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This new view shows a stellar nursery called NGC 3324. It was taken using the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the La Silla Observatory in Chile. The intense ultraviolet radiation from several of NGC 3324's hot young stars causes the gas cloud to glow with rich colors and has carved out a cavity in the surrounding gas and dust. NGC 3324 is located in the southern constellation of Carina (The Keel, part of Jason's ship the Argo) roughly 7500 light-years from Earth. It is on the northern outskirts of the chaotic environment of the Carina Nebula, which has been sculpted by many other pockets of star formation. A rich deposit of gas and dust in the NGC 3324 region fueled a burst of starbirth there several millions of years ago and led to the creation of several hefty and very hot stars that are prominent in the new picture. Stellar winds and intense radiation from these young stars have blown open a hollow in the surrounding gas and dust. This is most in evidence as the wall of material seen to the center right of this image. The ultraviolet radiation from the hot young stars knocks electrons out of hydrogen atoms, which are then recaptured, leading to a characteristic colored glow as the electrons cascade through the energy levels, showing the extent of the local diffuse gas. Other colors come from other elements, with the characteristic glow from doubly ionized oxygen making the central parts appear greenish-yellow. As with clouds in the Earth's sky, observers of nebulae can find likenesses within these cosmic clouds. One nickname for the NGC 3324 region is the Gabriela Mistral Nebula, after the Nobel Prize-winning Chilean poet. The edge of the wall of gas and dust at the right bears a strong resemblance to a human face in profile, with the "bump" in the center corresponding to a nose. The power of the Wide Field Imager on the MPG/ESO 2.2-meter telescope at ESO's La Silla Observatory also reveals many dark features in NGC 3324. Dust grains in these regions block out the light from the background glowing gas, creating shadowy, filigree features that add another layer of evocative structure to the rich vista. The sharp sight of the Hubble Space Telescope has also been trained on NGC 3324 in the past. Hubble can pick out finer details than the panoramic view of the Wide Field Imager, but only over a much smaller field of view. The two instruments when used in tandem can provide both "zoomed-in" and "zoomed-out" perspectives. credit: ESO/Nick Risinger (skysurvey.org)/Digitized Sky Survey 2. Music: John Dyson (from the album Moonwind) source: 🤍
NGC 3324 explained with its Cosmic Cliffs in the carina nebula that have recently been unraveled by James Webb's IRCAM in 8K. The nebula is full of amazing discoveries and interesting features that we go over in this video! #cosmiccliffs #ngc3324 #jameswebbimages
NASA James Webb Space Telescope Capture this in star-forming region NGC 3324 in the Carina Nebula
This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. Called the Cosmic Cliffs, Webb’s seemingly three-dimensional picture looks like craggy mountains on a moonlit evening. In reality, it is the edge of the giant, gaseous cavity within NGC 3324, and the tallest “peaks” in this image are about 7 light-years high. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The blistering, ultraviolet radiation from the young stars is sculpting the nebula’s wall by slowly eroding it away. Dramatic pillars tower above the glowing wall of gas, resisting this radiation. The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation. Music: Feels - Patrick Patrikios Credit: NASA, ESA, CSA, and STScI
This zoom into the Carina Nebula starts from a photograph from the Akira Fujii collection then transitions to a Digitized Sky Survey image. A picture taken by amateur astronomer Brad Moore in Australia precedes a final image taken by the Hubble Space Telescope. credit: NASA, ESA, and G. Bacon (STScI) source: 🤍
This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. Called the Cosmic Cliffs, Webb’s seemingly three-dimensional picture looks like craggy mountains on a moonlit evening. In reality, it is the edge of the giant, gaseous cavity within NGC 3324, and the tallest “peaks” in this image are about 7 light-years high. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image.
NGC 3324 est situé à la périphérie de la région chaotique de la nébuleuse de la Carène (NGC 3372). Un environnement riche en gaz et en poussière dans cette nébuleuse a donné naissance il y a quelques millions d'années à la formation de plusieurs étoiles massives très chaudes. Les rayonnements et les vents stellaires des jeunes étoiles ont expulsé la matière de la nébuleuse et ainsi produit un creux dans la nébuleuse. La matière expulsée forme d'ailleurs une région lumineuse qui forme la silhouette du visage de Gabriela Mistral que l'on voit sur les images. _ Music : Alone Together by Mona Wonderlick 🤍 Creative Commons — Attribution 3.0 Unported — CC BY 3.0 _
NASA James Webb Space Telescope Capture This in NGC 3324
NASA James Webb Space Telescope Capture Massive Supernova in NGC 3324
This zoom into the Carina Nebula starts from a photograph from the Akira Fujii collection then transitions to a Digitized Sky Survey image. A picture taken by amateur astronomer Brad Moore in Australia precedes a final image taken by the Hubble Space Telescope. Credit: NASA, ESA, and G. Bacon (STScI)
Nasa James Webb Space Telescope Capture NGC 3324
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Carina Nebula Credits: IMAGE: NASA, ESA, CSA, STScI
Provided to YouTube by Proton LLC Ngc 3324 · Space Depth Edge of Space ℗ 2013 Secrets Of The Sun Recordings Released on: 2013-03-25 Auto-generated by YouTube.
