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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] || ",
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        {
            "id": 5604,
            "url": "https://svs.gsfc.nasa.gov/5604/",
            "result_type": "Visualization",
            "release_date": "2026-01-27T18:00:00-05:00",
            "title": "March 3, 2026 Total Lunar Eclipse: Shadow View",
            "description": "On March 3, 2026, the Moon enters the Earth's shadow, creating a total lunar eclipse. This set of visualizations shows the view down the barrel of the Earth's shadow as the Moon moves through it, along with times at various stages.",
            "hits": 1022
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        {
            "id": 5609,
            "url": "https://svs.gsfc.nasa.gov/5609/",
            "result_type": "Visualization",
            "release_date": "2026-01-26T05:00:00-05:00",
            "title": "Heliophysics Satellite Fleet - 2026",
            "description": "A tour of the NASA Heliophysics fleet from near-Earth satellites out to the Voyagers beyond the heliopause.",
            "hits": 938
        },
        {
            "id": 31362,
            "url": "https://svs.gsfc.nasa.gov/31362/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-01-22T18:59:59-05:00",
            "title": "Circinus Galaxy Zoom",
            "description": "This shows the location of the Circinus galaxy on the sky. It begins with a ground-based photo of the constellation Circinus. The video closes in on the Circinus galaxy, using views from the Digitized Sky Survey and the Dark Energy Survey Camera. Continueing with an image of the galaxy from NASA’s Hubble Space Telescope, zooms in even more to the image of the galaxy’s core from NASA’s James Webb Space Telescope in near-infrared light.",
            "hits": 70
        },
        {
            "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": 139
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        {
            "id": 5587,
            "url": "https://svs.gsfc.nasa.gov/5587/",
            "result_type": "Visualization",
            "release_date": "2025-12-11T12:00:00-05:00",
            "title": "Moon Phase and Libration, 2026",
            "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.",
            "hits": 7832
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            "id": 5588,
            "url": "https://svs.gsfc.nasa.gov/5588/",
            "result_type": "Visualization",
            "release_date": "2025-12-11T12:00:00-05:00",
            "title": "Moon Phase and Libration, 2026 South Up",
            "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.",
            "hits": 801
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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] || ",
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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] || ",
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            "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] || ",
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        },
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            "id": 31356,
            "url": "https://svs.gsfc.nasa.gov/31356/",
            "result_type": "Animation",
            "release_date": "2025-08-30T01:59:59-04:00",
            "title": "Cosmic Caverns in the Cat’s Paw Nebula",
            "description": "This visualization explores a subset of toe bean-reminiscent structures within a section of the Cat’s Paw Nebula, a massive, local star-forming region located approximately 4,000 light-years away in the constellation Scorpius.",
            "hits": 54
        },
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            "id": 5576,
            "url": "https://svs.gsfc.nasa.gov/5576/",
            "result_type": "Visualization",
            "release_date": "2025-08-26T09:00:00-04:00",
            "title": "TROPICS Eyes Hurricane Erin",
            "description": "This animation tracks Hurricane Erin from August 10 through August 20, 2025. || Erin_v07_L1C_ch12_2025-08-28_121639.02708_print.jpg (1024x576) [138.3 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_searchweb.png (320x180) [86.9 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_thm.png (80x40) [6.2 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.mp4 (1920x1080) [17.4 MB] || channel_12 (1920x1080) [855 Item(s)] ||",
            "hits": 45
        },
        {
            "id": 14868,
            "url": "https://svs.gsfc.nasa.gov/14868/",
            "result_type": "Produced Video",
            "release_date": "2025-07-23T00:00:00-04:00",
            "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail",
            "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ",
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        },
        {
            "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": 31562
        },
        {
            "id": 31354,
            "url": "https://svs.gsfc.nasa.gov/31354/",
            "result_type": "Animation",
            "release_date": "2025-06-13T16:19:00-04:00",
            "title": "PUNCH",
            "description": "NASA’s PUNCH Releases Its First Images of Huge Eruptions from Sun",
            "hits": 152
        },
        {
            "id": 14857,
            "url": "https://svs.gsfc.nasa.gov/14857/",
            "result_type": "Produced Video",
            "release_date": "2025-06-11T14:10:00-04:00",
            "title": "NASA’s Webb Reveals Galaxy Population Driving Cosmic Renovation",
            "description": "Symbols mark the locations of young, low-mass galaxies bursting with new stars when the universe was about 800 million years old. Using a filter sensitive to such galaxies, NASA’s James Webb Space Telescope imaged them with the help of a natural gravitational lens created by the massive galaxy cluster Abell 2744. In all, 83 young galaxies were found, but only the 20 shown here (white diamonds) were selected for deeper study. The inset zooms into one of the galaxies. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025Alt text: Animation showing the locations of young, low-mass, starburst galaxies around galaxy cluster Abell 2744.Image description:White and yellow galaxies of various sizes and shapes appear against the blackness of space. Two bright stars in our own galaxy display prominent six-spike diffraction patterns with bluish rays, visible at center left and lower left. Then 20 white diamonds sweep across the image. One diamond enlarges to reveal an image of a young, low-mass, star-forming galaxy. It looks like a green oval against a red and green checked background. The enlarged image then shrinks back, and the diamonds sweep away. The sequence loops. || Pandora_stamp_60pct.gif (600x600) [961.0 KB] || ",
            "hits": 290
        },
        {
            "id": 14798,
            "url": "https://svs.gsfc.nasa.gov/14798/",
            "result_type": "Produced Video",
            "release_date": "2025-05-27T20:56:00-04:00",
            "title": "Astrophysics Multiwavelength Vertical Video",
            "description": "This page contains vertically-formatted Astrophysics videos that show multiwavelength content.",
            "hits": 182
        },
        {
            "id": 14819,
            "url": "https://svs.gsfc.nasa.gov/14819/",
            "result_type": "Produced Video",
            "release_date": "2025-05-06T10:45:00-04:00",
            "title": "NASA's NICER Studies Recurring Cosmic Crashes",
            "description": "Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" by Lee Groves [PRS] and Peter Geogre Marett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_thumbnail_NICER_QPE.jpg (1280x720) [225.7 KB] || YTframe_thumbnail_NICER_QPE_searchweb.png (320x180) [95.5 KB] || YTframe_thumbnail_NICER_QPE_thm.png [8.7 KB] || 14819_NICER_QPE_Good.mp4 (1920x1080) [70.6 MB] || 14819_NICER_QPE_Best.mp4 (1920x1080) [172.3 MB] || 14819_NICER_QPE_Captions.en_US.srt [2.8 KB] || 14819_NICER_QPE_Captions.en_US.vtt [2.7 KB] || 14819_NICER_QPE_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ",
            "hits": 134
        },
        {
            "id": 14802,
            "url": "https://svs.gsfc.nasa.gov/14802/",
            "result_type": "Produced Video",
            "release_date": "2025-03-28T14:31:59-04:00",
