{ "count": 299, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Type%22", "previous": null, "results": [ { "id": 31382, "url": "https://svs.gsfc.nasa.gov/31382/", "result_type": "Hyperwall Visual", "release_date": "2026-04-01T12:00:00-04:00", "title": "Bone Loss Research Aboard the ISS", "description": "The experiment tests how microgravity affects bone-forming and bone-degrading cells and explore potential ways to prevent bone loss. This research could help protect astronauts on future long-duration missions to the Moon and Mars, while also advancing treatments for millions of people on Earth who suffer from osteoporosis.", "hits": 779 }, { "id": 31384, "url": "https://svs.gsfc.nasa.gov/31384/", "result_type": "Hyperwall Visual", "release_date": "2026-04-01T12:00:00-04:00", "title": "Gigantic Jet Seen from the ISS", "description": "A Gigantic Jet event was photographed by NASA astronaut Nichole Ayers from aboard the International Space Station", "hits": 4828 }, { "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": 40549, "url": "https://svs.gsfc.nasa.gov/gallery/interstellar-boundary-explorer-ibex/", "result_type": "Gallery", "release_date": "2026-03-02T00:00:00-05:00", "title": "IBEX – Interstellar Boundary Explorer", "description": "The Interstellar Boundary Explorer (IBEX) is a NASA spacecraft studying how our heliosphere — the protective bubble surrounding the Sun and planets that is inflated by a constant stream of solar particles — interacts with interstellar space. IBEX created the first maps showing the interactions at that border, and how they change over time due to variations in the Sun’s activity. IBEX studies the heliosphere’s boundaries by measuring a type of uncharged particle called energetic neutral atoms.\n\nIBEX launched on Oct. 19, 2008, from the Ronald Reagan Ballistic Missile Defense Test Site, in the Republic of the Marshall Islands. \n\nLearn more: https://science.nasa.gov/mission/ibex/", "hits": 225 }, { "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": 40542, "url": "https://svs.gsfc.nasa.gov/gallery/dark-energy/", "result_type": "Gallery", "release_date": "2026-01-28T00:00:00-05:00", "title": "Dark Energy", "description": "Some 13.8 billion years ago, the universe began with a rapid expansion we call the big bang. After this initial expansion, which lasted a fraction of a second, gravity started to slow the universe down. But the cosmos wouldn’t stay this way. Nine billion years after the universe began, its expansion started to speed up, driven by an unknown force that scientists have named dark energy.\n\nBut what exactly is dark energy?\n\nThe short answer is: We don't know. But we do know that it exists, it’s making the universe expand at an accelerating rate, and approximately 68.3 to 70% of the universe is dark energy.", "hits": 870 }, { "id": 31360, "url": "https://svs.gsfc.nasa.gov/31360/", "result_type": "Hyperwall Visual", "release_date": "2025-12-01T18:59:59-05:00", "title": "NISAR First Light Imagery", "description": "The NISAR (NASA-ISRO Synthetic Aperture Radar) Earth-observing radar satellite’s first images of our planet’s surface are in, and they offer a glimpse of things to come as the joint mission between NASA and ISRO (Indian Space Research Organisation) approaches full science operations later this year.", "hits": 101 }, { "id": 40539, "url": "https://svs.gsfc.nasa.gov/gallery/artemis-iiscience/", "result_type": "Gallery", "release_date": "2025-08-15T00:00:00-04:00", "title": "Moon Visualizations, Animations, Videos - Artemis II Lunar Science", "description": "While the Artemis II crew will be the first humans to test NASA’s Orion spacecraft in space, they will also conduct science investigations that will inform future deep space missions. During the 10-day past the Moon and back, the Orion capsule will fly by the far side of the Moon — the side that always faces away from Earth. During this three-hour period, astronauts will analyze and photograph geologic features, such as impact craters and ancient lava flows. They will rely on the extensive geology training they received in the classroom and in Moon-like places on Earth to describe nuances in shapes, textures, and colors — the type of information that reveals the geologic history of an area. These skills will be critical to exploring the Moon’s South Pole region through future missions.\n\nLearn more about Artemis II lunar science.\nLearn more about all Artemis II science experiments\nLearn more about the Moon at science.nasa.gov/moon.\n\n**Note: This page will be continually updated through the Artemis II mission. **\n\nMedia Contact: Lonnie Shekhtman NASA’s Goddard Space Flight Center in Greenbelt, Md.", "hits": 11913 }, { "id": 31352, "url": "https://svs.gsfc.nasa.gov/31352/", "result_type": "Animation", "release_date": "2025-06-06T18:59:59-04:00", "title": "Leopard Spots", "description": "Images and video describing the 25th Martian sample collected by NASA’s Mars Perseverance rover – “Sapphire Canyon” – a sample taken from a vein-filled rock named “Cheyava Falls.”", "hits": 197 }, { "id": 5548, "url": "https://svs.gsfc.nasa.gov/5548/", "result_type": "Visualization", "release_date": "2025-06-05T07:00:59-04:00", "title": "Global Views of PACE Land Vegetation Data", "description": "Global view of three major classes of plant pigments observed by the PACE satellite: chlorophylls, carotenoids, and anthocyanins.", "hits": 177 }, { "id": 31350, "url": "https://svs.gsfc.nasa.gov/31350/", "result_type": "Animation", "release_date": "2025-05-27T18:59:59-04:00", "title": "Your Name In Landsat", "description": "The Landsat program, a joint venture between NASA and the U.S. Geological Survey (USGS), has been observing Earth for over 50 years, collecting breathtaking imagery and invaluable data used to study our planet’s changing surface.\r\n\r\nOn the Your Name In Landsat project page, users can type in their name, then view and export the graphic of that name spelled out in Earth features found in Landsat images.", "hits": 90 }, { "id": 14811, "url": "https://svs.gsfc.nasa.gov/14811/", "result_type": "Produced Video", "release_date": "2025-04-02T00:00:00-04:00", "title": "IMAP: Mapping The Heliosphere & Sun", "description": "The Interstellar Mapping and Acceleration Probe, or IMAP, will explore and map the very boundaries of our heliosphere — a huge bubble created by the Sun's wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.The mission’s investigation of the boundaries of the heliosphere will be primarily done with energetic neutral atoms, or ENAs. An ENA is a type of uncharged particle formed when an energetic positively charged ion runs into a slow-moving neutral atom. The ion picks up an extra negatively charged electron in the collision, making it neutral — hence the name energetic neutral atom. This process frequently happens wherever there is plasma in space, such as throughout the heliosphere, including its boundary.The IMAP-Lo, IMAP-HI, and IMAP-Ultra instruments on IMAP are imaging the energies and composition of ENAs.Learn more about IMAP: https://science.nasa.gov/mission/imap/ || ", "hits": 153 }, { "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": 5425, "url": "https://svs.gsfc.nasa.gov/5425/", "result_type": "Visualization", "release_date": "2025-02-27T09:45:00-05:00", "title": "Perpetual Ocean 2: Western Boundary Currents", "description": "This is the 'beauty shot version' of Perpetual Ocean 2: Western Boundary Currents. The visualization starts with a rotating globe showing ocean currents. The camera then zooms into the Kuroshio current, moves over the Indian Ocean to the Agulhas Current, then over to the Gulf Stream. The flows from the surface down to 600 meters deep are all white. Flows below 600 meters depth use the blue-cyan-white color table below.", "hits": 1204 }, { "id": 14781, "url": "https://svs.gsfc.nasa.gov/14781/", "result_type": "Produced Video", "release_date": "2025-02-25T13:00:00-05:00", "title": "NASA Interview Opportunities: Two Moon Deliveries with NASA Instruments Days from Landing", "description": "Associated cut b-roll