{ "count": 89, "next": null, "previous": null, "results": [ { "id": 14983, "url": "https://svs.gsfc.nasa.gov/14983/", "result_type": "Produced Video", "release_date": "2026-05-08T10:18:00-04:00", "title": "“Cosmic Echoes” Audio Activation", "description": "The experience guides listeners through a narrative journey across space exploration and science.", "hits": 310 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 347 }, { "id": 31371, "url": "https://svs.gsfc.nasa.gov/31371/", "result_type": "Hyperwall Visual", "release_date": "2026-03-10T06:59:59-04:00", "title": "Exposed Cranium", "description": "This video compares infrared views of the PMR 1 “Exposed Cranium” nebula taken by NASA’s retired Spitzer Space Telescope, as well as NASA’s James Webb Space Telecope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument).No description available.", "hits": 48 }, { "id": 31363, "url": "https://svs.gsfc.nasa.gov/31363/", "result_type": "Hyperwall Visual", "release_date": "2026-02-09T18:59:59-05:00", "title": "Observatory Comparison (Hubble/Spitzer/Webb)", "description": "This video compares images of the Helix Nebula from three NASA observatories: Hubble’s image in visible light, Spitzer’s infrared view, and Webb’s high-resolution near-infrared look.No description available.\r\n\r\nmore info: https://science.nasa.gov/asset/webb/observatory-comparison-hubble-spitzer-webb/", "hits": 93 }, { "id": 14933, "url": "https://svs.gsfc.nasa.gov/14933/", "result_type": "Produced Video", "release_date": "2025-12-04T09:00:00-05:00", "title": "XRISM Finds Elemental Bounty in Supernova Remnant", "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ", "hits": 114 }, { "id": 14866, "url": "https://svs.gsfc.nasa.gov/14866/", "result_type": "Produced Video", "release_date": "2025-07-15T00:00:00-04:00", "title": "Cosmic Desktop & Phone Wallpapers", "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||", "hits": 9250 }, { "id": 14798, "url": "https://svs.gsfc.nasa.gov/14798/", "result_type": "Produced Video", "release_date": "2025-05-27T20:56:00-04:00", "title": "Astrophysics Multiwavelength Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos that show multiwavelength content.", "hits": 102 }, { "id": 14658, "url": "https://svs.gsfc.nasa.gov/14658/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible Light || PRINT.jpg (1920x1080) [298.3 KB] || THUMB.jpg (1920x1080) [298.3 KB] || SEARCH.jpg (320x180) [27.0 KB] || Flight_Through_the_Orion_Nebula_in_Visible_Light_Dome_Version.mp4 (1920x1080) [225.5 MB] || 3840x3840_1x1_60p [0 Item(s)] || ", "hits": 81 }, { "id": 14661, "url": "https://svs.gsfc.nasa.gov/14661/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Infrared Light || PRINT.jpg (1920x1080) [206.5 KB] || THUMB.jpg (1920x1080) [206.5 KB] || SEARCH.jpg (320x180) [22.2 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.1 MB] || ", "hits": 57 }, { "id": 14662, "url": "https://svs.gsfc.nasa.gov/14662/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible and Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible and Infrared Light || PRINT.jpg (1920x1080) [159.4 KB] || THUMB.jpg (1920x1080) [159.4 KB] || SEARCH.jpg (320x180) [18.5 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Visible_and_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.3 MB] || ", "hits": 85 }, { "id": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 486 }, { "id": 14521, "url": "https://svs.gsfc.nasa.gov/14521/", "result_type": "Produced Video", "release_date": "2024-03-12T10:00:00-04:00", "title": "Using Infrared to Survey Our Galaxy’s Far Side", "description": "Observatories with smaller views of space have provided exquisite images of other galaxies, revealing complex structures. But studying our own galaxy’s anatomy is surprisingly difficult. The plane of the Milky Way covers such a large area on the sky that studying it in detail can take a very long time. Astronomers also must peer through thick dust that obscures distant starlight. Infrared light can pass through that dust and is a key tool for learning about the far side of our galaxy.Credit: NASA's Goddard Space Flight CenterMusic: \"Time Shift Equalibrium\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || GalacticPlaneIR_Split_Still.jpg (1920x1080) [430.6 KB] || GalacticPlaneIR_Split_Still_searchweb.png (320x180) [103.4 KB] || GalacticPlaneIR_Split_Still_thm.png (80x40) [7.6 KB] || 14521_Galactic_Plane_Infrared_good.mp4 (1920x1080) [51.0 MB] || 14521_GalacticPlaneIR_SRT_Captions.en_US.srt [1.0 KB] || 14521_GalacticPlaneIR_SRT_Captions.en_US.vtt [1.0 KB] || 14521_Galactic_Plane_Infrared_ProRes_1920x1080_30.mov (1920x1080) [923.1 MB] || 14521_Galactic_Plane_Infrared_Best.mp4 (1920x1080) [106.4 MB] || ", "hits": 97 }, { "id": 31273, "url": "https://svs.gsfc.nasa.gov/31273/", "result_type": "Hyperwall Visual", "release_date": "2024-01-31T00:00:00-05:00", "title": "NASA Telescopes Chase Down \"Green Monster\" in Star's Debris", "description": "Animations of images originally published at https://chandra.harvard.edu/photo/2024/casa/ and https://www.nasa.gov/image-article/nasa-telescopes-chase-down-green-monster-in-stars-debris/.Astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure called the “Green Monster”. Composite images from Chandra, Webb, Hubble, NuSTAR, and Spitzer reveal where elements such as silicon, iron, and titanium are located. Comparing where certain elements are with the location of the blast wave, researchers conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it. || ", "hits": 68 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 165 }, { "id": 14282, "url": "https://svs.gsfc.nasa.gov/14282/", "result_type": "Produced Video", "release_date": "2023-05-17T11:00:00-04:00", "title": "Spitzer, TESS Find Potential Earth-Size World Covered in Volcanoes", "description": "LP 791-18 d, illustrated here in an artist's concept, is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system. Astronomers discovered and studied the planet using data from NASA’s Spitzer Space Telescope and TESS (Transiting Exoplanet Survey Satellite) along with many other observatories.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || LP79118d_BeautyShot.jpg (2048x1152) [130.9 KB] || LP79118d_Temperate_Earth_BeautyShot_Full.jpg (5760x3240) [2.2 MB] || LP79118d_Temperate_Earth_BeautyShot_Full.png (5760x3240) [12.4 MB] || LP79118d_BeautyShot_searchweb.png (320x180) [59.9 KB] || LP79118d_BeautyShot_thm.png (80x40) [5.1 KB] || ", "hits": 77 }, { "id": 40461, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles7-echoesofthe-big-bang/", "result_type": "Gallery", "release_date": "2023-03-27T00:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "NASA studies the makeup and workings of the universe, from the smallest particles of matter and energy to its large-scale structure and evolution. Scientists look far back in space and time to learn the full cosmic history of stars and galaxies. They tease out details of the environments around black holes and observe the most powerful explosions since the big bang. NASA is discovering numerous planets beyond our solar system, decoding how planetary systems form, and learning how environments hospitable for life develop.\n\nWant to know more?\nNASA Universe Webb Space Telescope images Hubble Space Telescope", "hits": 74 }, { "id": 14259, "url": "https://svs.gsfc.nasa.gov/14259/", "result_type": "Produced Video", "release_date": "2022-12-15T10:55:00-05:00", "title": "Two Exoplanets May Be Water Worlds", "description": "Using data from NASA’s Hubble and Spitzer Space Telescopes, astronomers have found evidence that two exoplanets orbiting a star 218 light-years away are “water worlds,” where water makes up a large fraction of the entire planet.For more information, visit https://nasa.gov/hubble. Image Credit:Water World next to EarthBenoit Gougeon, Université de MontréalMusic & Sound“Space Museum” by Harry Gregson Williams [BMI] and Ho Ling Tang [BMI] via Atmosphere Music Ltd. [PRS] and Universal Production Music || ", "hits": 74 }, { "id": 31208, "url": "https://svs.gsfc.nasa.gov/31208/", "result_type": "Hyperwall Visual", "release_date": "2022-12-05T00:00:00-05:00", "title": "Webb vs Spitzer", "description": "Web vs Spitzer || Web_vs_Spitzer_00000_print.jpg (1024x576) [88.7 KB] || Web_vs_Spitzer_00000_searchweb.png (320x180) [81.9 KB] || Web_vs_Spitzer_00000_thm.png (80x40) [6.8 KB] || Web_vs_Spitzer_1080p30.mp4 (1920x1080) [38.4 MB] || Web_vs_Spitzer_1080p30.webm (1920x1080) [8.