            "title": "Earth to Space: A National Symphony Orchestra Concert",
            "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.",
            "hits": 119
        },
        {
            "id": 14784,
            "url": "https://svs.gsfc.nasa.gov/14784/",
            "result_type": "Produced Video",
            "release_date": "2025-02-13T14:00:00-05:00",
            "title": "PUNCH Mission Media Teleconference",
            "description": "NASA held a media teleconference at 2 p.m. EST on Tuesday, February 4, to share information about the agency’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, which is targeted to launch no earlier than Thursday, February 27, 2025.The agency’s PUNCH mission is a constellation of four small satellites. When they arrive in low Earth orbit, the satellites will make global, 3D observations of the Sun’s outer atmosphere, the corona, and help NASA learn how the mass and energy there become solar wind. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission will share a ride to space with NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) space telescope on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.The Southwest Research Institute in Boulder, Colorado, leads the PUNCH mission. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington.To learn more about PUNCH, please visit: nasa.gov/punch || ",
            "hits": 71
        },
        {
            "id": 14773,
            "url": "https://svs.gsfc.nasa.gov/14773/",
            "result_type": "Produced Video",
            "release_date": "2025-02-04T10:00:00-05:00",
            "title": "NASA's PUNCH Mission",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun’s corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.Watch the video to learn how imaging the Sun’s corona and the solar wind together will help scientists better understand the entire inner heliosphere — Sun, solar wind, and Earth — as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate.For more information visit science.nasa.gov/mission/punch || ",
            "hits": 100
        },
        {
            "id": 14776,
            "url": "https://svs.gsfc.nasa.gov/14776/",
            "result_type": "Produced Video",
            "release_date": "2025-01-30T14:00:00-05:00",
            "title": "PUNCH Satellites Integration and Testing",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ",
            "hits": 48
        },
        {
            "id": 14769,
            "url": "https://svs.gsfc.nasa.gov/14769/",
            "result_type": "Produced Video",
            "release_date": "2025-01-29T11:00:00-05:00",
            "title": "Social Media Shorts",
            "description": "A collection of assorted social media vertical videos. || ",
            "hits": 41
        },
        {
            "id": 14771,
            "url": "https://svs.gsfc.nasa.gov/14771/",
            "result_type": "Produced Video",
            "release_date": "2025-01-24T14:00:00-05:00",
            "title": "PUNCH Instruments",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ",
            "hits": 88
        },
        {
            "id": 14770,
            "url": "https://svs.gsfc.nasa.gov/14770/",
            "result_type": "Produced Video",
            "release_date": "2025-01-24T09:00:00-05:00",
            "title": "PUNCH Satellites Test Operations at Vandenberg Space Force Base",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ",
            "hits": 25
        },
        {
            "id": 14768,
            "url": "https://svs.gsfc.nasa.gov/14768/",
            "result_type": "Produced Video",
            "release_date": "2025-01-23T17:00:00-05:00",
            "title": "PUNCH Satellites Solar Array Deployment Test",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ",
            "hits": 65
        },
        {
            "id": 14767,
            "url": "https://svs.gsfc.nasa.gov/14767/",
            "result_type": "Produced Video",
            "release_date": "2025-01-23T16:00:00-05:00",
            "title": "PUNCH Satellites Arrival at Vandenberg Space Force Base",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ",
            "hits": 37
        },
        {
            "id": 14765,
            "url": "https://svs.gsfc.nasa.gov/14765/",
            "result_type": "Produced Video",
            "release_date": "2025-01-23T15:00:00-05:00",
            "title": "PUNCH Assembly and Testing",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ",
            "hits": 58
        },
        {
            "id": 40532,
            "url": "https://svs.gsfc.nasa.gov/gallery/punch/",
            "result_type": "Gallery",
            "release_date": "2025-01-22T00:00:00-05:00",
            "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch",
            "hits": 233
        },
        {
            "id": 14753,
            "url": "https://svs.gsfc.nasa.gov/14753/",
            "result_type": "Produced Video",
            "release_date": "2025-01-13T10:14:00-05:00",
            "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole",
            "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ",
            "hits": 180
        },
        {
            "id": 14744,
            "url": "https://svs.gsfc.nasa.gov/14744/",
            "result_type": "Produced Video",
            "release_date": "2025-01-03T00:00:00-05:00",
            "title": "GDC and DYNAMIC to Explore Earth’s Upper Atmosphere",
            "description": "Two upcoming missions, the Geospace Dynamics Constellation (GDC) and Dynamical Neutral Atmosphere-Ionosphere Coupling (DYNAMIC) will revolutionize our understanding of Earth’s upper atmosphere. This region includes Earth’s ionosphere, thermosphere, and mesosphere, and stretches from roughly 50 to 400 miles above Earth’s surface. Space weather disturbances can impact communications, navigation signals, and satellite orbits, and induce currents can trigger power outages on Earth — making the region a crucial area of study.GDC is a team of satellites that will study Earth’s upper atmosphere and provide the first direct global measurements of our planet’s dynamic and complex interface with the space environment. Working in tandem with the DYNAMIC spacecraft, scientists will be able paint a fuller picture of how energy transforms and travels throughout the upper atmosphere. GDC will fly at an altitude of 350-400 km.DYNAMIC is a pair of satellites that will work in tandem with GDC to study how changes in Earth’s lower atmosphere influence our planet’s upper atmosphere. Between the multiple spacecraft of GDC and DYNAMIC, simultaneous observations from different locations can give scientists a more complete picture of how atmospheric waves propagate up through this unique part of the atmosphere. DYNAMIC will fly at an altitude of 550-800 km. || ",
            "hits": 185
        },
        {
            "id": 5435,
            "url": "https://svs.gsfc.nasa.gov/5435/",
            "result_type": "Visualization",
            "release_date": "2024-12-12T12:00:00-05:00",
            "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm",
            "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ",
            "hits": 320
        },
        {
            "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": 630
        },
        {
            "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": 65
        },
        {
            "id": 5415,
            "url": "https://svs.gsfc.nasa.gov/5415/",
            "result_type": "Visualization",
            "release_date": "2024-11-22T09:00:00-05:00",
            "title": "Moon Phase and Libration, 2025",
            "description": "The geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2025, at hourly intervals.",
            "hits": 4549
        },
        {
            "id": 5416,
            "url": "https://svs.gsfc.nasa.gov/5416/",
            "result_type": "Visualization",
            "release_date": "2024-11-22T09:00:00-05:00",
            "title": "Moon Phase and Libration, 2025 South Up",
            "description": " || The data in the table for all of 2025 can be downloaded as a JSON file or as a text file. || ",
            "hits": 535
        },
        {
            "id": 14719,
            "url": "https://svs.gsfc.nasa.gov/14719/",
            "result_type": "Visualization",
            "release_date": "2024-11-13T09:00:00-05:00",
