{
    "count": 11,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 11491,
            "url": "https://svs.gsfc.nasa.gov/11491/",
            "result_type": "Produced Video",
            "release_date": "2014-02-24T19:00:00-05:00",
            "title": "Landsat 8 Onion Skin",
            "description": "Landsat satellites circle the globe every 99 minutes, collecting data about the land surfaces passing underneath.  After 16 days, the Landsat satellite has passed over every spot on the globe, and recorded data in 11 different wavelength regions.  The individual wavelength bands can be combined into color images, with different combinations of the 11 bands revealing different information about the condition of the land cover.The data for this video was collected by Landsat 5 on November 10, 2011. || ",
            "hits": 50
        },
        {
            "id": 11484,
            "url": "https://svs.gsfc.nasa.gov/11484/",
            "result_type": "Produced Video",
            "release_date": "2014-02-18T12:00:00-05:00",
            "title": "Engineering That Enables Science",
            "description": "A series of programs that define the spirit of engineering and showcase the unique capabilities within Goddard's Detector Systems Branch. || ",
            "hits": 17
        },
        {
            "id": 4040,
            "url": "https://svs.gsfc.nasa.gov/4040/",
            "result_type": "Visualization",
            "release_date": "2013-02-05T00:00:00-05:00",
            "title": "Florida Everglades LDCM Band Remix",
            "description": "The Landsat Data Continuity Mission (LDCM) is the future of Landsat satellites. LDCM launched on February 11, 2013. Landsat satellites view the Earth through a number of different bands. Each band captures imagery in different spectral wavelengths. Scientists can combine these bands a number of ways to obtain information about the satellite imagery. This visualization shows several different band combinations over the Florida Everglades. || ",
            "hits": 63
        },
        {
            "id": 4025,
            "url": "https://svs.gsfc.nasa.gov/4025/",
            "result_type": "Visualization",
            "release_date": "2013-01-20T00:00:00-05:00",
            "title": "Florida Everglades Onion Skin Stills",
            "description": "Landsat satellites view the Earth through a number of different bands. Each band captures imagery in different spectral wavelengths. Scientists can then combine these bands a number of ways to obtain information about the satellite imagery. These still images show several different band combinations alongside the resulting imagery over the Florida Everglades.These still images were produced for use on NASA travelling exhibits. || ",
            "hits": 26
        },
        {
            "id": 11005,
            "url": "https://svs.gsfc.nasa.gov/11005/",
            "result_type": "Produced Video",
            "release_date": "2012-06-25T00:00:00-04:00",
            "title": "Thermal Radiation and the Electromagnetic Spectrum",
            "description": "A short animation illustrating the relationship of temperature and wavelength.  Hotter objects have a shorter wavelength and cooler objects have a longer wavelength.  The animation also compares the wavelengths of visible light and thermal infrared radiation. || ",
            "hits": 365
        },
        {
            "id": 10251,
            "url": "https://svs.gsfc.nasa.gov/10251/",
            "result_type": "Produced Video",
            "release_date": "2008-05-31T00:00:00-04:00",
            "title": "GLAST Prelude, for Brass Quintet, Op.12",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institiutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S. Music composed by Nolan Gasser, © 2008 Music performed by the American Brass Quintet || ",
            "hits": 30
        },
        {
            "id": 10248,
            "url": "https://svs.gsfc.nasa.gov/10248/",
            "result_type": "Produced Video",
            "release_date": "2008-05-23T00:00:00-04:00",
            "title": "GLASTcast Episode 2:  What are Gamma Rays?",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  Somewhere out in the vast depths of space, a giant star explodes with the power of millions of suns. As the star blows up, a black hole forms at its center. The black hole blows two blowtorches in opposite directions, in narrow jets of gamma rays. NASA's Gamma-ray Large Area Space Telescope, or GLAST, will catch about 200 of these explosions, known as gamma-ray bursts, each year. GLAST's detailed observations may give astronomers the clues they need to unravel the mystery of what exactly produces these gamma-ray bursts, which are the brightest explosions in the universe since the Big Bang.  Interviews with (in order of appearance):  Phil Plait - Astronomer, Bad Astronomy David Thompson - GLAST Deputy Project Scientist, NASA Goddard Valerie Connaughton - GLAST Burst Monitor (GBM) Team, NASA Marshall/University of Alabama Neil Gehrels - GLAST Deputy Project Scientist, NASA Goddard Isabelle Grenier - Principal Investigator of the GLAST French contribution, French Atomic Energy Commission Peter Michaelson - Large Area Telescope (LAT) Principal Investigator, Stanford University Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall Martin Pohl - GLAST Interdisciplinary Scientist, Iowa State University Steve Ritz - GLAST Project Scientist, NASA Goddard || ",
            "hits": 21
        },
        {
            "id": 10220,
            "url": "https://svs.gsfc.nasa.gov/10220/",
            "result_type": "Produced Video",
            "release_date": "2008-05-20T00:00:00-04:00",
            "title": "Wide Field Camera 3: Seeing in Different Wavelengths (no labels)",
            "description": "The Wide Field Camera 3 (WFC3) allows Hubble to peer ever further into the mysteries of the cosmos — in several wavelengths. This animation shows the wide variety of features and objects WFC3 can observe at different wavelengths. || ",
            "hits": 18
        },
        {
            "id": 10221,
            "url": "https://svs.gsfc.nasa.gov/10221/",
            "result_type": "Produced Video",
            "release_date": "2008-05-20T00:00:00-04:00",
            "title": "Wide Field Camera 3: Seeing in Different Wavelengths (with labels)",
            "description": "The Wide Field Camera 3 (WFC3) allows Hubble to peer ever further into the mysteries of the cosmos — in several wavelengths. This animation shows the wide variety of features and objects WFC3 can observe at different wavelengths. || ",
            "hits": 20
        },
        {
            "id": 10222,
            "url": "https://svs.gsfc.nasa.gov/10222/",
            "result_type": "Produced Video",
            "release_date": "2008-05-20T00:00:00-04:00",
            "title": "Wide Field Camera 3: Redshift",
            "description": "The Wide Field Camera 3 (WFC3) gives Hubble greater sensitivity in Infrared wavelengths, thus enabling it to see objects more distant than instruments currently on board. || ",
            "hits": 13
        },
        {
            "id": 20113,
            "url": "https://svs.gsfc.nasa.gov/20113/",
            "result_type": "Animation",
            "release_date": "2007-09-07T00:00:00-04:00",
            "title": "Gamma Ray Creation",
            "description": "Gamma rays are the highest-energy forms of light in the electromagnetic spectrum and they can have over a billion times the energy of the type of light visible to the human eye. Gamma rays can be created in several different ways: a high-energy particle can collide with another particle, a particle can collide and annihilate with its anti-particle, an element can undergo radioactive decay, or a charged particle can be accelerated. In this animation, we see a high-energy photon collide with a free electron, which causes the creation of a gamma-ray. || ",
            "hits": 304
        }
    ]
}