{
    "count": 18,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 31019,
            "url": "https://svs.gsfc.nasa.gov/31019/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-01-15T15:00:00-05:00",
            "title": "Stephan's Quintet",
            "description": "This visualization uses Hubble data to simulate a flight past the galaxies known as Stephan’s Quintet, providing an illuminating perspective on their position and gravitational relationships to one another. || STScI-H-StephansQuintet_1920x1080.00001_print.jpg (1024x576) [38.8 KB] || STScI-H-StephansQuintet_1920x1080.00001_searchweb.png (320x180) [34.0 KB] || STScI-H-StephansQuintet_1920x1080.00001_thm.png (80x40) [3.5 KB] || STScI-H-StephansQuintet_1280x720.mp4 (1280x720) [18.9 MB] || STScI-H-StephansQuintet_1920x1080.mp4 (1920x1080) [41.5 MB] || STScI-H-StephansQuintet_1920x1080.webm (1920x1080) [10.6 MB] || STScI-H-StephansQuintet_640x360.mp4 (640x360) [5.0 MB] || STScI-H-StephansQuintet_H265-3180x2160.mp4 (3840x2160) [37.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || STScI-H-StephansQuintet_3180x2160.mp4 (3840x2160) [104.9 MB] || ",
            "hits": 77
        },
        {
            "id": 30994,
            "url": "https://svs.gsfc.nasa.gov/30994/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-10-15T10:00:00-04:00",
            "title": "Messier 82: Cigar Galaxy in Multiple Wavelengths",
            "description": "Massive burst of star formation in the core or M82 burst becomes clearer in infrared. || STScI-H-M82_1x-1920x1080.00001_print.jpg (1024x576) [79.3 KB] || STScI-H-M82_1x-1920x1080.00001_searchweb.png (320x180) [66.4 KB] || STScI-H-M82_1x-1920x1080.00001_thm.png (80x40) [4.5 KB] || STScI-H-M82_1x-1280x720.mp4 (1280x720) [5.0 MB] || STScI-H-M82_1x-1920x1080.mp4 (1920x1080) [11.8 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M82_1x-1920x1080.webm (1920x1080) [5.2 MB] || STSCI-H-M82_1x-3840x2160.mp4 (3840x2160) [12.8 MB] || STSCI-H-M82_1x-H265-3840x2160.mp4 (3840x2160) [6.0 MB] || STScI-H-M82_1x-640x360.mp4 (640x360) [1.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 107
        },
        {
            "id": 30981,
            "url": "https://svs.gsfc.nasa.gov/30981/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-08-20T10:00:00-04:00",
            "title": "Messier 81 in Multiple Wavelengths",
            "description": "Star-forming regions in M81 become evident in infrared. || STScI-J-M81_1x-1920x1080_0021_print.jpg (1920x1080) [580.2 KB] || STScI-J-M81_1x-1920x1080_0021_print_searchweb.png (320x180) [84.8 KB] || STScI-J-M81_1x-1920x1080_0021_print_thm.png (80x40) [6.0 KB] || STScI-J-M81_1x-1280x720.mp4 (1280x720) [5.2 MB] || STScI-J-M81_1x-1920x1080.mp4 (1920x1080) [11.2 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-J-M81_1x-1920x1080.webm (1920x1080) [3.5 MB] || STScI-J-M81_1x-640x360.mp4 (640x360) [1.7 MB] || STScI-J-M81_1x-3840x2160.mp4 (3840x2160) [8.4 MB] || STScI-J-M81_1x-H265-3840x2160.mp4 (3840x2160) [4.0 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 115
        },
        {
            "id": 30969,
            "url": "https://svs.gsfc.nasa.gov/30969/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-06-18T10:00:00-04:00",
            "title": "M101 (Pinwheel Galaxy)",
            "description": "This animation shows the Messier 101 (Pinwheel) Galaxy, with simulated rotation, in visible, then infrared, then X-ray, and finally all three combined. || STScI-H-M101_1x-1920x1080.00001_print.jpg (1024x576) [150.4 KB] || STScI-H-M101_1x-1920x1080.00001_searchweb.png (320x180) [99.4 KB] || STScI-H-M101_1x-1920x1080.00001_thm.png (80x40) [6.3 KB] || STScI-H-M101_1x-1280x720.mp4 (1280x720) [18.1 MB] || STScI-H-M101_1x-1920x1080.mp4 (1920x1080) [50.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M101_1x-1920x1080.webm (1920x1080) [5.6 MB] || STScI-H-M101_1x-640x360.mp4 (640x360) [7.8 MB] || STScI-H-M101_1x-3840x2160.mp4 (3840x2160) [32.3 MB] || STScI-H-M101_1x-H265-3840x2160.mp4 (3840x2160) [11.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 229
