{ "count": 67, "next": null, "previous": null, "results": [ { "id": 14917, "url": "https://svs.gsfc.nasa.gov/14917/", "result_type": "Infographic", "release_date": "2025-12-12T10:00:00-05:00", "title": "Roman Galactic Plane Survey", "description": "No description available.", "hits": 243 }, { "id": 14859, "url": "https://svs.gsfc.nasa.gov/14859/", "result_type": "Produced Video", "release_date": "2025-06-21T00:00:00-04:00", "title": "Webb Stellarium", "description": "Stellarium is an installation video designed for the Goddard Space Flight Center visitor center. It is playing temporarily in the room designed for Solarium, and installation built around Sun footage from the Solar Dynamics Observatory (SDO).\r\n\r\nStellarium sources James Webb Space Telescope imagery processed and provided by the Space Telescope Science Institute and available here.", "hits": 67 }, { "id": 31304, "url": "https://svs.gsfc.nasa.gov/31304/", "result_type": "Hyperwall Visual", "release_date": "2024-08-06T00:00:00-04:00", "title": "Take a Cosmic Road Trip this Summer with Chandra and Webb", "description": "Images combining data from NASA’s Chandra and Webb telescopes, of a cloud complex, a region of star formation, a spiral galaxy, and a galaxy cluster. || chandrawebb3-hw_print.jpg (1024x576) [176.0 KB] || chandrawebb3-hw_searchweb.png (320x180) [65.0 KB] || chandrawebb3-hw_thm.png (80x40) [6.0 KB] || chandrawebb3-hw.tif (5760x3240) [53.4 MB] || take-a-cosmic-road-trip-this-summer-with-chandra-and-webb.hwshow [311 bytes] || ", "hits": 85 }, { "id": 31284, "url": "https://svs.gsfc.nasa.gov/31284/", "result_type": "Hyperwall Visual", "release_date": "2024-05-27T00:00:00-04:00", "title": "The Webb Space Telescope Studies the Southern Ring Nebula", "description": "Webb Space Telescope NIRCam image || southern-ring-nebula_00433_print.jpg (1024x576) [198.6 KB] || southern-ring-nebula_00433.png (3840x2160) [8.6 MB] || NGC_3132_webb_NIRCam-STScI-01G8GZQ3ZFJRD8YF8YZWMAXCE3.png (4833x4501) [21.3 MB] || southern-ring-nebula_00433_searchweb.png (320x180) [90.4 KB] || southern-ring-nebula_00433_thm.png (80x40) [6.2 KB] || the-webb-space-telescope-studies-the-southern-ring-nebula-nircam-view.hwshow [274 bytes] || ", "hits": 222 }, { "id": 31283, "url": "https://svs.gsfc.nasa.gov/31283/", "result_type": "Hyperwall Visual", "release_date": "2024-05-22T00:00:00-04:00", "title": "Webb Space Telescope View of the Horsehead Nebula", "description": "Horsehead Nebula (Euclid, Hubble and Webb images) || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3.png (8983x3530) [35.2 MB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_print.jpg (1024x402) [143.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_searchweb.png (320x180) [90.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_thm.png (80x40) [15.8 KB] || ", "hits": 91 }, { "id": 31274, "url": "https://svs.gsfc.nasa.gov/31274/", "result_type": "Hyperwall Visual", "release_date": "2024-02-01T00:00:00-05:00", "title": "The Creation of Pillars", "description": "A Hyperwall ready version of the Space Telescope Science Institute video originally published at www.youtube.com/watch?v=Slx91ASCiXwA behind the scenes look at producing a scientific visualization of the famous Pillars of Creation in the Eagle Nebula.The AstroViz Project of NASA's Universe of Learning is creating an exploration into the iconic Pillars of Creation in the Eagle Nebula. This production reel provides a peek into the underlying science, the 2D image processing, and the development of 3D volumetric models of these star-forming wonders using visible and infrared data from the Hubble and Webb Space Telescopes. || ", "hits": 122 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 953 }, { "id": 14235, "url": "https://svs.gsfc.nasa.gov/14235/", "result_type": "Produced Video", "release_date": "2022-11-02T09:55:00-04:00", "title": "Hubble’s Inside The Image: N44 Superbubble", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the past 32 years. One of them is the breathtaking Nebula known as the N44 Superbubble.N44 is a complex nebula filled with glowing hydrogen gas, dark lanes of dust, massive stars, and many populations of stars of different ages. One of its most distinctive features, however, is the dark, starry gap called a “superbubble,” visible in the upper central region. In this video, Dr. Ken Carpenter takes us on a journey through the Nebula, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Video Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser; L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky SurveyPanther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), NigelSharp, Mark Hanna (NOAO)/WIYN/NSFMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Cosmic Call” by Immersive Music via Shutterstock Music || ", "hits": 72 }, { "id": 31186, "url": "https://svs.gsfc.nasa.gov/31186/", "result_type": "Hyperwall Visual", "release_date": "2022-08-09T00:00:00-04:00", "title": "Webb's Science Mission Begins: First Light Images", "description": "The Cartwheel Galaxy, a rare ring galaxy once shrouded in dust and mystery, has been unveiled by the imaging capabilities of NASA’s James Webb Space Telescope. The galaxy, which formed as a result of a collision between a large spiral galaxy and another smaller galaxy, not only retained a lot of its spiral character, but has also experienced massive changes throughout its structure. Webb’s high-precision instruments resolved individual stars and star-forming regions within the Cartwheel, and revealed the behavior of the black hole within its galactic center. These new details provide a renewed understanding of a galaxy in the midst of a slow transformation. || cartwheel_348_print.jpg (1024x576) [152.0 KB] || cartwheel_348.png (3840x2160) [9.1 MB] || webbs-science-mission-begins-first-light-images-cartwheel-galaxy.hwshow [314 bytes] || ", "hits": 113 }, { "id": 31188, "url": "https://svs.gsfc.nasa.gov/31188/", "result_type": "Hyperwall Visual", "release_date": "2022-08-09T00:00:00-04:00", "title": "Webb's Science Mission Begins: First Light Images As Compared to Hubble", "description": "NGC 3372: Eta Carinae Nebula || eta-carina-cliffs_1.00001_print.jpg (1024x576) [111.2 KB] || eta-carina-cliffs_1.00001_searchweb.png (320x180) [56.4 KB] || eta-carina-cliffs_1.00001_thm.png (80x40) [4.5 KB] || eta-carina-cliffs_1.mp4 (1920x1080) [17.2 MB] || eta-carina-cliffs_1.webm (1920x1080) [2.2 MB] || ", "hits": 76 }, { "id": 14180, "url": "https://svs.gsfc.nasa.gov/14180/", "result_type": "Produced Video", "release_date": "2022-07-25T12:00:00-04:00", "title": "The James Webb Space Telescope First Image Release Broadcast July 12, 2022", "description": "The first images taken by the Webb Space Telescope are revealed to the entire world during this broadcast. || ", "hits": 107 }, { "id": 14182, "url": "https://svs.gsfc.nasa.gov/14182/", "result_type": "B-Roll", "release_date": "2022-07-19T00:00:00-04:00", "title": "The James Webb Space Telescope First Image Review Meetings B-Roll", "description": "B-roll footage of scientists reviewing the first images from the Webb Space Telescope in the early release obseravation review meetings at the Space Telescope Science Institute in Baltimore, MD. || ", "hits": 76 }, { "id": 14024, "url": "https://svs.gsfc.nasa.gov/14024/", "result_type": "Produced Video", "release_date": "2021-11-30T09:55:00-05:00", "title": "Tour Stunning Hubble Nebulae Images", "description": "Over the years, the Hubble Space Telescope has taken hundreds of images of different kinds of incredible nebulae in our universe. A nebula is a giant cloud of dust and gas in space. There are different types of nebulae, ranging