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            "description": "B-roll package that corresponds to the following:<p><u><b>SUGGESTED QUESTIONS</b></u><p>What is a black hole and what did NASA and its partners discover?<p>How does a black hole destroy a star?<p>How did NASA and other observatories work together to capture this moment?<p>What new things did we learn from this catastrophic event?<p>How far away is this black hole? Could our Sun be eaten by a black hole?<p>Black holes are black right? How do scientists study something that can’t be seen?Where can we learn more?<p><p><u><b>QUESTIONS FOR LONGER INTERVIEWS:</b></u><p>How does a planet-hunting mission help us learn about black holes?<p>How did the scientists involved first learn about the event?<p>What is #BlackHoleWeek?<p><p><u><b>QUICK LINKS TO VIDEO AND AUDIO</u></b><p>Click for downloadable <a href=\"/13321#28068\">AUDIO SOUNDBITE</a> with NASA Scientist Knicole Colon.<p>Click for downloadable soundbites with <a href=\"/13321#28069\">NASA Scientist Knicole Colon</a><p>Click for downloadable soundbites with <a href=\"/13321#28070\">NASA Scientist Brad Cenko</a><p><p>Click for downloadable soundbites with <a href=\"/13321#28072\">Carnegie astronomer Tom Holoien</a>.",
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            "description": "<center><b>Observatories Collaborate to Catch Star-Gobbling Black Hole<br>NASA’s TESS Sees Its First Star-destroying Black Hole<br>Rare Black Hole Event Sheds Light on a Cosmic Mystery</center></b> <br>For the first time, NASA’s Transiting Exoplanet Survey Satellite (TESS) watched a black hole shred apart and devour a distant star from the moment the violent event began. This phenomenon only happens about once every 10,000 to 100,000 years in a galaxy the size of our own Milky Way!<br> <br>So what is a black hole and how hard is it to watch one destroy a star? Chat with scientists on Friday, Sept. 27, from 6:00 a.m. to 1:30 p.m. EDT to find out how they work together to spot these rare cosmic events and what we’re learning about them. Skype interviews are also available. HERE’s a link to the <a href=\"https://www.nasa.gov/feature/goddard/2019/nasa-s-tess-mission-spots-its-1st-star-shredding-black-hole\" target=\"_blank\">FEATURE STORY</a>. And HERE for a version of it in <a href=\"https://ciencia.nasa.gov/la-misión-tess-de-la-nasa-detecta-su-primer-agujero-negro-desgarrando-una-estrella-0\" target=\"_blank\">Spanish</a>.<br> <br>Scientists know black holes are integral to the life cycle of galaxies, but they’re incredibly difficult to study. Thanks to identification and coordination by the All-Sky Automated Survey for Supernovae [ASAS-SN, pronounced like “assassin”] and observations by TESS and other missions, including NASA’s Neil Gehrels Swift Observatory, astrophysicists are a step closer to understanding some of the most mysterious objects in the universe. <br><br><b><u>Schedule an Interview</u></b> <br>To schedule an interview please fill out our form: <a href=\"https://forms.gle/rH7Ct9LWqETGB1gC7\" target=\"_blank\">https://forms.gle/rH7Ct9LWqETGB1gC7</a><br>Interview location: NASA’s Goddard Space Flight Center in Greenbelt, Maryland<br> <br><b><u>Satellite Coordinates</u></b><br><b><font color=\"red\">HD Satellite Coordinates for G17-K18/Lower: Galaxy 17 Ku-band Xp 18 Slot Lower| 91.0 ° W Longitude | DL 12051.0 MHz | Vertical Polarity | QPSK/DVB-S | FEC 3/4 | SR 13.235 Mbps | DR 18.2954 MHz | HD 720p | Format MPEG2 | Chroma Level 4:2:0 | Audio Embedded</font></b><br> <br><b><u>Media contacts for partner institutions:</u></b><br>Natasha Metzler / Carnegie Institution, Strategic Communications/ nmetzler@carnegiescience.edu/ (202) 939-1142<br>Laura Arenschield / The Ohio State University, Research Communications / Arenschield.2@osu.edu<br><br>For more information check out <a href=\"https://twitter.com/NASAUniverse\" target=\"_blank\">@NASAUniverse</a> and <a href=\"https://twitter.com/search?q=%23BlackHoleWeek&src=typed_query\" target=\"_blank\">#BlackHoleWeek</a><br> <br>Questions? Contact michelle.z.handleman@nasa.gov or 301-286-0918.",
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    ],
    "missions": [],
    "series": [
        "Astrophysics Presentations",
        "Black Hole Week",
