{ "count": 214, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Elements%22", "previous": null, "results": [ { "id": 31376, "url": "https://svs.gsfc.nasa.gov/31376/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "SPHEREx All Sky Map 2025", "description": "Two passes of an all-sky mosaic image from NASAs SPHEREx space telescope, the first showing dust and gas and the second showing stars and galaxies.", "hits": 776 }, { "id": 14979, "url": "https://svs.gsfc.nasa.gov/14979/", "result_type": "Produced Video", "release_date": "2026-03-26T14:00:00-04:00", "title": "Early Testing of Aerogel and Silicon Detectors for TIGERISS", "description": "Nick Cannady, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, examines a block of silica aerogel in May 2025. Cannady uses the light weight material in detectors for the upcoming TIGERISS (Trans-Iron Galactic Element Recorder for the International Space Station) mission, which is designed to study high-speed charged particles called cosmic rays.Credit: NASA/Scott WiessingerAlt text: A man studies a transparent block of aerogel.Image description: A man with glasses wearing a blue checkered shirt examines a block of transparent material resting on a table. He is leaning and rests his right hand on the table. The block glows faintly blue. The table is gray with evenly spaced rows of holes. || Tigeriss-Aerogel__Nick_Cannady-3.jpg (6393x4718) [17.4 MB] || Tigeriss-AerogelNick_Cannady-3-small.jpg (3196x2359) [1.6 MB] || ", "hits": 194 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 744 }, { "id": 14884, "url": "https://svs.gsfc.nasa.gov/14884/", "result_type": "Produced Video", "release_date": "2026-01-29T11:00:00-05:00", "title": "NASA Supercomputer Probes Tangled Magnetospheres of Merging Neutron Stars", "description": "New supercomputer simulations explore the tangled magnetic structures around merging neutron stars. These structures, called magnetospheres, interact as the city-sized stars enter their final orbits. Magnetic field lines can connect both stars, break, and reconnect, while currents surge through surrounding plasma moving at nearly the speed of light. The simulations show that these systems may produce X-rays and gamma rays that future observatories should be able to detect. Credit: NASA’s Goddard Space Flight CenterAlt text: Narrated video introducing simulations of merging neutron star magnetospheresMusic: “A Theory Develops,” Pip Heywood [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NS_Binary_Sim_Still.jpg (5760x3240) [1.4 MB] || NS_Binary_Sim_Still_searchweb.png (320x180) [67.6 KB] || NS_Binary_Sim_Still_thm.png (80x40) [5.2 KB] || 14884_NeutronStarBinarySim2_good.mp4 (1920x1080) [220.4 MB] || 14884_NeutronStarBinarySim2_best.mp4 (1920x1080) [363.9 MB] || NeutronStarBinarySimulationCaptions.en_US.srt [2.4 KB] || NeutronStarBinarySimulationCaptions.en_US.vtt [2.2 KB] || 14884_NeutronStarBinarySim2_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || ", "hits": 448 }, { "id": 5609, "url": "https://svs.gsfc.nasa.gov/5609/", "result_type": "Visualization", "release_date": "2026-01-26T05:00:00-05:00", "title": "Heliophysics Satellite Fleet - 2026", "description": "A tour of the NASA Heliophysics fleet from near-Earth satellites out to the Voyagers beyond the heliopause.", "hits": 955 }, { "id": 14946, "url": "https://svs.gsfc.nasa.gov/14946/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Viewing an Exoplanet Transmission Spectrum", "description": "When planets orbiting distant stars are aligned just right, a host star's light can pass through its planet's atmosphere before reaching our telescopes. This alters the light, and by analyzing its spectrum, astronomers can find out what the planet’s atmosphere is made of. This animation is a quick visual representation of that process. || ", "hits": 347 }, { "id": 14945, "url": "https://svs.gsfc.nasa.gov/14945/", "result_type": "Produced Video", "release_date": "2026-01-09T09:00:00-05:00", "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars", "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ", "hits": 433 }, { "id": 14930, "url": "https://svs.gsfc.nasa.gov/14930/", "result_type": "Infographic", "release_date": "2025-12-18T10:00:00-05:00", "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles", "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel", "hits": 147 }, { "id": 14933, "url": "https://svs.gsfc.nasa.gov/14933/", "result_type": "Produced Video", "release_date": "2025-12-04T09:00:00-05:00", "title": "XRISM Finds Elemental Bounty in Supernova Remnant", "description": "Observations of the Cassiopeia A supernova remnant by the Resolve instrument aboard the NASA-JAXA XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft revealed strong evidence for potassium (green squares) in the southeast and northern parts of the remnant. Grids superposed on a multiwavelength image of the remnant represent the fields of view of two Resolve measurements made in December 2023. Each square represents one pixel of Resolve’s detector. Weaker evidence of potassium (yellow squares) in the west suggests that the original star may have had underlying asymmetries before it exploded. Credit: NASA’s Goddard Space Flight Center; X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandAlt text: The Cassiopeia A supernova remnant with the XRISM Resolve fields of viewImage description: Supernova remnant Cassiopeia A appears as a large circular object outlined by electric blue filaments, set against a black background. Strings of vibrant colors weave throughout, with blue representing Chandra data, red, green, and blue representing Webb data, and Hubble data showing a multitude of stars that dot the view. Two nearly square grids are laid on top of the remnant slightly overlapping. The upper grid has six squares filled yellow, representing weaker evidence for potassium. In the opposite corner of that grid, five squares are filled green, representing a positive potassium detection. The lower grid has six boxes filled green in a wide M-like shape. The image is labeled “North” at the top center, “West” on the right, and “Southeast” to the left. || cas_a_with_resolve_1.png (800x645) [96.7 KB] || cas_a_with_resolve_1_print.jpg (1024x825) [125.5 KB] || cas_a_with_resolve_1_searchweb.png (320x180) [120.5 KB] || cas_a_with_resolve_1_web.png (320x258) [161.2 KB] || cas_a_with_resolve_1_thm.png (80x40) [7.6 KB] || ", "hits": 309 }, { "id": 5535, "url": "https://svs.gsfc.nasa.gov/5535/", "result_type": "Visualization", "release_date": "2025-08-15T09:05:00-04:00", "title": "What Apollo Saw in Sunlight While in Orbit", "description": "A map showing the sunlit parts of the lunar surface that the Apollo astronauts could see from orbit. The darkened parts of the map were either never in sunlight or were beyond the horizon of the spacecraft.", "hits": 5410 }, { "id": 14881, "url": "https://svs.gsfc.nasa.gov/14881/", "result_type": "Animation", "release_date": "2025-08-13T00:00:00-04:00", "title": "Fermi Spacecraft Animations 2025", "description": "A beauty pass of NASA's Fermi Gamma-ray Space Telescope. The spacecraft fills the frame with a starry background at 0:05 and is fully in frame with Earth partially in the background at 0:11.Credit: NASA's Goddard Space Flight Center/CI Lab || Fermi_Beauty_Still.jpg (3840x2160) [250.1 KB] || Fermi_Beauty_Still_searchweb.png (320x180) [11.5 KB] || Fermi_Beauty_Still_thm.png (80x40) [1.6 KB] || Fermi_BeautyPass_1080.mp4 (1920x1080) [46.1 MB] || Fermi_BeautyPass_4k.mp4 (3840x2160) [113.7 MB] || Fermi_BeautyPass_V002_ProRes_4k.mov (3840x2160) [1.3 GB] || ", "hits": 98 }, { "id": 14868, "url": "https://svs.gsfc.nasa.gov/14868/", "result_type": "Produced Video", "release_date": "2025-07-23T00:00:00-04:00", "title": "XRISM Satellite X-rays Milky Way’s Sulfur in Detail", "description": "An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft.Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos.Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears.Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements.When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient's body, creating contrast in the detector.Scientists did something similar by picking a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed.Then they selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius.Using the Resolve instrument on XRISM, the researchers were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron.Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. XRISM’s observations could match a few of these compounds — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold.The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. || ", "hits": 95 }, { "id": 5571, "url": "https://svs.gsfc.nasa.gov/5571/", "result_type": "Visualization", "release_date": "2025-07-22T17:00:00-04:00", "title": "NASA's Fleet of Active Satellites (July 2025)", "description": "This visualization shows the orbits of NASA satellites considered operational as of July 2025. It includes both NASA-managed missions and those operated by partner organizations.", "hits": 1740 }, { "id": 5532, "url": "https://svs.gsfc.nasa.gov/5532/", "result_type": "Visualization", "release_date": "2025-07-18T08:00:00-04:00", "title": "Comparing ISS and ICESat-2 Coverage Across the Earth", "description": "These visualizations explore the orbits of the International Space Station (ISS) and the ICESat-2 satellite. The ISS reaches a maximum latitude of approximately ±51.6°, while ICESat-2 extends to about ±88°, allowing it to observe much closer to the poles.", "hits": 133 }, { "id": 14867, "url": "https://svs.gsfc.nasa.gov/14867/", "result_type": "Produced Video", "release_date": "2025-07-15T14:00:00-04:00", "title": "GEMx Animations", "description": "Conceptual animation illustrating the ER-2 aircraft collecting spectroscopic mineral data over the American West. || GEMxThumbnail.png (1948x1052) [1.5 MB] || GEMxThumbnail_print.jpg (1024x553) [118.0 KB] || GEMxThumbnail_searchweb.png (320x180) [55.7 KB] || GEMxThumbnail_thm.png (80x40) [8.2 KB] || GEMx_Interface_1080p.mov (1920x1080) [37.6 MB] || GEMx_Interface_4k.mp4 (3840x2160) [36.0 MB] || GEMx_Interface_ProRes.mov (3840x2160) [4.1 GB] || ", "hits": 54 }, { "id": 5258, "url": "https://svs.gsfc.nasa.gov/5258/", "result_type": "Visualization", "release_date": "2025-06-16T00:00:00-04:00", "title": "Tracking Satellites and Space Debris in Earth Orbit (Feb 2024)", "description": "This series of visualizations illustrates the population of objects orbiting Earth as of February 2024.", "hits": 3275 }, { "id": 14793, "url": "https://svs.gsfc.nasa.gov/14793/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Black Holes Vertical Video", "description": "This page collects Astrophysics vertical videos with black-hole-related content", "hits": 1400 }, { "id": 14802, "url": "https://svs.gsfc.nasa.gov/14802/", "result_type": "Produced Video", "release_date": "2025-03-28T14:31:59-04:00", "title": "Earth to Space: A National Symphony Orchestra Concert", "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.", "hits": 117 }, { "id": 20399, "url": "https://svs.gsfc.nasa.gov/20399/", "result_type": "Animation", "release_date": "2025-03-19T00:00:00-04:00", "title": "XMM-Newton spacecraft animations", "description": "Flyby animation of ESA's (European Space Agency's) XMM-Newton observatory as it orbits Earth.Credit: NASA/ESA || XMM_Beauty_Still.jpg (3840x2160) [449.2 KB] || XMM_Beauty_Still_searchweb.png (320x180) [38.6 KB] || XMM_Beauty_Shot_H264_V1.mp4 (3840x2160) [23.4 MB] || XMM_Beauty_Still_thm.png [3.3 KB] || XMM_Beauty_Shot_Prores_V1.mov (3840x2160) [807.2 MB] || ", "hits": 87 }, { "id": 14739, "url": "https://svs.gsfc.nasa.gov/14739/", "result_type": "Produced Video", "release_date": "2025-01-03T12:00:00-05:00", "title": "From the Moon, NASA’s LEXI Will Reveal Earth’s Magnetic Shield", "description": "NASA’s next mission to the Moon will carry an instrument called LEXI (the Lunar Environment Heliospheric X-ray Imager), which will provide the first-ever global view of the magnetic environment that shields Earth from solar radiation.From the surface of the Moon, LEXI will capture wide-field images of Earth's magnetic environment, or magnetosphere, in low-energy (or \"soft\") X-rays. LEXI will study changes in the magnetosphere and help us learn more about how it interacts with a stream of particles from the Sun called the solar wind, which can pose hazards for Artemis astronauts traveling to the Moon.Learn more about LEXI and its CLPS (Commercial Lunar Payload Services) flight to the Moon from Hyunju Connor, LEXI co-investigator at NASA’s Goddard Space Flight Center.More on LEXI: https://science.nasa.gov/science-research/heliophysics/nasas-lexi-will-provide-x-ray-vision-of-earths-magnetosphere/ || ", "hits": 198 }, { "id": 5443, "url": "https://svs.gsfc.nasa.gov/5443/", "result_type": "Visualization", "release_date": "2024-12-17T00:00:00-05:00", "title": "Heliophysics Sentinels 2024", "description": "There have been some changes since the 2022 Heliophysics Fleet. AIM and ICON have been decommissioned while two other instruments have been added. AWE is an instrument mounted on the ISS, and RAD is a particle detector on the Curiosity Mars rover. As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause. || ", "hits": 75 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 597 }, { "id": 14715, "url": "https://svs.gsfc.nasa.gov/14715/", "result_type": "Produced Video", "release_date": "2024-11-18T00:00:00-05:00", "title": "COBE Celebrates 35th Launch Anniversary", "description": "Technicians work on the COBE (Cosmic Background Explorer) spacecraft in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission launched into an Earth orbit in 1989 to make an all-sky map of the cosmic microwave background, the oldest light in the universe. The conical silver shield protects the scientific instruments from direct radiation from the Sun and Earth, isolates them from radio-frequency interference from the spacecraft transmitters and terrestrial sources, and provides thermal isolation for a dewar containing liquid helium coolant.Credit: NASA/COBE Science Team || COBE_in_gfsc_clean_room_1.jpg (1629x1600) [552.8 KB] || ", "hits": 221 }, { "id": 14677, "url": "https://svs.gsfc.nasa.gov/14677/", "result_type": "Produced Video", "release_date": "2024-10-02T10:00:00-04:00", "title": "NASA's TESS Spots Record-breaking Stellar Triplets", "description": "This artist’s concept illustrates how tightly the three stars in the system called TIC 290061484 orbit each other. If they were placed at the center of our solar system, all the stars’ orbits would be contained a space smaller than Mercury’s orbit around the Sun. The sizes of the triplet stars and the Sun are also to scale.Credit: NASA’s Goddard Space Flight Center || TESS_Triple_system_beauty_scale.jpg (3840x2160) [775.5 KB] || ", "hits": 483 }, { "id": 14681, "url": "https://svs.gsfc.nasa.gov/14681/", "result_type": "Produced Video", "release_date": "2024-10-01T11:00:00-04:00", "title": "Launch Your Creativity with Space Crafts", "description": "In honor of the completion of our Nancy Grace Roman Space Telescope’s spacecraft — the vehicle that will maneuver the observatory to its place in space and enable it to function once there — we’re bringing you some space crafts you can complete at home! || ", "hits": 77 }, { "id": 14603, "url": "https://svs.gsfc.nasa.gov/14603/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "NICER Hardware and Patch Kit", "description": "This video shows different components of NICER (Neutron star Interior Composition Explorer). The damaged thermal shield is a flight spare used during the patch testing process.0:00 A NICER patch slowly rotates counterclockwise. 0:14 A top-down view of the same patch, still rotating. 0:21 Another side view of the patch rotating. A gloved hand enters from the right-hand side, picks up the patch, and turns it on its side. The patch begins rotating again, so the tab on the bottom becomes visible. 1:03 A gloved hand slowly tilts a damaged thermal shield. 1:41 The thermal shield rests in a container that slowly rotates. 2:08 A gloved hand rotates a NICER X-ray concentrator. 2:30The camera moves past the X-ray concentrator. 2:52 A hand places a NICER sunshade on the table. 2:58 The sunshade rotates counterclockwise. 3:00 The sunshade rotates on its side.Credit:NASA/Sophia Roberts and Scott Wiessinger || Studio_Shoot_Single_Components.00001_print.jpg (1024x540) [16.9 KB] || Studio_Shoot_Single_Components.00001_searchweb.png (320x180) [23.1 KB] || Studio_Shoot_Single_Components.00001_thm.png (80x40) [2.1 KB] || Studio_Shoot_Single_Components.mp4 (4096x2160) [1.9 GB] || Studio_Shoot_Single_Components.mov (4096x2160) [12.7 GB] || ", "hits": 37 }, { "id": 31294, "url": "https://svs.gsfc.nasa.gov/31294/", "result_type": "Hyperwall Visual", "release_date": "2024-06-17T00:00:00-04:00", "title": "PACE Observes Namesake Plankton, Aerosols, Clouds and Ocean Ecosystem", "description": "Beautiful images from PACE show phytoplankton being swirled about by ocean currents of the coast off North America and in the Black Sea. || ", "hits": 103 }, { "id": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 316 }, { "id": 14581, "url": "https://svs.gsfc.nasa.gov/14581/", "result_type": "Produced Video", "release_date": "2024-05-23T10:00:00-04:00", "title": "Gliese 12 b: An Intriguing World Sized Between Earth and Venus", "description": "Gliese 12 b’s estimated size may be as large as Earth or slightly smaller — comparable to Venus in our solar system. This artist’s concept compares Earth with different possible Gliese 12 b interpretations, from no atmosphere to a thick Venus-like one. Follow-up observations with NASA’s James Webb Space Telescope will help determine just how much atmosphere the planet retains as well as its composition.Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)Alt text: Illustration of Earth compared to various models of Gliese 12 b Image description: At left, against a black background, floats an artist's concept of a nearly half-illuminated Earth, with clouds, blue oceans, and land areas rendered in green, tan, brown, and white. At right are three similarly illuminated planets, slightly smaller than Earth and each representing a possible interpretation of Gliese 12 b. The version on the left has a surface of blotchy reddish and brownish features and no atmosphere. The middle version has the same surface texture partly obscured by a hazy atmosphere. And the rightmost and smallest version of the planet has a thick, Venus-like atmosphere that obscures the surface completely. || Gl12b_Earth_Comparison_ac.jpg (3840x2160) [935.8 KB] || Gl12b_Earth_Comparison_ac_print.jpg (1024x576) [126.0 KB] || Gl12b_Earth_Comparison.jpg (3840x2160) [929.5 KB] || Gl12b_Earth_Comparison_ac_searchweb.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_web.png (320x180) [54.4 KB] || Gl12b_Earth_Comparison_ac_thm.png (80x40) [9.8 KB] || Gl12b_Earth_Comparison.tif (3840x2160) [6.4 MB] || ", "hits": 489 }, { "id": 14584, "url": "https://svs.gsfc.nasa.gov/14584/", "result_type": "Produced Video", "release_date": "2024-05-08T09:00:00-04:00", "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy", "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ", "hits": 147 }, { "id": 14574, "url": "https://svs.gsfc.nasa.gov/14574/", "result_type": "Produced Video", "release_date": "2024-05-06T10:00:00-04:00", "title": "Black Hole Week 2024 Poster and Media", "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.", "hits": 235 }, { "id": 14463, "url": "https://svs.gsfc.nasa.gov/14463/", "result_type": "Produced Video", "release_date": "2024-04-30T11:00:00-04:00", "title": "XRISM Mission Captures Unmatched Data With Just 36 Pixels", "description": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XRISM_36_Pixels_Still.jpg (1920x1080) [959.9 KB] || XRISM_36_Pixels_Still_searchweb.png (320x180) [94.7 KB] || XRISM_36_Pixels_Still_thm.png (80x40) [7.0 KB] || 14463_XRISM_36Pixels_Good.mp4 (1920x1080) [148.9 MB] || 14463_XRISM_36Pixels_Best.mp4 (1920x1080) [514.8 MB] || 14463_XRISM_36Pixels_Captions.en_US.srt [4.6 KB] || 14463_XRISM_36Pixels_Captions.en_US.vtt [4.4 KB] || 14463_XRISM_36Pixels_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || ", "hits": 79 }, { "id": 31273, "url": "https://svs.gsfc.nasa.gov/31273/", "result_type": "Hyperwall Visual", "release_date": "2024-01-31T00:00:00-05:00", "title": "NASA Telescopes Chase Down \"Green Monster\" in Star's Debris", "description": "Animations of images originally published at https://chandra.harvard.edu/photo/2024/casa/ and https://www.nasa.gov/image-article/nasa-telescopes-chase-down-green-monster-in-stars-debris/.Astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure called the “Green Monster”. Composite images from Chandra, Webb, Hubble, NuSTAR, and Spitzer reveal where elements such as silicon, iron, and titanium are located. Comparing where certain elements are with the location of the blast wave, researchers conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it. || ", "hits": 33 }, { "id": 14491, "url": "https://svs.gsfc.nasa.gov/14491/", "result_type": "Produced Video", "release_date": "2023-12-26T00:00:00-05:00", "title": "Roman Hardware Highlights", "description": "This video, covering the second half of 2025, opens with a person entering NASA’s Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility. The room is a class 10,000 clean room with over one million cubic feet of space.The outside half of Roman, called OSD, contains the solar panels and protective layers. The Deployable Aperture Cover, which protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces, which Roman will not experience in space. Then the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit inside the rocket fairing and then deploy in space to make a large flat plane that both collects light to generate electricity and helps keep the rest of Roman cool.In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right, and forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is behaving as they anticipated.While these tests occur, Roman’s inside half, containing the mirrors, instruments and support equipment, move into Goddard’s largest thermal vacuum chamber, the SES (Space Environment Simulator). This 40-foot-tall chamber can simulate the vacuum of space and the wide temperature range that Roman will experience there: from -310° Fahrenheit (-190° C) to 302° Fahrenheit (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned both horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.Music credit: “Our Journey Begins,” Dan Thiessen [BMI], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Roman_Hardware_Highlights_SummerFall2025_3.jpg (1280x720) [473.7 KB] || Roman_HH_Summer-Fall2025_10mbps.mp4 (1920x1080) [185.0 MB] || Roman_HH_Summer-Fall2025_25mbps.mp4 (1920x1080) [452.7 MB] || Roman_HH_Summer-Fall2025_YT.mp4 (1920x1080) [880.2 MB] || RomanHHLate2025Captions.en_US.srt [588 bytes] || RomanHHLate2025Captions.en_US.vtt [570 bytes] || Roman_HH_Summer-Fall2025_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || ", "hits": 219 }, { "id": 5157, "url": "https://svs.gsfc.nasa.gov/5157/", "result_type": "Visualization", "release_date": "2023-11-28T09:20:00-05:00", "title": "Fermi Catalog of Gamma-ray Pulsars", "description": "A visualization of the 294 pulsars in the Fermi gamma-ray pulsar catalog. The visualization starts with a full-sky Hammer projection view of the catalog. Different types of pulsars are indicated by different markers. The pulsar markers oscillate in size according to the object's pulsation frequency at actual speed. Millisecond pulsars are just shown as solid markers. The map then morphs into the full 3D view of the pulsar distribution, and we then fly out to give a top down view showing the distribution of gamma-ray pulsars in our galaxy. || pulsar3DMap_2160p30.00200_print.jpg (1024x576) [174.0 KB] || pulsar3DMap_2160p30.00200_searchweb.png (320x180) [72.3 KB] || pulsar3DMap_2160p30.00200_thm.png (80x40) [5.4 KB] || full (3840x2160) [0 Item(s)] || pulsar3DMap_2160p30.mp4 (3840x2160) [240.8 MB] || ", "hits": 136 }, { "id": 14401, "url": "https://svs.gsfc.nasa.gov/14401/", "result_type": "Produced Video", "release_date": "2023-10-31T10:00:00-04:00", "title": "NASA’s Eclipse Art", "description": "“The greatest scientists are artists as well.” ~Albert EinsteinArt and science have been treated as separate disciplines but have more in common than is often realized. Creativity is critical to making scientific breakthroughs, and art is often an expression (or product) of scientific knowledge. And both art and science begin in the experience of awe, of beholding something grand. The experience of a solar eclipse is a prime example of where these two human endeavors meet.Eclipses are celestial events we can predict with extreme precision, and their occurrence reveals fundamental truths about our place in the universe. Yet, as many eclipse watchers will attest, there is no anticipating how you will feel when experiencing one. The emotional resonance of eclipses is underlined by their presence in artforms in cultures across the world going back millennia.To celebrate the special role of eclipses in connecting art and science, creatives across NASA will be sharing their eclipse-inspired artwork in anticipation of two solar eclipses that will cross the United States on October 14, 2023, and April 8, 2024.The first two pieces in the series are presented below, with short biographies of their creators. || ", "hits": 83 }, { "id": 40502, "url": "https://svs.gsfc.nasa.gov/gallery/2024total-solar-eclipse-gallery/", "result_type": "Gallery", "release_date": "2023-10-31T00:00:00-04:00", "title": "2024 Total Solar Eclipse", "description": "On April 8, 2024, a total solar eclipse will cross North America, passing over Mexico, the United States, and Canada. A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. The sky will darken as if it were dawn or dusk.A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. People viewing the eclipse from locations where the Moon’s shadow completely covers the Sun – known as the path of totality – will experience a total solar eclipse. The sky will darken, as if it were dawn or dusk. Weather permitting, people along the path of totality will see the Sun’s corona, or outer atmosphere, which is usually obscured by the bright face of the Sun.Learn more about this total solar eclipse: solarsystem.nasa.gov/eclipses/2024\n", "hits": 412 }, { "id": 14420, "url": "https://svs.gsfc.nasa.gov/14420/", "result_type": "Produced Video", "release_date": "2023-10-02T12:00:00-04:00", "title": "Heliophysics Big Year Graphic Elements", "description": "The Heliophysics Big Year is a NASA-led public engagement campaign designed to promote heliophysics broadly, make heliophysics science and information accessible to all, and showcase ongoing efforts to understand the Sun and all that it touches. We are challenging the public to participate in as many Sun science activities as possible from October 2023 to December 2024, leading up to and around solar maximum.This page contains graphic elements for use in promotion and support of the Heliophysics Big Year. Anyone supporting the Heliophysics Big Year effort may use these resources in accordance with the guidance listed in the captions. || ", "hits": 63 }, { "id": 5169, "url": "https://svs.gsfc.nasa.gov/5169/", "result_type": "Interactive", "release_date": "2023-10-02T09:00:00-04:00", "title": "NASA Eclipse Explorer: An interactive guide to the 2017, 2023, and 2024 Solar Eclipses", "description": "|| An embedded version of the NASA Eclipse Explorer. The standalone version is available at https://go.nasa.gov/EclipseExplorer. || eclipse_explorer_screenshot_print.jpg (1024x661) [170.8 KB] || eclipse_explorer_screenshot.png (3456x2234) [6.1 MB] || eclipse_explorer_screenshot_searchweb.png (320x180) [73.4 KB] || eclipse_explorer_screenshot_thm.png (80x40) [8.9 KB] ||", "hits": 107 }, { "id": 40500, "url": "https://svs.gsfc.nasa.gov/gallery/annular-solar-eclipse2023/", "result_type": "Gallery", "release_date": "2023-09-19T00:00:00-04:00", "title": "2023 Annular Solar Eclipse", "description": "On Oct. 14, 2023, an annular solar eclipse will cross North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere can experience this eclipse.