will be added by 5 p.m. EST on Thursday, Feb. 27. || CLPS.jpeg (1800x720) [219.2 KB] || CLPS_print.jpg (1024x409) [94.0 KB] || CLPS_searchweb.png (320x180) [46.3 KB] || CLPS_thm.png [5.8 KB] || ", "hits": 373 }, { "id": 14771, "url": "https://svs.gsfc.nasa.gov/14771/", "result_type": "Produced Video", "release_date": "2025-01-24T14:00:00-05:00", "title": "PUNCH Instruments", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ", "hits": 92 }, { "id": 5432, "url": "https://svs.gsfc.nasa.gov/5432/", "result_type": "Visualization", "release_date": "2024-12-01T00:00:00-05:00", "title": "PACE and SWOT", "description": "This visualization begins with a view of the PACE and SWOT satellites orbiting Earth. The camera then pushes into a region in the Atlantic Ocean, and a view of chlorophyll data from PACE. Swaths of SWOT sea surface height anomaly data are added, with blues representing lower surface height and reds representing higher surface height. The PACE data then cycles between three layers of phytoplankton species - Picoeukaryotes, Prochlorococcus, and Synechococcus.", "hits": 98 }, { "id": 5423, "url": "https://svs.gsfc.nasa.gov/5423/", "result_type": "Visualization", "release_date": "2024-11-27T11:00:00-05:00", "title": "Gravity waves disturbing the stratospheric polar vortex", "description": "Animation 1: Changes in temperature and height on the surface of 850 Kelvin potential temperature. The mountain generated gravity waves create strong cooling  as the gravity waves propagate through the stratosphere, while the polar vortex (the cold blue ring) evolves to become colder. || stratospher850_039_T.02498_print.jpg (1024x576) [108.0 KB] || stratospher850_039_T.02498_searchweb.png (320x180) [50.4 KB] || stratospher850_039_T.02498_thm.png (80x40) [4.2 KB] || stratospher850_039_T_1080p30.mp4 (1920x1080) [52.0 MB] || stratospher850_039_T [0 Item(s)] || stratospher850_039_T.mp4 (3840x2160) [148.7 MB] || stratospher850_039_T.mp4.hwshow || ", "hits": 105 }, { "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": 5389, "url": "https://svs.gsfc.nasa.gov/5389/", "result_type": "Visualization", "release_date": "2024-11-14T00:00:00-05:00", "title": "Tracking methane with EMIT and AVIRIS-3", "description": "Methane plumes can now be detected using the airborne AVIRIS-3 spectrometer in addition to EMIT on the International Space Station.", "hits": 160 }, { "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": 14634, "url": "https://svs.gsfc.nasa.gov/14634/", "result_type": "Produced Video", "release_date": "2024-07-25T14:00:00-04:00", "title": "Fermi Finds Novel Feature in BOAT Gamma-Ray Burst", "description": "The brightest gamma-ray burst yet recorded gave scientists a new high-energy feature to study. Learn what NASA’s Fermi mission saw, and what this feature may be telling us about the burst’s light-speed jets. Credit: NASA's Goddard Space Flight CenterMusic: “Tides,” Jon Cotton [PRS] and Ben Niblett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Distant_GRB_still.jpg (3840x2160) [2.5 MB] || 14634_Fermi_GRB_Emission_Line_Under100.mp4 (1920x1080) [90.7 MB] || 14634_Fermi_GRB_Emission_Line_Best.mp4 (1920x1080) [422.0 MB] || 14634FermiGRBEmissionLine_Captions.en_US.srt [4.4 KB] || 14634FermiGRBEmissionLine_Captions.en_US.vtt [4.2 KB] || 14634_Fermi_GRB_Emission_Line_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || ", "hits": 149 }, { "id": 31296, "url": "https://svs.gsfc.nasa.gov/31296/", "result_type": "Hyperwall Visual", "release_date": "2024-06-21T00:00:00-04:00", "title": "Coming in Hot — NASA’s Chandra Checks Habitability of Exoplanets", "description": "Credits:Movie: Cal Poly Pomona/B. Binder; Illustration: NASA/CXC/M.Weiss || chandra-exoplanets.00001_print.jpg (1024x576) [195.6 KB] || chandra-exoplanets.00001_searchweb.png (320x180) [78.4 KB] || chandra-exoplanets.00001_thm.png (80x40) [5.7 KB] || chandra-exoplanets.mp4 (1280x720) [63.9 MB] || chandra-exoplanets.webm (1280x720) [7.0 MB] || coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets.hwshow [319 bytes] || ", "hits": 227 }, { "id": 31291, "url": "https://svs.gsfc.nasa.gov/31291/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb Identifies Tiniest Free-Floating Brown Dwarf", "description": "This image from the NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope shows the central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs: objects too small to be stars but larger than most planets. They found three brown dwarfs that are less than eight times the mass of Jupiter. The smallest weighs just three to four times Jupiter, challenging theories for star formation.The wispy curtains filling the image are interstellar material reflecting the light from the cluster’s stars – what is known as a reflection nebula. The material also includes carbon-containing molecules known as polycyclic aromatic hydrocarbons, or PAHs. The bright star closest to the center of the frame is actually a pair of type B stars in a binary system, which are the most massive stars in the cluster. Winds from these stars may help sculpt the large loop seen on the right side of the field of view. || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_print.jpg (1024x1372) [393.6 KB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam.png (3788x5077) [24.7 MB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam-hw.png (3840x2160) [4.8 MB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_searchweb.png (320x180) [111.1 KB] || STScI-01HFC8K9A4CX579GP4QMDX2QBY-nircam_thm.png (80x40) [14.4 KB] || webb-identifies-tiniest-free-floating-brown-dwarf-nircam.hwshow [364 bytes] || ", "hits": 134 }, { "id": 31293, "url": "https://svs.gsfc.nasa.gov/31293/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Hubble Telescopes Affirm Universe's Expansion Rate", "description": "This image of NGC 5468, a galaxy located about 130 million light-years from Earth, combines data from the Hubble and James Webb space telescopes. This is the farthest galaxy in which Hubble has identified Cepheid variable stars. These are important milepost markers for measuring the expansion rate of the universe. The distance calculated from Cepheids has been cross-correlated with a type Ia supernova in the galaxy. Type Ia supernovae are so bright they are used to measure cosmic distances far beyond the range of the Cepheids, extending measurements of the universe's expansion rate deeper into space.CreditsNASA, ESA, CSA, STScI, Adam G. Riess (JHU, STScI) || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_print.jpg (1024x576) [160.4 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb.png (3214x3233) [16.1 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw.png (3840x2160) [7.7 MB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_searchweb.png (320x180) [58.9 KB] || STScI-01HQ6CMS8HDH8EAR4EHEAKSP5N-hst-webb-hw_thm.png (80x40) [8.5 KB] || webb-hubble-telescopes-affirm-universes-expansion-rate.hwshow [366 bytes] || ", "hits": 310 }, { "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": 487 }, { "id": 5259, "url": "https://svs.gsfc.nasa.gov/5259/", "result_type": "Visualization", "release_date": "2024-04-19T10:00:00-04:00", "title": "PACE - First Look at OCI, HARP2, and SPEXone data", "description": "This visualization begins with a view of the PACE spacecraft orbiting Earth. A swath of true color imagery is exposed as the spacecraft passes over each location. The camera then zooms into the southeastern coast of the US, revealing several data layers from the PACE science instruments, including chlorophyll, a phytoplankton community map (Picoeukaryotes, Prochlorococcus, and Synechococcus), and aerosols. || PACE_EarthDay2024.03800_print.jpg (1024x576) [142.8 KB] || PACE_EarthDay2024.03800_searchweb.png (320x180) [79.9 KB] || PACE_EarthDay2024.03800_thm.png (80x40) [6.1 KB] || PACE_EarthDay2024_1080p60.mp4 (1920x1080) [35.6 MB] || PACE_EarthDay2024 (3840x2160) [256.0 KB] || PACE_EarthDay2024_2160p60.mp4 (3840x2160) [119.8 MB] || ", "hits": 52 }, { "id": 14551, "url": "https://svs.gsfc.nasa.gov/14551/", "result_type": "Produced Video", "release_date": "2024-03-25T06:00:00-04:00", "title": "The