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        {
            "id": 14985,
            "url": "https://svs.gsfc.nasa.gov/14985/",
            "result_type": "Produced Video",
            "release_date": "2026-05-13T09:00:00-04:00",
            "title": "TESS Reveals Dazzling Night Sky",
            "description": "This view of the whole sky was constructed from 96 TESS sectors. By the end of September 2025, when the last image of this mosaic was captured, TESS had discovered 679 exoplanets (blue dots) and 5,165 candidates (orange dots). The glowing arc running through the center is the plane of the Milky Way. The Large Magellanic Cloud can be seen along the bottom edge just left of center. Black areas within the oval indicate regions TESS has not yet imaged.Credit: NASA/MIT/TESS and Veselin Kostov (University of Maryland College Park)Alt text: Oval projection of the TESS night sky with exoplanet markersImage description: This oval view of the night sky features a U-shaped band of greyish white running downward from top left to bottom center and then upward to top right. The left side of the U is brighter than the right. Blue and orange dots speckle the image, representing confirmed and candidate exoplanets, respectively. Along the oval’s equator, there are a few black lines and blocks of the sky that are a slightly different shade than the rest of the image. There is an empty black block in the upper left. || TESS_both_bin4_planets-Half.jpg (7740x3900) [11.9 MB] || TESS_both_bin4_planets.jpg (15480x7800) [51.2 MB] || TESS_both_bin4_planets.png (15480x7800) [107.6 MB] || TESS_both_bin4_planets-Half_searchweb.png (320x180) [90.2 KB] || TESS_both_bin4_planets-Half_thm.png (80x40) [5.6 KB] || ",
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        {
            "id": 14979,
            "url": "https://svs.gsfc.nasa.gov/14979/",
            "result_type": "Produced Video",
            "release_date": "2026-03-26T14:00:00-04:00",
            "title": "Early Testing of Aerogel and Silicon Detectors for TIGERISS",
            "description": "Nick Cannady, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, examines a block of silica aerogel in May 2025. Cannady uses the light weight material in detectors for the upcoming TIGERISS (Trans-Iron Galactic Element Recorder for the International Space Station) mission, which is designed to study high-speed charged particles called cosmic rays.Credit: NASA/Scott WiessingerAlt text: A man studies a transparent block of aerogel.Image description: A man with glasses wearing a blue checkered shirt examines a block of transparent material resting on a table. He is leaning and rests his right hand on the table. The block glows faintly blue. The table is gray with evenly spaced rows of holes. || Tigeriss-Aerogel__Nick_Cannady-3.jpg (6393x4718) [17.4 MB] || Tigeriss-AerogelNick_Cannady-3-small.jpg (3196x2359) [1.6 MB] || ",
            "hits": 100
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        {
            "id": 14968,
            "url": "https://svs.gsfc.nasa.gov/14968/",
            "result_type": "Produced Video",
            "release_date": "2026-03-25T12:00:00-04:00",
            "title": "XRISM Clocks Hot Wind of Galaxy M82",
            "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ",
            "hits": 140
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        {
            "id": 14991,
            "url": "https://svs.gsfc.nasa.gov/14991/",
            "result_type": "Produced Video",
            "release_date": "2026-03-20T12:00:00-04:00",
            "title": "Argonne Assembles, Tests Early ComPair-2 Hardware",
            "description": "Tim Cundiff, an engineering specialist at Argonne National Laboratory in Lemont, Illinois, monitors the automated wire bond of a ComPair-2 detector layer in April 2025. Image courtesy of Argonne National LaboratoryAlt text: A man in a lab uses a microscope.Image description: A man in a white clean suit, gloves, safety glasses, and a hairnet sits in front of a piece of machinery in a laboratory and peers into a microscope. Behind him is a long bench covered in scientific equipment and computers. In front of him, inside the machinery, are what look like two black treads that loop in and out of frame. || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9.jpg (2000x1125) [1.1 MB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_searchweb.png (320x180) [124.6 KB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_thm.png (80x40) [27.3 KB] || ",
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        {
            "id": 14980,
            "url": "https://svs.gsfc.nasa.gov/14980/",
            "result_type": "Produced Video",
            "release_date": "2026-02-26T12:00:00-05:00",
            "title": "Prototype ComPair-2 Gamma-Ray Detectors Complete Thermal Vacuum Testing",
            "description": "Prototype gamma-ray detectors for the ComPair-2 mission rests in a thermal vacuum chamber after testing in June 2025 at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The ComPair-2 team tested the detectors’ performance at hot and cold temperatures over the course of a week and the overall survivability of the layer itself. Credit: NASA/Sophia RobertsAlt text: A piece of equipment sits inside a chamber in a lab. Image description: A cylindrical metal chamber at the center of the image has its door swung all the way open. Inside are silver-wrapped ComPair-2 detectors attached to many copper-colored wires. The chamber is in a lab with white walls and has tubes, wires, and other pieces of equipment attached. || ComPair2_TVAC-1-small.jpg (4096x2732) [3.2 MB] || ComPair2_TVAC-1.jpg (8192x5464) [30.6 MB] || ",
            "hits": 93
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        {
            "id": 14955,
            "url": "https://svs.gsfc.nasa.gov/14955/",
            "result_type": "Produced Video",
            "release_date": "2026-01-27T09:00:00-05:00",
            "title": "NASA Tests LISA Development Units",
            "description": "A prototype charge management device for the future LISA (Laser Interferometer Space Antenna) mission sits on a lab bench at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The device will reduce the buildup of electric charge on the gold-platinum test masses that float freely inside each of the three LISA spacecraft. The University of Florida in Gainesville and Fibertek Inc. in McNair, Virginia, are developing the device. Credit: NASA/Dennis HenryAlt text: An instrument rests on a lab bench.Image description: A silver box with red and black connector caps on one side rests on a white lab bench with a blue mat on top. Three black cables connect to the box and another yellow cable curls around it. || GSFC_20250602_LISA_006584.jpg (8098x5399) [11.3 MB] || ",
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            "id": 14945,
            "url": "https://svs.gsfc.nasa.gov/14945/",
            "result_type": "Produced Video",
            "release_date": "2026-01-09T09:00:00-05:00",
            "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars",
            "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ",
            "hits": 258
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        {
            "id": 14935,
            "url": "https://svs.gsfc.nasa.gov/14935/",
            "result_type": "Infographic",
            "release_date": "2025-12-18T13:00:00-05:00",
            "title": "Milky Way Anatomy",
            "description": "This infographic with artist’s concept views of our Milky Way galaxy highlights its main components: the disk, bulge, stellar halo, and dark matter halo. Scientists have a pretty good idea of the Milky Way’s overall structure, but since we’re nestled inside it, fine details are hard to see. Astronomers have used observations from different telescopes to piece together our galaxy's anatomy, and future observatories like NASA's Nancy Grace Roman Space Telescope will make the picture even clearer. || Milky_Way_Anatomy_Infographic_Simple_Final_print.jpg (1024x512) [118.4 KB] || Milky_Way_Anatomy_Infographic_Simple_Final.jpg (4320x2160) [1.2 MB] || Milky_Way_Anatomy_Infographic_Simple_Final.png (4320x2160) [6.5 MB] || Milky_Way_Anatomy_Infographic_Simple_Final_searchweb.png (320x180) [68.0 KB] || Milky_Way_Anatomy_Infographic_Simple_Final_thm.png (80x40) [5.1 KB] || ",
            "hits": 1860
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            "id": 14930,
            "url": "https://svs.gsfc.nasa.gov/14930/",
            "result_type": "Infographic",
            "release_date": "2025-12-18T10:00:00-05:00",
            "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles",
            "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel",
            "hits": 204
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        {
            "id": 14917,
            "url": "https://svs.gsfc.nasa.gov/14917/",
            "result_type": "Infographic",
            "release_date": "2025-12-12T10:00:00-05:00",
            "title": "Roman Galactic Plane Survey",
            "description": "No description available.",
            "hits": 195
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        {
            "id": 14916,
            "url": "https://svs.gsfc.nasa.gov/14916/",
            "result_type": "Produced Video",
            "release_date": "2025-12-08T09:30:00-05:00",
            "title": "Black Hole Eats Star: The Longest GRB Ever Seen",
            "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ",
            "hits": 531
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        {
            "id": 14933,
            "url": "https://svs.gsfc.nasa.gov/14933/",
            "result_type": "Produced Video",
            "release_date": "2025-12-04T09:00:00-05:00",
            "title": "XRISM Finds Elemental Bounty in Supernova Remnant",
            "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ",
            "hits": 202
        },
        {
            "id": 14931,
            "url": "https://svs.gsfc.nasa.gov/14931/",
            "result_type": "Infographic",
            "release_date": "2025-12-04T00:00:00-05:00",
            "title": "Roman By The Numbers Infographic",
            "description": "NASA's Nancy Grace Roman Space Telescope will survey vast swaths of sky during its five-year primary mission. During that time, scientists expect it to see an incredible number of new object, including stars, galaxies, black holes and planets outside our solar system, known as exoplanets. This infographic previews some of the discoveries scientists anticipate from Roman's data deluge. || Roman_ByTheNumbers_Infographic_half.jpg (2000x1125) [498.6 KB] || Roman_ByTheNumbers_Infographic_print.jpg (1024x576) [223.6 KB] || Roman_ByTheNumbers_Infographic.png (4000x2250) [2.0 MB] || Roman_ByTheNumbers_Infographic.jpg (4000x2250) [1.0 MB] || Roman_ByTheNumbers_Infographic_searchweb.png (320x180) [75.1 KB] || Roman_ByTheNumbers_Infographic_thm.png (80x40) [7.1 KB] || ",
