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    "results": [
        {
            "id": 14753,
            "url": "http://svs.gsfc.nasa.gov/14753/",
            "result_type": "Produced Video",
            "release_date": "2025-01-13T10:14:00-05:00",
            "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole",
            "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ",
            "hits": 134
        },
        {
            "id": 14530,
            "url": "http://svs.gsfc.nasa.gov/14530/",
            "result_type": "Produced Video",
            "release_date": "2024-02-21T08:00:00-05:00",
            "title": "Goldstone Apple Valley Radio Telescope (GAVRT) Solar Patrol",
            "description": "The Goldstone Apple Valley Radio Telescope (GAVRT) is located in Goldstone, California. It is a reconfigured antenna used for teaching purposes.The GAVRT program teaches K-12 students how to calibrate this 34-meter antenna (known as Deep Space Station-28), collect and distribute science data through the Internet and get excited about radio astronomy. Students collaborate with scientists who are working on the same mission and are recognized as part of the science team. Data collected and analyzed by the students is used by NASA in their studies of the solar system.During the April 8, 2024, total solar eclipse, NASA’s Jet Propulsion Laboratory, educators at the Lewis Center for Education Research in Southern California, and participants in the center’s Solar Patrol citizen science program will observe solar “active regions” – the magnetically complex regions that form over sunspots – as the Moon moves over them. The Moon’s gradual passage across the Sun blocks different portions of the active region at different times, allowing scientists to distinguish light signals coming from one portion versus another. The technique, first used during the May 2012 annular eclipse, revealed details on the Sun the telescope couldn’t otherwise detect. || ",
            "hits": 51
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        {
            "id": 40502,
            "url": "http://svs.gsfc.nasa.gov/gallery/2024total-solar-eclipse-gallery/",
            "result_type": "Gallery",
            "release_date": "2023-10-31T00:00:00-04:00",
            "title": "2024 Total Solar Eclipse",
            "description": "On April 8, 2024, a total solar eclipse will cross North America, passing over Mexico, the United States, and Canada. A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. The sky will darken as if it were dawn or dusk.A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. People viewing the eclipse from locations where the Moon’s shadow completely covers the Sun – known as the path of totality – will experience a total solar eclipse. The sky will darken, as if it were dawn or dusk. Weather permitting, people along the path of totality will see the Sun’s corona, or outer atmosphere, which is usually obscured by the bright face of the Sun.Learn more about this total solar eclipse: solarsystem.nasa.gov/eclipses/2024\n",
            "hits": 282
        },
        {
            "id": 14170,
            "url": "http://svs.gsfc.nasa.gov/14170/",
            "result_type": "Produced Video",
            "release_date": "2022-08-10T10:00:00-04:00",
            "title": "NASA’s Fermi Confirms 'PeVatron' Supernova Remnant",
            "description": "Explore how astronomers located a supernova remnant that fires up protons to energies 10 times greater than the most powerful particle accelerator on Earth.Credit: NASA’s Goddard Space Flight CenterMusic: New Philosopher by Laurent Dury; Universal Production MusicWatch this video on the NASA Goddard YouTube channelComplete transcript available. || 14170-Found__A_PeVatron.01978_print.jpg (1024x576) [61.1 KB] || 14170-_PeVatron.webm (1920x1080) [15.1 MB] || 14170-_PeVatron.mp4 (1920x1080) [136.6 MB] || 14170-PeVatron.en_US.vtt [2.3 KB] || 14170-PeVatron.mov (1920x1080) [1.8 GB] || ",
            "hits": 141
        },
        {
            "id": 14146,
            "url": "http://svs.gsfc.nasa.gov/14146/",
            "result_type": "Produced Video",
            "release_date": "2022-05-04T00:00:00-04:00",
            "title": "Black Hole Desktop & Phone Wallpapers",
            "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ",
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        },
        {
            "id": 4807,
            "url": "http://svs.gsfc.nasa.gov/4807/",
