, scheduled for tomorrow around 23:00 hrs IST. 🌓 It's all happening, and we can't contain our excitement!
🌎 Join us as we celebrate India's strides in space exploration and the bold ambitions of Chandrayaan-3 to unlock the secrets of the Moon's south pole. 🌠 Let's cheer on the incredible scientists and engineers at ISRO as they lead us into a new era of lunar discovery! 🚀
Read the full article here ➡️
#Chandrayaan3 #MoonMission #SpaceExploration #ISRO #LunarConquest #IndiaInSpace
🚀✨ Just released! The James Webb Space Telescope has captured a stunning image of the dwarf galaxy NGC 4449, showcasing its vibrant starburst activity! Located 12.5 million light-years away, this galaxy is a stellar nursery with intense star formation visible across its entire structure. 🌌🔭 Dive into the cosmic fireworks and explore the secrets of galactic evolution. Check out the breathtaking details and learn more about this fascinating discovery! Learn more here -
🌌 Cosmic Dance Unveiled! 🌌
Meet Stephan's Quintet: a spectacular galactic group where four galaxies sway together, 290 million light-years away, while a fifth, NGC 7320, glides closer at just 40 million light-years. Thanks to the James Webb Space Telescope, we now see this cosmic ballet in stunning clarity—a mosaic of 150 million pixels showing young stars, shock waves, and swirling gas trails!
But it’s not just eye candy. Webb’s insights into the supermassive black hole in NGC 7319 are rewriting what we know about galaxy evolution and black hole behavior. Discover the wonders hidden in Stephan’s Quintet! ✨ #JamesWebb #StephansQuintet
The James Webb Space Telescope has once again left us in awe with its groundbreaking discoveries! 🚀🔭
In the Orion Nebula, located 1,300 light-years from Earth, astronomers have unveiled a cosmic enigma – Jupiter Mass Binary Objects (JuMBOs)! 🪐🪐 These pairs of planet-like entities challenge the very foundations of our understanding of the universe.
🌠 How did they form? Why are they there? These are questions that have left scientists scratching their heads. This discovery hints at something fundamentally new about star and planet formation.
As Webb continues to probe deeper into the mysteries of the cosmos, we are reminded of the boundless wonders our universe holds. 🌠🤯
Read the full article here and embark on a cosmic journey of discovery.
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Shocking footage of islamic terrorists burning alive captives. This is what Israel is fighting against. This war is our war, war of humanity against Muslim terrorists.
Never miss another James Webb Discovery. Tracking all the amazing discoveries made by the James Webb Space Telescope at https://www.jameswebbdiscovery.com, Follow now!
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