Countdown Is On For The Historic Solar Eclipse On April 8th That Will Sweep Across the U.S. Are You Ready for It?", "description": "Scroll down the page for the cut b-roll for the live shots and a canned interview available for easy download || Total_Solar_Eclipse_Banner_4.3.24.jpg (1800x720) [134.2 KB] || Total_Solar_Eclipse_Banner_4.3.24_print.jpg (1024x409) [62.3 KB] || Total_Solar_Eclipse_Banner_4.3.24_searchweb.png (320x180) [32.4 KB] || Total_Solar_Eclipse_Banner_4.3.24_thm.png (80x40) [5.0 KB] || ", "hits": 123 }, { "id": 31276, "url": "https://svs.gsfc.nasa.gov/31276/", "result_type": "Hyperwall Visual", "release_date": "2024-02-08T00:00:00-05:00", "title": "Curiosity's Hazcams Capture a Day on Mars", "description": "A hyperwall ready version of animation publised at https://photojournal.jpl.nasa.gov/catalog/PIA26209NASA's Curiosity Mars rover recorded two 25-frame videos showing the passage of 12 hours on Nov. 8, 2023, the 4,002nd Martian day, or sol, of the mission. The images were captured with Curiosity's front and rear Hazard-Avoidance Cameras, or Hazcams. A long series of images can be put together to create a video so that scientists can look for passing clouds or dust devils, which teach them more about the Martian environment. The perfect time for doing this type of work is when Curiosity is less active for long stretches, as it was during Mars solar conjunction. The lack of robotic arm motion and driving during conjunction allowed the Hazcams to image for 12 hours of a day for the first time. While these Hazcam videos didn't reveal any clouds or dust activity, they did capture the passage of time as the Sun rose and set. || ", "hits": 113 }, { "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": 34 }, { "id": 5200, "url": "https://svs.gsfc.nasa.gov/5200/", "result_type": "Visualization", "release_date": "2023-12-11T12:00:00-05:00", "title": "Mars Disappearing Solar Wind: MAVEN Visualizations", "description": "This data visualization depicts a period of decreased solar wind at Mars that occurred on December 25, 2022, causing the planet’s magnetosphere to expand outward. Ion velocity and density data collected by the MAVEN spacecraft is presented using a color-mapped satellite orbit tail and vectors along MAVEN’s orbit. || maven_solar_wind_comp.02715_print.jpg (1024x576) [84.4 KB] || maven_solar_wind_comp.02715_searchweb.png (320x180) [47.3 KB] || maven_solar_wind_comp.02715_thm.png (80x40) [4.3 KB] || maven_solar_wind_comp (3840x2160) [0 Item(s)] || maven_solar_wind_comp_2160p60.mp4 (3840x2160) [187.6 MB] || maven_solar_wind_comp_prores.mov (3840x2160) [10.1 GB] || ", "hits": 271 }, { "id": 14477, "url": "https://svs.gsfc.nasa.gov/14477/", "result_type": "Produced Video", "release_date": "2023-12-11T12:00:00-05:00", "title": "The Day the Solar Wind Disappeared from Mars", "description": "Learn about the “disappearance” of the solar wind at Mars that was witnessed by MAVEN – an event last seen nearly a quarter-century ago at Earth.Complete transcript available.Universal Production Music: “Space Museum” by Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]; “Currents and Crime Scenes” by Dylan Matthew Love and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || MAVEN_Solar_Wind_Disappear_V4_print.jpg (1024x576) [142.7 KB] || MAVEN_Solar_Wind_Disappear_V4.jpg (1280x720) [459.3 KB] || MAVEN_Solar_Wind_Disappear_V4.png (1280x720) [800.2 KB] || MAVEN_Solar_Wind_Disappear_V4_searchweb.png (320x180) [69.9 KB] || MAVEN_Solar_Wind_Disappear_V4_thm.png (80x40) [6.5 KB] || 14477_MAVEN_Solar_Wind_Disappear_720.mp4 (1280x720) [43.4 MB] || 14477_MAVEN_Solar_Wind_Disappear_1080.mp4 (1920x1080) [243.1 MB] || MavenSolarWindCaptionsV2.en_US.srt [3.8 KB] || MavenSolarWindCaptionsV2.en_US.vtt [3.6 KB] || 14477_MAVEN_Solar_Wind_Disappear_4K.mp4 (3840x2160) [3.0 GB] || 14477_MAVEN_Solar_Wind_Disappear_ProRes.mov (3840x2160) [20.7 GB] || ", "hits": 164 }, { "id": 5177, "url": "https://svs.gsfc.nasa.gov/5177/", "result_type": "Visualization", "release_date": "2023-12-07T00:00:00-05:00", "title": "Polarimetry Data (HARP) and PACE orbit", "description": "This visualization begins with a view of several HARP sample data swaths depicting total radiance and polarized radiance with feature callouts. The camera then pulls back to reveal the PACE spacecraft orbit HARP2 instrument swath (shown in orange). || pace_polarimetry.02020_print.jpg (1024x576) [141.8 KB] || pace_polarimetry.02020_searchweb.png (320x180) [70.1 KB] || pace_polarimetry.02020_thm.png (80x40) [5.3 KB] || pace_polarimetry_1080p60.mp4 (1920x1080) [43.4 MB] || pace_polarimetry (3840x2160) [512.0 KB] || pace_polarimetry_2160p30.mp4 (3840x2160) [118.7 MB] || pace_polarimetry_2160p60.mp4 (3840x2160) [126.6 MB] || pace_polarimetry_prores.mov (3840x2160) [6.8 GB] || ", "hits": 33 }, { "id": 14434, "url": "https://svs.gsfc.nasa.gov/14434/", "result_type": "Produced Video", "release_date": "2023-11-28T09:20:00-05:00", "title": "NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars", "description": "This visualization shows 294 gamma-ray pulsars, first plotted on an image of the entire starry sky as seen from Earth and then transitioning to a view from above our galaxy. The symbols show different types of pulsars. Young pulsars blink in real time except for the Crab, which pulses slower because its rate is only slightly lower than the video frame rate. Millisecond pulsars remain steady, pulsing too quickly to see. The Crab, Vela, and Geminga were among the 11 gamma-ray pulsars known before Fermi launched. Other notable objects are also highlighted. Distances are shown in light-years (abbreviated ly).Credit: NASA’s Goddard Space Flight CenterMusic: \"Fascination\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Pulsar_Still.jpg (3840x2160) [3.5 MB] || Pulsar_Still_searchweb.png (320x180) [105.5 KB] || Pulsar_Still_thm.png (80x40) [7.0 KB] || 14434_Fermi_Pulsar_Locations_1080.mp4 (1920x1080) [93.9 MB] || 14434_Fermi_Pulsar_Locations_1080.webm (1920x1080) [10.0 MB] || Pulsar_Captions.en_US.srt [46 bytes] || Pulsar_Captions.en_US.vtt [56 bytes] || 14434_Fermi_Pulsar_Locations_4k_Good.mp4 (3840x2160) [112.8 MB] || 14434_Fermi_Pulsar_Locations_4k_Best.mp4 (3840x2160) [689.2 MB] || 14434_Fermi_Pulsar_Locations_ProRes_3840x2160_2997.mov (3840x2160) [4.5 GB] || ", "hits": 215 }, { "id": 14438, "url": "https://svs.gsfc.nasa.gov/14438/", "result_type": "Produced Video", "release_date": "2023-10-24T10:00:00-04:00", "title": "Why NASA's Roman Mission Will Study Milky Way's Flickering Lights", "description": "Watch this video to learn about time-domain astronomy and how time will be a key element in the Nancy Grace Roman Space Telescope's galactic bulge survey.Music: \"Elapsing Time\" and \"Beyond Truth\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_TDA-GBS_Still.jpg (1920x1080) [716.0 KB] || Roman_TDA-GBS_Still_print.jpg (1024x576) [206.4 KB] || Roman_TDA-GBS_Still_searchweb.png (320x180) [95.5 KB] || Roman_TDA-GBS_Still_thm.png (80x40) [7.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Sub100.mp4 (1920x1080) [91.9 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.webm (1920x1080) [32.