from sites where stars are being born under gravitational pressures to expanding gaseous remnants thrown off by dying stars. Hubble Senior Project Scientist, Dr. Jennifer Wiseman, takes us on a tour of some of our universe’s most incredible Nebulae. For more information, visit https://nasa.gov/hubble. Additional Credits:Zoom in to Orion Nebula:Ground-based image taken by Akira Fujii, zoom in on the star formation region of the Orion Nebula observed by Martin KornmesserZoom in to the Cat’s Eye Nebula:NASA, ESA, HEIC, NOT, Digitized Sky Survey 2, the Hubble Heritage Team (STScI/AURA) and Romano Corradi (Isaac Newton Group of Telescopes, Spain)Music Credits: “Magic Mars” by Bernhard Hering [GEMA], Martin Wester [GEMA], Matthias Kruger [GEMA], via Ed.Berlin Production Music / Universal Production Music GmbH [GEMA], and Universal Production Music || ", "hits": 163 }, { "id": 13999, "url": "https://svs.gsfc.nasa.gov/13999/", "result_type": "Produced Video", "release_date": "2021-11-24T09:55:00-05:00", "title": "Sonification of the Bubble Nebula", "description": "In this Hubble image, a super-hot, massive star is blowing an enormous bubble into space. Fittingly named the Bubble Nebula, this beautiful cosmic object is roughly seven light-years across and resides 7,100 light-years from Earth. Scanned from top to bottom, color is mapped to pitch in this sonification of the nebula. The bright blue of the bubble can be heard as higher pitches; the red and orange regions’ lower pitches are heard most clearly at the beginning on the left and in the top half of the bubble in the middle. Brightness controls the volume and stars are represented by chimes.Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ", "hits": 220 }, { "id": 13998, "url": "https://svs.gsfc.nasa.gov/13998/", "result_type": "Produced Video", "release_date": "2021-11-16T09:55:00-05:00", "title": "Sonification of the Butterfly Nebula", "description": "This spectacular Hubble image of the Butterfly Nebula shows a colorful view of star death. The \"wings\" of the butterfly are regions of gas heated to more than 36,000° F (about 20,000° C) that are tearing across space at more than 600,000 miles an hour (966,000 kph)! Vertical position is mapped to pitch – meaning that light towards the top of the image is higher pitched. The nebula is played on strings and synthetic tones, while stars are represented by digital harp. Brightness controls the volume, and the tilted hourglass orientation of the nebula produces an overall rising motion, with the prominent iron-rich jet producing a quick rise near the center.Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ", "hits": 114 }, { "id": 14018, "url": "https://svs.gsfc.nasa.gov/14018/", "result_type": "Produced Video", "release_date": "2021-11-08T12:28:00-05:00", "title": "Hubble's Image of N44", "description": "Download image of N44 || Thumb.jpg (1920x1080) [989.0 KB] || Print.jpg (1920x1080) [989.0 KB] || hubble_n44_wfc3_large.jpg (1159x1593) [1.2 MB] || Search.jpg (320x180) [55.0 KB] || N44_WFC3_ACS_mosaic_.tif (14478x19908) [1.6 GB] || ", "hits": 127 }, { "id": 13997, "url": "https://svs.gsfc.nasa.gov/13997/", "result_type": "Produced Video", "release_date": "2021-11-05T09:55:00-04:00", "title": "Sonification of NGC 2392", "description": "About 5,000 light-years from Earth, the stunning nebula NGC 2392 formed after the demise of a star like our Sun. In this sonification, the image is scanned clockwise like a radar. The radius is mapped to pitch, so light farther from the center is higher pitched. The outline of the nebula’s shell can be heard in the rising and falling of pitch, punctuated by its spokes. Brightness controls the volume. Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ", "hits": 76 }, { "id": 13983, "url": "https://svs.gsfc.nasa.gov/13983/", "result_type": "Produced Video", "release_date": "2021-11-01T09:55:00-04:00", "title": "Hubble's Field Guide to Nebulae", "description": "Nebulae are some of the most resplendent objects in the universe, but it’s easy to confuse which one is an “emission nebula,” and which one is an “absorption nebula.” Thankfully, this “Field Guide” will give you a quick rundown so you can impress all of your friends with your Nebulae Knowledge! And thanks to the Hubble Space Telescope, we can study all sorts of nebulae in all of their magnificent forms. For more information, visit https://nasa.gov/hubble. Additional Credits:Photo Logo Opener by Tony Ivonin via Motion ArrayMusic Credits: “Himalayan Temple” by Jan Pham Huu Tri [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music || ", "hits": 107 }, { "id": 13320, "url": "https://svs.gsfc.nasa.gov/13320/", "result_type": "Produced Video", "release_date": "2021-03-18T08:55:00-04:00", "title": "Hubble Shows Torrential Outflows from Infant Stars May Not Stop Them from Growing", "description": "Though our galaxy is an immense city of at least 200 billion stars, the details of how they formed remain largely cloaked in mystery. Scientists know that stars form from the collapse of huge hydrogen clouds that are squeezed under gravity to the point where nuclear fusion ignites. But only about 30 percent of the cloud’s initial mass winds up as a newborn star. Where does the rest of the hydrogen go during such a terribly inefficient process?For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Additional Visualizations:Zoom In To Star Formation: ESA, Silicon WorldsWide Image of Orion Complex: Image courtesy of Rogelio Bernal Andreo, DeepSkyColors.comHerschel and Rosette Nebula: ESA - C. CarreauSpace Cloud: ESA/Hubble (M. Kornmesser & L. L. Christensen)Zoom out of Milky Way: ESA, Silicon WorldsMusic Credits: \"Winter Solstice\" by Laetitia Frenod [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM], and Universal Production Music. || ", "hits": 48 }, { "id": 31143, "url": "https://svs.gsfc.nasa.gov/31143/", "result_type": "Hyperwall Visual", "release_date": "2020-05-04T00:00:00-04:00", "title": "Hubble Marks 30 Years in Space With Tapestry of Blazing Starbirth", "description": "Original aspect ratio of Hubble image. || heic2007a_4716x3240_print.jpg (1024x576) [161.9 KB] || heic2007a_4716x3240_searchweb.png (320x180) [83.5 KB] || heic2007a_4716x3240_thm.png (80x40) [8.5 KB] || heic2007a_4716x3240.tif (5760x3240) [34.1 MB] || heic2007a_4716x3240.hwshow [77 bytes] || ", "hits": 49 }, { "id": 13599, "url": "https://svs.gsfc.nasa.gov/13599/", "result_type": "Produced Video", "release_date": "2020-04-29T13:00:00-04:00", "title": "Hubble's Cosmic Reef Image Flyby", "description": "This science visualization presents the dramatic landscape of two nebulas in the Large Magellanic Cloud. The video takes viewers on a close-up tour of the nebulas' three-dimensional structures, as deduced by scientists and artists. The visualization is an interpretation of the nebulas' complex structure and is based on images by NASA's Hubble Space Telescope.For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble.Visualization Credits:Greg Bacon, Joseph DePasquale, Leah Hustak, Joseph Olmsted, Alyssa Pagan, Dani Player, and Frank Summers [ STScI ]Music credits: \"Cosmic Reef\" by J. DePasquale [ STScI ] || ", "hits": 60 }, { "id": 13285, "url": "https://svs.gsfc.nasa.gov/13285/", "result_type": "Produced Video", "release_date": "2019-11-05T13:00:00-05:00", "title": "TESS's Southern Sky Panorama", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) spent a year imaging the southern sky in its search for worlds beyond our solar system. Dive into a mosaic of these images to see what TESS has found so far. Credit: NASA's Goddard Space Flight CenterMusic: “Phenomenon\" from Above