            "hits": 168
        },
        {
            "id": 14928,
            "url": "https://svs.gsfc.nasa.gov/14928/",
            "result_type": "Produced Video",
            "release_date": "2025-11-20T10:00:00-05:00",
            "title": "TESS Triples Size of Pleiades Star Cluster",
            "description": "These young, hot blue stars are members of the Pleiades open star cluster and reside about 430 light-years away in the northern constellation Taurus. The brightest stars are visible to the unaided eye during evenings from October to April. A new study finds the cluster to be triple the size previously thought — and shows that its stars are scattered across the night sky. The Schmidt telescope at the Palomar Observatory in California captured this color-composite image. Credit: NASA, ESA, and AURA/CaltechAlt text: Members of the Pleiades shine in blue. Image description: The Pleiades are shown in this image. Six of the stars, all blue-white, are larger than the others and have diffraction spikes and faint blue circles around them. Other, smaller blue stars are also scattered across the image. Patches of swirling blue dust surround some of the stars. || STScI-01EVVEYWX1TA3MGBK5F6EFQVGQ.jpg (4877x3513) [1.1 MB] || ",
            "hits": 544
        },
        {
            "id": 14866,
            "url": "https://svs.gsfc.nasa.gov/14866/",
            "result_type": "Produced Video",
            "release_date": "2025-07-15T00:00:00-04:00",
            "title": "Cosmic Desktop & Phone Wallpapers",
            "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||",
            "hits": 11811
        },
        {
            "id": 14856,
            "url": "https://svs.gsfc.nasa.gov/14856/",
            "result_type": "Infographic",
            "release_date": "2025-06-20T10:00:00-04:00",
            "title": "Roman Space Telescope to Scale with Tyrannosaurus rex",
            "description": "A comparison of the Nancy Grace Roman Space Telescope with a Tyrannosaurus rex. They have the same approximate length and weight.",
            "hits": 52
        },
        {
            "id": 14799,
            "url": "https://svs.gsfc.nasa.gov/14799/",
            "result_type": "Produced Video",
            "release_date": "2025-05-27T20:54:00-04:00",
            "title": "Astrophysics: Observing the Universe Vertical Video",
            "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.",
            "hits": 404
        },
        {
            "id": 14836,
            "url": "https://svs.gsfc.nasa.gov/14836/",
            "result_type": "Infographic",
            "release_date": "2025-05-07T00:00:00-04:00",
            "title": "Roman Systems Infographic",
            "description": "This infographic shows the two major subsystems that make up NASA’s Nancy Grace Roman Space Telescope. The subsystems are each undergoing testing prior to being joined together this fall. || Roman_Systems_Infographic_V1_Final_print.jpg (1024x576) [160.5 KB] || Roman_Systems_Infographic_V1_Final_16bit.png (3840x2160) [30.7 MB] || Roman_Systems_Infographic_V1_Final_8bit.png (3840x2160) [8.2 MB] || Roman_Systems_Infographic_V1_Final.jpg (3840x2160) [1.2 MB] || Roman_Systems_Infographic_V1_Final_searchweb.png (320x180) [88.8 KB] || Roman_Systems_Infographic_V1_Final_thm.png [6.4 KB] || ",
            "hits": 142
        },
        {
            "id": 14820,
            "url": "https://svs.gsfc.nasa.gov/14820/",
            "result_type": "Infographic",
            "release_date": "2025-04-24T12:00:00-04:00",
            "title": "Roman's Core Surveys Infographics",
            "description": "NASA’s Nancy Grace Roman Space Telescope’s three main observing programs, highlighted in this infographic, will enable astronomers to view the universe as never before, revealing billions of cosmic objects strewn across enormous swaths of space-time.Credit: NASA’s Goddard Space Flight Center || Roman_CoreSurveys_Infographic_print.jpg (1024x640) [155.3 KB] || Roman_CoreSurveys_Infographic.png (8000x5000) [28.6 MB] || Roman_CoreSurveys_Infographic.jpg (8000x5000) [2.5 MB] || Roman_CoreSurveys_Infographic_Half.jpg (4000x2500) [1.3 MB] || Roman_CoreSurveys_Infographic_searchweb.png (320x180) [72.9 KB] || Roman_CoreSurveys_Infographic_thm.png [6.6 KB] || ",
            "hits": 263
        },
        {
            "id": 14809,
            "url": "https://svs.gsfc.nasa.gov/14809/",
            "result_type": "Produced Video",
            "release_date": "2025-03-24T00:00:00-04:00",
            "title": "Testing AstroPix, A New Gamma-Ray Detector",
            "description": "An AstroPix detector board rests inside a protective tray in a lab at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The squares in the center are silicon pixel gamma-ray sensors. There are two more under the rectangular copper bus bar, which carries data from the sensors to rest of the A-STEP system. The detector connects to a high-power voltage board and other electronics. Credit: NASA/Sophia RobertsAlt text: Electronic components rest on a lab tableImage description: What looks like a large computer chip — an AstroPix detector — rests inside a white tray on a blue lab bench. The detector is green and has two reflective squares in the middle with a long copper rectangle at right parallel to them. Black wires attached to the bottom of the chip connect it to other pieces of equipment and circuit boards on the lab bench. || ASTEP_Chips3.jpg (8192x5464) [32.7 MB] || ASTEP_Chips3_half.jpg (4096x2732) [3.1 MB] || ASTEP_Chips3_half_searchweb.png (320x180) [109.8 KB] || ASTEP_Chips3_half_thm.png [11.5 KB] || ",
            "hits": 28
        },
        {
            "id": 14780,
            "url": "https://svs.gsfc.nasa.gov/14780/",
            "result_type": "Produced Video",
            "release_date": "2025-02-10T10:00:00-05:00",
            "title": "NASA Scientists Spot Candidate for Speediest Exoplanet System",
            "description": "This artist's concept visualizes stars near the center of our Milky Way galaxy. Each has a trail indicating its speed –– the longer the trail, the faster it's moving. NASA scientists recently discovered a candidate for a particularly speedy star, visualized near the center of this image, with an orbiting planet. If confirmed, the pair sets a record for fastest known exoplanet system.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC) || StarTrails-sm.jpg (1200x675) [337.2 KB] || StarTrails.jpg (4800x2700) [1.9 MB] || star-trails-final-ac.jpg (4800x2700) [4.1 MB] || StarTrails_searchweb.png (320x180) [95.4 KB] || StarTrails.tif (4800x2700) [13.7 MB] || StarTrails_thm.png [11.2 KB] || ",
            "hits": 91
        },
        {
            "id": 14775,
            "url": "https://svs.gsfc.nasa.gov/14775/",
            "result_type": "Produced Video",
            "release_date": "2025-01-29T10:00:00-05:00",
            "title": "Roman Instrument Posters",
            "description": "NASA’s Roman Coronagraph Instrument will greatly advance our ability to directly image exoplanets, or planets and disks around other stars.Credit: NASA/JPLDigital version of poster with back panelPress version of poster with back panel. FOR PRINT || CGI_Digital_12x18.jpg (1837x2737) [1.1 MB] || CGI_Digital_12x18-1.jpg (3663x5475) [5.7 MB] || CGI_Digital_12x18-1.png (3663x5475) [39.5 MB] || ",
            "hits": 25
        },
        {
            "id": 14680,
            "url": "https://svs.gsfc.nasa.gov/14680/",
            "result_type": "Produced Video",
            "release_date": "2025-01-09T00:00:00-05:00",
            "title": "Astronauts Prepare for NICER Repair Training",
            "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague participated in a training exercise at the NBL (Neutral Buoyancy Laboratory) at NASA’s Johnson Space Center in Houston. They were rehearsing activities related to repairing NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.Before any spacewalk, astronauts practice and refine procedures in the NBL to simulate — as closely as possible on Earth — the conditions under which they’ll complete the task in space.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s X-ray measurements during orbital daytime.The NICER team developed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ",
            "hits": 83
        },
        {
            "id": 14678,
            "url": "https://svs.gsfc.nasa.gov/14678/",
            "result_type": "Produced Video",
            "release_date": "2025-01-07T00:00:00-05:00",
            "title": "Astronauts Practice NICER Repair",
            "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague practiced a repair for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station. The training exercise took place in the (NBL) Neutral Buoyancy Laboratory at NASA’s Johnson Space Center in Houston.Before any spacewalk, astronauts rehearse activities in the NBL to simulate — as much as possible — the conditions under which they’ll complete the task in space.In May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the instrument. The damage allows sunlight to reach the detectors during the station’s daytime, saturating sensors and interfering with NICER’s X-ray measurements. The damage does not impact nighttime observations.The NICER team developed a plan to cover the largest areas of damage using five patches, each shaped like a piece of pie, to be inserted into the instrument’s sunshades and locked in place. || ",
            "hits": 86
        },
        {
            "id": 14679,
            "url": "https://svs.gsfc.nasa.gov/14679/",
            "result_type": "Produced Video",
            "release_date": "2024-12-13T00:00:00-05:00",
            "title": "NICER Caddy Preparation",
            "description": "In Spring 2024, scientists and engineers at NASA prepared and packed a patch kit for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s measurements during orbital daytime.The NICER team designed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ",
            "hits": 61
        },
        {
            "id": 14707,
            "url": "https://svs.gsfc.nasa.gov/14707/",
            "result_type": "Produced Video",
            "release_date": "2024-11-25T11:00:00-05:00",
            "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3",
            "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ",
            "hits": 206
        },
        {
            "id": 14650,
            "url": "https://svs.gsfc.nasa.gov/14650/",
            "result_type": "Produced Video",
            "release_date": "2024-11-25T00:00:00-05:00",
            "title": "EXCITE 2024: Infrared Detector and Spectrometer",
            "description": "EXCITE (EXoplanet Climate Infrared TElescope) is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during long-duration scientific balloon trips over Antarctica.These images, taken in July 2024, show Peter Nagler and Nat DeNigris preparing EXCITE’s infrared detector and installing it into the mission’s spectrometer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. At the time, the EXCITE team was gearing up for a test flight in Fort Sumner, New Mexico. || ",