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Web_vs_Spitzer_2160p30.mp4 (3840x2160) [130.4 MB] || ", "hits": 41 }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "result_type": "Produced Video", "release_date": "2022-04-06T13:00:00-04:00", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "hits": 85 }, { "id": 13898, "url": "https://svs.gsfc.nasa.gov/13898/", "result_type": "Produced Video", "release_date": "2021-07-30T09:55:00-04:00", "title": "Lyman Spitzer: Making Space For Hubble", "description": "Seventy-five years ago, astronomer Lyman Spitzer envisioned a future for space exploration that deepened humanity’s curiosity about the cosmos. A visionary behind the Hubble Space Telescope, Spitzer was among the earliest astronomers pioneering a revolutionary way to explore the universe through astronomical satellites. His vision came over a decade before the launch of the first satellite, Sputnik, as well as the establishment of NASA itself. While the fundamental concept of sending a large telescope into space wasn’t new, the reality of doing so was.Seventy-five years ago, astronomer Lyman Spitzer envisioned a future for space exploration that deepened humanity’s curiosity about the cosmos. A visionary behind the Hubble Space Telescope, Spitzer was among the earliest astronomers pioneering a revolutionary way to explore the universe through astronomical satellites. His vision came over a decade before the launch of the first satellite, Sputnik, as well as the establishment of NASA itself. While the fundamental concept of sending a large telescope into space wasn’t new, the reality of doing so was.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Anisha Engineer: Lead WriterGrace Weikert: NarrationImage Credits of Dr. Spitzer:The Princeton Plasma Physics LaboratoryDon MortonDenise ApplewhiteMusic Credits: \"Lead Train\" by Sebastian Barnaby Robertson [BMI] and Tristan Calder [ASCAP] via Killer Tracks [BMI], Soundcast Music [SESAC], and Universal Production Music. || ", "hits": 60 }, { "id": 13737, "url": "https://svs.gsfc.nasa.gov/13737/", "result_type": "Produced Video", "release_date": "2021-04-08T14:00:00-04:00", "title": "NASA’s NICER Finds X-ray Boosts in the Crab Pulsar’s Radio Bursts", "description": "Observations from NASA’s Neutron star Interior Composition Explorer (NICER) show X-ray boosts linked in the Crab pulsar's random giant radio pulses. Watch to learn more. Credit: NASA's Goddard Space Flight CenterMusic: \"The Awakening\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Crab_Radio_Still.jpg (1920x1080) [865.4 KB] || Crab_Radio_Still_searchweb.png (320x180) [65.9 KB] || Crab_Radio_Still_thm.png (80x40) [5.2 KB] || 13737_Crab_Pulsar_Radio_Bursts_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.mp4 (1920x1080) [275.3 MB] || 13737_Crab_Pulsar_Radio_Bursts_1080.mp4 (1920x1080) [114.7 MB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.webm (1920x1080) [15.2 MB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.srt [2.6 KB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.vtt [2.6 KB] || ", "hits": 222 }, { "id": 13794, "url": "https://svs.gsfc.nasa.gov/13794/", "result_type": "Infographic", "release_date": "2021-02-12T14:00:00-05:00", "title": "NASA’s TESS Finds New Worlds in a River of Stars", "description": "This illustration sketches out the main features of TOI 451, a triple-planet system located 400 light-years away in the constellation Eridanus.Credit: NASA’s Goddard Space Flight Center || TOI_451_infographic_1920.png (1920x1080) [2.6 MB] || TOI_451_infographic_1920_print.jpg (1024x576) [129.4 KB] || TOI_451_infographic_3840.png (3840x2160) [8.2 MB] || TOI_451_infographic_1920_searchweb.png (320x180) [73.0 KB] || TOI_451_infographic_1920_thm.png (80x40) [6.5 KB] || ", "hits": 40 }, { "id": 13708, "url": "https://svs.gsfc.nasa.gov/13708/", "result_type": "Produced Video", "release_date": "2020-09-16T11:00:00-04:00", "title": "Potential Giant World Circles a Tiny Star", "description": "Watch to learn how a possible giant planet may have survived its tiny star’s chaotic history. Jupiter-size WD 1856 b is nearly seven times larger than the white dwarf it orbits every day and a half. Astronomers discovered it using data from NASA’s Transiting Exoplanet Survey Satellite and now-retired Spitzer Space Telescope.Credit: NASA/JPL-Caltech/NASA's Goddard Space Flight CenterMusic: \"Titanium\" from Killer Tracks.Complete transcript available. || wd_1856_still.jpg (1920x1080) [306.2 KB] || wd_1856_still_print.jpg (1024x576) [106.2 KB] || wd_1856_still_searchweb.png (320x180) [46.5 KB] || wd_1856_still_web.png (320x180) [46.5 KB] || wd_1856_still_thm.png (80x40) [4.2 KB] || WD_1856_HQ.mp4 (1920x1080) [279.8 MB] || WD_1856_LQ.mp4 (1920x1080) [146.4 MB] || WD_1856_prores.mov (1920x1080) [1.5 GB] || WD_1856_LQ.webm (1920x1080) [17.1 MB] || WD_1856_prores.en_US.srt [3.0 KB] || WD_1856_prores.en_US.vtt [2.9 KB] || ", "hits": 180 }, { "id": 13648, "url": "https://svs.gsfc.nasa.gov/13648/", "result_type": "Produced Video", "release_date": "2020-06-24T11:00:00-04:00", "title": "TESS, Spitzer Missions Discover a Unique Young World", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) and retired Spitzer Space Telescope have found a young Neptune-size world orbiting AU Microscopii, a cool, nearby M-type red dwarf star surrounded by a vast disk of debris. The discovery makes the system a touchstone for understanding how stars and planets form and evolve. Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Music: \"Web Of Intrigue\" from Universal Production Music.Complete transcript available. || au_mic_still.jpg (1920x1080) [286.6 KB] || au_mic_still_print.jpg (1024x576) [94.9 KB] || au_mic_still_searchweb.png (320x180) [41.3 KB] || au_mic_still_web.png (320x180) [41.3 KB] || au_mic_still_thm.png (80x40) [3.8 KB] || au_mic_HQ.mp4 (1920x1080) [112.1 MB] || au_mic_LQ.mp4 (1920x1080) [118.3 MB] || au_mic_prores.mov (1920x1080) [1.1 GB] || au_mic_LQ.webm (1920x1080) [13.1 MB] || au_mic_LQ.en_US.srt [2.2 KB] || au_mic_LQ.en_US.vtt [2.1 KB] || ", "hits": 78 }, { "id": 13496, "url": "https://svs.gsfc.nasa.gov/13496/", "result_type": "Produced Video", "release_date": "2020-01-06T19:15:00-05:00", "title": "TESS Mission’s First Earth-size World in Star’s Habitable-zone", "description": "Take a tour through TOI 700, a planetary system 100 light-years away in the constellation Dorado. One of the system’s residents is TOI 700 d, the first Earth-size habitable-zone planet discovered by NASA’s Transiting Exoplanet Survey Satellite. Credit: NASA’s Goddard Space Flight Center.Music: \"Family Tree\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TOI_700d.jpg (1920x1080) [397.4 KB] || TOI_700d_print.jpg (1024x576) [128.3 KB] || TOI_700d_searchweb.png (320x180) [65.8 KB] || TOI_700d_thm.png (80x40) [5.5 KB] || 13496_TOI700_Earth-size_1080.webm (1920x1080) [25.7 MB] || 13496_TOI700_Earth-size_1080.mp4 (1920x1080) [229.2 MB] || 13496_TOI700_Earth-size_1080_Best.mp4 (1920x1080) [394.2 MB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.srt [4.4 KB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.vtt [4.4 KB] || 13496_TOI700_Earth-size_ProRes_1920x1080.mov (1920x1080) [2.7 GB] || ", "hits": 527 }, { "id": 13294, "url": "https://svs.gsfc.nasa.gov/13294/", "result_type": "Produced Video", "release_date": "2019-08-25T09:55:00-04:00", "title": "Hubble Celebrates Spitzer's 16th Birthday", "description": "To celebrate Spitzer's 16th birthday, the Hubble Space Telescope team decided to put together a special present for their fellow \"observing buddy.\"Hubble and Spitzer have observed many of the same astronomical objects over the years; and with Spitzer getting data from infrared, and Hubble getting data from visible, ultraviolet, and some near-infrared, the two telescopes have helped uncover some of the mysteries of the universe.For more information, visit nasa.gov/hubble.Credit: NASA’s Goddard Space Flight Center / Paul MorrisMusic Credits: \"Friends Hold Fast\" by Tarek Modi [PRS]; Killer Tracks Production Music || ", "hits": 37 }, { "id": 30995, "url": "https://svs.gsfc.nasa.gov/30995/", "result_type": "Hyperwall Visual", "release_date": "2018-10-29T10:00:00-04:00", "title": "Sombrero Galaxy in Multiple Wavelengths", "description": "The Sombrero Galaxy's dust and inner flat disk are very clear in the infrared. || STScI-H-Sombrero_1x-1920x1080.00001_print.jpg (1024x576) [67.0 KB] || STScI-H-Sombrero_1x-1920x1080.00001_searchweb.png (320x180) [69.7 KB] || STScI-H-Sombrero_1x-1920x1080.00001_thm.png (80x40) [4.8 KB] || STScI-H-Sombrero_1x-1280x720.mp4 (1280x720) [3.3 MB] || STScI-H-Sombrero_1x-1920x1080.mp4 (1920x1080) [7.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-Sombrero_1x-1920x1080.webm (1920x1080) [3.9 MB] || STScI-H-Sombrero_1x-640x360.mp4 (640x360) [1.0 MB] || STScI-H-Sombrero_1x-3840x2160.mp4 (3840x2160) [6.5 MB] || STScI-H-Sombrero_1x-H265-3840x2160.mp4 (3840x2160) [2.8 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 131 }, { "id": 30994, "url": "https://svs.gsfc.nasa.gov/30994/", "result_type": "Hyperwall Visual", "release_date": "2018-10-15T10:00:00-04:00", "title": "Messier 82: Cigar Galaxy in Multiple Wavelengths", "description": "Massive burst of star formation in the core or M82 burst becomes clearer in infrared. || STScI-H-M82_1x-1920x1080.00001_print.jpg (1024x576) [79.3 KB] || STScI-H-M82_1x-1920x1080.00001_searchweb.png (320x180) [66.4 KB] || STScI-H-M82_1x-1920x1080.00001_thm.png (80x40) [4.5 KB] || STScI-H-M82_1x-1280x720.mp4 (1280x720) [5.0 MB] || STScI-H-M82_1x-1920x1080.mp4 (1920x1080) [11.8 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M82_1x-1920x1080.webm (1920x1080) [5.2 MB] || STSCI-H-M82_1x-3840x2160.mp4 (3840x2160) [12.8 MB] || STSCI-H-M82_1x-H265-3840x2160.mp4 (3840x2160) [6.0 MB] || STScI-H-M82_1x-640x360.mp4 (640x360) [1.