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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": 118
        },
        {
            "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": 95
        },
        {
            "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": 97
        },
        {
            "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": 85
        },
        {
            "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": 240
        },
        {
            "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": 69
        },
        {
            "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": 132
        },
        {
            "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": 939
        },
        {
            "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": 127
        },
        {
            "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": 103
        },
        {
            "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": 408
        },
        {
            "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": 1291
        },
        {
            "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": 188
        },
        {
            "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": 33
        },
        {
            "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": 153
        },
        {
            "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": 260
        },
        {
            "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": 338
        },
        {
            "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": 731
        }
    ]
}