            "title": "Swift Studies Gas-Churning Monster Black Holes",
            "description": "Watch as a gas cloud encounters two supermassive black holes. The complex interplay of gravitational and frictional forces causes the cloud to condense and heat. Some of the gas is ejected from the system with each orbit of the black holes.Credit: F. Goicovic et al. 2016Music: \"Forgotten Fortunes,\" Magnum Opus [ASCAP] , Universal Production MusicComplete transcript available. || Sim_Video_Still.jpg (3840x2160) [744.6 KB] || Sim_Video_Still_searchweb.png (320x180) [37.6 KB] || Sim_Video_Still_thm.png (80x40) [3.4 KB] || BH_Binary_TD_Sim_1080_Final.mp4 (1920x1080) [38.5 MB] || BH_Binary_TD_Sim_4k_Final.mp4 (3840x2160) [45.5 MB] || BH_Binary_TD_Sim_4k_Final_best.mp4 (3840x2160) [67.9 MB] || 14719_BinaryBHTDE_Captions.en_US.srt [57 bytes] || 14719_BinaryBHTDE_Captions.en_US.vtt [67 bytes] || BH_Binary_TD_Sim_4k_Final_ProRes.mov (3840x2160) [1.5 GB] || ",
            "hits": 145
        },
        {
            "id": 5405,
            "url": "https://svs.gsfc.nasa.gov/5405/",
            "result_type": "Visualization",
            "release_date": "2024-10-11T00:00:00-04:00",
            "title": "TROPICS Monitors Milton",
            "description": "Hurricane Milton transversing through the Gulf of Mexico, starting October 5, 2024 through October 9, 2024 when it made landfall along the western Florida coast. || Milton_v02_2024-10-11_1120.02500_print.jpg (1024x576) [132.9 KB] || Milton_v02_2024-10-11_1120.02500_searchweb.png (320x180) [85.7 KB] || Milton_v02_2024-10-11_1120.02500_thm.png (80x40) [6.6 KB] || Milton_v02_2024-10-11_1120.mp4 (1920x1080) [12.4 MB] || 1920x1080_16x9_30p [0 Item(s)] || Milton_v02_2024-10-11_1120.webm (1920x1080) [2.9 MB] || tropics-monitors-milton.hwshow || ",
            "hits": 22
        },
        {
            "id": 14677,
            "url": "https://svs.gsfc.nasa.gov/14677/",
            "result_type": "Produced Video",
            "release_date": "2024-10-02T10:00:00-04:00",
            "title": "NASA's TESS Spots Record-breaking Stellar Triplets",
            "description": "This artist’s concept illustrates how tightly the three stars in the system called TIC 290061484 orbit each other. If they were placed at the center of our solar system, all the stars’ orbits would be contained a space smaller than Mercury’s orbit around the Sun. The sizes of the triplet stars and the Sun are also to scale.Credit: NASA’s Goddard Space Flight Center || TESS_Triple_system_beauty_scale.jpg (3840x2160) [775.5 KB] || ",
            "hits": 479
        },
        {
            "id": 14681,
            "url": "https://svs.gsfc.nasa.gov/14681/",
            "result_type": "Produced Video",
            "release_date": "2024-10-01T11:00:00-04:00",
            "title": "Launch Your Creativity with Space Crafts",
            "description": "In honor of the completion of our Nancy Grace Roman Space Telescope’s spacecraft — the vehicle that will maneuver the observatory to its place in space and enable it to function once there — we’re bringing you some space crafts you can complete at home! || ",
            "hits": 77
        },
        {
            "id": 5390,
            "url": "https://svs.gsfc.nasa.gov/5390/",
            "result_type": "Visualization",
            "release_date": "2024-09-27T00:00:00-04:00",
            "title": "TROPICS Tracks Hurricane Helene",
            "description": "This data visualization shows TROPICS tracking Hurricane Helene throughout most of its life cycle. On September 27th Helene rapidly intensified to a category 4 hurricane before making landfall on the Florida bend. Although weakened after landfall it was still a category 1 hurricane as it hit Georgia and a Tropical Strom over western North Carolina. || Helene0927_v93_2024-10-01_1139.02900_print.jpg (1024x576) [125.4 KB] || Helene0927_v93_2024-10-01_1139.02900_searchweb.png (320x180) [81.2 KB] || Helene0927_v93_2024-10-01_1139.02900_thm.png (80x40) [6.2 KB] || Helene0927_v93_2024-10-01_1139.mp4 (1920x1080) [17.4 MB] || final [0 Item(s)] || ",
            "hits": 98
        },
        {
            "id": 31306,
            "url": "https://svs.gsfc.nasa.gov/31306/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-08-28T00:00:00-04:00",
            "title": "CYGNSS Wind Speed",
            "description": "Animation of wind speed || cygnss_wind_speed_20240220_print.jpg (1024x576) [268.7 KB] || cygnss_wind_speed_20240220_searchweb.png (320x180) [75.5 KB] || cygnss_wind_speed_20240220_thm.png (80x40) [8.5 KB] || cygnss_wind_speed_20240220.tif (1920x1080) [2.4 MB] || cygnss_wind_speed_1080p30.webm (1920x1080) [57.1 MB] || cygnss_wind_speed_1080p30.mp4 (1920x1080) [409.7 MB] || cygnss_wind_speed.hwshow [204 bytes] || ",
            "hits": 55
        },
        {
            "id": 31307,
            "url": "https://svs.gsfc.nasa.gov/31307/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-08-28T00:00:00-04:00",
            "title": "CYGNSS Soil Moisture",
            "description": "Animation of soil moisture || cygnss_soil_moisture_20240609_print.jpg (1024x576) [148.5 KB] || cygnss_soil_moisture_20240609_searchweb.png (320x180) [45.0 KB] || cygnss_soil_moisture_20240609_thm.png (80x40) [7.4 KB] || cygnss_soil_moisture_20240609.tif (1920x1080) [1.0 MB] || cygnss_soil_moisture_1080p30.webm (1920x1080) [17.5 MB] || cygnss_soil_moisture_1080p30.mp4 (1920x1080) [101.8 MB] || cygnss_soil_moisture.hwshow [210 bytes] || ",
            "hits": 46
        },
        {
            "id": 5362,
            "url": "https://svs.gsfc.nasa.gov/5362/",
            "result_type": "Visualization",
            "release_date": "2024-08-23T00:00:00-04:00",
            "title": "TROPICS Tracks Hurricane Debby",
            "description": "This data visualization starts by showing the constellation of cubesats that make up the TROPICS mission collecting data across the globe. The camera then pushes in tighter to show Tropical Depression Debby over Haiti. We then follow Debby's path over Cuba as it begins to organize into a Tropical Storm. It then strengthens to a category 1 hurricane in the Gulf of Mexico right before hitting Florida, where it quickly weakens back into a Tropical Storm. It then slowly moves over Georgia and South Carolina flooding both those states. || tropics_debbyL1c_v90_2024-08-15_1016.02928_print.jpg (1024x576) [146.7 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_searchweb.png (320x180) [86.0 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_thm.png (80x40) [6.4 KB] || tropics_debbyL1c_v90_2024-08-15_1016_1080p30.mp4 (1920x1080) [31.8 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4 (3840x2160) [94.7 MB] || 3840x2160_16x9_30p [0 Item(s)] || tropics_debbyL1c_v90_2024-08-15_1016.webm (3840x2160) [20.4 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4.hwshow || ",
            "hits": 42
        },
        {
            "id": 31304,
            "url": "https://svs.gsfc.nasa.gov/31304/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-08-06T00:00:00-04:00",
            "title": "Take a Cosmic Road Trip this Summer with Chandra and Webb",
            "description": "Images combining data from NASA’s Chandra and Webb telescopes, of a cloud complex, a region of star formation, a spiral galaxy, and a galaxy cluster. || chandrawebb3-hw_print.jpg (1024x576) [176.0 KB] || chandrawebb3-hw_searchweb.png (320x180) [65.0 KB] || chandrawebb3-hw_thm.png (80x40) [6.0 KB] || chandrawebb3-hw.tif (5760x3240) [53.4 MB] || take-a-cosmic-road-trip-this-summer-with-chandra-and-webb.hwshow [311 bytes] || ",
            "hits": 65
        },
        {
            "id": 5331,
            "url": "https://svs.gsfc.nasa.gov/5331/",
            "result_type": "Visualization",
            "release_date": "2024-07-24T00:00:00-04:00",
            "title": "Hurricane Beryl via TROPICS",
            "description": "Animation starts with the orbiting constellation of satellites known as TROPICS. As soon as Hurricane Beryl appears, the camera zooms in closer to watch the storm develop as the TROPICS satellites capture the evolving storm with each swath pass. || tropics_beryl_v75_2024-07-12_1732.02650_print.jpg (1024x576) [146.0 KB] || tropics_beryl_v75_2024-07-12_1732.02650_searchweb.png (320x180) [83.3 KB] || tropics_beryl_v75_2024-07-12_1732.02650_thm.png (80x40) [6.5 KB] || tropics_beryl_v75_2024-07-12_1732.mp4 (1920x1080) [34.3 MB] || 1920x1080_16x9_30p [0 Item(s)] || tropics_beryl_v75_2024-07-12_1732.webm (1920x1080) [7.1 MB] || tropics_beryl_v75_2024-07-12_1732.hwshow [508 bytes] || ",