            "hits": 38
        },
        {
            "id": 14725,
            "url": "https://svs.gsfc.nasa.gov/14725/",
            "result_type": "Produced Video",
            "release_date": "2024-11-25T00:00:00-05:00",
            "title": "EXCITE 2024: Payload Prep",
            "description": "In August 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both Arctic and Antarctic, with the latter offering longer duration flights optimum for observing planets for their entire orbit. || ",
            "hits": 33
        },
        {
            "id": 14726,
            "url": "https://svs.gsfc.nasa.gov/14726/",
            "result_type": "Produced Video",
            "release_date": "2024-11-25T00:00:00-05:00",
            "title": "EXCITE 2024: Launch and Recovery",
            "description": "On August 31, 2024, the EXCITE (EXoplanet Climate Infrared TElescope) team conducted a test flight of their telescope from NASA’s Columbia Scientific Balloon Facility in Fort Sumner, New Mexico.EXCITE's goal is to study atmospheres around hot Jupiters, gas giant exoplanets that complete an orbit once every one to two days and have temperatures in the thousands of degrees.The telescope is designed fly to about 132,000 feet (40 kilometers) via a scientific balloon filled with helium. That takes it above 99.5% of Earth’s atmosphere. At that altitude, it can observe multiple infrared wavelengths with little interference. In the future, EXCITE could take observations over both the north and south poles, although flights over Antarctica allow for longer-duration flights at a latitude optimum for observing planets for their entire orbit. || ",
            "hits": 50
        },
        {
            "id": 14720,
            "url": "https://svs.gsfc.nasa.gov/14720/",
            "result_type": "Produced Video",
            "release_date": "2024-11-22T10:00:00-05:00",
            "title": "COBE All-Sky Map 360 Video With Narration",
            "description": "View the entire sky with the microwave eyes of NASA’s COBE (Cosmic Background Explorer) satellite in this immersive video. COBE took the first baby picture of the universe, revealing slight temperature variations when the cosmos was just 380,000 years old. This image shows the entire sky using four years of observations by COBE’s Differential Microwave Radiometer. The central plane of our galaxy runs across the middle, and its center is marked by a white X. Red indicates hotter regions, blue colder. The fluctuations are extremely faint, varying by only 1 part in 100,000 from the average temperature. They represent density variations in the early universe thought to have given rise to the structures we see today. After stripping away foreground emission arising from dust, hot gas, and charged particles interacting with magnetic fields in our galaxy, COBE data revealed tiny variations in the temperature of the cosmic microwave background — the oldest light in the universe — for the first time.(This video is formatted for 360-degree use.)Credit: NASA's Goddard Space Flight CenterMusic: “Meetings in Underwater Ruins,” Philippe Andre Vandenhende [SACEM], Olivier Louis Perrot [SACEM] and Idriss-El-Mehdi Bennani [SACEM], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Design_hybrid_COBE_360.jpg (1280x720) [235.1 KB] || YTframe_Design_hybrid_COBE_360_searchweb.png (320x180) [80.8 KB] || YTframe_Design_hybrid_COBE_360_thm.png (80x40) [9.2 KB] || 14720_COBE_360_Captions.en_US.srt [4.7 KB] || 14720_COBE_360_Captions.en_US.vtt [4.4 KB] || 14720_COBE_360_Narrated_Good.mp4 (8192x4096) [131.8 MB] || 14720_COBE_360_Narrated_Best.mp4 (8192x4096) [503.2 MB] || ",
            "hits": 1119
        },
        {
            "id": 11738,
            "url": "https://svs.gsfc.nasa.gov/11738/",
            "result_type": "Infographic",
            "release_date": "2024-11-20T00:00:00-05:00",
            "title": "Infographic: NASA's Neil Gehrels Swift Observatory",
            "description": "This infographic summarizes key aspects of NASA's Swift mission, from its instruments to scientific results gleaned from 20 years of operations. Swift is still going strong, and the observatory remains a key part of NASA’s strategy to monitor the changing sky with multiple telescopes using different approaches for studying the cosmos.Credit: NASA's Goddard Space Flight CenterClick the download button to select from a range of sizes. || Swift_20_Infographic_Quarter.jpg (1550x1991) [1.2 MB] || Swfit_20_Poster_CMYK.jpg (6200x7965) [19.2 MB] || Swift_20_Infographic_Full.jpg (6200x7965) [7.4 MB] || Swift_20_Infographic_Full.png (6200x7965) [34.2 MB] || Swift_20_Infographic_Half.jpg (3100x3983) [3.2 MB] || Swift_20_Infographic_Half.png (3100x3983) [10.5 MB] || Swift_20_Infographic_Full.jpg.dzi [178 bytes] || Swift_20_Infographic_Full.jpg_files [4.0 KB] || ",
            "hits": 97
        },
        {
            "id": 20394,
            "url": "https://svs.gsfc.nasa.gov/20394/",
            "result_type": "Animation",
            "release_date": "2024-11-12T15:00:00-05:00",
            "title": "Habitable Worlds Observatory (HWO) Animations and Stills",
            "description": "This page contains artist's concept computer renderings of a current possible design for the Habitable Worlds Observatory. HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ",
            "hits": 170
        },
        {
            "id": 20395,
            "url": "https://svs.gsfc.nasa.gov/20395/",
            "result_type": "Animation",
            "release_date": "2024-11-12T15:00:00-05:00",
            "title": "Habitable Worlds Observatory Additional Spacecraft Designs",
            "description": "The Habitable Worlds Observatory is early in its development.  Many designs are under consideration.  These artist's concept animations show some of the options.HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ",
            "hits": 248
        },
        {
            "id": 14698,
            "url": "https://svs.gsfc.nasa.gov/14698/",
            "result_type": "Produced Video",
            "release_date": "2024-10-22T11:00:00-04:00",
            "title": "NASA Reveals LISA Engineering Development Unit Telescope",
            "description": "NASA has revealed the first look at a full-scale prototype for six telescopes that will enable, in the next decade, the space-based detection of gravitational waves — ripples in space-time caused by merging black holes and other cosmic sources.The LISA (Laser Interferometer Space Antenna) mission is led by ESA (European Space Agency) in partnership with NASA to detect gravitational waves by using lasers to measure precise distances — down to picometers, or trillionths of a meter — between a trio of spacecraft distributed in a vast configuration larger than the Sun. Each side of the triangular array will measure nearly 1.6 million miles, or 2.5 million kilometers.Twin telescopes aboard each spacecraft will both transmit and receive infrared laser beams to track their companions, and NASA is supplying all six of them to the LISA mission. The prototype, called the Engineering Development Unit Telescope, will provide guidance as engineers and scientists work toward building the flight hardware.In May, the prototype, which was manufactured and assembled by L3Harris Technologies in Rochester, New York, arrived at NASA's Goddard Space Flight Center in Greenbelt, Maryland. The primary mirror is coated in gold to better reflect the infrared lasers and to reduce heat loss from a surface exposed to cold space since the telescope will operate best when close to room temperature. The prototype is made entirely from an amber-colored glass-ceramic called Zerodur, manufactured by Schott in Mainz, Germany. The material is widely used for telescope mirrors and other applications requiring high precision because its shape changes very little over a wide range of temperatures. || ",
            "hits": 75
        },
        {
            "id": 14705,
            "url": "https://svs.gsfc.nasa.gov/14705/",
            "result_type": "Produced Video",
            "release_date": "2024-10-21T14:00:00-04:00",
            "title": "A-STEP’s AstroPix Detectors Get Ready for Flight",
            "description": "Scientists and engineers at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, have been preparing a new gamma-ray detector called AstroPix for an upcoming rocket payload called A-STEP (AstroPix Sounding Rocket Technology dEmonstration Payload).Each detector contains four silicon sensors, and each sensor incorporates 1,225 pixels. A-STEP will carry a three-detector stack to the edge of space on the SubTEC-10 sounding rocket, which will launch in 2025 from NASA’s Wallops Flight Facility in Virginia. The flight’s primary goal is to successfully operate the detectors, with a secondary goal of measuring the rate of impacts from cosmic rays, high-energy particles from space. || ",
            "hits": 62
        },
        {
            "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": 89
        },
        {
            "id": 14604,
            "url": "https://svs.gsfc.nasa.gov/14604/",
            "result_type": "Produced Video",
            "release_date": "2024-06-12T10:00:00-04:00",
            "title": "NASA’s Roman Mission Gets Cosmic ‘Sneak Peek’ From Supercomputers",
            "description": "This graphic highlights part of a new simulation of what NASA’s Nancy Grace Roman Space Telescope could see when it launches by May 2027. The background spans about 0.11 square degrees (roughly equivalent to half of the area of sky covered by a full Moon), representing less than half the area Roman will see in a single snapshot. The inset zooms in to a region 300 times smaller, showcasing a swath of brilliant synthetic galaxies at Roman’s full resolution. Having such a realistic simulation helps scientists study the physics behind cosmic images –– both synthetic ones like these and future real ones. Researchers will use the observations for many types of science, including testing our understanding of the origin, evolution, and ultimate fate of the universe.Credit: C. Hirata and K. Cao (OSU) and NASA’s Goddard Space Flight Center || Roman_Simulation_Popout_2k_deg.jpg (2048x2048) [979.2 KB] || ",
            "hits": 57
        },
        {
            "id": 14524,
            "url": "https://svs.gsfc.nasa.gov/14524/",
            "result_type": "Infographic",
            "release_date": "2024-05-07T10:00:00-04:00",
            "title": "Primordial Black Holes",
            "description": "This artist's concept takes a fanciful approach to imagining small primordial black holes. In reality, such tiny black holes would have a difficult time forming the accretion disks that make them visible here.Credit: NASA's Goddard Space Flight Center || Primordial_Black_Hole_Still_1080.jpg (1920x1080) [275.1 KB] || Primordial_Black_Hole_Still_4k_print.jpg (1024x576) [51.1 KB] || Primordial_Black_Hole_Still_4k.jpg (3840x2160) [2.5 MB] || Primordial_Black_Hole_Still_4k.png (3840x2160) [7.3 MB] || Primordial_Black_Hole_Still_4k_searchweb.png (320x180) [61.5 KB] || Primordial_Black_Hole_Still_4k_thm.png (80x40) [5.6 KB] || ",
