{ "count": 328, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Comparison%22", "previous": null, "results": [ { "id": 14991, "url": "https://svs.gsfc.nasa.gov/14991/", "result_type": "Produced Video", "release_date": "2026-03-20T12:00:00-04:00", "title": "Argonne Assembles, Tests Early ComPair-2 Hardware", "description": "Tim Cundiff, an engineering specialist at Argonne National Laboratory in Lemont, Illinois, monitors the automated wire bond of a ComPair-2 detector layer in April 2025. Image courtesy of Argonne National LaboratoryAlt text: A man in a lab uses a microscope.Image description: A man in a white clean suit, gloves, safety glasses, and a hairnet sits in front of a piece of machinery in a laboratory and peers into a microscope. Behind him is a long bench covered in scientific equipment and computers. In front of him, inside the machinery, are what look like two black treads that loop in and out of frame. || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9.jpg (2000x1125) [1.1 MB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_searchweb.png (320x180) [124.6 KB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_thm.png (80x40) [27.3 KB] || ", "hits": 85 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 506 }, { "id": 14980, "url": "https://svs.gsfc.nasa.gov/14980/", "result_type": "Produced Video", "release_date": "2026-02-26T12:00:00-05:00", "title": "Prototype ComPair-2 Gamma-Ray Detectors Complete Thermal Vacuum Testing", "description": "Prototype gamma-ray detectors for the ComPair-2 mission rests in a thermal vacuum chamber after testing in June 2025 at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The ComPair-2 team tested the detectors’ performance at hot and cold temperatures over the course of a week and the overall survivability of the layer itself. Credit: NASA/Sophia RobertsAlt text: A piece of equipment sits inside a chamber in a lab. Image description: A cylindrical metal chamber at the center of the image has its door swung all the way open. Inside are silver-wrapped ComPair-2 detectors attached to many copper-colored wires. The chamber is in a lab with white walls and has tubes, wires, and other pieces of equipment attached. || ComPair2_TVAC-1-small.jpg (4096x2732) [3.2 MB] || ComPair2_TVAC-1.jpg (8192x5464) [30.6 MB] || ", "hits": 115 }, { "id": 14976, "url": "https://svs.gsfc.nasa.gov/14976/", "result_type": "Produced Video", "release_date": "2026-02-20T00:00:00-05:00", "title": "Fermi's 15-year View of the Gamma-Ray Sky", "description": "This image shows the entire sky as seen by Fermi's Large Area Telescope. Lighter colors indicate brighter gamma-ray sources. The map is centered on the center of our galaxy. The most prominent feature is the bright, diffuse glow running along the middle of the map, which marks the central plane of our Milky Way galaxy. The gamma rays there are mostly produced when energetic particles accelerated in the shock waves of supernova remnants collide with gas atoms and even light between the stars. Many of the star-like features above and below the Milky Way plane are distant galaxies powered by supermassive black holes. Many of the bright sources along the plane are pulsars. The image was constructed from 15 years of observations using front-converting gamma rays with energies greater than 1 GeV. Hammer projection with black background.Credit: NASA/DOE/Fermi LAT CollaborationAlt text: Fermi 15-year all-sky gamma-ray mapImage description: A colorful oval map sits in the middle of a black background. The oval is predominantly royal blue, striped with an irregular bright red, orange, and yellow band horizontally across the center, which shows the plane of our Milky Way galaxy. Smaller dots and splotches in red, orange, yellow, and white appear throughout the oval. || intens_ait_180m_gt1000_psf3_gal_0p1.png (3600x1800) [2.9 MB] || intens_ait_180m_gt1000_psf3_gal_0p1_print.jpg (1024x512) [290.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_searchweb.png (320x180) [74.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_thm.png (80x40) [4.6 KB] || ", "hits": 188 }, { "id": 31363, "url": "https://svs.gsfc.nasa.gov/31363/", "result_type": "Hyperwall Visual", "release_date": "2026-02-09T18:59:59-05:00", "title": "Observatory Comparison (Hubble/Spitzer/Webb)", "description": "This video compares images of the Helix Nebula from three NASA observatories: Hubble’s image in visible light, Spitzer’s infrared view, and Webb’s high-resolution near-infrared look.No description available.\r\n\r\nmore info: https://science.nasa.gov/asset/webb/observatory-comparison-hubble-spitzer-webb/", "hits": 443 }, { "id": 20412, "url": "https://svs.gsfc.nasa.gov/20412/", "result_type": "Animation", "release_date": "2026-01-21T11:00:00-05:00", "title": "Artemis II Flight Path Animations", "description": "Animated Flight Path of Artemis II and comparison with NASA's Lunar Reconnaissance Orbiter and the Apollo mission orbits.", "hits": 380598 }, { "id": 5586, "url": "https://svs.gsfc.nasa.gov/5586/", "result_type": "Visualization", "release_date": "2026-01-20T12:00:00-05:00", "title": "Extreme Mass Ratio Black Hole Inspirals (EMRIs)", "description": "Shows seven unique black hole inspirals.", "hits": 738 }, { "id": 14942, "url": "https://svs.gsfc.nasa.gov/14942/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Roman and Webb Comparison Graphics from Far and Wide", "description": "This page contains individual animation clips from the Far and Wide series. These clips all focus on the relationship between the Nancy Grace Roman and James Webb space telescopes: how they are different and how they will work together. These animations may be useful in presentations and other video products. || ", "hits": 186 }, { "id": 31359, "url": "https://svs.gsfc.nasa.gov/31359/", "result_type": "Hyperwall Visual", "release_date": "2025-11-19T18:59:59-05:00", "title": "Immense Stellar Jet in Sh2-284", "description": "This video shows the relative size of two different protostellar jets imaged by NASA’s James Webb Space Telescope. The first image shown is an extremely large protostellar jet located in Sh2-284, 15,000 light-years away from Earth. The outflows from the massive central protostar, which weighs 10 times our Sun, span about 8 light-years across. In comparison, a jet imaged by Webb in the nearby low-mass star-forming region of Rho Ophiuchi is just one light-year long.", "hits": 56 }, { "id": 5503, "url": "https://svs.gsfc.nasa.gov/5503/", "result_type": "Visualization", "release_date": "2025-11-19T12:00:00-05:00", "title": "ESCAPADE Theoretical Flight Through Active Mars Magnetosphere", "description": "NASA's Escape and Plasma Acceleration Dynamics Explorers mission, or ESCAPADE, aims to study Mars' real-time response to the solar wind and how the Martian magnetosphere changes over time, helping us better understand Mars' climate history. In this data visualization, we use the September 13, 2017 solar storm that arrived at Mars as an example of a storm that the twin ESCAPADE spacecraft might study.", "hits": 395 }, { "id": 31358, "url": "https://svs.gsfc.nasa.gov/31358/", "result_type": "Hyperwall Visual", "release_date": "2025-11-12T18:59:59-05:00", "title": "Sagittarius B2 | NIRCam MIRI Filter comparison", "description": "NIRCam filters capture near-infrared light,the images tend to show stars more prominently with features like diffraction spikes, as stars are brighter at shorter wavelengths. MIRI (Mid-Infrared Instrument) Saggitarious A in unprecedented detail, including glowing cosmic dust heated by very young massive stars. The reddest area on the right half of MIRI’s image, known as Sagittarius B2 North, is one of the most molecularly rich regions known, but astronomers have never seen it with such clarity.", "hits": 78 }, { "id": 14856, "url": "https://svs.gsfc.nasa.gov/14856/", "result_type": "Infographic", "release_date": "2025-06-20T10:00:00-04:00", "title": "Roman Space Telescope to Scale with Tyrannosaurus rex", "description": "A comparison of the Nancy Grace Roman Space Telescope with a Tyrannosaurus rex. They have the same approximate length and weight.", "hits": 51 }, { "id": 14792, "url": "https://svs.gsfc.nasa.gov/14792/", "result_type": "Produced Video", "release_date": "2025-05-27T20:57:00-04:00", "title": "Astrophysics Missions Vertical Video", "description": "This page collects vertical videos related to specific Astrophysics missions and their hardware or capabilities.", "hits": 106 }, { "id": 5514, "url": "https://svs.gsfc.nasa.gov/5514/", "result_type": "Visualization", "release_date": "2025-04-07T09:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere for Fulldome", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents and magnetic fields combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 274 }, { "id": 5502, "url": "https://svs.gsfc.nasa.gov/5502/", "result_type": "Visualization", "release_date": "2025-04-07T00:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents (green colors) and magnetic fields (pink lines) combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 344 }, { "id": 14794, "url": "https://svs.gsfc.nasa.gov/14794/", "result_type": "Produced Video", "release_date": "2025-03-11T00:00:00-04:00", "title": "Developing NASA’s ComPair-2 Detectors", "description": "ComPair-2 will host a gamma-ray tracker with 10 layers, each with 380 silicon detectors, like the engineering test unit shown here. This trial version allows the mission team to test the electronics, measure how well the detectors work together, and develop assembly procedures for each layer. Credit: NASA/Sophia RobertsAlt text: Scientific hardware on a table Image description: A square piece of scientific hardware rests on a table on top of a silver cover. The hardware has a white board on the bottom with a silver peg at each corner. Inside the pegs is a black square with orange and green electronic components. The green runs along the bottom of the square and takes up the left corner of the black square. The orange electronic components run in 20 stripes along the black square. The orange is interspersed with black. || ComPair2-3_print.jpg (1024x683) [631.9 KB] || ComPair2-3.jpg (8192x5464) [29.1 MB] || ComPair2-3_searchweb.png (320x180) [124.5 KB] || ComPair2-3_web.png (320x213) [137.6 KB] || ComPair2-3_thm.png [28.0 KB] || ", "hits": 26 }, { "id": 31338, "url": "https://svs.gsfc.nasa.gov/31338/", "result_type": "Hyperwall Visual", "release_date": "2025-01-30T06:00:00-05:00", "title": "Mice Adapting to Microgravity", "description": "Video Showing Mice Adapting to Microgravity || mice-in-space-fs.00001_print.jpg (1024x576) [28.0 KB] || mice-in-space-fs.00512_print.jpg (1024x576) [55.6 KB] || mice-in-space-fs.00512_searchweb.png (320x180) [45.2 KB] || mice-in-space-fs.webm (1920x1080) [17.5 MB] || mice-in-space-fs.mp4 (1920x1080) [229.4 MB] || mice-in-space-fs.00512_thm.png [4.4 KB] || ", "hits": 183 }, { "id": 31323, "url": "https://svs.gsfc.nasa.gov/31323/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GOES East vs GMAO – Global GeoColor Imagery", "description": "gmao-plot-all-colorbars-goes-east-vs-gmao_print.jpg (1024x576) [168.6 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao.png (3840x2160) [6.9 MB] || gmao-plot-all-colorbars-goes-east-vs-gmao_searchweb.png (320x180) [78.