        "Narrated Movies"
    ],
    "tapes": [],
    "papers": [],
    "datasets": [],
    "nasa_science_categories": [
        "Universe"
    ],
    "keywords": [
        "Ast",
        "Astrophysics",
        "Black Hole",
        "HDTV",
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    "recommended_pages": [],
    "related": [
        {
            "id": 13326,
            "url": "https://svs.gsfc.nasa.gov/13326/",
            "page_type": "Produced Video",
            "title": "Black Hole Accretion Disk Visualization",
            "description": "This movie shows a complete revolution around a simulated black hole and its accretion disk following a path that is perpendicular to the disk. The black hole’s extreme gravitational field redirects and distorts light coming from different parts of the disk, but exactly what we see depends on our viewing angle. The greatest distortion occurs when viewing the system nearly edgewise.  As our viewpoint rotates around the black hole, we see different parts of the fast-moving gas in the accretion disk moving directly toward us. Due to a phenomenon called \"relativistic Doppler beaming,\" gas in the disk that's moving toward us makes that side of the disk appear brighter, the opposite side darker. This effect disappears when we're directly above or below the disk because, from that angle, none of the gas is moving directly toward us.When our viewpoint passes beneath the disk, it looks like the gas is moving in the opposite direction. This is no different that viewing a clock from behind, which would make it look like the hands are moving counter-clockwise.CORRECTION: In earlier versions of the 360-degree movies on this page, these important effects were not apparent. This was due to a minor mistake in orienting the camera relative to the disk. The fact that it was not initially discovered by the NASA scientist who made the movie reflects just how bizarre and counter-intuitive black holes can be! Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman || BH_Accretion_Disk_Sim_360_4k_Prores.00001_print.jpg (1024x1024) [33.2 KB] || BH_Accretion_Disk_Sim_360_4k_Prores.00001_searchweb.png (320x180) [17.0 KB] || BH_Accretion_Disk_Sim_360_4k_Prores.00001_thm.png (80x40) [1.9 KB] || BH_Accretion_Disk_Sim_360_1080.mp4 (1080x1080) [19.0 MB] || BH_Accretion_Disk_Sim_360_1080.webm (1080x1080) [2.8 MB] || 360 (3840x3840) [0 Item(s)] || BH_Accretion_Disk_Sim_360_4k.mp4 (3840x3840) [119.2 MB] || BH_Accretion_Disk_Sim_360_4k_Prores.mov (3840x3840) [1020.1 MB] || ",
            "release_date": "2019-09-25T13:00:00-04:00",
            "update_date": "2024-08-14T22:44:35.426607-04:00",
            "main_image": {
                "id": 392576,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013300/a013326/BH_Accretion_Disk_Sim_360_4k_Prores.00001_print.jpg",
                "filename": "BH_Accretion_Disk_Sim_360_4k_Prores.00001_print.jpg",
                "media_type": "Image",
                "alt_text": "This movie shows a complete revolution around a simulated black hole and its accretion disk following a path that is perpendicular to the disk. The black hole’s extreme gravitational field redirects and distorts light coming from different parts of the disk, but exactly what we see depends on our viewing angle. The greatest distortion occurs when viewing the system nearly edgewise.  As our viewpoint rotates around the black hole, we see different parts of the fast-moving gas in the accretion disk moving directly toward us. Due to a phenomenon called \"relativistic Doppler beaming,\" gas in the disk that's moving toward us makes that side of the disk appear brighter, the opposite side darker. This effect disappears when we're directly above or below the disk because, from that angle, none of the gas is moving directly toward us.When our viewpoint passes beneath the disk, it looks like the gas is moving in the opposite direction. This is no different that viewing a clock from behind, which would make it look like the hands are moving counter-clockwise.CORRECTION: In earlier versions of the 360-degree movies on this page, these important effects were not apparent. This was due to a minor mistake in orienting the camera relative to the disk. The fact that it was not initially discovered by the NASA scientist who made the movie reflects just how bizarre and counter-intuitive black holes can be! Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman",