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Good.mp4 (1920x1080) [215.7 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Best.mp4 (1920x1080) [744.2 MB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_Captions.en_US.srt [6.0 KB] || 14438_Roman_TimeDomain_GalacticBulgeSurvey_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || ", "hits": 96 }, { "id": 14435, "url": "https://svs.gsfc.nasa.gov/14435/", "result_type": "B-Roll", "release_date": "2023-10-17T00:00:00-04:00", "title": "Aerial Views of Goddard: Visitor Center", "description": "General afternoon drone footage of the rocket garden, flights between the Visitor Center and Gift Shop toward and away from the rocket garden, and ascents and descents along the Delta B looking west-northwest into the center. Captured June 13, 2023.Credit: NASA/Francis Reddy || Summer_VC_general_still.jpg (3840x2160) [2.5 MB] || Goddard_VCSummerGeneral_1080_30_15mbps.webm (1920x1080) [24.7 MB] || Goddard_VCSummerGeneral_1080_30_15mbps.mp4 (1920x1080) [370.4 MB] || Goddard_VCSummerGeneral_4k60_25mbps.mp4 (3840x2160) [617.5 MB] || Goddard_VCSummer_General_4k60_100mbps.mp4 (3840x2160) [2.4 GB] || ", "hits": 52 }, { "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": 52 }, { "id": 14402, "url": "https://svs.gsfc.nasa.gov/14402/", "result_type": "Produced Video", "release_date": "2023-09-20T13:00:00-04:00", "title": "Simulated Gravitational Wave All-Sky Image", "description": "Watch as gravitational waves from a simulated population of compact binary systems combine into a synthetic map of the entire sky. Such systems contain white dwarfs, neutron stars, or black holes in tight orbits. Maps like this using real data will be possible once space-based gravitational wave observatories become active in the next decade. The center of our Milky Way galaxy lies at the center of this all-sky view, with the galactic plane extending across the middle. Brighter spots indicate sources with stronger signals and lighter colors indicate those with higher frequencies. Larger colored patches show sources whose positions are less well known. The inset shows the frequency and strength of the gravitational signal, as well as the sensitivity limit for LISA (Laser Interferometer Space Antenna), an observatory now being designed by ESA (European Space Agency) in collaboration with NASA for launch in the 2030s.Credit: NASA’s Goddard Space Flight CenterMusic: \"Shadowless\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || LISA_AllSky_withInset_Still.jpg (2985x1497) [795.1 KB] || LISA_AllSky_1080.mp4 (1920x1080) [22.8 MB] || LISA_AllSky_1080.webm (1920x1080) [2.5 MB] || LISA_AllSky_4k.mp4 (3840x2160) [60.4 MB] || LISA_AllSky_SRT_Captions.en_US.srt [205 bytes] || LISA_AllSky_SRT_Captions.en_US.vtt [218 bytes] || LISA_AllSky_ProRes_3840x2160_30.mov (3840x2160) [992.4 MB] || ", "hits": 87 }, { "id": 5145, "url": "https://svs.gsfc.nasa.gov/5145/", "result_type": "Visualization", "release_date": "2023-08-30T00:00:00-04:00", "title": "Franklin Re-intensifies over the Western Atlantic", "description": "Hurricane Franklin in the Atlantic on August 29, 2023 at 2:41Z || Franklin_001.4300_print.jpg (1024x576) [237.7 KB] || Franklin_001.4300_searchweb.png (320x180) [108.1 KB] || Franklin_001.4300_thm.png (80x40) [8.4 KB] || Franklin_001_1080p30_2.mp4 (1920x1080) [52.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Franklin_001_1080p30_2.webm (1920x1080) [5.7 MB] || Franklin_001_1080p30_2.mp4.hwshow [188 bytes] || ", "hits": 62 }, { "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": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 331 }, { "id": 40462, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles3-earthas-art/", "result_type": "Gallery", "release_date": "2023-05-01T00:00:00-04:00", "title": "Cosmic Cycles 3 Earth as Art", "description": "Starting in 1972, nine Landsat satellites have orbited Earth, taking images of the surface. This unprecedented coverage has been tremendously useful to the scientific community, but it has also produced thousands of beautiful high-resolution images of the complex patterns of our world. From the fractal patterns of mountain ranges and river deltas to the precise geometry of agriculture, Landsat has rendered Earth as a work of art.", "hits": 42 }, { "id": 14309, "url": "https://svs.gsfc.nasa.gov/14309/", "result_type": "Produced Video", "release_date": "2023-03-15T11:00:00-04:00", "title": "Fermi Captures Dynamic Gamma-ray Sky", "description": "Watch a cosmic gamma-ray fireworks show in this animation using just a year of data from the Large Area Telescope (LAT) aboard NASA’s Fermi Gamma-ray Space Telescope. Each object’s magenta circle grows as it brightens and shrinks as it dims. The yellow circle represents the Sun following its apparent annual path across the sky. The animation shows a subset of the LAT gamma-ray records now available for more than 1,500 objects in a new, continually updated repository. Over 90% of these sources are a type of galaxy called a blazar, powered by the activity of a supermassive black hole.Credit: NASA’s Marshall Space Flight Center/Daniel Kocevski || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_ProRes_3840x2160.mov (3840x2160) [170.3 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1600.gif (1600x900) [6.5 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_1050.gif (1050x590) [3.2 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark.gif (800x450) [2.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.mp4 (3840x2160) [12.1 MB] || Fermi_LAT_LCR_Feb2022-Feb2023_Dark_4k.webm (3840x2160) [1.9 MB] || ", "hits": 113 }, { "id": 14301, "url": "https://svs.gsfc.nasa.gov/14301/", "result_type": "Produced Video", "release_date": "2023-03-08T10:00:00-05:00", "title": "Millions of Galaxies Emerge in New Simulated Images From NASA's Roman", "description": "This video begins by showing the most distant galaxies in the simulated deep field image in red. As it zooms out, layers of nearer (yellow and white) galaxies are added to the frame. By studying different cosmic epochs, Roman will be able to trace the universe's expansion history, study how galaxies developed over time, and much more.Credit: Caltech-IPAC/R. Hurt and M. Troxel || Roman_Zoom_still.jpg (1920x1080) [515.9 KB] || Roman_Zoom_still_searchweb.png (320x180) [106.4 KB] || Roman_Zoom_still_thm.png (80x40) [6.6 KB] || Roman_Zoom-HD2K.mp4 (1920x1080) [25.3 MB] || Roman_Zoom-HD2K.webm (1920x1080) [2.7 MB] || ", "hits": 72 }, { "id": 14281, "url": "https://svs.gsfc.nasa.gov/14281/", "result_type": "Produced Video", "release_date": "2023-01-26T11:00:00-05:00", "title": "Fermi Spots Gamma-ray Eclipsing 'Spider Systems'", "description": "An orbiting star begins to eclipse its partner, a rapidly rotating, superdense stellar remnant called a pulsar, in this illustration. The pulsar emits multiwavelength beams of light that rotate in and out of view and produces outflows that heat the star’s facing side, blowing away material and eroding its partner.Credit: NASA/Sonoma State University, Aurore Simonnet || GamRayEclipseG22.jpg (1800x1200) [1.1 MB] || GamRayEclipseG22_searchweb.png (320x180) [70.2 KB] || GamRayEclipseG22_thm.png (80x40) [6.8 KB] || ", "hits": 78 }, { "id": 5052, "url": "https://svs.gsfc.nasa.gov/5052/", "result_type": "Visualization", "release_date": "2022-12-12T00:00:00-05:00", "title": "Post-Fire: Assessing Downstream Effects on Hydrology and Water Quality (Thomas Fire)", "description": "Tracing Hydrological impacts of wildfires to understand downstream landslide risks; an example of the 2017 Thomas Fire, Southern California. || thomas_fire_FINAL_035_HD.04500_print.jpg (1024x576) [211.6 KB] || thomas_fire_FINAL_035_HD.04500_searchweb.png (320x180) [81.0 KB] || thomas_fire_FINAL_035_HD.04500_thm.png (80x40) [6.0 KB] || thomas_fire_FINAL_035_HD_1080p59.94.mp4 (1920x1080) [28.5 MB] || 1920x1080_16x9_60p (1920x1080) [256.0 KB] || thomas_fire_FINAL_035_HD_1080p59.94.webm (1920x1080) [6.9 MB] || thomas_fire_FINAL_035_4k_2160p59.94.mp4 (3840x2160) [90.0 MB] || 9600x3240_16x9_30p (9600x3240) [128.0 KB] || 3840x2160_16x9_60p (3840x2160) [256.0 KB] || ", "hits": 37 }, { "id": 14223, "url": "https://svs.gsfc.nasa.gov/14223/", "result_type": "Produced Video", "release_date": "2022-10-20T06:00:00-04:00", "title": "NOAA and NASA Continue Mission to Monitor Extreme Weather and EnhanceForecasts with JPSS-2 Launching Nov. 1 Live Shots", "description": "Associated cut b-roll and pre-recorded interview will be added on Friday, Oct 28th by 4:00 p.m. ET || Screen_Shot_2022-10-19_at_5.13.17_PM.png (3250x1072) [3.1 MB] || Screen_Shot_2022-10-19_at_5.13.17_PM_print.jpg (1024x337) [80.1 KB] || Screen_Shot_2022-10-19_at_5.13.17_PM_searchweb.png (320x180) [93.3 KB] || Screen_Shot_2022-10-19_at_5.13.17_PM_thm.png (80x40) [10.5 KB] || ", "hits": 19 }, { "id": 5035, "url": "https://svs.gsfc.nasa.gov/5035/", "result_type": "Visualization", "release_date": "2022-09-25T00:00:00-04:00", "title": "Fiona Becomes a Major Hurricane in the Atlantic", "description": "Hurricane Fiona west of Bermuda on September 23, 2022 at 6:06 UTC. || Fiona0923L_001.4300_print.jpg (1024x576) [285.1 KB] || Fiona0923L_001.4300_searchweb.png (180x320) [114.1 KB] || Fiona0923L_001.4300_thm.png (80x40) [8.5 KB] || Fiona0923L_001_1080p30_2.mp4 (1920x1080) [84.