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    "results": [
        {
            "id": 14523,
            "url": "https://svs.gsfc.nasa.gov/14523/",
            "result_type": "Produced Video",
            "release_date": "2024-07-25T09:00:00-04:00",
            "title": "Understanding Cosmic Dawn",
            "description": "In this 15-minute \"mini podcast\", NASA astrosphysicist Michelle Thaller talks about the early universe, the cosmic dark ages, cosmic dawn and why these different stages happened.Credit: NASA's Goddard Space Flight CenterComplete transcript available. || CosmicDawnPodcast_ThumbnailFinal.jpg (1920x1080) [178.2 KB] || Cosmic_Dawn_MiniPodcast_FINAL.mp3 [21.8 MB] || CosmicDawnPodcastCaptions.en_US.srt [24.6 KB] || CosmicDawnPodcastCaptions.en_US.vtt [23.3 KB] || ",
            "hits": 128
        },
        {
            "id": 14604,
            "url": "https://svs.gsfc.nasa.gov/14604/",
            "result_type": "Produced Video",
            "release_date": "2024-06-12T10:00:00-04:00",
            "title": "NASA’s Roman Mission Gets Cosmic ‘Sneak Peek’ From Supercomputers",
            "description": "This graphic highlights part of a new simulation of what NASA’s Nancy Grace Roman Space Telescope could see when it launches by May 2027. The background spans about 0.11 square degrees (roughly equivalent to half of the area of sky covered by a full Moon), representing less than half the area Roman will see in a single snapshot. The inset zooms in to a region 300 times smaller, showcasing a swath of brilliant synthetic galaxies at Roman’s full resolution. Having such a realistic simulation helps scientists study the physics behind cosmic images –– both synthetic ones like these and future real ones. Researchers will use the observations for many types of science, including testing our understanding of the origin, evolution, and ultimate fate of the universe.Credit: C. Hirata and K. Cao (OSU) and NASA’s Goddard Space Flight Center || Roman_Simulation_Popout_2k_deg.jpg (2048x2048) [979.2 KB] || ",
            "hits": 86
        },
        {
            "id": 14598,
            "url": "https://svs.gsfc.nasa.gov/14598/",
            "result_type": "Produced Video",
            "release_date": "2024-06-07T00:00:00-04:00",
            "title": "Cruising the Cosmic Web (Dome Version)",
            "description": "Cruising the Cosmic Web || PRINT.jpg (1920x1080) [250.5 KB] || THUMB.jpg (1920x1080) [250.5 KB] || SEARCH.jpg (320x180) [20.0 KB] || Cruising_the_Cosmic_Web,_V2_Dome_Version.mp4 (1280x720) [36.0 MB] || 1024x1024_1x1_30p [256.0 KB] || 2200x2200_1x1_30p [256.0 KB] || ",
            "hits": 486
        },
        {
            "id": 14375,
            "url": "https://svs.gsfc.nasa.gov/14375/",
            "result_type": "Infographic",
            "release_date": "2023-06-27T10:00:00-04:00",
            "title": "NASA’s Roman and ESA’s Euclid Will Team Up To Investigate Dark Energy",
            "description": "Euclid (left) is a medium-class ESA mission.  The Nancy Grace Roman Space Telescope (right) is an upcoming NASA flagship mission.  Both will study the history of the universe and bring new insight to the mystery of dark energy.Credit: NASA's Goddard Space Flight Center; ESA/ATG medialab || Euclid-Roman_Graphic_Final.jpg (1920x1080) [476.1 KB] || Euclid-Roman_Graphic_Final_searchweb.png (320x180) [101.4 KB] || Euclid-Roman_Graphic_Final_thm.png (80x40) [7.9 KB] || ",
            "hits": 91
        },
        {
            "id": 14269,
            "url": "https://svs.gsfc.nasa.gov/14269/",
            "result_type": "Produced Video",
            "release_date": "2023-01-09T13:10:00-05:00",
            "title": "NASA’s Webb Telescope Links Galaxies Near and Far",
            "description": "A trio of faint objects (circled) captured in the James Webb Space Telescope’s deep image of the galaxy cluster SMACS 0723 exhibit properties remarkably similar to rare, small galaxies called “green peas” found much closer to home. The cluster’s mass makes it a gravitational lens, which both magnifies and distorts the appearance of background galaxies. We view these early peas as they existed when the universe was about 5% its current age of 13.8 billion years. The farthest pea, at left, contains just 2% the oxygen abundance of a galaxy like our own and might be the most chemically primitive galaxy yet identified. Credit: NASA, ESA, CSA, and STScI || early_peas_behind_SMACS_0723_1080_print.jpg (1024x880) [161.9 KB] || early_peas_behind_SMACS_0723_1080.png (2513x2160) [3.8 MB] || early_peas_behind_SMACS_0723_2160.png (2513x2160) [3.8 MB] || early_peas_behind_SMACS_0723_full.png (3840x3302) [8.2 MB] || early_peas_behind_SMACS_0723_1080_searchweb.png (320x180) [71.2 KB] || early_peas_behind_SMACS_0723_1080_web.png (320x275) [103.8 KB] || early_peas_behind_SMACS_0723_1080_thm.png (80x40) [5.1 KB] || ",