and Below Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Southern_Sky_Still.jpg (1920x1080) [892.0 KB] || Southern_Sky_Still_print.jpg (1024x576) [222.5 KB] || Southern_Sky_Still_searchweb.png (320x180) [66.5 KB] || Southern_Sky_Still_thm.png (80x40) [5.0 KB] || 13285_TESS_SouthernSky_Small_720.webm (1280x720) [26.3 MB] || 13285_TESS_SouthernSky_Small_720.mp4 (1280x720) [250.7 MB] || 13285_TESS_SouthernSky_1080.mp4 (1920x1080) [492.4 MB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.srt [4.3 KB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.vtt [4.3 KB] || 13285_TESS_SouthernSky_Best_1080.mp4 (1920x1080) [1.2 GB] || 13285_TESS_SouthernSky_ProRes_1920x1080_30.mov (1920x1080) [3.5 GB] || tesss-southern-sky-panorama-movie.hwshow || 07a_tess_coverage.hwshow [190 bytes] || ", "hits": 155 }, { "id": 31045, "url": "https://svs.gsfc.nasa.gov/31045/", "result_type": "Hyperwall Visual", "release_date": "2019-06-28T10:00:00-04:00", "title": "The Colorful Structure of the Ring Nebula", "description": "A visualization of the 3D structure of the Ring Nebula based on visible light observations from the Hubble Space Telescope and infrared observations from the Large Binocular Telescope. || ring_zbc_hw-example-frame-1920x1080.png (1920x1080) [778.5 KB] || ring_zbc_hw-example-frame-1920x1080_print.jpg (1024x576) [41.2 KB] || ring_zbc_hw-example-frame-1920x1080_searchweb.png (320x180) [29.9 KB] || ring_zbc_hw-example-frame-1920x1080_thm.png (80x40) [2.5 KB] || ring_zbc_hw-1920x1080p30.webm (1920x1080) [14.7 MB] || ring_zbc_hw-1920x1080p30.mp4 (1920x1080) [189.2 MB] || the-colorful-structure-of-the-ring-nebula.hwshow [233 bytes] || ", "hits": 154 }, { "id": 31027, "url": "https://svs.gsfc.nasa.gov/31027/", "result_type": "Hyperwall Visual", "release_date": "2019-03-25T10:00:00-04:00", "title": "Triangulum Galaxy Mosaic", "description": "Full Hubble mosaic image of the Triangulum galaxy (M33), composed of 54 Hubble fields of view stitched together. The borders of individual Hubble images trace the jagged edge of the mosaic, which spans 19,400 light-years across. || STSCI-H-p1901a-f-32073x41147_print.jpg (1024x1313) [262.9 KB] || STSCI-H-p1901a-q-8019x10287.png (8019x10287) [134.5 MB] || STSCI-H-p1901a-h-16307x20574.png (16037x20574) [542.5 MB] || STSCI-H-p1901a-f-32073x41147_searchweb.png (320x180) [73.3 KB] || STSCI-H-p1901a-f-32073x41147_thm.png (80x40) [5.8 KB] || STSCI-H-p1901a-f-32073x41147.tif.dzi (32073x41147) [181 bytes] || STSCI-H-p1901a-f-32073x41147.tif_files (1x1) [4.0 KB] || STSCI-H-p1901a-f-32073x41147.tif (32073x41147) [1.7 GB] || ", "hits": 76 }, { "id": 12552, "url": "https://svs.gsfc.nasa.gov/12552/", "result_type": "Produced Video", "release_date": "2019-02-08T11:00:00-05:00", "title": "NASA's Webb is Sound after Completing Critical Milestones", "description": "NASA's James Webb Space Telescope has successfully passed another series of critical testing milestones on its march to the launchpad. In recent acoustic and vibration tests, technicians and engineers exposed Webb's spacecraft element to brutal dynamic mechnical environmental conditions to ensure it will endure the rigors of a rocket launch to space. || ", "hits": 37 }, { "id": 13109, "url": "https://svs.gsfc.nasa.gov/13109/", "result_type": "B-Roll", "release_date": "2018-11-28T00:00:00-05:00", "title": "The James Webb Space Telescope's Spacecraft Element Tent Cover B-Roll", "description": "B-Roll footage of engineers at Northrop Grumman in Los Angeles California, covering the James Webb Space Telescope's Spacecraft Element with a tent cover before it was moved to the acoustic testing facility for testing. || Spacecraft_Element_Tent_Cover_Screenshot_print.jpg (1024x568) [113.8 KB] || Spacecraft_Element_Tent_Cover_Screenshot.png (2856x1586) [5.6 MB] || Spacecraft_Element_Tent_Cover_Screenshot_searchweb.png (320x180) [92.6 KB] || Spacecraft_Element_Tent_Cover_Screenshot_thm.png (80x40) [7.0 KB] || JWST_NG_Tent_Cover_B-Roll_A.mov (1920x1080) [7.8 GB] || JWST_NG_Tent_Cover_B-Roll_A.mp4 (1920x1080) [573.8 MB] || JWST_NG_Tent_Cover_B-Roll_A.webm (1920x1080) [59.6 MB] || ", "hits": 39 }, { "id": 13115, "url": "https://svs.gsfc.nasa.gov/13115/", "result_type": "B-Roll", "release_date": "2018-11-28T00:00:00-05:00", "title": "The James Webb Space Telescope's Spacecraft Element Tent Cover Time-Lapse B-Roll", "description": "A time-lapse of engineers at Northrop Grumman in Los Angeles California, covering the James Webb Space Telescope's Spacecraft Element with a tent cover before it was moved to the acoustic testing facility for testing. || Time-Lapse_Screenshot_print.jpg (1024x572) [130.9 KB] || Time-Lapse_Screenshot.png (2864x1602) [5.8 MB] || Time-Lapse_Screenshot_searchweb.png (320x180) [108.9 KB] || Time-Lapse_Screenshot_thm.png (80x40) [7.9 KB] || JWST_Northrop_Tent_Cover_Time-Lapse.mov (1920x1080) [9.4 GB] || JWST_Northrop_Tent_Cover_Time-Lapse.mp4 (1920x1080) [692.0 MB] || JWST_Northrop_Tent_Cover_Time-Lapse.webm (1920x1080) [66.7 MB] || JWST_Northrop_Tent_Cover_Time-Lapse_4k.mov (3840x2160) [38.1 GB] || JWST_Northrop_Tent_Cover_Time-Lapse_4k.mp4 (3840x2160) [691.8 MB] || ", "hits": 34 }, { "id": 13116, "url": "https://svs.gsfc.nasa.gov/13116/", "result_type": "B-Roll", "release_date": "2018-11-28T00:00:00-05:00", "title": "The James Webb Space Telescope's Spacecraft Element Moved for Acoustic Testing B-Roll", "description": "B-Roll footage of engineers at Northrop Grumman in Los Angeles California, moving the James Webb Space Telescope's Spacecraft Element into the acoustic testing facility for testing. || Spacecraft_Element_Move_Screenshot_print.jpg (1024x573) [109.4 KB] || Spacecraft_Element_Move_Screenshot.png (2858x1600) [6.6 MB] || Spacecraft_Element_Move_Screenshot_searchweb.png (320x180) [87.3 KB] || Spacecraft_Element_Move_Screenshot_thm.png (80x40) [6.3 KB] || Spacecraft_Move_to_M1_B-Roll_A.mov (1920x1080) [10.0 GB] || Spacecraft_Move_to_M1_B-Roll_A.mp4 (1920x1080) [738.9 MB] || Spacecraft_Move_to_M1_B-Roll_A.webm (1920x1080) [76.3 MB] || ", "hits": 32 }, { "id": 30960, "url": "https://svs.gsfc.nasa.gov/30960/", "result_type": "Hyperwall Visual", "release_date": "2018-06-04T10:00:00-04:00", "title": "Eagle Nebula: M16 Wide", "description": "This series of images shows the environment around the Pillars of Creation, the Eagle Nebula, Messier 16. The images reveal the nebula in optical, X-ray, mid-infrared, and far-infrared light. || STScI-H-M16wide_1x-1920x1080.00001_print.jpg (1024x576) [163.7 KB] || STScI-H-M16wide_1x-1920x1080.00001_searchweb.png (320x180) [108.4 KB] || STScI-H-M16wide_1x-1920x1080.00001_thm.png (80x40) [6.9 KB] || STScI-H-M16wide_1x-1280x720.mp4 (1280x720) [8.5 MB] || STScI-H-M16wide_1x-1920x1080.mp4 (1920x1080) [17.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M16wide_1x-1920x1080.webm (1920x1080) [5.2 MB] || STScI-H-M16wide_1x-640x360.mp4 (640x360) [2.9 MB] || STScI-H-M16wide_1x-3840x2160.mp4 (3840x2160) [17.1 MB] || STScI-H-M16wide_1x-H265-3840x2160.mp4 (3840x2160) [7.