                "width": 1024,
                "height": 1024,
                "pixels": 1048576
            }
        },
        {
            "id": 13239,
            "url": "https://svs.gsfc.nasa.gov/13239/",
            "page_type": "Produced Video",
            "title": "Zoom In on Galaxy M87",
            "description": "This movie zooms into galaxy M87 using real visible light, X-ray and radio pictures of the galaxy, its jet of high-speed particles, and the shadow of its central black hole. || ",
            "release_date": "2019-09-24T09:00:00-04:00",
            "update_date": "2023-05-03T13:45:37.786185-04:00",
            "main_image": {
                "id": 392438,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013200/a013239/m87_thumb_01.png",
                "filename": "m87_thumb_01.png",
                "media_type": "Image",
                "alt_text": "This movie is available both with and without on-screen text.Credit: NASA's Goddard Space Flight CenterMusic: \"Tension Underlying\" from Universal Production Music",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 13238,
            "url": "https://svs.gsfc.nasa.gov/13238/",
            "page_type": "Produced Video",
            "title": "Highlights From TESS's First Year",
            "description": "Here are highlights from TESS's first year of science operations.  All exoplanet animations are illustrations.Credit: NASA's Goddard Space Flight CenterMusic: \"Elapsing Time\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_First_Year_Still.jpg (1920x1080) [515.9 KB] || TESS_First_Year_Still_print.jpg (1024x576) [182.2 KB] || TESS_First_Year_Still_searchweb.png (320x180) [70.7 KB] || TESS_First_Year_Still_thm.png (80x40) [5.3 KB] || 13238_TESS_First_Year_ProRes_1920x1080.mov (1920x1080) [2.4 GB] || 13238_TESS_First_Year_Best.mp4 (1920x1080) [483.9 MB] || 13238_TESS_First_Year_Good.mp4 (1920x1080) [184.7 MB] || 13238_TESS_First_Year_ProRes_1920x1080.webm (1920x1080) [20.0 MB] || TESS_First_Year_SRT_Captions.en_US.srt [3.7 KB] || TESS_First_Year_SRT_Captions.en_US.vtt [3.7 KB] || ",
            "release_date": "2019-07-25T09:50:00-04:00",
            "update_date": "2023-05-03T13:45:46.958727-04:00",
            "main_image": {
                "id": 394894,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013200/a013238/TESS_First_Year_Still.jpg",
                "filename": "TESS_First_Year_Still.jpg",
                "media_type": "Image",
                "alt_text": "Here are highlights from TESS's first year of science operations.  All exoplanet animations are illustrations.Credit: NASA's Goddard Space Flight CenterMusic: \"Elapsing Time\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 12855,
            "url": "https://svs.gsfc.nasa.gov/12855/",
            "page_type": "Produced Video",
            "title": "Mysterious ‘Cow’ Blast Studied with NASA Telescopes",
            "description": "Watch what scientists think happens when a black hole tears apart a hot, dense white dwarf star. A team working with observations from NASA’s Neil Gehrels Swift Observatory suggest this process explains a mysterious outburst known as AT2018cow. Credit: NASA's Goddard Space Flight CenterMusic: \"Curious Events\" from Killer TracksWatch this video on the JPL YouTube channel.Complete transcript available. || AT2018COW_Labeled_Still_3_print.jpg (1024x576) [66.0 KB] || AT2018COW_Labeled_Still_3.jpg (3840x2160) [494.0 KB] || AT2018COW_Labeled_Still_3_searchweb.png (320x180) [56.8 KB] || AT2018COW_Labeled_Still_3_thm.png (80x40) [5.5 KB] || AT2018COW_Labeled_Music_Intro_3_1080.mp4 (1920x1080) [116.5 MB] || AT2018COW_Labeled_Music_Intro_3_1080p.mov (1920x1080) [161.2 MB] || AT2018COW_Labeled_Music_Intro_3_1080.webm (1920x1080) [13.2 MB] || AT2018COW_Labeled_Music_Intro_3_ProRes_3840x2160.mov (3840x2160) [4.7 GB] || AT2018COW_Labeled_Music_Intro_3_4k.mp4 (3840x2160) [436.5 MB] || AT2018COW_Labeled_Music_Intro_3_4K.mov (3840x2160) [241.6 MB] || AT2018COW_SRT_Captions.en_US.srt [1.2 KB] || AT2018COW_SRT_Captions.en_US.vtt [1.3 KB] || ",
            "release_date": "2019-01-10T13:00:00-05:00",