        },
        {
            "id": 30957,
            "url": "https://svs.gsfc.nasa.gov/30957/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-25T10:00:00-04:00",
            "title": "Flight Through the Orion Nebula in Visible and Infrared Light",
            "description": "This visualization zooms into the Orion Nebula and then flies through a 3D model using both visible light (Hubble Space Telescope) and infrared light (Spitzer Space Telescope) views. || orion_vis_ir_zoom_xfade-1920x1080.png (1920x1080) [1.2 MB] || orion_vis_ir_zoom_xfade-1920x1080_print.jpg (1024x576) [66.7 KB] || orion_vis_ir_zoom_xfade-3840x2160.png (3840x2160) [3.5 MB] || orion_vis_ir_zoom_xfade-1920x1080_searchweb.png (320x180) [66.6 KB] || orion_vis_ir_zoom_xfade-1920x1080_thm.png (80x40) [5.7 KB] || orion_vis_ir_zoom_xfade-1920x1080p30.mp4 (1920x1080) [406.0 MB] || orion_vis_ir_zoom_xfade-3840x2160p30.webm (3840x2160) [25.1 MB] || orion_vis_ir_zoom_xfade-3840x2160p30.mp4 (3840x2160) [836.9 MB] || flight-through-the-orion-nebula-in-visible-and-infrared-light-4k.hwshow || flight-through-the-orion-nebula-in-visible-and-infrared-light-hd.hwshow || ",
            "hits": 117
        },
        {
            "id": 30954,
            "url": "https://svs.gsfc.nasa.gov/30954/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-23T12:00:00-04:00",
            "title": "Celestial Lightsabers: Stellar Jets in HH24",
            "description": "This visualization combines a two-dimensional zoom and a three-dimensional flight to showcase the resemblance to a double-bladed lightsaber seen in the Hubble Space Telescope's striking image of the Herbig-Haro object known as HH24. || hh24_fly-example_frame-1920x1080.png (1920x1080) [1.6 MB] || hh24_fly-example_frame-1920x1080_print.jpg (1024x576) [43.0 KB] || hh24_fly-example_frame-1920x1080_searchweb.png (320x180) [56.6 KB] || hh24_fly-example_frame-1920x1080_thm.png (80x40) [4.8 KB] || hh24_zoom_fly-b-1920x1080p30.mov (1920x1080) [228.0 MB] || hh24_zoom_fly-b-1920x1080p30.mp4 (1920x1080) [15.6 MB] || hh24_zoom_fly-b-1920x1080p30.webm (1920x1080) [4.6 MB] || ",
            "hits": 40
        },
        {
            "id": 30953,
            "url": "https://svs.gsfc.nasa.gov/30953/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-23T11:00:00-04:00",
            "title": "Evaporating Peaks: Pillars in the Monkey Head Nebula",
            "description": "This scientific visualization zooms from the night sky to some pillars in the Monkey Head Nebula (aka NGC 2174). After cross-fading to an infrared view, the sequence showcases the 3D nature of these gaseous peaks. || ngc2174_zoom_reveal-example_frame-1920x1080.png (1920x1080) [2.3 MB] || ngc2174_zoom_reveal-example_frame-1920x1080_print.jpg (1024x576) [105.3 KB] || ngc2174_zoom_reveal-example_frame-1920x1080_searchweb.png (320x180) [92.0 KB] || ngc2174_zoom_reveal-example_frame-1920x1080_thm.png (80x40) [6.6 KB] || ngc2174_zoom_reveal-b-1920x1080.wmv (1920x1080) [46.2 MB] || ngc2174_zoom_reveal-b-1920x1080.m4v (1920x1080) [45.7 MB] || ngc2174_zoom_reveal-1920x1080p30.webm (1920x1080) [6.5 MB] || ngc2174_zoom_reveal-1920x1080p30.mov (1920x1080) [375.6 MB] || evaporating-peaks-pillars-in-the-monkey-head-nebula.hwshow [337 bytes] || ",
            "hits": 60
        },
        {
            "id": 30947,
            "url": "https://svs.gsfc.nasa.gov/30947/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-15T14:00:00-04:00",
            "title": "Orion Nebula from Hubble",