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Carina Nebula Credits: IMAGE: NASA, ESA, CSA, STScI
Zoom into The Huge Cosmic Bump in NGC 3324 Captured by James Webb Space Telescope
NASA James Webb Space Telescope Capture This in Star-Forming Region NGC 3324 of Carina Nebula.
~~~ 🤍 ~~~ The edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars. Located roughly 7,600 light-years away, NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. [NASA, ESA, CSA, STScI]: 🤍 ~~~ Music from Tunetank.com VictorWayne - Calm Spirit (Copyright Free Music) Download free: 🤍 MelancholicBird - Deep Ocean Meditation (Copyright Free Music) Download free: 🤍 ~~~
This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. Called the Cosmic Cliffs, Webb’s seemingly three-dimensional picture looks like craggy mountains on a moonlit evening. In reality, it is the edge of the giant, gaseous cavity within NGC 3324, and the tallest “peaks” in this image are about 7 light-years high. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. Credits: NASA, ESA, CSA, and STScI
Esta nebulosa tiene el nombre de Mistral en honor a esta gran poetisa por el parecido de su rostro con la formación de dicha nebulosa. Dejamos una de los tantos poemas que hacen referencia a los cielos. Canción de Taurus Búscame por el cielo y me verás pacer. Ahora no soy rojo como cuando era res. Subí de un salto al cielo y aquí me puse a arder.
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Carina Nebula Credits: IMAGE: NASA, ESA, CSA, STScI
Scientists taking a “deep dive” into one of the iconic first images from the NASA/ESA/CSA James Webb Space Telescope have discovered dozens of energetic jets and outflows from young stars previously hidden by dust clouds. The discovery marks the beginning of a new era of investigating how stars like our Sun form, and how the radiation from nearby massive stars might affect the development of planets. Dozens of previously hidden jets and outflows from young stars are revealed in this new image from Webb’s Near-Infrared Camera (NIRCam). This image separates out several wavelengths of light from the First Image revealed on 12 July 2022, which highlights molecular hydrogen, a vital ingredient for star formation. Insets on the right-hand side highlight three regions of the Cosmic Cliffs with particularly active molecular hydrogen outflows. The Cosmic Cliffs, a region at the edge of a gigantic, gaseous cavity within the star cluster NGC 3324, has long intrigued astronomers as a hotbed for star formation. While well-studied by the NASA/ESA Hubble Space Telescope, many details of star formation in NGC 3324 remain hidden at visible-light wavelengths. Webb is perfectly primed to tease out these long-sought-after details since it is built to detect jets and outflows seen only in the infrared at high resolution. Webb’s capabilities also allow researchers to track the movement of other features previously captured by Hubble. Recently, by analyzing data from a specific wavelength of infrared light (4.7 microns), astronomers discovered two dozen previously unknown outflows from extremely young stars revealed by molecular hydrogen. Webb’s observations uncovered a gallery of objects ranging from small fountains to burbling behemoths that extend light-years from the forming stars. Many of these protostars are poised to become low mass stars, like our Sun. Molecular hydrogen is a vital ingredient for making new stars and an excellent tracer of the early stages of their formation. As young stars gather material from the gas and dust that surround them, most also eject a fraction of that material back out again from their polar regions in jets and outflows. These jets then act like a snowplow, bulldozing into the surrounding environment. Visible in Webb’s observations is the molecular hydrogen getting swept up and excited by these jets. Previous observations of jets and outflows looked mostly at nearby regions and more evolved objects that are already detectable in the visual wavelengths seen by Hubble. The unparalleled sensitivity of Webb allows observations of more distant regions, while its infrared optimization probes into the dust-sampling younger stages. Together this provides astronomers with an unprecedented view into environments that resemble the birthplace of our solar system. In analyzing the new Webb observations, astronomers are also gaining insights into how active these star-forming regions are, even in a relatively short time span. By comparing the position of previously known outflows in this region caught by Webb, to archival data by Hubble from 16 years ago, the scientists were able to track the speed and direction in which the jets are moving. This science was conducted on observations collected as part of Webb’s Early Release Observations Program. The paper was published in the Monthly Notices of the Royal Astronomical Society in December 2022. In this image, red, green, and blue were assigned to Webb’s NIRCam data at 4.7, 4.44, and 1.87 microns (F470N, F444W, and F187N filters, respectively).