            "hits": 119
        },
        {
            "id": 14001,
            "url": "https://svs.gsfc.nasa.gov/14001/",
            "result_type": "Infographic",
            "release_date": "2021-11-09T10:00:00-05:00",
            "title": "Roman Space Telescope High Latitude Wide Area Survey",
            "description": "This illustration compares the relative sizes of the areas of sky covered by two surveys: Roman’s High Latitude Wide Area Survey, outlined in blue, and the largest mosaic led by Hubble, the Cosmological Evolution Survey (COSMOS), shown in red. In current plans, the Roman survey will be more than 1,000 times broader than Hubble’s. Roman will also explore more distant realms of space than most other telescopes have probed in previous efforts to study why the expansion of the universe is speeding up. Credit: NASA's Goddard Space Flight Center || Roman_HLS_FINAL_1080.png (2160x1080) [9.8 MB] || Roman_HLS_FINAL_1080.jpg (2160x1080) [800.5 KB] || Roman_HLS_FINAL_1080_print.jpg (1024x512) [224.7 KB] || Roman_HLS_Final_Full.jpg (8000x4000) [3.8 MB] || Roman_HLS_FINAL_Half.png (4000x2000) [31.6 MB] || Roman_HLS_FINAL_Half.jpg (4000x2000) [1.7 MB] || Roman_HLS_FINAL_Full.png (8000x4000) [114.3 MB] || Roman_HLS_FINAL_1080_searchweb.png (320x180) [90.3 KB] || Roman_HLS_FINAL_1080_thm.png (80x40) [6.9 KB] || ",
            "hits": 117
        },
        {
            "id": 10662,
            "url": "https://svs.gsfc.nasa.gov/10662/",
            "result_type": "Produced Video",
            "release_date": "2021-04-14T00:00:00-04:00",
            "title": "Webb Science Simulations: Planetary Systems and Origins of Life",
            "description": "Supercomputer simulations of planeratry evolution. Part 1: Turbulent Molecular Cloud Nebula with Protostellar ObjectsThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Drs. Alexei Kritsuk and Michael Norman to visualize a computational data set of a turbulent molecular cloud nebula forming protostellar objects and accretion disks approximately 100 AU in diameter, on the order of the size of our solar system. AVL used its Amore software to interpolate and render the Adaptive Mesh Refinement (AMR) simulation generated from ENZO code for cosmology and astrophysics. The AMR simulation was developed by Drs. Kritsuk and Norman at the Laboratory for Computational Astrophysics. The AMR simulation generated more than 2 terabytes of data and follows star formation processes in a self-gravitating turbulent molecular cloud with a dynamic range of half-a-million in linear scale, resolving both the large-scale filamentary structure of the molecular cloud (~5 parsec) and accretion disks around emerging young protostellar objects (down to 2 AU).  Part 2: Protoplanetary Disk and Planet FormationThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Dr. Aaron Boley to visualize the 16,000 year evolution of a young, isolated protoplanetary disk which surrounds a newly-formed protostar. The disk forms spiral arms and a dense clump as a result of gravitational collapse. Dr. Aaron Boley developed this computational model to investigate the response of young disks to mass accretion from their surrounding envelopes, including the direct formation of planets and brown dwarfs through gravitational instability.  The main formation mechanism for gas giant planets has been debated within the scientific community for over a decade. One of these theories is 'direct formation through gravitational instability.' If the self-gravity of the gas overwhelms the disk's thermal pressure and the stabilizing effect of differential rotation, the gas closest to the protostar rotates faster than gas farther away. In this scenario, regions of the gaseous disk collapse and form a planet directly. The study, presented in Boley (2009), explores whether mass accretion in the outer regions of disks can lead to such disk fragmentation. The simulations show that clumps can form in situ at large disk radii. If the clumps survive, they can become gas giants on wide orbits, e.g., Fomalhaut b, or even more massive objects called brown dwarfs. Whether a disk forms planets at large radii and, if so, the number of planets that form, depend on how much of the envelope mass is distributed at large distances from the protostar.  The results of the simulations suggest that there are two modes of gas giant planet formation. The first mode occurs early in the disk's lifetime, at large radii, and through the disk instability mechanism. After the main accretion phase is over, gas giants can form in the inner disk, over a period of a million years, through the core accretion mechanism, which researchers are addressing in other studies.Thanks to R. H. Durisen, L. Mayer, and G. Lake for comments and discussions relating to this research. This study was supported in part by the University of Zurich, Institute for Theoretical Physics, and by a Swiss Federal Grant. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.AVL at NCSA, University of Illinois. || ",