            "result_type": "Visualization",
            "release_date": "2021-04-21T00:00:00-04:00",
            "title": "M87: Telescopes Unite in Unprecedented Observations of Famous Black Hole",
            "description": "Beginning with the Event Horizon Telescope's now iconic image of M87, this video takes viewers on a journey through the data from several telescopes. The video shows data across many factors of 10 in scale, both of wavelengths of light and physical size. || M87_EHT_Multiwavelength_Zoom_print.png (1024x576) [271.1 KB] || M87_EHT_Multiwavelength_Zoom_print.jpg (1024x576) [70.0 KB] || M87_EHT_Multiwavelength_Zoom_STILL.png (3840x2160) [2.1 MB] || M87_EHT_Multiwavelength_Zoom_thm.png (320x180) [40.0 KB] || M87_EHT_Multiwavelength_Zoom_print_thm.png (80x40) [3.9 KB] || M87_EHT_Multiwavelength_Zoom_1080p30.mp4 (1920x1080) [9.7 MB] || M87_EHT_Multiwavelength_Zoom_1080p30.webm (1920x1080) [8.4 MB] || M87_EHT_Multiwavelength_Zoom_2160p30.mp4 (3840x2160) [28.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || M87_EHT_Multiwavelength_Zoom_1080p30.mp4.hwshow [202 bytes] || ",
            "hits": 195
        },
        {
            "id": 20338,
            "url": "http://svs.gsfc.nasa.gov/20338/",
            "result_type": "Animation",
            "release_date": "2020-12-08T15:00:00-05:00",
            "title": "SunRISE Beauty Pass",
            "description": "A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events. || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_print.jpg (1024x576) [172.5 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_searchweb.png (320x180) [87.2 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_thm.png (80x40) [5.9 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.mov (3840x2160) [695.8 MB] || SUNRISE-shot1_v06_4k_30fps_h264.mp4 (3840x2160) [13.7 MB] || SUNRISE-shot1_v06_4k (3840x2160) [32.0 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.webm (3840x2160) [5.3 MB] || ",
            "hits": 50
        },
        {
            "id": 13751,
            "url": "http://svs.gsfc.nasa.gov/13751/",
            "result_type": "Produced Video",
            "release_date": "2020-11-04T11:00:00-05:00",
            "title": "NASA Missions Team Up to Study Unique Magnetar Outburst",
            "description": "On April 28, space- and ground-based observatories detected powerful, simultaneous X-ray and radio bursts from a source in our galaxy. Watch to see how this unique event helps solve the longstanding puzzle of fast radio bursts observed in other galaxies.Credit: NASA's Goddard Space Flight CenterMusic: \"Jupiter's Eye\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_FRB_Still.jpg (1920x1080) [535.5 KB] || Magnetar_FRB_Still_searchweb.png (320x180) [65.5 KB] || Magnetar_FRB_Still_thm.png (80x40) [4.8 KB] || 13751_Magnetar_FRB_Best_1080.webm (1920x1080) [25.7 MB] || 13751_Magnetar_FRB_1080.mp4 (1920x1080) [237.4 MB] || 13751_Magnetar_FRB_Best_1080.mp4 (1920x1080) [741.8 MB] || Fast_Radio_Burst_SRT_Captions.en_US.srt [4.5 KB] || Fast_Radio_Burst_SRT_Captions.en_US.vtt [4.5 KB] || 13751_Magnetar_FRB_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ",
            "hits": 523
        },
        {
            "id": 13696,
            "url": "http://svs.gsfc.nasa.gov/13696/",
            "result_type": "Produced Video",
            "release_date": "2020-08-25T11:00:00-04:00",
            "title": "Young Active Galaxy with ‘TIE Fighter’ Shape",
            "description": "This illustration shows two views of the active galaxy TXS 0128+554, located around 500 million light-years away. Left: The galaxy’s central jets appear as they would if we viewed them both at the same angle. The black hole, embedded in a disk of dust and gas, launches a pair of particle jets traveling at nearly the speed of light. Scientists think gamma rays (magenta) detected by NASA’s Fermi Gamma-ray Space Telescope originate from the base of these jets. As the jets collide with material surrounding the galaxy, they form identical lobes seen at radio wavelengths (orange). The jets experienced two distinct bouts of activity, which created the gap between the lobes and the black hole. Right: The galaxy appears in its actual orientation, with its jets tipped out of our line of sight by about 50 degrees.Credit: NASA’s Goddard Space Flight Center || TXS0128_Side-by-Side_FInal.jpg (7680x2160) [1.8 MB] || TXS0128_Side-by-Side_FInal_Half.jpg (3840x1080) [601.5 KB] || TXS0128_Side-by-Side_FInal_print.jpg (1024x288) [45.4 KB] || TXS0128_Side-by-Side_FInal.jpg.dzi (7680x2160) [178 bytes] || TXS0128_Side-by-Side_FInal.jpg_files (1x1) [4.0 KB] || ",