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Carina Nebula Credits: IMAGE: NASA, ESA, CSA, STScI
NGC 3324 porównanie James Webb vs Hubble 4K NGC 3324 comparison James Webb vs Hubble 4K NGC 3324 porównanie teleskop Webba i teleskop Hubble'a Credit NASA, ESA, and The Hubble Heritage Team (STScI/AURA) Music Hans Zimmer - Interstellar: Main Theme [EPIC Piano Solo] by Magnus Baumgartl
NASA James Webb Space Telescope Two Cosmic Cliffs with Bright Stars in NGC 3324
Zoom into the Dark Black Hole with 2 bright Stars inin NGC 3324 Captured by James Webb Telescope
🤍 🤍 Starting from a broad view of the Milky Way, this zoom video closes in on spectacular region of star formation called NGC 3324 within the constellation of Carina (The Keel of Jason's ship, Argo). The final very detailed view comes from the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. Credit:ESO/Nick Risinger (skysurvey.org)/Digitized Sky Survey 2. Zooming in on the star formation region NGC 3324
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Panning across this star-forming region, dramatic dark towers of cool gas and dust are seen rising above a glowing wall of gas. The high-energy radiation blazing out from the hot, young stars in NGC 3324 is sculpting the wall of the nebula by slowly eroding it away.
This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. Image credit: Image credit: NASA, ESA, CSA, and STScI NASA site: 🤍
#Nebulosa #Astronomía #Astrofotografía Nebulosa Gabriela Mistral y Cúmulo NGC 3294 Telescopio William Optic ZS 73 Cámara Canon Rebel T6 Fecha de Captura: 02.12.2019
🤍#smoothingrelaxationpeacefulrelaxingmusic #shortsfeed #zoomingintothecarinanebula #jameswebb'sfirstimage zooming #brightbluestarformingincarinanebula #NGC3324incarinanebula
This image from the NASA/ESA/CSA James Webb Space Telescope depicts IC 1623, an entwined pair of interacting galaxies which lies around 270 million light-years from Earth in the constellation Cetus. The two galaxies in IC 1623 are plunging headlong into one another in a process known as a galaxy merger. Their collision has ignited a frenzied spate of star formation known as a starburst, creating new stars at a rate more than twenty times that of the Milky Way galaxy. This interacting galaxy system is particularly bright at infrared wavelengths, making it a perfect proving ground for Webb’s ability to study luminous galaxies. A team of astronomers captured IC 1623 across the infrared portions of the electromagnetic spectrum using a trio of Webb’s cutting-edge scientific instruments: MIRI, NIRSpec, and NIRCam. In so doing, they provided an abundance of data that will allow the astronomical community at large to fully explore how Webb’s unprecedented capabilities will help to unravel the complex interactions in galactic ecosystems. These observations are also accompanied by data from other observatories, including the NASA/ESA Hubble Space Telescope, and will help set the stage for future observations of galactic systems with Webb. The merger of these two galaxies has long been of interest to astronomers, and has previously been imaged by Hubble and by other space telescopes. The ongoing, extreme starburst causes intense infrared emission, and the merging galaxies may well be in the process of forming a supermassive black hole. A thick band of dust has blocked these valuable insights from the view of telescopes like Hubble. However, Webb’s infrared sensitivity and its impressive resolution at those wavelengths allows it to see past the dust and has resulted in the spectacular image above, a combination of MIRI and NIRCam imagery. The luminous core of the galaxy merger turns out to be both very bright and highly compact, so much so that Webb’s diffraction spikes appear atop the galaxy in this image. The 8-pronged, snowflake-like diffraction spikes are created by the interaction of starlight with the physical structure of the telescope. The spiky quality of Webb’s observations is particularly noticeable in images containing bright stars, such as Webb’s first deep field image.
#shorts These comparison photos of a young star-forming region called NGC 3324 in the Carina Nebula, taken by Webb, (left) and Hubble, (right), showcase Webb’s abilities to peer through cosmic dust and unveil hundreds of previously hidden stars and background galaxies. Credit: NASA's Goddard Space Flight Center Music: Interstellar theme - tiktok version cover by dorian marko
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth. Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Carina Nebula Credits: IMAGE: NASA, ESA, CSA, STScI
NASA James Webb Space Telescope Capture This Bright Star Arc Formation in Carina Nebula NGC 3324
#Telescopio #Nebula #Astrofotografia *Nebulosa NGC 3324 *Ubicado en la constelación de Carina. *Conocida también como Nebulosa Gabriela Mistral Telescopio Celestron Newton 8" F/5 Cámara Canon Rebel T6 Apilado: -Deep Sky Staker Procesado: -Fitswork -Photoshop Fecha de Captura: 04.01.2019
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![ESO: Zoom Into NGC 3324 [720p]](https://i.ytimg.com/vi/QBz_424svRM/mqdefault.jpg "ESO: Zoom Into NGC 3324 [720p]")
![Zoom Into NGC 3324 In Carina Nebula (2008) [720p]](https://i.ytimg.com/vi/kYF5fVxuZ2E/mqdefault.jpg "Zoom Into NGC 3324 In Carina Nebula (2008) [720p]")