            "update_date": "2023-05-03T13:46:09.584975-04:00",
            "main_image": {
                "id": 397979,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012800/a012855/AT2018COW_Labeled_Still_3_print.jpg",
                "filename": "AT2018COW_Labeled_Still_3_print.jpg",
                "media_type": "Image",
                "alt_text": "Watch what scientists think happens when a black hole tears apart a hot, dense white dwarf star. A team working with observations from NASA’s Neil Gehrels Swift Observatory suggest this process explains a mysterious outburst known as AT2018cow. Credit: NASA's Goddard Space Flight CenterMusic: \"Curious Events\" from Killer TracksWatch this video on the JPL YouTube channel.Complete transcript available.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 12887,
            "url": "https://svs.gsfc.nasa.gov/12887/",
            "page_type": "Produced Video",
            "title": "TESS Coverage Animations",
            "description": "Animation showing the TESS spacecraft and the coverage of its four cameras.  Each camera covers a 24 degrees-square patch of sky and the four cameras are arranged in a vertical strip called an observation sector. || TESS_FOVAnimation_SH1_Text_frame.1687.png (1920x1080) [3.1 MB] || TESS_FOVAnimation_SH1_Text_frame.1687_print.jpg (1024x576) [106.2 KB] || TESS_FOVAnimation_SH1_4K_Text_frame.1687.png (3840x2160) [12.0 MB] || TESS_FOVAnimation_SH1_Text_frame.1687_searchweb.png (320x180) [75.3 KB] || TESS_FOVAnimation_SH1_Text_frame.1687_thm.png (80x40) [4.9 KB] || TESS_FOVAnimation_SH1_Final_v01-HD_1080p.mov (1920x1080) [86.8 MB] || TESS_FOVAnimation_SH1_Final_v01.webm (1920x1080) [4.2 MB] || FOV (3840x2160) [0 Item(s)] || TESS_FOVAnimation_SH1_Final_4K_Text_v01_H264.mov (3840x2160) [133.1 MB] || TESS_FOVAnimation_SH1_Final_v01.mov (1920x1080) [2.0 GB] || TESS_FOVAnimation_SH1_Final_4K_Text_v01.mov (3840x2160) [8.0 GB] || ",
            "release_date": "2018-03-28T12:45:00-04:00",
            "update_date": "2025-01-06T01:32:58.118322-05:00",
            "main_image": {
                "id": 405929,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012800/a012887/TESS_FOVAnimation_SH1_Text_frame.1687.png",
                "filename": "TESS_FOVAnimation_SH1_Text_frame.1687.png",
                "media_type": "Image",
                "alt_text": "Animation showing the TESS spacecraft and the coverage of its four cameras.  Each camera covers a 24 degrees-square patch of sky and the four cameras are arranged in a vertical strip called an observation sector.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 20272,
            "url": "https://svs.gsfc.nasa.gov/20272/",
            "page_type": "Animation",
            "title": "TESS Spacecraft Animations",
            "description": "Beauty Pass of TESS spacecraft || Beauty_One_00687_print.jpg (1024x576) [54.5 KB] || Beauty_One_00687_searchweb.png (180x320) [51.6 KB] || Beauty_One_00687_thm.png (80x40) [4.6 KB] || Tess_B_one_h264.webm (1920x1080) [1.8 MB] || Tess_B_one_h264.mov (1920x1080) [298.0 MB] || B1 (3840x2160) [0 Item(s)] || Beauty_One_2160p60.mp4 (3840x2160) [24.4 MB] || Tess_B_one_ProRes.mov (3840x2160) [2.0 GB] || ",
            "release_date": "2018-01-08T10:00:00-05:00",
            "update_date": "2024-12-29T23:27:18.420501-05:00",
            "main_image": {
                "id": 408182,
                "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020200/a020272/Beauty_One_00687_print.jpg",
                "filename": "Beauty_One_00687_print.jpg",
                "media_type": "Image",
                "alt_text": "Beauty Pass of TESS spacecraft",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 12499,
            "url": "https://svs.gsfc.nasa.gov/12499/",
            "page_type": "Produced Video",
            "title": "Swift Charts a Star's 'Death Spiral' into Black Hole",