            "hits": 1239
        },
        {
            "id": 14574,
            "url": "https://svs.gsfc.nasa.gov/14574/",
            "result_type": "Produced Video",
            "release_date": "2024-05-06T10:00:00-04:00",
            "title": "Black Hole Week 2024 Poster and Media",
            "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.",
            "hits": 208
        },
        {
            "id": 14476,
            "url": "https://svs.gsfc.nasa.gov/14476/",
            "result_type": "Produced Video",
            "release_date": "2024-01-11T11:10:00-05:00",
            "title": "Fermi Mission Detects Surprising Gamma-Ray Feature Beyond Our Galaxy",
            "description": "This artist’s concept shows the entire sky in gamma rays with magenta circles illustrating the uncertainty in the direction from which more high-energy gamma rays than average seem to be arriving. In this view, the plane of our galaxy runs across the middle of the map. The circles enclose regions with a 68% (inner) and a 95% chance of containing the origin of these gamma rays. Credit: NASA’s Goddard Space Flight Center || Dark_Fermi_Dipole.jpg (3840x2160) [506.2 KB] || Dark_Fermi_Dipole.png (3840x2160) [8.9 MB] || Dark_Fermi_Dipole_searchweb.png (320x180) [57.6 KB] || Dark_Fermi_Dipole_thm.png (80x40) [5.4 KB] || ",
            "hits": 171
        },
        {
            "id": 14492,
            "url": "https://svs.gsfc.nasa.gov/14492/",
            "result_type": "Produced Video",
            "release_date": "2024-01-05T08:50:00-05:00",
            "title": "XRISM Reveals Its First Look at X-ray Cosmos",
            "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ",
            "hits": 69
        },
        {
            "id": 14487,
            "url": "https://svs.gsfc.nasa.gov/14487/",
            "result_type": "Produced Video",
            "release_date": "2023-12-18T13:00:00-05:00",
            "title": "BurstCube Completes Magnetic Calibration",
            "description": "BurstCube is a mission developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. It is expected to launch in March 2024. This CubeSat will detect short gamma-ray bursts, brief flashes of the highest-energy form of light. Dense stellar remnants called neutron stars create these bursts when they collide with other neutron stars or black holes. Short gamma-ray bursts, which last less than 2 seconds, are important sources for gravitational wave discoveries and multimessenger astronomy. BurstCube will use Earth’s magnetic field to orientate itself as it scans the sky. To do so, the mission team had to map the spacecraft’s own magnetic field using a special facility at NASA’s Wallops Flight Facility in Virginia. The magnetic calibration chamber generates a known magnetic field that cancels out Earth’s. The team's measurements of BurstCube’s field in the chamber will help figure out where the satellite is pointing once in space, so scientists can locate gamma-ray bursts and tell other observatories where to look. || ",
            "hits": 49
        },
        {
            "id": 14460,
            "url": "https://svs.gsfc.nasa.gov/14460/",
            "result_type": "Produced Video",
            "release_date": "2023-11-16T11:00:00-05:00",
            "title": "Roman Wide Field Instrument Fully Integrated at Ball Aerospace",
            "description": "Animated GIF showing the actual Wide Field Instrument wrapped in protective material and transitioning to a computer rendering of the instrument showing some of the interior detail. The focal plane assembly, which contains Roman's 18 detectors, is highlighted.Credit: NASA's Goddard Space Flight Center/Ball Aerospace || WFI_X-ray_V2.gif (547x800) [4.0 MB] || ",
            "hits": 48
        },
        {
            "id": 14461,
            "url": "https://svs.gsfc.nasa.gov/14461/",
            "result_type": "Produced Video",
            "release_date": "2023-11-16T11:00:00-05:00",
            "title": "Roman Primary Mirror Completed at L3Harris",
            "description": "Short animated GIF transitioning from a photograph of the Nancy Grace Roman Space Telescope primary mirror in a clean room to a computer model of the spacecraft showing how the mirror is positioned within the spacecraft.Credit: NASA's Goddard Space Flight Center/L3 Harris || Mirror_overlay_.gif (800x450) [2.7 MB] || ",
            "hits": 53
        },
        {
            "id": 14437,
            "url": "https://svs.gsfc.nasa.gov/14437/",
            "result_type": "Produced Video",
            "release_date": "2023-10-24T00:00:00-04:00",
            "title": "Nancy Grace Roman Space Telescope Partner Maps",
            "description": "This world map of Nancy Grace Roman Space Telescope partner institutes shows the international effort to realize this mission.  Dish icons represent ground stations that will send and recieve data to the spacecraft once it is on orbit.Credit: NASA's Goddard Space Flight CenterThe Australia inset of this map was originally created by Lokal_Profil and sourced from Wikimedia Commons. || Roman_World_Partner_Map_Aug24_10k.jpg (10000x5000) [6.2 MB] || Roman_World_Partner_Map_Aug24_10k.png (10000x5000) [12.6 MB] || Roman_World_Partner_Map_Aug24_5k.jpg (5000x2500) [2.4 MB] || Roman_World_Partner_Map_Aug24_5k.png (5000x2500) [6.0 MB] || Roman_World_Partner_Map_Aug24_5k_print.jpg (1024x512) [196.1 KB] || Roman_World_Partner_Map_Aug24_5k_searchweb.png (320x180) [79.6 KB] || Roman_World_Partner_Map_Aug24_5k_thm.png (80x40) [5.7 KB] || Roman_World_Partner_Map_Aug24_10k.png.dzi [179 bytes] || Roman_World_Partner_Map_Aug24_10k.png_files [4.0 KB] || ",
            "hits": 98
        },
        {
            "id": 14436,
            "url": "https://svs.gsfc.nasa.gov/14436/",
            "result_type": "Produced Video",
            "release_date": "2023-10-18T11:00:00-04:00",
            "title": "Traveler and Friends Halloween Pumpkin Stencils",
            "description": "Get ready to take off on a Halloween adventure with these pumpkin stencils featuring our fearless Traveler and their stellar friends!Not familiar with the Traveler?  Watch all their adventures on NASA+. || ",
            "hits": 31
        },
        {
            "id": 14422,
            "url": "https://svs.gsfc.nasa.gov/14422/",
            "result_type": "Produced Video",
            "release_date": "2023-10-06T00:00:00-04:00",
            "title": "Roman's Instrument Carrier Arrives",
            "description": "The Nancy Grace Roman Space Telescope's Instrument Carrier arrives at NASA's Goddard Space Flight Center.  The workers remove the grid-like structure from the truck container that brought it and move it into a clean tent.  Once there, engineers remove the protective wrapping and inspect the carbon fiber struts.  The Instrument Carrier sits between the primary mirror and spacecraft bus and will hold Roman's  Wide Field Instrument and Coronagraph technology demonstration.Music: \"Knowledge and Process\" from Universal Production MusicComplete transcript available. || Roman_Instrument_Carrier.jpg (1849x1004) [426.6 KB] || Roman_Instrument_Carrier_searchweb.png (320x180) [105.1 KB] || Roman_Instrument_Carrier_thm.png (80x40) [10.6 KB] || Roman_Instrument_Carrier_Arrival_Good.webm (1920x1080) [13.2 MB] || Roman_Instrument_Carrier_Arrival_Good.mp4 (1920x1080) [105.1 MB] || Roman_Instrument_Carrier_Arrival_Best.mp4 (1920x1080) [257.6 MB] || Roman_Instrument_Carrier_Arrival_Captions.en_US.srt [894 bytes] || Roman_Instrument_Carrier_Arrival_Captions.en_US.vtt [907 bytes] || Roman_Instrument_Carrier_Arrival_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ",
            "hits": 30
        },
        {
            "id": 14402,
            "url": "https://svs.gsfc.nasa.gov/14402/",
            "result_type": "Produced Video",
            "release_date": "2023-09-20T13:00:00-04:00",
            "title": "Simulated Gravitational Wave All-Sky Image",
            "description": "Watch as gravitational waves from a simulated population of compact binary systems combine into a synthetic map of the entire sky. Such systems contain white dwarfs, neutron stars, or black holes in tight orbits. Maps like this using real data will be possible once space-based gravitational wave observatories become active in the next decade. The center of our Milky Way galaxy lies at the center of this all-sky view, with the galactic plane extending across the middle. Brighter spots indicate sources with stronger signals and lighter colors indicate those with higher frequencies. Larger colored patches show sources whose positions are less well known. The inset shows the frequency and strength of the gravitational signal, as well as the sensitivity limit for LISA (Laser Interferometer Space Antenna), an  observatory now being designed by ESA (European Space Agency) in collaboration with NASA for launch in the 2030s.Credit: NASA’s Goddard Space Flight CenterMusic: \"Shadowless\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || LISA_AllSky_withInset_Still.jpg (2985x1497) [795.1 KB] || LISA_AllSky_1080.mp4 (1920x1080) [22.8 MB] || LISA_AllSky_1080.webm (1920x1080) [2.5 MB] || LISA_AllSky_4k.mp4 (3840x2160) [60.4 MB] || LISA_AllSky_SRT_Captions.en_US.srt [205 bytes] || LISA_AllSky_SRT_Captions.en_US.vtt [218 bytes] || LISA_AllSky_ProRes_3840x2160_30.mov (3840x2160) [992.4 MB] || ",
            "hits": 78
        },
        {
            "id": 14373,
            "url": "https://svs.gsfc.nasa.gov/14373/",
            "result_type": "Infographic",
            "release_date": "2023-08-08T10:00:00-04:00",
            "title": "ComPair Infographic",
            "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ",
            "hits": 53
        },
        {
            "id": 14374,
            "url": "https://svs.gsfc.nasa.gov/14374/",
            "result_type": "Infographic",
            "release_date": "2023-08-03T11:00:00-04:00",
            "title": "A Guide to Cosmic Temperatures",
            "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ",
            "hits": 953
        },
        {
            "id": 14389,
            "url": "https://svs.gsfc.nasa.gov/14389/",
            "result_type": "Produced Video",
            "release_date": "2023-08-01T13:00:00-04:00",
            "title": "XRISM Additional Images",
            "description": "The XRISM spacecraft during acoustic testing at JAXA's Tsukuba Space Center in December 2022. These and other tests confirm that the spacecraft can withstand the severe vibrations and sounds of its rocket launch.Credit: JAXA || XRISM_Acoustic_12_23_22.jpg (2832x4240) [6.9 MB] || ",
            "hits": 24
        },
        {
            "id": 14372,
            "url": "https://svs.gsfc.nasa.gov/14372/",
            "result_type": "B-Roll",
            "release_date": "2023-07-20T10:00:00-04:00",
            "title": "ComPair Thermal Vacuum Photos",
