{
    "count": 31,
    "next": null,
    "previous": null,
    "results": [
        {
            "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": 179
        },
        {
            "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": 141
        },
        {
            "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": 373
        },
        {
            "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": 54
        },
        {
            "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": 104
        },
        {
            "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": 77
        },
        {
            "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": 51
        },
        {
            "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": 286
        },
        {
            "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": 26
        },
        {
            "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": 83
        },
        {
            "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": 68
        },
        {
            "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": 113
        },
        {
            "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": 52
        },
        {
            "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": 342
        },
        {
            "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": 85
        },
        {
            "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": 129
        },
        {
            "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": 73
        },
        {
            "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": 201
        },
        {
            "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": 174
        },
        {
            "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": 255
        },
        {
            "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": 424
        },
        {
            "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": 106
        },
        {
            "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": 307
        },
        {
            "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": 64
        },
        {
            "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": 112
        },
        {
            "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": 74
        },
        {
            "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": 98
        },
        {
            "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": 74
        },
        {
            "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": 307
        },
        {
            "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": 130
        },
        {
            "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": 53
        }
    ]
}