            "hits": 264
        },
        {
            "id": 31035,
            "url": "https://svs.gsfc.nasa.gov/31035/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-04-26T12:00:00-04:00",
            "title": "A Flight Through the CANDELS Ultra Deep Survey Field",
            "description": "This visualization traverses the CANDELS Ultra Deep Survey (UDS) field to showcase the varied appearances of galaxies and their three-dimensional distribution. The sequence features a dense cluster of galaxies about 6 billion light-years away and extends to galaxies at more than twice that distance. Because the light from these galaxies has travelled for billions of years across space, the images show the galaxies as they appeared billions of years ago. In addition, the expansion of space has redshifted the light of these galaxies toward longer wavelengths (i.e., to the red end of the visible-light region and into the infrared-light region). The changes seen in galaxies during the fly-through illustrate the changes in galaxy structure and appearance over billions of years of cosmic history. CANDELS is an acronym for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey project. One of the largest projects ever done with the Hubble Space Telescope, CANDELS surveyed five fields to study the development of galaxies over time. The CANDELS observations of the UDS field complement ground-based observations from the United Kingdom Infrared Telescope. Astronomers and visual artists extracted over 26,000 galaxies from the Hubble UDS images and created a computer model based on the measured and estimated properties. Note that the distances used in the visualization are significantly compressed for cinematic purposes. || ",
            "hits": 77
        },
        {
            "id": 30681,
            "url": "https://svs.gsfc.nasa.gov/30681/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-09-25T13:00:00-04:00",
            "title": "Exploring the Hubble eXtreme Deep Field",
            "description": "A flight through the galaxies of the Hubble eXtreme Deep Field || hxdf_fly-example_frame-1920x1080.png (1920x1080) [1.2 MB] || hxdf_fly-example_frame-1920x1080.jpg (1920x1080) [167.7 KB] || hxdf_fly-example_frame-1920x1080_searchweb.png (180x320) [67.3 KB] || hxdf_fly-example_frame-1920x1080_thm.png (80x40) [6.0 KB] || hxdf_fly-b-1920x1080.wmv (1920x1080) [19.4 MB] || hxdf_fly-b-1920x1080p30.mov (1920x1080) [27.7 MB] || hxdf_fly-b-1920x1080.m4v (1920x1080) [13.2 MB] || hxdf_fly-b-1280x720.wmv (1280x720) [11.7 MB] || hxdf_fly-b-1280x720.m4v (1280x720) [6.2 MB] || hxdf_fly-b-1920x1080p30.webm (1920x1080) [2.8 MB] || hxdf_fly-b-30681.key [9.2 MB] || hxdf_fly-b-30681.pptx [6.7 MB] || ",
            "hits": 180
        },
        {
            "id": 11388,
            "url": "https://svs.gsfc.nasa.gov/11388/",
            "result_type": "Produced Video",
            "release_date": "2013-10-30T14:00:00-04:00",
            "title": "Suzaku Study Points to Early Cosmic 'Seeding'",
            "description": "Most of the universe's heavy elements, including the iron in our blood, formed early in cosmic history and spread throughout the universe, according to a new study of the Perseus Galaxy Cluster using Japan's Suzaku satellite. Between 2009 and 2011, researchers from the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly run by Stanford University and the Department of Energy's SLAC National Accelerator Laboratory in California, used Suzaku's unique capabilities to map the distribution of iron throughout the Perseus Galaxy Cluster. What they found is remarkable: Across the cluster, which spans more than 11 million light-years of space, the concentration of X-ray-emitting iron is essentially uniform in all directions.This tells astronomers that iron — and by extension other heavy elements — already was widely dispersed throughout the universe when the cluster began to form. Explaining this helps scientists better understand what the universe was like 10 to 12 billion years ago, a time when rapid-fire supernova explosions were common and black holes were especially active. || ",