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 157 }, { "id": 13059, "url": "https://svs.gsfc.nasa.gov/13059/", "result_type": "Produced Video", "release_date": "2018-10-04T11:00:00-04:00", "title": "Hubble Archive - Pre-Launch", "description": "This is a recorded interview from Voice of America. In this program, Dr. Fred Whipple discusses sending a telescope above the earth's atmosphere to transcend the atmosphere's obscuring of the view of space. He talks about plans for the Orbiting Astronomical Observatory (OAO,) which was a precursor to the Hubble Space Telescope.National Archive webpage: https://catalog.archives.gov/id/105636SVS webpage: https://svs.gsfc.nasa.gov/13059National Archives Identifier: 105636Local Identifier: 306.10-23Creator: U.S. Information AgencyFrom: Record Group 306: Records of the U.S. Information Agency, 1900-2003This item was broadcast 07/10/1959Production Series: New Horizons in Science || GSFC_19590710_HST_a001_thumbnail.jpg (1280x720) [49.0 KB] || GSFC_19590710_HST_a001.en_US.srt [5.8 KB] || GSFC_19590710_HST_a001.en_US.vtt [5.5 KB] || GSFC_19590710_HST_a001.mp3 [4.4 MB] || ", "hits": 79 }, { "id": 30992, "url": "https://svs.gsfc.nasa.gov/30992/", "result_type": "Hyperwall Visual", "release_date": "2018-10-01T10:00:00-04:00", "title": "Galactic Center in Multiple Infrared Wavelengths", "description": "The densely packed starfields at our galaxy's center are hidden behind dust clouds and only become visible in infrared light. || STScI-J_IRU-GalacticCenter_1x-1920x1080.00001_print.jpg (1024x576) [263.9 KB] || STScI-J_IRU-GalacticCenter_1x-1920x1080.00001_searchweb.png (320x180) [117.5 KB] || STScI-J_IRU-GalacticCenter_1x-1920x1080.00001_thm.png (80x40) [6.2 KB] || STScI-J_IRU-GalacticCenter_1x-1280x720.mp4 (1280x720) [8.0 MB] || STScI-J_IRU-GalacticCenter_1x-1920x1080.mp4 (1920x1080) [16.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J_IRU-GalacticCenter_1x-1920x1080.webm (1920x1080) [3.8 MB] || STScI-J_IRU-GalacticCenter_1x-640x360.mp4 (640x360) [2.3 MB] || STScI-J_IRU-GalacticCenter_1x-3840x2160.mp4 (3840x2160) [17.9 MB] || STScI-J_IRU-GalacticCenter_1x-H265-3840x2160.mp4 (3840x2160) [8.0 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 179 }, { "id": 30991, "url": "https://svs.gsfc.nasa.gov/30991/", "result_type": "Hyperwall Visual", "release_date": "2018-09-17T10:00:00-04:00", "title": "Mountains of Creation in Visible and Infrared", "description": "The infrared view of the \"Mountains of Creation\" reveals columns of dust sculpted by the light of young stars. || STScI-J_IRU-MtnsOfCreation_1x-1920x1080.00001_print.jpg (1024x576) [189.6 KB] || STScI-J_IRU-MtnsOfCreation_1x-1920x1080.00001_searchweb.png (320x180) [115.5 KB] || STScI-J_IRU-MtnsOfCreation_1x-1920x1080.00001_thm.png (80x40) [6.3 KB] || STScI-J_IRU-MtnsOfCreation_1x-1280x720.mp4 (1280x720) [4.3 MB] || STScI-J_IRU-MtnsOfCreation_1x-1920x1080.mp4 (1920x1080) [9.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J_IRU-MtnsOfCreation_1x-1920x1080.webm (1920x1080) [2.6 MB] || STScI-J_IRU-MtnsOfCreation_1x-640x360.mp4 (640x360) [1.3 MB] || STScI-J_IRU-MtnsOfCreation_1x-3840x2160.mp4 (3840x2160) [7.8 MB] || STScI-J_IRU-MtnsOfCreation_1x-H265-3840x2160.mp4 (3840x2160) [3.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 68 }, { "id": 30990, "url": "https://svs.gsfc.nasa.gov/30990/", "result_type": "Hyperwall Visual", "release_date": "2018-09-10T10:00:00-04:00", "title": "Andromeda Galaxy in Visible and Infrared", "description": "While Andromeda is a spiral galaxy, its dust falls largely in a huge ring structure, possibly caused by gravitational interactions with its smaller satellite galaxies. || STScI-J-Andromeda_1x-1920x1080.00001_print.jpg (1024x576) [193.1 KB] || STScI-J-Andromeda_1x-1920x1080.00001_searchweb.png (320x180) [107.5 KB] || STScI-J-Andromeda_1x-1920x1080.00001_thm.png (80x40) [5.8 KB] || STScI-J-Andromeda_1x-1280x720.mp4 (1280x720) [5.6 MB] || STScI-J-Andromeda_1x-1920x1080.mp4 (1920x1080) [13.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J-Andromeda_1x-1920x1080.webm (1920x1080) [2.7 MB] || STScI-J-Andromeda_1x-640x360.mp4 (640x360) [1.6 MB] || STScI-J-Andromeda_1x-3840x2160.mp4 (3840x2160) [11.8 MB] || STScI-J-Andromeda_1x-H265-3840x2160.mp4 (3840x2160) [6.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 8193x2410_16x9_30p (8193x2410) [0 Item(s)] || ", "hits": 327 }, { "id": 30981, "url": "https://svs.gsfc.nasa.gov/30981/", "result_type": "Hyperwall Visual", "release_date": "2018-08-20T10:00:00-04:00", "title": "Messier 81 in Multiple Wavelengths", "description": "Star-forming regions in M81 become evident in infrared. || STScI-J-M81_1x-1920x1080_0021_print.jpg (1920x1080) [580.2 KB] || STScI-J-M81_1x-1920x1080_0021_print_searchweb.png (320x180) [84.8 KB] || STScI-J-M81_1x-1920x1080_0021_print_thm.png (80x40) [6.0 KB] || STScI-J-M81_1x-1280x720.mp4 (1280x720) [5.2 MB] || STScI-J-M81_1x-1920x1080.mp4 (1920x1080) [11.2 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J-M81_1x-1920x1080.webm (1920x1080) [3.5 MB] || STScI-J-M81_1x-640x360.mp4 (640x360) [1.7 MB] || STScI-J-M81_1x-3840x2160.mp4 (3840x2160) [8.4 MB] || STScI-J-M81_1x-H265-3840x2160.mp4 (3840x2160) [4.0 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 178 }, { "id": 30980, "url": "https://svs.gsfc.nasa.gov/30980/", "result_type": "Hyperwall Visual", "release_date": "2018-08-06T10:00:00-04:00", "title": "Barred Galaxy (NGC 253) in Multiple Wavelengths", "description": "NGC 253, characterized by its vigorous star formation and spiral dust lanes, reveals its underlying structure in multiple wavelengths. || STScI-J-NGC253_1x-1920x1080.00001_print.jpg (1024x576) [54.1 KB] || STScI-J-NGC253_1x-1920x1080.00001_searchweb.png (320x180) [65.9 KB] || STScI-J-NGC253_1x-1920x1080.00001_thm.png (80x40) [4.7 KB] || STScI-J-NGC253_1x-1280x720.mp4 (1280x720) [2.7 MB] || STScI-J-NGC253_1x-1920x1080.mp4 (1920x1080) [5.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J-NGC253_1x-1920x1080.webm (1920x1080) [3.7 MB] || STScI-J-NGC253_1x-640x360.mp4 (640x360) [868.5 KB] || STScI-J-NGC253_1x-3840x2160.mp4 (3840x2160) [4.2 MB] || STScI-J-NGC253_1x-H265-3840x2160.mp4 (3840x2160) [2.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 141 }, { "id": 12949, "url": "https://svs.gsfc.nasa.gov/12949/", "result_type": "Produced Video", "release_date": "2018-07-02T13:00:00-04:00", "title": "Star Collision", "description": "Light bursts from the collision of two neutron stars. || Neutron_Star_Merger_Still_1_1024x576.jpg (1024x576) [148.9 KB] || Neutron_Star_Merger_Still_1.jpg (3840x2160) [2.4 MB] || Neutron_Star_Merger_Still_1_searchweb.png (320x180) [88.4 KB] || Neutron_Star_Merger_Still_1_thm.png (80x40) [7.3 KB] || ", "hits": 388 }, { "id": 30970, "url": "https://svs.gsfc.nasa.gov/30970/", "result_type": "Hyperwall Visual", "release_date": "2018-06-25T10:00:00-04:00", "title": "Kepler Supernova Remnant", "description": "This animation shows the remnant of Kepler's Supernova, shown first in infrared, then visible, then low energy X-ray, then high-energy X-ray emission and finally in combination. || STScI-H-KeplerSNR_1x-1920x1080.00001_print.jpg (1024x576) [18.4 KB] || STScI-H-KeplerSNR_1x-1920x1080.00001_searchweb.png (320x180) [15.9 KB] || STScI-H-KeplerSNR_1x-1920x1080.00001_thm.png (80x40) [2.1 KB] || STScI-H-KeplerSNR_1x-1280x720.mp4 (1280x720) [1.8 MB] || STScI-H-KeplerSNR_1x-1920x1080.mp4 (1920x1080) [3.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-KeplerSNR_1x-1920x1080.webm (1920x1080) [6.4 MB] || STScI-H-KeplerSNR_1x-640x360.mp4 (640x360) [708.9 KB] || STScI-H-KeplerSNR_1x-3840x2160.mp4 (3840x2160) [3.8 MB] || STScI-H-KeplerSNR_1x-H265-3840x2160.mp4 (3840x2160) [2.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 170 }, { "id": 30969, "url": "https://svs.gsfc.nasa.gov/30969/", "result_type": "Hyperwall Visual", "release_date": "2018-06-18T10:00:00-04:00", "title": "M101 (Pinwheel Galaxy)", "description": "This animation shows the Messier 101 (Pinwheel) Galaxy, with simulated rotation, in visible, then infrared, then X-ray, and finally all three combined. || STScI-H-M101_1x-1920x1080.00001_print.jpg (1024x576) [150.4 KB] || STScI-H-M101_1x-1920x1080.00001_searchweb.png (320x180) [99.4 KB] || STScI-H-M101_1x-1920x1080.00001_thm.png (80x40) [6.3 KB] || STScI-H-M101_1x-1280x720.mp4 (1280x720) [18.1 MB] || STScI-H-M101_1x-1920x1080.mp4 (1920x1080) [50.