\n\nAn annular solar eclipse happens when the Moon passes between the Sun and Earth while it is at or near its farthest point from Earth. Because the Moon is farther away from Earth than usual, it appears smaller than the Sun and does not completely cover the star. Because of this, the Sun will appear like a “ring of fire” in the sky for those in the path of annularity.\n\nDuring an annular eclipse, it is never safe to look directly at the Sun without specialized eye protection designed for solar viewing.\n\nLearn more about this annular solar eclipse: solarsystem.nasa.gov/eclipses/2023", "hits": 129 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth 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": 255 }, { "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": 339 }, { "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Heliophysics 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": 195 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 53 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 978 }, { "id": 31237, "url": "https://svs.gsfc.nasa.gov/31237/", "result_type": "Hyperwall Visual", "release_date": "2023-07-26T00:00:00-04:00", "title": "Ozonewatch 2022", "description": "Plots showing the size of the ozone hole between 1979 and 2022. || 2022-ozone-all-elements_print.jpg (1024x576) [89.7 KB] || 2022-ozone-all-elements.png (3840x2160) [1.2 MB] || 2022-ozone-all-elements_searchweb.png (320x180) [37.1 KB] || 2022-ozone-all-elements_thm.png (80x40) [4.3 KB] || 2022-ozone-all-elements.hwshow [77 bytes] || ", "hits": 107 }, { "id": 14344, "url": "https://svs.gsfc.nasa.gov/14344/", "result_type": "B-Roll", "release_date": "2023-05-05T15:00:00-04:00", "title": "Roman's Primary Structure - B-Roll Footage", "description": "The primary structure that will serve as the “bones” of NASA’s Nancy Grace Roman Space Telescope has moved into the big clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The spacecraft bus, Roman’s primary support element, will now be built upon this skeletal framework. Roman will help unravel the secrets of dark energy and dark matter, search for and image exoplanets, and explore many topics in infrared astrophysics.It’s partly made up of a central cylinder with a top deck that will support most of the observatory. Each of its six sides has a compartment that will house key electronics and other hardware needed to operate the observatory. Major spacecraft elements, such as its power, attitude control and propulsion systems, will be housed within the primary structure. The high-gain antenna will be installed beneath it, and the lowermost part of the primary structure will attach the spacecraft to the rocket during launch.The structure is mainly made of a special grade of aluminum that’s strong, yet lightweight. To reduce the weight even further, most of its exterior is partly hollowed out in a triangular pattern called an isogrid. Even though it’s large – about 14 feet (4.3 meters) long, 12 feet (3.7 meters) wide, and 6.5 feet (2 meters) tall – the primary structure weighs just 3,600 pounds (1,600 kilograms). || ", "hits": 89 }, { "id": 5093, "url": "https://svs.gsfc.nasa.gov/5093/", "result_type": "Visualization", "release_date": "2023-04-14T09:00:00-04:00", "title": "Solar Eclipse Animation Elements", "description": "Due to their relative scale and distances, the disks of the Sun and the Moon appear to be almost the same size in the sky when standing on Earth. This means that even though the Moon is much smaller than the Sun, it can block most or all of the Sun's light, resulting in a dark shadow over Earth called a solar eclipse.These videos are designed to help describe some of the dynamics that determine how solar eclipses work and why they are important for those of us living on Earth. || ", "hits": 389 }, { "id": 14283, "url": "https://svs.gsfc.nasa.gov/14283/", "result_type": "Produced Video", "release_date": "2023-01-27T09:00:00-05:00", "title": "Trumpler 14", "description": "Trumpler 14 is located 8,000 light-years away in the Carina Nebula, a huge star formation region. This 500,000-year-old star cluster has one of the highest concentrations of massive stars in our entire Milky Way Galaxy.A small nugget of cold molecular hydrogen, called a Bok globule, is silhouetted subtly against the star cluster.Furiously burning their hydrogen fuel, the cluster’s blue-white stars will soon explode as supernovae in a few million years. The combination of stellar ‘winds’ and supernova blast waves will carve out cavities for a new generation of stars to be born.This image was made with data from 2005 and 2006 taken with Hubble’s Advanced Camera for Surveys. It combines blue, visible, and infrared broadband filters that combine with filters that isolate the emissions of elements such as oxygen and nitrogen from the glowing gas that surrounds the cluster.Image credit: NASA, ESA, and J. Maíz Apellániz (Institute of Astrophysics of Andalusia, Spain); Acknowledgment: N. Smith (University of Arizona)For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Music credit: “Do What You Love” by Sinan Hosgel [GEMA] via Berlin Production Music [GEMA] and Universal Production Music || ", "hits": 41 }, { "id": 14254, "url": "https://svs.gsfc.nasa.gov/14254/", "result_type": "Produced Video", "release_date": "2022-12-07T13:00:00-05:00", "title": "NASA Intv Opportunity: Record-Breaking Artemis I Mission will Splashdown on Dec. 11th Live Shots", "description": "Media resources including b-roll can be found here https://www.nasa.gov/content/artemis-i-media-resources || Artemis_1_Banner-3.png (1200x480) [429.1 KB] || Artemis_1_Banner-3_print.jpg (1024x409) [72.4 KB] || Artemis_1_Banner-3_searchweb.png (320x180) [58.7 KB] || Artemis_1_Banner-3_thm.png (80x40) [5.3 KB] || ", "hits": 368 }, { "id": 14255, "url": "https://svs.gsfc.nasa.gov/14255/", "result_type": "Produced Video", "release_date": "2022-12-07T11:00:00-05:00", "title": "NASA’s Fermi, Swift Capture Revolutionary Gamma-Ray Burst", "description": "Watch to learn how an event called GRB 211211A rocked scientists’s understanding of gamma-ray bursts – the most powerful explosions in the cosmos.Credit: NASA’s Goddard Space Flight CenterMusic Credits: \"Finished Plate\" by Airglo and \"Binary Fission\" by Tom KaneWatch this video on the NASA Goddard YouTube channel. || Title_Card_Revolutionary_GRB.jpg (1920x1080) [1.5 MB] || Title_Card_Revolutionary_GRB_searchweb.png (320x180) [100.7 KB] || Title_Card_Revolutionary_GRB_thm.png (80x40) [7.3 KB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.mp4 (1920x1080) [171.9 MB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst_ProRes.mov (1920x1080) [2.2 GB] || NASA’s_Fermi,_Swift_Capture_Revolutionary_Gamma-Ray_Burst.webm (1920x1080) [18.4 MB] || Long_GRB_Captions.en_US.srt [2.8 KB] || Long_GRB_Captions.en_US.vtt [2.8 KB] || ", "hits": 155 }, { "id": 4898, "url": "https://svs.gsfc.nasa.gov/4898/", "result_type": "Visualization", "release_date": "2022-11-23T00:00:00-05:00", "title": "Heliophysics Sentinels 2022", "description": "There has been one significant change since the 2020 Heliophysics Fleet. SET has been decommissioned. As of Fall 2022, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 43 }, { "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": 33 }, { "id": 31201, "url": "https://svs.gsfc.nasa.gov/31201/", "result_type": "Hyperwall Visual", "release_date": "2022-10-26T00:00:00-04:00", "title": "Ozonewatch 2021", "description": "Plots showing the size of the ozone hole. || 2021-ozone-all-elements_print.jpg (1024x576) [107.5 KB] || 2021-ozone-all-elements.png (3840x2160) [1.5 MB] || 2021-ozone-all-elements_searchweb.png (320x180) [44.0 KB] || 2021-ozone-all-elements_thm.png (80x40) [4.7 KB] || ozonewatch-2021-season.hwshow [292 bytes] || ", "hits": 71 }, { "id": 14211, "url": "https://svs.gsfc.nasa.gov/14211/", "result_type": "Produced Video", "release_date": "2022-09-20T07:30:00-04:00", "title": "SAM: 10 Years at Gale Crater", "description": "Watch this video on the NASA Goddard Instagram Page.Music is \"Good Omens\" by Count Zero and Rohan Stevenson and \"Lightspeed\" by Gresby Race Nash of Universal Production Music || 14211_SAM_REEL.00145_print.jpg (1024x1820) [183.2 KB] || 14211_SAM_REEL.00145_searchweb.png (320x180) [65.0 KB] || 14211_SAM_REEL.00145_thm.png (80x40) [5.9 KB] || 14211_SAM_REEL.mp4 (1080x1920) [196.8 MB] || 14211_SAM_REEL.webm (1080x1920) [11.7 MB] || sam_reel.en_US.srt [2.6 KB] || sam_reel.en_US.vtt [2.5 KB] || ", "hits": 41 }, { "id": 14181, "url": "https://svs.gsfc.nasa.gov/14181/", "result_type": "Produced Video", "release_date": "2022-08-04T13:00:00-04:00", "title": "Roman Interactive Stills", "description": "Right-side view of the Roman Space Telescope. Highlighted parts available under \"Download Options\" || ROMAN_interactive_Spacecraft_V009_R_Off_2080_print.jpg (1024x576) [57.5 KB] || ROMAN_interactive_V009_R_Roman_off_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080.png (2080x1170) [751.5 KB] || ROMAN_interactive_V009_R_Roman_on_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_V009_R_Roman_comms_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Comms_2080.png (2080x1170) [771.3 KB] || ROMAN_interactive_V009_R_Roman_support_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Support_2080.png (2080x1170) [768.7 KB] || ROMAN_interactive_V009_R_Roman_tele_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_Tele_2080.png (2080x1170) [776.8 KB] || ROMAN_interactive_V009_R_Roman_SP_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_SP_2080.png (2080x1170) [786.4 KB] || ROMAN_interactive_V009_R_Roman_WFI_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_WFI_2080.png (2080x1170) [772.1 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_searchweb.png (320x180) [26.4 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_thm.png (80x40) [3.0 KB] || ", "hits": 47 }, { "id": 14188, "url": "https://svs.gsfc.nasa.gov/14188/", "result_type": "Produced Video", "release_date": "2022-07-21T14:00:00-04:00", "title": "Behind the Scenes of Elements of Webb", "description": "Sophia Roberts and Mike McClare talk about what it took to produce the Elements of Webb series.Music: \"Aquiver,\" \"Crystalline,\" \"Tinderbox,\" \"Spring into Life,\" Universal Production MusicComplete transcript available. || BTSElementsthumb_print.jpg (1024x623) [144.7 KB] || BTSElementsthumb.png (2996x1824) [7.8 MB] || BTSElementsthumb_searchweb.png (320x180) [101.7 KB] || BTSElementsthumb_thm.png (80x40) [11.2 KB] || BTS_Elements_of_Webb-final.mov (1920x1080) [3.0 GB] || BTS_Elements_of_Webb-final.mp4 (1920x1080) [343.1 MB] || BTS_Elements_of_Webb-final.webm (1920x1080) [24.3 MB] || BTS_Elements.en_US.srt [4.8 KB] || BTS_Elements.en_US.vtt [4.5 KB] || ", "hits": 44 }, { "id": 40440, "url": "https://svs.gsfc.nasa.gov/gallery/2022goddard-summer-film-fest/", "result_type": "Gallery", "release_date": "2022-07-19T00:00:00-04:00", "title": "2022 Goddard Summer Film Fest", "description": "See highlights of Goddard’s achievements over the past year in astrophysics, Earth science, heliophysics and planetary science. Highlights will include missions such as the James Webb Space Telescope, OSIRIS-REx, Landsat 9, Hubble Space Telescope, Parker Solar Probe, Fermi, ICESat-2, Lunar Reconnaissance Orbiter, Lucy and much more.", "hits": 81 }, { "id": 14146, "url": "https://svs.gsfc.nasa.gov/14146/", "result_type": "Produced Video", "release_date": "2022-05-04T00:00:00-04:00", "title": "Black Hole Desktop & Phone Wallpapers", "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ", "hits": 9484 }, { "id": 4996, "url": "https://svs.gsfc.nasa.gov/4996/", "result_type": "Visualization", "release_date": "2022-05-02T10:15:00-04:00", "title": "An Orrery of Black Holes and Their Companions", "description": "Full visualization of the binary system black hole orrery with labels and legend included.Credit: NASA's Scientific Visualization Studio || explainerComp_5-27-2022a_2160p60.02000_print.jpg (1024x576) [54.7 KB] || explainerComp_5-27-2022a (3840x2160) [0 Item(s)] || explainerComp_5-27-2022a_2160p60.mp4 (3840x2160) [35.7 MB] || explainerComp_5-27-2022a_2160p60.webm (3840x2160) [26.6 MB] || ", "hits": 126 }, { "id": 4982, "url": "https://svs.gsfc.nasa.gov/4982/", "result_type": "Visualization", "release_date": "2022-04-21T09:00:00-04:00", "title": "Complete 2021 Hurricane Season", "description": "This special version of the 2021 Hurricane Season data visualization uses all the below layers to show the entire 2021 Hurricane Season, but elements of it were sped up in post production to accelerate the data when no hurricanes are present. This provides the viewer with a more compact experience that focuses exclusively on the hurricanes. || hurr2021_comp5speed_2160p30.04733_print.jpg (1024x576) [248.6 KB] || hurr2021_speedComp7_1080p30.mp4 (1920x1080) [437.0 MB] || Sample_Speed_Composite (3840x2160) [0 Item(s)] || hurr2021_speedComp7.webm (3840x2160) [91.3 MB] || hurr2021_speedComp7.mp4 (3840x2160) [197.5 MB] || ", "hits": 86 }, { "id": 14132, "url": "https://svs.gsfc.nasa.gov/14132/", "result_type": "Produced Video", "release_date": "2022-04-12T00:00:00-04:00", "title": "Black Hole Week: Black Hole GIFs", "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ", "hits": 468 }, { "id": 14126, "url": "https://svs.gsfc.nasa.gov/14126/", "result_type": "Produced Video", "release_date": "2022-04-01T00:00:00-04:00", "title": "SDO Video Toolkit", "description": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files || New_Trebuchet_mkII.00300_print.jpg (1024x576) [336.5 KB] || New_Trebuchet_mkII.00300_print_searchweb.png (320x180) [95.4 KB] || New_Trebuchet_mkII.00300_print_thm.png (80x40) [6.2 KB] || New_Trebuchet_mkII.mp4 (1920x1080) [32.4 MB] || New_Trebuchet_mkII.webm (1920x1080) [3.7 MB] || New_Trebuchet_mkII.mov (1920x1080) [443.3 MB] || New_Trebuchet_mkII.mp4.hwshow [115 bytes] || ", "hits": 448 }, { "id": 20358, "url": "https://svs.gsfc.nasa.gov/20358/", "result_type": "Animation", "release_date": "2022-02-16T12:00:00-05:00", "title": "Webb Mirror Alignment Animations", "description": "Crowded field yields light on NIRCam instrument to check it's properly functioning for its key role in aligning Webb's mirrors. || WEBB_FL_4k_30fps_ProRes.00125_print.jpg (1024x576) [194.9 KB] || WEBB_FL_1K_30fps.mp4 (1000x562) [2.4 MB] || WEBB_FL_HD_30fps.mp4 (1920x1080) [4.9 MB] || WEBB_FL_4k_30fps_ProRes.mov (3840x2160) [450.6 MB] || WEBB_FL_4k_30fps_h264.mp4 (3840x2160) [5.5 MB] || WEBB_FL_4k (3840x2160) [8.0 KB] || WEBB_FL_4k_30fps_h264.webm (3840x2160) [1.2 MB] || ", "hits": 134 }, { "id": 14014, "url": "https://svs.gsfc.nasa.gov/14014/", "result_type": "Produced Video", "release_date": "2022-01-26T00:00:00-05:00", "title": "Elements of Webb: Elements Seeking Elements Ep12", "description": "Elements of Webb EP12: Seeking Elements || 12-Seeking_-_Dark.jpg (1920x1080) [795.3 KB] || 12-Seeking_-_Dark_print.jpg (1024x576) [315.1 KB] || 12-Seeking_-_Dark_searchweb.png (320x180) [73.2 KB] || 12-Seeking_-_Dark_web.png (320x180) [73.2 KB] || 12-Seeking_-_Dark_thm.png (80x40) [6.5 KB] || 12_-_Seeking_Elements_ProRes.mov (1920x1080) [4.9 GB] || 12_-_Seeking_Elements.mp4 (1920x1080) [391.3 MB] || 12_-_Seeking_Elements.webm (1920x1080) [41.3 MB] || 12_-_Seeking_Elements.en_US.srt [6.2 KB] || 12_-_Seeking_Elements.en_US.vtt [6.1 KB] || ", "hits": 20 }, { "id": 14013, "url": "https://svs.gsfc.nasa.gov/14013/", "result_type": "Produced Video", "release_date": "2022-01-19T00:00:00-05:00", "title": "Elements of Webb: Super Black Ep11", "description": "Elements of Webb EP11: Super Black || SuperBlack_-_Dark.jpg (1920x1080) [1015.6 KB] || SuperBlack_-_Dark_print.jpg (1024x576) [430.6 KB] || SuperBlack_-_Dark_searchweb.png (320x180) [97.2 KB] || SuperBlack_-_Dark_web.png (320x180) [97.2 KB] || SuperBlack_-_Dark_thm.png (80x40) [7.7 KB] || 11-Elements_-_SuperBlack_draft_2.mp4 (1920x1080) [224.9 MB] || 11-Elements_-_SuperBlack_ProRes.mov (1920x1080) [3.1 GB] || 11-Elements_-_SuperBlack_draft_2.webm (1920x1080) [24.2 MB] || 11-Elements_-_SuperBlack.en_US.srt [3.9 KB] || 11-Elements_-_SuperBlack.en_US.vtt [3.9 KB] || ", "hits": 22 }, { "id": 14012, "url": "https://svs.gsfc.nasa.gov/14012/", "result_type": "Produced Video", "release_date": "2022-01-12T00:00:00-05:00", "title": "Elements of Webb: Salt Ep10", "description": "Elements of Webb EP10: Salt || 10-Salt_-_Dark.jpg (1920x1080) [793.8 KB] || 10-Salt_-_Dark_print.jpg (1024x576) [329.5 KB] || 10-Salt_-_Dark_searchweb.png (320x180) [86.4 KB] || 10-Salt_-_Dark_web.png (320x180) [86.4 KB] || 10-Salt_-_Dark_thm.png (80x40) [7.2 KB] || 10_-_Elements_-_Salt_ProRes.mov (1920x1080) [2.7 GB] || 10_-_Elements_-_Salt-2.mp4 (1920x1080) [211.9 MB] || 10_-_Elements_-_Salt-2.webm (1920x1080) [22.5 MB] || 10_-_Elements_-_Salt.en_US.srt [3.4 KB] || 10_-_Elements_-_Salt.en_US.vtt [3.4 KB] || ", "hits": 21 }, { "id": 14011, "url": "https://svs.gsfc.nasa.gov/14011/", "result_type": "Produced Video", "release_date": "2022-01-05T00:00:00-05:00", "title": "Elements of Webb: Helium Ep 09", "description": "Elements of Webb EP09: Helium || 9-Helium_-_Dark.jpg (1920x1080) [681.7 KB] || Helium_-_Dark.jpg (1920x1080) [681.7 KB] || 9-Helium_-_Dark_print.jpg (1024x576) [287.9 KB] || 9-Helium_-_Dark_searchweb.png (320x180) [75.4 KB] || 9-Helium_-_Dark_web.png (320x180) [75.4 KB] || 9-Helium_-_Dark_thm.png (80x40) [7.1 