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    "results": [
        {
            "id": 14255,
            "url": "https://svs.gsfc.nasa.gov/14255/",
            "result_type": "Produced Video",
            "release_date": "2022-12-07T11:00:00-05:00",
            "title": "NASA’s Fermi, Swift Capture Revolutionary Gamma-Ray Burst",
            "description": "Watch to learn how an event called GRB 211211A rocked scientists’s understanding of gamma-ray bursts – the most powerful explosions in the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic Credits: \"Finished Plate\" by Airglo and \"Binary Fission\" by Tom KaneWatch this video on the NASA Goddard YouTube channel. || Title_Card_Revolutionary_GRB.jpg (1920x1080) [1.5 MB] || Title_Card_Revolutionary_GRB_searchweb.png (320x180) [100.7 KB] || Title_Card_Revolutionary_GRB_thm.png (80x40) [7.3 KB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.mp4 (1920x1080) [171.9 MB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst_ProRes.mov (1920x1080) [2.2 GB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.webm (1920x1080) [18.4 MB] || Long_GRB_Captions.en_US.srt [2.8 KB] || Long_GRB_Captions.en_US.vtt [2.8 KB] || ",
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        },
        {
            "id": 11292,
            "url": "https://svs.gsfc.nasa.gov/11292/",
            "result_type": "Produced Video",
            "release_date": "2013-06-03T11:00:00-04:00",
            "title": "Water on the Moon",
            "description": "Since the 1960’s, scientists have suspected that frozen water could survive in cold, dark craters at the Moon’s poles.  While previous lunar missions have detected hints of water on the Moon, new data from the Lunar Reconnaissance Orbiter (LRO) pinpoints areas near the south pole where water is likely to exist.  The key to this discovery is hydrogen, the main ingredient in water: LRO uses its Lunar Exploration Neutron Detector, or LEND, to measure how much hydrogen is trapped within the lunar soil.  By combining years of LEND data, scientists see mounting evidence of hydrogen-rich areas near the Moon’s south pole, strongly suggesting the presence of frozen water. || ",
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        {
            "id": 4057,
            "url": "https://svs.gsfc.nasa.gov/4057/",
            "result_type": "Visualization",
            "release_date": "2013-03-25T00:00:00-04:00",
            "title": "LEND Looks for Water at the South Pole",
            "description": "Since Lunar Reconnaissance Orbiter (LRO) entered lunar orbit in 2009, its neutron detector, LEND, has been counting the neutrons coming from the Moon's surface.Neutrons are created when galactic cosmic rays strike atoms in the lunar regolith. These neutrons bounce from atom to atom like billiard balls, losing energy with each collision. Along the way, some of these neutrons escape into space, where LEND can detect them.The presence of hydrogen in the lunar soil reduces the number of neutrons that escape. To map out likely deposits of water ice, LEND scientists look for this deficit of neutrons in the epithermal (medium) energy range.If the deficit were simply due to random fluctuations, the hydrogen map would never coalesce into a sharp image, but as this animation shows, the map of epithermal neutron deficit at the south pole of the Moon improves over time and converges on particular spots. These include especially strong signals in the permanently shadowed parts of Cabeus and Shoemaker craters, where ice would be completely shielded from the sun. But LEND and other missions have found signs of water in places that aren't permanently shadowed while apparently excluding some places that are, both of which are surprising and exciting discoveries. || ",
            "hits": 516
        },
        {
            "id": 4043,
            "url": "https://svs.gsfc.nasa.gov/4043/",
            "result_type": "Visualization",
            "release_date": "2013-03-06T11:00:00-05:00",
            "title": "LRO Peers into Permanent Shadows",
            "description": "The Moon's permanently shadowed regions, or PSRs, are places on the Moon that haven't seen the Sun in millions, or even billions, of years. The Earth's tilted axis allows sunlight to fall everywhere on its surface, even at the poles, for at least part of the year. But the Moon's tilt relative to the Sun is only 1.6°, not enough to get sunlight into some deep craters near the lunar north and south poles. PSRs are therefore some of the coldest, darkest places in the solar system.Because of that, PSRs are expected to be excellent traps for volatiles, chemicals that would normally vaporize and escape into space, and this includes water. Lunar Reconnaissance Orbiter (LRO) includes several instruments designed to peer into the PSR darkness and measure temperature, reflectivity, and neutron absorption, all of which are clues to what chemicals might be hiding there. This animation shows where the PSRs are and in what ways LRO can see inside them. || ",
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        {
            "id": 10743,
            "url": "https://svs.gsfc.nasa.gov/10743/",
            "result_type": "Produced Video",
            "release_date": "2011-03-31T00:00:00-04:00",
            "title": "LEND: The Lunar Neutron Counter",
            "description": "How would you find out where to look for water on the Moon? NASA's Lunar Reconnaissance Orbiter has a unique answer: Count the neutrons coming from the Moon! By measuring the relative amounts of slow and fast neutrons coming from soil on the Moon, scientists think they can estimate the amount of hydrogen. And it's believed that where there's hydrogen, there might also be water! Find out more about LEND by watching this video. || ",
            "hits": 73
        },
        {
            "id": 20157,
            "url": "https://svs.gsfc.nasa.gov/20157/",
            "result_type": "Animation",
            "release_date": "2008-07-21T12:00:00-04:00",
            "title": "Neutron Stars - A Closer Perspective:",
            "description": "Two views of a Neutron Star: First, a closeup view of a neutron star cycling before, during and after a gamma ray burst and second, crossing a Protoplanetary Nebula toward an elusive Neutron Star || ",
            "hits": 122
        },
        {
            "id": 2750,
            "url": "https://svs.gsfc.nasa.gov/2750/",
            "result_type": "Visualization",
            "release_date": "2003-09-02T12:00:00-04:00",
            "title": "RHESSI Observes 2.2 MeV Line Emission from a Solar Flare",
            "description": "The solar flare at Active Region 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission. || ",
            "hits": 32
        }
    ]
}