            "description": "This animation illustrates how debris from a tidally disrupted star collides with itself, creating shock waves that emit ultraviolet and optical light far from the black hole. According to Swift observations of ASASSN-14li, these clumps took about a month to fall back to the black hole, where they produced changes in the X-ray emission that correlated with the earlier UV and optical changes.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || TD_Shocks_Still_print.jpg (1024x576) [115.2 KB] || TD_Shocks_Still.png (3840x2160) [32.6 MB] || TD_Shocks_Still.jpg (3840x2160) [922.7 KB] || TD_Shocks_Still_searchweb.png (320x180) [59.5 KB] || TD_Shocks_Still_thm.png (80x40) [4.8 KB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_1080.mov (1920x1080) [50.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_youtube_hq.mov (1920x1080) [25.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Good_1080.m4v (1920x1080) [44.4 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.m4v (960x540) [10.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_HD.wmv (1920x1080) [6.9 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.webm (960x540) [3.8 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv_subtitles.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_SRT_Captions.en_US.srt [509 bytes] || 12499_Tidal_Disruption_SRT_Captions.en_US.vtt [522 bytes] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_ProRes_1920x1080_2997.mov (1920x1080) [591.1 MB] || ",
            "release_date": "2017-03-20T14:00:00-04:00",
            "update_date": "2024-10-06T23:41:33.941280-04:00",
            "main_image": {
                "id": 416492,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012499/TD_Shocks_Still_print.jpg",
                "filename": "TD_Shocks_Still_print.jpg",
                "media_type": "Image",
                "alt_text": "This animation illustrates how debris from a tidally disrupted star collides with itself, creating shock waves that emit ultraviolet and optical light far from the black hole. According to Swift observations of ASASSN-14li, these clumps took about a month to fall back to the black hole, where they produced changes in the X-ray emission that correlated with the earlier UV and optical changes.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 12005,
            "url": "https://svs.gsfc.nasa.gov/12005/",
            "page_type": "Produced Video",
            "title": "Massive Black Hole Shreds Passing Star",
            "description": "A star approaching too close to a massive black hole is torn apart by tidal forces, as shown in this artist's rendering. Filaments containing much of the star's mass fall toward the black hole. Eventually these gaseous filaments merge into a smooth, hot disk glowing brightly in X-rays. As the disk forms, its central region heats up tremendously, which drives a flow of material, called a wind, away from the disk.   Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here. || Swift_Tidal_Disruption_2_Still_print.jpg (1024x576) [172.7 KB] || Swift_Tidal_Disruption_2_Still.jpg (1920x1080) [606.7 KB] || Swift_Tidal_Disruption_2_Still_web.png (320x180) [98.5 KB] || Swift_Tidal_Disruption_2_Still_thm.png (80x40) [6.8 KB] || Swift_Tidal_Disruption_2_Still_searchweb.png (320x180) [98.4 KB] || APPLE_TV_12005_Swift_Tidal_Music_FINAL_appletv_subtitles.m4v (1280x720) [37.5 MB] || 12005_Swift_Tidal_Music_MPEG4_1920X1080_2997.mp4 (1920x1080) [40.5 MB] || 12005_Swift_Tidal_Music_MPEG4_1920X1080_2997.webm (1920x1080) [7.7 MB] || WMV_12005_Swift_Tidal_Music_FINAL_HD.wmv (1920x1080) [49.6 MB] || APPLE_TV_12005_Swift_Tidal_Music_FINAL_appletv.m4v (1280x720) [37.4 MB] || 12005_Swift_Tidal_SRT_Captions.en_US.vtt [261 bytes] || 12005_Swift_Tidal_Music_FINAL_lowres.mp4 (480x272) [10.6 MB] || NASA_PODCAST_12005_Swift_Tidal_Music_FINAL_ipod_sm.mp4 (320x240) [12.3 MB] || 12005_Swift_Tidal_SRT_Captions.en_US.srt [248 bytes] || 12005_Swift_Tidal_Music_ProRes_1920x1080_5994.mov (1920x1080) [2.1 GB] || 12005_Swift_Tidal_Music_H264_Good_1920x1080_2997.mov (1920x1080) [301.2 MB] || 12005_Swift_Tidal_Music_FINAL_youtube_hq.mov (1920x1080) [1.3 GB] || 12005_Swift_Tidal_Music_H264_Best_1920x1080_5994.mov (1920x1080) [2.5 GB] || ",
            "release_date": "2015-10-21T13:00:00-04:00",
            "update_date": "2023-05-03T13:49:12.574389-04:00",
            "main_image": {
                "id": 439527,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012000/a012005/Swift_Tidal_Disruption_2_Still.jpg",
                "filename": "Swift_Tidal_Disruption_2_Still.jpg",
                "media_type": "Image",