            "hits": 62
        },
        {
            "id": 13582,
            "url": "http://svs.gsfc.nasa.gov/13582/",
            "result_type": "Produced Video",
            "release_date": "2020-04-20T11:00:00-04:00",
            "title": "NASA Reveals Alien Composition of 2I/Borisov, First Interstellar Comet",
            "description": "When amateur astronomer Gennady Borisov discovered an interstellar comet zipping through our solar system on Aug. 30, 2019, scientists promptly turned their telescopes towards it hoping to catch a glimpse of this rare and ephemeral event. When the scientists peeked inside the halo of gas that formed around the comet as it came closer to the Sun and its ices began to vaporize, they detected something peculiar. 2I/Borisov was releasing gas with a greater concentration of carbon monoxide (CO) than anyone had detected in any comet at a similar distance from the Sun.Song is \"Tides\" from Universal Production Music. || 13582_thumb2.jpg (3840x2160) [335.5 KB] || 13582_Comet_Borisov_YouTube_MASTER.00435_searchweb.png (320x180) [77.0 KB] || 13582_Comet_Borisov_YouTube_MASTER.00435_thm.png (80x40) [4.0 KB] || 13582_Comet_Borisov_MASTER_twitter_720.mp4 (1280x720) [26.3 MB] || 13582_Comet_Borisov_facebook_720.mp4 (1280x720) [151.3 MB] || 13582_Comet_Borisov.webm (960x540) [48.7 MB] || 13582_Comet_Borisov_MASTER.mov.en_US.srt [2.8 KB] || 13582_Comet_Borisov_MASTER.mov.en_US.vtt [2.7 KB] || 13582_Comet_Borisov_YouTube_MASTER.mp4 (3840x2160) [155.4 MB] || ",
            "hits": 70
        },
        {
            "id": 13556,
            "url": "http://svs.gsfc.nasa.gov/13556/",
            "result_type": "Produced Video",
            "release_date": "2020-02-14T03:00:00-05:00",
            "title": "Astrophysics Valentines",
            "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ",
            "hits": 98
        },
        {
            "id": 40409,
            "url": "http://svs.gsfc.nasa.gov/gallery/fermi-stills/",
            "result_type": "Gallery",
            "release_date": "2020-01-22T00:00:00-05:00",
            "title": "Fermi Stills",
            "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.",
            "hits": 146
        },
        {
            "id": 13239,
            "url": "http://svs.gsfc.nasa.gov/13239/",
            "result_type": "Produced Video",
            "release_date": "2019-09-24T09:00:00-04:00",
            "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. || ",
            "hits": 118
        },
        {
            "id": 13156,
            "url": "http://svs.gsfc.nasa.gov/13156/",
            "result_type": "Produced Video",
            "release_date": "2019-03-19T12:00:00-04:00",
            "title": "NASA’s Fermi Satellite Clocks a ‘Cannonball’ Pulsar",
            "description": "New radio observations combined with 10 years of data from NASA’s Fermi Gamma-ray Space Telescope have revealed a runaway pulsar that escaped the blast wave of the supernova that formed it. Credit: NASA’s Goddard Space Flight CenterMusic: \"Forensic Scientist\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available.See the bottom of the page for a version without on-screen text. || CTA1_Still.jpg (1920x1080) [291.7 KB] || CTA1_Still_print.jpg (1024x576) [137.4 KB] || CTA1_Still_searchweb.png (320x180) [86.6 KB] || CTA1_Still_thm.png (80x40) [7.2 KB] || 13156_CTB1_Cannonball_Pulsar_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 13156_CTB1_Cannonball_Pulsar_Best.mov (1920x1080) [727.8 MB] || 13156_CTB1_Cannonball_Pulsar_Good.mp4 (1920x1080) [400.9 MB] || 13156_CTB1_Cannonball_Pulsar.mp4 (1920x1080) [147.3 MB] || 13156_CTB1_Cannonball_Pulsar.m4v (1920x1080) [144.6 MB] || 13156_CTB1_Cannonball_Pulsar_ProRes_1920x1080_2997.webm (1920x1080) [15.7 MB] || 13156_CTB1_Cannonball_Pulsar_SRT_Captions.en_US.srt [1.9 KB] || 13156_CTB1_Cannonball_Pulsar_SRT_Captions.en_US.vtt [1.9 KB] || ",
            "hits": 85
        },
        {
            "id": 13097,
            "url": "http://svs.gsfc.nasa.gov/13097/",
            "result_type": "Produced Video",
            "release_date": "2018-10-17T12:30:00-04:00",
            "title": "Fermi Scientists Introduce Gamma-ray Constellations",