KB] || 9-Elements-Helium_ProRes.mov (1920x1080) [3.7 GB] || 9-Elements-Helium.mp4 (1920x1080) [288.4 MB] || 9-Elements-Helium.webm (1920x1080) [30.3 MB] || 9-Elements-Helium.en_US.srt [5.1 KB] || 9-Elements-Helium.en_US.vtt [5.1 KB] || ", "hits": 24 }, { "id": 14010, "url": "https://svs.gsfc.nasa.gov/14010/", "result_type": "Produced Video", "release_date": "2021-12-29T00:00:00-05:00", "title": "Elements of Webb: Silicon Ep08", "description": "Elements of Webb EP07: Silicon || Silicon__-_Dark.jpg (1920x1080) [577.3 KB] || 8-Silicon__-_Dark.jpg (1920x1080) [577.3 KB] || Silicon__-_Dark_print.jpg (1024x576) [279.3 KB] || Silicon__-_Dark_searchweb.png (320x180) [76.0 KB] || Silicon__-_Dark_web.png (320x180) [76.0 KB] || Silicon__-_Dark_thm.png (80x40) [7.0 KB] || 8-Elements-Silicon_ProRes.mov (1920x1080) [1.8 GB] || 8-Elements-Silicon.mp4 (1920x1080) [132.1 MB] || 8-Elements-Silicon.webm (1920x1080) [14.1 MB] || 8-Elements-Silicon.en_US.srt [2.3 KB] || 8-Elements-Silicon.en_US.vtt [2.3 KB] || ", "hits": 34 }, { "id": 14009, "url": "https://svs.gsfc.nasa.gov/14009/", "result_type": "Produced Video", "release_date": "2021-12-22T00:00:00-05:00", "title": "Elements of Webb: Carbon Ep07", "description": "Elements of Webb EP07: Carbon || Backplane_-_Dark.jpg (1920x1080) [894.6 KB] || Backplane_-_Dark_print.jpg (1024x576) [398.3 KB] || Backplane_-_Dark_searchweb.png (320x180) [94.5 KB] || Backplane_-_Dark_web.png (320x180) [94.5 KB] || Backplane_-_Dark_thm.png (80x40) [7.4 KB] || 7-Elements-Carbon_Backplane_ProRes.mov (1920x1080) [2.0 GB] || 7-Elements-Carbon_Backplane-2.mp4 (1920x1080) [149.3 MB] || 7-Elements-Carbon_Backplane-2.webm (1920x1080) [16.2 MB] || 7-Elements-Carbon_Backplane.en_US.srt [2.3 KB] || 7-Elements-Carbon_Backplane.en_US.vtt [2.3 KB] || ", "hits": 17 }, { "id": 14008, "url": "https://svs.gsfc.nasa.gov/14008/", "result_type": "Produced Video", "release_date": "2021-12-15T00:00:00-05:00", "title": "Elements of Webb: Kapton Ep06", "description": "Elements of Webb EP06: Kapton. || 6-Kapton_-_Dark.jpg (1920x1080) [977.3 KB] || 6-Kapton_-_Dark_print.jpg (1024x576) [406.3 KB] || 6-Kapton_-_Dark_searchweb.png (320x180) [90.7 KB] || 6-Kapton_-_Dark_web.png (320x180) [90.7 KB] || 6-Kapton_-_Dark_thm.png (80x40) [6.9 KB] || 6-Elements-Kapton_Prores.mov (1920x1080) [2.6 GB] || 6-Elements-Kapton-2.mp4 (1920x1080) [204.8 MB] || 6-Elements-Kapton-2.webm (1920x1080) [22.6 MB] || 6-Elements-Kapton.en_US.srt [3.5 KB] || 6-Elements-Kapton.en_US.vtt [3.5 KB] || ", "hits": 34 }, { "id": 14007, "url": "https://svs.gsfc.nasa.gov/14007/", "result_type": "Produced Video", "release_date": "2021-12-08T00:00:00-05:00", "title": "Elements of Webb: Beryllium Part 3 Ep05", "description": "Elements of Webb EP 05: Beryllium Part 3. Where Does Beryllium Really Come From? || Beryllium_3_-_dark.jpg (1920x1080) [682.4 KB] || Beryllium_3_-_dark_print.jpg (1024x576) [286.4 KB] || Beryllium_3_-_dark_searchweb.png (320x180) [77.2 KB] || Beryllium_3_-_dark_web.png (320x180) [77.2 KB] || Beryllium_3_-_dark_thm.png (80x40) [6.9 KB] || 5-Elements_-_Beryllium_3_ProRes.mov (1920x1080) [2.7 GB] || 5-Elements_-_Beryllium_3.en_US.srt [3.8 KB] || 5-Elements_-_Beryllium_3.en_US.vtt [3.8 KB] || 5-Elements_-_Beryllium_3-2.mp4 (2300x1080) [211.4 MB] || 5-Elements_-_Beryllium_3.mp4 (2300x1080) [211.4 MB] || 5-Elements_-_Beryllium_3-2.webm (2300x1080) [22.7 MB] || ", "hits": 18 }, { "id": 14006, "url": "https://svs.gsfc.nasa.gov/14006/", "result_type": "Produced Video", "release_date": "2021-12-01T00:00:00-05:00", "title": "Elements of Webb: Beryllium Part 2 Ep04", "description": "Elements of Webb EP04: Beryllium. Where Does Beryllium Come From? || Beryllium_2_-_Dark.jpg (1920x1080) [649.9 KB] || Beryllium_2_-_Dark_print.jpg (1024x576) [274.6 KB] || Beryllium_2_-_Dark_searchweb.png (320x180) [82.2 KB] || Beryllium_2_-_Dark_web.png (320x180) [82.2 KB] || Beryllium_2_-_Dark_thm.png (80x40) [6.8 KB] || 4-Elements_-_Beryllium_2_ProRes.mov (1920x1080) [3.6 GB] || 4-Elements_-_Beryllium_2.mp4 (1920x1080) [264.9 MB] || 4-Elements_-_Beryllium_2-2.mp4 (1920x1080) [264.9 MB] || 4-Elements_-_Beryllium_2.webm (1920x1080) [28.2 MB] || 4-Elements_-_Beryllium_2.en_US.srt [4.2 KB] || 4-Elements_-_Beryllium_2.en_US.vtt [4.2 KB] || ", "hits": 37 }, { "id": 14005, "url": "https://svs.gsfc.nasa.gov/14005/", "result_type": "Produced Video", "release_date": "2021-11-24T00:00:00-05:00", "title": "Elements of Webb: Beryllium Part 1 Ep03", "description": "Have you heard of beryllium? It’s a rare lightweight metal used as the primary material on the Webb Telescope. This episode explores the reason this expensive metal is perfect for Webb. Special thanks to LA Gauge for hosting the media team. #UnfoldTheUniverse || Beryllium_1_dark.jpg (1920x1080) [898.1 KB] || Beryllium_1_dark_print.jpg (1024x576) [388.6 KB] || Beryllium_1_dark_searchweb.png (320x180) [85.0 KB] || Beryllium_1_dark_web.png (320x180) [85.0 KB] || Beryllium_1_dark_thm.png (80x40) [7.1 KB] || 03-Elements-Beryllium_1_ProRes.mov (1920x1080) [3.1 GB] || 3-Elements-Beryllium_1.mp4 (1920x1080) [241.4 MB] || 3-Elements-Beryllium_1.webm (1920x1080) [25.7 MB] || 03-Elements-Beryllium_1.en_US.srt [4.2 KB] || 03-Elements-Beryllium_1.en_US.vtt [4.2 KB] || ", "hits": 29 }, { "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": 300 }, { "id": 14004, "url": "https://svs.gsfc.nasa.gov/14004/", "result_type": "Produced Video", "release_date": "2021-11-17T00:00:00-05:00", "title": "Elements of Webb: Gold Part 2 Ep02", "description": "Elements of Webb EP02: Gold Part Two || 2-Gold_2_-_Dark.jpg (1920x1080) [1.1 MB] || 2-Gold_2_-_Dark_print.jpg (1024x576) [473.1 KB] || 2-Gold_2_-_Dark_searchweb.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_web.png (320x180) [100.6 KB] || 2-Gold_2_-_Dark_thm.png (80x40) [7.5 KB] || 2-Elements_-_Gold_2.webm (1920x1080) [34.9 MB] || 2-Elements_-_Gold_2.en_US.srt [5.8 KB] || 2-Elements_-_Gold_2.en_US.vtt [5.8 KB] || 2-Elements_-_Gold_2_ProRes.mov (1920x1080) [4.2 GB] || 2-Elements_-_Gold_2.mp4 (1920x1080) [324.5 MB] || elements-of-webb-gold-part-2-ep02.hwshow [293 bytes] || ", "hits": 29 }, { "id": 14003, "url": "https://svs.gsfc.nasa.gov/14003/", "result_type": "Produced Video", "release_date": "2021-11-10T00:00:00-05:00", "title": "Elements of Webb: Gold Part 1 Ep01", "description": "Elements of Webb EP01: Gold Part One || 1-Gold_1_-_Dark.jpg (1920x1080) [958.4 KB] || 1-Gold_1_-_Dark_print.jpg (1024x576) [388.7 KB] || 1-Gold_1_-_Dark_searchweb.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_web.png (320x180) [90.4 KB] || 1-Gold_1_-_Dark_thm.png (80x40) [7.4 KB] || 1-Elements-_Gold_1.webm (1920x1080) [25.6 MB] || 1-Elements-_Gold_1.en_US.srt [4.1 KB] || 1-Elements-_Gold_1_ProRes.mov (1920x1080) [3.2 GB] || 1-Elements-_Gold_1.mp4 (1920x1080) [239.5 MB] || elements-of-webb-gold-part-1-ep01.hwshow [291 bytes] || ", "hits": 29 }, { "id": 14002, "url": "https://svs.gsfc.nasa.gov/14002/", "result_type": "Produced Video", "release_date": "2021-11-09T00:00:00-05:00", "title": "Elements of Webb: Series Introduction Ep0", "description": "Elements of Webb EP00: Introduction || EP00-_Elements_Series_Introduction.jpg (1920x1080) [738.1 KB] || EP00-_Elements_Series_Introduction_print.jpg (1024x576) [333.2 KB] || EP00-_Elements_Series_Introduction_searchweb.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_web.png (320x180) [87.8 KB] || EP00-_Elements_Series_Introduction_thm.png (80x40) [7.1 KB] || 0-Elements_of_Webb_-_Introduction_1.mp4 (1920x1080) [89.2 MB] || 0-Elements_of_Webb_-_Introduction_1.webm (1920x1080) [9.4 MB] || 0-Elements_of_Webb_-_Introduction_1.en_US.srt [1.3 KB] || 0-Elements_of_Webb_-_Introduction_1.en_US.vtt [1.3 KB] || 0-Elements_of_Webb_-_Introduction.mov (1920x1080) [1.1 GB] || elements-of-webb-series-introduction-ep0.hwshow [332 bytes] || ", "hits": 37 }, { "id": 13873, "url": "https://svs.gsfc.nasa.gov/13873/", "result_type": "Produced Video", "release_date": "2021-07-01T00:00:00-04:00", "title": "Periodic Table of the Elements: Origins of the Elements", "description": "The periodic table organizes all the known elements by atomic number, which is the number of protons in each atom of the element. This version of the table, which draws on data compiled by astronomer Jennifer Johnson from Ohio State University, shows our current understanding of how each element found on Earth was originally produced. Most of them ultimately have cosmic origins. Some elements were created with the birth of the universe, while others were made during the lives or deaths of stars. The Nancy Grace Roman Space Telescope will help us understand the cosmic era when stars first began forming. The mission will help scientists learn more about how elements were created and distributed throughout galaxies.The related Tumblr post is here. || ", "hits": 1703 }, { "id": 4927, "url": "https://svs.gsfc.nasa.gov/4927/", "result_type": "Visualization", "release_date": "2021-05-22T00:00:00-04:00", "title": "Arctic Sea Ice 2020-2021, Domemaster Format", "description": "Full visualization, all elements, 30 fps. || sea_ice_2021_max_dome_4096p30_h265.00001_print.jpg (1024x1024) [51.2 KB] || sea_ice_2021_max_dome_4096p30_h265.mp4 (4096x4096) [19.1 MB] || sea_ice_2021_max_dome_4096p30_h265.webm (4096x4096) [11.9 MB] || ", "hits": 39 }, { "id": 4887, "url": "https://svs.gsfc.nasa.gov/4887/", "result_type": "Visualization", "release_date": "2021-03-01T10:00:00-05:00", "title": "Heliophysics Sentinels 2020 (Forecast Version)", "description": "In addition to the NASA missions used in research for space weather (see 2020 Heliophysics Fleet) there are additional missions operated by NOAA used for space weather forecasting. As of spring 2020, here's a tour of the NASA and NOAA Heliophysics fleets from the near-Earth satellites out to the inner solar system.