            "description": "Orion Nebula from Hubble (2006) || orion_nebula-hst-9000x9000_print.jpg (1024x1024) [161.5 KB] || orion_nebula-hst-9000x9000.png (9000x9000) [79.3 MB] || orion_nebula-hst-9000x9000_searchweb.png (320x180) [85.2 KB] || orion_nebula-hst-9000x9000_thm.png (80x40) [6.3 KB] || orion-nebula-from-hubble.hwshow [218 bytes] || ",
            "hits": 463
        },
        {
            "id": 30941,
            "url": "https://svs.gsfc.nasa.gov/30941/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-04-23T10:00:00-04:00",
            "title": "Colliding Galaxies (NGC 2207)",
            "description": "This animation shows the interacting galaxy pair NGC 2207, first in optical light, then in infrared, in X-ray, and finally in combination. || STScI-H-NGC2207_1x-1920x1080.00001_print.jpg (1024x576) [157.8 KB] || STScI-H-NGC2207_1x-1920x1080.00001_searchweb.png (320x180) [92.0 KB] || STScI-H-NGC2207_1x-1920x1080.00001_thm.png (80x40) [6.5 KB] || STScI-H-NGC2207_1x-1280x720.mp4 (1280x720) [4.5 MB] || STScI-H-NGC2207_1x-1920x1080.mp4 (1920x1080) [9.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-NGC2207_1x-1920x1080.webm (1920x1080) [4.9 MB] || STScI-H-NGC2207_1x-640x360.mp4 (640x360) [1.5 MB] || STScI-H-NGC2207_1x-3840x2160.mp4 (3840x2160) [8.8 MB] || STScI-H-NGC2207_1x-H265-3840x2160.mp4 (3840x2160) [4.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 188
        },
        {
            "id": 30860,
            "url": "https://svs.gsfc.nasa.gov/30860/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-02-28T12:00:00-05:00",
            "title": "Mystic Mountain: Pillars in the Carina Nebula from Hubble",
            "description": "A collection of pillars in the Carina Nebula create a gaseous landscape nicknamed \"Mystic Mountain\" || carina_mystic_mountain_wide-hst-3218x3240_print.jpg (1024x1031) [214.6 KB] || carina_mystic_mountain_wide-hst-3218x3240.png (3218x3240) [14.7 MB] || carina_mystic_mountain_wide-hst-3218x3240_searchweb.png (320x180) [92.5 KB] || carina_mystic_mountain_wide-hst-3218x3240_thm.png (80x40) [6.7 KB] || carina_mystic_mountain_wide-hst-308560.key [15.2 MB] || carina_mystic_mountain_wide-hst-308560.pptx [14.8 MB] || mystic-mountain-pillars-in-the-carina-nebula-from-hubble.hwshow [362 bytes] || ",
            "hits": 113
        },
        {
            "id": 30859,
            "url": "https://svs.gsfc.nasa.gov/30859/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-02-28T10:00:00-05:00",
            "title": "Gaseous Pillar in the Carina Nebula from Hubble",
            "description": "Gaseous Pillar and Stellar Jet in the Carina Nebula || carina_pillar_jet_ff-hst-3183x3240_print.jpg (1024x1042) [320.1 KB] || carina_pillar_jet_ff-hst-3183x3240.png (3183x3240) [16.1 MB] || carina_pillar_jet_ff-hst-3183x3240_searchweb.png (320x180) [94.4 KB] || carina_pillar_jet_ff-hst-3183x3240_thm.png (80x40) [9.0 KB] || carina_pillar_jet_ff-hst-30859.key [16.6 MB] || carina_pillar_jet_ff-hst-30859.pptx [16.1 MB] || gaseous-pillar-in-the-carina-nebula-from-hubble.hwshow [339 bytes] || ",
            "hits": 53
        },
        {
            "id": 11821,
            "url": "https://svs.gsfc.nasa.gov/11821/",
            "result_type": "Produced Video",
            "release_date": "2015-03-25T14:00:00-04:00",
            "title": "Suzaku, Herschel Link a Black-hole 'Wind' to a Galactic Gush",
