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    "results": [
        {
            "id": 14930,
            "url": "https://svs.gsfc.nasa.gov/14930/",
            "result_type": "Infographic",
            "release_date": "2025-12-18T10:00:00-05:00",
            "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles",
            "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel",
            "hits": 276
        },
        {
            "id": 14928,
            "url": "https://svs.gsfc.nasa.gov/14928/",
            "result_type": "Produced Video",
            "release_date": "2025-11-20T10:00:00-05:00",
            "title": "TESS Triples Size of Pleiades Star Cluster",
            "description": "These young, hot blue stars are members of the Pleiades open star cluster and reside about 430 light-years away in the northern constellation Taurus. The brightest stars are visible to the unaided eye during evenings from October to April. A new study finds the cluster to be triple the size previously thought — and shows that its stars are scattered across the night sky. The Schmidt telescope at the Palomar Observatory in California captured this color-composite image. Credit: NASA, ESA, and AURA/CaltechAlt text: Members of the Pleiades shine in blue. Image description: The Pleiades are shown in this image. Six of the stars, all blue-white, are larger than the others and have diffraction spikes and faint blue circles around them. Other, smaller blue stars are also scattered across the image. Patches of swirling blue dust surround some of the stars. || STScI-01EVVEYWX1TA3MGBK5F6EFQVGQ.jpg (4877x3513) [1.1 MB] || ",
            "hits": 488
        },
        {
            "id": 31186,
            "url": "https://svs.gsfc.nasa.gov/31186/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-08-09T00:00:00-04:00",
            "title": "Webb's Science Mission Begins: First Light Images",
            "description": "The Cartwheel Galaxy, a rare ring galaxy once shrouded in dust and mystery, has been unveiled by the imaging capabilities of NASA’s James Webb Space Telescope. The galaxy, which formed as a result of a collision between a large spiral galaxy and another smaller galaxy, not only retained a lot of its spiral character, but has also experienced massive changes throughout its structure. Webb’s high-precision instruments resolved individual stars and star-forming regions within the Cartwheel, and revealed the behavior of the black hole within its galactic center. These new details provide a renewed understanding of a galaxy in the midst of a slow transformation. || cartwheel_348_print.jpg (1024x576) [152.0 KB] || cartwheel_348.png (3840x2160) [9.1 MB] || webbs-science-mission-begins-first-light-images-cartwheel-galaxy.hwshow [314 bytes] || ",
            "hits": 97
        },
        {
            "id": 31188,
            "url": "https://svs.gsfc.nasa.gov/31188/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-08-09T00:00:00-04:00",
            "title": "Webb's Science Mission Begins: First Light Images As Compared to Hubble",
            "description": "NGC 3372: Eta Carinae Nebula || eta-carina-cliffs_1.00001_print.jpg (1024x576) [111.2 KB] || eta-carina-cliffs_1.00001_searchweb.png (320x180) [56.4 KB] || eta-carina-cliffs_1.00001_thm.png (80x40) [4.5 KB] || eta-carina-cliffs_1.mp4 (1920x1080) [17.2 MB] || eta-carina-cliffs_1.webm (1920x1080) [2.2 MB] || ",
            "hits": 66
        },
        {
            "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": 71
        },
        {
            "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": 206
        },
        {
            "id": 30948,
            "url": "https://svs.gsfc.nasa.gov/30948/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-15T15:00:00-04:00",
            "title": "Core of Globular Star Cluster Omega Centauri from Hubble",
            "description": "A close-up of stars in the core of the globular star cluster Omega Centauri from the Hubble Space Telescope. || omega_cen_core-hst-6310x3225_print.jpg (1024x523) [395.8 KB] || omega_cen_core-hst-6310x3225.png (6310x3225) [46.0 MB] || omega_cen_core-hst-6310x3225_searchweb.png (320x180) [146.6 KB] || omega_cen_core-hst-6310x3225_thm.png (80x40) [7.5 KB] || core-of-globular-star-cluster-omega-cenaturi-from-hubble.hwshow [252 bytes] || ",
            "hits": 113
        },
        {
            "id": 30947,