            "hits": 23
        },
        {
            "id": 31288,
            "url": "https://svs.gsfc.nasa.gov/31288/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-06-13T00:00:00-04:00",
            "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A",
            "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ",
            "hits": 316
        },
        {
            "id": 31290,
            "url": "https://svs.gsfc.nasa.gov/31290/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-06-13T00:00:00-04:00",
            "title": "Webb and Hubble's Views of Spiral Galaxy NGC 628",
            "description": "animated comparison || NGC_628-HST_Webb-1080p.00001_print.jpg (1024x576) [334.0 KB] || NGC_628-HST_Webb-1080p.mp4 (1920x1080) [58.7 MB] || NGC_628-HST_Webb-4k.mp4 (3840x2160) [221.7 MB] || webb-and-hubbles-views-of-spiral-galaxy-ngc-628-4k-movie.hwshow [350 bytes] || ",
            "hits": 357
        },
        {
            "id": 31292,
            "url": "https://svs.gsfc.nasa.gov/31292/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-06-13T00:00:00-04:00",
            "title": "Webb Probes an Extreme Starburst Galaxy",
            "description": "Starburst galaxy M82 was observed by the Hubble Space Telescope in 2006, which showed the galaxy’s edge-on spiral disk, shredded clouds, and hot hydrogen gas. The James Webb Space Telescope has observed M82’s core, capturing in unprecedented detail the structure of the galactic wind and characterizing individual stars and star clusters.The Webb image is from the telescope’s NIRCam (Near-Infrared Camera) instrument. The red filaments trace the shape of the cool component of the galactic wind via polycyclic aromatic hydrocarbons (PAHs). PAHs are very small dust grains that survive in cooler temperatures but are destroyed in hot conditions. The structure of the emission is similar to that of the ionized gas, suggesting PAHs may be replenished from cooler molecular material as it is ionized. || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_print.jpg (1024x576) [178.7 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw.png (3840x2160) [10.9 MB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_searchweb.png (320x180) [74.1 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset-hw_thm.png (80x40) [5.4 KB] || STScI-01HRD1Z19WZYMNB8J1BNVSS1HE-inset.png (16260x7030) [87.9 MB] || webb-probes-an-extreme-starburst-galaxy-hst-v-webb.hwshow [356 bytes] || ",
            "hits": 59
        },
        {
            "id": 14581,
            "url": "https://svs.gsfc.nasa.gov/14581/",
            "result_type": "Produced Video",
            "release_date": "2024-05-23T10:00:00-04:00",
            "title": "Gliese 12 b: An Intriguing World Sized Between Earth and Venus",
            "description": "Gliese 12 b’s estimated size may be as large as Earth or slightly smaller — comparable to Venus in our solar system. This artist’s concept compares Earth with different possible Gliese 12 b interpretations, from no atmosphere to a thick Venus-like one. Follow-up observations with NASA’s James Webb Space Telescope will help determine just how much atmosphere the planet retains as well as its composition.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Alt text: Illustration of Earth compared to various models of Gliese 12 b Image description: At left, against a black background, floats an artist's concept of a nearly half-illuminated Earth, with clouds, blue oceans, and land areas rendered in green, tan, brown, and white. At right are three similarly illuminated planets, slightly smaller than Earth and each representing a possible interpretation of Gliese 12 b. The version on the left has a surface of blotchy reddish and brownish features and no atmosphere. The middle version has the same surface texture partly obscured by a hazy atmosphere. And the rightmost and smallest version of the planet has a thick, Venus-like atmosphere that obscures the surface completely. || Gl12b_Earth_Comparison_ac.jpg (3840x2160) [935.8 KB] || Gl12b_Earth_Comparison_ac_print.jpg (1024x576) [126.0 KB] || Gl12b_Earth_Comparison.jpg (3840x2160) [929.5 KB] || Gl12b_Earth_Comparison_ac_searchweb.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_web.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_thm.png (80x40) [9.8 KB] || Gl12b_Earth_Comparison.tif (3840x2160) [6.4 MB] || ",
            "hits": 489
        },
        {
            "id": 31283,
            "url": "https://svs.gsfc.nasa.gov/31283/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-05-22T00:00:00-04:00",
            "title": "Webb Space Telescope View of the Horsehead Nebula",
            "description": "Horsehead Nebula (Euclid, Hubble and Webb images) || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3.png (8983x3530) [35.2 MB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_print.jpg (1024x402) [143.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_searchweb.png (320x180) [90.1 KB] || STScI-01HV6QEKG49SGS0JAAC3KQ3CGW-horsehead-x3_thm.png (80x40) [15.8 KB] || ",
            "hits": 80
        },
        {
            "id": 14590,
            "url": "https://svs.gsfc.nasa.gov/14590/",
            "result_type": "Produced Video",
            "release_date": "2024-05-14T09:55:00-04:00",
            "title": "Webb Captures New Views Of The Horsehead Nebula",
            "description": "Astronomers have used NASA’s James Webb Space Telescope to survey the Horsehead Nebula in incredible detail.The Horsehead Nebula is an iconic area in the constellation Orion where massive stars are being born.Combining views from many telescopes allows astronomers to understand the inner workings of this nebula like never before. From Euclid, to Hubble, and now Webb, we can learn more about our universe thanks to these amazing machines.For more information, visit https://webb.nasa.gov/. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Liz Landau: ScriptIsabelle Yan: ProducerImage: NASA, ESA, CSA, STScIMusic Credit:\"Ambition\" by Baxter Jervis [ASCAP] via Atmosphere Music Ltd. [PRS], and Universal Production Music. || ",
            "hits": 52
        },
        {
            "id": 14584,
            "url": "https://svs.gsfc.nasa.gov/14584/",
            "result_type": "Produced Video",
            "release_date": "2024-05-08T09:00:00-04:00",
            "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy",
            "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ",
            "hits": 147
        },
        {
            "id": 14522,
            "url": "https://svs.gsfc.nasa.gov/14522/",
            "result_type": "Produced Video",
            "release_date": "2024-04-16T12:00:00-04:00",
            "title": "Fermi Sees No Gamma Rays from Nearby Supernova",
            "description": "Even when it doesn’t detect gamma rays, NASA’s Fermi Gamma-ray Space Telescope helps astronomers learn more about the universe.Credit: NASA’s Goddard Space Flight CenterMusic: \"Trial\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Fermi_Missing_GR_Still.jpg (1920x1080) [757.8 KB] || Fermi_Missing_GR_Still_searchweb.png (320x180) [86.6 KB] || Fermi_Missing_GR_Still_thm.png (80x40) [6.5 KB] || 14522_Fermi_Missing_GammaRays_Captions.en_US.srt [3.4 KB] || 14522_Fermi_Missing_GammaRays_Captions.en_US.vtt [3.2 KB] || 14522_Fermi_Missing_GammaRays_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 14522_Fermi_Missing_GammaRays_Good.mp4 (1920x1080) [110.3 MB] || 14522_Fermi_Missing_GammaRays_Best.mp4 (1920x1080) [382.1 MB] || ",
            "hits": 133
        },
        {
            "id": 14561,
            "url": "https://svs.gsfc.nasa.gov/14561/",
            "result_type": "Produced Video",
            "release_date": "2024-04-03T09:55:00-04:00",
            "title": "NASA's Webb Probes an Extreme Starburst Galaxy",
            "description": "A team of astronomers has used NASA’s James Webb Space Telescope to survey the starburst galaxy Messier 82 (M82). Located 12 million light-years away in the constellation Ursa Major, this galaxy is relatively compact in size but hosts a frenzy of star formation activity. For comparison, M82 is sprouting new stars 10 times faster than the Milky Way galaxy.Using Webb to Inspect the activity in galaxies like these can deepen astronomers’ understanding of the early universe by getting a closer look at the physical conditions that foster the formation of new stars.For more information, visit https://webb.nasa.gov/. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Isabelle Yan: ProducerDr. Stefanie N Milam: VoiceoverThaddeus Cesari: ScriptAbigail Major, STScI: ScriptImage: NASA, ESA, CSA, STScIMusic Credit:\"A Simpler Time\" by Oskari Nurminen [ASCAP] via Universal Publishing Prod. Music Nordic [STIM], and Universal Production Music. || ",