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 164 }, { "id": 30957, "url": "https://svs.gsfc.nasa.gov/30957/", "result_type": "Hyperwall Visual", "release_date": "2018-05-25T10:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible and Infrared Light", "description": "This visualization zooms into the Orion Nebula and then flies through a 3D model using both visible light (Hubble Space Telescope) and infrared light (Spitzer Space Telescope) views. || orion_vis_ir_zoom_xfade-1920x1080.png (1920x1080) [1.2 MB] || orion_vis_ir_zoom_xfade-1920x1080_print.jpg (1024x576) [66.7 KB] || orion_vis_ir_zoom_xfade-3840x2160.png (3840x2160) [3.5 MB] || orion_vis_ir_zoom_xfade-1920x1080_searchweb.png (320x180) [66.6 KB] || orion_vis_ir_zoom_xfade-1920x1080_thm.png (80x40) [5.7 KB] || orion_vis_ir_zoom_xfade-1920x1080p30.mp4 (1920x1080) [406.0 MB] || orion_vis_ir_zoom_xfade-3840x2160p30.webm (3840x2160) [25.1 MB] || orion_vis_ir_zoom_xfade-3840x2160p30.mp4 (3840x2160) [836.9 MB] || flight-through-the-orion-nebula-in-visible-and-infrared-light-4k.hwshow || flight-through-the-orion-nebula-in-visible-and-infrared-light-hd.hwshow || ", "hits": 163 }, { "id": 30956, "url": "https://svs.gsfc.nasa.gov/30956/", "result_type": "Hyperwall Visual", "release_date": "2018-05-24T12:00:00-04:00", "title": "The Red Bubble: Supernova Remnant SNR 0509-67.5", "description": "The nebula SNR 0509-67.5, nicknamed the \"Red Bubble\", is the result of a supernova explosion of a star. || red_bubble-sample_frame-1920x1080.png (1920x1080) [971.0 KB] || red_bubble-sample_frame-1920x1080_print.jpg (1024x576) [114.5 KB] || red_bubble-sample_frame-1920x1080_searchweb.png (320x180) [62.8 KB] || red_bubble-sample_frame-1920x1080_thm.png (80x40) [5.6 KB] || red_bubble-1920x1080.webm (1920x1080) [23.3 MB] || red_bubble-1920x1080.wmv (1920x1080) [23.7 MB] || red_bubble-1920x1080.m4v (1920x1080) [23.3 MB] || red_bubble-1920x1080p30.mov (1920x1080) [109.6 MB] || red_bubble-3840x2160p30.mp4 (3840x2160) [142.8 MB] || the-red-bubble-supernova-remnant-snr-0509-675-4k.hwshow [316 bytes] || the-red-bubble-supernova-remnant-snr-0509-675-hd.hwshow [316 bytes] || ", "hits": 83 }, { "id": 30954, "url": "https://svs.gsfc.nasa.gov/30954/", "result_type": "Hyperwall Visual", "release_date": "2018-05-23T12:00:00-04:00", "title": "Celestial Lightsabers: Stellar Jets in HH24", "description": "This visualization combines a two-dimensional zoom and a three-dimensional flight to showcase the resemblance to a double-bladed lightsaber seen in the Hubble Space Telescope's striking image of the Herbig-Haro object known as HH24. || hh24_fly-example_frame-1920x1080.png (1920x1080) [1.6 MB] || hh24_fly-example_frame-1920x1080_print.jpg (1024x576) [43.0 KB] || hh24_fly-example_frame-1920x1080_searchweb.png (320x180) [56.6 KB] || hh24_fly-example_frame-1920x1080_thm.png (80x40) [4.8 KB] || hh24_zoom_fly-b-1920x1080p30.mov (1920x1080) [228.0 MB] || hh24_zoom_fly-b-1920x1080p30.mp4 (1920x1080) [15.6 MB] || hh24_zoom_fly-b-1920x1080p30.webm (1920x1080) [4.6 MB] || ", "hits": 50 }, { "id": 30953, "url": "https://svs.gsfc.nasa.gov/30953/", "result_type": "Hyperwall Visual", "release_date": "2018-05-23T11:00:00-04:00", "title": "Evaporating Peaks: Pillars in the Monkey Head Nebula", "description": "This scientific visualization zooms from the night sky to some pillars in the Monkey Head Nebula (aka NGC 2174). After cross-fading to an infrared view, the sequence showcases the 3D nature of these gaseous peaks. || ngc2174_zoom_reveal-example_frame-1920x1080.png (1920x1080) [2.3 MB] || ngc2174_zoom_reveal-example_frame-1920x1080_print.jpg (1024x576) [105.3 KB] || ngc2174_zoom_reveal-example_frame-1920x1080_searchweb.png (320x180) [92.0 KB] || ngc2174_zoom_reveal-example_frame-1920x1080_thm.png (80x40) [6.6 KB] || ngc2174_zoom_reveal-b-1920x1080.wmv (1920x1080) [46.2 MB] || ngc2174_zoom_reveal-b-1920x1080.m4v (1920x1080) [45.7 MB] || ngc2174_zoom_reveal-1920x1080p30.webm (1920x1080) [6.5 MB] || ngc2174_zoom_reveal-1920x1080p30.mov (1920x1080) [375.6 MB] || evaporating-peaks-pillars-in-the-monkey-head-nebula.hwshow [337 bytes] || ", "hits": 69 }, { "id": 30951, "url": "https://svs.gsfc.nasa.gov/30951/", "result_type": "Hyperwall Visual", "release_date": "2018-05-16T10:00:00-04:00", "title": "Supernova Remnant Cassiopeia A from Hubble", "description": "The nebula known as Cassiopeia A is composed of tattered remains of a star that exploded more than 300 years ago. || cas_a_2004_12-hst-10252x7379_print.jpg (1024x737) [249.8 KB] || cas_a_2004_12-hst-10252x7379_searchweb.png (320x180) [100.4 KB] || cas_a_2004_12-hst-10252x7379_thm.png (80x40) [8.7 KB] || cas_a_2004_12-hst-10252x7379.png (10252x7379) [122.0 MB] || supernova-remnant-cassiopeia-a-from-hubble.hwshow [238 bytes] || ", "hits": 150 }, { "id": 30947, "url": "https://svs.gsfc.nasa.gov/30947/", "result_type": "Hyperwall Visual", "release_date": "2018-05-15T14:00:00-04:00", "title": "Orion Nebula from Hubble", "description": "Orion Nebula from Hubble (2006) || orion_nebula-hst-9000x9000_print.jpg (1024x1024) [161.5 KB] || orion_nebula-hst-9000x9000.png (9000x9000) [79.3 MB] || orion_nebula-hst-9000x9000_searchweb.png (320x180) [85.2 KB] || orion_nebula-hst-9000x9000_thm.png (80x40) [6.3 KB] || orion-nebula-from-hubble.hwshow [218 bytes] || ", "hits": 305 }, { "id": 30944, "url": "https://svs.gsfc.nasa.gov/30944/", "result_type": "Hyperwall Visual", "release_date": "2018-05-07T10:00:00-04:00", "title": "Vision Across the Full Spectrum: The Crab Nebula, from Radio to X-ray", "description": "This animation shows the Crab Nebula from the lowest-frequency light (radio), to infrared, visible, ultraviolet, and finally X-ray. || STScI-H-CrabNebula_1x-1920x1080.00001_print.jpg (1024x576) [40.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_searchweb.png (320x180) [26.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_thm.png (80x40) [2.3 KB] || STScI-H-CrabNebula_1x-1280x720.mp4 (1280x720) [3.8 MB] || STScI-H-CrabNebula_1x-1920x1080.mp4 (1920x1080) [7.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-CrabNebula_1x-1920x1080.webm (1920x1080) [8.0 MB] || STScI-H-CrabNebula_1x-640x360.mp4 (640x360) [1.4 MB] || STScI-H-CrabNebula_1x-3840x2160.mp4 (3840x2160) [16.2 MB] || STScI-H-CrabNebula_1x-H265_3840x2160.mp4 (3840x2160) [3.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 260 }, { "id": 12940, "url": "https://svs.gsfc.nasa.gov/12940/", "result_type": "Produced Video", "release_date": "2018-05-03T00:00:00-04:00", "title": "360 Facebook Live - Hubble's 28th Anniversary", "description": "NASA's Hubble Space Telescope team broadcast live in 360 degrees on Facebook from the Space Telescope Operations Control Center at NASA's Goddard Space Flight Center for Hubble's 28th anniversary on April 24, 2018. || ", "hits": 37 }, { "id": 30943, "url": "https://svs.gsfc.nasa.gov/30943/", "result_type": "Hyperwall Visual", "release_date": "2018-04-30T10:00:00-04:00", "title": "Lagoon Nebula: Visible and Infrared Views", "description": "This video compares the colorful Hubble Space Telescope visible-light image of the core of the Lagoon Nebula and a Hubble infrared-light view of the same region. || STScI-H-M8-Lagoon_1x-1920x1080.00001_print.jpg (1024x576) [93.9 KB] || STScI-H-M8-Lagoon_1x-1920x1080.00001_searchweb.png (320x180) [84.2 KB] || STScI-H-M8-Lagoon_1x-1920x1080.00001_thm.png (80x40) [6.2 KB] || STScI-H-M8-Lagoon_1x-1280x720.mp4 (1280x720) [3.3 MB] || STScI-H-M8-Lagoon_1x-1920x1080.mp4 (1920x1080) [7.2 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M8-Lagoon_1x-1280x720.webm (1280x720) [2.5 MB] || STScI-H-M8-Lagoon_1x-1920x1080.webm (1920x1080) [2.4 MB] || STScI-H-M8-Lagoon_1x-640x360.mp4 (640x360) [1.2 MB] || STScI-H-M8-Lagoon_1x-3840x2160.mp4 (3840x2160) [5.4 MB] || STScI-H-M8-Lagoon_1x_H265-3840x2160.mp4 (3840x2160) [2.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 71 }, { "id": 30940, "url": "https://svs.gsfc.nasa.gov/30940/", "result_type": "Hyperwall Visual", "release_date": "2018-04-11T10:00:00-04:00", "title": "Pillars in the Carina Nebula (HH901)", "description": "This animation shows Herbig Haro 901 (HH901), a large pillar of gas and dust with eruptive young stars inside the Carina Nebula. The animation reveals the object in two Hubble Space Telescope images: first in visible light and then in infrared light. || STScI-H-HH901_1x-1920x1080.00001_print.jpg (1024x576) [155.3 KB] || STScI-H-HH901_1x-1920x1080.00001_searchweb.png (320x180) [104.2 KB] || STScI-H-HH901_1x-1920x1080.00001_thm.png (80x40) [7.2 KB] || STScI-H-HH901_1x-1920x1080.mp4 (1920x1080) [10.8 MB] || STScI-H-HH901_1x-1280x720.mp4 (1280x720) [4.