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M101_1x-1920x1080.webm (1920x1080) [5.6 MB] || STScI-H-M101_1x-640x360.mp4 (640x360) [7.8 MB] || STScI-H-M101_1x-3840x2160.mp4 (3840x2160) [32.3 MB] || STScI-H-M101_1x-H265-3840x2160.mp4 (3840x2160) [11.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 329 }, { "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": 333 }, { "id": 30961, "url": "https://svs.gsfc.nasa.gov/30961/", "result_type": "Hyperwall Visual", "release_date": "2018-06-04T10:00:00-04:00", "title": "Milky Way Center in Multiple Wavelengths", "description": "This animation reveals the center of our Milky Way galaxy, first in near-infrared, then mid-infrared, then X-ray light, and then all three in combination. || STScI-H-MWC_1x-1920x1080.00001_print.jpg (1024x576) [153.0 KB] || STScI-H-MWC_1x-1920x1080.00001_searchweb.png (320x180) [94.5 KB] || STScI-H-MWC_1x-1920x1080.00001_thm.png (80x40) [5.5 KB] || STScI-H-MWC_1x-1280x720.mp4 (1280x720) [8.4 MB] || STScI-H-MWC_1x-1920x1080.mp4 (1920x1080) [18.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-MWC_1x-1920x1080.webm (1920x1080) [4.5 MB] || STScI-H-MWC_1x-640x360.mp4 (640x360) [2.8 MB] || STScI-H-MWC_1x-3840x2160.mp4 (3840x2160) [15.7 MB] || STScI-H-MWC_1x-H265-3840x2160.mp4 (3840x2160) [8.8 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || ", "hits": 402 }, { "id": 30959, "url": "https://svs.gsfc.nasa.gov/30959/", "result_type": "Hyperwall Visual", "release_date": "2018-05-28T10:00:00-04:00", "title": "The Orion Nebula: Visible and Infrared Views", "description": "This animation showcases the Orion Nebula, first in infrared light (Spitzer), then in visible light (Hubble), and finally a blend of the two images in a multi-color mosaic. || STScI-H-Orion_1x-1920x1080.00001_print.jpg (1024x576) [71.8 KB] || STScI-H-Orion_1x-1920x1080.00001_searchweb.png (320x180) [54.4 KB] || STScI-H-Orion_1x-1920x1080.00001_thm.png (80x40) [4.1 KB] || STScI-H-Orion_1x-1280x720.mp4 (1280x720) [4.5 MB] || STScI-H-Orion_1x-1920x1080.mp4 (1920x1080) [8.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-Orion_1x-1280x720.webm (1280x720) [4.1 MB] || STScI-H-Orion_1x-640x360.mp4 (640x360) [2.1 MB] || STScI-H-Orion_1x-3840x2160.mp4 (3840x2160) [9.7 MB] || STScI-H-Orion_1x-H265_3840x2160.mp4 (3840x2160) [3.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 362 }, { "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": 244 }, { "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": 264 }, { "id": 30941, "url": "https://svs.gsfc.nasa.gov/30941/", "result_type": "Hyperwall Visual", "release_date": "2018-04-23T10:00:00-04:00", "title": "Colliding Galaxies (NGC 2207)", "description": "This animation shows the interacting galaxy pair NGC 2207, first in optical light, then in infrared, in X-ray, and finally in combination. || STScI-H-NGC2207_1x-1920x1080.00001_print.jpg (1024x576) [157.8 KB] || STScI-H-NGC2207_1x-1920x1080.00001_searchweb.png (320x180) [92.0 KB] || STScI-H-NGC2207_1x-1920x1080.00001_thm.png (80x40) [6.5 KB] || STScI-H-NGC2207_1x-1280x720.mp4 (1280x720) [4.5 MB] || STScI-H-NGC2207_1x-1920x1080.mp4 (1920x1080) [9.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-NGC2207_1x-1920x1080.webm (1920x1080) [4.9 MB] || STScI-H-NGC2207_1x-640x360.mp4 (640x360) [1.5 MB] || STScI-H-NGC2207_1x-3840x2160.mp4 (3840x2160) [8.8 MB] || STScI-H-NGC2207_1x-H265-3840x2160.mp4 (3840x2160) [4.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 245 }, { "id": 12844, "url": "https://svs.gsfc.nasa.gov/12844/", "result_type": "Produced Video", "release_date": "2018-02-05T11:00:00-05:00", "title": "Hubble Observes Atmospheres of TRAPPIST-1 Exoplanets in the Habitable Zone", "description": "Astronomers using the Hubble Space Telescope have conducted the first spectroscopic survey of Earth-sized planets in the TRAPPIST-1 system's habitable zone. Hubble reveals that at least the inner five planets do not seem to contain puffy, hydrogen-rich atmospheres similar to gaseous planets such as Neptune. This means the atmospheres may be more shallow and rich in heavier gases like carbon dioxide, methane, and oxygen.Find the full story and press release at hubblesite.org.Read the joint Hubble and Spitzer findings on nasa.gov.The science paper is available from Nature Astronomy. || ", "hits": 111 }, { "id": 12740, "url": "https://svs.gsfc.nasa.gov/12740/", "result_type": "Produced Video", "release_date": "2017-10-16T10:00:00-04:00", "title": "Doomed Neutron Stars Create Blast of Light and Gravitational Waves", "description": "This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue). Credit: NASA's Goddard Space Flight Center/CI LabMusic: \"Exploding Skies\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Neutron_Star_Merger_Still_2_new_1080.png (1920x1080) [2.5 MB] || Neutron_Star_Merger_Still_2_new_1080.jpg (1920x1080) [167.3 KB] || Neutron_Star_Merger_Still_2_new_print.jpg (1024x576) [50.4 KB] || Neutron_Star_Merger_Still_2_new.png (3840x2160) [7.7 MB] || Neutron_Star_Merger_Still_2_new.jpg (3840x2160) [1.0 MB] || Neutron_Star_Merger_Still_2_new_thm.png (80x40) [4.4 KB] || Neutron_Star_Merger_Still_2_new_searchweb.png (320x180) [51.4 KB] || 12740_NS_Merger_Update_1080.m4v (1920x1080) [50.3 MB] || 12740_NS_Merger_Update_H264_1080.mp4 (1920x1080) [96.9 MB] || 12740_NS_Merger_Update_1080p.mov (1920x1080) [101.9 MB] || NS_Merger_SRT_Captions.en_US.srt [417 bytes] || NS_Merger_SRT_Captions.en_US.vtt [399 bytes] || 12740_NS_Merger_4k_Update.webm (3840x2160) [10.0 MB] || 12740_NS_Merger_4k_Update_H264.mp4 (3840x2160) [254.9 MB] || 12740_NS_Merger_4k_Update_H264.mov (3840x2160) [516.7 MB] || 12740_NS_Merger_4k_Update_ProRes_3840x2160_5994.mov (3840x2160) [5.1 GB] || 12740_NS_Merger_4k_Update_H264.hwshow [90 bytes] || ", "hits": 1045 }, { "id": 12541, "url": "https://svs.gsfc.nasa.gov/12541/", "result_type": "Produced Video", "release_date": "2017-05-29T12:00:00-04:00", "title": "Earth-Sized Worlds", "description": "A system of seven Earth-sized exoplanets has the potential for liquid water. || ssc2017-01b_16x9_1024x576.jpg (1024x576) [99.8 KB] || ssc2017-01b_16x9_1920x1080.jpg (1920x1080) [223.9 KB] || ssc2017-01b_16x9_1920x1080_searchweb.png (320x180) [68.5 KB] || ssc2017-01b_16x9_1920x1080_thm.png (80x40) [8.2 KB] || ssc2017-01b_16x9.tif (3200x1800) [3.7 MB] || ", "hits": 40 }, { "id": 12621, "url": "https://svs.gsfc.nasa.gov/12621/", "result_type": "Produced Video", "release_date": "2017-05-25T13:00:00-04:00", "title": "Star Gives Birth to Possible Black Hole in Hubble and Spitzer Images", "description": "Music credit: \"High Heelz\" by Donn Wilkerson [BMI] and Lance Sumner [BMI]; Killer Tracks BMI; Killer Tracks Production MusicWatch this video on the NASA Goddard YouTube channel. || Hubble_black_hole_birth_thumbnail.png (1920x1080) [3.4 MB] || Hubble_black_hole_birth_thumbnail_print.jpg (1024x576) [163.2 KB] || Hubble_black_hole_birth_thumbnail_searchweb.png (320x180) [126.7 KB] || Hubble_black_hole_birth_thumbnail_thm.png (80x40) [7.9 KB] || Hubble_black_hole_birth_H264.mp4 (1920x1080) [228.3 MB] || Hubble_black_hole_birth_H264.webm (1920x1080) [26.8 MB] || Hubble_black_hole_birth_APR422.mov (1920x1080) [5.8 GB] || Hubble_black_hole_birth.en_US.srt [4.7 KB] || Hubble_black_hole_birth.en_US.vtt [4.7 KB] || ", "hits": 158 }, { "id": 40325, "url": "https://svs.gsfc.nasa.gov/gallery/tess/", "result_type": "Gallery", "release_date": "2017-05-17T00:00:00-04:00", "title": "TESS", "description": "The Transiting Exoplanet Survey Satellite\n TESS is a NASA Explorer mission launched in 2018 to study exoplanets, or planets orbiting stars outside our solar system. TESS will discover thousands of exoplanets in orbit around the brightest stars in the sky. It will monitor more than 200,000 stars, looking for temporary dips in brightness caused by planets transiting across these stars. This first-ever spaceborne all-sky transit survey will identify a wide range of planets, from Earth-sized to gas giants. The mission will find exoplanet candidates for follow-up observation from missions like the James Webb Space Telescope, which will determine whether these candidates could support life. For more information, please visit the TESS website.", "hits": 532 }, { "id": 30866, "url": "https://svs.gsfc.nasa.gov/30866/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanet Lineup", "description": "TRAPPIST-1 Exoplanets Lineup || ssc2017-01a_print.jpg (1024x512) [58.5 KB] || ssc2017-01a_searchweb.png (320x180) [29.4 KB] || ssc2017-01a_thm.png (80x40) [5.7 KB] || ssc2017-01a.tif (6000x3000) [4.1 MB] || trappist-1-exoplanet-lineup.hwshow [206 bytes] || ", "hits": 111 }, { "id": 30867, "url": "https://svs.gsfc.nasa.gov/30867/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanets Illustration", "description": "TRAPPIST-1 Exoplanets Illustration || ssc2017-01d_crop_print.jpg (1024x574) [81.6 KB] || ssc2017-01d_crop_searchweb.png (320x180) [58.9 KB] || ssc2017-01d_crop_thm.png (80x40) [6.3 KB] || ssc2017-01d_crop.tif (3600x2021) [6.0 MB] || trappist-1-exoplanets-illustration.hwshow [290 bytes] || ", "hits": 48 }, { "id": 30868, "url": "https://svs.gsfc.nasa.gov/30868/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanets Infrared Observations", "description": "TRAPPIST-1 Exoplanets Infrared Observations || ssc2017-01e_print.jpg (1024x576) [125.4 KB] || ssc2017-01e_searchweb.png (320x180) [43.5 KB] || ssc2017-01e_thm.png (80x40) [6.4 KB] || ssc2017-01e.tif (4800x2700) [1.5 MB] || trappist-1-exoplanets-infrared-observations.hwshow [289 bytes] || ", "hits": 48 }, { "id": 30869, "url": "https://svs.gsfc.nasa.gov/30869/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanets Statistics", "description": "TRAPPIST-1 Exoplanets Statistics || ssc2017-01f_print.jpg (1024x576) [105.6 KB] || ssc2017-01f_searchweb.png (320x180) [41.4 KB] || ssc2017-01f_thm.png (80x40) [6.6 KB] || ssc2017-01f.tif (6000x3375) [4.3 MB] || trappist-1-exoplanets-statistics.hwshow [211 bytes] || ", "hits": 259 }, { "id": 30870, "url": "https://svs.gsfc.nasa.gov/30870/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanets Comparison to Our Solar System", "description": "TRAPPIST-1 Exoplanets Comparison to Our Solar System || ssc2017-01g_print.jpg (1024x819) [115.0 KB] || ssc2017-01g_searchweb.png (320x180) [34.4 KB] || ssc2017-01g_thm.png (80x40) [5.8 KB] || ssc2017-01g.tif (4500x3600) [1.7 MB] || trappist-1-exoplanets-comparison-to-our-solar-system.hwshow [298 bytes] || ", "hits": 419 }, { "id": 30871, "url": "https://svs.gsfc.nasa.gov/30871/", "result_type": "Hyperwall Visual", "release_date": "2017-03-22T00:00:00-04:00", "title": "TRAPPIST-1 Exoplanets and the Habitable Zone", "description": "TRAPPIST-1 Exoplanets and the Habitable Zone || ssc2017-01h_print.jpg (1024x575) [93.1 KB] || ssc2017-01h_searchweb.png (320x180) [40.3 KB] || ssc2017-01h_thm.png (80x40) [6.7 KB] || ssc2017-01h.tif (5295x2978) [3.2 MB] || trappist-1-exoplanets-and-the-habitable-zone.hwshow [223 bytes] || ", "hits": 159 }, { "id": 12514, "url": "https://svs.gsfc.nasa.gov/12514/", "result_type": "Produced Video", "release_date": "2017-02-21T12:00:00-05:00", "title": "Exoplanet Live Shots 2.23.17", "description": "B-roll and canned interviews will be added Thursday 2/23 in the morning. Click for more about the news conference on Feb. 22nd. || Exoplanets_LS_2_print.jpg (1024x756) [714.5 KB] || Exoplanets_LS_2.jpg (2696x1992) [3.4 MB] || Exoplanets_LS_2_searchweb.png (320x180) [80.3 KB] || Exoplanets_LS_2_thm.png (80x40) [5.4 KB] || ", "hits": 40 }, { "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": 76 }, { "id": 12417, "url": "https://svs.gsfc.nasa.gov/12417/", "result_type": "Produced Video", "release_date": "2017-01-13T13:00:00-05:00", "title": "WFIRST 2017 AAS Hyperwall Presentation", "description": "New hyperwall resources for Neil Gehrels' 2017 AAS talk. Most visuals are 5760x3240 and designed for a 3x3 hyperwall with 1920x1080 screens. || ", "hits": 70 }, { "id": 30834, "url": "https://svs.gsfc.nasa.gov/30834/", "result_type": "Hyperwall Visual", "release_date": "2016-12-06T00:00:00-05:00", "title": "NASA's Astrophysics Fleet", "description": "Astrophysics Fleet || astro-fleet-spiral-07-24-2024_print.jpg (1024x575) [163.0 KB] || astro-fleet-spiral-07-24-2024.png (2560x1439) [2.0 MB] || astro-fleet-spiral-07-24-2024_searchweb.png (320x180) [85.2 KB] || astro-fleet-spiral-07-24-2024_thm.png (80x40) [7.4 KB] || nasas-astrophysics-fleet.hwshow [306 bytes] ||", "hits": 456 }, { "id": 12233, "url": "https://svs.gsfc.nasa.gov/12233/", "result_type": "Produced Video", "release_date": "2016-05-03T18:16:11-04:00", "title": "Galaxy Clusters", "description": "Explore how individual galaxies assemble into colossal cosmic communities. || c-1024.jpg (1024x576) [124.4 KB] || c-1280.jpg (1280x720) [170.2 KB] || c-1920.jpg (1920x1080) [247.3 KB] || c-1024_print.jpg (1024x576) [135.9 KB] || c-1024_searchweb.png (320x180) [82.3 KB] || c-1024_web.png (320x180) [82.3 KB] || c-1024_thm.png (80x40) [14.9 KB] || ", "hits": 114 }, { "id": 12194, "url": "https://svs.gsfc.nasa.gov/12194/", "result_type": "Produced Video", "release_date": "2016-04-07T12:55:00-04:00", "title": "The Compton Legacy: A Quarter-century of Gamma-ray Science", "description": "This illustration of the Compton Gamma Ray Observatory shows the locations of its four instruments, the Burst And Transient Source Experiment (BATSE), the Oriented Scintillation Spectrometer Experiment (OSSE), the Imaging Compton Telescope (COMPTEL), and the Energetic Gamma Ray Experiment Telescope (EGRET). Credit: NASA's Goddard Space Flight Center || GRO_cutaway_labels_1080.jpg (1920x1081) [668.9 KB] || GRO_cutaway_labels_2160.jpg (3840x2161) [5.2 MB] || GRO_cutaway_labels_2160_searchweb.png (320x180) [116.1 KB] || GRO_cutaway_labels_2160_thm.png (80x40) [12.2 KB] || ", "hits": 138 }, { "id": 12102, "url": "https://svs.gsfc.nasa.gov/12102/", "result_type": "Produced Video", "release_date": "2016-01-04T00:00:00-05:00", "title": "Fermi Hyperwall--2016 AAS, A Walk Through Fermi Science", "description": "3x3 hyperwall-resolution image of the Fermi Gamma-ray Space Telescope with instruments labeled.Credit: NASA/JIm Grossmann || Fermi_Hyperwall_2_2_Instruments_5760_print.jpg (1024x576) [86.4 KB] || Fermi_Hyperwall_2_2_Instruments_5760.png (5760x3240) [32.3 MB] || fermi-2-2-Instruments.hwshow [294 bytes] || For additional Fermi hyperwall visuals please check the second hyperwall page || ", "hits": 82 }, { "id": 40262, "url": "https://svs.gsfc.nasa.gov/gallery/hubble-space-telescope/", "result_type": "Gallery", "release_date": "2015-12-04T00:00:00-05:00", "title": "Hubble Space Telescope", "description": "Since its launch in 1990, the Hubble Space Telescope has changed our fundamental understanding of the universe. Hubble’s unique design, allowing it to be repaired and upgraded with advanced technology by astronauts, has made it one of NASA’s longest-living and most valuable observatories. Today, Hubble continues to provide views of cosmic wonders never before seen and is still at the forefront of astronomy.\nThe Hubble Space Telescope is an international collaboration between NASA and the European Space Agency (ESA).For more information visit us at https://nasa.gov/hubble or follow us on social media @NASAHubble.", "hits": 656 }, { "id": 30684, "url": "https://svs.gsfc.nasa.gov/30684/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T15:00:00-04:00", "title": "Flyby of JWST at L2 Point", "description": "A flyby of the James Webb Space Telescope at the second LaGrange point || jwst_flyby-example_frame-1920x1080.png (1920x1080) [1.4 MB] || jwst_flyby-example_frame-1920x1080.jpg (1080x1920) [148.1 KB] || jwst_flyby-example_frame-1920x1080_searchweb.png (180x320) [52.2 KB] || jwst_flyby-example_frame-1920x1080_thm.png (80x40) [4.1 KB] || jwst_flyby-b-1920x1080.wmv (1920x1080) [31.2 MB] || jwst_flyby-b-1280x720.wmv (1280x720) [19.6 MB] || jwst_flyby-b-1280x720.m4v (1280x720) [19.1 MB] || jwst_flyby-b-1920x1080.m4v (1920x1080) [31.1 MB] || jwst_flyby-b-1920x1080p24.webm (1920x1080) [4.6 MB] || jwst_flyby-b-30684.key [22.3 MB] || jwst_flyby-b-30684.pptx [19.9 MB] || jwst_flyby-b-1920x1080p24.mov (1920x1080) [176.2 MB] || flyby-of-jwst-at-l2-point.hwshow [218 bytes] || ", "hits": 48 }, { "id": 30685, "url": "https://svs.gsfc.nasa.gov/30685/", "result_type": "Hyperwall Visual", "release_date": "2015-09-25T15:00:00-04:00", "title": "Pan Past JWST at L2 Point", "description": "A pan past the James Webb Space Telescope at the second LaGrange point || jwst_pan-example_frame-1920x1080.jpg (1920x1080) [312.9 KB] || jwst_pan-example_frame-1920x1080.png (1080x1920) [2.1 MB] || jwst_pan-example_frame-1920x1080_searchweb.png (180x320) [83.9 KB] || jwst_pan-example_frame-1920x1080_thm.png (80x40) [4.6 KB] || jwst_pan-b-1280x720.wmv (1280x720) [27.4 MB] || jwst_pan-b-1280x720.m4v (1280x720) [26.8 MB] || jwst_pan-b-1920x1080.m4v (1920x1080) [43.6 MB] || jwst_pan-b-1920x1080.wmv (1920x1080) [44.4 MB] || jwst_pan-b-1920x1080p24.webm (1920x1080) [6.5 MB] || jwst_pan-b-30685.key [30.4 MB] || jwst_pan-b-30685.pptx [27.9 MB] || jwst_pan-b-1920x1080p24.mov (1920x1080) [255.7 MB] || pan-past-jwst-at-l2-point.hwshow [216 bytes] || ", "hits": 97 }, { "id": 40111, "url": "https://svs.gsfc.nasa.gov/gallery/astro-star/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Star Listing", "description": "No description available.", "hits": 77 }, { "id": 40244, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-universe/", "result_type": "Gallery", "release_date": "2015-07-24T00:00:00-04:00", "title": "Hyperwall Universe", "description": "hyperwall-ready visualizations about astrophysics\nReturn to Main Hyperwall Gallery.", "hits": 9 }, { "id": 