Saturn's Rings Shine In Webb's Spectacular Infrared Portrait. Read Full Article Here

NASA Animation Sizes Up the Universe’s Biggest Black Holes

Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

Music: "In the Stars" from Universal Production Music

So, how exactly will the JWST go about studying these mysterious, ultra-dense objects? Well, black holes are known for their intense gravitational pull, which can cause nearby matter to heat up and emit radiation. The JWST's infrared capabilities will allow it to detect and study this radiation in detail, providing new insights into the behavior of black holes.

One of the key goals of the JWST's black hole research is to better understand the process of accretion, in which matter falls into the black hole and releases energy in the form of radiation. By studying this process in different types of black holes, the JWST could help shed light on some of the most fundamental questions in astrophysics, such as how galaxies form and evolve over time.

But the JWST won't just be looking at black holes in isolation. It will also be studying the way that black holes interact with their surrounding environments, including the stars and gas clouds that surround them. This could help us understand how black holes shape the evolution of galaxies and the wider universe.

All in all, the JWST's black hole research is set to be a game-changer for our understanding of the cosmos.

Witness the Enigmatic Protostar L152 through the Eyes of the James Webb Space Telescope

Exploring the Cosmic Wonders: Witness the Enigmatic Protostar L152 through the Eyes of the James Webb Space Telescope 🌌🔍 Dive into the captivating universe as we journey closer to protostar L152, unveiling its mesmerizing details captured by the collaborative NASA/ESA/CSA James Webb Space Telescope. Read more here - https://www.jameswebbdiscovery.com/discoveries/webb-reveals-protostar-features-within-the-dark-cloud-l1527 🚀🔭

Credit: ESA/Webb, NASA, CSA, unWISE/JPL-Caltech/D. Lang (Perimeter Institute), E. Slawik, N. Risinger, N. Bartmann, M. Zamani 📸🌠 Music: Tonelabs – The Red North

Latest James Webb Telescope Observation Schedule published

jameswebbdiscovery.com

James Webb Discovery - James Webb Space Telescope Weekly Schedule June 19, 2023 to June 25, 2023

James Webb Space Telescope Weekly Schedule June 19, 2023 to June 25, 2023

Pillars of Creation

Observation Alert! James Webb Space Telescope targets NGC-1448. Read full article here

In a remarkable feat, the James Webb Space Telescope has recently turned its discerning gaze towards the distant NGC-1448 galaxy, situated nearly edge-on in the Horologium constellation.

Black Holes: The Universe’s Most Mysterious Giants!

Check out this mind-blowing diagram that breaks down the anatomy of a black hole, one of the most enigmatic phenomena in the cosmos. From the event horizon to the singularity, black holes challenge everything we know about physics and space-time.

Swipe left to dive deep into the science behind these cosmic wonders! 🕳️Learn more --> https://www.jameswebbdiscovery.com/universe/100-fascinating-facts-about-black-holes

#BlackHole #SpaceExploration #CosmicMystery #NASA #Astrophysics #ScienceFacts #Universe

What are 100 space facts ?

Read full article here with 100 space facts.

Are you ready to embark on an interstellar adventure? 🚀🌠 We've got a treat for all the space enthusiasts out there! Our latest article is a mind-blowing compilation of 100 Space Facts that will leave you starstruck and craving for more! 🌌💫

From the breathtaking beauty of the Pillars of Creation to the mind-boggling vastness of the universe, we've curated a list that will ignite your cosmic curiosity like never before! 🪐🌟

Discover why the Moon's footprints will last for millions of years, how a teaspoon of neutron star material weighs millions of tons, and so much more! 🌕🌠

👉 Click here read the full article and journey through the wonders of space! 📖🔭✨

Tag a fellow stargazer and let's explore the universe together! 🌌🌠

Discovery Alert! In a new discovery released on September 14, 2023, James Webb Telescope reveals A Close-Up of Stellar Birth in HH 211. Read full article here

Prepare to be captivated by the breathtaking beauty of space! NASA's James Webb Space Telescope has gifted us with a mesmerizing glimpse into the birth of celestial bodies, courtesy of Herbig-Haro 211 (HH 211). This cosmic wonder resembles the early days of our own Sun and offers invaluable insights into star formation.

🌟 Herbig-Haro objects are cosmic masterpieces born when stellar winds and gas jets from newborn stars collide with nearby interstellar matter at astonishing speeds. In Webb's high-resolution, near-infrared image, HH 211 shines with exquisite detail, showcasing a series of dazzling bow shocks to the southeast and northwest. But that's not all—this image unveils a slender bipolar jet that powers these shocks in unprecedented detail.

💫 What makes this image even more fascinating is the dance of molecules within this turbulent environment. Molecular hydrogen, carbon monoxide, silicon monoxide, and more become electrified, emitting infrared light that Webb artfully captures. This light provides a map of the intricate structure of the celestial outflows.

📸 Credits go to ESA/Webb, NASA, CSA, and T. Ray from the Dublin Institute for Advanced Studies for this celestial masterpiece.

Ready to embark on a cosmic journey? Dive into the full article and explore the cosmic wonders Webb has unveiled: here

#NASA #WebbTelescope #StellarBirth #CosmicWonders #SpaceDiscovery #Astronomy #HerbigHaro211 🚀🌠

Webb reveals new structures within iconic supernova

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)

Stunning image of the dwarf galaxy NGC 4449 from the Webb Telescope

🚀✨ 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 -