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-HH901_1x-1920x1080.webm (1920x1080) [2.7 MB] || STScI-H-HH901_1x-640x360.mp4 (640x360) [1.6 MB] || STScI-H-HH901_1x-3840x2160.mp4 (3840x2160) [8.8 MB] || STScI-H-HH901_1x_H265-3840x2160.mp4 (3840x2160) [4.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 125 }, { "id": 12909, "url": "https://svs.gsfc.nasa.gov/12909/", "result_type": "B-Roll", "release_date": "2018-03-27T10:00:00-04:00", "title": "James Webb Space Telescope Update B-Roll", "description": "Webb Telescope assembly b-roll and animations || THUMBNAIL_ONLY-Webb_Assembly-video-file-b-roll.jpg (1920x1080) [1.1 MB] || THUMBNAIL_ONLY-Webb_Assembly-video-file-b-roll_print.jpg (1024x576) [511.0 KB] || THUMBNAIL_ONLY-Webb_Assembly-video-file-b-roll_searchweb.png (320x180) [114.2 KB] || THUMBNAIL_ONLY-Webb_Assembly-video-file-b-roll_thm.png (80x40) [8.0 KB] || Webb_Assembly-video-file-b-roll.mov (1920x1080) [6.5 GB] || Webb_Assembly-video-file-b-roll-h264.mp4 (1920x1080) [510.5 MB] || Webb_Assembly-video-file-b-roll.webm (1920x1080) [52.4 MB] || ", "hits": 39 }, { "id": 30860, "url": "https://svs.gsfc.nasa.gov/30860/", "result_type": "Hyperwall Visual", "release_date": "2017-02-28T12:00:00-05:00", "title": "Mystic Mountain: Pillars in the Carina Nebula from Hubble", "description": "A collection of pillars in the Carina Nebula create a gaseous landscape nicknamed \"Mystic Mountain\" || carina_mystic_mountain_wide-hst-3218x3240_print.jpg (1024x1031) [214.6 KB] || carina_mystic_mountain_wide-hst-3218x3240.png (3218x3240) [14.7 MB] || carina_mystic_mountain_wide-hst-3218x3240_searchweb.png (320x180) [92.5 KB] || carina_mystic_mountain_wide-hst-3218x3240_thm.png (80x40) [6.7 KB] || carina_mystic_mountain_wide-hst-308560.key [15.2 MB] || carina_mystic_mountain_wide-hst-308560.pptx [14.8 MB] || mystic-mountain-pillars-in-the-carina-nebula-from-hubble.hwshow [362 bytes] || ", "hits": 146 }, { "id": 30859, "url": "https://svs.gsfc.nasa.gov/30859/", "result_type": "Hyperwall Visual", "release_date": "2017-02-28T10:00:00-05:00", "title": "Gaseous Pillar in the Carina Nebula from Hubble", "description": "Gaseous Pillar and Stellar Jet in the Carina Nebula || carina_pillar_jet_ff-hst-3183x3240_print.jpg (1024x1042) [320.1 KB] || carina_pillar_jet_ff-hst-3183x3240.png (3183x3240) [16.1 MB] || carina_pillar_jet_ff-hst-3183x3240_searchweb.png (320x180) [94.4 KB] || carina_pillar_jet_ff-hst-3183x3240_thm.png (80x40) [9.0 KB] || carina_pillar_jet_ff-hst-30859.key [16.6 MB] || carina_pillar_jet_ff-hst-30859.pptx [16.1 MB] || gaseous-pillar-in-the-carina-nebula-from-hubble.hwshow [339 bytes] || ", "hits": 74 }, { "id": 30858, "url": "https://svs.gsfc.nasa.gov/30858/", "result_type": "Hyperwall Visual", "release_date": "2017-02-28T09:00:00-05:00", "title": "Star Cluster Westerlund 2 in Nebula Gum 29 from Hubble", "description": "Star Cluster Westerlund 2 at the Heart of the Nebula Gum 29 || westerlund2-hst-4324x3240_print.jpg (1024x767) [249.9 KB] || westerlund2-hst-4324x3240.png (4324x3240) [20.5 MB] || westerlund2-hst-4324x3240_searchweb.png (320x180) [108.6 KB] || westerlund2-hst-4324x3240_thm.png (80x40) [7.4 KB] || westerlund2-hst-30858.key [21.0 MB] || westerlund2-hst-30858.pptx [20.5 MB] || ", "hits": 81 }, { "id": 30792, "url": "https://svs.gsfc.nasa.gov/30792/", "result_type": "Hyperwall Visual", "release_date": "2017-02-27T11:00:00-05:00", "title": "The Helix Nebula from Hubble", "description": "The Iridescent Glory of the Helix Nebula, from Hubble || helix-hst-3240x3240_print.jpg (1024x1024) [116.2 KB] || helix-hst-3240x3240.png (3240x3240) [15.8 MB] || helix-hst-3240x3240_searchweb.png (320x180) [69.2 KB] || helix-hst-3240x3240_thm.png (80x40) [5.2 KB] || helix-hst-30792.key [16.2 MB] || helix-hst-30792.pptx [15.9 MB] || the-helix-nebula-from-hubble.hwshow [290 bytes] || ", "hits": 381 }, { "id": 30796, "url": "https://svs.gsfc.nasa.gov/30796/", "result_type": "Hyperwall Visual", "release_date": "2017-02-27T10:00:00-05:00", "title": "Hubble's Panoramic View of the Tarantula Nebula", "description": "Several million young stars are vying for attention in this NASA Hubble Space Telescope image of a raucous stellar breeding ground. Early astronomers gave the nebula its \"tarantula\" nickname because the glowing filaments of gas resemble spider legs. The nebula is located in the Large Magellanic Cloud, a small compainon galaxy to our Milky Way galaxy. This star-forming region is the brightest visible in a neighboring galaxy and is home to the most massive stars ever seen.The nebula is close enough to Earth that Hubble can resolve individual stars, giving astronomers important information about the stars' birth and evolution. It is one of only a few star-forming regions outside of our galaxy that astronomers can study in so much detail. The star-birthing frenzy may be partly fueled by its close proximity to another companion galaxy, the Small Magellanic Cloud.The image reveals the stages of star birth, from embryonic stars a few thousand years old still wrapped in cocoons of dark gas to behemoths that die young in supernova explosions. In this star-forming factory, Hubble shows star clusters of various ages, from about 2 million to about 25 million years old.The region's sparkling centerpiece is a giant, young star cluster (left of center) named NGC 2070, only 2 million years old. Its stellar inhabitants number roughly 500,000. The cluster is a hotbed for young, massive stars. Its dense core, known as R136, is packed with some of the heftiest stars found in the nearby universe, weighing more than 100 times the mass of our Sun.The massive stars are carving deep cavities in the surrounding material by unleashing a torrent of ultraviolet light, Besides sculpting the gaseous terrain, the brilliant stars also may be triggering a successive generation of offspring. When the radiation hits dense walls of gas, it creates shocks, which may be generating a new wave of star birth.The colors represent the hot gas that dominates regions of the image. Red signifies hydrogen gas and blue, oxygen. || ", "hits": 77 }, { "id": 12434, "url": "https://svs.gsfc.nasa.gov/12434/", "result_type": "Produced Video", "release_date": "2017-01-13T14:30:00-05:00", "title": "Astronomical Object Beauty Sequences", "description": "5760x320 resolution video designed for 3x3 hyperwall use. || ", "hits": 44 }, { "id": 30773, "url": "https://svs.gsfc.nasa.gov/30773/", "result_type": "Hyperwall Visual", "release_date": "2016-04-21T00:00:00-04:00", "title": "The Bubble Nebula (NGC 7635) from Hubble", "description": "To mark Hubble's 26th birthday, astronomers captured this balloon-like sphere of gas. || bubble-hst-7857x7462_print.jpg (1024x972) [193.4 KB] || bubble-hst-7857x7462.png (7857x7462) [73.8 MB] || bubble-hst-3412x3240.png (3412x3240) [16.3 MB] || bubble-hst-7857x7462_searchweb.png (320x180) [97.1 KB] || bubble-hst-7857x7462_thm.png (80x40) [19.5 KB] || the-bubble-nebula-ngc-7635-from-hubble.hwshow [302 bytes] || ", "hits": 57 }, { "id": 30782, "url": "https://svs.gsfc.nasa.gov/30782/", "result_type": "Hyperwall Visual", "release_date": "2016-04-21T00:00:00-04:00", "title": "A Flight Into the Bubble Nebula", "description": "This visualization of the Bubble Nebula begins with a ground-based view that encompasses the glowing cloud. The high-energy light from the massive O star, BD +60°2522, is responsible