            "hits": 41
        },
        {
            "id": 14515,
            "url": "https://svs.gsfc.nasa.gov/14515/",
            "result_type": "Produced Video",
            "release_date": "2024-02-01T09:55:00-05:00",
            "title": "Sonification of the Mice Galaxies",
            "description": "The Mice Galaxies are a colliding pair of galaxies, that will eventually merge into a single galaxy. They’re located about 300 million light-years away in the constellation Coma Berenices. In this data sonification, scientists represented brightness with volume and pitch – brighter light is louder and lower pitched. The vertical position of objects in the image is used to control the pitch of sustained musical strings, and cymbals swell following the brightness of the galaxy cores. Listen for a cymbal crash played for the foreground star with diffraction spikes, too! Credit: NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M. Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA; Sonification: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ",
            "hits": 52
        },
        {
            "id": 14504,
            "url": "https://svs.gsfc.nasa.gov/14504/",
            "result_type": "Produced Video",
            "release_date": "2024-01-29T10:00:00-05:00",
            "title": "Hubble's Inside the Image: Antennae Galaxies",
            "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of the Antennae Galaxies.The Antennae Galaxies, officially designated as NGC 4038 and NGC 4039, present a celestial ballet within the vast cosmic theater. Located approximately 68 million light-years away in the Corvus constellation, these interacting galaxies are entangled in a cosmic dance, their long tidal tails resembling the antennae of an insect, hence their name.In this video, Dr. Jennifer Wiseman explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. ChristensenMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production MusicPREMIUM BEAT BY SHUTTERSTOCKThe Search by Northern Points || ",
            "hits": 81
        },
        {
            "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": 193
        },
        {
            "id": 14498,
            "url": "https://svs.gsfc.nasa.gov/14498/",
            "result_type": "Produced Video",
            "release_date": "2024-01-11T11:05:00-05:00",
            "title": "Finding A New Galactic 'Fossil'",
            "description": "Some 5 million years ago, a black hole eruption in the galaxy NGC 4945 set off a star-formation frenzy and shot a vast cloud of gas into intergalactic space. Watch and learn how two X-ray telescopes revealed the story.Music Credits: Universal Production Music\"Planetary Horizons\" by Jia Lee\"Eyes Peeled\" by Bard\"Sprinkle of Mischief\" by Ash and HaroldWatch this video on the NASA Goddard YouTube channel.Credit: NASA’s Goddard Space Flight Center",
            "hits": 124
        },
        {
            "id": 14499,
            "url": "https://svs.gsfc.nasa.gov/14499/",
            "result_type": "Produced Video",
            "release_date": "2024-01-05T11:00:00-05:00",
            "title": "Hubble’s Inside The Image: Abell 2744",
            "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of Abell 2744.Abell 2744, known as Pandora's Cluster, nestled in the Sculptor constellation, emerges as a celestial marvel. This cosmic spectacle showcases an intricate dance of galaxies, clusters, and dark matter, captivating astronomers and enthusiasts alike.In this video, Dr. Brian Welch explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. Christensen Hubble Space Eclipsing The Sun Animation:ESA/Hubble - M. Kornmesser Animation of Galaxy Cluster With Gravitational LensingESA/Hubble - L. Calçada Artist’s Impression of Gravitational Lensing:ESA/Hubble - M. KornmesserMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music\"Frozen Waves Instrumental\" by Matthew Nicholson [PRS], and Suki Jeanette Finn [PRS] via Universal Production Music || ",
            "hits": 29
        },
        {
            "id": 14493,
            "url": "https://svs.gsfc.nasa.gov/14493/",
            "result_type": "Produced Video",
            "release_date": "2024-01-05T09:55:00-05:00",
            "title": "Hubble’s Inside The Image: The Eagle Nebula",
            "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of The Pillars of Creation.The Pillars of Creation in the Eagle Nebula, situated in the Serpens constellation, stand as celestial marvels. Composed of interstellar gas and dust, these towering structures captivate astronomers and stargazers alike. Shaped by the potent forces of stellar winds and radiation, the pillars, resembling cosmic sentinels, showcase vibrant hues. Functioning as crucibles for stellar birth, they facilitate the creation of new stars in a delicate dance of destruction and formation. The Pillars of Creation in the Eagle Nebula offer a captivating spectacle, inviting observers to contemplate the profound dynamics at play within our ever-evolving cosmic tapestry.In this video, Dr. Jennifer Wiseman explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationESA/Hubble (M. Kornmesser & L. L. Christensen) Light Echo AnimationNASA/ESA/Hubble - M. KornmesserMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music. || ",
            "hits": 106
        },
        {
            "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": 145
        },
        {
            "id": 14458,
            "url": "https://svs.gsfc.nasa.gov/14458/",
            "result_type": "Produced Video",
            "release_date": "2023-12-17T09:55:00-05:00",
            "title": "Hubble’s Inside The Image: RS Puppis",
            "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of RS Puppis.RS Puppis is a remarkable and highly luminous Cepheid variable star located in the constellation Puppis, known for its regular pulsations and dramatic changes in brightness.In this video, Dr. Padi Boyd explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationESA/Hubble (M. Kornmesser & L. L. Christensen) Light Echo AnimationNASA/ESA/Hubble - M. KornmesserMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music. || ",
            "hits": 58
        },
        {
            "id": 20388,
            "url": "https://svs.gsfc.nasa.gov/20388/",
            "result_type": "Animation",
            "release_date": "2023-12-05T14:00:00-05:00",
            "title": "PUNCH Spacecraft Beauty Passes",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in Sun-synchronous, low Earth orbit that will make global, 3D observations of the young solar wind, from the outermost solar atmosphere to the inner heliopshere. Images of unprecedented quality will help to close a 60-year gap in measurements of understanding of what occurs in this region of space. PUNCH will share a ride to space with NASA’s Jet Propulsion Laboratory’s Spectro-Photometer for the History of the Universe, Epoch of Re-ionization, and Ices Explorer (SPHEREx) mission. The missions launched on March 11, 2025, on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.Get the latest updates on NASA's PUNCH blog. || ",
            "hits": 63
        },
        {
            "id": 31267,
            "url": "https://svs.gsfc.nasa.gov/31267/",
            "result_type": "Hyperwall Visual",
            "release_date": "2023-11-28T00:00:00-05:00",
            "title": "Landsat and Sentinel NDVI, 2022",
            "description": "The Harmonized Landsat and Sentinel-2 (HLS) project is a NASA initiative aiming to produce a seamless surface reflectance record from the Operational Land Imager (OLI) and Multi-Spectral Instrument (MSI) aboard Landsat-8/9 and Sentinel-2A/B remote sensing satellites, respectively. These animations show a year's worth of HLS data near Columbus, Nebraska from 2022. One animation includes the cloudy scenes and the other has cloud-free or mostly cloud-free scenes. ||",
            "hits": 179
        },
        {