11856, "url": "https://svs.gsfc.nasa.gov/11856/", "result_type": "B-Roll", "release_date": "2015-04-20T00:00:00-04:00", "title": "Hubble's 25th Anniversary Resource B-Roll Collection", "description": "Best of Hubble Broll includes launch and deploy, and Extravehicular Activity. || Screen_Shot_2015-04-16_at_5.33.09_PM.png (1616x903) [1.6 MB] || Screen_Shot_2015-04-16_at_5.33.09_PM_print.jpg (1024x572) [127.2 KB] || Screen_Shot_2015-04-16_at_5.33.09_PM_web.jpg (319x178) [19.9 KB] || Screen_Shot_2015-04-16_at_5.33.09_PM_searchweb.png (320x180) [87.4 KB] || Screen_Shot_2015-04-16_at_5.33.09_PM_web.png (320x178) [86.5 KB] || Screen_Shot_2015-04-16_at_5.33.09_PM_thm.png (80x40) [8.2 KB] || Best_of_Hubble_appletv.m4v (960x540) [322.7 MB] || Best_of_Hubble_youtube_hq.mov (1280x720) [1.0 GB] || Best_of_Hubble_1280x720.wmv (1280x720) [395.9 MB] || Best_of_Hubble_prores.mov (1280x720) [11.6 GB] || Best_of_Hubble_youtube_hq.webm (1280x720) [84.8 MB] || Best_of_Hubble_720x480.wmv (720x480) [366.8 MB] || Best_of_Hubble_ipod_lg.m4v (640x360) [126.5 MB] || Best_of_Hubble.mov (640x360) [322.1 MB] || Best_of_Hubble_nasaportal.mov (640x360) [322.1 MB] || Best_of_Hubble_ipod_sm.mp4 (320x240) [67.5 MB] || ", "hits": 124 }, { "id": 30570, "url": "https://svs.gsfc.nasa.gov/30570/", "result_type": "Hyperwall Visual", "release_date": "2015-01-15T00:00:00-05:00", "title": "The Long March to WFIRST", "description": "First image in presentation || 1-IRAS_allsky_big_print.jpg (1024x515) [229.0 KB] || 1-IRAS_allsky_big.jpg (2779x1400) [777.6 KB] || 1-IRAS_allsky_big_searchweb.png (320x180) [62.3 KB] || 1-IRAS_allsky_big_web.png (320x161) [53.3 KB] || 1-IRAS_allsky_big_thm.png (80x40) [8.5 KB] || george_helou_01-IRAS_allsky_big.hwshow [85 bytes] || Dr. George Helou's AAS presentation from January 2015 || ", "hits": 16 }, { "id": 30574, "url": "https://svs.gsfc.nasa.gov/30574/", "result_type": "Hyperwall Visual", "release_date": "2015-01-15T00:00:00-05:00", "title": "Science from the Frontier Fields", "description": "Frontier Fields by Steve Rodney, Johns Hopkins University. First slide in presentation. || aas225_hyperwall_rodney01_print.jpg (1024x574) [125.3 KB] || aas225_hyperwall_rodney01_web.jpg (319x179) [43.8 KB] || aas225_hyperwall_rodney01_searchweb.png (320x180) [70.2 KB] || aas225_hyperwall_rodney01_thm.png (80x40) [19.6 KB] || aas225_hyperwall_rodney01.tif (4104x2304) [10.6 MB] || aas225_hyperwall_rodney01.hwshow [96 bytes] || Dr. Steve Rodney's presentation from AAS January 2015 || ", "hits": 29 }, { "id": 30560, "url": "https://svs.gsfc.nasa.gov/30560/", "result_type": "Hyperwall Visual", "release_date": "2015-01-02T00:00:00-05:00", "title": "NASA's Spitzer Telescope Brings 360-Degree View of Galaxy to Our Fingertips", "description": "360 degree mosaic of Milky Way Galaxy || ssc2014-02a_print.jpg (1024x618) [141.1 KB] || ssc2014-02a_web.jpg (319x193) [38.6 KB] || ssc2014-02a_searchweb.png (320x180) [71.2 KB] || ssc2014-02a_web.png (320x193) [71.6 KB] || ssc2014-02a_thm.png (80x40) [19.8 KB] || ssc2014-02a.tif (4000x2417) [7.3 MB] || ssc2014-02a.hwshow [71 bytes] || ", "hits": 171 }, { "id": 11694, "url": "https://svs.gsfc.nasa.gov/11694/", "result_type": "Produced Video", "release_date": "2014-12-30T11:00:00-05:00", "title": "Galactic Hybrid", "description": "The Sombrero galaxy is not what it seems. This cosmic neighbor, also known as M104, lies 28 million light-years from our home galaxy, the Milky Way. Its thin, flat disk, rimmed by dark lanes of dust, spans 50,000 light-years and wraps around a brilliant central bulge of stars. Images of M104 taken in visible light by NASA’s Hubble Space Telescope appear to show a spiral galaxy not unlike our own. But space telescopes sensitive to other forms of light uncovered a different story. In 2012, infrared views acquired by NASA’s Spitzer spacecraft revealed M104’s disk was actually embedded within a huge, egg-shaped, or elliptical, galaxy. How the two galaxies came to be one is unknown, but the discovery may help scientists better understand the way galaxies evolve. Explore the images to see views of M104 observed in different wavelengths of light. || ", "hits": 44 }, { "id": 11594, "url": "https://svs.gsfc.nasa.gov/11594/", "result_type": "Produced Video", "release_date": "2014-08-12T11:00:00-04:00", "title": "Hidden Space", "description": "Clouds of gas and dust fill the space between the stars. Like giant puffs of smoke, these cosmic particles have a tendency to obscure objects from detection. But by using NASA's Spitzer Space Telescope, researchers can look through the clouds and see the heat radiated from distant stars, planets and even other galaxies. Since 2003, the telescope has utilized wavelengths in the infrared spectrum to uncover a hidden universe of never-before-seen places and phenomenon. Here are five mind-blowing images of the Milky Way taken by Spitzer. || ", "hits": 49 }, { "id": 11543, "url": "https://svs.gsfc.nasa.gov/11543/", "result_type": "Produced Video", "release_date": "2014-06-12T00:00:00-04:00", "title": "Galaxy Panorama", "description": "Light shining from stars in the Milky Way can take thousands of years to reach our eyes. That is, if clouds of interstellar gas and dust don’t get in the way. But dust isn’t just some astronomical nuisance. These tiny particles may one day condense into newborn stars, which may then go on to host a system of planets. Over the past 10 years, NASA’s Spitzer space telescope has snapped more than 2 million images of the Milky Way’s gas, dust and stars in infrared light—a type of light that is invisible to humans but pierces through dense cosmic clouds. Now, the images have been stitched into a seamless portrait that provides a 360-degree view of our galaxy from the perspective of Earth. Watch the video to learn more. || ", "hits": 450 }, { "id": 30467, "url": "https://svs.gsfc.nasa.gov/30467/", "result_type": "Hyperwall Visual", "release_date": "2013-11-01T12:00:00-04:00", "title": "Under the 'Wing\" of the Small Magellanic Cloud", "description": "The Small Magellanic Cloud (SMC) is one of the Milky Way's closest galactic neighbors. Even though it is a small, or so-called dwarf galaxy, the SMC is so bright that it is visible to the unaided eye from the Southern Hemisphere and near the equator. Many navigators, including Ferdinand Magellan who lends his name to the SMC, used it to help find their way across the oceans. NASA's Chandra X-ray telescope has made the first detection of X-ray emission from young solar-type stars—stars with characteristics broadly similar to those of our sun—that lie outside our Milky Way galaxy. These stars live in a region known as the \"Wing\" of the SMC. This image of the Wing is a composite that combines data from three sources into one. X-ray data from Chandra are shown in purple; optical (i.e., visible) light seen by the Hubble Space Telescope is in red, green, and blue; and infrared data from the Spitzer Space Telescope are colored red. X-rays from young stars trace the activity and strength of stellar magnetic fields. Magnetic activity provides clues to a star's convection (the rising and falling of hot gas in the star's interior) and rotation rates. The combined X-ray, optical, and infrared data also reveal, for the first time outside our galaxy, objects that resemble very young, lowmass stars, which scientists call \"young stellar objects.\" These objects have ages of a few thousand years and are still embedded in the pillar of dust and gas from which stars form.Used in 2014 Calendar. || ", "hits": 84 }, { "id": 30099, "url": "https://svs.gsfc.nasa.gov/30099/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "A Far Away Star Cluster", "description": "High-mass stars are important because they are responsible for much of the energy pumped into a galaxy over its lifetime. Unfortunately, these stars aren’t understood very well because they are usually found relatively far away in places where lots of gas and dust impede our view. This star cluster (NGC 281) however, is an exception since it is far enough away from the plane of our galaxy that not a lot of dust and gas obscure its view. The high-mass stars have powerful winds flowing from their surfaces and intense radiation that heats surrounding gas, boiling it away into interstellar space. This process results in the formation of the large columns of gas and dust seen on the left side of the image. These structures likely contain newly forming stars. The eventual deaths of massive stars as supernovas will also seed the galaxy with material and energy. Here we see NGC 281 in X-rays from Chandra and infrared data from Spitzer. || ", "hits": 17 }, { "id": 30100, "url": "https://svs.gsfc.nasa.gov/30100/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "Solving Mysteries in Space", "description": "In 185 A.D., Chinese astronomers noted a \"guest star\" that mysteriously