for ionizing the entire region. The virtual camera flies through the foreground stars and approaches the central bubble imaged by Hubble. The massive star continuously sheds some of its outer material in a mass-loss wind, which has blown a bubble of gas seven light-years across.The video's three-dimensional perspective emphasizes the extended nature of the structure and the fact that BD +60°2522 is not located at the center. The pressure inside the bubble is able to expand more rapidly in the directions away from the surrounding nebula. The computer model incorporates both scientific and artistic interpretation of the data. In particular, distances are significantly compressed. || ", "hits": 47 }, { "id": 30683, "url": "https://svs.gsfc.nasa.gov/30683/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T15:00:00-04:00", "title": "Bright Pillars in the Carina Nebula", "description": "Flight into the \"Mystic Mountain\" pillars of gas in the Carina Nebula || mystic_mountain_example_frame-1920x1080.jpg (1920x1080) [322.8 KB] || mystic_mountain_example_frame-1920x1080.png (1920x1080) [2.4 MB] || mystic_mountain_example_frame-1920x1080_searchweb.png (180x320) [88.6 KB] || mystic_mountain_example_frame-1920x1080_thm.png (80x40) [6.5 KB] || mystic_mountain-b-1920x1080.wmv (1920x1080) [23.8 MB] || mystic_mountain-b-1920x1080.m4v (1920x1080) [23.3 MB] || mystic_mountain-b-1280x720.wmv (1280x720) [14.5 MB] || mystic_mountain-b-1280x720.m4v (1280x720) [14.3 MB] || mystic_mountain-b-1920x1080p30.webm (1920x1080) [3.4 MB] || mystic_mountain-b-30683.key [17.9 MB] || mystic_mountain-b-30683.pptx [15.3 MB] || mystic_mountain-b-1920x1080p30.mov (1920x1080) [136.2 MB] || bright-pillars-in-the-carina-nebula.hwshow [233 bytes] || ", "hits": 68 }, { "id": 30682, "url": "https://svs.gsfc.nasa.gov/30682/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T14:00:00-04:00", "title": "Star-forming Region Sharpless 2-106", "description": "A 3D visualization of the star-formonig region Sharpless 2-106 || s106-example_frame-1920x1080.png (1920x1080) [1.8 MB] || s106-example_frame-1920x1080.jpg (1920x1080) [217.2 KB] || s106-example_frame-1920x1080_searchweb.png (180x320) [74.0 KB] || s106-example_frame-1920x1080_thm.png (80x40) [6.0 KB] || s106-b-1920x1080.m4v (1920x1080) [34.8 MB] || s106-b-1920x1080.wmv (1920x1080) [35.4 MB] || s106-b-1280x720.wmv (1280x720) [21.8 MB] || s106-b-1280x720.m4v (1280x720) [21.5 MB] || s106-b-1920x1080p30.webm (1920x1080) [5.2 MB] || s106-b-30682.key [24.6 MB] || s106-b-30682.pptx [22.1 MB] || s106-b-1920x1080p30.mov (1920x1080) [134.0 MB] || star-forming-region-sharpless-2-106.hwshow [222 bytes] || ", "hits": 86 }, { "id": 30679, "url": "https://svs.gsfc.nasa.gov/30679/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T13:00:00-04:00", "title": "The Horsehead Nebula in Infrared Light", "description": "A visualization of the gaseous landscape of the Horsehead Nebula as seen in infrared light || horsehead_ir-example_frame-1920x1080.jpg (1920x1080) [273.6 KB] || horsehead_ir-example_frame-1920x1080_searchweb.png (180x320) [86.5 KB] || horsehead_ir-example_frame-1920x1080_thm.png (80x40) [15.1 KB] || horsehead_ir-b-1920x1080p30.mov (1920x1080) [91.4 MB] || horsehead_ir-b-H264_1920x1080.m4v (1920x1080) [23.2 MB] || horsehead_ir-b-WMV9_1920x1080.wmv (1920x1080) [23.9 MB] || horsehead_ir-b-H264_1280x720.m4v (1280x720) [12.3 MB] || horsehead_ir-b-WMV9_1280x720.wmv (1280x720) [14.7 MB] || horsehead_ir-b-1920x1080p30.webm (1920x1080) [3.4 MB] || horsehead_ir-b-H264_30679.key [15.6 MB] || horsehead_ir-b-H264_30679.pptx [13.1 MB] || the-horsehead-nebula-in-infrared-light.hwshow [233 bytes] || ", "hits": 116 }, { "id": 30667, "url": "https://svs.gsfc.nasa.gov/30667/", "result_type": "Hyperwall Visual", "release_date": "2015-09-24T11:00:00-04:00", "title": "Visualization of the Veil Supernova Remnant", "description": "This 3-D visualization flies across a small portion of the Veil Nebula as photographed by the Hubble Space Telescope. This region is a small part of a huge expanding remnant from a star that exploded many thousands of years ago. Hubble resolves tangled rope-like filaments of glowing gases.The 3-D model has been created for illustrative purposes and shows that that the giant bubble of gas has a thin, rippled surface. It also highlights that the emission from different chemical elements arises from different layers of gas within the nebula. In the imagery, emission from hydrogen, sulfur, and oxygen are shown in red, green, and blue, respectively. || ", "hits": 67 }, { "id": 30666, "url": "https://svs.gsfc.nasa.gov/30666/", "result_type": "Hyperwall Visual", "release_date": "2015-09-24T09:00:00-04:00", "title": "Flight to Star Cluster Westerlund 2", "description": "This visualization provides a three-dimensional perspective on Hubble's 25th anniversary image of the nebula Gum 29 with the star cluster Westerlund 2 at its core. The flight traverses the foreground stars and approaches the lower left rim of the nebula Gum 29. Passing through the wispy darker clouds on the near side, the journey reveals bright gas illuminated by the intense radiation of the newly formed stars of cluster Westerlund 2. Within the nebula, several pillars of dark, dense gas are being shaped by the energetic light and strong stellar winds from the brilliant cluster of thousands of stars. || ", "hits": 68 }, { "id": 11725, "url": "https://svs.gsfc.nasa.gov/11725/", "result_type": "Produced Video", "release_date": "2015-01-07T13:15:00-05:00", "title": "NASA Missions Take an Unparalleled Look into Superstar Eta Carinae", "description": "Explore Eta Carinae from the inside out with the help of supercomputer simulations and data from NASA satellites and ground-based observatories. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Eta_Car_Density_XY_R10_R100_STILL_1920.jpg (1920x1080) [804.4 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_print.jpg (1024x576) [52.0 KB] || Eta_Car_Density_XY_R10_R100_STILL.jpg (4928x2772) [874.1 KB] || Eta_Car_Density_XY_R10_R100_STILL.png (4928x2772) [36.6 MB] || Eta_Car_Density_XY_R10_R100_STILL_1920_web.jpg (320x180) [13.1 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_searchweb.png (320x180) [55.9 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920_thm.png (80x40) [8.0 KB] || Eta_Car_Density_XY_R10_R100_STILL_1920.tiff (1920x1080) [11.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.webm (960x540) [30.5 MB] || G2015-001_Eta_Car_Binary_Final_ipod_lg.m4v (640x360) [43.2 MB] || G2015-001_Eta_Car_Binary.en_US.vtt [5.2 KB] || G2015-001_Eta_Car_Binary.en_US.srt [5.2 KB] || G2015-001_Eta_Car_Binary_Final_ipod_sm.mp4 (320x240) [22.8 MB] || G2015-001_Eta_Car_Binary_Final_appletv_subtitles.m4v (960x540) [103.9 MB] || G2015-001_Eta_Car_Binary_Final_appletv.m4v (960x540) [104.0 MB] || G2015-001_Eta_Car_Binary_Final_1280x720.wmv (1280x720) [107.6 MB] || 11725_Eta_Car_Binary2_MPEG4_1920X1080_2997.mp4 (1920x1080) [116.9 MB] || 11725_Eta_Car_Binary2_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || 11725_Eta_Car_Binary2_H264_Best_1920x1080_2997.mov (1920x1080) [2.6 GB] || 11725_Eta_Car_Binary2_H264_Good_1920x1080_2997.mov (1920x1080) [506.2 MB] || Eta_Car_Density_XY_R10_R100_STILL.tiff (4928x2772) [104.2 MB] || ", "hits": 136 }, { "id": 11722, "url": "https://svs.gsfc.nasa.gov/11722/", "result_type": "Produced Video", "release_date": "2015-01-07T13:00:00-05:00", "title": "Supercomputer Simulations of Eta Carinae", "description": "Density simulation. This movie shows a wide view of the system looking down on the orbital plane of the two stars, which are located at the center. The view spans 3,200 times the average distance