            "description": "Team members work on the ComPair balloon instrument before it begins testing in a thermal vacuum chamber at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. ComPair project manager Regina Caputo (front right), graduate student Nicholas Kirschner (George Washington University, left), and research scientist Nicholas Cannady (University of Maryland Baltimore County, rear) examine ComPair's various components to determine what needs to be “harnessed,” or connected via cable to power systems and the onboard computer.Credit: NASA/Scott Wiessinger || ComPair_TVac_IMG_2141.png (5319x3546) [30.9 MB] || ComPair_TVac_IMG_2141.jpg (5319x3546) [6.0 MB] || ComPair_TVac_IMG_2141_half.jpg (2659x1773) [1.4 MB] || ",
            "hits": 34
        },
        {
            "id": 14380,
            "url": "https://svs.gsfc.nasa.gov/14380/",
            "result_type": "Produced Video",
            "release_date": "2023-07-19T00:00:00-04:00",
            "title": "Icy Earth-mass Rogue Planet",
            "description": "This artist’s concept shows an ice-encrusted, Earth-mass rogue planet drifting through space alone.Credit: NASA’s Goddard Space Flight Center || Icy_Rogue_Planet_Final.jpg (1920x1080) [518.5 KB] || Icy_Rogue_Planet_Final_searchweb.png (320x180) [78.5 KB] || Icy_Rogue_Planet_Final_thm.png (80x40) [5.1 KB] || ",
            "hits": 238
        },
        {
            "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": 63
        },
        {
            "id": 14282,
            "url": "https://svs.gsfc.nasa.gov/14282/",
            "result_type": "Produced Video",
            "release_date": "2023-05-17T11:00:00-04:00",
            "title": "Spitzer, TESS Find Potential Earth-Size World Covered in Volcanoes",
            "description": "LP 791-18 d, illustrated here in an artist's concept, is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system. Astronomers discovered and studied the planet using data from NASA’s Spitzer Space Telescope and TESS (Transiting Exoplanet Survey Satellite) along with many other observatories.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || LP79118d_BeautyShot.jpg (2048x1152) [130.9 KB] || LP79118d_Temperate_Earth_BeautyShot_Full.jpg (5760x3240) [2.2 MB] || LP79118d_Temperate_Earth_BeautyShot_Full.png (5760x3240) [12.4 MB] || LP79118d_BeautyShot_searchweb.png (320x180) [59.9 KB] || LP79118d_BeautyShot_thm.png (80x40) [5.1 KB] || ",
            "hits": 92
        },
        {
            "id": 14317,
            "url": "https://svs.gsfc.nasa.gov/14317/",
            "result_type": "Produced Video",
            "release_date": "2023-03-28T13:50:00-04:00",
            "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst",
            "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ",
            "hits": 159
        },
        {
            "id": 14301,
            "url": "https://svs.gsfc.nasa.gov/14301/",
            "result_type": "Produced Video",
            "release_date": "2023-03-08T10:00:00-05:00",
            "title": "Millions of Galaxies Emerge in New Simulated Images From NASA's Roman",
            "description": "This video begins by showing the most distant galaxies in the simulated deep field image in red. As it zooms out, layers of nearer (yellow and white) galaxies are added to the frame. By studying different cosmic epochs, Roman will be able to trace the universe's expansion history, study how galaxies developed over time, and much more.Credit: Caltech-IPAC/R. Hurt and M. Troxel || Roman_Zoom_still.jpg (1920x1080) [515.9 KB] || Roman_Zoom_still_searchweb.png (320x180) [106.4 KB] || Roman_Zoom_still_thm.png (80x40) [6.6 KB] || Roman_Zoom-HD2K.mp4 (1920x1080) [25.3 MB] || Roman_Zoom-HD2K.webm (1920x1080) [2.7 MB] || ",
            "hits": 141
        },
        {
            "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": 122
        },
        {
            "id": 14281,
            "url": "https://svs.gsfc.nasa.gov/14281/",
            "result_type": "Produced Video",
            "release_date": "2023-01-26T11:00:00-05:00",
            "title": "Fermi Spots Gamma-ray Eclipsing 'Spider Systems'",
            "description": "An orbiting star begins to eclipse its partner, a rapidly rotating, superdense stellar remnant called a pulsar, in this illustration. The pulsar emits multiwavelength beams of light that rotate in and out of view and produces outflows that heat the star’s facing side, blowing away material and eroding its partner.Credit: NASA/Sonoma State University, Aurore Simonnet || GamRayEclipseG22.jpg (1800x1200) [1.1 MB] || GamRayEclipseG22_searchweb.png (320x180) [70.2 KB] || GamRayEclipseG22_thm.png (80x40) [6.8 KB] || ",
            "hits": 83
        },
        {
            "id": 14265,
            "url": "https://svs.gsfc.nasa.gov/14265/",
            "result_type": "Produced Video",
            "release_date": "2023-01-20T00:00:00-05:00",
            "title": "TESS 2022 Sky Views",
            "description": "This all-sky mosaic was constructed from 912 TESS images. By late October 2022, when the last image of this mosaic was captured, TESS had discovered 266 exoplanets and 4,258 candidates. The north and south ecliptic poles – the ends of imaginary lines extending above and below the center of Earth's orbit around the Sun – lie at the top and bottom of the image. The Andromeda galaxy is the small, bright oval near the upper right edge. The Lage Magellanic Cloud can be seen along the bottom edge just left of center. Above and to the left of it shine the Small Magellanic Cloud and the bright star cluster 47 Tucanae. Molleweide projection. Credit: NASA/MIT/TESS and Ethan Kruse (University of Maryland College Park) || TESS_NandS_12-2022.png (15000x7500) [85.3 MB] || TESS_NandS_12-2022.jpg (15000x7500) [43.4 MB] || TESS_NandS_12-2022_5k.jpg (5000x2500) [4.0 MB] || TESS_NandS_12-2022_5k_print.jpg (1024x512) [104.0 KB] || TESS_NandS_12-2022_5k_searchweb.png (320x180) [55.7 KB] || TESS_NandS_12-2022_5k_thm.png (80x40) [4.8 KB] || ",
            "hits": 185
        },
        {
            "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": 75
        },
        {
            "id": 14227,
            "url": "https://svs.gsfc.nasa.gov/14227/",
            "result_type": "Produced Video",
            "release_date": "2022-10-13T15:30:00-04:00",
            "title": "NASA Missions Detect Record-Breaking Burst",
            "description": "Swift’s X-Ray Telescope captured the afterglow of GRB 221009A about an hour after it was first detected. The bright rings form as a result of X-rays scattered by otherwise unobservable dust layers within our galaxy that lie in the direction of the burst. The dark vertical line is an artifact of the imaging system.Credit: NASA/Swift/A. Beardmore (University of Leicester) || XRT_image_crop.jpg (1084x1080) [629.3 KB] || XRT_image_crop_print.jpg (1024x1020) [657.0 KB] || XRT_image_crop_searchweb.png (320x180) [133.7 KB] || XRT_image_crop_web.png (320x318) [191.7 KB] || XRT_image_crop_thm.png (80x40) [26.1 KB] || ",
            "hits": 214
        },
        {
            "id": 14189,
            "url": "https://svs.gsfc.nasa.gov/14189/",
            "result_type": "Produced Video",
            "release_date": "2022-08-19T12:45:00-04:00",
            "title": "50th Anniversary of NASA's Copernicus Mission",
            "description": "Watch: This vintage segment on Copernicus comes from a 1973 edition of “The Science Report,” a long-running film series produced by the U.S. Information Agency. Credit: National Archives (306-SR-138B)Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || OAO-CopernicusFilm.02735_print.jpg (1024x768) [108.8 KB] || OAO-CopernicusFilm.mov (1440x1080) [2.1 GB] || OAO-CopernicusFilm.mp4 (1440x1080) [235.2 MB] || OAO-CopernicusFilm.webm (1440x1080) [24.5 MB] || OAO-CopernicusFilm.en_US.srt [3.8 KB] || OAO-CopernicusFilm.en_US.vtt [3.8 KB] || ",
            "hits": 117
        },
        {
            "id": 14170,
            "url": "https://svs.gsfc.nasa.gov/14170/",
            "result_type": "Produced Video",
            "release_date": "2022-08-10T10:00:00-04:00",
            "title": "NASA’s Fermi Confirms 'PeVatron' Supernova Remnant",
            "description": "Explore how astronomers located a supernova remnant that fires up protons to energies 10 times greater than the most powerful particle accelerator on Earth.Credit: NASA’s Goddard Space Flight CenterMusic: New Philosopher by Laurent Dury; Universal Production MusicWatch this video on the NASA Goddard YouTube channelComplete transcript available. || 14170-Found__A_PeVatron.01978_print.jpg (1024x576) [61.1 KB] || 14170-_PeVatron.webm (1920x1080) [15.1 MB] || 14170-_PeVatron.mp4 (1920x1080) [136.6 MB] || 14170-PeVatron.en_US.vtt [2.3 KB] || 14170-PeVatron.mov (1920x1080) [1.8 GB] || ",
            "hits": 266
        },
        {
            "id": 14181,
            "url": "https://svs.gsfc.nasa.gov/14181/",
            "result_type": "Produced Video",
            "release_date": "2022-08-04T13:00:00-04:00",
            "title": "Roman Interactive Stills",
            "description": "Right-side view of the Roman Space Telescope.  Highlighted parts available under \"Download Options\" || ROMAN_interactive_Spacecraft_V009_R_Off_2080_print.jpg (1024x576) [57.5 KB] || ROMAN_interactive_V009_R_Roman_off_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080.png (2080x1170) [751.5 KB] || ROMAN_interactive_V009_R_Roman_on_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_V009_R_Roman_comms_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Comms_2080.png (2080x1170) [771.3 KB] || ROMAN_interactive_V009_R_Roman_support_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Support_2080.png (2080x1170) [768.7 KB] || ROMAN_interactive_V009_R_Roman_tele_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_Tele_2080.png (2080x1170) [776.8 KB] || ROMAN_interactive_V009_R_Roman_SP_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_SP_2080.png (2080x1170) [786.4 KB] || ROMAN_interactive_V009_R_Roman_WFI_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_WFI_2080.png (2080x1170) [772.1 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_searchweb.png (320x180) [26.4 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_thm.png (80x40) [3.0 KB] || ",
            "hits": 62
        },
        {
            "id": 14146,
            "url": "https://svs.gsfc.nasa.gov/14146/",
            "result_type": "Produced Video",
            "release_date": "2022-05-04T00:00:00-04:00",
            "title": "Black Hole Desktop & Phone Wallpapers",
            "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ",
            "hits": 6388
        },
        {
            "id": 14130,
            "url": "https://svs.gsfc.nasa.gov/14130/",
            "result_type": "Produced Video",
            "release_date": "2022-04-07T14:00:00-04:00",
            "title": "Fermi Searches for Gravitational Waves From Monster Black Holes",
            "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ",