appeared in the sky and stayed for about 8 months. By the 1960s, scientists had determined that the mysterious object was, in fact, a supernova. Later, they figured out that this supernova remnant, now known as RCW 86, was located about 8,000 light years away. Today, astronomers have taken data from four different telescopes to make this stunning new image. Here, X-rays from Chandra and XMM-Newton have been combined with infrared data from the Spitzer Space Telescope and the WISE mission. These data show that the explosion from nearly 2,000 years ago was caused by a so-called Type 1A supernova. This type of supernova happens when a white dwarf star pulls too much material from a companion star, causing a thermonuclear explosion to go off. || ", "hits": 39 }, { "id": 30111, "url": "https://svs.gsfc.nasa.gov/30111/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "The Largest-Known Spiral Galaxy", "description": "The spectacular barred spiral galaxy NGC 6872 has ranked among the biggest stellar systems for decades. This enormous spiral is 522,000 light-years across from the tip of one outstretched arm to the tip of the other, making it about five times the size of our home galaxy, the Milky Way. The galaxy's unusual size and appearance stem from interaction with a much smaller disk galaxy named IC 4970 (circled in yellow), which has only about one-fifth the mass of NGC 6872. This previously unsuspected tidal dwarf galaxy candidate appears only in the ultraviolet. The odd couple is located 212 million light-years from Earth in the southern constellation Pavo. This composite image of the giant barred spiral galaxy NGC 6872 combines ultraviolet data from NASA's Galaxy Evolution Explorer (GALEX) and infrared data acquired by NASA's Spitzer Space Telescope with visible light images from the European Southern Observatory's Very Large Telescope. Images of lower resolution from the Digital Sky Survey were used to fill in marginal areas not covered by the other data. || ", "hits": 200 }, { "id": 30142, "url": "https://svs.gsfc.nasa.gov/30142/", "result_type": "Hyperwall Visual", "release_date": "2013-10-17T12:00:00-04:00", "title": "W3 Star-Forming Complex in Perseus by Spitzer and SOFIA", "description": "This mid-infrared image of the W3A star cluster in the inset was captured by the FORCAST camera on the SOFIA flying observatory in 2011. It is overlaid on a near-infrared image of the W3 star-forming region from the Spitzer space telescope. The SOFIA image scale is 150 x 100 arcseconds, and the red, green and blue colors represent 37, 20 and 7 μm. The red, green and blue colors in the background image from Spitzer represent 7.9, 4.5, 3.6 μm. || ", "hits": 16 }, { "id": 11298, "url": "https://svs.gsfc.nasa.gov/11298/", "result_type": "Produced Video", "release_date": "2013-06-28T00:00:00-04:00", "title": "Sun Emits a Solstice CME", "description": "On June 20, 2013, at 11:24 p.m., the sun erupted with an Earth-directed coronal mass ejection or CME, a solar phenomenon that can send billions of tons of particles into space that can reach Earth one to three days later. These particles cannot travel through the atmosphere to harm humans on Earth, but they can affect electronic systems in satellites and on the ground. Experimental NASA research models, based on observations from NASA's Solar Terrestrial Relations Observatory and ESA/NASA's Solar and Heliospheric Observatory show that the CME left the sun at speeds of around 1350 miles per second, which is a fast speed for CMEs. Earth-directed CMEs can cause a space weather phenomenon called a geomagnetic storm, which occurs when they funnel energy into Earth's magnetic envelope, the magnetosphere, for an extended period of time. The CME's magnetic fields peel back the outermost layers of Earth's fields changing their very shape. Magnetic storms can degrade communication signals and cause unexpected electrical surges in power grids. They also can cause aurora. Storms are rare during solar minimum, but as the sun's activity ramps up every 11 years toward solar maximum—currently expected in late 2013—large storms occur several times per year.In the past, geomagnetic storms caused by CMEs of this strength and direction have usually been mild. In addition, the CME may pass by additional spacecraft: Messenger, STEREO B, Spitzer, and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from the solar material. || ", "hits": 135 }, { "id": 11285, "url": "https://svs.gsfc.nasa.gov/11285/", "result_type": "Produced Video", "release_date": "2013-05-13T10:30:00-04:00", "title": "First X-Class Solar Flares of 2013", "description": "On May 13, 2013, the sun emitted an X2.8-class flare, peaking at 12:05 p.m. EDT. This is the the strongest X-class flare of 2013 so far, surpassing in strength the X1.7-class flare that occurred 14 hours earlier. It is the 16th X-class flare of the current solar cycle and the third-largest flare of that cycle. The second-strongest was an X5.4 event on March 7, 2012. The strongest was an X6.9 on Aug. 9, 2011.On May 12, 2013, the sun emitted a significant solar flare, peaking at 10 p.m. EDT. This flare is classified as an X1.7, making it the first X-class flare of 2013. The flare was also associated with another solar phenomenon, called a coronal mass ejection (CME) that can send solar material out into space. This CME was not Earth-directed. The May 12 flare was also associated with a coronal mass ejection, another solar phenomenon that can send billions of tons of solar particles into space, which can affect electronic systems in satellites and on the ground. Experimental NASA research models show that the CME left the sun at 745 miles per second and is not Earth-directed, however its flank may pass by the STEREO-B and Spitzer spacecraft, and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from solar material. There is some particle radiation associated with this event, which is what can concern operators of interplanetary spacecraft since the particles can trip computer electronics on board. || ", "hits": 160 }, { "id": 11236, "url": "https://svs.gsfc.nasa.gov/11236/", "result_type": "Produced Video", "release_date": "2013-04-18T00:00:00-04:00", "title": "Flash In The Dark", "description": "A distant object suddenly bursts with light, then darkens. Space telescopes Spitzer and Hubble have watched this phenomenon repeat like clockwork every 25 days. The light appears to emanate from a protostar named LRLL 54361. It is not the first object to blink in this unusual way, but it is both the brightest and the most regular one ever observed. Astronomers think LRLL 54361 may actually consist of two newborn stars in a binary system. Drawn together by gravity, they circle around each other, kicking up nearby dust and gas. This material then slams back into the stars, causing a blast of radiation and—there!—a flash of bright light. If this theory holds true, LRLL 54361 will teach us more about how binary stars form. Watch the video to see its light flash at increased speed in a time-lapse sequence of images from the Hubble Space Telescope. || ", "hits": 33 }, { "id": 11209, "url": "https://svs.gsfc.nasa.gov/11209/", "result_type": "Produced Video", "release_date": "2013-02-14T14:00:00-05:00", "title": "Fermi Proves Supernova Remnants Produce Cosmic Rays", "description": "A new study using observations from NASA's Fermi Gamma-ray Space Telescope reveals the first clear-cut evidence that the expanding debris of exploded stars produces some of the fastest-moving matter in the universe. This discovery is a major step toward meeting one of Fermi's primary mission goals.Cosmic rays are subatomic particles that move through space at nearly the speed of light. About 90 percent of them are protons, with the remainder consisting of electrons and atomic nuclei. In their journey across the galaxy, the electrically charged particles become deflected by magnetic fields. This scrambles their paths and makes it impossible to trace their origins directly.Through a variety of mechanisms, these speedy particles can lead to the emission of gamma rays, the most powerful form of light and a signal that travels to us directly from its sources.Two supernova remnants, known as IC 443 and W44, are expanding into cold, dense clouds of interstellar gas. This material emits gamma rays when struck by high-speed particles escaping the remnants.Scientists have been unable to ascertain which particle is responsible for this emission because cosmic-ray protons and electrons give rise to gamma rays with similar energies. Now, after analyzing four years of data, Fermi scientists see a gamma-ray feature from both remnants that, like a fingerprint, proves the culprits are protons.When cosmic-ray protons smash into normal protons, they produce a short-lived particle called a neutral pion. The pion quickly decays into a pair of gamma