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_thm.png (80x40) [6.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_1080p30.mp4 (1920x1080) [12.9 MB] ||", "hits": 40 }, { "id": 31324, "url": "https://svs.gsfc.nasa.gov/31324/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GMAO Band09 Obs Caribbean GMAO vs. GOES", "description": "GMAO Caribbean GOES vs GMAO || 3840x2160_16x9_30p [0 Item(s)] || GMAO Band09 Obs Caribbean GMAO vs. GOES ||", "hits": 17 }, { "id": 5389, "url": "https://svs.gsfc.nasa.gov/5389/", "result_type": "Visualization", "release_date": "2024-11-14T00:00:00-05:00", "title": "Tracking methane with EMIT and AVIRIS-3", "description": "Methane plumes can now be detected using the airborne AVIRIS-3 spectrometer in addition to EMIT on the International Space Station.", "hits": 174 }, { "id": 5340, "url": "https://svs.gsfc.nasa.gov/5340/", "result_type": "Interactive", "release_date": "2024-07-26T11:00:00-04:00", "title": "NASA Climate Legacies: An interactive tool to explore generational differences in the experience of a changing climate", "description": " || An embedded version of the NASA Climate Legacies. The standalone version is available at https://svs.gsfc.nasa.gov/webapps/climate-legacies. || NASA-climate-legacies.png (1920x1361) [201.1 KB] || NASA-climate-legacies_print.jpg (1024x725) [96.7 KB] || NASA-climate-legacies_searchweb.png (320x180) [19.8 KB] || NASA-climate-legacies_thm.png (80x40) [3.1 KB] || ", "hits": 105 }, { "id": 14634, "url": "https://svs.gsfc.nasa.gov/14634/", "result_type": "Produced Video", "release_date": "2024-07-25T14:00:00-04:00", "title": "Fermi Finds Novel Feature in BOAT Gamma-Ray Burst", "description": "The brightest gamma-ray burst yet recorded gave scientists a new high-energy feature to study. Learn what NASA’s Fermi mission saw, and what this feature may be telling us about the burst’s light-speed jets. Credit: NASA's Goddard Space Flight CenterMusic: “Tides,” Jon Cotton [PRS] and Ben Niblett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Distant_GRB_still.jpg (3840x2160) [2.5 MB] || 14634_Fermi_GRB_Emission_Line_Under100.mp4 (1920x1080) [90.7 MB] || 14634_Fermi_GRB_Emission_Line_Best.mp4 (1920x1080) [422.0 MB] || 14634FermiGRBEmissionLine_Captions.en_US.srt [4.4 KB] || 14634FermiGRBEmissionLine_Captions.en_US.vtt [4.2 KB] || 14634_Fermi_GRB_Emission_Line_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || ", "hits": 152 }, { "id": 31299, "url": "https://svs.gsfc.nasa.gov/31299/", "result_type": "Hyperwall Visual", "release_date": "2024-07-24T00:00:00-04:00", "title": "The Penguin and the Egg (Interacting Galaxies Arp 142)", "description": "ARP 142 as seen by Hubble vs. Webb || penguin-and-the-egg_print.jpg (1024x576) [59.0 KB] || penguin-and-the-egg.png (3840x2160) [4.6 MB] || penguin-and-the-egg_searchweb.png (320x180) [30.6 KB] || penguin-and-the-egg_thm.png (80x40) [2.5 KB] || penguin-and-the-egg_1080p.mp4 (1920x1080) [10.1 MB] || penguin-and-the-egg_1080p.webm (1920x1080) [1.5 MB] || penguin-and-the-egg_4k.mp4 (3840x2160) [31.2 MB] || the-penguin-and-the-egg-4k.hwshow [292 bytes] || the-penguin-and-the-egg-1080p.hwshow [301 bytes] || ", "hits": 88 }, { "id": 40520, "url": "https://svs.gsfc.nasa.gov/gallery/solar-cycle25/", "result_type": "Gallery", "release_date": "2024-06-28T00:00:00-04:00", "title": "Solar Cycle 25", "description": "The Solar Cycle 25 Prediction Panel, an international group of experts co-sponsored by NASA and the National Oceanic and Atmospheric Administration (NOAA), announced that solar minimum occurred in December 2019, marking the start of Solar Cycle 25. Since then, the Sun’s activity has been steadily increasing as it approaches solar maximum — the peak of Solar Cycle 25.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again. At its peak, the Sun’s magnetic poles flip.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts, including eruptions known as solar flares and coronal mass ejections, can disturb satellites and communication signals traveling around Earth. Scientists study the solar cycle so we can better understand and predict solar activity.", "hits": 549 }, { "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": 321 }, { "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": 328 }, { "id": 31285, "url": "https://svs.gsfc.nasa.gov/31285/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "The Webb Space Telescope Studies the \"Cosmic Cliffs\" in NGC 3324", "description": "The seemingly three-dimensional “Cosmic Cliffs” showcases Webb’s capabilities to peer through obscuring dust and shed new light on how stars form. Webb reveals emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. This landscape of “mountains” and “valleys” is actually the edge of a nearby stellar nursery called NGC 3324 at the northwest corner of the Carina Nebula.So-called mountains — some towering about 7 light-years high — are speckled with glittering, young stars imaged in infrared light. A cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located above the area shown in this image. The blistering, ultraviolet radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Dramatic pillars rise above the glowing wall of gas, resisting this radiation. The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation.Objects in the earliest, rapid phases of star formation are difficult to capture, but Webb’s extreme sensitivity, spatial resolution and imaging capability can chronicle these elusive events. || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_print.jpg (1024x593) [318.7 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution.png (3840x2224) [10.2 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png (14575x8441) [113.7 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_searchweb.png (320x180) [116.3 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_thm.png (80x40) [13.5 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png.dzi [179 bytes] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png_files [4.0 KB] || the-webb-space-telescope-studies-the-cosmic-cliffs-in-ngc-3324-still.hwshow [430 bytes] || ", "hits": 368 }, { "id": 31287, "url": "https://svs.gsfc.nasa.gov/31287/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "Webb and Hubble Combine to Create Most Colorful View of Universe", "description": "This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope. To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies that could be described as one of the most colorful views of the universe ever created.MACS0416 is a galaxy cluster located about 4.3 billion light-years from Earth, meaning that light we see now left the cluster shortly after the formation of our solar system. This cluster magnifies the light from more distant background galaxies through gravitational lensing. As a result, the research team has been able to identify magnified supernovae and even very highly magnified individual stars.Those colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amount of dust, as detected by Webb. The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes.In this image, blue represents data at wavelengths of 0.435 and 0.606 microns (Hubble filters F435W and F606W); cyan is 0.814, 0.9, and 1.05 microns (Hubble filters F814W, and F105W and Webb filter F090W); green is 1.15, 1.25, 1.4, 1.5, and 1.6 microns (Hubble filters F125W, F140W, and F160W, and Webb filters F115W and F150W); yellow is 2.00 and 2.77 microns (Webb filters F200W, and F277W); orange is 3.56 microns (Webb filter F356W); and red represents data at 4.1 and 4.44 microns (Webb filters F410M and F444W). || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_print.jpg (1024x949) [349.8 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite.png (4457x4133) [34.