            "url": "https://svs.gsfc.nasa.gov/30947/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-15T14:00:00-04:00",
            "title": "Orion Nebula from Hubble",
            "description": "Orion Nebula from Hubble (2006) || orion_nebula-hst-9000x9000_print.jpg (1024x1024) [161.5 KB] || orion_nebula-hst-9000x9000.png (9000x9000) [79.3 MB] || orion_nebula-hst-9000x9000_searchweb.png (320x180) [85.2 KB] || orion_nebula-hst-9000x9000_thm.png (80x40) [6.3 KB] || orion-nebula-from-hubble.hwshow [218 bytes] || ",
            "hits": 369
        },
        {
            "id": 30858,
            "url": "https://svs.gsfc.nasa.gov/30858/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-02-28T09:00:00-05:00",
            "title": "Star Cluster Westerlund 2 in Nebula Gum 29 from Hubble",
            "description": "Star Cluster Westerlund 2 at the Heart of the Nebula Gum 29 || westerlund2-hst-4324x3240_print.jpg (1024x767) [249.9 KB] || westerlund2-hst-4324x3240.png (4324x3240) [20.5 MB] || westerlund2-hst-4324x3240_searchweb.png (320x180) [108.6 KB] || westerlund2-hst-4324x3240_thm.png (80x40) [7.4 KB] || westerlund2-hst-30858.key [21.0 MB] || westerlund2-hst-30858.pptx [20.5 MB] || ",
            "hits": 74
        },
        {
            "id": 30796,
            "url": "https://svs.gsfc.nasa.gov/30796/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-02-27T10:00:00-05:00",
            "title": "Hubble's Panoramic View of the Tarantula Nebula",
            "description": "Several million young stars are vying for attention in this NASA Hubble Space Telescope image of a raucous stellar breeding ground. Early astronomers gave the nebula its \"tarantula\" nickname because the glowing filaments of gas resemble spider legs. The nebula is located in the Large Magellanic Cloud, a small compainon galaxy to our Milky Way galaxy. This star-forming region is the brightest visible in a neighboring galaxy and is home to the most massive stars ever seen.The nebula is close enough to Earth that Hubble can resolve individual stars, giving astronomers important information about the stars' birth and evolution. It is one of only a few star-forming regions outside of our galaxy that astronomers can study in so much detail. The star-birthing frenzy may be partly fueled by its close proximity to another companion galaxy, the Small Magellanic Cloud.The image reveals the stages of star birth, from embryonic stars a few thousand years old still wrapped in cocoons of dark gas to behemoths that die young in supernova explosions. In this star-forming factory, Hubble shows star clusters of various ages, from about 2 million to about 25 million years old.The region's sparkling centerpiece is a giant, young star cluster (left of center) named NGC 2070, only 2 million years old. Its stellar inhabitants number roughly 500,000. The cluster is a hotbed for young, massive stars. Its dense core, known as R136, is packed with some of the heftiest stars found in the nearby universe, weighing more than 100 times the mass of our Sun.The massive stars are carving deep cavities in the surrounding material by unleashing a torrent of ultraviolet light, Besides sculpting the gaseous terrain, the brilliant stars also may be triggering a successive generation of offspring. When the radiation hits dense walls of gas, it creates shocks, which may be generating a new wave of star birth.The colors represent the hot gas that dominates regions of the image. Red signifies hydrogen gas and blue, oxygen. || ",
            "hits": 74
        },
        {
            "id": 30666,
            "url": "https://svs.gsfc.nasa.gov/30666/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-09-24T09:00:00-04:00",
            "title": "Flight to Star Cluster Westerlund 2",
            "description": "This visualization provides a three-dimensional perspective on Hubble's 25th anniversary image of the nebula Gum 29 with the star cluster Westerlund 2 at its core. The flight traverses the foreground stars and approaches the lower left rim of the nebula Gum 29. Passing through the wispy darker clouds on the near side, the journey reveals bright gas illuminated by the intense radiation of the newly formed stars of cluster Westerlund 2. Within the nebula, several pillars of dark, dense gas are being shaped by the energetic light and strong stellar winds from the brilliant cluster of thousands of stars. || ",
            "hits": 52
        }
    ]
}