            "hits": 87
        },
        {
            "id": 30134,
            "url": "https://svs.gsfc.nasa.gov/30134/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Physics of the Cosmos",
            "description": "Missions that make up Physics of the Cosmos Program || physics_of_the_cosmos_print.jpg (1024x574) [203.5 KB] || physics_of_the_cosmos.png (4104x2304) [10.6 MB] || physics_of_the_cosmos_searchweb.png (320x180) [97.9 KB] || physics_of_the_cosmos_thm.png (80x40) [6.8 KB] || For More Information || See [http://pcos.gsfc.nasa.gov](http://pcos.gsfc.nasa.gov) || ",
            "hits": 79
        },
        {
            "id": 11093,
            "url": "https://svs.gsfc.nasa.gov/11093/",
            "result_type": "Produced Video",
            "release_date": "2012-10-11T13:00:00-04:00",
            "title": "Atomic Interferometry",
            "description": "Einstein predicted gravity waves in his general theory of relativity, but to date these ripples in the fabric of space-time have never been observed. Now a scientific research technique called Atomic Interferometry is trying to re-write the canon. In conjunction with researchers at Stanford University, scientists at NASA Goddard are developing a system to measure the faint gravitational vibrations generated by movement of massive objects in the universe. The scientific payoff could be important, helping better clarify key issues in our understanding of cosmology. But application payoff could be substantial, too, with the potential to develop profound advances in fields like geolocation and timekeeping. In this video we examine how the system would work, and the scientific underpinnings of the research effort. || ",
            "hits": 42
        },
        {
            "id": 11008,
            "url": "https://svs.gsfc.nasa.gov/11008/",
            "result_type": "Produced Video",
            "release_date": "2012-06-21T16:00:00-04:00",
            "title": "WMAP—From the Archives",
            "description": "On June 20, 2012, Dr. Charles Bennett and the WMAP team were awarded the Gruber Cosmology Prize. The Wilkinson Microwave Anisotropy Probe (WMAP) was built and launched by NASA to measure a remnant of the early universe - its oldest light. The conditions of the early times are imprinted on this light. It is the result of what happened earlier, and a backlight for the later development of the universe. This light lost energy as the universe expanded over 13.7 billion years, so WMAP now sees the light as microwaves. By making accurate measurements of microwave patterns, WMAP has answered many longstanding questions about the universe's age, composition and development.This video from Goddard's tape archive features Dr. Bennett after the first results were announced in 2003. || ",
            "hits": 117
        },
        {
            "id": 10661,
            "url": "https://svs.gsfc.nasa.gov/10661/",
            "result_type": "Produced Video",
            "release_date": "2010-11-01T00:00:00-04:00",
            "title": "JWST Science Simulations: Galaxy Formation",
            "description": "Supercomputer Simulations of Galaxy Formation and Evolution. This visualization shows small galaxies forming, interacting, and merging to make ever-larger galaxies. This 'hierarchical structure formation' is driven by gravity and results in the creation of galaxies with spiral arms much like our own Milky Way galaxy. The Adaptive Mesh Refinement (AMR) simulation generated from ENZO code for cosmology and astrophysics was developed by Drs. Brian O'Shea and Michael Norman. The AMR code generated 1.8 terabytes of data and was computed at NCSA. AVL used Amore software (http://avl.ncsa.illinois.edu/what-we-do/software) to interpolate and render 2700 frames (42 gigabytes of HD images). The simulation spans a time period of 13.7 billion years. This visualization provides insight into the assembly and formation of galaxies. James Webb Space Telescope (JWST) will probe the earliest periods of galaxy formation by looking deep into space to see the first galaxies that form in the universe, only a few hundred million years after the Big Bang. The Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Drs. Brian O'Shea and Michael Norman to visualize the formation of a Milky Way-type galaxy. The Adaptive Mesh Refinement (AMR) simulation generated from ENZO code for cosmology and astrophysics was developed by Drs. Brian O'Shea and Michael Norman. The AMR code generated 1.8 terabytes of data and was computed at NCSA. AVL used Amore software (http://avl.ncsa.illinois.edu/what-we-do/software) to interpolate and render 2700 frames (42 gigabytes of HD images). The simulation spans a time period of 13.7 billion years. This visualization provides insight into the assembly and formation of galaxies. James Webb Space Telescope (JWST) will probe the earliest periods of galaxy formation by looking deep into space to see the first galaxies that form in the universe, only a few hundred million years after the Big Bang.AVL(http://avl.ncsa.illinois.edu/) at NCSA (http://ncsa.illinois.edu/), University of Illinois (www.illinois.edu) || ",