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Fiona0923L_001_1080p30_2.webm (1920x1080) [6.3 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || Fiona0923L_4K_2160p60.mp4 (3840x2160) [399.3 MB] || Fiona0923L_001_1080p30_2.mp4.hwshow [190 bytes] || ", "hits": 52 }, { "id": 40447, "url": "https://svs.gsfc.nasa.gov/gallery/visualizationsfor-educators/", "result_type": "Gallery", "release_date": "2022-08-17T00:00:00-04:00", "title": "Visualizations for Educators", "description": "Phenomena are observable events that occur in nature. Data visualizations can offer new ways for students to experience and explore Earth and space phenomena that happen over large scales of time and at great distances. This gallery includes visualizations of phenomena that support topics that are taught in middle and high school and are aligned with select Next Generation Science Standards.\n\n\nThis gallery was curated by Anne Arundle County Science Teachers Margaret Graham and Jeremy Milligan with support from Dr. Rachel Connolly during the summer of 2022. A video showing how Jeremy Milligan uses SVS resources to develop a phenomena-based lesson is also available.", "hits": 286 }, { "id": 14175, "url": "https://svs.gsfc.nasa.gov/14175/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Expanding Our View (2022 STScI presentation)", "description": "Complete PowerPoint file with all slides and notes || PPT_still.jpg (3840x2160) [750.6 KB] || roman-expanding-our-view-presentation.pptx [76.2 MB] || Slide #1 – Onscreen before presentation begins and during introductionCredit: STScI, NASA || Slide1_print.jpg (1024x576) [98.1 KB] || Slide1.png (3840x2160) [3.4 MB] || Slide1.jpg (3840x2160) [750.6 KB] || Slide1_searchweb.png (320x180) [63.9 KB] || Slide1_thm.png (80x40) [5.6 KB] || ", "hits": 55 }, { "id": 4976, "url": "https://svs.gsfc.nasa.gov/4976/", "result_type": "Visualization", "release_date": "2022-04-13T10:00:00-04:00", "title": "Seaflow Search for Prochlorococcus", "description": "Overview of data collected from research ship paths through the north Pacific Ocean measuring the phytoplankton species Prochlorococcus with an instrument called Seaflow. Additionally, results from the Darwin global ocean ecosystem computer model show interactions between Prochlorococcus, a copiotrophic heterotrophic bacteria and a shared grazer that limits the poleward extent of Prochlorococcus. || cruise_2-25-2022b_2022-02-25_1746.01500_print.jpg (1024x576) [71.2 KB] || cruise_2-25-2022b_2022-02-25_1746.01500_searchweb.png (320x180) [34.3 KB] || cruise_2-25-2022b_2022-02-25_1746.01500_thm.png (80x40) [3.4 KB] || cruise_2-25-2022b_2022-02-25_1746.webm (1920x1080) [12.8 MB] || annotated (1920x1080) [256.0 KB] || withAnnotation (3840x2160) [256.0 KB] || cruise_2-25-2022b_2022-02-25_1746.mp4 (1920x1080) [179.4 MB] || seaflowCruise_4k_3-31-2022b_2022-03-31_1056_2160p30.mp4 (3840x2160) [531.2 MB] || cruise_2-25-2022b_2022-02-25_1746.mp4.hwshow [238 bytes] || ", "hits": 55 }, { "id": 4977, "url": "https://svs.gsfc.nasa.gov/4977/", "result_type": "Visualization", "release_date": "2022-04-13T10:00:00-04:00", "title": "Darwin Model of Ocean Microbes Updated", "description": "Left: Older Darwin model of global ocean microbiome showing no drop-off of Prochlorococcus populations in arctic regions.Right: New Darwin model, updated to show interactions between heterotrophic bacteria and shared grazer, which prevents Prochlorococcus habitat extending poleward. || seaflow_x4_2-26d_comp.01620_print.jpg (1024x576) [259.0 KB] || seaflow_x4_2-26d_comp.01620_searchweb.png (320x180) [79.6 KB] || seaflow_x4_2-26d_comp.01620_thm.png (80x40) [5.6 KB] || seaflow_x4_2-26d_comp.webm (1920x1080) [12.7 MB] || 1920x1080_16x9_30p (1920x1080) [256.0 KB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || seaflow_x4_2-26d_comp.mp4 (1920x1080) [407.3 MB] || seaflowOverviewCOMP_4k_4-5-2022a_2160p30.mp4 (3840x2160) [863.7 MB] || seaflow_x4_2-26d_comp.mp4.hwshow [214 bytes] || ", "hits": 55 }, { "id": 31180, "url": "https://svs.gsfc.nasa.gov/31180/", "result_type": "Hyperwall Visual", "release_date": "2022-03-10T10:00:00-05:00", "title": "NASA and Agriculture: From Seeds to Satellites", "description": "Complete transcript available. || ComClas_Final_Cut.00148_print.jpg (1024x576) [55.5 KB] || Screen_Shot_2022-03-03_at_1.29.01_PM.png (2478x1382) [1.5 MB] || ComClas_Final_Cut.00148_searchweb.png (320x180) [45.5 KB] || ComClas_Final_Cut.00148_web.png (320x180) [45.5 KB] || ComClas_Final_Cut.00148_thm.png (80x40) [4.1 KB] || ComClas_Final_Cut.webm (1920x1080) [8.0 MB] || ComClas_Final_Cut.mp4 (1920x1080) [126.1 MB] || ComClas_Final_Cut_otter_ai.en_US.srt [1009 bytes] || ComClas_Final_Cut_otter_ai.en_US.vtt [1022 bytes] || ", "hits": 201 }, { "id": 4968, "url": "https://svs.gsfc.nasa.gov/4968/", "result_type": "Visualization", "release_date": "2022-03-09T09:00:00-05:00", "title": "Iowa Cropland 2001-2020", "description": "Modeled Iowa corn (yellow) and soybean (green) yields from 2001-2020. || IowaCrops_2022-02-17_1606.01240_print.jpg (1024x576) [479.4 KB] || IowaCrops_2022-02-17_1606.01240_searchweb.png (320x180) [124.0 KB] || IowaCrops_2022-02-17_1606.01240_web.png (320x180) [124.0 KB] || IowaCrops_2022-02-17_1606.01240_thm.png (80x40) [7.7 KB] || IowaCrops_2022-02-17_1606_1080p30.webm (1920x1080) [12.7 MB] || IowaCrops_2022-02-17_1606_1080p30.mp4 (1920x1080) [267.3 MB] || main (3840x2160) [0 Item(s)] || IowaCrops_2022-02-17_1606.mp4 (3840x2160) [491.4 MB] || IowaCrops_2022-02-17_1606_1080p30.mp4.hwshow [199 bytes] || ", "hits": 40 }, { "id": 14115, "url": "https://svs.gsfc.nasa.gov/14115/", "result_type": "Produced Video", "release_date": "2022-03-08T13:00:00-05:00", "title": "NASA's NICER Tracks a Magnetar's Hot Spots", "description": "Explore how NASA’s Neutron star Interior Composition Explorer (NICER) tracked brilliant hot spots on the surface of an erupting magnetar – from 13,000 light-years away. Credit: NASA's Goddard Space Flight CenterMusic: \"Particles and Fields\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_Still.jpg (1920x1080) [574.3 KB] || Magnetar_Still_print.jpg (1024x576) [229.0 KB] || Magnetar_Still_searchweb.png (320x180) [66.1 KB] || Magnetar_Still_thm.png (80x40) [5.2 KB] || 14115_Merging_Magnetar_HotSpots_1080_Best.webm (1920x1080) [17.4 MB] || 14115_Merging_Magnetar_HotSpots_1080.mp4 (1920x1080) [158.9 MB] || 14115_Merging_Magnetar_HotSpots_1080_Best.mp4 (1920x1080) [382.0 MB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.srt [2.1 KB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.vtt [2.1 KB] || 14115_Merging_Magnetar_HotSpots_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || ", "hits": 210 }, { "id": 14095, "url": "https://svs.gsfc.nasa.gov/14095/", "result_type": "Produced Video", "release_date": "2022-02-09T09:00:00-05:00", "title": "NASA’s New Views of Venus’ Surface From Space", "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ", "hits": 861 }, { "id": 14055, "url": "https://svs.gsfc.nasa.gov/14055/", "result_type": "Produced Video", "release_date": "2021-12-20T22:00:00-05:00", "title": "Parker Solar Probe's WISPR Images Inside The Sun's Atmosphere", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. As Parker Solar Probe flew through the corona, its WISPR instrument captured images.The Wide-Field Imager for Parker Solar Probe (WISPR) is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment.To image the solar atmosphere, WISPR uses the heat shield to block most of the Sun’s light, which would otherwise obscure the much fainter corona. Specially designed baffles and occulters reflect and absorb the residual stray light that has been reflected or diffracted off the edge of the heat shield or other parts of the spacecraft.WISPR uses two cameras with radiation-hardened Active Pixel Sensor CMOS detectors. These