{
    "count": 4,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 14297,
            "url": "https://svs.gsfc.nasa.gov/14297/",
            "result_type": "Produced Video",
            "release_date": "2023-03-01T10:00:00-05:00",
            "title": "How NASA's Roman Space Telescope Will Rewind the Universe",
            "description": "In this simulated view of the deep cosmos, each dot represents a galaxy. The three small squares show Hubble's field of view, and each reveals a different region of the synthetic universe. Roman will be able to quickly survey an area as large as the whole zoomed-out image, which will give us a glimpse of the universe’s largest structures.Credits: NASA’s Goddard Space Flight Center/A. Yung || Yung_Stucture_Survey-Hubble.gif (800x800) [10.9 MB] || Yung_Structure_Survey-Hubble_ProRes.mov (800x800) [36.3 MB] || Yung_Structure_Survey-Hubble_800.mp4 (800x800) [6.4 MB] || Yung_Structure_Survey-Hubble_800.webm (800x800) [1.6 MB] || ",
            "hits": 134
        },
        {
            "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": 367
        },
        {
            "id": 10663,
            "url": "https://svs.gsfc.nasa.gov/10663/",
            "result_type": "Produced Video",
            "release_date": "2010-11-01T00:00:00-04:00",
            "title": "Webb Science Simulations: Re-Ionization Era",
            "description": "The visualization shows galaxies, composed of gas, stars and dark matter, colliding and forming filaments in the large-scale universe providing a view of the Cosmic Web. The Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Drs. Renyue Cen and Jeremiah Ostriker to visualize a simulation of the nonlinear cosmological evolution of the universe.  Drs. Cen and Ostriker developed one of the largest cosmological hydrodynamic simulations and computed over 749 gigabytes of raw data at the NCSA in 2005. AVL used Amore software (http://avl.ncsa.illinois.edu/what-we-do/software) to interpolate and render approximately 322 gigabytes of a subset of the computed data. The simulation begins about 20 million years after the Big Bang - about 13.7 billion years ago - and extends until the present day.AVL(http://avl.ncsa.illinois.edu/) at NCSA (http://ncsa.illinois.edu/), University of Illinois (www.illinois.edu) || ",
            "hits": 279
        },
        {
            "id": 10223,
            "url": "https://svs.gsfc.nasa.gov/10223/",
            "result_type": "Produced Video",
            "release_date": "2008-05-20T00:00:00-04:00",
            "title": "Cosmic Origins Spectrograph: Large Scale Structure of the Universe",
            "description": "The Cosmic Origins Spectrograph (COS) instrument will be placed in the Hubble Space Telescope during Service Mission 4. It's primary science objectives are the study of the origins of large scale structure in the Universe, the formation and evolution of galaxies, the origin of stellar and planetary systems, and the cold interstellar medium. This animation zooms out from our Milky Way galaxy to show the cosmic web, or large scale structure of the Universe. || ",
            "hits": 114
        }
    ]
}