between Earth and the sun, or 298 billion miles (478 billion kilometers). Lighter colors indicate greater densities, with the highest densities occurring near the primary and in the wind interaction region. The faster wind of the smaller star carves a spiral cavity into the dense wind of the primary star, and this structure expands outward with the primary wind at about 1 million mph (1.6 million km/h. || R100_density_xy_axes_and_colorbar_print.jpg (1024x1024) [84.9 KB] || R100_density_xy_axes_and_colorbar.png (4096x4096) [2.8 MB] || R100_density_xy_axes_and_colorbar_web.jpg (320x320) [17.8 KB] || Eta_Car_R100_Density_XY_H264_Good_1024x1024_searchweb.png (320x180) [57.8 KB] || Eta_Car_R100_Density_XY_H264_Good_1024x1024.mov (1024x1024) [3.8 MB] || Eta_Car_R100_Density_XY_H264_Good_1024x1024.webm (1024x1024) [2.4 MB] || Eta_Car_R100_Density_XY_4k.mov (4096x4096) [876.4 MB] || ", "hits": 102 }, { "id": 30774, "url": "https://svs.gsfc.nasa.gov/30774/", "result_type": "Hyperwall Visual", "release_date": "2015-01-05T00:00:00-05:00", "title": "Pillars in the Eagle Nebula from Hubble (2014)", "description": "Hubble revisits the famous Pillars of Creation and reveals new details in a wider view. || eagle_pillars_2015-hst-3107x3240_print.jpg (1024x1067) [213.1 KB] || eagle_pillars_2015-hst-3107x3240.png (3107x3240) [16.6 MB] || eagle_pillars_2015-hst-6780x7071.png (6780x7071) [91.0 MB] || eagle_pillars_2015-hst-3107x3240_searchweb.png (320x180) [89.7 KB] || eagle_pillars_2015-hst-3107x3240_thm.png (80x40) [6.9 KB] || pillars-in-the-eagle-nebula-from-hubble-2014.hwshow [332 bytes] || ", "hits": 116 }, { "id": 20220, "url": "https://svs.gsfc.nasa.gov/20220/", "result_type": "Animation", "release_date": "2014-11-18T00:00:00-05:00", "title": "Bennu's Journey", "description": "Bennu's Journey is a 6-minute animated movie about NASA's OSIRIS-REx mission, asteroid Bennu, and the formation of our solar system. Born from the rubble of a violent collision, hurled through space for millions of years, asteroid Bennu has had a tough life in a rough neighborhood - the early solar system. Bennu's Journey shows what is known and what remains mysterious about the evolution of Bennu and the planets. By retrieving a sample of Bennu, OSIRIS-REx will teach us more about the raw ingredients of the solar system and our own origins.The animation was produced in an 8 x 3 aspect ratio at a resolution of 5760 x 2160 and is available in its full resolution, 4K Ultra HD, 1080HD and 720HD versions in both a letter boxed and a 16 x 9 cropped format. || ", "hits": 57 }, { "id": 20221, "url": "https://svs.gsfc.nasa.gov/20221/", "result_type": "Animation", "release_date": "2014-11-18T00:00:00-05:00", "title": "Bennu's Journey Animation Resource Page", "description": "Full resolution frames for Hyperwall || Bennus_Journey_AE_Edit_00125_print.jpg (1024x384) [27.5 KB] || Bennus_Journey_AE_Edit_00125_searchweb.png (320x180) [24.4 KB] || Bennus_Journey_AE_Edit_00125_web.png (320x120) [13.1 KB] || Bennus_Journey_AE_Edit_00125_thm.png (80x40) [2.5 KB] || BennuEditFrames30fps (5760x2160) [0 Item(s)] || ", "hits": 43 }, { "id": 20218, "url": "https://svs.gsfc.nasa.gov/20218/", "result_type": "Animation", "release_date": "2014-10-27T15:00:00-04:00", "title": "Bennu's Journey Resource Page", "description": "Bennu's Journey Poster 2 || BennuPoster01small.jpg (1286x1932) [4.6 MB] || BennuPoster01.jpg (8400x12621) [38.8 MB] || BennuPoster01small_web.png (320x480) [608.1 KB] || BennuPoster01.tif (8400x12621) [405.0 MB] || This page contains desktop wallpapers and posters for the OSIRIS-REx movie, \"Bennu's Journey.\" Check back every week for more wallpapers and posters. || ", "hits": 57 }, { "id": 11293, "url": "https://svs.gsfc.nasa.gov/11293/", "result_type": "Produced Video", "release_date": "2013-06-03T14:00:00-04:00", "title": "NASA Swift Provides the Best-Ever UV View of the Nearest Galaxies", "description": "Astronomers at NASA's Goddard Space Flight Center in Greenbelt, Md., and the Pennsylvania State University in University Park, Pa., have used NASA's Swift satellite to create the most detailed surveys of the Large and Small Magellanic Clouds, the two closest major galaxies, in ultraviolet light.Thousands of images were assembled into seamless portraits of the main body of each galaxy to produce the highest-resolution surveys of the Magellanic Clouds at ultraviolet wavelengths. The project was proposed by Stefan Immler, an astronomer at Goddard.The Large and Small Magellanic Clouds, or LMC and SMC for short, lie about 163,000 and 200,000 light-years away, respectively, and orbit each other as well as our own Milky Way galaxy. Compared to the Milky Way, the LMC has about one-tenth its physical size and only 1 percent of its mass. The SMC is only half the size of the LMC and contains about two-thirds of its mass. The new images reveal about a million ultraviolet sources within the LMC and about 250,000 in the SMC. Viewing in the ultraviolet allows astronomers to suppress the light of normal stars like the sun, which are not very bright at these higher energies, and provide a clearer picture of the hottest stars and star-formation regions. Only Swift's Ultraviolet/Optical Telescope, or UVOT, is capable of producing such high-resolution wide-field multi-color surveys in the ultraviolet. The LMC and SMC images range from 1,600 to 3,300 angstroms, UV wavelengths largely blocked by Earth's atmosphere. The Large and Small Magellanic Clouds are readily visible from the Southern Hemisphere as faint, glowing patches in the night sky. The galaxies are named after Ferdinand Magellan, the Portuguese explorer who in 1519 led an expedition to sail around the world. He and his crew were among the first Europeans to sight the objects.Watch this video on YouTube. || ", "hits": 198 }, { "id": 10874, "url": "https://svs.gsfc.nasa.gov/10874/", "result_type": "Produced Video", "release_date": "2013-04-17T16:00:00-04:00", "title": "Science in the Media Press Conference", "description": "This video supports the Science in the Media curriculum module, which culminates with students playing the role of reporters viewing this simulated press conference and writing a story about it. The findings discussed in the video are actual results from the Suzaku satellite.Science in the Media curriculum module here. || ", "hits": 47 }, { "id": 10991, "url": "https://svs.gsfc.nasa.gov/10991/", "result_type": "Produced Video", "release_date": "2012-07-03T08:00:00-04:00", "title": "A Young Star Flaunts its X-ray Spots", "description": "Using combined data from a trio of orbiting X-ray telescopes, including NASA's Chandra X-ray Observatory and the Japan-led Suzaku satellite, astronomers have obtained a rare glimpse of the powerful phenomena that accompany a still-forming star. A new study based on these observations indicates that intense magnetic fields drive torrents of gas into the stellar surface, where they heat large areas to millions of degrees. X-rays emitted by these hot spots betray the newborn star's rapid rotation.Astronomers first took notice of the young star, known as V1647 Orionis, in January 2004, near the peak of an outburst. The eruption had brightened the star so much that it illuminated a conical patch of dust now known as McNeil's Nebula. Both the star and the nebula are located about 1,300 light-years away in the constellation Orion. Astronomers quickly determined that V1647 Ori was a protostar, a stellar infant still partly swaddled in its birth cloud. Protostars have not yet developed the energy-generating capabilities of a normal star such as the sun, which fuses hydrogen into helium in its core. For V1647 