detectors are used in place of traditional CCDs because they are lighter and use less power. They are also less susceptible to effects of radiation damage from cosmic rays and other high-energy particles, which are a big concern close to the Sun. The camera’s lenses are made of a radiation hard BK7, a common type of glass used for space telescopes, which is also sufficiently hardened against the impacts of dust.WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, D.C. (principal investigator Russell Howard), which will also develop the observing program. || ", "hits": 650 }, { "id": 13867, "url": "https://svs.gsfc.nasa.gov/13867/", "result_type": "Produced Video", "release_date": "2021-11-30T10:00:00-05:00", "title": "Lasers in Space: NASA is launching a new era of communications in space Dec. 5 Live Shots", "description": "Quick link to associated B-ROLL for the live shots.Quick link to canned interview with LCRD Project Manager GLENN JACKSON. || LCRD.png (1512x502) [959.2 KB] || LCRD_print.jpg (1024x339) [75.8 KB] || LCRD_searchweb.png (320x180) [103.8 KB] || LCRD_thm.png (80x40) [11.1 KB] || ", "hits": 35 }, { "id": 4914, "url": "https://svs.gsfc.nasa.gov/4914/", "result_type": "Visualization", "release_date": "2021-09-01T00:00:00-04:00", "title": "Impact of Climate Change on Global Wheat Yields", "description": "Data visualization of predicted Wheat yields through the end of this centaury based on an ensemble of crop and climate models. || WheatMapFuture.01000_print.jpg (1024x576) [123.1 KB] || WheatMapFuture.01000_searchweb.png (320x180) [54.6 KB] || WheatMapFuture.01000_web.png (320x180) [54.6 KB] || WheatMapFuture.01000_thm.png (80x40) [5.4 KB] || WheatMapFuture_1080p.mp4 (1920x1080) [21.7 MB] || WheatMapFuture.mp4 (3840x2160) [79.7 MB] || WheatMapFuture.webm (3840x2160) [6.4 MB] ||", "hits": 132 }, { "id": 13876, "url": "https://svs.gsfc.nasa.gov/13876/", "result_type": "Produced Video", "release_date": "2021-07-12T10:00:00-04:00", "title": "TESS Finds Related Stars Have Young Exoplanets", "description": "Stellar siblings over 130 light-years away host two systems of teenage planets. Watch to learn how NASA’s Transiting Exoplanet Survey Satellite discovered these young worlds and what they might tell us about the evolution of planetary systems everywhere, including our own.Music Credit: \"Building Ideas\" from Universal Production MusicCredit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || tess_stellar_siblings_label.jpg (1920x1080) [572.8 KB] || stellar_siblings_still_01.jpg (1920x1080) [536.3 KB] || stellar_siblings_still_01_print.jpg (1024x576) [179.0 KB] || stellar_siblings_still_01_searchweb.png (320x180) [57.0 KB] || stellar_siblings_still_01_web.png (320x180) [57.0 KB] || stellar_siblings_still_01_thm.png (80x40) [4.7 KB] || TESS_stellar_siblings_HQ.mp4 (1920x1080) [286.2 MB] || TESS_stellar_siblings_LQ.mp4 (1920x1080) [150.7 MB] || TESS_stellar_siblings_prores.mov (1920x1080) [1.6 GB] || TESS_stellar_siblings_LQ.webm (1920x1080) [16.0 MB] || TESS_stellar_siblings_prores.en_US.srt [2.0 KB] || TESS_stellar_siblings_prores.en_US.vtt [2.0 KB] || ", "hits": 135 }, { "id": 13860, "url": "https://svs.gsfc.nasa.gov/13860/", "result_type": "Produced Video", "release_date": "2021-06-17T16:00:00-04:00", "title": "Animation of USPS Stamps Featuring NASA's Solar Dynamic Observatory", "description": "The U.S. Postal Service illuminates the light and warmth of our nearest star by highlighting these stunning images of the Sun on stamps. These images come from NASA’s Solar Dynamics Observatory, a spacecraft launched in February 2010 to keep a constant watch on the Sun.The Sun is the only star that humans are able to observe in great detail, making it a vital source of information about the universe. The Solar Dynamics Observatory lets us see the Sun in wavelengths of ultraviolet light that would otherwise be invisible to our eyes. Each black-and-white image is colorized to the bright hues seen here.The stamps highlight different features on the Sun that help scientists learn about how our star works and how its constantly churning magnetic fields create the solar activity we see. Sunspots, coronal holes and coronal loops, for example, can reveal how those magnetic fields dance through the Sun and its atmosphere. Observing plasma blasts and solar flares can help us better understand and mitigate the impact of such eruptions on technology in space.The Sun Science stamps are being issued as Forever stamps, which will always be equal in value to the current First-Class Mail 1-ounce price. || ", "hits": 48 }, { "id": 13852, "url": "https://svs.gsfc.nasa.gov/13852/", "result_type": "Produced Video", "release_date": "2021-05-26T10:00:00-04:00", "title": "NASA’s Roman Mission to Probe Cosmic Secrets Using Exploding Stars", "description": "NASA’s upcoming Nancy Grace Roman Space Telescope will see thousands of exploding stars called supernovae across vast stretches of time and space. Using these observations, astronomers aim to shine a light on several cosmic mysteries, providing a window onto the universe’s distant past and hazy present.Credit: NASA's Goddard Space Flight CenterMusic: \"Relentless Data\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Supernova_IA_1285_print.jpg (1024x576) [53.0 KB] || Supernova_IA_1285.png (3840x2160) [5.0 MB] || Supernova_IA_1285_searchweb.png (320x180) [46.9 KB] || Supernova_IA_1285_thm.png (80x40) [4.6 KB] || 13852_Roman_Standard_Candle_Supernovae_1080_Best.webm (1920x1080) [28.3 MB] || 13852_Roman_Standard_Candle_Supernovae_1080.mp4 (1920x1080) [136.7 MB] || 13852_Roman_Standard_Candle_Supernovae_1080_Best.mp4 (1920x1080) [654.2 MB] || 13852RomanStandardCandleSupernovaeCaptionsFix.en_US.srt [4.7 KB] || 13852RomanStandardCandleSupernovaeCaptionsFix.en_US.vtt [4.7 KB] || 13852_Roman_Standard_Candle_Supernovae_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 113 }, { "id": 20344, "url": "https://svs.gsfc.nasa.gov/20344/", "result_type": "Animation", "release_date": "2021-05-26T10:00:00-04:00", "title": "Type Ia Supernovae Animations", "description": "White Dwarf establishing shot. || WDStar_4k_60fps_ProRes.00600_print.jpg (1024x576) [27.4 KB] || WDStar_4k_60fps_ProRes.00600_searchweb.png (320x180) [30.7 KB] || WDStar_4k_60fps_ProRes.00600_thm.png (80x40) [3.2 KB] || WDStar_4k_60fps_h264.mp4 (3840x2160) [37.3 MB] || WDStar_4k (3840x2160) [0 Item(s)] || WDStar_4k_60fps_ProRes.webm (3840x2160) [4.1 MB] || WDStar_4k_60fps_ProRes.mov (3840x2160) [3.0 GB] || ", "hits": 348 }, { "id": 13737, "url": "https://svs.gsfc.nasa.gov/13737/", "result_type": "Produced Video", "release_date": "2021-04-08T14:00:00-04:00", "title": "NASA’s NICER Finds X-ray Boosts in the Crab Pulsar’s Radio Bursts", "description": "Observations from NASA’s Neutron star Interior Composition Explorer (NICER) show X-ray boosts linked in the Crab pulsar's random giant radio pulses. Watch to learn more. Credit: NASA's Goddard Space Flight CenterMusic: \"The Awakening\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Crab_Radio_Still.jpg (1920x1080) [865.4 KB] || Crab_Radio_Still_searchweb.png (320x180) [65.9 KB] || Crab_Radio_Still_thm.png (80x40) [5.2 KB] || 13737_Crab_Pulsar_Radio_Bursts_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.mp4 (1920x1080) [275.3 MB] || 13737_Crab_Pulsar_Radio_Bursts_1080.mp4 (1920x1080) [114.7 MB] || 13737_Crab_Pulsar_Radio_Bursts_Best_1080.webm (1920x1080) [15.2 MB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.srt [2.6 KB] || 13737_Crab_Pulsar_Radio_Bursts_SRT_Captions.en_US.vtt [2.6 KB] || ", "hits": 142 }, { "id": 13806, "url": "https://svs.gsfc.nasa.gov/13806/", "result_type": "Produced Video", "release_date": "2021-03-12T11:00:00-05:00", "title": "Scientists Build a Detailed Image of U Mon Binary", "description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ", "hits": 28 }, { "id": 13805, "url": "https://svs.gsfc.nasa.gov/13805/", "result_type": "Produced Video", "release_date": "2021-02-22T11:00:00-05:00", "title": "Swift Links Neutrino to Star-destroying Black Hole", "description": "Watch how a monster black hole ripping apart