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite-hw.png (3840x2160) [9.6 MB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_searchweb.png (320x180) [105.9 KB] || STScI-01HDHAVM4K4220Z79YTMP1K7VM-composite_thm.png (80x40) [13.0 KB] || webb-and-hubble-combine-to-create-most-colorful-view-of-universe-composite-image.hwshow [394 bytes] || ", "hits": 197 }, { "id": 31286, "url": "https://svs.gsfc.nasa.gov/31286/", "result_type": "Hyperwall Visual", "release_date": "2024-05-28T00:00:00-04:00", "title": "Webb Space Telescope Studies the Pillars of Creation", "description": "Webb MIRI ImageNASA’s James Webb Space Telescope’s mid-infrared view of the Pillars of Creation strikes a chilling tone. Thousands of stars that exist in this region disappear – and seemingly endless layers of gas and dust become the centerpiece.The detection of dust by Webb’s Mid-Infrared Instrument (MIRI) is extremely important – dust is a major ingredient for star formation. Many stars are actively forming in these dense blue-gray pillars. When knots of gas and dust with sufficient mass form in these regions, they begin to collapse under their own gravitational attraction, slowly heat up – and eventually form new stars.Although the stars appear missing, they aren’t. Stars typically do not emit much mid-infrared light. Instead, they are easiest to detect in ultraviolet, visible, and near-infrared light. In this MIRI view, two types of stars can be identified. The stars at the end of the thick, dusty pillars have recently eroded the material surrounding them. They show up in red because their atmospheres are still enshrouded in cloaks of dust. In contrast, blue tones indicate stars that are older and have shed most of their gas and dust.Mid-infrared light also details dense regions of gas and dust. The red region toward the top, which forms a delicate V shape, is where the dust is both diffuse and cooler. And although it may seem like the scene clears toward the bottom left of this view, the darkest gray areas are where densest and coolest regions of dust lie. Notice that there are many fewer stars and no background galaxies popping into view.Webb’s mid-infrared data will help researchers determine exactly how much dust is in this region – and what it’s made of. These details will make models of the Pillars of Creation far more precise. Over time, we will begin to more clearly understand how stars form and burst out of these dusty clouds over millions of years. || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars.png (1987x1817) [4.1 MB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_print.jpg (1024x576) [125.2 KB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres.png (3840x2160) [4.3 MB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_searchweb.png (320x180) [65.3 KB] || STScI-01GFRYYRTCTMX197BY86MBFCR9-pillars-hwres_thm.png (80x40) [7.3 KB] || webb-space-telescope-studies-the-pillars-of-creation.hwshow [368 bytes] || ", "hits": 396 }, { "id": 5276, "url": "https://svs.gsfc.nasa.gov/5276/", "result_type": "Visualization", "release_date": "2024-05-27T00:00:00-04:00", "title": "Change in Night Lights between 2012 and 2023", "description": "This global, flat map view of night lights data begins with a time series depicting annual averages from 2012 to 2023. The lights then fade away to reveal night lights change between 2012 and 2023, with regions of more light depicted in purple and regions with less light depicted in orange. The sequence then repeats with two pop-out, zoomed-in views of India and Ukraine.", "hits": 1338 }, { "id": 31284, "url": "https://svs.gsfc.nasa.gov/31284/", "result_type": "Hyperwall Visual", "release_date": "2024-05-27T00:00:00-04:00", "title": "The Webb Space Telescope Studies the Southern Ring Nebula", "description": "Webb Space Telescope NIRCam image || southern-ring-nebula_00433_print.jpg (1024x576) [198.6 KB] || southern-ring-nebula_00433.png (3840x2160) [8.6 MB] || NGC_3132_webb_NIRCam-STScI-01G8GZQ3ZFJRD8YF8YZWMAXCE3.png (4833x4501) [21.3 MB] || southern-ring-nebula_00433_searchweb.png (320x180) [90.4 KB] || southern-ring-nebula_00433_thm.png (80x40) [6.2 KB] || the-webb-space-telescope-studies-the-southern-ring-nebula-nircam-view.hwshow [274 bytes] || ", "hits": 167 }, { "id": 14576, "url": "https://svs.gsfc.nasa.gov/14576/", "result_type": "Visualization", "release_date": "2024-05-06T13:00:00-04:00", "title": "NASA Black Hole Visualization Takes Viewers Beyond the Brink", "description": "In this flight toward a supermassive black hole, labels highlight many of the fascinating features produced by the effects of general relativity along the way. This supercomputer visualization tracks a camera as it approaches, briefly orbits, and then crosses the event horizon — the point of no return — of a supersized black hole similar in mass to the one at the center of our galaxy. Credit: NASA's Goddard Space Flight Center/J. Schnittman and B. PowellMusic: “Tidal Force,” Thomas Daniel Bellingham [PRS], Universal Production Music“Memories” from Digital Juice“Path Finder,” Eric Jacobsen [TONO] and Lorenzo Castellarin [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14576_BHPlunge_Explain_Still.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail.jpg (3840x2160) [1.2 MB] || 14576_PageThumbnail_searchweb.png (180x320) [85.0 KB] || 14576_PageThumbnail_thm.png (80x40) [9.6 KB] || 14576_BHPlunge_Explainer_1080.mp4 (1920x1080) [319.5 MB] || 14576_BHPlunge_Explainer_Captions.en_US.srt [2.5 KB] || 14576_BHPlunge_Explainer_Captions.en_US.vtt [2.4 KB] || 14576_BHPlunge_Explainer_4k.mp4 (3840x2160) [1.5 GB] || 14576_BHPlunge_Explainer_4kYouTube.mp4 (3840x2160) [3.0 GB] || 14576_BHPlunge_Explainer_ProRes_3840x2160_2997.mov (3840x2160) [12.8 GB] || ", "hits": 1628 }, { "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": 38 }, { "id": 5229, "url": "https://svs.gsfc.nasa.gov/5229/", "result_type": "Visualization", "release_date": "2024-02-23T17:30:00-05:00", "title": "Moon Essentials: Seasons", "description": "An animation of the Moon's seasons. The left half of the frame shows the 1.5° tilt of the Moon's axis (light blue) relative to the Sun. The right half shows the seasonal change in lighting at the Moon's South Pole. || comp.0001_print.jpg (1024x576) [86.4 KB] || comp.0001_searchweb.png (320x180) [57.8 KB] || comp.0001_thm.png (80x40) [5.4 KB] || comp (1920x1080) [0 Item(s)] || seasons_1080p30.mp4 (1920x1080) [11.5 MB] || seasons_720p30.mp4 (1280x720) [4.0 MB] || seasons_360p30.mp4 (640x360) [1.3 MB] || ", "hits": 1047 }, { "id": 14399, "url": "https://svs.gsfc.nasa.gov/14399/", "result_type": "Produced Video", "release_date": "2023-12-20T11:00:00-05:00", "title": "Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky", "description": "From solar flares to black hole jets: NASA’s Fermi Gamma-ray Space Telescope has produced a unique time-lapse tour of the dynamic high-energy sky. Fermi Deputy Project Scientist Judy Racusin narrates this movie, which compresses 14 years of gamma-ray observations into 6 minutes. Credit: NASA’s Goddard Space Flight Center and NASA/DOE/LAT CollaborationMusic: \"Expanding Shell\" written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Video descriptive text available. || Fermi_14Year_Narrated_Still_print.jpg (1024x576) [157.6 KB] || Fermi_14Year_Narrated_Still.jpg (3840x2160) [891.9 KB] || Fermi_14Year_Narrated_Still_searchweb.png (320x180) [39.2 KB] || Fermi_14Year_Narrated_Still_thm.png (80x40) [4.2 KB] || 14399_Fermi_14Year_Narrated_sub100.mp4 (1920x1080) [90.5 MB] || 14399_Fermi_14Year_Narrated_1080.webm (1920x1080) [49.4 MB] || 14399_Fermi_14Year_Narrated_1080.mp4 (1920x1080) [908.7 MB] || Fermi_14Year_Narrated_SRT_Captions.en_US.srt [8.4 KB] || Fermi_14Year_Narrated_SRT_Captions.en_US.vtt [8.0 KB] || 14399_Fermi_14Year_Narrated_4k.mp4 (3840x2160) [2.2 GB] || 14399_Fermi_14Year_Narrated_ProRes_3840x2160_2997.mov (3840x2160) [19.4 GB] || ", "hits": 132 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 332 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 326 }, { "id": 14405, "url": "https://svs.gsfc.nasa.gov/14405/", "result_type": "Produced Video", "release_date": "2023-08-25T10:00:00-04:00", "title": "XRISM: Exploring the Hidden X-ray Cosmos", "description": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim || YTframe_XRISM_Exploring_XrayCosmos.jpg (1280x720) [668.5 KB] || YTframe_XRISM_Exploring_XrayCosmos_searchweb.png (320x180) [100.3 KB] || YTframe_XRISM_Exploring_XrayCosmos_thm.png (80x40) [7.6 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.srt [7.8 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.vtt [7.4 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mov (3840x2160) [21.6 GB] || ", "hits": 234 }, { "id": 5142, "url": "https://svs.gsfc.nasa.gov/5142/", "result_type": "Visualization", "release_date": "2023-08-24T10:45:00-04:00", "title": "TEMPO - Nitrogen Dioxide Air Pollution Over North America", "description": "High levels of nitrogen dioxide can be seen over multiple urban areas across the North America and the Caribbean. Detailed views of three regions show high levels of nitrogen dioxide over cities in the morning and enhanced levels of nitrogen dioxide over major highways. As the day progresses, morning pollution often dissipates then rises again as cities enter their second rush hour. Since TEMPO uses visible sunlight to make measurements, cloudy areas appear as missing data in the visualization.", "hits": 244 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 42 }, { "id": 14372, "url": "https://svs.gsfc.nasa.gov/14372/", "result_type": "B-Roll", "release_date": "2023-07-20T10:00:00-04:00", "title": "ComPair Thermal Vacuum Photos", "description": "Team members work on the ComPair balloon instrument before it begins testing in a thermal vacuum chamber at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. ComPair project manager Regina Caputo (front right), graduate student Nicholas Kirschner (George Washington University, left), and research scientist Nicholas Cannady (University of Maryland Baltimore County, rear) examine ComPair's various components to determine what needs to be “harnessed,” or connected via cable to power systems and the onboard computer.Credit: NASA/Scott Wiessinger || ComPair_TVac_IMG_2141.png (5319x3546) [30.9 MB] || ComPair_TVac_IMG_2141.jpg (5319x3546) [6.0 MB] || ComPair_TVac_IMG_2141_half.jpg (2659x1773) [1.4 MB] || ", "hits": 51 }, { "id": 5112, "url": "https://svs.gsfc.nasa.gov/5112/", "result_type": "Visualization", "release_date": "2023-07-12T11:00:00-04:00", "title": "Landsat Next Planned Orbits and Swath Coverage (version 2)", "description": "Lansdat Next trio of satellites orbiting and revealing data. It takes Landsat Next 6 days to get full coverage of the earth (aside from areas near the poles). This visualization shows two full cycles of coverage. || landsat_next.048.02000_print.jpg (1024x576) [68.5 KB] || landsat_next.048.02000_searchweb.png (320x180) [38.0 KB] || landsat_next.048.02000_thm.png (80x40) [3.6 KB] || landsat_next.048_1080p59.94.mp4 (1920x1080) [29.2 