            "hits": 362
        },
        {
            "id": 10118,
            "url": "https://svs.gsfc.nasa.gov/10118/",
            "result_type": "Produced Video",
            "release_date": "2007-07-30T00:00:00-04:00",
            "title": "Journey Through the Cosmic Web: Cosmic Cruising 2",
            "description": "This animation flies through the cosmic web of the early universe. At the end, we see the Hubble Space Telescope collecting data points.Launched in 1990, the Hubble Space Telescope (HST) has revolutionized astronomy by providing unprecedented views of the Universe. Hubble's spectral range extends from the ultraviolet, through the visible, and into the near-infrared. NASA will fly a servicing mission in 2008 to bring two new science instruments to Hubble - the Cosmic Origins Spectrograph and the Wide Field Camera 3. New gyros and batteries will extend Hubble's life through 2013. || ",
            "hits": 357
        },
        {
            "id": 10121,
            "url": "https://svs.gsfc.nasa.gov/10121/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The WMAP Spacecraft",
            "description": "Scientists using NASA's Wilkinson Microwave Anistropy Probe (WMAP) have created the most detailed portrait of the infant Universe. By capturing the afterglow of the Big Bang, called the cosmic microwave background (CMB), we now believe the Universe to be 13.7 billion years olf. Encoded in these patterns is much-anticipated information about the fundamental properties of the early Universe. WMAP launched on June 30, 2001. || ",
            "hits": 139
        },
        {
            "id": 10122,
            "url": "https://svs.gsfc.nasa.gov/10122/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "WMAP Hard at Work",
            "description": "Scientists using NASA's Wilkinson Microwave Anistropy Probe (WMAP) have created the most detailed portrait of the infant Universe. By capturing the afterglow of the Big Bang, called the cosmic microwave background (CMB), we now believe the Universe to be 13.7 billion years old. Encoded in these patterns is much-anticipated information about the fundamental properties of the early Universe. WMAP launched on June 30, 2001. || ",
            "hits": 113
        },
        {
            "id": 10123,
            "url": "https://svs.gsfc.nasa.gov/10123/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "WMAP's Portrait of the Early Universe",
            "description": "Scientists using NASA's Wilkinson Microwave Anistropy Probe (WMAP) have created the most detailed portrait of the infant Universe. By capturing the afterglow of the Big Bang, called the cosmic microwave background (CMB), we now believe the Universe to be 13.7 billion years old. Encoded in these patterns is much—anticipated information about the fundamental properties of the early Universe. WMAP launched on June 30, 2001. || ",
            "hits": 352
        },
        {
            "id": 10128,
            "url": "https://svs.gsfc.nasa.gov/10128/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Big Bang",
            "description": "This dominant cosmological theory suggests the Universe began nearly 13.7 billion years ago, expanding rapidly from a very dense and incredibly hot state. Eventually, stars ignited and galaxies slowly formed. The Big Bang theory has been imporved and advanced especially through NASA's Cosmic Background Explorer (COBE) and WMAP missions. This animation conceptualizes these explosive beginnings of the Universe. || ",
            "hits": 1031
        },
        {
            "id": 10129,
            "url": "https://svs.gsfc.nasa.gov/10129/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Dark Ages",
            "description": "This animation shows in a cube what the early universe was like - very dense until bubbles formed creating pockets that gave birth to the first stars and galaxies. || DarkAges0738.jpg (1280x720) [61.2 KB] || DarkAges0738_web.png (320x180) [92.6 KB] || DarkAges0738_thm.png (80x40) [7.5 KB] || DarkAges_HD_LARGE_QT_Video_2.webmhd.webm (960x540) [4.2 MB] || DarkAges_HD_LARGE_QT_Video_2.mov (1280x720) [75.7 MB] || DarkAges_HD_LARGE_QT_Video_1.mp4 (1280x720) [19.9 MB] || 1280x720_16x9 (1280x720) [128.0 KB] || dark_ages_720p.m2v (1280x720) [5.7 MB] || dark_ages_512x288.m1v (512x288) [8.6 MB] || ",