Ori, that stage lies millions of years in the future. Until then, the protostar shines from the heat energy released by the gas that continues to fall onto it, much of which originates in a rotating circumstellar disk.The mass of V1647 Ori is likely only about 80 percent of the sun's, but its low density bloats it to nearly five times the sun's size. Infrared measurements show that most of the star's surface has a temperature around 6,400 degrees Fahrenheit (3,500 C), or about a third cooler than the sun's. Yet during outbursts, the protostar's X-ray brightness increases by 100 times and the temperature of its X-ray-emitting regions reaches about 90 million F (50 million C). The team found strong similarities among 11 separate X-ray light curves based on data from Chandra, Suzaku and the European Space Agency's XMM-Newton satellites. These similarities allowed them to identify cyclic X-ray variations establishing that the star spins once each day. V1647 Ori is among the youngest stars whose spin rates have been determined using an X-ray-based technique.The cyclic X-ray changes represent the appearance and disappearance of hot regions on the star that rotate in and out of view. The model that best agrees with the observations, say the researchers, involves two hot spots of unequal brightness located on opposite sides of the star. Both spots are thought to be pancake-shaped areas about the size of the sun, but the more southerly spot is about five times brighter. || ", "hits": 54 }, { "id": 10958, "url": "https://svs.gsfc.nasa.gov/10958/", "result_type": "Produced Video", "release_date": "2012-05-02T08:00:00-04:00", "title": "Pursuit of Light", "description": "Perhaps more than all other federal agencies, NASA tells stories about big things: big places, big data, big ideas. Using extraordinarily high resolution data sets from some of the most innovative and powerful scientific instruments ever built, the media team at NASA Goddard presents PURSUIT OF LIGHT. The presentation showcases top level goals of NASA's Science Mission Directorate, with an eye toward capturing the imagination of mainstream audiences. Data visualizations at resolutions far greater than HDTV present NASA's science goals like never before. Interspersed with inventive live action footage also designed to make use of that vast canvas, this six and a half minute presentation captivates and moves viewers.PURSUIT OF LIGHT was designed expressly for a screen technology called The Hyperwall, a system largely perfected at NASA Goddard Space Flight Center. The Hyperwall itself is a platform best suited for big themes. With colossal screen resolution and an ultrawide presentational style, moving images played there take on a vast sense of scale and power. PURSUIT OF LIGHT employs the strength of this remarkable system and pushes it further than ever before, presenting stories about the Earth, The Moon, The Sun, The Planets, and the deep sky, wrapped in poetic implication about the humanity's imperative need to explore. This show will play prominently on touring Hyperwalls around the country as well as on the web. || ", "hits": 37 }, { "id": 10767, "url": "https://svs.gsfc.nasa.gov/10767/", "result_type": "Produced Video", "release_date": "2011-05-11T12:00:00-04:00", "title": "NASA's Fermi Spots 'Superflares' in the Crab Nebula", "description": "The famous Crab Nebula supernova remnant has erupted in an enormous flare five times more powerful than any previously seen from the object. The outburst was first detected by NASA's Fermi Gamma-ray Space Telescope on April 12 and lasted six days.The nebula, which is the wreckage of an exploded star whose light reached Earth in 1054, is one of the most studied objects in the sky. At the heart of an expanding gas cloud lies what's left of the original star's core, a superdense neutron star that spins 30 times a second. With each rotation, the star swings intense beams of radiation toward Earth, creating the pulsed emission characteristic of spinning neutron stars (also known as pulsars). Apart from these pulses, astrophysicists regarded the Crab Nebula to be a virtually constant source of high-energy radiation. But in January, scientists associated with several orbiting observatories — including NASA's Fermi, Swift and Rossi X-ray Timing Explorer — reported long-term brightness changes at X-ray energies.Scientists think that the flares occur as the intense magnetic field near the pulsar undergoes sudden restructuring. Such changes can accelerate particles like electrons to velocities near the speed of light. As these high-speed electrons interact with the magnetic field, they emit gamma rays in a process known as synchrotron emission.To account for the observed emission, scientists say that the electrons must have energies 100 times greater than can be achieved in any particle accelerator on Earth. This makes them the highest-energy electrons known to be associated with any cosmic source.Based on the rise and fall of gamma rays during the April outbursts, scientists estimate that the size of the emitting region must be comparable in size to the solar system. If circular, the region must be smaller than roughly twice Pluto's average distance from the sun.For more Crab Nebula media go to #10708. || ", "hits": 93 }, { "id": 10708, "url": "https://svs.gsfc.nasa.gov/10708/", "result_type": "Produced Video", "release_date": "2011-01-12T12:00:00-05:00", "title": "A Flickering X-ray Candle", "description": "The Crab Nebula, created by a supernova seen nearly a thousand years ago, is one of the sky's most famous \"star wrecks.\" For decades, most astronomers have regarded it as the steadiest beacon at X-ray energies, but data from orbiting observatories show unexpected variations, showing astronomers their hard X-ray \"standard candle\" isn't as steady as they once thought. From 1999 to 2008, the Crab brightened and faded by as much as 3.5 percent a year, and since 2008, it has faded by 7 percent. The Gamma-ray Burst Monitor on NASA's Fermi satellite first detected the decline, and Fermi's Large Area Telescope also spotted two gamma-ray flares at even higher energies. Scientists think the X-rays reveal processes deep within the nebula, in a region powered by a rapidly spinning neutron star — the core of the star that blew up. But figuring out exactly where the Crab's X-rays are changing over the long term will require a new generation of X-ray telescopes. || ", "hits": 59 }, { "id": 10659, "url": "https://svs.gsfc.nasa.gov/10659/", "result_type": "Produced Video", "release_date": "2010-10-28T00:00:00-04:00", "title": "JWST Feature - Planetary Evolution", "description": "A fully produced video about planetary evolution and how the Webb Telelscope's ability to see inside dense clouds of gas and dust will help us better understand solar system formation and evolution. || ", "hits": 164 }, { "id": 30775, "url": "https://svs.gsfc.nasa.gov/30775/", "result_type": "Hyperwall Visual", "release_date": "2006-01-11T00:00:00-05:00", "title": "Hubble and Spitzer Composite of the Orion Nebula", "description": "Hubble and Spitzer collaborate to show hundreds of baby stars and strong stellar winds shaping the gas and dust of the Orion Nebula || orion_nebula_vis_ir-hst_sst-3240x3240_print.jpg (1024x1024) [228.6 KB] || orion_nebula_vis_ir-hst_sst-3240x3240.png (3240x3240) [10.9 MB] || orion_nebula_vis_ir-hst_sst-6000x6000.png (6000x6000) [41.2 MB] || orion_nebula_vis_ir-hst_sst-3240x3240_searchweb.png (320x180) [107.4 KB] || orion_nebula_vis_ir-hst_sst-3240x3240_thm.png (80x40) [22.7 KB] || hubble-and-spitzer-composite-of-the-orion-nebula.hwshow [346 bytes] || ", "hits": 96 } ] }