MB] || landsat_next.048_2160p59.94.mp4 (3840x2160) [84.5 MB] || landsat_next_hyperwall_preview.mp4 (2400x810) [35.4 MB] || landsat_next (3840x2160) [256.0 KB] || landsat_next (9600x3240) [256.0 KB] || ", "hits": 75 }, { "id": 14354, "url": "https://svs.gsfc.nasa.gov/14354/", "result_type": "B-Roll", "release_date": "2023-05-25T00:00:00-04:00", "title": "ComPair Gamma-Ray Balloon Mission", "description": "Carolyn Kierans, principal investigator for the ComPair balloon mission at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, works on the instrument in this video. First, she assembles a layer of the tracker, which is housed in an aluminum casing. Next, she shows one of the tracker’s silicon detectors. Then she takes the lid off the tracker.Credit: NASA/Sophia Roberts || Unassembled_Parts_of_ComPair.01740_print.jpg (1024x540) [148.3 KB] || Unassembled_Parts_of_ComPair.01740_searchweb.png (320x180) [94.0 KB] || Unassembled_Parts_of_ComPair.01740_thm.png (80x40) [7.0 KB] || Unassembled_Parts_of_ComPair.webm (4096x2160) [18.2 MB] || Unassembled_Parts_of_ComPair.mp4 (4096x2160) [570.8 MB] || ", "hits": 34 }, { "id": 5104, "url": "https://svs.gsfc.nasa.gov/5104/", "result_type": "Visualization", "release_date": "2023-05-23T00:00:00-04:00", "title": "Two Decades of Changes in Nitrogen Dioxide and Fine Particulate Pollution in the U.S.", "description": "A data visualization of particulate matter 2.5 (PM2.5) data for the Washington DC region spanning 2000-2018 (annual averages). Higher values are represented with dark red and lower values are represented with bright yellow. This view uses the hybrid PM 2.5 color bar with a range of 5 to 20. || pm25_dc_annual.2018_print.jpg (1024x576) [216.4 KB] || pm25_dc_annual.2018_searchweb.png (320x180) [75.7 KB] || pm25_dc_annual.2018_thm.png (80x40) [6.2 KB] || pm25_dc_annual (3840x2160) [0 Item(s)] || pm25_dc_annual_2160p1.mp4 (3840x2160) [30.8 MB] || pm25_dc_annual_2160p60_prores.mov (3840x2160) [41.0 MB] || pm25_dc_annual_2160p1.webm (3840x2160) [1.9 MB] || ", "hits": 76 }, { "id": 5102, "url": "https://svs.gsfc.nasa.gov/5102/", "result_type": "Visualization", "release_date": "2023-05-11T12:00:00-04:00", "title": "When Coronal Holes are Smiling.... - October 26, 2022", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.In another example of pareidolia (Wikipedia) we have what appears to be a smiling face in the SDO/AIA 193 Angstrom filters formed by the arrangement of the darker coronal holes. Coronal holes form at the footpoints of open magnetic field lines which form a 'fast track' for the outflowing solar wind. These 'open' field lines do not connect back to the Sun but instead reach out to the heliopause and interstellar medium. The fast solar wind has an average speed of about 750 kilometers per second, compared to the slow solar wind with speeds from 300 to 500 kilometers per second.For comparison, we include the same time frame from the AIA 171 Angstrom filter where the 'face' is much less pronounced. || ", "hits": 109 }, { "id": 40462, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles3-earthas-art/", "result_type": "Gallery", "release_date": "2023-05-01T00:00:00-04:00", "title": "Cosmic Cycles 3 Earth as Art", "description": "Starting in 1972, nine Landsat satellites have orbited Earth, taking images of the surface. This unprecedented coverage has been tremendously useful to the scientific community, but it has also produced thousands of beautiful high-resolution images of the complex patterns of our world. From the fractal patterns of mountain ranges and river deltas to the precise geometry of agriculture, Landsat has rendered Earth as a work of art.", "hits": 46 }, { "id": 5098, "url": "https://svs.gsfc.nasa.gov/5098/", "result_type": "Visualization", "release_date": "2023-04-24T09:00:00-04:00", "title": "Relative Wetness Root Zone Versus Groundwater Comparison", "description": "Sample composite showing the comparison between the root zone relative wetness data to groundwater wetness data. The root zone is approximately 1 meter below the surface as opposed to groundwater which is deeper. Seeing these side-by-side allows the viewer to see that the root zone data changes much more rapidly than the deeper stored groundwater data. || root_n_grnd.4k.2676_print.jpg (1024x576) [173.0 KB] || root_n_grnd.4k.2676_searchweb.png (320x180) [73.6 KB] || root_n_grnd.4k.2676_web.png (320x180) [73.6 KB] || root_n_grnd.1080p30.mp4 (1920x1080) [50.5 MB] || root_n_grnd.1080p30.webm (1920x1080) [10.7 MB] || Sample_Composite (3840x2160) [0 Item(s)] || root_n_grnd.2160p30.mp4 (3840x2160) [118.5 MB] || ", "hits": 20 }, { "id": 14309, "url": "https://svs.gsfc.nasa.gov/14309/", "result_type": "Produced Video", "release_date": "2023-03-15T11:00:00-04:00", "title": "Fermi Captures Dynamic Gamma-ray Sky", "description": "Watch a cosmic gamma-ray fireworks show in this animation using just a year of data from the Large Area Telescope (LAT) aboard NASA’s Fermi Gamma-ray Space Telescope. Each object’s magenta circle grows as it brightens and shrinks as it dims. The yellow circle represents the Sun following its apparent annual path across the sky. The animation shows a subset of the LAT gamma-ray records now available for more than 1,500 objects in a new, continually updated repository. Over 90% of these sources are a type of galaxy called a blazar, powered by the activity of a supermassive black hole.Credit: NASA’s Marshall Space Flight Center/Daniel Kocevski || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_ProRes_3840x2160.mov (3840x2160) [170.3 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1600.gif (1600x900) [6.5 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1050.gif (1050x590) [3.2 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark.gif (800x450) [2.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.mp4 (3840x2160) [12.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.webm (3840x2160) [1.9 MB] || ", "hits": 127 }, { "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": 136 }, { "id": 31207, "url": "https://svs.gsfc.nasa.gov/31207/", "result_type": "Hyperwall Visual", "release_date": "2022-11-09T00:00:00-05:00", "title": "Changes in Zachariæ Isstrøm, North East Greenland, from Landsat – 1999-2022", "description": "Zachariae Isstrom glacier, 1999-2022 || ZI-update-2022_00000_print.jpg (1024x576) [314.7 KB] || ZI-update-2022_00000_searchweb.png (320x180) [133.7 KB] || ZI-update-2022_00000_thm.png (80x40) [8.0 KB] || ZI-update-2022_1080p30_3.mp4 (1920x1080) [44.7 MB] || ZI-update-2022_1080p30_3.webm (1920x1080) [6.7 MB] || time-series (3840x2160) [0 Item(s)] || ZI-update-2022_2160p30_3.mp4 (3840x2160) [145.8 MB] || ", "hits": 34 }, { "id": 31199, "url": "https://svs.gsfc.nasa.gov/31199/", "result_type": "Hyperwall Visual", "release_date": "2022-10-31T00:00:00-04:00", "title": "Earth Surface Mineral Dust Source Investigation (EMIT) for hyperwall", "description": "Animation showing location of EMIT on the ISS || emit_on_iss_print.jpg (1024x576) [93.5 KB] || emit_on_iss.png (3840x2160) [3.2 MB] || emit_on_iss_searchweb.png (320x180) [67.7 KB] || emit_on_iss_thm.png (80x40) [6.1 KB] || emit_on_iss_1080p60.mp4 (1920x1080) [10.8 MB] || emit_on_iss_1080p60.webm (1920x1080) [3.0 MB] || emit_on_iss_2160p60.mp4 (3840x2160) [28.3 MB] || emit_on_iss.hwshow [198 bytes] || Images and videos prepared for hyperwall for EMIT. || ", "hits": 30 }, { "id": 31202, "url": "https://svs.gsfc.nasa.gov/31202/", "result_type": "Hyperwall Visual", "release_date": "2022-10-27T00:00:00-04:00", "title": "Pillars of Creation: Hubble vs Webb", "description": "Comparison of the Pillars ofCreation; Hubble vs Webb || Pillars_of_creation_00000_print.jpg (1024x576) [178.0 KB] || Pillars_of_creation_00000_searchweb.png (320x180) [92.8 KB] || Pillars_of_creation_00000_web.png (320x180) [92.8 KB] || Pillars_of_creation_00000_thm.png (80x40) [6.6 KB] || Pillars_of_creation_1080p30.mp4 (1920x1080) [57.2 MB] || Pillars_of_creation_1080p30.webm (1920x1080) [9.3 MB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || Pillars_of_creation_2160p30_h265.mp4 (3840x2160) [74.0 MB] || ", "hits": 137 }, { "id": 31197, "url": "https://svs.gsfc.nasa.gov/31197/", "result_type": "Hyperwall Visual", "release_date": "2022-10-26T00:00:00-04:00", "title": "Carina Nebula Webb vs Hubble", "description": "Carina Nebula comparison of James Web vs HubbleThese comparison photos of a young star-forming region called NGC 3324 in the Carina Nebula, taken by Webb, (left) and Hubble, (right), showcase Webb’s abilities to peer through cosmic dust and unveil hundreds of previously hidden stars and background galaxies. Taken by NASA’s James Webb Space Telescope, this image reveals for the first time areas of stellar birth captured in infrared light by the Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). Webb’s NIRCam – with its crisp resolution and unparalleled sensitivity – unveils emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. In MIRI’s view, young stars and their planet-forming disks shine brightly in the mid-infrared, appearing pink and red. Hot dust, hydrocarbons, and other chemical compounds on the surface of the ridges glow, giving the appearance of jagged rocks.Webb’s detailed image captured in infrared light (left) is juxtaposed with a color composite image (right) of separate exposures made by Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Planetary Camera 2 (WFPC2). In Hubble’s image on the right, sulfur is represented by red, oxygen by blue, and hydrogen by green.Webb’s new observations of NGC 3324 will shed light on stellar processes and reveal the impact of star formation on the evolution of gigantic clouds of gas and dust.For more information: https://www.nasa.gov/image-feature/goddard/2022/nasa-s-webb-reveals-cosmic-cliffs-glittering-landscape-of-star-birth || carina_nebula_00000_print.jpg (1024x576) [202.8 KB] || carina_nebula_00000_searchweb.png (320x180) [96.5 KB] || carina_nebula_00000_web.png (320x180) [96.5 KB] || carina_nebula_00000_thm.png (80x40) [6.9 KB] || carina_nebula_720p30.mp4 (1280x720) [22.5 MB] || carina_nebula_720p30.webm (1280x720) [9.4 MB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || carina_nebula_2160p30_h265.mp4 (3840x2160) [57.7 MB] || ", "hits": 136 }, { "id": 14204, "url": "https://svs.gsfc.nasa.gov/14204/", "result_type": "Produced Video", "release_date": "2022-08-31T09:00:00-04:00", "title": "Mars Patchy Proton Aurora", "description": "NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission and the United Arab Emirates’ Emirates Mars Mission (EMM) have released joint observations of dynamic proton aurora events at Mars. Remote auroral observations by EMM paired with in-situ plasma observations made by MAVEN open new avenues for understanding the Martian atmosphere. This collaboration was made possible by recent data-sharing between the two missions and highlights the value of multi-point observations in space.Learn more about this discovery by MAVEN and EMM. || ", "hits": 63 }, { "id": 14174, "url": "https://svs.gsfc.nasa.gov/14174/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Rebekah Hounsell 2022 AAS Roman Hyperwall Talk", "description": "Title slide.Credit: NASA's Goddard Space Flight Center || rebekah_hounsell_roman_title_print.jpg (1024x576) [250.4 KB] || rebekah_hounsell_roman_title.png (3840x2160) [10.3 MB] || rebekah_hounsell_roman_title_searchweb.png (320x180) [111.8 KB] || rebekah_hounsell_roman_title_thm.png (80x40) [8.1 KB] || ", "hits": 33 }, { "id": 14175, "url": "https://svs.gsfc.nasa.gov/14175/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Expanding Our View (2022 STScI presentation)", "description": "Complete PowerPoint file with all slides and notes || PPT_still.jpg (3840x2160) [750.6 KB] || roman-expanding-our-view-presentation.pptx [76.2 MB] || Slide #1 – Onscreen before presentation begins and during introductionCredit: STScI, NASA || Slide1_print.jpg (1024x576) [98.1 KB] || Slide1.png (3840x2160) [3.4 MB] || Slide1.jpg (3840x2160) [750.6 KB] || Slide1_searchweb.png (320x180) [63.9 KB] || Slide1_thm.png (80x40) [5.6 KB] || ", "hits": 52 }, { "id": 4971, "url": "https://svs.gsfc.nasa.gov/4971/", "result_type": "Visualization", "release_date": "2022-06-07T10:00:00-04:00", "title": "Monitoring Changing Waters using the Gulf of Maine Atlantic Time Series (GNATS)", "description": "Visualization of 20 years of data from the Gulf of Maine North Atlantic Time Series (GNATS). The data shown are temperatures at the water's surface and below the surface. Satellite based sea surface temperatures are also shown. This version does not include date or color bar overlays. || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_print.jpg (1024x576) [149.8 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_thm.png (80x40) [6.1 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_searchweb.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_web.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.mp4 (1920x1080) [76.4 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.webm (1920x1080) [12.0 MB] || 3840x2160_16x9_60p (3840x2160) [1.0 MB] || 9600x3240_16x9_30p (9600x3240) [1.0 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_2160p59.94.mp4 (3840x2160) [249.3 MB] || preview_5x3_hyperwall_gulf_of_maine.mp4 (2400x810) [129.1 MB] || ", "hits": 79 }, { "id": 5009, "url": "https://svs.gsfc.nasa.gov/5009/", "result_type": "Visualization", "release_date": "2022-06-01T00:00:00-04:00", "title": "Dixie and Caldor Wildfires Locator Maps - 2021", "description": "Perimeters of Dixie and Caldor wildfires located in California. The extent of the Dixie wildfire is as of October 22, 2021, while the extent of the Caldor wildfire is as of October 6, 2021. The dropdown menu offers multiple resolutions for a 32:27 aspect ratio. || fires_preview.jpg (1024x864) [167.1 KB] || fires_16000.png (16000x13500) [19.6 MB] || fires_3840.png (3840x3240) [11.1 MB] || fires_16000_searchweb.png (320x180) [71.5 KB] || fires_16000_thm.png (80x40) [5.2 KB] || ", "hits": 27 }, { "id": 14090, "url": "https://svs.gsfc.nasa.gov/14090/", "result_type": "Produced Video", "release_date": "2022-02-12T00:00:00-05:00", "title": "Fermi's 12-year View of the Gamma-ray Sky", "description": "This image shows the entire sky as seen by Fermi's Large Area Telescope. The most prominent feature is the bright, diffuse glow running along the middle of the map, which marks the central plane of our Milky Way galaxy. The gamma rays there are mostly produced when energetic particles accelerated in the shock waves of supernova remnants collide with gas atoms and even light between the stars. Many of the star-like features above and below the Milky Way plane are distant galaxies powered by supermassive black holes. Many of the bright sources along the plane are pulsars. The image was constructed from 12 years of observations using front-converting gamma rays with energies greater than 1 GeV. Hammer projection.Credit: NASA/DOE/Fermi LAT Collaboration || Fermi_144-month_Fermi_all-sky_hammer_2160x1080.png (2160x1080) [2.4 MB] || Fermi_144-month_Fermi_all-sky_hammer_2160x1080_print.jpg (1024x512) [306.6 KB] || Fermi_144-month_Fermi_all-sky_hammer_4000x2000.png (4000x2000) [7.0 MB] || Fermi_144-month_Fermi_all-sky_hammer_3600x1800.png (3600x1800) [4.9 MB] || ", "hits": 163 }, { "id": 14047, "url": "https://svs.gsfc.nasa.gov/14047/", "result_type": "Produced Video", "release_date": "2021-12-20T09:55:00-05:00", "title": "Hubble and Webb: A New Golden Age of Astronomy", "description": "The scientific community is incredibly excited to have these two highly complementary observatories operating together. With their collaboration, they will push the boundaries of knowledge on the backdrop of a rapidly evolving astronomical landscape. A wealth of multiwavelength and now multi-messenger astrophysical observatories, from space and from the ground, are currently operating or being planned, Hubble and Webb will work together to advance our collective understanding of the universe, ushering in a new golden age of astronomy!For more information, visit https://nasa.gov/hubble. Additional Credits:Comparison of Hubble and James Webb mirror: ESA/M. KornmesserESO ALMA Timelapse: ESOMusic Credits: \"Wonderful Nature\" by July Tourret [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music. || ", "hits": 35 }, { "id": 40433, "url": "https://svs.gsfc.nasa.gov/gallery/science-ona-sphere-gallery/", "result_type": "Gallery", "release_date": "2021-11-23T00:00:00-05:00", "title": "Science On a Sphere Gallery", "description": "Content for NOAA's Science on a Sphere and related spherical display platforms.", "hits": 303 }, { "id": 13947, "url": "https://svs.gsfc.nasa.gov/13947/", "result_type": "Produced Video", "release_date": "2021-10-19T12:00:00-04:00", "title": "Video Visions of the Future", "description": "Inspired by the \"Visions of the Future\" poster series created by NASA’s Jet Propulsion Laboratory in Southern California, this inspirational video imagines a time when space tourists flock to the Moon, vacation in the clouds of Venus, kayak on Saturn’s moon Titan, and visit planets beyond our solar system.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) and NASA/JPL-CaltechMusic: \"Life Choices\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Exoplanet_Kepler16b_Frame.jpg (1920x1080) [485.3 KB] || Exoplanet_Kepler16b_Frame_searchweb.png (320x180) [62.9 KB] || Exoplanet_Kepler16b_Frame_thm.png (80x40) [5.7 KB] || 13947_Travel_Poster_1080.mp4 (1920x1080) [68.2 MB] || 13947_Travel_Poster_Best_1080.webm (1920x1080) [9.8 MB] || 13947_Travel_Poster_Best_1080.mp4 (1920x1080) [200.8 MB] || 13947_Travel_Poster_ProRes_1920x1080_24.mov (1920x1080) [940.6 MB] || 13947_Travel_Poster_SRT_Captions.en_US.srt [1.7 KB] || 13947_Travel_Poster_SRT_Captions.en_US.vtt [1.7 KB] || ", "hits": 198 }, { "id": 4915, "url": "https://svs.gsfc.nasa.gov/4915/", "result_type": "Visualization", "release_date": "2021-08-09T00:00:00-04:00", "title": "A Global view of Normalized Difference Vegetation Index (NDVI) Anomaly in crop-growing regions from 2000 to 2021", "description": "This visualization shows the NDVI anomaly from the year 2000 to 2021 in areas where maize, rice, soybeans, spring wheat or winter wheat are grown. Green colors indicate more than average vegetatation while orange colors indicate less productive areas.Coming soon to our YouTube channel. || NDVI_anomaly_2000-2021.11770.png (1920x1080) [897.2 KB] || NDVI_anomaly_2000-2021.11770_print.jpg (1024x576) [79.6 KB] || NDVI_anomaly_2000-2021.11770_searchweb.png (320x180) [39.8 KB] || NDVI_anomaly_2000-2021.11770_thm.png (80x40) [4.5 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || NDVI_anomaly_2000-2021_1080p30.webm (1920x1080) [60.4 MB] || NDVI_anomaly_2000-2021_1080p30.mp4 (1920x1080) [146.7 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || captions_silent.31356.en_US.srt [43 bytes] || NDVI_Anomaly_2000_2021_4k_2160p30.mp4 (3840x2160) [608.3 MB] || NDVI_anomaly_2000-2021_1080p30.mp4.hwshow [196 bytes] || ", "hits": 274 }, { "id": 4916, "url": "https://svs.gsfc.nasa.gov/4916/", "result_type": "Visualization", "release_date": "2021-08-09T00:00:00-04:00", "title": "Normalized Difference Vegetation Index (NDVI) Anomaly in crop-growing regions for selected years", "description": "This visualization shows the NDVI anomaly in areas where maize, rice, soybeans, spring wheat or winter wheat are grown over the United States, Australia, Russia, Europe and southern Africa during certain years. Green colors indicate more than average vegetatation while orange colors indicate less productive areas.Coming soon to our YouTube channel. || NDVI_anomaly_regions.1020_print.jpg (1024x576) [140.2 KB] || NDVI_anomaly_regions.1020_searchweb.png (320x180) [72.6 KB] || NDVI_anomaly_regions.1020_thm.png (80x40) [5.9 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || NDVI_anomaly_regions_1080p30.mp4 (1920x1080) [110.9 MB] || captions_silent.31363.en_US.srt [43 bytes] || NDVI_anomaly_regions_1080p30.mp4.hwshow [194 bytes] || ", "hits": 93 }, { "id": 