            "id": 5187,
            "url": "https://svs.gsfc.nasa.gov/5187/",
            "result_type": "Visualization",
            "release_date": "2023-11-16T08:00:00-05:00",
            "title": "Moon Phase and Libration, 2024",
            "description": " || The data in the table for all of 2024 can be downloaded as a JSON file or as a text file. || moon.0001.jpg (730x730) [87.6 KB] || comp.0001.tif (5760x3240) [14.8 MB] || ",
            "hits": 1382
        },
        {
            "id": 5188,
            "url": "https://svs.gsfc.nasa.gov/5188/",
            "result_type": "Visualization",
            "release_date": "2023-11-16T08:00:00-05:00",
            "title": "Moon Phase and Libration, 2024 South Up",
            "description": " || The data in the table for all of 2024 can be downloaded as a JSON file or as a text file. || moon.0001.jpg (730x730) [87.3 KB] || comp.0001.tif (5760x3240) [15.0 MB] || ",
            "hits": 208
        },
        {
            "id": 40509,
            "url": "https://svs.gsfc.nasa.gov/gallery/earth-now-dashboard/",
            "result_type": "Gallery",
            "release_date": "2023-10-16T00:00:00-04:00",
            "title": "Earth Now Dashboard",
            "description": "NASA satellites provide data on Earth's land, ecosystems, water, air temperature, and climate - and have done so for more than 50 years. Earth information from space supports decision makers, partners, and people in developing the tools they need to mitigate, adapth, and respond to our changing planet.\n\nThe visualizations featured on this dashboard show the latest imagery available.\n\n\n\n\n\n\n\n",
            "hits": 154
        },
        {
            "id": 5147,
            "url": "https://svs.gsfc.nasa.gov/5147/",
            "result_type": "Visualization",
            "release_date": "2023-09-26T17:00:00-04:00",
            "title": "GEOS-FP Near-Surface Temperature",
            "description": "Near-surface temperature is calculated by sampling 3-D atmospheric fields from NASA’s GEOS-FP system 3 meters above Earth’s surface. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.",
            "hits": 95
        },
        {
            "id": 5148,
            "url": "https://svs.gsfc.nasa.gov/5148/",
            "result_type": "Visualization",
            "release_date": "2023-09-26T17:00:00-04:00",
            "title": "GEOS-FP Near-Surface Wind Speed",
            "description": "Near-surface wind speed is calculated by sampling 3-D atmospheric fields from NASA’s GEOS-FP system 10 meters above Earth’s surface. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.",
            "hits": 109
        },
        {
            "id": 5149,
            "url": "https://svs.gsfc.nasa.gov/5149/",
            "result_type": "Visualization",
            "release_date": "2023-09-26T17:00:00-04:00",
            "title": "GEOS-FP Precipitation and Clouds",
            "description": "Precipitation and clouds are calculated using fields from NASA’s GEOS-FP system. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions, which can be used to estimate the formation of clouds along with rain and snowfall.",
            "hits": 90
        },
        {
            "id": 5150,
            "url": "https://svs.gsfc.nasa.gov/5150/",
            "result_type": "Visualization",
            "release_date": "2023-09-26T17:00:00-04:00",
            "title": "GEOS-FP Near-Surface Humidity",
            "description": "Near-surface Humidity, also known as specific humidity (Q2M) from NASA’s GEOS-FP system. GEOS-FP combines millions of weather observations with a predictive model to create a global best estimate of weather conditions that are used to begin a forecast.",
            "hits": 115
        },
        {
            "id": 14408,
            "url": "https://svs.gsfc.nasa.gov/14408/",
            "result_type": "Produced Video",
            "release_date": "2023-09-07T11:00:00-04:00",
            "title": "Swift Spots a Snacking Black Hole Using a New Trick",
            "description": "Watch to learn how an update to NASA’s Neil Gehrels Swift Observatory allowed it to catch a supersized black hole in a distant galaxy munching repeatedly on a circling star. Credit: NASA’s Goddard Space Flight CenterMusic: \"Teapot Waltz\" by Benjamin Parsons from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Repeating_TDE_Still.jpg (1920x1080) [446.8 KB] || Repeating_TDE_Still_searchweb.png (320x180) [63.3 KB] || Repeating_TDE_Still_thm.png (80x40) [4.6 KB] || 14408_Repeating_TDE_sub100.mp4 (1920x1080) [89.7 MB] || Repeating_TDE_SRT_Captions.en_US.srt [1.7 KB] || Repeating_TDE_SRT_Captions.en_US.vtt [1.6 KB] || 14408_Repeating_TDE_ProRes_1920x1080_2997.mov (1920x1080) [1.2 GB] || 14408_Repeating_TDE_1080.mp4 (1920x1080) [186.2 MB] || ",
            "hits": 79
        },
        {
            "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": 978
        },
        {
            "id": 14379,
            "url": "https://svs.gsfc.nasa.gov/14379/",
            "result_type": "Produced Video",
            "release_date": "2023-06-29T13:00:00-04:00",
            "title": "Landsat Next Defined",
            "description": "Landsat Next is on the horizon—the new mission will not only ensure continuity of the longest space-based record of Earth’s land surface, it will fundamentally transform the breadth and depth of actionable information freely available to end users. || LNext_Thumb.png (1280x720) [553.8 KB] || LNext_JPG.png (1280x720) [553.8 KB] || NASA_LNext_Final.02354_print.jpg (1024x576) [75.2 KB] || NASA_LNext_Final.02354_searchweb.png (320x180) [49.6 KB] || NASA_LNext_Final.mp4 (1920x1080) [1.5 GB] || NASA_LNext_Final.webm (1920x1080) [86.7 MB] || LandsatNext.en_US.srt [20.8 KB] || LandsatNext.en_US.vtt [19.8 KB] || ",
            "hits": 71
        },
        {
            "id": 40484,
            "url": "https://svs.gsfc.nasa.gov/gallery/nasaand-agriculture/",
            "result_type": "Gallery",
            "release_date": "2023-06-08T00:00:00-04:00",
            "title": "NASA and Agriculture Video",
            "description": "The farmers responsible for the food that reaches your plate need a lot of a very precious and limited resource, water. NASA works with farmers like Dwane Roth of Kansas to help them track their water use. Roth says that farmers like him are seeing more frequent, hotter days with less rain. “We need to grow more with less and get as much out of each drop of water we can,” he says. NASA helps to promote the use of Earth observations to strengthen food security. One solution is OpenET, a system that puts near-real-time water data into the hands of farmers in the United States.",
            "hits": 123
        },
        {
            "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": 64
        },
        {
            "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": 126
        },
        {
            "id": 14287,
            "url": "https://svs.gsfc.nasa.gov/14287/",
            "result_type": "Produced Video",
            "release_date": "2023-03-16T14:00:00-04:00",
            "title": "Hubble’s Inside The Image: Crab Nebula",
            "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking Crab Nebula.With an apparent magnitude of 8.4 and located 6,500 light-years from Earth in the constellation Taurus, the Crab Nebula can be spotted with a small telescope and is best observed in January. The nebula was discovered by English astronomer John Bevis in 1731, and later observed by Charles Messier who mistook it for Halley’s Comet. Messier’s observation of the nebula inspired him to create a catalog of celestial objects that might be mistaken for comets.In this video, Dr. Padi Boyd takes us on a journey through the Nebula, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSF. Crab Nebula Zoom VisualizationCredit: ESA/Hubble, Digitized Sky Survey, Nick Risinger (skysurvey.org) Dark Matter Gravitational Lensing AnimationCredit: NASA's Goddard Space Flight Center Conceptual Image LabMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Night Call” by Timothy Paul Handels [SABAM] via Pedigree Cuts [PRS] and Universal Production Music || ",
            "hits": 50
        },
        {
            "id": 14312,
            "url": "https://svs.gsfc.nasa.gov/14312/",
            "result_type": "Produced Video",
            "release_date": "2023-03-16T12:00:00-04:00",