                "alt_text": "A star approaching too close to a massive black hole is torn apart by tidal forces, as shown in this artist's rendering. Filaments containing much of the star's mass fall toward the black hole. Eventually these gaseous filaments merge into a smooth, hot disk glowing brightly in X-rays. As the disk forms, its central region heats up tremendously, which drives a flow of material, called a wind, away from the disk.   Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA Goddard YouTube channel.For complete transcript, click here.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 10867,
            "url": "https://svs.gsfc.nasa.gov/10867/",
            "page_type": "Produced Video",
            "title": "Swift HD Beauty Shot",
            "description": "Animation of the Swift spacecraft. || ",
            "release_date": "2011-11-09T12:00:00-05:00",
            "update_date": "2023-05-03T13:53:29.095223-04:00",
            "main_image": {
                "id": 481368,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010800/a010867/swif0266_print.jpg",
                "filename": "swif0266_print.jpg",
                "media_type": "Image",
                "alt_text": "Beauty pass animation showing the spacecraft moving into sunlight and past the Earth to end facing out into space.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 10807,
            "url": "https://svs.gsfc.nasa.gov/10807/",
            "page_type": "Produced Video",
            "title": "NASA's Swift Satellite Spots Black Hole Devouring A Star",
            "description": "In late March 2011, NASA's Swift satellite alerted astronomers to intense and unusual high-energy flares from a new source in the constellation Draco. They soon realized that the source, which is now known as Swift J1644+57, was the result of a truly extraordinary event — the awakening of a distant galaxy's dormant black hole as it shredded and consumed a star. The galaxy is so far away that the radiation from the blast has traveled 3.9 billion years before reaching Earth. Most galaxies, including our own, possess a central supersized black hole weighing millions of times the sun's mass. According to the new studies, the black hole in the galaxy hosting Swift J1644+57 may be twice the mass of the four-million-solar-mass black hole lurking at the center of our own Milky Way galaxy. As a star falls toward a black hole, it is ripped apart by intense tides. The gas is corralled into a disk that swirls around the black hole and becomes rapidly heated to temperatures of millions of degrees. The innermost gas in the disk spirals toward the black hole, where rapid motion and magnetism creates dual, oppositely directed \"funnels\" through which some particles may escape. Particle jets driving matter at velocities greater than 80-90 percent the speed of light form along the black hole's spin axis. In the case of Swift J1644+57, one of these jets happened to point straight at Earth.Theoretical studies of tidally disrupted stars suggested that they would appear as flares at optical and ultraviolet energies. The brightness and energy of a black hole's jet is greatly enhanced when viewed head-on. The phenomenon, called relativistic beaming, explains why Swift J1644+57 was seen at X-ray energies and appeared so strikingly luminous. When first detected on March 28, the flares were initially assumed to signal a gamma-ray burst, one of the nearly daily short blasts of high-energy radiation often associated with the death of a massive star and the birth of a black hole in the distant universe. But as the emission continued to brighten and flare, astronomers realized that the most plausible explanation was the tidal disruption of a sun-like star seen as beamed emission. || ",
            "release_date": "2011-08-24T13:00:00-04:00",
            "update_date": "2023-05-03T13:53:40.776982-04:00",
            "main_image": {
                "id": 484419,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010800/a010807/BlackHoleAnimation_00730.jpg",
                "filename": "BlackHoleAnimation_00730.jpg",
                "media_type": "Image",