            "hits": 163
        },
        {
            "id": 14074,
            "url": "https://svs.gsfc.nasa.gov/14074/",
            "result_type": "Produced Video",
            "release_date": "2022-03-22T10:00:00-04:00",
            "title": "The Roman Space Telescope's High Latitude Survey Pointing Scheme",
            "description": "The sequence and layout of the Roman Space Telescope's High Latitude Spectroscopic Survey tiling pattern.Credit: NASA's Goddard Space Flight Center || Roman_HLSS_Pointing_Scheme_Still_print.jpg (1024x576) [119.5 KB] || Roman_HLSS_Pointing_Scheme_Still.jpg (3840x2160) [1.1 MB] || Roman_HLSS_Pointing_Scheme_Still_searchweb.png (320x180) [53.3 KB] || Roman_HLSS_Pointing_Scheme_Still_thm.png (80x40) [5.1 KB] || Roman_HLSS_Pointing_Scheme_FINAL_4k.mp4 (3840x2160) [25.1 MB] || Roman_HLSS_Pointing_Scheme_FINAL_4k.webm (3840x2160) [9.1 MB] || Roman_HLSS_Pointing_Scheme_FINAL_ProRes_3840x2160_5994.mov (3840x2160) [1.7 GB] || ",
            "hits": 298
        },
        {
            "id": 14107,
            "url": "https://svs.gsfc.nasa.gov/14107/",
            "result_type": "Infographic",
            "release_date": "2022-03-22T10:00:00-04:00",
            "title": "Roman Space Telescope Redshift Infographic",
            "description": "This graphic illustrates how cosmological redshift works and how it offers information about the universe’s evolution. The universe is expanding, and that expansion stretches light traveling through space. The more it has stretched, the greater the redshift and the greater the distance the light has traveled. As a result, we need telescopes with infrared detectors to see light from the first, most distant galaxies.Credit: NASA, ESA, Leah Hustak (STScI) || Roman_CosmologicalRedshift_Vertical_v3.png (1920x4843) [1.3 MB] || Roman_CosmologicalRedshift_Vertical_v3_print.jpg (1024x2582) [361.6 KB] || ",
            "hits": 162
        },
        {
            "id": 14099,
            "url": "https://svs.gsfc.nasa.gov/14099/",
            "result_type": "Produced Video",
            "release_date": "2022-02-28T00:00:00-05:00",
            "title": "Black Hole Week Assets",
            "description": "This page will introduce you to the world, characters, colors, and fonts of Black Hole Week. NASA celebrated Black Hole Week in 2019, 2021 and May, 2022.The world of Black Hole Week is bold, colorful, and a bit retro. It's also populated by a fun bunch of characters, including a little blue explorer (called the \"Traveler\") and their black hole friends. Below, you'll find tons of helpful images, GIFs, and other materials to get you going if you want to join in!If you are having trouble downloading the ZIP or AI files, please contact Barb Mattson: barb.mattson@nasa.gov || ",
            "hits": 95
        },
        {
            "id": 14075,
            "url": "https://svs.gsfc.nasa.gov/14075/",
            "result_type": "Produced Video",
            "release_date": "2022-01-17T00:00:00-05:00",
            "title": "Roman x Webb Comics",
            "description": "Space is like a box of chocolates, you never know what you're gonna get! This #ValentinesDay, we want to give you 18 sweet cosmic treats! Check out the thread below to learn more about these astro bites.See how Roman could help us learn more about these cosmic delights 1/10 nasa.gov/RomanOn X || VALENTINES_2024_Labels2.jpg (4172x4704) [1.8 MB] || VALENTINES_2024_Labels2.png (4172x4704) [6.6 MB] || ",
            "hits": 45
        },
        {
            "id": 14020,
            "url": "https://svs.gsfc.nasa.gov/14020/",
            "result_type": "Produced Video",
            "release_date": "2022-01-14T10:45:00-05:00",
            "title": "Where's Nancy?",
            "description": " || WheresNancy_print.jpg (1024x576) [286.4 KB] || WheresNancy.jpg (3840x2160) [2.5 MB] || WheresNancy_searchweb.png (320x180) [115.4 KB] || WheresNancy_thm.png (80x40) [15.7 KB] || ",
            "hits": 32
        },
        {
            "id": 13921,
            "url": "https://svs.gsfc.nasa.gov/13921/",
            "result_type": "Produced Video",
            "release_date": "2022-01-10T10:00:00-05:00",
            "title": "The Roman Space Telescope's Simulated Ultra-Deep Field Image",
            "description": "This video demonstrates how Roman could expand on Hubble’s iconic Ultra Deep Field image. While a similar Roman observation would be just as sharp as Hubble’s and see equally far back in time, it could reveal an area 300 times larger, offering a much broader view of cosmic ecosystems. Credit: NASA’s Goddard Space Flight CenterMusic: \"Subterranean Secret\" and \"Expectant Aspect\" from Universal Production Music.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SUDF_Footprint_print.jpg (1024x576) [232.0 KB] || SUDF_Footprint.jpg (3840x2160) [2.7 MB] || SUDF_Footprint_thm.png (80x40) [4.3 KB] || SUDF_Footprint_searchweb.png (320x180) [71.2 KB] || SUDF_Footprint_web.png (320x180) [71.2 KB] || 13921_Roman_Simulated_UDF_1080.webm (1920x1080) [24.4 MB] || 13921_Roman_Simulated_UDF_SRT_Captions.en_US.srt [3.8 KB] || 13921_Roman_Simulated_UDF_SRT_Captions.en_US.vtt [3.9 KB] || 13921_Roman_Simulated_UDF_ProRes_1920x1080_2997.mov (1920x1080) [3.0 GB] || 13921_Roman_Simulated_UDF_1080_Best.mp4 (1920x1080) [439.7 MB] || 13921_Roman_Simulated_UDF_1080.mp4 (1920x1080) [228.8 MB] || ",
            "hits": 93
        },
        {
            "id": 14001,
            "url": "https://svs.gsfc.nasa.gov/14001/",
            "result_type": "Infographic",
            "release_date": "2021-11-09T10:00:00-05:00",
            "title": "Roman Space Telescope High Latitude Wide Area Survey",
            "description": "This illustration compares the relative sizes of the areas of sky covered by two surveys: Roman’s High Latitude Wide Area Survey, outlined in blue, and the largest mosaic led by Hubble, the Cosmological Evolution Survey (COSMOS), shown in red. In current plans, the Roman survey will be more than 1,000 times broader than Hubble’s. Roman will also explore more distant realms of space than most other telescopes have probed in previous efforts to study why the expansion of the universe is speeding up. Credit: NASA's Goddard Space Flight Center || Roman_HLS_FINAL_1080.png (2160x1080) [9.8 MB] || Roman_HLS_FINAL_1080.jpg (2160x1080) [800.5 KB] || Roman_HLS_FINAL_1080_print.jpg (1024x512) [224.7 KB] || Roman_HLS_Final_Full.jpg (8000x4000) [3.8 MB] || Roman_HLS_FINAL_Half.png (4000x2000) [31.6 MB] || Roman_HLS_FINAL_Half.jpg (4000x2000) [1.7 MB] || Roman_HLS_FINAL_Full.png (8000x4000) [114.3 MB] || Roman_HLS_FINAL_1080_searchweb.png (320x180) [90.3 KB] || Roman_HLS_FINAL_1080_thm.png (80x40) [6.9 KB] || ",
            "hits": 96
        },
        {
            "id": 13873,
            "url": "https://svs.gsfc.nasa.gov/13873/",
            "result_type": "Produced Video",
            "release_date": "2021-07-01T00:00:00-04:00",
            "title": "Periodic Table of the Elements: Origins of the Elements",
            "description": "The periodic table organizes all the known elements by atomic number, which is the number of protons in each atom of the element.  This version of the table, which draws on data compiled by astronomer Jennifer Johnson from Ohio State University, shows our current understanding of how each element found on Earth was originally produced. Most of them ultimately have cosmic origins. Some elements were created with the birth of the universe, while others were made during the lives or deaths of stars. The Nancy Grace Roman Space Telescope will help us understand the cosmic era when stars first began forming. The mission will help scientists learn more about how elements were created and distributed throughout galaxies.The related Tumblr post is here. || ",
            "hits": 2044
        },
        {
            "id": 13831,
            "url": "https://svs.gsfc.nasa.gov/13831/",
            "result_type": "Produced Video",
            "release_date": "2021-04-15T13:00:00-04:00",
            "title": "NASA Visualization Probes the Doubly Warped World of Binary Black Holes",
            "description": "Explore how the extreme gravity of two orbiting supermassive black holes distorts our view. In this visualization, disks of bright, hot, churning gas encircle both black holes, shown in red and blue to better track the light source. The red disk orbits the larger black hole, which weighs 200 million times the mass of our Sun, while its smaller blue companion weighs half as much. Zooming into each black hole reveals multiple, increasingly warped images of its partner. Watch to learn more. Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman and Brian P. PowellMusic: \"Gravitational Field\" from Orbit.  Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Supermassive_BlackHole_Binary_Still.jpg (3840x2160) [726.7 KB] || Supermassive_BlackHole_Binary_Still_searchweb.png (320x180) [18.9 KB] || Supermassive_BlackHole_Binary_Still_thm.png (80x40) [2.5 KB] || 13831_BlackHoleBinary_Simulation_1080.webm (1920x1080) [23.8 MB] || 13831_BlackHoleBinary_Simulation_1080.mp4 (1920x1080) [234.7 MB] || 13831_BlackHoleBinary_Simulation_4k.mp4 (3840x2160) [348.3 MB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4 (3840x2160) [936.6 MB] || 13831_BlackHoleBinary_Simulation_ProRes_3840x2160_30.mov (3840x2160) [4.1 GB] || 13831_BlackHoleBinary_Simulation_4k_Best.mp4.hwshow [137 bytes] || ",
            "hits": 298
        },
        {
            "id": 13827,
            "url": "https://svs.gsfc.nasa.gov/13827/",
            "result_type": "Produced Video",
            "release_date": "2021-03-31T10:00:00-04:00",
            "title": "Viewing Exoplanet Transits in the Milky Way",
            "description": "This graphic highlights the search areas of three planet-hunting missions: the upcoming Nancy Grace Roman Space Telescope, the Transiting Exoplanet Survey Satellite (TESS), and the retired Kepler Space Telescope. Astronomers expect Roman to discover roughly 100,000 transiting planets, worlds that periodically dim the light of their stars as they cross in front of them.. While other missions, including Kepler's extended K2 survey (not pictured in this graphic), have unveiled relatively nearby planets, Roman will reveal a wealth of worlds much farther from home.Credit: NASA's Goddard Space Flight Center || Exoplanet_Transit_FOV_Graphic_Half.png (1950x1950) [16.3 MB] || Exoplanet_Transit_FOV_Graphic.png (3900x3900) [59.4 MB] || Exoplanet_Transit_FOV_Graphic.jpg (3900x3900) [1.6 MB] || Exoplanet_Transit_FOV_Graphic_searchweb.png (320x180) [95.5 KB] || Exoplanet_Transit_FOV_Graphic_thm.png (80x40) [7.6 KB] || ",
            "hits": 68
        },
        {
            "id": 13794,
            "url": "https://svs.gsfc.nasa.gov/13794/",
            "result_type": "Infographic",
            "release_date": "2021-02-12T14:00:00-05:00",
            "title": "NASA’s TESS Finds New Worlds in a River of Stars",
