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Nebulas NGC 2014 & NGC 2020 in Large Magellanic Cloud: Wide-field View | ESO
This wide-field view captures the pair of nebulae NGC 2014 and NGC 2020 in the constellation of Dorado (The Swordfish). These two glowing clouds of gas, in the center of the frame, are located in the Large Magellanic Cloud, one of the Milky Way’s satellite galaxies. Both are sculpted by powerful winds from hot young stars.
This view was created from images forming part of the Digitized Sky Survey 2.
Credit: European Space Agency/Hubble, Digitized Sky Survey 2
Glowing Nebulas NGC 2014 & NGC 2020 in the Large Magellanic Cloud | ESO
The European Southern Observatory's Very Large Telescope (VLT) has captured a detailed view of a star-forming region in the Large Magellanic Cloud—one of the Milky Way's satellite galaxies. This sharp image reveals two glowing clouds of gas. NGC 2014 (right) is irregularly shaped and red and its neighbor, NGC 2020, is round and blue. These odd and very different forms were both sculpted by powerful stellar winds from extremely hot newborn stars that also radiate into the gas, causing it to glow brightly.
This science visualization presents the dramatic landscape of two nebulas in the Large Magellanic Cloud. The video, based on images by NASA's Hubble Space Telescope, takes viewers on a close-up tour of the nebulas' three-dimensional structures, as envisioned by scientists and artists.
The video begins with the Hubble view of NGC 2014 (lower left) and NGC 2020 (upper right). The region has been nicknamed the "Cosmic Reef," because of its resemblance to an undersea world. The camera then flies past myriad stars for a close-up look at NGC 2014. The first stop is the bubble of hot gas on the left that has a coral-like appearance. Energetic ultraviolet light from the system's most massive stars has heated the gas, while strong stellar winds (streams of charged particles) help create its bubble structure.
The journey continues into the heart of the nebula, home to extraordinarily massive and bright stars. The glowing gas in this region is bathed in the stars' intense luminosity. In contrast, the dark, denser gas is resisting that radiation, and is blown back to form craggy, mountainous shapes. The virtual flight moves past ridges, valleys, and pockets of new star formation.
The camera then rises up and over a ridge of NGC 2014, revealing the three-dimensional structure of neighboring NGC 2020. The Wolf-Rayet star at its core is the mammoth, intensely hot source of this nebula. Episodes of outbursts from the young star have produced cloudy rings and clumps in the bright blue gas. While Hubble views NGC 2020 looking down the axis of the stellar outflows, the visualization finishes with a side view that illustrates the nebula's double-lobed structure.
Credit: NASA, European Space Agency, G. Bacon, J. DePasquale, L. Hustak, J. Olmstead, A. Pagan, D. Player, and F. Summers (STScI)
This video pans across a diverse landscape of colorful, iridescent gases, streamers of dust, and a plethora of brilliant newborn stars in the nebula NGC 2014, located 163,000 light-years away in the Large Magellanic Cloud, a satellite galaxy of our Milky Way. The camera then sweeps toward a blue ring of glowing oxygen in neighboring nebula NGC 2020. The blue gas is formed by a torrential gaseous outflow from a lone, massive, super-hot star at its center.
Credit: NASA, ESA, and A. Pagan (Space Telescope Science Institute)
This video begins by zooming into the Large Magellanic Cloud, a satellite galaxy of our Milky Way, located 163,000 light-years away. The small galaxy is ablaze with new star formation. The camera zooms up on one such region, called NGC 2014, which is full of colorful, glowing gases energized by a central cluster of newborn stars. The blue, ring-like feature at lower left (NGC 2020) is formed by a torrential gaseous outflow from a lone, massive, super-hot star at its center.
Credit: NASA, European Space Agency, and A. Pagan (Space Telescope Science Institute)
Acknowledgement: A. Fujii and Digitized Sky Survey
A Tapestry of Blazing Starbirth: Nebulas NGC 2014 & NGC 2020 | Hubble
This image is one of the most photogenic examples of the many turbulent stellar nurseries the NASA/European Space Agency Hubble Space Telescope has observed during its 32-year lifetime. The portrait features the giant nebula NGC 2014 and its neighbor NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, approximately 163,000 light-years away.
Credit: NASA, European Space Agency, and the Space Telescope Science Institute (STScI)
Zoom into The Fornax Galaxy Cluster & Galaxy NGC 1365 | ESO
The Fornax Galaxy Cluster is one of the closest of such groupings beyond our Local Group of galaxies. This pan sequence, based on a new VLT Survey Telescope image, shows the central part of the cluster in great detail. The field includes the elegant barred-spiral galaxy NGC 1365 and the big elliptical galaxy NGC 1399.
Panning Across The Fornax Galaxy Cluster & Galaxy NGC 1365 | ESO
The Fornax Galaxy Cluster is one of the closest of such groupings beyond our Local Group of galaxies. This pan sequence, based on a Very Large Telescope (VLT) survey image, shows the central part of the cluster in great detail. The field includes the elegant barred-spiral galaxy NGC 1365 and the big elliptical galaxy NGC 1399.
At the lower-right is the elegant barred-spiral galaxy NGC 1365 and to the left the big elliptical NGC 1399. The Fornax Galaxy Cluster is one of the closest of such groupings beyond our Local Group of galaxies. This new VLT Survey Telescope image shows the central part of the cluster in great detail.