13897, "url": "https://svs.gsfc.nasa.gov/13897/", "result_type": "Produced Video", "release_date": "2021-08-04T17:00:00-04:00", "title": "TESS Tunes into an All-sky ‘Symphony’ of Red Giants", "description": "This visualization shows the new sample of oscillating red giant stars (colored dots) discovered by NASA’s Transiting Exoplanet Survey Satellite. The colors map to each 24-by-96-degree swath of the sky observed during the mission's first two years. The view then changes to show the positions of these stars within our galaxy, based on distances determined by ESA’s (the European Space Agency’s) Gaia mission. The scale shows distances in kiloparsecs, each equal to 3,260 light-years, and extends nearly 20,000 light-years from the Sun.Credit: Kristin Riebe, Leibniz Institute for Astrophysics Potsdam || tess_red_giant_visualization_still.jpg (1920x1080) [649.4 KB] || tess_red_giant_visualization_still_print.jpg (1024x576) [269.5 KB] || tess_red_giant_visualization_still_searchweb.png (320x180) [81.2 KB] || tess_red_giant_visualization_still_web.png (320x180) [81.2 KB] || tess_red_giant_visualization_still_thm.png (80x40) [5.7 KB] || tess_red_giant_visualization_HQ.mp4 (1920x1080) [97.4 MB] || tess_red_giant_visualization_LQ.mp4 (1920x1080) [61.1 MB] || tess_red_giant_visualization_prores.mov (1920x1080) [760.0 MB] || tess_red_giant_visualization_LQ.webm (1920x1080) [10.8 MB] || tess_red_giant_visualization_LQ.en_US.srt [526 bytes] || tess_red_giant_visualization_LQ.en_US.vtt [539 bytes] || ", "hits": 198 }, { "id": 4826, "url": "https://svs.gsfc.nasa.gov/4826/", "result_type": "Visualization", "release_date": "2021-04-19T12:00:00-04:00", "title": "Brazil and Novo Progresso Land Use Data Over Time", "description": "This animation begins by showing the similar sizes between the country of Brazil and the United States. It then cycles through over three decades of classification data for the entire Northern half of Brazil. We then zoom down to the town of Novo Progresso and compare its relative size to the San Francisco Bay region. Next we cycle through over three decades of transformation in the region showing how the north/south corridor of this region changed over time. Lastly, we fade in 2019 fire data to indicate how the data will continue to change into the upcoming year. || novo_progressov_finalcomp.2009_print.jpg (1024x576) [287.1 KB] || novo_progressov_finalcomp.2009_searchweb.png (180x320) [105.7 KB] || novo_progressov_finalcomp.2009_thm.png (80x40) [7.3 KB] || novo_progressov_finalcomp_1080p30.mp4 (1920x1080) [48.9 MB] || example_composite (1920x1080) [0 Item(s)] || novo_progressov_finalcomp_1080p30.webm (1920x1080) [7.9 MB] || novo_progressov_finalcomp_1080p30.mp4.hwshow [199 bytes] || ", "hits": 59 }, { "id": 4900, "url": "https://svs.gsfc.nasa.gov/4900/", "result_type": "Visualization", "release_date": "2021-04-19T00:00:00-04:00", "title": "Novo Progresso Deforestation Soccer Field Comparison", "description": "Animation begins with a stylized bright green soccer field. Soccer fields then fall into place over a recently deforested field showing the estimated size of the newly cleared field. The camera then pulls back to reveal all the recently deforested areas (shown in bright green) around Novo Progresso from 2017 to 2018. || soccer_comp.0700_print.jpg (1024x576) [161.5 KB] || soccer_comp.0700_searchweb.png (320x180) [85.8 KB] || soccer_comp.0700_thm.png (80x40) [14.1 KB] || soccer_2017_2018_1080p30.mp4 (1920x1080) [28.6 MB] || 2017_to_2018 (1920x1080) [0 Item(s)] || soccer_2017_2018_1080p30.webm (1920x1080) [5.7 MB] || soccer_2017_2018_1080p30.mp4.hwshow [190 bytes] || ", "hits": 41 }, { "id": 4872, "url": "https://svs.gsfc.nasa.gov/4872/", "result_type": "Visualization", "release_date": "2020-11-17T00:00:00-05:00", "title": "Deviation of Modeled Normal Pollution Levels from Measurements Following COVID-19 Lockdown", "description": "Deviation from modeled normal nitrogen dioxide levels after COVID-19 lockdowns || covid_19_7_day_no2.0810_print.jpg (1024x576) [207.7 KB] || covid_19_7_day_no2.0810_searchweb.png (320x180) [83.4 KB] || covid_19_7_day_no2.0810_thm.png (80x40) [6.4 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || covid_19_7_day_no2_1080p30.mp4 (1920x1080) [25.3 MB] || covid_19_7_day_no2_1080p30.webm (1920x1080) [5.0 MB] || covid_19_7_day_no2_1080p30.mp4.hwshow [192 bytes] || ", "hits": 34 }, { "id": 13738, "url": "https://svs.gsfc.nasa.gov/13738/", "result_type": "Produced Video", "release_date": "2020-10-19T11:30:00-04:00", "title": "OSIRIS-REx Science and Engineering Briefing", "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ", "hits": 41 }, { "id": 13724, "url": "https://svs.gsfc.nasa.gov/13724/", "result_type": "Produced Video", "release_date": "2020-09-24T14:25:00-04:00", "title": "OSIRIS-REx: Countdown to TAG", "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ", "hits": 58 }, { "id": 4823, "url": "https://svs.gsfc.nasa.gov/4823/", "result_type": "Visualization", "release_date": "2020-09-11T00:00:00-04:00", "title": "Draining the Oceans", "description": "Data visualization of the draining of the Earth's oceans. The visualization simulates an incremental drop of 10 meters of the water’s level on Earth’s surface. As time progresses and the oceans drain, it becomes evident that underwater mountain ranges are bigger in size and trenches are deeper in comparison to those on dry land. While water drains quickly closer to continents, it drains slowly in our planet’s deepest trenches. || OceanDrain_3840x2160_60fps_0837_print.jpg (1024x576) [259.5 KB] || OceanDrain_3840x2160_60fps_0837_print_searchweb.png (320x180) [97.8 KB] || OceanDrain_3840x2160_60fps_0837_print_thm.png (80x40) [7.8 KB] || OceanDrain_1920x1080_30fps.mp4 (1920x1080) [44.2 MB] || OceanDrain_1920x1080_30fps.webm (1920x1080) [4.3 MB] || OceanDrain (3840x2160) [0 Item(s)] || OceanDrain (3840x2160) [0 Item(s)] || OceanDrain_3840x2160_60fps_0837.tif (3840x2160) [31.6 MB] || OceanDrain_3840x2160_30fps.mp4 (3840x2160) [154.1 MB] || OceanDrain_1920x1080_30fps.mp4.hwshow [192 bytes] || ", "hits": 630 }, { "id": 20323, "url": "https://svs.gsfc.nasa.gov/20323/", "result_type": "Animation", "release_date": "2020-09-09T12:00:00-04:00", "title": "OSIRIS-REx Sampling Area to Scale: Animations", "description": "OSIRIS-REx is NASA’s first asteroid sample return mission. Its main science goal is to collect a sample of near-Earth asteroid Bennu for return to Earth in 2023. These animations show a size comparison of the planned sample collection area before arriving at Bennu (orange), and after arriving at Bennu (blue). The original mission plan envisioned a sample site with a diameter of 164 feet (50 m). However, the sampling region for site Nightingale is approximately 26 ft (8 m) in diameter. The area safe enough for the spacecraft to touch is the width of a few parking spaces. || ", "hits": 36 }, { "id": 13667, "url": "https://svs.gsfc.nasa.gov/13667/", "result_type": "Produced Video", "release_date": "2020-07-24T16:00:00-04:00", "title": "The Roman Space Telescope's Immense Data Volume", "description": "This infographic showcases the difference in data volume between the Nancy Grace Roman, Webb and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.Credit: NASA's Goddard Space Flight Center || Roman_Data_Scale_Final_1080.png (1920x1080) [9.7 MB] || Roman_Data_Scale_Final_1080.jpg (1920x1080) [515.8 KB] || Roman_Data_Scale_Final_1080_print.jpg (1024x576) [99.3 KB] || Roman_Data_Scale_Final.png (3840x2160) [38.9 MB] || Roman_Data_Scale_Final.jpg (3840x2160) [1.9 MB] || ", "hits": 100 }, { "id": 40414, "url": "https://svs.gsfc.nasa.gov/gallery/webb-arapp-media/", "result_type": "Gallery", "release_date": "2020-04-02T00:00:00-04:00", "title": "Webb AR App Media", "description": "Backend video content to support the Webb AR app!", "hits": 113 }, { "id": 4791, "url": "https://svs.gsfc.nasa.gov/4791/", "result_type": "Visualization", "release_date": "2020-02-24T10:00:00-05:00", "title": "Apollo 13 Moon View Using LRO Data", "description": "Path 75:02:00 − 80:01:50. The path of the Apollo 13 spacecraft near the Moon. The one-minute animation covers five hours of real time, at 10 seconds per frame. The view is centered on the lunar north pole, with the center of the near side facing the top of the frame. Versions both with and without the annotations in the bottom right are available, as are the separate components (Moon and path with alpha, starry background). || path.0900_print.jpg (1024x576) [59.6 KB] || path.0900_thm.png (80x40) [2.3 KB] || path.0900_searchweb.png (320x180) [43.9 KB] || path_annotated_1080p30.mp4 (1920x1080) [16.1 MB] || path_annotated_720p30.mp4 (1280x720) [7.3 MB] || path_annotated_720p30.webm (1280x720) [7.0 MB] || path_1080p30.mp4 (1920x1080) [14.9 MB] || path_720p30.mp4 (1280x720) [6.6 MB] || path_ann (3840x2160) [0 Item(s)] || path_stars (3840x2160) [0 Item(s)] || path (3840x2160) [0 Item(s)] || path_comp (3840x2160) [0 Item(s)] || path_annotated_2160p30.mp4 (3840x2160) [50.4 MB] || path_360p30.mp4 (640x360) [1.5 MB] || path_2160p30.mp4 (3840x2160) [43.7 MB] || path_annotated_360p30.mp4 (640x360) [1.8 MB] || path_2160p30_prores.mov (3840x2160) [4.3 GB] || path_1080p30.mp4.hwshow [178 bytes] || ", "hits": 904 }, { "id": 31106, "url": "https://svs.gsfc.nasa.gov/31106/", "result_type": "Hyperwall Visual", "release_date": "2020-02-12T00:00:00-05:00", "title": "Fires Light Up Mount Vesuvius", "description": "Wildfires on Mount Vesuvius || volcano-vesuvius_print.jpg (1024x576) [98.9 KB] || volcano-vesuvius.png (3840x2160) [3.5 MB] || volcano-vesuvius_searchweb.png (320x180) [66.4 KB] || volcano-vesuvius_thm.png (80x40) [5.3 KB] || fires-light-up-mount-vesuvius.hwshow [285 bytes] || ", "hits": 30 }, { "id": 13521, "url": "https://svs.gsfc.nasa.gov/13521/", "result_type": "Produced Video", "release_date": "2020-01-14T14:00:00-05:00", "title": "Primary Mirror Size Comparison Between Webb and Hubble", "description": "Webb Telescope and Hubble Telescope primary mirror comparison with person as reference. || JWST_2020_composite_mirror_with_Person.00028_print.jpg (1024x576) [29.9 KB] || JWST_2020_composite_mirror_with_Person.00028_searchweb.png (180x320) [38.2 KB] || JWST_2020_composite_mirror_with_Person.00028_web.png (320x180) [38.2 KB] || JWST_2020_composite_mirror_with_Person.00028_thm.png (80x40) [3.9 KB] || JWST_2020_composite_mirror_with_Person.mov (3840x2160) [866.1 MB] || JWST_2020_composite_mirror_with_Person.webm (3840x2160) [3.0 MB] || JWST_2020_composite_mirror_with_Person.mp4 (3840x2160) [9.6 MB] || ", "hits": 367 }, { "id": 13522, "url": "https://svs.gsfc.nasa.gov/13522/", "result_type": "Produced Video", "release_date": "2020-01-14T14:00:00-05:00", "title": "Spacecraft Size Comparison Between the Webb Space Telescope and the Hubble Space Telescope", "description": "Size comparison between the Webb Space Telescope and the Hubble Space Telescope. || JWST_v_HST_TTable_4k_woPerson.00029_print.jpg (1024x576) [44.4 KB] || JWST_v_HST_TTable_4k_woPerson.00029_searchweb.png (320x180) [35.8 KB] || JWST_v_HST_TTable_4k_woPerson.00029_thm.png (80x40) [3.9 KB] || JWST_v_HST_TTable_4k_woPerson.mov (3840x2160) [1.8 GB] || JWST_v_HST_TTable_4k_woPerson.mp4 (3840x2160) [11.5 MB] || JWST_v_HST_TTable_4k_woPerson.webm (3840x2160) [4.1 MB] || ", "hits": 137 }, { "id": 13497, "url": "https://svs.gsfc.nasa.gov/13497/", "result_type": "Produced Video", "release_date": "2020-01-05T14:00:00-05:00", "title": "Simulated Image Demonstrates the Power of NASA’s Nancy Grace Roman Space Telescope", "description": "Watch the video to learn more about the Roman Space Telescope's simulated image.Credit: NASA's Goddard Space Flight CenterMusic: \"Flight Impressions\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Simulated_Image_Still.jpg (1920x1080) [891.1 KB] || 13497_Simulated_Image_Roman_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13497_Simulated_Image_Roman_Best_1080.mp4 (1920x1080) [936.5 MB] || 13497_Simulated_Image_Roman_1080.mp4 (1920x1080) [291.8 MB] || 13497_Simulated_Image_Roman_1080.webm (1920x1080) [22.4 MB] || Simulated_Image_Roman_SRT_Captions.en_US.srt [3.6 KB] || Simulated_Image_Roman_SRT_Captions.en_US.vtt [3.6 KB] || ", "hits": 66 }, { "id": 13489, "url": "https://svs.gsfc.nasa.gov/13489/", "result_type": "Produced Video", "release_date": "2019-12-12T14:00:00-05:00", "title": "OSIRIS-REx: X Marks the Spot - 2019 AGU Press Conference", "description": "Close-up images of the OSIRIS-REx sample site candidates on asteroid Bennu.Credit: NASA/Goddard/University of Arizona || Bennu_Site_Candidates_CloseUp_print.jpg (1024x575) [150.1 KB] || Bennu_Site_Candidates_CloseUp.png (7999x4499) [15.5 MB] || ", "hits": 38 }, { "id": 13437, "url": "https://svs.gsfc.nasa.gov/13437/", "result_type": "Produced Video", "release_date": "2019-12-09T14:00:00-05:00", "title": "Operation IceBridge - Arctic NOAA Flights", "description": "In Spring of 2016, Operation IceBridge conducted its eight spring Arctic survey of polar ice over the course of five weeks. Six research flights studying sea ice were based in Thule, Greenland, while ten that focused on land ice flew out of Kangerlussuaq in southern Greenland.For the survey, the crew utilized National Oceanic and Atmospheric Administration’s P-3 Orion Hurricane Hunter plane. NASA's Wallops Flight Facility in Virginia provided the laser altimeter and one of the infrared cameras on the P-3. IceBridge's three radar instruments came from the Center for Remote Sensing of Ice Sheets at the University of Kansas, while NASA's Ames Research Center at Moffett Field, California, provided the Digital Mapping System, and the University of Colorado loaned the second infrared camera.During this campaign the IceBridge aircraft flew under the path of Sentinel-3A, a recently launched ESA satellite that carries a radar altimeter that gauges sea ice thickness. Scientists will compare the Sentinel-3A measurements to the data IceBridge collected over the same spots with its radar and laser altimeters. This comparison will help validate and refine Sentinel-3A’s data gathering. || ", "hits": 29 }, { "id": 13200, "url": "https://svs.gsfc.nasa.gov/13200/", "result_type": "Produced Video", "release_date": "2019-07-29T10:00:00-04:00", "title": "NASA’s TESS Finds Three New Worlds", "description": "This infographic illustrates key features of the TOI 270 system, located about 73 light-years away in the southern constellation Pictor. The three known planets were discovered by NASA’s Transiting Exoplanet Survey Satellite through periodic dips in starlight caused by each orbiting world. Insets show information about the planets, including their relative sizes, and how they compare to Earth. Temperatures given for TOI 270’s planets are equilibrium temperatures, calculated without the warming effects of any possible atmospheres. Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || TOI_270_Infographic_Final_print.jpg (1024x576) [64.1 KB] || TOI_270_Infographic_Final.png (5760x3240) [17.4 MB] || TOI_270_Infographic_Final.jpg (5760x3240) [2.0 MB] || TOI_270_Infographic_Final-halfsize.png (2880x1620) [5.4 MB] || TOI_270_Infographic_Final-halfsize.jpg (2880x1620) [484.0 KB] || TOI_270_Infographic_Final_searchweb.png (320x180) [47.7 KB] || TOI_270_Infographic_Final_thm.png (80x40) [4.9 KB] || ", "hits": 233 }, { "id": 31032, "url": "https://svs.gsfc.nasa.gov/31032/", "result_type": "Hyperwall Visual", "release_date": "2019-04-08T00:00:00-04:00", "title": "Historic Floods Inundate Nebraska", "description": "Comparison of imagery of Omaha in March 2018 and 2019 shows flooding in 2019 || omaha_oli_flooding_2019_print.jpg (1024x576) [246.2 KB] || omaha_oli_flooding_2019.png (3840x2160) [12.9 MB] || omaha_oli_flooding_2019_searchweb.png (320x180) [124.7 KB] || omaha_oli_flooding_2019_thm.png (80x40) [6.8 KB] || omaha_oli_flooding_2019_1080p.mp4 (1920x1080) [3.0 MB] || omaha_oli_flooding_2019_720p.mp4 (1280x720) [1.6 MB] || omaha_oli_flooding_2019_720p.webm (1280x720) [635.5 KB] || omaha_oli_flooding_2019_3840p.mp4 (3840x2160) [8.5 MB] || ", "hits": 90 }, { "id": 13149, "url": "https://svs.gsfc.nasa.gov/13149/", "result_type": "Produced Video", "release_date": "2019-04-04T15:00:00-04:00", "title": "GLOBE Observer Clouds: Getting Started", "description": "Learn how to use the GLOBE Observer app to observe clouds. || 13149_GLOBE_Clouds_How_To_Thumbnail_print.jpg (1024x572) [65.8 KB] || 13149_GLOBE_Clouds_How_To_Thumbnail.png (3342x1868) [6.7 MB] || 13149_GLOBE_Clouds_How_To_Thumbnail_searchweb.png (320x180) [77.6 KB] || 13149_GLOBE_Clouds_How_To_Thumbnail_thm.png (80x40) [5.5 KB] || 13149_GLOBE_Clouds_How_To_Final.mov (1920x1080) [3.8 GB] || 13149_GLOBE_Clouds_How_To_Final.webm (960x540) [59.4 MB] || 13149_GLOBE_Clouds_How_To_Final_lowres.mp4 (1280x720) [49.1 MB] || FACEBOOK_720_13149_GLOBE_Clouds_How_To_Final_facebook_720.mp4 (1280x720) [146.1 MB] || TWITTER_720_13149_GLOBE_Clouds_How_To_Final_twitter_720.mp4 (1280x720) [28.5 MB] || YOUTUBE_1080_13149_GLOBE_Clouds_How_To_Final_youtube_1080.mp4 (1920x1080) [207.1 MB] || YOUTUBE_720_13149_GLOBE_Clouds_How_To_Final_youtube_720.mp4 (1280x720) [196.8 MB] || 13149_GLOBE_Clouds_How_To.en_US.srt [2.2 KB] || 13149_GLOBE_Clouds_How_To.en_US.vtt [2.2 KB] || ", "hits": 63 }, { "id": 4733, "url": "https://svs.gsfc.nasa.gov/4733/", "result_type": "Visualization", "release_date": "2019-04-04T00:00:00-04:00", "title": "Hyperwall: Scouting the Apollo 11 Landing Site", "description": "This sequence of images from Apollo 10 looks west across southern Mare Tranquillitatis. The Apollo 11 landing site is circled in green. The bright crater at about 7 o'clock within the circle is West crater. Black and white, 70mm magazine R, AS10-31-4607 to 11. || apollo10_as10-31-4607_print.jpg (1024x345) [81.6 KB] || apollo10_as10-31-4607_searchweb.png (320x180) [47.4 KB] || apollo10_as10-31-4607_thm.png (80x40) [3.9 KB] || apollo10_as10-31-4607.tif (9600x3240) [13.8 MB] || apollo-10-photo-sequence-of-apollo-11-site.hwshow [237 bytes] || ", "hits": 646 }, { "id": 13113, "url": "https://svs.gsfc.nasa.gov/13113/", "result_type": "Produced Video", "release_date": "2018-12-12T15:00:00-05:00", "title": "AGU 2018 - Expected Data and Scientific Discovery from NASA’s Parker Solar Probe", "description": "Animation of NASA's Parker Solar Probe in the solar wind. Credit: NASA/GSFC/CIL/Brian Monroe || 1_Nicky_ParkerBeautyPass_1.00200_print.jpg (1024x576) [34.0 KB] || 1_Nicky_ParkerBeautyPass_1.mp4 (1920x1080) [24.5 MB] || 1_Nicky_ParkerBeautyPass_1.webm (1920x1080) [2.4 MB] || ", "hits": 35 }, { "id": 4572, "url": "https://svs.gsfc.nasa.gov/4572/", "result_type": "Visualization", "release_date": "2018-11-14T14:00:00-05:00", "title": "The Hiawatha Impact Crater", "description": "The series of visualizations below are derived from satellite imagery and radar sounding. They portray both the location and size of the 31-kilometer-wide impact crater beneath Hiawatha Glacier. They also portray the structure of the glacier ice that flows into and fills the crater.The Hiawatha impact crater was first suspected to exist in the summer of 2015, from examination of a compilation of Greenland's sub-ice topography radar measurements made by NASA over two decades. The visualizations of the subsurface shown below are derived from a spring 2016 airborne survey by Germany's Alfred Wegener Institute, using a new ultrawideband radar sounder developed by the Center for Remote Sensing of Ice Sheets at The University of Kansas. Subsequent helicopter visits to the deglaciated terrain in front of Hiawatha Glacier by scientists from the Natural History Museum in Denmark recovered sediment samples from the main river that discharges water from beneath Hiawatha Glacier, through the northwestern rim breach. Laboratory examination revealed that these sediment samples contained shocked quartz and elevated platinum-group-element concentrations, both signs that the sediment records evidence of the impact of an iron asteroid more than one kilometer wide. The Hiawatha impact crater is potentially one of the youngest large impact craters on Earth.In the visualizations below, the elevation of the