                "alt_text": "On March 28, 2011, NASA's Swift detected intense X-ray flares thought to be caused by a black hole devouring a star. In one model, illustrated here, a sun-like star on an eccentric orbit plunges too close to its galaxy's central black hole. About half of the star's mass feeds an accretion disk around the black hole, which in turn powers a particle jet that beams radiation toward Earth. Credit: NASA/Goddard Space Flight Center/CI Lab",
                "width": 1280,
                "height": 720,
                "pixels": 921600
            }
        }
    ],
    "sources": [],
    "products": [
        {
            "id": 13237,
            "url": "https://svs.gsfc.nasa.gov/13237/",
            "page_type": "Produced Video",
            "title": "TESS Catches Its First Star-destroying Black Hole",
            "description": "When a star strays too close to a black hole, intense tides break it apart into a stream of gas. The tail of the stream escapes the system, while the rest of it swings back around, surrounding the black hole with a disk of debris. This video includes images of a tidal disruption event called ASASSN-19bt taken by NASA’s Transiting Exoplanet Survey Satellite (TESS) and Swift missions, as well as an animation showing how the event unfolded. Credit: NASA’s Goddard Space Flight CenterMusic: \"Games Show Sphere 03\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_TDE_Still_print.jpg (1024x576) [87.3 KB] || TESS_TDE_Still.jpg (3840x2160) [629.6 KB] || TESS_TDE_Still_searchweb.png (320x180) [68.3 KB] || TESS_TDE_Still_thm.png (80x40) [5.3 KB] || 13237_TESS_TDE_ProRes_1920x1080.mov (1920x1080) [1.6 GB] || 13237_TESS_TDE_1080_Best.mp4 (1920x1080) [380.2 MB] || 13237_TESS_TDE_1080.mp4 (1920x1080) [125.6 MB] || 13237_TESS_TDE_1080_Best.webm (1920x1080) [12.6 MB] || 13237_TESS_TDE_SRT_Captions.en_US.srt [2.2 KB] || 13237_TESS_TDE_SRT_Captions.en_US.vtt [2.2 KB] || ",
            "release_date": "2019-09-26T11:00:00-04:00",
            "update_date": "2023-05-03T13:45:37.411479-04:00",
            "main_image": {
                "id": 394872,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013200/a013237/TESS_TDE_Still_print.jpg",
                "filename": "TESS_TDE_Still_print.jpg",
                "media_type": "Image",
                "alt_text": "When a star strays too close to a black hole, intense tides break it apart into a stream of gas. The tail of the stream escapes the system, while the rest of it swings back around, surrounding the black hole with a disk of debris. This video includes images of a tidal disruption event called ASASSN-19bt taken by NASA’s Transiting Exoplanet Survey Satellite (TESS) and Swift missions, as well as an animation showing how the event unfolded. \r\rCredit: NASA’s Goddard Space Flight Center\rMusic: \"Games Show Sphere 03\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 13322,
            "url": "https://svs.gsfc.nasa.gov/13322/",
            "page_type": "Animation",
            "title": "NASA's Guide To Black Hole Safety",
            "description": "Have you ever thought about visiting a black hole? We sure hope not. However, if you're absolutely convinced that a black hole is your ideal vacation spot, watch this video before you blast off to learn more about them and (more importantly) how to stay safe.You can also download a handy safety brochure, watch short clips to learn different things about black holes, and even get some short glimpses into the lives of black holes and the explorers that want to visit them. || ",
            "release_date": "2019-09-23T10:00:00-04:00",
            "update_date": "2023-05-03T13:45:38.256787-04:00",
            "main_image": {
                "id": 392476,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013300/a013322/black_hole_week_01_what_is_a_black_hole_thumb_print.jpg",
                "filename": "black_hole_week_01_what_is_a_black_hole_thumb_print.jpg",
                "media_type": "Image",
                "alt_text": "Black Hole 101: What Is a Black Hole?Want to know more about black holes, but don't have a lot of time? This short video will give you a quick overview of some of the most interesting features of black holes.Credit: NASA's Goddard Space Flight CenterMusic: \"Dinner With the Vicar\" from Universal Production MusicComplete transcript available.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        }
    ],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}