a star may have launched a ghost particle toward Earth. Astronomers have long predicted that tidal disruption events could produce high-energy neutrinos, nearly massless particles from outside our galaxy traveling close to the speed of light. One recent event, named AT2019dsg, provides the first proof this prediction is true but has challenged scientists’ assumptions of where and when these elusive particles might form during these destructive outbursts. Credit: NASA’s Goddard Space Flight CenterMusic: \"Diagnostic Report\" from Universal Production MusicComplete transcript available. || AT2019dsg_prores_still.jpg (1920x1080) [299.2 KB] || AT2019dsg_prores_still_print.jpg (1024x576) [119.5 KB] || AT2019dsg_prores_still_searchweb.png (180x320) [42.6 KB] || AT2019dsg_prores_still_web.png (320x180) [42.6 KB] || AT2019dsg_prores_still_thm.png (80x40) [4.1 KB] || AT2019dsg_HQ.mp4 (1920x1080) [347.5 MB] || AT2019dsg_LQ.mp4 (1920x1080) [191.3 MB] || AT2019dsg_prores.mov (1920x1080) [1.7 GB] || AT2019dsg_LQ.webm (1920x1080) [21.5 MB] || AT2019dsg_LQ.en_US.srt [3.7 KB] || AT2019dsg_LQ.en_US.vtt [3.7 KB] || ", "hits": 95 }, { "id": 13792, "url": "https://svs.gsfc.nasa.gov/13792/", "result_type": "Produced Video", "release_date": "2021-01-13T12:15:00-05:00", "title": "NASA Missions Unveil Magnetar Eruptions in Nearby Galaxies", "description": "On April 15, 2020, a wave of X-rays and gamma rays lasting only a fraction of a second triggered detectors on NASA and European spacecraft. The event was a giant flare from a magnetar, a type of city-sized stellar remnant that boasts the strongest magnetic fields known. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Collision Course-Alternative Version\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MGF_Video_Still.jpg (1920x1080) [602.3 KB] || MGF_Video_Still_print.jpg (1024x576) [264.7 KB] || MGF_Video_Still_searchweb.png (320x180) [74.9 KB] || MGF_Video_Still_thm.png (80x40) [5.7 KB] || 13792_Magnetar_Giant_Flare_ProRes_1920x1080_2997.mov (1920x1080) [2.6 GB] || 13792_Magnetar_Giant_Flare_best_1080.mp4 (1920x1080) [498.6 MB] || 13792_Magnetar_Giant_Flare_good_1080.mp4 (1920x1080) [221.6 MB] || 13792_Magnetar_Giant_Flare_best_1080.webm (1920x1080) [24.0 MB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.srt [4.0 KB] || 13792_Magnetar_Giant_Flare_SRT_Captions.en_US.vtt [4.0 KB] || ", "hits": 228 }, { "id": 13776, "url": "https://svs.gsfc.nasa.gov/13776/", "result_type": "Produced Video", "release_date": "2020-12-15T21:00:00-05:00", "title": "2020 AGU Roundtable: What will we learn from Solar Cycle 25?", "description": "Solar Cycle 25 is here, ushering in the next season of space weather from the Sun. As our star’s activity ramps up—a natural part of its roughly 11-year cycle—scientists are eager to test their predictions. In this AGU 2020 media roundtable, scientists will discuss outstanding questions in solar cycle science, what opportunities this new cycle provides researchers, and how we track progress in predictions. || ", "hits": 91 }, { "id": 20338, "url": "https://svs.gsfc.nasa.gov/20338/", "result_type": "Animation", "release_date": "2020-12-08T15:00:00-05:00", "title": "SunRISE Beauty Pass", "description": "A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events. || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_print.jpg (1024x576) [172.5 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_searchweb.png (320x180) [87.2 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_thm.png (80x40) [5.9 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.mov (3840x2160) [695.8 MB] || SUNRISE-shot1_v06_4k_30fps_h264.mp4 (3840x2160) [13.7 MB] || SUNRISE-shot1_v06_4k (3840x2160) [32.0 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.webm (3840x2160) [5.3 MB] || ", "hits": 55 }, { "id": 13751, "url": "https://svs.gsfc.nasa.gov/13751/", "result_type": "Produced Video", "release_date": "2020-11-04T11:00:00-05:00", "title": "NASA Missions Team Up to Study Unique Magnetar Outburst", "description": "On April 28, space- and ground-based observatories detected powerful, simultaneous X-ray and radio bursts from a source in our galaxy. Watch to see how this unique event helps solve the longstanding puzzle of fast radio bursts observed in other galaxies.Credit: NASA's Goddard Space Flight CenterMusic: \"Jupiter's Eye\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_FRB_Still.jpg (1920x1080) [535.5 KB] || Magnetar_FRB_Still_searchweb.png (320x180) [65.5 KB] || Magnetar_FRB_Still_thm.png (80x40) [4.8 KB] || 13751_Magnetar_FRB_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || 13751_Magnetar_FRB_Best_1080.mp4 (1920x1080) [741.8 MB] || 13751_Magnetar_FRB_1080.mp4 (1920x1080) [237.4 MB] || 13751_Magnetar_FRB_Best_1080.webm (1920x1080) [25.7 MB] || Fast_Radio_Burst_SRT_Captions.en_US.srt [4.5 KB] || Fast_Radio_Burst_SRT_Captions.en_US.vtt [4.5 KB] || ", "hits": 231 }, { "id": 13687, "url": "https://svs.gsfc.nasa.gov/13687/", "result_type": "Produced Video", "release_date": "2020-08-14T10:00:00-04:00", "title": "NASA Spacecraft Uncover Mystery Behind Auroral Beads", "description": "A special type of aurora, draped east-west across the night sky like a glowing pearl necklace, is helping scientists better understand the science of auroras and their powerful drivers out in space. Known as auroral beads, these lights often show up just before large auroral displays, which are caused by electrical storms in space called substorms. Until now, scientists weren’t sure if auroral beads are somehow connected to other auroral displays as a phenomenon in space that precedes substorms, or if they are caused by disturbances closer to Earth’s atmosphere.But powerful new computer models, combined with observations from NASA’s Time History of Events and Macroscale Interactions during Substorms – THEMIS – mission, have provided the first direct evidence of the events in space that lead to the appearance of these beads, and demonstrated the important role they play in our local space environment. || ", "hits": 80 }, { "id": 13647, "url": "https://svs.gsfc.nasa.gov/13647/", "result_type": "Produced Video", "release_date": "2020-06-25T07:45:00-04:00", "title": "NASA, ESA, JAXA Release Global View of COVID-19 Impacts", "description": "NASA, ESA (European Space Agency) and JAXA (Japan Aerospace Exploration Agency) have created a dashboard of satellite data showing impacts on the environment and socioeconomic activity caused by the global response to the coronavirus (COVID-19) pandemic.The dashboard will be released on Thursday, June 25 during a tri-agency media briefing. The briefing speakers are:•Josef Aschbacher, director of ESA Earth Observation Programmes•Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate•Koji Terada, vice president and director general for the Space Technology Directorate at JAXA•Shin-ichi Sobue, project manager for JAXA’s ALOS-2 mission•Ken Jucks, program scientist for NASA’s OCO-2 and Aura missions•Anca Anghelea, open data scientist, ESA Earth observation programmes || ", "hits": 98 }, { "id": 13648, "url": "https://svs.gsfc.nasa.gov/13648/", "result_type": "Produced Video", "release_date": "2020-06-24T11:00:00-04:00", "title": "TESS, Spitzer Missions Discover a Unique Young World", "description": "NASA’s Transiting Exoplanet Survey Satellite (TESS) and retired Spitzer Space Telescope have found a young Neptune-size world orbiting AU Microscopii, a cool, nearby M-type red dwarf star surrounded by a vast disk of debris. The discovery makes the system a touchstone for understanding how stars and planets form and evolve. Credit: NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Music: \"Web Of Intrigue\" from Universal Production Music.Complete transcript available. || au_mic_still.jpg (1920x1080) [286.6 KB] || au_mic_still_print.jpg (1024x576) [94.9 KB] || au_mic_still_searchweb.png (320x180) [41.3 KB] || au_mic_still_web.png (320x180) [41.3 KB] || au_mic_still_thm.png (80x40) [3.8 KB] || au_mic_HQ.mp4 (1920x1080) [112.1 MB] || au_mic_LQ.mp4 (1920x1080) [118.3 MB] || au_mic_prores.mov (1920x1080) [1.1 GB] || au_mic_LQ.webm (1920x1080) [13.1 MB] || au_mic_LQ.en_US.srt [2.2 KB] || au_mic_LQ.en_US.vtt [2.1 KB] || ", "hits": 68 }, { "id": 13605, "url": "https://svs.gsfc.nasa.gov/13605/", "result_type": "Produced Video", "release_date": "2020-05-13T11:00:00-04:00", "title": "TESS Aids Breakthrough in Puzzling Stellar Flashes", "description": "Watch the pulsations of a Delta Scuti star! In this illustration, the star changes in brightness when internal sound waves at different frequencies cause parts of the star to expand and contract. In one pattern, the whole star expands and contracts, while in a second, opposite hemispheres swell and shrink out of sync. In reality, a single star exhibits many pulsation patterns that can tell astronomers about its age, composition and internal structure. The exact light variations astronomers observe also depend on how the star's spin axis angles toward us. Delta Scuti stars spin so rapidly they flatten into ovals, which jumbles these signals and makes them harder to decode. Now, thanks to NASA's Transiting Exoplanet Survey Satellite, astronomers are deciphering some of them.