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        {
            "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": 374
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        {
            "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": 332
        },
        {
            "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": 86
        },
        {
            "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": 271
        },
        {
            "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": 60
        },
        {
            "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": 50
        },
        {
            "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": 114
        },
        {
            "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": 84
        },
        {
            "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": 114
        },
        {
            "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": 91
        },
        {
            "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": 308
        },
        {
            "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": 88
        }
    ]
}