            "title": "NASA Tracks Freddy, Longest-lived Tropical Cyclone on Record",
            "description": "Music: \"Enlightenment,\" Universal Production MusicComplete transcript available.Video Descriptive Text available. || Freddy_thumb.png (1720x941) [2.8 MB] || Freddy_thumb_print.jpg (1024x560) [181.6 KB] || Freddy_thumb_searchweb.png (180x320) [115.5 KB] || Freddy_thumb_thm.png (80x40) [10.8 KB] || TC_Freddy_prores.webm (1920x1080) [8.2 MB] || Freddy.en_US.srt [2.7 KB] || Freddy.en_US.vtt [2.6 KB] || TC_Freddy.mp4 (1920x1080) [99.7 MB] || TC_Freddy_prores.mov (1920x1080) [1.4 GB] || ",
            "hits": 180
        },
        {
            "id": 14264,
            "url": "https://svs.gsfc.nasa.gov/14264/",
            "result_type": "Produced Video",
            "release_date": "2023-01-10T13:00:00-05:00",
            "title": "TESS Finds System’s Second Earth-Size World",
            "description": "Watch to learn about TOI 700 e, a newly discovered Earth-size planet with an Earth-size sibling. Credit: NASA/JPL-Caltech/Robert Hurt/NASA’s Goddard Space Flight CenterMusic Credit: Dream Box by Carl David HarmsWatch this video on the NASA Goddard YouTube channel. || Title_Card_TOI700_e.jpg (1920x1080) [1.2 MB] || Second_Habitable_World_in_TOI700.00250_print.jpg (1024x576) [50.0 KB] || Second_Habitable_World_in_TOI700.00250_searchweb.png (320x180) [50.3 KB] || Second_Habitable_World_in_TOI700.00250_thm.png (80x40) [3.4 KB] || Second_Habitable_World_in_TOI700.mp4 (1920x1080) [69.1 MB] || Second_Habitable_World_in_TOI700.webm (1920x1080) [7.7 MB] || Second_Habitable_World_in_TOI700_ProRes.mov (1920x1080) [948.8 MB] || Second_Habitable_World_in_TOI700.en_US.srt [1.1 KB] || Second_Habitable_World_in_TOI700.en_US.vtt [1.1 KB] || ",
            "hits": 596
        },
        {
            "id": 14255,
            "url": "https://svs.gsfc.nasa.gov/14255/",
            "result_type": "Produced Video",
            "release_date": "2022-12-07T11:00:00-05:00",
            "title": "NASA’s Fermi, Swift Capture Revolutionary Gamma-Ray Burst",
            "description": "Watch to learn how an event called GRB 211211A rocked scientists’s understanding of gamma-ray bursts – the most powerful explosions in the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic Credits: \"Finished Plate\" by Airglo and \"Binary Fission\" by Tom KaneWatch this video on the NASA Goddard YouTube channel. || Title_Card_Revolutionary_GRB.jpg (1920x1080) [1.5 MB] || Title_Card_Revolutionary_GRB_searchweb.png (320x180) [100.7 KB] || Title_Card_Revolutionary_GRB_thm.png (80x40) [7.3 KB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.mp4 (1920x1080) [171.9 MB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst_ProRes.mov (1920x1080) [2.2 GB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.webm (1920x1080) [18.4 MB] || Long_GRB_Captions.en_US.srt [2.8 KB] || Long_GRB_Captions.en_US.vtt [2.8 KB] || ",
            "hits": 155
        },
        {
            "id": 5048,
            "url": "https://svs.gsfc.nasa.gov/5048/",
            "result_type": "Visualization",
            "release_date": "2022-11-09T13:00:00-05:00",
            "title": "Moon Phase and Libration, 2023",
            "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) ||  || ",
            "hits": 1012
        },
        {
            "id": 5049,
            "url": "https://svs.gsfc.nasa.gov/5049/",
            "result_type": "Visualization",
            "release_date": "2022-11-09T13:00:00-05:00",
            "title": "Moon Phase and Libration, 2023 South Up",
            "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) ||  || ",
            "hits": 153
        },
        {
            "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": 329
        },
        {
            "id": 5021,
            "url": "https://svs.gsfc.nasa.gov/5021/",
            "result_type": "Visualization",
            "release_date": "2022-10-11T00:00:00-04:00",
            "title": "NOAA-21, NOAA-20, and Suomi NPP satellite orbits",
            "description": "This short animation shows the orbits of JPSS-2 (NOAA-21), NOAA-20, and Suomi-NPP, after JPSS-2 is fully commissioned and all science products are provisional, notionally a year after its 2022 launch. When the JPSS-2 satellite reaches polar orbit, it will be renamed NOAA-21. NOAA-21 will provide the same observations as its sister satellites, NOAA-20 and Suomi-NPP. Once fully operational NOAA plans to place NOAA-21 in a quarter orbit ahead of Suomi-NPP, and NOAA 20 will be a quarter orbit behind SNPP. || JPSS2-NOAA20-SNPP.2500_print.jpg (1024x576) [77.0 KB] || JPSS2-NOAA20-SNPP_1080p60.mp4 (1920x1080) [10.0 MB] || JPSS2-NOAA20-SNPP_1080p60.webm (1920x1080) [3.1 MB] || JPSS2-NOAA20-SNPP (3840x2160) [0 Item(s)] || JPSS2-NOAA20-SNPP_2160p60.mp4 (3840x2160) [33.9 MB] || ",
            "hits": 201
        },
        {
            "id": 5032,
            "url": "https://svs.gsfc.nasa.gov/5032/",
            "result_type": "Visualization",
            "release_date": "2022-09-28T14:00:00-04:00",
            "title": "November 8, 2022 Total Lunar Eclipse: Shadow View",
            "description": "Universal Time (UTC). The Moon moves right to left, passing through the penumbra and umbra, leaving in its wake an eclipse diagram with the times at various stages of the eclipse. || shadow_diagram_utc_202211_print.jpg (1024x576) [79.0 KB] || shadow_diagram_utc_202211_searchweb.png (320x180) [44.6 KB] || shadow_diagram_utc_202211_thm.png (80x40) [4.8 KB] || umbracam_utc_202211_1080p30.mp4 (1920x1080) [13.1 MB] || umbracam_utc_202211_720p30.mp4 (1280x720) [7.2 MB] || umbracam_utc_202211_720p30.webm (1280x720) [11.0 MB] || umbracam_utc_202211_2160p30.mp4 (3840x2160) [37.3 MB] || umbracam_utc_202211_360p30.mp4 (640x360) [2.6 MB] || utc (3840x2160) [0 Item(s)] || shadow_diagram_utc_202211.tif (3840x2160) [5.8 MB] || umbracam_utc_202211_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 205
        },
        {
            "id": 5018,
            "url": "https://svs.gsfc.nasa.gov/5018/",
            "result_type": "Visualization",
            "release_date": "2022-09-14T13:00:00-04:00",
            "title": "BAMS Cover: Mapping Global Precipitation",
            "description": "BAMS cover as published, showing the evolution of the coverage of precipitation observations provided by passive microwave satellite sensors from 1985-2015. || Aug22_cover_proof3_print.jpg (1024x1353) [370.4 KB] || Aug22_cover_proof3_searchweb.png (320x180) [88.5 KB] || Aug22_cover_proof3_thm.png (80x40) [7.5 KB] || Aug22_cover_proof3.tiff (2450x3238) [9.8 MB] || ",
            "hits": 26
        },
        {
            "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": 235
        },
        {
            "id": 14157,
            "url": "https://svs.gsfc.nasa.gov/14157/",
            "result_type": "Produced Video",
            "release_date": "2022-05-26T09:00:00-04:00",
            "title": "Sonification of NGC 1300",
            "description": "The majestic spiral galaxy NGC 1300’s arms hold blue clusters of young stars, pink clouds of star formation, and dark lanes of dust. To represent this image with sound, scientists assigned louder volume to brighter light. Light farther from the center is pitched higher as a counterclockwise radar scans across the galaxy. NGC 1300 resides nearly 70 million light-years away in the constellation Eridanus. Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)For more information about the Hubble Space Telescope and its images, visit https://nasa.gov/hubble. || ",
            "hits": 68
        },
        {
            "id": 14148,
            "url": "https://svs.gsfc.nasa.gov/14148/",
            "result_type": "Produced Video",
            "release_date": "2022-05-05T12:45:00-04:00",
            "title": "Magnetic Flip Drives Flare-Up of Monster Black Hole",
            "description": "Explore the unusual eruption of 1ES 1927+654, a galaxy located 236 million light-years away in the constellation Draco. A sudden reversal of the magnetic field around its million-solar-mass black hole may have triggered the outburst.Credit: NASA’s Goddard Space Flight Center Music: \"Water Dance\" and \"Alternate Worlds\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ChangingLookAGN_Still1.jpg (1920x1080) [822.9 KB] || ChangingLookAGN_Still1_searchweb.png (320x180) [79.5 KB] || ChangingLookAGN_Still1_thm.png (80x40) [6.2 KB] || 14148_ChangingLook_AGN_1080.webm (1920x1080) [24.8 MB] || 14148_ChangingLook_AGN_Sub100MB.mp4 (1920x1080) [91.5 MB] || 14148_ChangingLook_AGN_1080.mp4 (1920x1080) [246.5 MB] || 14148_ChangingLook_AGN_Best_1080.mp4 (1920x1080) [534.7 MB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.srt [4.2 KB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.vtt [4.3 KB] || 14148_ChangingLook_AGN_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ",