            "hits": 121
        },
        {
            "id": 10130,
            "url": "https://svs.gsfc.nasa.gov/10130/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Cosmic Dawn (Still Image with Titles)",
            "description": "About 300,000 years after the Big Bang, the Universe spread out enough that free electrons and protons could form atomic hydrogen. These atoms readily absorb light, thus creating an opaque murky era known as the cosmic Dark Ages. Roughly 900 million years later, the Universe underwent a Reionization Period. The earliest stars and quasars generated enough ultraviolet light to turn hydrogen atoms back into protons and electrons. These areas began as bubbles, continually spreading until light was permitted to travel freely through the Universe. This moment has been dubbed the Cosmic Dawn. || ",
            "hits": 59
        },
        {
            "id": 10131,
            "url": "https://svs.gsfc.nasa.gov/10131/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Cosmic Dawn (Still Image Without Titles)",
            "description": "About 300,000 years after the Big Bang, the Universe spread out enough that free electrons and protons could form atomic hydrogen. These atoms readily absorb light, thus creating an opaque murky era known as the cosmic Dark Ages. Roughly 900 million years later, the Universe underwent a Reionization Period. The earliest stars and quasars generated enough ultraviolet light to turn hydrogen atoms back into protons and electrons. These areas began as bubbles, continually spreading until light was permitted to travel freely through the Universe. This moment has been dubbed the Cosmic Dawn. || ",
            "hits": 109
        },
        {
            "id": 10133,
            "url": "https://svs.gsfc.nasa.gov/10133/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "The Helium Atom",
            "description": "Helium nuclei were created in the Big Bang and contain two protons and two neutrons each. Helium is the second most abundant element, comprising roughly one quarter of the mass of the Universe. This animation zooms into a standard helium atom, showing its protons (green), neutrons (white), and electrons (blue). || ",
            "hits": 289
        },
        {
            "id": 10135,
            "url": "https://svs.gsfc.nasa.gov/10135/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "Dark Energy Expands the Universe",
            "description": "It is believed that after the Big Bang, the universe originally decelerated in its expansion, but then 'changed gears' and began to accelerate. The unknown force causing this recent acceleration is dubbed the 'Dark Energy.' This visualization flies through a series of galaxy clusters, the largerst gravitationally-bound objects in the Universe. || ",
            "hits": 439
        },
        {
            "id": 10137,
            "url": "https://svs.gsfc.nasa.gov/10137/",
            "result_type": "Produced Video",
            "release_date": "2007-07-03T00:00:00-04:00",
            "title": "Brane Theory of Multiple Dimensions",
            "description": "This animation attempts to convey the Brane Theory of Multiple Dimensions in which there are multiple universes, the touching of any two causing an event such as the Big Bang. || ",
            "hits": 600
        },
        {
            "id": 97,
            "url": "https://svs.gsfc.nasa.gov/97/",
            "result_type": "Visualization",
            "release_date": "1996-02-08T12:00:00-05:00",
            "title": "Images of Earth and Space: The Role of Visualization in NASA Science",
            "description": "This compilation video contains visualizations of Earth and Space Sciences resulting from supercomputer models. The excerpted visualizations include: Ocean Planet, El Niño, Ozone 1991, Clouds, Changes in Glacier Bay, Alaska, Biosphere, Lunar Topography from the Clementine Mission, Musculoskeletal Modeling Dynamic Simulations, Simulations of the Breakup and Dynamical Evolution of Comet Shoemaker-Levy 9, Convective Penetration in Stellar Interiors, Topological Features of a Compressible Plasma Vortex Sheet: A Model for the Outer Heliospheric Solar Wind, R-Aquarii Jet, The Evolution of Distorted Black Holes, Rayleigh-Taylor Instability in a Supernova, Galaxy Harassment, N-Body Simulation of the Cold Dark Matter Cosmology. || ",
            "hits": 137
        }
    ]
}