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 34 }, { "id": 13571, "url": "https://svs.gsfc.nasa.gov/13571/", "result_type": "Produced Video", "release_date": "2020-10-29T00:00:00-04:00", "title": "GLOBE Observer Why Observe?: Tree Height", "description": "Music: “Enchanted Woodland” by Brice Davoli [SACEM] & Valeria Deniz [SACEM]; Koka Media & Universal Publishing Production Music France; Universal Production Music“Tales of Everlasting Winter” by Brice Davoli [SACEM]; Koka Media & Universla Publishing Production Music France; Universal Production Music“Puzzled,\" \"Intrigues and Plots,\" & \"Pulsing Mallets\" by Laurent Dury [SACEM]; Koka Media & Universal Publishing Production Music France; Universal Production Music“Foreign Land” by Hannes Gottwald [GEMA] & Sinan Hosgel [GEMA]; Ed. Berlin Production Music/Universal Production Music GmbH; Universal Production Music || WhyObserve_TreeHeight.png (1920x1080) [3.5 MB] || WhyObserve_TreeHeight_print.jpg (1024x576) [205.4 KB] || WhyObserve_TreeHeight_searchweb.png (320x180) [99.7 KB] || WhyObserve_TreeHeight_thm.png (80x40) [7.1 KB] || 13571_WhyObserveTreeHeight_FINAL.mov (1920x1080) [14.8 GB] || FACEBOOK_720_13571_WhyObserveTreeHeight_FINAL_VX-314630_facebook_720.mp4 (1280x720) [744.0 MB] || YOUTUBE_1080_13571_WhyObserveTreeHeight_FINAL_VX-314630_youtube_1080.mp4 (1920x1080) [1018.9 MB] || 13571_WhyObserveTreeHeight_FINAL_VX-314630_lowres.mp4 (1280x720) [200.3 MB] || 13571_WhyObserveTreeHeight_FINAL_VX-314630.webm (960x540) [296.3 MB] || 13571_WhyObserveTreeHeight_FINAL.en_US.srt [15.4 KB] || 13571_WhyObserveTreeHeight_FINAL.en_US.vtt [14.8 KB] || ", "hits": 23 }, { "id": 13710, "url": "https://svs.gsfc.nasa.gov/13710/", "result_type": "Produced Video", "release_date": "2020-10-05T13:00:00-04:00", "title": "TESS's Northern Sky Vista", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) spent nearly a year imaging the northern sky in its search for worlds beyond our solar system. Explore this panorama to see what TESS has found so far.Credit: NASA's Goddard Space Flight CenterMusic: \"Strolling\" from Above and Below. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Northern_and_Southern_Still.jpg (1920x1080) [699.1 KB] || 13710_TESS_Northern_Tour_Best_1080.webm (1920x1080) [33.4 MB] || 13710_TESS_Northern_Tour_1080.mp4 (1920x1080) [423.5 MB] || 13710_TESS_Northern_Tour_SRT_Captions.en_US.srt [4.9 KB] || 13710_TESS_Northern_Tour_SRT_Captions.en_US.vtt [4.9 KB] || 13710_TESS_Northern_Tour_Best_1080.mp4 (1920x1080) [1.1 GB] || 13710_TESS_Northern_Tour_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || ", "hits": 58 }, { "id": 4822, "url": "https://svs.gsfc.nasa.gov/4822/", "result_type": "Visualization", "release_date": "2020-09-15T10:00:00-04:00", "title": "Heliophysics Sentinels 2020", "description": "There have been few changes since the 2018 Heliophysics Fleet. Van Allen Probes and SORCE have been decommissioned, while Solar Orbiter, ICON and SET have been added. As of spring 2020, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 39 }, { "id": 4855, "url": "https://svs.gsfc.nasa.gov/4855/", "result_type": "Visualization", "release_date": "2020-08-27T15:00:00-04:00", "title": "NASA's GPM captures powerful Hurricane Laura over Louisiana", "description": "This visualization shows Hurricane Laura over the Gulf Coast states approximately 7 hours after making landfall on the morning of August 27, 2020. || cam_laura1240ZShape.2340_print.jpg (1024x576) [195.0 KB] || cam_laura1240ZShape.2340_searchweb.png (320x180) [99.6 KB] || cam_laura1240ZShape.2340_thm.png (80x40) [7.4 KB] || laura1240Z_1080p30.mp4 (1920x1080) [41.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || laura1240Z_1080p30.webm (1920x1080) [4.1 MB] || laura1240Z_1080p30.mp4.hwshow [184 bytes] || ", "hits": 24 }, { "id": 13682, "url": "https://svs.gsfc.nasa.gov/13682/", "result_type": "Produced Video", "release_date": "2020-08-11T09:55:00-04:00", "title": "Hubble and Whale Sharks?", "description": "While you might not think that sharks and the Hubble Space Telescope have a lot in common, it turns out they share an incredible bond!For more information, visit https://nasa.gov/hubble.Credit: NASA's Goddard Space Flight CenterPaul Morris (USRA): Lead ProducerVideos, Images, and Audio Effects: Page Turning Whoosh by dauzkobza via Motion ArrayWind by LuLuProduction via Motion ArrayCamera Sound Pack 1 by Blue Kangaroo via Motion ArrayCrunchy Bite SFX Pack by WARP EFX via Motion ArrayWater Splash by Motion Audio via Motion ArrayFlying Through the Realistic Clouds(Left-Right) by MambaTV via Motion ArrayPOV Water Surface by v_creative via Motion ArrayDing by Media_M via Motion ArrayBell Ding by dauzkobza via Motion ArrayWhoosh Pack by BANT via Motion ArrayCartoon Love Elements by FXBox via Motion ArrayShining Hearts Animation by action_7 via Motion ArrayPop Up by Motion Audio via Motion ArrayPolaroid Photos Opener by Rocksolid via Motion ArrayUnderwater by erhnbcc via Motion ArrayWhale Shark by Alexpunker via Motion ArrayWhale Shark At Surface by Alexpunker via Motion ArrayWhale Shark In Ocean by Alexpunker via Motion ArrayWhale Shark At Sea by Alexpunker via Motion ArrayShark by designprojects via Motion ArrayFingerprints Background by Alex39 via Motion ArrayWhale Shark Still Image by Amber CookWhale Shark Video with Diver by Tom CampbellMusic Credits:“Happy Tulip” by Stéphane Caisson [ SACEM ]. Koka Media [ SACEM ], Universal Publishing Production Music France [ SACEM ], and Universal Production Music || ", "hits": 43 }, { "id": 13624, "url": "https://svs.gsfc.nasa.gov/13624/", "result_type": "Produced Video", "release_date": "2020-05-21T12:00:00-04:00", "title": "Launching America: Goddard's Role in Keeping Astronauts Connected to Earth", "description": "Music: \"Never Looking Back\" by Frederik Wiedman; Enigma; Killer Tracks [BMI]; Universal Production Music || 13624_DM2_KeepingAstronautsConnected.00067_print.jpg (1024x576) [102.6 KB] || 13624_DM2_KeepingAstronautsConnected.00067_searchweb.png (320x180) [91.2 KB] || 13624_DM2_KeepingAstronautsConnected.00067_thm.png (80x40) [7.2 KB] || 13624_DM2_KeepingAstronautsConnected.mov (1920x1080) [1.7 GB] || 13624_DM2_KeepingAstronautsConnected_lowres.mp4 (1280x720) [24.6 MB] || 3624_DM2_KeepingAstronautsConnected_youtube_1080.mp4 (1920x1080) [138.4 MB] || 13624_DM2_KeepingAstronautsConnected_facebook_720.mp4 (1280x720) [100.5 MB] || 13624_DM2_KeepingAstronautsConnected_twitter_720.mp4 (1280x720) [17.7 MB] || 13624_DM2_KeepingAstronautsConnected.webm (960x540) [34.5 MB] || 13624_DM2_KeepingAstronautsConnected.en_US.srt [1.7 KB] || 13624_DM2_KeepingAstronautsConnected.en_US.vtt [1.7 KB] || ", "hits": 46 }, { "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": 848 }, { "id": 13530, "url": "https://svs.gsfc.nasa.gov/13530/", "result_type": "Produced Video", "release_date": "2020-01-30T00:00:00-05:00", "title": "Mirror Quadrants for XRISM", "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ", "hits": 91 }, { "id": 13484, "url": "https://svs.gsfc.nasa.gov/13484/", "result_type": "Produced Video", "release_date": "2019-12-04T13:00:00-05:00", "title": "Parker Solar Probe First Findings - Media Telecon", "description": "NASA to Present First Parker Solar Probe Findings in Media TeleconferenceNASA will announce the first results from the Parker Solar Probe mission, the agency's mission to \"touch\" the Sun, during a media teleconference at 1:30 pm EST on Wednesday, Dec. 4, 2019.Parker has traveled closer to our star than any human-made object before it. The teleconference will discuss the first papers from the principal investigators of the mission’s four instruments. The papers will be published online Wednesday in Nature at 1 pm EST.The teleconference audio will stream live at:https://www.nasa.gov/nasaliveParticipants in the call are: •Nicola Fox, director of the Heliophysics Division, Science Mission Directorate, NASA Headquarters, Washington•Stuart Bale, principal investigator of the FIELDS instrument at the University of California, Berkeley•Justin Kasper, principal investigator of the SWEAP instrument at the University of Michigan in Ann Arbor•Russ Howard, principal investigator of the WISPR instrument at the Naval Research Laboratory in Washington•David McComas, principal investigator of the ISʘIS instrument at Princeton University in Princeton, N.J. || ", "hits": 69 }, { "id": 13419, "url": "https://svs.gsfc.nasa.gov/13419/", "result_type": "Animation", "release_date": "2019-11-07T13:00:00-05:00", "title": "NICER Catches Milestone X-ray