Barred Spiral Galaxy NGC 1365: Infrared View | ESO’s HAWK-I
This striking new image, taken with the powerful HAWK-I infrared camera on the European Southern Observatory’s Very Large Telescope (VLT) at Paranal Observatory in Chile, shows NGC 1365. This beautiful barred spiral galaxy is part of the Fornax cluster of galaxies, and lies about 60 million light-years from Earth.
The picture was created from images taken through Y, J, H and K filters and the exposure times were 4, 4, 7 and 12 minutes respectively.
Credit: European Southern Observatory (ESO)/P. Grosbøl
At around 60 million light-years from Earth, the Great Barred Spiral Galaxy NGC 1365 is captured beautifully in this image by the NASA/European Space Agency Hubble Space Telescope. Located in the constellation of Fornax (The Furnace), the blue and fiery orange swirls show us where stars have just formed and the dusty sites of future stellar nurseries.
At the outer edge of the image, enormous star-forming regions within NGC 1365 can be seen. The bright, light-blue regions indicate the presence of hundreds of baby stars that formed from coalescing gas and dust within the galaxy's outer arms.
This Hubble image was captured as part of a joint survey with the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile. The survey will help scientists understand how the diversity of galaxy environments observed in the nearby Universe influence the formation of stars and star clusters. Expected to image over 100,000 gas clouds and star-forming regions beyond our Milky Way, the PHANGS survey is expected to uncover and clarify many of the links between cold gas clouds, star formation and the overall shape and morphology of galaxies.
Credit: European Space Agency /Hubble & NASA, J. Lee and the PHANGS-HST Team
Barred Spiral Galaxy NGC 1365 | James Webb Space Telescope
Judy Schmidt: "Dusty, barred spiral galaxy NGC 1365. Interestingly, the dust bar is not nearly as prominent as it is in visible light. In the center is a modest active galactic nucleus (AGN). The circumnuclear dust is also quite striking. This time, I was happy to receive the PHANGS team's reduction of the data. Makes it much easier because their mosaic was much better matched and aligned."
Distance: about 56 million light-years
Technical details:
Red (screen layer mode): MIRI F2100W
Orange: MIRI F1130W
Cyan: MIRI F770W
Extra overall brightness in grayscale: MIRI F1000W
North is not up.
Credit: NASA/European Space Agency (ESA)/Space Telescope Science Institute (STScI)/Canadian Space Agency (CSA)/J. Lee and the PHANGS-HST Team
Orbital Sunset above Earth's South Pacific Ocean | International Space Station
An orbital sunset is pictured from the International Space Station as it was soaring 267 miles above the south Pacific Ocean.
Expedition 67 Crew
Commander Oleg Artemyev (Russia)
Roscosmos Flight Engineers: Denis Matveev and Sergey Korsakov (Russia)
NASA Flight Engineers: Kjell Lindgren, Bob Hines, Jessica Watkins (USA)
European Space Agency (ESA) Flight Engineer: Samantha Cristoforetti (Italy)
An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.
Learn more about the important research being operated on Station:
Journey to Our Own Milky Way's Black Hole | National Science Foundation
Dimensional animation flying the viewer into the center of the Milky Way galaxy to the planet earth, geolocating the EHT telescopes around the planet, return to the galaxy and the S-stars orbiting the black hole in the center of our galaxy, Sgr A*.
Credit: National Science Foundation Black Hole PIRE Project, University of Arizona
Turbulent Cauldron of Starbirth in N in Centaurus A Galaxy | Hubble
The NASA/European Space Agency Hubble Space Telescope offers a stunning unprecedented close-up view of a turbulent firestorm of starbirth along a nearly edge-on dust disk girdling Centaurus A, the nearest active galaxy to Earth.
Distance:13 million light years
Credit: E.J. Schreier, (Space Telescope Science Institute) and NASA/European Space Agency (ESA)
Galaxy Centaurus A: Revisiting an Old Friend | NASA's Chandra X-ray Observatory
Just weeks after NASA's Chandra X-ray Observatory began operations in 1999, the telescope pointed at Centaurus A (Cen A, for short). This galaxy, at a distance of about 12 million light years from Earth, contains a gargantuan jet blasting away from a central supermassive black hole.
Since then, Chandra has returned its attention to this galaxy, each time gathering more data. And, like an old family photo that has been digitally restored, new processing techniques are providing astronomers with a new look at this old galactic friend.
This image of Cen A contains data from observations, equivalent to over nine and a half days worth of observing time, taken between 1999 and 2012. In this image, the lowest-energy X-rays Chandra detects are in red, while the medium-energy X-rays are green, and the highest-energy ones are blue.
As in all of Chandra's images of Cen A, this one shows the spectacular jet of outflowing material that is generated by the giant black hole at the galaxy's center. The new image also highlights a dust lane that wraps around the waist of the galaxy. Astronomers think this feature is a remnant of a collision that Cen A experienced with a smaller galaxy millions of years ago.
In addition to allowing for the creation of new images, the data housed in Chandra's extensive archive on Cen A provide a rich resource for a wide range of scientific investigations. For example, in 2013, researchers published new findings on the point-like X-ray sources in Cen A. They found that these sources had masses that fell into two categories. These separate groups correspond to systems where either a neutron star or a black hole is pulling material from a companion star. Information like this may tell us important details about the way the massive stars explode, and gives us even more reason to appreciate this new view of a familiar object.
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