            "description": "Scientists with NASA’s Fermi Gamma-ray Space Telescope devised a set of constellations for the high-energy sky to highlight the mission’s 10th year of operations. Characters from modern myths, like the Hulk and the time-warping TARDIS from “Doctor Who,” represent one source of inspiration. Others include scientific concepts and tools, like the Fermi Satellite, and famous landmarks in countries contributing to the development and operation of Fermi. The mission has mapped about 3,000 gamma-ray sources -- 10 times the number known before its launch and comparable to the number of bright stars in the traditional constellations. The background shows the gamma-ray sky as mapped by Fermi. The prominent reddish band is the plane of our own galaxy, the Milky Way; brighter colors indicate brighter gamma-ray sources. Credit: NASA || GR_Constellations-NorthFermi_FullSize_FInal.gif (1920x930) [4.4 MB] || ",
            "hits": 55
        },
        {
            "id": 12218,
            "url": "http://svs.gsfc.nasa.gov/12218/",
            "result_type": "Produced Video",
            "release_date": "2016-04-28T12:00:00-04:00",
            "title": "Fermi Helps Link a Cosmic Neutrino to a Blazar Outburst",
            "description": "NASA Goddard scientist Roopesh Ojha explains how Fermi and TANAMI uncovered the first plausible link between a blazar eruption and a neutrino from deep space. Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || UniverseHD1845_print.jpg (1024x576) [135.3 KB] || UniverseHD1845_searchweb.png (320x180) [85.8 KB] || UniverseHD1845_web.png (180x320) [85.8 KB] || UniverseHD1845_thm.png (80x40) [6.3 KB] || UniverseHD1845.tif (1920x1080) [7.9 MB] || 12218_Fermi_Blazar_Neutrino_FINAL_appletv.webm (1280x720) [30.3 MB] || 12218_Fermi_Blazar_Neutrino_FINAL_appletv.m4v (1280x720) [138.0 MB] || 12218_Fermi_Blazar_Neutrino_FINAL_appletv_subtitles.m4v (1280x720) [138.1 MB] || 12218_Fermi_Blazar_Neutrino_H264_Good_1920x1080_2997.mov (1920x1080) [315.8 MB] || 12218_Fermi_Blazar_Neutrino.mp4 (1920x1080) [292.0 MB] || 12218_Fermi_Blazar_Neutrino_SRT_Captions.en_US.srt [4.8 KB] || 12218_Fermi_Blazar_Neutrino_SRT_Captions.en_US.vtt [4.8 KB] || 12218_Fermi_Blazar_Neutrino_FINAL_youtube_hq.mov (1920x1080) [1.3 GB] || 12218_Fermi_Blazar_Neutrino_FINAL_lowres.mp4 (480x272) [38.6 MB] || 12218_Fermi_Blazar_Neutrino_H264_Best_1920x1080_2997.mov (1920x1080) [2.3 GB] || 12218_Fermi_Blazar_Neutrino_ProRes_1920x1080_2997.mov (1920x1080) [3.6 GB] || ",
            "hits": 87
        },
        {
            "id": 30680,
            "url": "http://svs.gsfc.nasa.gov/30680/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-09-25T13:00:00-04:00",
            "title": "Active Galaxy Hercules A: Visible & Radio Comparison",
            "description": "A comparison of visible and radio views of the active galaxy Hercules A || hercules_a-example_frame-1920x1080.png (1920x1080) [532.7 KB] || hercules_a-example_frame-1920x1080.jpg (1920x1080) [67.4 KB] || hercules_a-example_frame-1920x1080_searchweb.png (180x320) [25.1 KB] || hercules_a-example_frame-1920x1080_thm.png (80x40) [3.2 KB] || hercules_a-b-1920x1080.m4v (1920x1080) [8.7 MB] || hercules_a-b-1920x1080.wmv (1920x1080) [21.8 MB] || hercules_a-b-1920x1080p30.mov (1920x1080) [21.7 MB] || hercules_a-b-1280x720.m4v (1280x720) [3.4 MB] || hercules_a-b-1280x720.wmv (1280x720) [11.8 MB] || hercules_a-b-1920x1080p30.webm (1920x1080) [4.1 MB] || hercules_a-b-30680.key [6.0 MB] || hercules_a-b-30680.pptx [3.6 MB] || active-galaxy-hercules-a.hwshow [217 bytes] || ",
            "hits": 85
        },
        {
            "id": 11216,
            "url": "http://svs.gsfc.nasa.gov/11216/",
            "result_type": "Produced Video",
            "release_date": "2014-02-20T11:00:00-05:00",
            "title": "Black Widow Pulsars Consume Their Mates",
            "description": "Black widow spiders and their Australian cousins, known as redbacks, are notorious for an unsettling tendency to kill and devour their male partners. Astronomers have noted similar behavior among two rare breeds of binary system that contain rapidly spinning neutron stars, also known as pulsars. The essential features of black widow and redback binaries are that they place a normal but very low-mass star in close proximity to a millisecond pulsar, which has disastrous consequences for the star. Black widow systems contain stars that are both physically smaller and of much lower mass than those found in redbacks.So far, astronomers have found at least 18 black widows and nine redbacks within the Milky Way, and additional members of each class have been discovered within the dense globular star