            "description": "This movie illustrates how black-hole feedback works in quasars. Dense gas and dust in the center simultaneously fuels the black hole and shrouds it from view. The black-hole wind propels large-scale outflows of cold gas and powers a shock wave that clears gas and dust from the central galaxy.Video credit: NASA's Goddard Space Flight Center || Suzaku_Quasar_Wind_STILL.png (1920x1080) [8.1 MB] || Suzaku_Quasar_Wind_STILL_print.jpg (1024x576) [41.8 KB] || Suzaku_Quasar_Wind_STILL_searchweb.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_web.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_thm.png (80x40) [7.9 KB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.webm (960x540) [3.3 MB] || 11821_Suzaku_Quasar_Wind_FINAL.mov (1920x1080) [333.5 MB] || 1920x1080_16x9_30p (1920x1080) [32.0 KB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Best_1920x1080_2997.mov (1920x1080) [295.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Good_1920x1080_2997.mov (1920x1080) [36.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL-MPEG4_1920X1080_2997.mp4 (1920x1080) [13.0 MB] || 11821_Suzaku_Quasar_Wind_FINAL_1280x720.wmv (1280x720) [13.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.m4v (960x540) [13.6 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_lg.m4v (640x360) [5.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_sm.mp4 (320x240) [2.6 MB] || ",
            "hits": 44
        },
        {
            "id": 30571,
            "url": "https://svs.gsfc.nasa.gov/30571/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-01-15T00:00:00-05:00",
            "title": "Science with SOFIA",
            "description": "First image in presentation || sofia_montage_print.jpg (1024x575) [201.0 KB] || sofia_montage.png (4098x2304) [7.8 MB] || sofia_montage_searchweb.png (320x180) [106.7 KB] || sofia_montage_web.png (320x179) [106.7 KB] || sofia_montage_thm.png (80x40) [8.4 KB] || randolf_klein_sofia.hwshow [60 bytes] || Dr. Randolf Klein's AAS presentation from January 2015 || ",
            "hits": 32
        },
        {
            "id": 30774,
            "url": "https://svs.gsfc.nasa.gov/30774/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-01-05T00:00:00-05:00",
            "title": "Pillars in the Eagle Nebula from Hubble (2014)",
            "description": "Hubble revisits the famous Pillars of Creation and reveals new details in a wider view. || eagle_pillars_2015-hst-3107x3240_print.jpg (1024x1067) [213.1 KB] || eagle_pillars_2015-hst-3107x3240.png (3107x3240) [16.6 MB] || eagle_pillars_2015-hst-6780x7071.png (6780x7071) [91.0 MB] || eagle_pillars_2015-hst-3107x3240_searchweb.png (320x180) [89.7 KB] || eagle_pillars_2015-hst-3107x3240_thm.png (80x40) [6.9 KB] || pillars-in-the-eagle-nebula-from-hubble-2014.hwshow [332 bytes] || ",
            "hits": 99
        },
        {
            "id": 30124,
            "url": "https://svs.gsfc.nasa.gov/30124/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "A Journey Into Andromeda",
            "description": "Andromeda galaxy–also called M31 by astronomers–is the largest galaxy in the Local Group, the group of galaxies that our Milky Way galaxy also belongs to. The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope (HST) Multi-cycle program to map roughly a third of M31’s star forming disk, using 6 filters covering from the ultraviolet through the near infrared. With HST’s resolution and sensitivity, the disk of M31 will be resolved into more than 100 million stars, enabling a wide range of scientific endeavors.This movie starts with a 1.5 x 3.0 kiloparsec (KPC) view of part of Andromeda's major star forming ring. The field contains millions of stars, mottled by filaments of dust, which dim and redden the background stars. As the movie begins, it zooms into the region, revealing a rich mix of old red stars and young blue stars, along with occasional background galaxies and emission line nebulosity. As the movie pans across, it moves into regions of intense star formation, traced by thousands of bright blue stars.Satellite: Hubble Space Telescope || ",
            "hits": 72
        },
        {
            "id": 30142,
            "url": "https://svs.gsfc.nasa.gov/30142/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "W3 Star-Forming Complex in Perseus by Spitzer and SOFIA",