            "description": "This illustration sketches out the main features of TOI 451, a triple-planet system located 400 light-years away in the constellation Eridanus.Credit: NASA’s Goddard Space Flight Center || TOI_451_infographic_1920.png (1920x1080) [2.6 MB] || TOI_451_infographic_1920_print.jpg (1024x576) [129.4 KB] || TOI_451_infographic_3840.png (3840x2160) [8.2 MB] || TOI_451_infographic_1920_searchweb.png (320x180) [73.0 KB] || TOI_451_infographic_1920_thm.png (80x40) [6.5 KB] || ",
            "hits": 304
        },
        {
            "id": 13802,
            "url": "https://svs.gsfc.nasa.gov/13802/",
            "result_type": "Produced Video",
            "release_date": "2021-02-02T00:00:00-05:00",
            "title": "Roman Coloring Pages",
            "description": "Our Nancy Grace Roman Space Telescope presents: two new color pages! Unleash your creativity to bring these celestial scenes to life. || ",
            "hits": 45
        },
        {
            "id": 13710,
            "url": "https://svs.gsfc.nasa.gov/13710/",
            "result_type": "Produced Video",
            "release_date": "2020-10-05T13:00:00-04:00",
            "title": "TESS's Northern Sky Vista",
            "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) spent nearly a year imaging the northern sky in its search for worlds beyond our solar system. Explore this panorama to see what TESS has found so far.Credit: NASA's Goddard Space Flight CenterMusic: \"Strolling\" from Above and Below. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Northern_and_Southern_Still.jpg (1920x1080) [699.1 KB] || 13710_TESS_Northern_Tour_Best_1080.webm (1920x1080) [33.4 MB] || 13710_TESS_Northern_Tour_1080.mp4 (1920x1080) [423.5 MB] || 13710_TESS_Northern_Tour_SRT_Captions.en_US.srt [4.9 KB] || 13710_TESS_Northern_Tour_SRT_Captions.en_US.vtt [4.9 KB] || 13710_TESS_Northern_Tour_Best_1080.mp4 (1920x1080) [1.1 GB] || 13710_TESS_Northern_Tour_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || ",
            "hits": 64
        },
        {
            "id": 13726,
            "url": "https://svs.gsfc.nasa.gov/13726/",
            "result_type": "Produced Video",
            "release_date": "2020-10-05T13:00:00-04:00",
            "title": "TESS Northern and Southern Mosaics",
            "description": "This plot combines the TESS northern and southern mosaics to show the extent of its primary mission survey. The yearlong southern panorama (bottom) was completed in July 2019, and the northern imaging was completed in July 2020.  The prominent glowing band is the Milky Way, our galaxy seen edgewise. The ecliptic – the plane of Earth's orbit and the apparent yearly path of the Sun through the stars – runs straight across the middle of the map. Credit: NASA/MIT/TESS and Ethan Kruse (USRA) || TESS_North-South_Mollweide_Ecliptic_15k.jpg (15000x7500) [40.4 MB] || TESS_North-South_Mollweide_Ecliptic_1080.jpg (2160x1080) [821.7 KB] || TESS_North-South_Mollweide_Ecliptic_7k.jpg (7500x3750) [9.9 MB] || TESS_North-South_Mollweide_Ecliptic_1080_print.jpg (1024x512) [146.3 KB] || TESS_North-South_Mollweide_Ecliptic_1080_searchweb.png (320x180) [66.5 KB] || TESS_North-South_Mollweide_Ecliptic_1080_thm.png (80x40) [7.2 KB] || TESS_North-South_Mollweide_Ecliptic_30k.png (30000x15000) [135.8 MB] || ",
            "hits": 73
        },
        {
            "id": 4856,
            "url": "https://svs.gsfc.nasa.gov/4856/",
            "result_type": "Visualization",
            "release_date": "2020-09-09T13:00:00-04:00",
            "title": "An Elsewhere Starfield",
            "description": "The randomized star map in celestial coordinates, at five different resolutions. (Or more generically: The galactic plane is tilted 63° in the coordinate frame of the image.) || starmap_random_2020_4k_print.jpg (1024x512) [37.1 KB] || starmap_random_2020_4k_searchweb.png (320x180) [67.0 KB] || starmap_random_2020_4k_thm.png (80x40) [4.3 KB] || starmap_random_2020_4k.exr (4096x2048) [34.1 MB] || starmap_random_2020_8k.exr (8192x4096) [123.8 MB] || starmap_random_2020_16k.exr (16384x8192) [423.3 MB] || starmap_random_2020_32k.exr (32768x16384) [1.4 GB] || starmap_random_2020_64k.exr (65536x32768) [3.8 GB] || ",
            "hits": 444
        },
        {
            "id": 13696,
            "url": "https://svs.gsfc.nasa.gov/13696/",
            "result_type": "Produced Video",
            "release_date": "2020-08-25T11:00:00-04:00",
            "title": "Young Active Galaxy with ‘TIE Fighter’ Shape",
            "description": "This illustration shows two views of the active galaxy TXS 0128+554, located around 500 million light-years away. Left: The galaxy’s central jets appear as they would if we viewed them both at the same angle. The black hole, embedded in a disk of dust and gas, launches a pair of particle jets traveling at nearly the speed of light. Scientists think gamma rays (magenta) detected by NASA’s Fermi Gamma-ray Space Telescope originate from the base of these jets. As the jets collide with material surrounding the galaxy, they form identical lobes seen at radio wavelengths (orange). The jets experienced two distinct bouts of activity, which created the gap between the lobes and the black hole. Right: The galaxy appears in its actual orientation, with its jets tipped out of our line of sight by about 50 degrees.Credit: NASA’s Goddard Space Flight Center || TXS0128_Side-by-Side_FInal.jpg (7680x2160) [1.8 MB] || TXS0128_Side-by-Side_FInal_Half.jpg (3840x1080) [601.5 KB] || TXS0128_Side-by-Side_FInal_print.jpg (1024x288) [45.4 KB] || TXS0128_Side-by-Side_FInal.jpg.dzi (7680x2160) [178 bytes] || TXS0128_Side-by-Side_FInal.jpg_files (1x1) [4.0 KB] || ",
            "hits": 114
        },
        {
            "id": 13280,
            "url": "https://svs.gsfc.nasa.gov/13280/",
            "result_type": "Produced Video",
            "release_date": "2020-08-19T00:00:00-04:00",
            "title": "Assembling XRISM's X-ray Mirrors",
            "description": "Team members Lawrence Lozipone of Stinger Ghaffarian Technologies, Inc. and Yang Soong, a researcher at the University of Maryland, College Park, work with flight mirrors for the X-ray Imaging and Spectroscopy Mission (XRISM). Nested aluminum mirror segments – 1,624 of them for each X-ray Mirror Assembly – focus the incoming X-rays for the satellite's science instruments. Credit: NASA's Goddard Space Flight Center || XRISM_Cleanroom_B-roll_1080Still.jpg (1920x1080) [727.5 KB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.mov (1920x1080) [7.0 GB] || XRISM_Cleanroom_B-roll_1080.mp4 (1920x1080) [991.6 MB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.webm (1920x1080) [52.0 MB] || ",
            "hits": 91
        },
        {
            "id": 13667,
            "url": "https://svs.gsfc.nasa.gov/13667/",
            "result_type": "Produced Video",
            "release_date": "2020-07-24T16:00:00-04:00",
            "title": "The Roman Space Telescope's Immense Data Volume",
            "description": "This infographic showcases the difference in data volume between the Nancy Grace Roman, Webb and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.Credit: NASA's Goddard Space Flight Center || Roman_Data_Scale_Final_1080.png (1920x1080) [9.7 MB] || Roman_Data_Scale_Final_1080.jpg (1920x1080) [515.8 KB] || Roman_Data_Scale_Final_1080_print.jpg (1024x576) [99.3 KB] || Roman_Data_Scale_Final.png (3840x2160) [38.9 MB] || Roman_Data_Scale_Final.jpg (3840x2160) [1.9 MB] || ",
            "hits": 297
        },
        {
            "id": 13605,
            "url": "https://svs.gsfc.nasa.gov/13605/",
            "result_type": "Produced Video",
            "release_date": "2020-05-13T11:00:00-04:00",
            "title": "TESS Aids Breakthrough in Puzzling Stellar Flashes",
            "description": "Watch the pulsations of a Delta Scuti star! In this illustration, the star changes in brightness when internal sound waves at different frequencies cause parts of the star to expand and contract. In one pattern, the whole star expands and contracts, while in a second, opposite hemispheres swell and shrink out of sync. In reality, a single star exhibits many pulsation patterns that can tell astronomers about its age, composition and internal structure. The exact light variations astronomers observe also depend on how the star's spin axis angles toward us. Delta Scuti stars spin so rapidly they flatten into ovals, which jumbles these signals and makes them harder to decode. Now, thanks to NASA's Transiting Exoplanet Survey Satellite, astronomers are deciphering some of them.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || Exterior_still.jpg (1920x1080) [460.3 KB] || 13605_Delta_Scuti_Pulsation_ProRes_1920x1080_2997.mov (1920x1080) [523.3 MB] || 13605_Delta_Scuti_Pulsation.mp4 (1920x1080) [36.1 MB] || 13605_Delta_Scuti_Pulsation.webm (1920x1080) [3.6 MB] || ",
            "hits": 112
        },
        {
            "id": 13570,
            "url": "https://svs.gsfc.nasa.gov/13570/",
            "result_type": "Produced Video",
            "release_date": "2020-04-27T11:00:00-04:00",
            "title": "Swift Tracks Water from Interstellar Visitor Borisov",
            "description": "Watch how NASA’s Neil Gehrels Swift Observatory tracked water production by interstellar comet 2I/Borisov as it sped through the solar system. On average, Borisov produced enough water to fill a standard bathtub in 10 seconds. It shares many traits with solar system comets, which may mean that comets form similarly in different planetary systems.Credit: NASA’s Goddard Space Flight CenterMusic: \"Mesmeric Thoughts\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Swift_Comet_Still.jpg (1920x1080) [599.5 KB] || Swift_Comet_Still_searchweb.png (320x180) [94.6 KB] || Swift_Comet_Still_thm.png (80x40) [6.0 KB] || 13570_Swift_Interstellar_Comet.webm (1920x1080) [17.2 MB] || 13570_Swift_Interstellar_Comet_SRT_Captions.en_US.vtt [2.1 KB] || 13570_Swift_Interstellar_Comet_SRT_Captions.en_US.srt [2.1 KB] || 13570_Swift_Interstellar_Comet_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || 13570_Swift_Interstellar_Comet_Best_1080.mp4 (1920x1080) [375.4 MB] || 13570_Swift_Interstellar_Comet.mp4 (1920x1080) [159.3 MB] || ",
            "hits": 70
        },
        {
            "id": 13583,
            "url": "https://svs.gsfc.nasa.gov/13583/",
            "result_type": "Infographic",
            "release_date": "2020-04-20T10:00:00-04:00",
            "title": "Hubble, Roman and Webb Space Telescopes Infographic",
            "description": "This infographic shows the complementary capabilities of select instruments on three of NASA's flagship missions: the Hubble Space Telescope and the currently under development Nancy Grace Roman Space Telescope and James Webb Space Telescope. Hubble views the cosmos in infrared, visible and ultraviolet light, providing a more comprehensive, high-resolution view of individual objects. The Roman Space Telescope will expand on Hubble’s infrared observations specifically, using a much larger field of view to create enormous panoramas of the universe with the same high resolution. Webb will also conduct high-resolution infrared observations, peering across farther stretches of space with a narrower field of view.Credit: NASA's Goddard Space Flight Center || HRJ_Infographic_Final2.png (4560x6680) [20.0 MB] || HRJ_Infographic_Final2.jpg (4560x6680) [5.2 MB] || HRJ_Infographic_Final2_HalfSize.jpg (2280x3340) [2.1 MB] || HRJ_Infographic_Final2_HalfSize.png (2280x3340) [8.8 MB] || ",