rays. This emission falls within a specific band of energies associated with the rest mass of the neutral pion, and it declines steeply toward lower energies. Detecting this low-end cutoff is clear proof that the gamma rays arise from decaying pions formed by protons accelerated within the supernova remnants.In 1949, the Fermi telescope's namesake, physicist Enrico Fermi, suggested that the highest-energy cosmic rays were accelerated in the magnetic fields of interstellar gas clouds. In the decades that followed, astronomers showed that supernova remnants were the galaxy's best candidate sites for this process.?A charged particle trapped in a supernova remnant's magnetic field moves randomly throughout it and occasionally crosses through the explosion's leading shock wave. Each round trip through the shock ramps up the particle's speed by about 1 percent. After many crossings, the particle obtains enough energy to break free and escapes into the galaxy as a newborn cosmic ray. The Fermi discovery builds on a strong hint of neutral pion decay in W44 observed by the Italian Space Agency's AGILE gamma-ray observatory and published in late 2011.Watch this video on YouTube. || ", "hits": 147 }, { "id": 11116, "url": "https://svs.gsfc.nasa.gov/11116/", "result_type": "Produced Video", "release_date": "2012-10-25T10:00:00-04:00", "title": "Reviving Fomalhaut b", "description": "A second look at data from NASA's Hubble Space Telescope is reanimating the claim that the nearby star Fomalhaut hosts a massive exoplanet. The study suggests that the planet, named Fomalhaut b, is a rare and possibly unique object that is completely shrouded by dust. Fomalhaut is the brightest star in the constellation Piscis Austrinus and lies 25 light-years away. In November 2008, Hubble astronomers announced the exoplanet, named Fomalhaut b, as the first one ever directly imaged in visible light around another star. The object was imaged just inside a vast ring of debris surrounding but offset from the host star. The planet's location and mass — about three times Jupiter's — seemed just right for its gravity to explain the ring's appearance. Recent studies have claimed that this planetary interpretation is incorrect. Based on the object's apparent motion and the lack of an infrared detection by NASA's Spitzer Space Telescope, they argue that the object is a short-lived dust cloud unrelated to any planet. A new analysis, however, brings the planet conclusion back to life.Watch this video on YouTube. || ", "hits": 138 }, { "id": 11080, "url": "https://svs.gsfc.nasa.gov/11080/", "result_type": "Produced Video", "release_date": "2012-09-20T00:00:00-04:00", "title": "Inside Out", "description": "What happens when a star explodes? Astronomers sorting through pieces of a star that burst about 330 years ago discovered it might have blown up from the inside out. Data from ground-based observatories and NASA's Chandra and Spitzer space telescopes reveal material forged deep inside the star, such as iron, was on the outer edge of the explosion. The blast, called a supernova, takes place when a massive star runs out of fuel and collapses under its own gravity. This process ignites a runaway nuclear reaction that can outshine a hundred billion suns. The explosion, meanwhile, can launch elements into space—including those found in the star's core—that give rise to new stars, planets and even life. Watch the video to see how astronomers pieced together the inside-out nature of the explosion by mapping the trail of elements it left behind. || ", "hits": 55 }, { "id": 30135, "url": "https://svs.gsfc.nasa.gov/30135/", "result_type": "Hyperwall Visual", "release_date": "2011-11-30T12:00:00-05:00", "title": "SOFIA views a star-forming region", "description": "The name W40 designates this object's number in a catalog of HII regions, clouds of ionized hydrogen often associated with star formation and massive stars. W40 is in the constellation Aquila the Eagle, visible in the Northern hemisphere's autumn sky. W40 itself is a difficult target for optical astronomers because it lies less than 3 degrees from the central plane of the Milky Way, at a distance of about 1600 light years behind obscuring clouds of interstellar dust and gas.This three image comparison shows W40 in visible, near-infrared and mid-infrared wavelengths. The visible-light image on the left is from the Digitized Sky Survey. The W40 region is not especially prominent at visual wavelengths due to intervening interstellar dust. The near-infrared image in the middle is a composite produced by SOFIA Basic Science Principal Investigators Shuping and Vacca using archived Spitzer infrared space telescope data. The interstellar dust in the foreground and within the W40 region is mostly transparent at these wavelengths, so W40 stands out prominently and one can view into the interior of the nebula to see embedded protostars. Some of these objects were labeled with IRS (\"InfraRed Source\") numbers by earlier investigators. The mid-infrared image on the right is a composite of 5.4 micron (blue), 24.2 micron (green) and 34.8 micron (red) images taken with SOFIA's FORCAST camera in May 2011.The field of view is approximate 3 arcminutes on a side. The bright sources in this image are protostars and thermal emission from dust and gas. Emission at 24 and 35 microns is primarily from warm dust. Some of the protostars can be seen in the Spitzer near-infrared image, but the SOFIA data allow easier determination of their dust temperatures. The hottest object, appearing blue and located at lower left, has very little dust surrounding it and is likely nearest to completing its evolution into a fully-fledged star. The other protostars represented by white in this color balance are cooler and thus have a large amount of circumstellar dust, some of it probably in a disk surrounding the central star. || ", "hits": 35 }, { "id": 40073, "url": "https://svs.gsfc.nasa.gov/gallery/astro/", "result_type": "Gallery", "release_date": "2010-07-12T00:00:00-04:00", "title": "Goddard's Astrophysics Gallery", "description": "This multimedia gallery assembles and organizes the astrophysics content on the Scientific Visualization Studio website. All of NASA's Goddard Space Flight Center's animations, visualizations, videos and still images relating to the universe beyond our Solar System are here. Browse through the basic categories or find Goddard's most recent releases under each specific astronomical feature. Find all the content relating to a particular satellite under \"Missions.\" Most entries have multiple downloadable formats and several resolutions.", "hits": 348 }, { "id": 10566, "url": "https://svs.gsfc.nasa.gov/10566/", "result_type": "Produced Video", "release_date": "2010-02-13T00:00:00-05:00", "title": "Fermi Explores Supernova Remnants", "description": "Fermi's Large Area Telescope (LAT) resolved gamma rays with energies a billion times greater than that of visible light from supernova remnants of different ages and in different environments. W51C, W44 and IC 443 are middle-aged remnants between 4,000 and 30,000 years old. The youngest remnant, Cassiopeia A, is only 330 years old and appears to the LAT as a point source. The images bring astronomers a step closer to understanding the source of some of the universe's most energetic particles — cosmic rays. The emissions are likely the result of accelerated protons interacting with nearby gas clouds, but other possibilities have not been eliminated. Astrophysicists believe that supernova remnants are the galaxy's best candidate sites for cosmic-ray acceleration. These observations provide further validation to the notion that supernova remnants act as enormous accelerators for cosmic particles. || ", "hits": 72 }, { "id": 10374, "url": "https://svs.gsfc.nasa.gov/10374/", "result_type": "Produced Video", "release_date": "2009-01-28T01:00:00-05:00", "title": "Spitzer Exoplanet Observation of HD 80606b", "description": "HD 80606b is a gas giant planet in an eccentric orbit around its star. Every 111 days, the planet passes within 2.8 million miles of the star's surface. During the close approach of Nov. 20, 2007, NASA's Spitzer Space Telescope observed the system for 30 hours. Scientists modeled the response of the planet's upper atmosphere to the extreme heating. The animation based on their simulations begins 4.4 days after closest approach, when the hot hemisphere has rotated into view. A massive storm has formed in response to the pulse of heat delivered during the planet's close swing past its star. Successive frames, spaced every 12 hours, show the hot spot rotating out of view. The Spitzer observations represent the first time astronomers have detected weather changes in real time on a planet outside our solar system. || ", "hits": 78 }, { "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": 40 } ] }