Burst", "description": "At about 10:04 p.m. EDT on Aug. 20, NASA’s Neutron star Interior Composition Explorer (NICER) telescope on the International Space Station detected a sudden spike of X-rays caused by a massive thermonuclear flash on the surface of a pulsar, the crushed remains of a star that long ago exploded as a supernova. The X-ray burst, the brightest seen by NICER so far, came from an object named SAX J1808.4-3658, or J1808 for short. The observations reveal many phenomena that have never been seen together in a single burst. In addition, the subsiding fireball briefly brightened again for reasons astronomers cannot yet explain. The data reveal a two-step change in brightness, which scientists think is caused by the ejection of separate layers from the pulsar surface, and other features that will help them decode the physics of these powerful events.The explosion, which astronomers classify as a Type I X-ray burst, released as much energy in 20 seconds as the Sun does in nearly 10 days.J1808 is located about 11,000 light-years away in the constellation Sagittarius, spins at a dizzying 401 rotations each second, and is one member of a binary system. Its companion is a brown dwarf, an object larger than a giant planet yet too small to be a star. A steady stream of hydrogen gas flows from the companion toward the neutron star, and it accumulates in a vast storage structure called an accretion disk.Hydrogen raining onto the pulsar's surface forms a hot, ever-deepening global “sea.” At the base of this layer, temperatures and pressures increase until hydrogen nuclei fuse to form helium nuclei, which produces energy — a process at work in the core of our Sun. The helium settles out and builds up a layer of its own. Eventually, the conditions allow helium nuclei to fuse into carbon. The helium erupts explosively and unleashes a thermonuclear fireball across the entire pulsar surface.As the burst started, NICER data show that its X-ray brightness leveled off for almost a second before increasing again at a slower pace. The researchers interpret this “stall” as the moment when the energy of the blast built up enough to blow the pulsar’s hydrogen layer into space. The fireball continued to build for another two seconds and then reached its peak, blowing off the more massive helium layer. The helium expanded faster, overtook the hydrogen layer before it could dissipate, and then slowed, stopped and settled back down onto the pulsar’s surface. Following this phase, the pulsar briefly brightened again by roughly 20 percent for reasons the team does not yet understand. || ", "hits": 84 }, { "id": 13285, "url": "https://svs.gsfc.nasa.gov/13285/", "result_type": "Produced Video", "release_date": "2019-11-05T13:00:00-05:00", "title": "TESS's Southern Sky Panorama", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) spent a year imaging the southern sky in its search for worlds beyond our solar system. Dive into a mosaic of these images to see what TESS has found so far. Credit: NASA's Goddard Space Flight CenterMusic: “Phenomenon\" from Above and Below Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Southern_Sky_Still.jpg (1920x1080) [892.0 KB] || Southern_Sky_Still_print.jpg (1024x576) [222.5 KB] || Southern_Sky_Still_searchweb.png (320x180) [66.5 KB] || Southern_Sky_Still_thm.png (80x40) [5.0 KB] || 13285_TESS_SouthernSky_Small_720.webm (1280x720) [26.3 MB] || 13285_TESS_SouthernSky_Small_720.mp4 (1280x720) [250.7 MB] || 13285_TESS_SouthernSky_1080.mp4 (1920x1080) [492.4 MB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.srt [4.3 KB] || 13285_TESS_SouthernSky_SRT_Captions.en_US.vtt [4.3 KB] || 13285_TESS_SouthernSky_Best_1080.mp4 (1920x1080) [1.2 GB] || 13285_TESS_SouthernSky_ProRes_1920x1080_30.mov (1920x1080) [3.5 GB] || tesss-southern-sky-panorama-movie.hwshow || 07a_tess_coverage.hwshow [190 bytes] || ", "hits": 148 }, { "id": 13325, "url": "https://svs.gsfc.nasa.gov/13325/", "result_type": "Produced Video", "release_date": "2019-09-24T13:00:00-04:00", "title": "The Nancy Grace Roman Space Telescope's Coronagraph Instrument", "description": "Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.Credit: NASA's Goddard Space Flight CenterMusic: \"Concept of Motion\" from Universe Production MusicComplete transcript available. || Roman_CGI_Still.jpg (1920x1080) [396.1 KB] || 13325_Roman_CGI_1080.mp4 (1920x1080) [96.8 MB] || 13325_Roman_CGI_Final_ProRes_1920x1080_2997.mov (1920x1080) [1.3 GB] || 13325_Roman_CGI_1080.webm (1920x1080) [13.9 MB] || Roman_CGI_SRT_Captions.en_US.srt [2.4 KB] || Roman_CGI_SRT_Captions.en_US.vtt [2.4 KB] || ", "hits": 134 }, { "id": 31049, "url": "https://svs.gsfc.nasa.gov/31049/", "result_type": "Hyperwall Visual", "release_date": "2019-08-07T00:00:00-04:00", "title": "The A-Train & C-Train", "description": "A-Train_C-Train_TimeSeps2018_HW || A-Train_C-Train_TimeSeps2018_HW_print.jpg (1024x576) [932.9 KB] || A-Train_C-Train_TimeSeps2018_HW.jpg (5760x3240) [13.3 MB] || A-Train_C-Train_TimeSeps2018_HW_searchweb.png (320x180) [89.3 KB] || A-Train_C-Train_TimeSeps2018_HW_thm.png (80x40) [6.8 KB] || the-a-train-c-train-time-seps.hwshow [315 bytes] || ", "hits": 96 }, { "id": 4718, "url": "https://svs.gsfc.nasa.gov/4718/", "result_type": "Visualization", "release_date": "2019-05-23T00:00:00-04:00", "title": "Visualization Elements for Global Freshwater Campaign", "description": "The following visualizations and animations were created in support of the video release \"NASA Follows Changing Freshwater from Space,\" entry ID 13227, for use as elements within the video. || ", "hits": 23 }, { "id": 13143, "url": "https://svs.gsfc.nasa.gov/13143/", "result_type": "Produced Video", "release_date": "2019-02-11T21:00:00-05:00", "title": "NASA's Mission Through Dangerous Space Is Going Out in Style", "description": "B-roll for Van Allen Probe Live Shot. Answers the following suggested questions: You may think space is empty, but there is a lot there that we can’t see. What are space weather and radiation belts?How do you observe the radiation belts?A new radiation belt was discovered several years ago. Tell us about that discovery.Can you tell us about the final mission that the Van Allen probes are going on?How do radiation belts affect space travel, astronauts and the space station?Where can we learn more? || broll.00001_print.jpg (1024x576) [114.9 KB] || broll.00001_print_print.jpg (1024x576) [66.2 KB] || broll.00001_print_searchweb.png (320x180) [95.8 KB] || broll.00001_print_thm.png (80x40) [7.7 KB] || broll.webm (1280x720) [21.1 MB] || broll.mp4 (1280x720) [212.1 MB] || broll.mov (1280x720) [2.8 GB] || ", "hits": 56 }, { "id": 4360, "url": "https://svs.gsfc.nasa.gov/4360/", "result_type": "Visualization", "release_date": "2018-12-10T11:00:00-05:00", "title": "Heliophysics Sentinels 2018", "description": "This movie presents the trajectories of the heliophysics fleet from close to Earth to out beyond the heliopause. || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_print.jpg (1024x576) [74.5 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_searchweb.png (180x320) [65.6 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_thm.png (80x40) [5.1 KB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4 (1920x1080) [40.3 MB] || Sentinels2018.Sentinels2Voyager_1080p30.webm (1920x1080) [6.3 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Sentinels2018.Sentinels2Voyager_2160p30.mp4 (3840x2160) [125.7 MB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4.hwshow || ", "hits": 45 }, { "id": 4698, "url": "https://svs.gsfc.nasa.gov/4698/", "result_type": "Visualization", "release_date": "2018-12-09T00:00:00-05:00", "title": "Earth Observing Fleet (October 2018)", "description": "NASA's Earth Science Fleet as of October 2018 || fleet201810_hd01.07410_print.jpg (1024x576) [71.1 KB] || fleet201810_hd01.07410_searchweb.png (320x180) [64.9 KB] || fleet201810_hd01.07410_thm.png (80x40) [4.8 KB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || fleet201810_hd01.webm (1920x1080) [51.8 MB] || fleet201810_hd01.mp4 (1920x1080) [229.8 MB] || 9600x3240_16x9_30p (9600x3240) [0 Item(s)] || fleet201810_hd01.mp4.hwshow [182 bytes] || ", "hits": 38 }, { "id": 13094, "url": "https://svs.gsfc.nasa.gov/13094/", "result_type": "Produced Video", "release_date": "2018-11-08T13:00:00-05:00", "title": "Multimessenger Timeline Resources", "description": "The media elements below appear in the multimessenger astronomy video \"Luck Favors the Prepared.\" || A simple animation of a gamma ray moving through space.Credit: NASA's Goddard Space Flight Center || Gamma_Ray_animation.00001_print.jpg (1024x576) [15.9 KB] || Gamma_Ray_animation.00001_print_searchweb.png (320x180) [22.1 KB] || Gamma_Ray_animation.00001_print_thm.png (80x40) [2.3 KB] || Gamma_Ray_animation.mov (1280x720) [51.5 MB] || Gamma_Ray_animation.webm (1280x720) [773.0 KB] || || ", "hits": 84 }, { "id": 40365, "url": "https://svs.gsfc.nasa.gov/gallery/earth-science-oct2018-briefing/", "result_type": "Gallery", "release_date": "2018-10-18T00:00:00-04:00", "title": "Earth Science Overview Oct 2018 Briefing", "description": "No description available.", "hits": 89 } ] }