            "hits": 429
        },
        {
            "id": 13578,
            "url": "https://svs.gsfc.nasa.gov/13578/",
            "result_type": "Produced Video",
            "release_date": "2020-04-13T11:00:00-04:00",
            "title": "NASA Missions Study a Nova's Shock Waves",
            "description": "NASA’s Fermi and NuSTAR space telescopes, together with another satellite named BRITE-Toronto, are providing new insights into a nova explosion that erupted in 2018. Detailed measurements of bright flares in the explosion clearly show that shock waves power most of the nova's visible light.  Credit: NASA’s Goddard Space Flight CenterMusic: \"Scientist\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || novastill01.jpg (3840x2160) [1.1 MB] || novastill01_searchweb.png (320x180) [76.8 KB] || novastill01_thm.png (80x40) [6.7 KB] || 13578_Nova_Carinae_Best.webm (1920x1080) [13.8 MB] || novastill01.tif (3840x2160) [31.7 MB] || 13578_Nova_Carinae_SRT_Captions.en_US.srt [2.2 KB] || 13578_Nova_Carinae_SRT_Captions.en_US.vtt [2.2 KB] || 13578_Nova_Carinae_Best.mp4 (1920x1080) [319.4 MB] || 13578_Nova_Carinae_Good.mp4 (1920x1080) [129.0 MB] || 13578_Nova_Carinae_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ",
            "hits": 154
        },
        {
            "id": 13556,
            "url": "https://svs.gsfc.nasa.gov/13556/",
            "result_type": "Produced Video",
            "release_date": "2020-02-14T03:00:00-05:00",
            "title": "Astrophysics Valentines",
            "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ",
            "hits": 65
        },
        {
            "id": 13530,
            "url": "https://svs.gsfc.nasa.gov/13530/",
            "result_type": "Produced Video",
            "release_date": "2020-01-30T00:00:00-05:00",
            "title": "Mirror Quadrants for XRISM",
            "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ",
            "hits": 60
        },
        {
            "id": 13526,
            "url": "https://svs.gsfc.nasa.gov/13526/",
            "result_type": "Infographic",
            "release_date": "2020-01-24T10:00:00-05:00",
            "title": "What Makes an Exoplanet Habitable?",
            "description": "Explore this infographic to learn more about the many different factors that make a planet potentially habitable. Complete text transcript available.Machine readable version available.Credit: NASA Goddard Space Flight Center || Infographic_24x70_inset.jpg (1920x1080) [201.2 KB] || Habitability_Infographic_CROP_print.jpg (1024x702) [120.2 KB] || Habitability_Infographic_CROP.png (6667x4573) [1.7 MB] || Habitability_Infographic_FULL_24x70_2024Update.png (6667x19500) [5.4 MB] || Habitability_Infographic_CROP_searchweb.png (320x180) [47.0 KB] || Habitability_Infographic_CROP_thm.png (80x40) [5.7 KB] || ",
            "hits": 459
        },
        {
            "id": 13511,
            "url": "https://svs.gsfc.nasa.gov/13511/",
            "result_type": "Produced Video",
            "release_date": "2020-01-05T15:00:00-05:00",
            "title": "Distant Galaxy Group Caught Driving Ancient Cosmic Makeover",
            "description": "This animation shows EGS77’s place in cosmic history, flies to the galaxies, and illustrates how ultraviolet light from their stars create bubbles of ionized hydrogen around them.Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || reionization_animation_with_label_122019.00001_print.jpg (1024x576) [69.7 KB] || reionization_animation_with_label_122019.mp4 (1920x1080) [83.2 MB] || reionization_animation_with_label_122019.webm (1920x1080) [4.0 MB] || reionization_animation_with_label_122019.mov (1920x1080) [433.6 MB] || ",
            "hits": 246
        },
        {
            "id": 13497,
            "url": "https://svs.gsfc.nasa.gov/13497/",
            "result_type": "Produced Video",
            "release_date": "2020-01-05T14:00:00-05:00",
            "title": "Simulated Image Demonstrates the Power of NASA’s Nancy Grace Roman Space Telescope",
            "description": "Watch the video to learn more about the Roman Space Telescope's simulated image.Credit: NASA's Goddard Space Flight CenterMusic: \"Flight Impressions\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Simulated_Image_Still.jpg (1920x1080) [891.1 KB] || 13497_Simulated_Image_Roman_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13497_Simulated_Image_Roman_Best_1080.mp4 (1920x1080) [936.5 MB] || 13497_Simulated_Image_Roman_1080.mp4 (1920x1080) [291.8 MB] || 13497_Simulated_Image_Roman_1080.webm (1920x1080) [22.4 MB] || Simulated_Image_Roman_SRT_Captions.en_US.srt [3.6 KB] || Simulated_Image_Roman_SRT_Captions.en_US.vtt [3.6 KB] || ",
            "hits": 199
        },
        {
            "id": 13209,
            "url": "https://svs.gsfc.nasa.gov/13209/",
            "result_type": "Produced Video",
            "release_date": "2019-12-19T12:00:00-05:00",
            "title": "NASA’s Fermi Finds Vast ‘Halo’ Around Nearby Pulsar",
            "description": "Astronomers using data from NASA’s Fermi mission have discovered a pulsar with a faint gamma-ray glow that spans a huge part of the sky. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Insight\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Geminga_Still.jpg (1920x1080) [177.1 KB] || Geminga_Still_print.jpg (1024x576) [65.2 KB] || Geminga_Still_searchweb.png (320x180) [75.1 KB] || Geminga_Still_thm.png (80x40) [5.6 KB] || 13209_Fermi_Geminga_Halo_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || 13209_Fermi_Geminga_Halo_1080_Best.mp4 (1920x1080) [294.5 MB] || 13209_Fermi_Geminga_Halo_1080_Best.webm (1920x1080) [15.3 MB] || 13209_Fermi_Geminga_Halo_1080_Good.mp4 (1920x1080) [144.1 MB] || Fermi_Geminga_Halo_SRT_Captions.en_US.srt [1.7 KB] || Fermi_Geminga_Halo_SRT_Captions.en_US.vtt [1.7 KB] || ",
            "hits": 98
        },
        {
            "id": 13427,
            "url": "https://svs.gsfc.nasa.gov/13427/",
            "result_type": "Produced Video",
            "release_date": "2019-11-20T13:00:00-05:00",
            "title": "A New Era in Gamma-ray Science",
            "description": "On Jan. 14, 2019, the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) observatory in the Canary Islands captured the highest-energy light every recorded from a gamma-ray burst. MAGIC began observing the fading burst just 50 seconds after it was detected thanks to positions provided by NASA's Fermi and Swift spacecraft (top left and right, respectively, in this illustration). The gamma rays packed energy up to 10 times greater than previously seen. Credit: NASA/Fermi and Aurore Simonnet, Sonoma State University || GRB190114CbASimonnet.jpg (2475x3300) [4.5 MB] || GRB190114CbASimonnet_searchweb.png (320x180) [106.4 KB] || GRB190114CbASimonnet_thm.png (80x40) [6.6 KB] || ",
            "hits": 84
        },
        {
            "id": 13267,
            "url": "https://svs.gsfc.nasa.gov/13267/",
            "result_type": "Produced Video",
            "release_date": "2019-11-05T13:00:00-05:00",
            "title": "TESS Southern Hemisphere Sector Images",
            "description": "Sector 1.The Transiting Exoplanet Survey Satellite (TESS) observed this strip of stars and galaxies in the southern sky from July 25, 2018, to August 22, 2018. TESS captured this individual image during one 30-minute period on 2018-08-07 at 04:59:42 UTC. The Large and Small Magellanic Clouds appear on the right-hand side. || TESS_Sector_1.png (16774x4272) [75.1 MB] || TESS_Sector_1.jpeg (16774x4272) [27.6 MB] || TESS_Sector_1_halfsize.jpeg (8387x2136) [9.7 MB] || TESS_Sector_1_halfsize.png (8387x2136) [9.7 MB] || ",
            "hits": 147
        },
        {
            "id": 13285,
            "url": "https://svs.gsfc.nasa.gov/13285/",
            "result_type": "Produced Video",
            "release_date": "2019-11-05T13:00:00-05:00",
            "title": "TESS's Southern Sky Panorama",
            "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) spent a year imaging the southern sky in its search for worlds beyond our solar system. Dive into a mosaic of these images to see what TESS has found so far. Credit: NASA's Goddard Space Flight CenterMusic: “Phenomenon\" from Above and Below Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Southern_Sky_Still.jpg (1920x1080) [892.0 KB] || Southern_Sky_Still_print.jpg (1024x576) [222.5 KB] || Southern_Sky_Still_searchweb.png (320x180) [66.5 KB] || Southern_Sky_Still_thm.png (80x40) [5.0 KB] || 13285_TESS_SouthernSky_Small_720.webm (1280x720) [26.3 MB] || 13285_TESS_SouthernSky_Small_720.mp4 (1280x720) [250.7 MB] || 13285_TESS_SouthernSky_1080.mp4 (1920x1080) [492.4 MB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.srt [4.3 KB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.vtt [4.3 KB] || 13285_TESS_SouthernSky_Best_1080.mp4 (1920x1080) [1.2 GB] || 13285_TESS_SouthernSky_ProRes_1920x1080_30.mov (1920x1080) [3.5 GB] || tesss-southern-sky-panorama-movie.hwshow || 07a_tess_coverage.hwshow [190 bytes] || ",
            "hits": 142
        },
        {
            "id": 13324,
            "url": "https://svs.gsfc.nasa.gov/13324/",
            "result_type": "Produced Video",
            "release_date": "2019-09-25T09:00:00-04:00",
            "title": "Black Hole Safety: Desktop & Phone Wallpaper",
            "description": "So you’ve planned your trip to a black hole, you’ve packed your bags, and you’ve even watched the pre-flight safety video. If you haven’t yet watched the video, however, we highly recommend you click the image below. Don’t worry, we’ll wait.Now then, want to make black hole travel an even bigger part of your daily life? Wishing that black holes actually WERE portals to dimensions filled with unicorns and space potatoes? Download these phone and desktop wallpapers to fill your screens. || ",
            "hits": 62
        },
        {
            "id": 13322,
            "url": "https://svs.gsfc.nasa.gov/13322/",
            "result_type": "Animation",
            "release_date": "2019-09-23T10:00:00-04:00",
            "title": "NASA's Guide To Black Hole Safety",
            "description": "Have you ever thought about visiting a black hole? We sure hope not. However, if you're absolutely convinced that a black hole is your ideal vacation spot, watch this video before you blast off to learn more about them and (more importantly) how to stay safe.You can also download a handy safety brochure, watch short clips to learn different things about black holes, and even get some short glimpses into the lives of black holes and the explorers that want to visit them. || ",
            "hits": 255
        }
    ]
}