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            "id": 14830,
            "url": "https://svs.gsfc.nasa.gov/14830/",
            "result_type": "Produced Video",
            "release_date": "2025-04-23T09:00:00-04:00",
            "title": "Carruthers Geocorona Observatory Images",
            "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ",
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        {
            "id": 13506,
            "url": "https://svs.gsfc.nasa.gov/13506/",
            "result_type": "Produced Video",
            "release_date": "2019-12-20T17:00:00-05:00",
            "title": "Solar Wind Interacting with Earth's Magnetic Field",
            "description": "A conceptual animation showing solar wind interacting with Earth's magnetic field and causing atmospheric loss at the polar cusps. || YOUTUBE_1080_13506_Atmospheric_Escape_youtube_1080.00001_print.jpg (1024x576) [77.5 KB] || YOUTUBE_1080_13506_Atmospheric_Escape_youtube_1080.00001_searchweb.png (320x180) [74.4 KB] || YOUTUBE_1080_13506_Atmospheric_Escape_youtube_1080.00001_web.png (320x180) [74.4 KB] || YOUTUBE_1080_13506_Atmospheric_Escape_youtube_1080.00001_thm.png (80x40) [6.3 KB] || YOUTUBE_1080_13506_Atmospheric_Escape_youtube_1080.mp4 (1920x1080) [43.1 MB] || FACEBOOK_720_13506_Atmospheric_Escape_facebook_720.mp4 (1280x720) [32.8 MB] || TWITTER_720_13506_Atmospheric_Escape_twitter_720.mp4 (1280x720) [5.7 MB] || FACEBOOK_720_13506_Atmospheric_Escape_facebook_720.webm (1280x720) [3.0 MB] || PRORES_B-ROLL_13506_Atmospheric_Escape_prores_b-roll.mov (1280x720) [227.8 MB] || YOUTUBE_4K_13506_Atmospheric_Escape_youtube_4k.mp4 (3840x2160) [187.6 MB] || 13506_Atmospheric_Escape_Prores.mov (3840x2160) [2.4 GB] || ",
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        {
            "id": 13514,
            "url": "https://svs.gsfc.nasa.gov/13514/",
            "result_type": "Produced Video",
            "release_date": "2019-12-20T17:00:00-05:00",
            "title": "The Cusp Aurora",
            "description": "A conceptual animation showing electrons traveling down Earth's magnetic field lines, colliding into oxygen atoms in Earth's atmosphere and causing oxygen molecules to escape and release red light causing the cusp aurora. || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.00888_print.jpg (1024x576) [70.9 KB] || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.00888_searchweb.png (320x180) [64.8 KB] || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.00888_web.png (320x180) [64.8 KB] || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.00888_thm.png (80x40) [4.4 KB] || FACEBOOK_720_13514_Cusp_Aurora_from_ground_facebook_720.mp4 (1280x720) [49.5 MB] || TWITTER_720_13514_Cusp_Aurora_from_ground_twitter_720.mp4 (1280x720) [8.0 MB] || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.webm (1920x1080) [4.9 MB] || YOUTUBE_1080_13514_Cusp_Aurora_from_ground_youtube_1080.mp4 (1920x1080) [64.2 MB] || PRORES_B-ROLL_13514_Cusp_Aurora_from_ground_prores_b-roll.mov (1280x720) [346.4 MB] || YOUTUBE_4K_13514_Cusp_Aurora_from_ground_youtube_4k.mp4 (3840x2160) [285.2 MB] || 13514_Cusp_Aurora_from_ground_Prores.mov (3840x2160) [3.9 GB] || ",
            "hits": 65
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        {
            "id": 13430,
            "url": "https://svs.gsfc.nasa.gov/13430/",
            "result_type": "Produced Video",
            "release_date": "2019-11-14T12:00:00-05:00",
            "title": "Why NASA is sending rockets into Earth’s leaky atmosphere",
            "description": "In the tiny Arctic town of Ny-Ålesund, where polar bears outnumber people, winter means three months without sunlight. The unending darkness is ideal for those who seek a strange breed of northern lights, normally obscured by daylight. When these unusual auroras shine, Earth’s atmosphere leaks into space.NASA scientists traveled to Ny-Ålesund to launch rockets through these auroras and witness oxygen particles right in the middle of their escape. Piercing these fleeting auroras, some 300 miles high, would require strategy, patience — and a fair bit of luck. This was NASA’s VISIONS-2 mission, and this is their story.VISIONS-2 was just the first of many. Over the coming months, rocket teams from all over the world will launch rockets into this region as part of the Grand Challenge Initiative—Cusp, an international collaboration to study the mysteries of the polar atmosphere. || ",
            "hits": 53
        },
        {
            "id": 12503,
            "url": "https://svs.gsfc.nasa.gov/12503/",
            "result_type": "Produced Video",
            "release_date": "2017-02-06T14:00:00-05:00",
            "title": "Planets of Red Dwarf Stars May Face Oxygen Loss in Habitable Zones",
            "description": "In this artist’s concept, X-ray and extreme ultraviolet light from a young red dwarf star cause ions to escape from an exoplanet’s atmosphere. Scientists have developed a model that estimates the oxygen ion escape rate on planets around red dwarfs, which plays an important role in determining an exoplanet’s habitability. To determine a star’s habitable zone, scientists have traditionally considered how much heat the star emits. Stars more massive than our sun produce more heat and light, so the habitable zone must be farther out. Smaller, cooler stars yield close-in habitable zones. || ExoVolcano1920x1080.00033_print.jpg (1024x576) [85.3 KB] || ExoVolcano1920x1080.00033_searchweb.png (320x180) [71.2 KB] || ExoVolcano1920x1080.00033_thm.png (80x40) [5.6 KB] || ExoVolcano1920x1080.mov (1920x1080) [6.2 GB] || ExoVolcano1920x1080Letterbox.mov (1920x1080) [6.2 GB] || NASA_TV_ExoVolcano1920x1080.mpeg (1280x720) [81.7 MB] || ExoVolcano1920x1080_appletv.m4v (1280x720) [12.8 MB] || ExoVolcano1920x1080_youtube_hq.mov (1920x1080) [25.2 MB] || NASA_TV_ExoVolcano1920x1080.webm (1280x720) [2.3 MB] || ExoVolcano1920x1080.wmv [0 bytes] || ExoVolcano1920x1080_ipod_sm.mp4 (320x240) [4.8 MB] || ",
            "hits": 108
        },
        {
            "id": 12208,
            "url": "https://svs.gsfc.nasa.gov/12208/",
            "result_type": "Produced Video",
            "release_date": "2016-06-20T09:00:00-04:00",
            "title": "The Electric Wind of Venus",
            "description": "Venus has an \"electric wind\" strong enough to remove the components of water from its upper atmosphere. This action may have played a significant role in stripping Earth's twin planet of its oceans, according to new research results from the European Space Agency's Venus Express mission led by NASA-funded researchers. Lead author of the research paper, Glyn Collinson, explains that \"electric wind\" can strip Earth-like planets of oceans and atmospheres. || ",
            "hits": 109
        }
    ]
}