            "description": "This mid-infrared image of the W3A star cluster in the inset was captured by the FORCAST camera on the SOFIA flying observatory in 2011. It is overlaid on a near-infrared image of the W3 star-forming region from the Spitzer space telescope. The SOFIA image scale is 150 x 100 arcseconds, and the red, green and blue colors represent 37, 20 and 7 μm. The red, green and blue colors in the background image from Spitzer represent 7.9, 4.5, 3.6 μm. || ",
            "hits": 27
        },
        {
            "id": 30135,
            "url": "https://svs.gsfc.nasa.gov/30135/",
            "result_type": "Hyperwall Visual",
            "release_date": "2011-11-30T12:00:00-05:00",
            "title": "SOFIA views a star-forming region",
            "description": "The name W40 designates this object's number in a catalog of HII regions, clouds of ionized hydrogen often associated with star formation and massive stars. W40 is in the constellation Aquila the Eagle, visible in the Northern hemisphere's autumn sky. W40 itself is a difficult target for optical astronomers because it lies less than 3 degrees from the central plane of the Milky Way, at a distance of about 1600 light years behind obscuring clouds of interstellar dust and gas.This three image comparison shows W40 in visible, near-infrared and mid-infrared wavelengths. The visible-light image on the left is from the Digitized Sky Survey. The W40 region is not especially prominent at visual wavelengths due to intervening interstellar dust. The near-infrared image in the middle is a composite produced by SOFIA Basic Science Principal Investigators Shuping and Vacca using archived Spitzer infrared space telescope data. The interstellar dust in the foreground and within the W40 region is mostly transparent at these wavelengths, so W40 stands out prominently and one can view into the interior of the nebula to see embedded protostars. Some of these objects were labeled with IRS (\"InfraRed Source\") numbers by earlier investigators. The mid-infrared image on the right is a composite of 5.4 micron (blue), 24.2 micron (green) and 34.8 micron (red) images taken with SOFIA's FORCAST camera in May 2011.The field of view is approximate 3 arcminutes on a side. The bright sources in this image are protostars and thermal emission from dust and gas. Emission at 24 and 35 microns is primarily from warm dust. Some of the protostars can be seen in the Spitzer near-infrared image, but the SOFIA data allow easier determination of their dust temperatures. The hottest object, appearing blue and located at lower left, has very little dust surrounding it and is likely nearest to completing its evolution into a fully-fledged star. The other protostars represented by white in this color balance are cooler and thus have a large amount of circumstellar dust, some of it probably in a disk surrounding the central star. || ",
            "hits": 93
        },
        {
            "id": 30775,
            "url": "https://svs.gsfc.nasa.gov/30775/",
            "result_type": "Hyperwall Visual",
            "release_date": "2006-01-11T00:00:00-05:00",
            "title": "Hubble and Spitzer Composite of the Orion Nebula",
            "description": "Hubble and Spitzer collaborate to show hundreds of baby stars and strong stellar winds shaping the gas and dust of the Orion Nebula || orion_nebula_vis_ir-hst_sst-3240x3240_print.jpg (1024x1024) [228.6 KB] || orion_nebula_vis_ir-hst_sst-3240x3240.png (3240x3240) [10.9 MB] || orion_nebula_vis_ir-hst_sst-6000x6000.png (6000x6000) [41.2 MB] || orion_nebula_vis_ir-hst_sst-3240x3240_searchweb.png (320x180) [107.4 KB] || orion_nebula_vis_ir-hst_sst-3240x3240_thm.png (80x40) [22.7 KB] || hubble-and-spitzer-composite-of-the-orion-nebula.hwshow [346 bytes] || ",
            "hits": 97
        }
    ]
}