topography of the bed, the ice surface and the radar curtains have been exaggerated ten times in order to better illustrate their structure. || ", "hits": 189 }, { "id": 4687, "url": "https://svs.gsfc.nasa.gov/4687/", "result_type": "Visualization", "release_date": "2018-09-28T00:00:00-04:00", "title": "El Nino Fueled Rains Swamp South America", "description": "Since the middle of 2015, meteorologists have warned that El Niño could bring unusually wet weather to Paraguay, Uruguay, Argentina, and southern Brazil. The first image shows a view of this region before the flood and the second is after the December/January El Nino rains swamped this part of South America. || OneBeforeAfterFLoodSA-ArgentinaParaguay02.00001_print.jpg (1024x576) [252.4 KB] || OneBeforeAfterFLoodSA-ArgentinaParaguay02.00001_searchweb.png (320x180) [131.8 KB] || OneBeforeAfterFLoodSA-ArgentinaParaguay02.00001_thm.png (80x40) [7.7 KB] || OneBeforeAfterFLoodSA-ArgentinaParaguay02.mp4 (3840x2160) [71.7 MB] || ElNinoFlood (3240x3240) [0 Item(s)] || OneBeforeAfterFLoodSA-ArgentinaParaguay02.webm (3840x2160) [8.8 MB] || rioparaguay02.hwshow [207 bytes] || ", "hits": 62 }, { "id": 13072, "url": "https://svs.gsfc.nasa.gov/13072/", "result_type": "Produced Video", "release_date": "2018-09-19T12:00:00-04:00", "title": "Parker Solar Probe First Light Data", "description": "Just over a month into its mission, Parker Solar Probe has returned first-light data from each of its four instrument suites. These early observations – while not yet examples of the key science observations Parker Solar Probe will take closer to the Sun – show that each of the instruments is working well. The instruments work in tandem to measure the Sun's electric and magnetic fields, particles from the Sun and the solar wind, and capture images of the environment around the spacecraft. The mission’s first close approach to the Sun will be in November 2018, but even now, the instruments are able to gather measurements of what’s happening in the solar wind closer to Earth. || ", "hits": 123 }, { "id": 40359, "url": "https://svs.gsfc.nasa.gov/gallery/sdostillsand-graphics/", "result_type": "Gallery", "release_date": "2018-09-13T10:02:59-04:00", "title": "SDO: Stills and Graphics", "description": "No description available.", "hits": 283 }, { "id": 4678, "url": "https://svs.gsfc.nasa.gov/4678/", "result_type": "Visualization", "release_date": "2018-09-07T00:00:00-04:00", "title": "Rink Glacier Multi-Year Surface Elevation Comparison", "description": "Since 1993, the Airborne Topographic Mapper or ATM has been monitoring elevation changes of 160 outlet glaciers in Greenland, many of them on an almost annual basis. Rink Glacier in central west Greenland is one example of a 25-year-long time series of elevation changes. In these visualizations, elevation data for each aircraft flight over the glacier are illustrated using spheres 1m in diameter, with each sphere representing a specific measurement. When viewed together, the spheres form sheets defining the observed surface of the glacier for a given year. The spheres are colored by year, and over time we can see how the glacier's elevation changes. Towards the end of the visualization, the study area of the Rink Glacier is compared to the future coverage of the Ice, Cloud and land Elevation Satellite-2 (ICESat-2), as represented by bright green crisscrossing ground tracks. || ", "hits": 26 }, { "id": 40358, "url": "https://svs.gsfc.nasa.gov/gallery/sdopresentation-resources/", "result_type": "Gallery", "release_date": "2018-09-07T00:00:00-04:00", "title": "SDO: Presentation Resources", "description": "No description available.", "hits": 64 }, { "id": 40355, "url": "https://svs.gsfc.nasa.gov/gallery/sdo/", "result_type": "Gallery", "release_date": "2018-08-31T00:00:00-04:00", "title": "SDO – Solar Dynamics Observatory", "description": "Since its launch on Feb. 11, 2010, the Solar Dynamics Observatory (SDO) has studied the solar atmosphere to help us understand the Sun’s influence on Earth. Every 12 seconds, SDO images the Sun in 10 wavelengths of ultraviolet light, each of which reveals different solar features. These images help us explain where the Sun's energy comes from, how the inside of the Sun works, and how the Sun’s atmosphere stores and releases energy in dramatic eruptions that can influence Earth.\n\nLearn more: https://science.nasa.gov/mission/sdo/", "hits": 828 }, { "id": 13016, "url": "https://svs.gsfc.nasa.gov/13016/", "result_type": "Produced Video", "release_date": "2018-07-25T00:00:00-04:00", "title": "Mars Evolution from Wet to Dry", "description": "These animations were originally created to accompany Invisible Mars, a Science-on-a-Sphere live presentation for the MAVEN mission. The animations have been rendered for use in other formats, including the NASA Hyperwall. Learn more about MAVEN and about the Lunar and Planetary Institute.Credit: Created for the MAVEN mission by the Lunar and Planetary Institute || ", "hits": 356 }, { "id": 12991, "url": "https://svs.gsfc.nasa.gov/12991/", "result_type": "Produced Video", "release_date": "2018-07-10T14:00:00-04:00", "title": "NASA Surveys Hurricane Damage to Puerto Rico's Forests", "description": "Overview of field expedition to Puerto Rico in April 2018, to survey the recovery of forests since Hurricanes Irma and Maria hit the island seven months before.Complete transcript available.Music: Treehouse Imaginations by Zachary Scott Lemon [BMI]Down Terrace by Damien Deschamps [SACEM]Reloj by Kevin Carbo [BMI]Living Forest by Luca Proietti [SIAE]Watch this video on the NASA Goddard YouTube channel. || 12991-mangroves_and_plane_wing_IMG_0852.jpg (5184x3456) [1.3 MB] || 12991-mangroves_and_plane_wing_IMG_0852_searchweb.png (320x180) [84.2 KB] || 12991-mangroves_and_plane_wing_IMG_0852_thm.png (80x40) [6.2 KB] || 12991_Puerto_Rico_lidar_V2_prores.mov (1920x1080) [8.9 GB] || 12991_Puerto_Rico_lidar_V2_youtube_1080.mp4 (1920x1080) [558.3 MB] || 12991_Puerto_Rico_lidar_V2.mp4 (1920x1080) [328.9 MB] || 12991_Puerto_Rico_lidar_V2_large.mp4 (1920x1080) [343.8 MB] || 12991_Puerto_Rico_lidar_V2_youtube_720.mp4 (1280x720) [563.1 MB] || 12991_Puerto_Rico_lidar_twitter_720.mp4 (1280x720) [78.7 MB] || 12991_Puerto_Rico_lidar.webm (1920x1080) [39.1 MB] || 12991_Puerto_Rico_lidar-captions.en_US.srt [7.4 KB] || 12991_Puerto_Rico_lidar-captions.en_US.vtt [7.4 KB] || ", "hits": 30 }, { "id": 12989, "url": "https://svs.gsfc.nasa.gov/12989/", "result_type": "Produced Video", "release_date": "2018-07-03T11:00:00-04:00", "title": "Superstar Eta Carinae Shoots Cosmic Rays", "description": "Zoom into Eta Carinae, where the outflows of two massive stars collide and shoot accelerated particles cosmic rays into space.Credit: NASA’s Goddard Space Flight Center Music: \"Expectant Aspect\" from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Eta_Car_CR_Still.jpg (1920x1080) [307.1 KB] || Eta_Car_CR_Still_print.jpg (1024x576) [127.9 KB] || Eta_Car_CR_Still_searchweb.png (320x180) [98.2 KB] || Eta_Car_CR_Still_thm.png (80x40) [7.3 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.webm (1920x1080) [16.1 MB] || 12989_Eta_Car_CosmicRay_1080.m4v (1920x1080) [155.6 MB] || 12989_Eta_Car_CosmicRay_1080.mp4 (1920x1080) [234.6 MB] || 12989_Eta_Car_CosmicRay_1080p.mov (1920x1080) [311.6 MB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.srt [2.0 KB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.vtt [2.0 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.mov (1920x1080) [2.1 GB] || ", "hits": 181 }, { "id": 4659, "url": "https://svs.gsfc.nasa.gov/4659/", "result_type": "Visualization", "release_date": "2018-06-27T00:00:00-04:00", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (hydrogen alpha filter)", "description": "This movie is generated from imagery collected by the NSO GONG network of solar observatories. It is not time-synchronized to the related observations by the Solar Dynamics Observatory (SDO). || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_print.jpg (1024x576) [25.1 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_searchweb.png (320x180) [20.9 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_thm.png (80x40) [2.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || BBSO_Halpha_2011JuneUh_HD1080i_p30.mp4 (1920x1080) [2.8 MB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.webm (1920x1080) [1.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || BBSO_Halpha_2011JuneUh_2160p30.mp4 (3840x2160) [11.4 MB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.mp4.hwshow [200 bytes] || ", "hits": 42 }, { "id": 30963, "url": "https://svs.gsfc.nasa.gov/30963/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Probing Kilauea’s Plume", "description": "These images, created using data from the Multi-angle Imaging Spectroradiometer (MISR) on Terra, show the height of the sulfur-rich plume from Hawaii's Kilauea on May 6, 2018. || probing_plume.png (1920x1080) [1.7 MB] || probing_plume_print.jpg (1024x576) [139.0 KB] || probing_plume_searchweb.png (320x180) [78.6 KB] || probing_plume_thm.png (80x40) [6.0 KB] || probing-kilaueas-plume.hwshow [272 bytes] || ", "hits": 26 }, { "id": 30951, "url": "https://svs.gsfc.nasa.gov/30951/", "result_type": "Hyperwall Visual", "release_date": "2018-05-16T10:00:00-04:00", "title": "Supernova Remnant Cassiopeia A from Hubble", "description": "The nebula known as Cassiopeia A is composed of tattered remains of a star that exploded more than 300 years ago. || cas_a_2004_12-hst-10252x7379_print.jpg (1024x737) [249.8 KB] || cas_a_2004_12-hst-10252x7379_searchweb.png (320x180) [100.4 KB] || cas_a_2004_12-hst-10252x7379_thm.png (80x40) [8.7 KB] || cas_a_2004_12-hst-10252x7379.png (10252x7379) [122.0 MB] || supernova-remnant-cassiopeia-a-from-hubble.hwshow [238 bytes] || ", "hits": 136 }, { "id": 40348, "url": "https://svs.gsfc.nasa.gov/gallery/esddatafor-societal-benefits/", "result_type": "Gallery", "release_date": "2018-04-24T00:00:00-04:00", "title": "ESD data for Societal Benefit", "description": "No description available.", "hits": 233 } ] }