clusters that orbit our galaxy. One black widow system, named PSR J1311-3430 and discovered in 2012, sets the record for the tightest orbit of its class and contains one of the heaviest neutron stars known. The pulsar's featherweight companion, which is only a dozen or so times the mass of Jupiter and just 60 percent of its size, completes an orbit every 93 minutes – less time than it takes to watch most movies. The side of the star facing the pulsar is heated to more than 21,000 degrees Fahrenheit (nearly 12,000 C), or more than twice as hot as the sun's surface. Recent studies allow a range of values extending down to 2 solar masses for the pulsar, making it one of the most massive neutron stars known. Watch the video to learn more about this system and its discovery from some of the scientists involved. || ",
            "hits": 111
        },
        {
            "id": 10964,
            "url": "http://svs.gsfc.nasa.gov/10964/",
            "result_type": "Produced Video",
            "release_date": "2012-06-21T09:00:00-04:00",
            "title": "Using Quasars to Measure the Earth: A Brief History of VLBI",
            "description": "VLBI, or Very Long Baseline Interferometry, is a technique that uses multiple radio telescopes to very precisely measure the Earth's orientation. It was originally invented back in the 1960s to take better pictures of quasars, but scientists soon found out that if you threw the process in reverse, you could measure how the ground beneath the telescopes moves around, how long days really are, and how the Earth wobbles on its axis as it revolves around the sun! Learn more about VLBI here!This video is presented in both stereoscopic 3D and standard 2D versions. The labels below will help you pick which video is right for your display! || ",
            "hits": 64
        },
        {
            "id": 10910,
            "url": "http://svs.gsfc.nasa.gov/10910/",
            "result_type": "Produced Video",
            "release_date": "2012-02-23T14:00:00-05:00",
            "title": "Looking Down a Well: A Brief History of Geodesy",
            "description": "Geodesy is a field of study that deals with the measurement and representation of the Earth, and it all started when a clever human named Eratosthenes discovered that you could measure the circumference of the Earth by looking down a well. Over time, the field of geodesy has expanded and evolved dramatically, and NASA uses technology like radio telescopes, ground surveys, and satellites to contribute! Learn more about geodesy in this video! || ",
            "hits": 93
        },
        {
            "id": 10869,
            "url": "http://svs.gsfc.nasa.gov/10869/",
            "result_type": "Produced Video",
            "release_date": "2012-01-10T11:00:00-05:00",
            "title": "NASA's RXTE Helps Pinpoint Launch of 'Bullets' in a Black Hole's Jet",
            "description": "Using observations from NASA's Rossi X-ray Timing Explorer (RXTE) satellite and the National Science Foundation's (NSF) Very Long Baseline Array (VLBA) radio telescope, an international team of astronomers has identified the moment when a black hole in our galaxy launched superfast knots of gas into space. Racing outward at about one-quarter the speed of light, these \"bullets\" of ionized gas are thought to arise from a region located just outside the black hole's event horizon, the point beyond which nothing can escape.The research centered on the mid-2009 outburst of a binary system known as H1743-322, located about 28,000 light-years away toward the constellation Scorpius. Discovered by NASA's HEAO-1 satellite in 1977, the system is composed of a normal star and a black hole of modest but unknown masses. Their orbit around each other is measured in days, which puts them so close together that the black hole pulls a continuous stream of matter from its stellar companion. The flowing gas forms a flattened accretion disk millions of miles across, several times wider than our sun, centered on the black hole. As matter swirls inward, it is compressed and heated to tens of millions of degrees, so hot that it emits X-rays.Some of the infalling matter becomes re-directed out of the accretion disk as dual, oppositely directed jets. Most of the time, the jets consist of a steady flow of particles. Occasionally, though, they morph into more powerful outflows that hurl massive gas blobs at significant fractions of the speed of light. || ",
            "hits": 46
        }
    ]
}