            "hits": 232
        },
        {
            "id": 4980,
            "url": "https://svs.gsfc.nasa.gov/4980/",
            "result_type": "Visualization",
            "release_date": "2022-03-24T01:02:00-04:00",
            "title": "May 15-16, 2022 Total Lunar Eclipse: Shadow View",
            "description": "Eastern Daylight Time (EDT). The Moon moves right to left, passing through the penumbra and umbra, leaving in its wake an eclipse diagram with the times at various stages of the eclipse. || shadow_diagram_edt_202205_print.jpg (1024x576) [85.9 KB] || moon.2355_searchweb.png (320x180) [48.4 KB] || moon.2355_thm.png (80x40) [5.0 KB] || umbracam_edt_202205_1080p30.mp4 (1920x1080) [12.2 MB] || umbracam_edt_202205_720p30.mp4 (1280x720) [6.7 MB] || umbracam_edt_202205_720p30.webm (1280x720) [9.4 MB] || umbracam_edt_202205_2160p30.mp4 (3840x2160) [35.5 MB] || umbracam_edt_202205_360p30.mp4 (640x360) [2.4 MB] || shadow_diagram_edt_202205.tif (3840x2160) [6.7 MB] || edt (3840x2160) [0 Item(s)] || umbracam_edt_202205_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 114
        },
        {
            "id": 14115,
            "url": "https://svs.gsfc.nasa.gov/14115/",
            "result_type": "Produced Video",
            "release_date": "2022-03-08T13:00:00-05:00",
            "title": "NASA's NICER Tracks a Magnetar's Hot Spots",
            "description": "Explore how NASA’s Neutron star Interior Composition Explorer (NICER) tracked brilliant hot spots on the surface of an erupting magnetar – from 13,000 light-years away. Credit: NASA's Goddard Space Flight CenterMusic: \"Particles and Fields\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_Still.jpg (1920x1080) [574.3 KB] || Magnetar_Still_print.jpg (1024x576) [229.0 KB] || Magnetar_Still_searchweb.png (320x180) [66.1 KB] || Magnetar_Still_thm.png (80x40) [5.2 KB] || 14115_Merging_Magnetar_HotSpots_1080_Best.webm (1920x1080) [17.4 MB] || 14115_Merging_Magnetar_HotSpots_1080.mp4 (1920x1080) [158.9 MB] || 14115_Merging_Magnetar_HotSpots_1080_Best.mp4 (1920x1080) [382.0 MB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.srt [2.1 KB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.vtt [2.1 KB] || 14115_Merging_Magnetar_HotSpots_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || ",
            "hits": 201
        },
        {
            "id": 20345,
            "url": "https://svs.gsfc.nasa.gov/20345/",
            "result_type": "Animation",
            "release_date": "2022-03-01T00:00:00-05:00",
            "title": "TROPICS Mission Animations",
            "description": "The NASA Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats (TROPICS) mission is a constellation of state-of-the-science observing platforms that will measure temperature and humidity soundings and precipitation with spatial resolution comparable to current operational passive microwave sounders but with unprecedented temporal resolution (median revisit time of 50 minutes).Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || Tropics_Beauty_Shot_ProRes.00540_print.jpg (1024x576) [95.4 KB] || Tropics_Beauty_Shot_H264_1080.mp4 (1920x1080) [76.4 MB] || Tropics_Beauty_Shot_H264_1080.webm (1920x1080) [3.4 MB] || Tropics_Beauty_Shot_H264_4k.mp4 (3840x2160) [309.1 MB] || Tropics_Beauty_Shot_ProRes.mov (3840x2160) [3.1 GB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || Tropics_Beauty_Shot_ProRes.webm (3840x2160) [10.3 MB] || ",
            "hits": 36
        },
        {
            "id": 14015,
            "url": "https://svs.gsfc.nasa.gov/14015/",
            "result_type": "Produced Video",
            "release_date": "2021-11-19T09:00:00-05:00",
            "title": "Terra Orbital Drift Video",
            "description": "\"From Small Beginnings,\" by Jay Price [PRS]; Universal Production Music || 14015_4938_TerraDrift_FINAL.02577_print.jpg (1024x576) [113.6 KB] || 14015_4938_TerraDrift_FINAL.02577_searchweb.png (320x180) [53.9 KB] || 14015_4938_TerraDrift_FINAL.02577_thm.png (80x40) [5.2 KB] || 14015_4938_TerraDrift_FINAL.mov (1920x1080) [2.8 GB] || 14015_4938_TerraDrift_FINAL_lowres.mp4 (1280x720) [39.6 MB] || 14015_YOUTUBE_1080_4938_TerraDrift_FINAL_youtube_1080.mp4 (1920x1080) [181.1 MB] || 4938_TerraDrift_FINAL.webm (960x540) [41.8 MB] || 14015_FACEBOOK_720_4938_TerraDrift_FINAL_facebook_720.mp4 (1280x720) [153.7 MB] || 14015_YOUTUBE_4K_4938_TerraDrift_FINAL_youtube_4k.mp4 (3840x2160) [899.2 MB] || 14015_4938_TerraDrift_FINAL.en_US.srt [2.8 KB] || 14015_4938_TerraDrift_FINAL.en_US.vtt [2.7 KB] || ",
            "hits": 154
        },
        {
            "id": 4955,
            "url": "https://svs.gsfc.nasa.gov/4955/",
            "result_type": "Visualization",
            "release_date": "2021-11-18T10:00:00-05:00",
            "title": "Moon Phase and Libration, 2022",
            "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) ||  || ",
            "hits": 954
        },
        {
            "id": 4956,
            "url": "https://svs.gsfc.nasa.gov/4956/",
            "result_type": "Visualization",
            "release_date": "2021-11-18T09:59:00-05:00",
            "title": "Moon Phase and Libration, 2022 South Up",
            "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) ||  || ",
            "hits": 364
        },
        {
            "id": 4953,
            "url": "https://svs.gsfc.nasa.gov/4953/",
            "result_type": "Visualization",
            "release_date": "2021-11-04T12:00:00-04:00",
            "title": "November 19, 2021 <i>Almost</i> Total Lunar Eclipse",
            "description": "The Moon moves right to left, passing through the penumbra and umbra, leaving in its wake an eclipse diagram with the times at various stages of the eclipse. All times are UTC. || moon.1475_print.jpg (1024x576) [66.4 KB] || eclipse_202111_umbra_1080p30.mp4 (1920x1080) [10.1 MB] || eclipse_202111_umbra_720p30.mp4 (1280x720) [5.9 MB] || umbra (1920x1080) [0 Item(s)] || eclipse_202111_umbra_720p30.webm (1280x720) [8.6 MB] || eclipse_202111_umbra_360p30.mp4 (640x360) [2.4 MB] || eclipse_202111_umbra_1080p30.mp4.hwshow [194 bytes] || ",
            "hits": 71
        },
        {
            "id": 13969,
            "url": "https://svs.gsfc.nasa.gov/13969/",
            "result_type": "Produced Video",
            "release_date": "2021-10-21T00:00:00-04:00",
            "title": "Geospace Dynamics Constellation",
            "description": "\"Moonstone,\" by Rainman [PRS]; Atmosphere; Universal Production Music || 13969_GDC_Mission_FINAL.mov (1920x1080) [4.9 GB] || GDC_MissionVideo_Still.png (1920x1080) [3.7 MB] || GDC_Mission_SITLL.jpg (1920x1080) [441.3 KB] || 13969_GDC_Mission_FINAL_lowres.mp4 (1280x720) [62.3 MB] || TWITTER_720_13969_GDC_Mission_FINAL_twitter_720.mp4 (1280x720) [42.8 MB] || 13969_GDC_Mission_FINAL.webm (960x540) [94.7 MB] || YOUTUBE_1080_13969_GDC_Mission_FINAL_youtube_1080.mp4 (1920x1080) [339.8 MB] || 13969_GDC_Mission_FINAL.en_US.srt [4.8 KB] || 13969_GDC_Mission_FINAL.en_US.vtt [4.6 KB] || YOUTUBE_4K_13969_GDC_Mission_FINAL_youtube_4k.mp4 (3840x2160) [1.4 GB] || ",
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        {
            "id": 4938,
            "url": "https://svs.gsfc.nasa.gov/4938/",
            "result_type": "Visualization",
            "release_date": "2021-09-24T15:00:00-04:00",
            "title": "Terra Orbit Drift",
            "description": "This visualization illustrates the milestones of Terra’s drift in orbit and showcases its impacts to shadow length and swath width from the change in crossing time. || terra_orbit_drift_comp_4685_print.jpg (1024x576) [115.6 KB] || terra_orbit_drift_comp_4685_searchweb.png (320x180) [55.9 KB] || terra_orbit_drift_comp_4685_thm.png (80x40) [5.5 KB] || terra_orbit_drift_comp_1080p60.mp4 (1920x1080) [20.0 MB] || terra_orbit_drift_comp_1080p60.webm (1920x1080) [9.5 MB] || terra_orbit_drift_comp (3840x2160) [512.0 KB] || terra_orbit_drift_comp_2160p60.mp4 (3840x2160) [56.9 MB] || ",
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    ]
}