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || Exterior_still.jpg (1920x1080) [460.3 KB] || 13605_Delta_Scuti_Pulsation_ProRes_1920x1080_2997.mov (1920x1080) [523.3 MB] || 13605_Delta_Scuti_Pulsation.mp4 (1920x1080) [36.1 MB] || 13605_Delta_Scuti_Pulsation.webm (1920x1080) [3.6 MB] || ", "hits": 57 }, { "id": 20315, "url": "https://svs.gsfc.nasa.gov/20315/", "result_type": "Animation", "release_date": "2020-03-30T10:00:00-04:00", "title": "Roman Space Telescope Microlensing Animations", "description": "This animation illustrates the concept of gravitational microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the warped space-time around the foreground star. This star is then a virtual magnifying glass, amplifying the brightness of the background source star, so we refer to the foreground star as the lens star. If the lens star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. Thus we discover the presence of exoplanets, and measure its mass and separation from its star. Credit: NASA's Goddard Space Flight Center/CI LabWatch this video on the NASA.gov Video YouTube channel. || WFIRST_Microlensing_S1a_4k_30fps_ProRes.00236_print.jpg (1024x576) [57.6 KB] || WFIRST_Microlensing_S1a_4k_30fps_ProRes.mov (3840x2160) [1.9 GB] || WFIRST_Microlensing_S1a_4k_30fps_h264.mp4 (3840x2160) [20.7 MB] || S1a (3840x2160) [64.0 KB] || WFIRST_Microlensing_S1a_4k_30fps_h264.webm (3840x2160) [2.9 MB] || ", "hits": 138 }, { "id": 13556, "url": "https://svs.gsfc.nasa.gov/13556/", "result_type": "Produced Video", "release_date": "2020-02-14T03:00:00-05:00", "title": "Astrophysics Valentines", "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ", "hits": 80 }, { "id": 31115, "url": "https://svs.gsfc.nasa.gov/31115/", "result_type": "Hyperwall Visual", "release_date": "2020-02-12T00:00:00-05:00", "title": "Airglow over Australia", "description": "airglow over australia seen from the ISS || airglow-australia_print.jpg (1024x576) [150.3 KB] || airglow-australia.png (3840x2160) [15.1 MB] || airglow-australia_searchweb.png (320x180) [80.8 KB] || airglow-australia_thm.png (80x40) [4.7 KB] || airglow-over-australia.hwshow [280 bytes] || ", "hits": 181 }, { "id": 31098, "url": "https://svs.gsfc.nasa.gov/31098/", "result_type": "Hyperwall Visual", "release_date": "2020-01-31T00:00:00-05:00", "title": "Beyond City Lights—Java Sea", "description": "Beyond City Lights—Java Sea || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_print.jpg (1024x576) [114.4 KB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8.png (5760x3240) [13.6 MB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_searchweb.png (320x180) [78.2 KB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_thm.png (80x40) [4.7 KB] || beyond-city-lightsjava-sea.hwshow [336 bytes] || ", "hits": 116 }, { "id": 40409, "url": "https://svs.gsfc.nasa.gov/gallery/fermi-stills/", "result_type": "Gallery", "release_date": "2020-01-22T00:00:00-05:00", "title": "Fermi Stills", "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.", "hits": 271 }, { "id": 13496, "url": "https://svs.gsfc.nasa.gov/13496/", "result_type": "Produced Video", "release_date": "2020-01-06T19:15:00-05:00", "title": "TESS Mission’s First Earth-size World in Star’s Habitable-zone", "description": "Take a tour through TOI 700, a planetary system 100 light-years away in the constellation Dorado. One of the system’s residents is TOI 700 d, the first Earth-size habitable-zone planet discovered by NASA’s Transiting Exoplanet Survey Satellite. Credit: NASA’s Goddard Space Flight Center.Music: \"Family Tree\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TOI_700d.jpg (1920x1080) [397.4 KB] || TOI_700d_print.jpg (1024x576) [128.3 KB] || TOI_700d_searchweb.png (320x180) [65.8 KB] || TOI_700d_thm.png (80x40) [5.5 KB] || 13496_TOI700_Earth-size_1080.webm (1920x1080) [25.7 MB] || 13496_TOI700_Earth-size_1080.mp4 (1920x1080) [229.2 MB] || 13496_TOI700_Earth-size_1080_Best.mp4 (1920x1080) [394.2 MB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.srt [4.4 KB] || TESS_TOI700_Earth-size_SRT_Captions.en_US.vtt [4.4 KB] || 13496_TOI700_Earth-size_ProRes_1920x1080.mov (1920x1080) [2.7 GB] || ", "hits": 464 }, { "id": 13209, "url": "https://svs.gsfc.nasa.gov/13209/", "result_type": "Produced Video", "release_date": "2019-12-19T12:00:00-05:00", "title": "NASA’s Fermi Finds Vast ‘Halo’ Around Nearby Pulsar", "description": "Astronomers using data from NASA’s Fermi mission have discovered a pulsar with a faint gamma-ray glow that spans a huge part of the sky. Watch to learn more.Credit: NASA’s Goddard Space Flight CenterMusic: \"Insight\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Geminga_Still.jpg (1920x1080) [177.1 KB] || Geminga_Still_print.jpg (1024x576) [65.2 KB] || Geminga_Still_searchweb.png (320x180) [75.1 KB] || Geminga_Still_thm.png (80x40) [5.6 KB] || 13209_Fermi_Geminga_Halo_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || 13209_Fermi_Geminga_Halo_1080_Best.mp4 (1920x1080) [294.5 MB] || 13209_Fermi_Geminga_Halo_1080_Best.webm (1920x1080) [15.3 MB] || 13209_Fermi_Geminga_Halo_1080_Good.mp4 (1920x1080) [144.1 MB] || Fermi_Geminga_Halo_SRT_Captions.en_US.srt [1.7 KB] || Fermi_Geminga_Halo_SRT_Captions.en_US.vtt [1.7 KB] || ", "hits": 72 }, { "id": 13422, "url": "https://svs.gsfc.nasa.gov/13422/", "result_type": "Produced Video", "release_date": "2019-12-17T10:00:00-05:00", "title": "A New Kind of Explosion on the Sun", "description": "Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Credit: Light Hearted Angst by Dewey Dellay || ReconnThumb.jpg (1920x1080) [156.1 KB] || ReconnThumb_searchweb.png (320x180) [100.6 KB] || ReconnThumb_thm.png (80x40) [7.3 KB] || ForcedReconnV2_Twitter.mp4 (1920x1080) [29.6 MB] || ForcedReconnV2.webm (1920x1080) [14.8 MB] || ForcedReconnV2.mp4 (1920x1080) [134.9 MB] || ForcedReconnV2_FB.mp4 (1920x1080) [155.5 MB] || ForcedReconnV2_YouTube.mp4 (1920x1080) [207.3 MB] || ForcedReconnV2.en_US.srt [2.6 KB] || ForcedReconnV2.en_US.vtt [2.6 KB] || ForcedReconnV2.mov (1920x1080) [1.7 GB] || ", "hits": 124 }, { "id": 13477, "url": "https://svs.gsfc.nasa.gov/13477/", "result_type": "Produced Video", "release_date": "2019-12-09T14:00:00-05:00", "title": "Operation IceBridge - Spring Svalbard Sea Ice", "description": "On April 7, 2017, Operation IceBridge flew the distinct Zig Zag East mission. This flight started in the rugged fjords of Svalbard, passed over hundreds of miles of sea ice en route to the North Pole, flew through the narrow Nares Strait, and finally returned the team back to Thule Air Base in Greenland. The clip below shows dramatic sea ice encountered north of Svalbard as the mission prepard to cross the Fram Strait (the primary pathway that sea ice from the Arctic Basin gets out to warmer ocean). This type of sea ice is commonly referred to as broken pack ice. || ", "hits": 21 }, { "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": 68 }, { "id": 13427, "url": "https://svs.gsfc.nasa.gov/13427/", "result_type": "Produced Video", "release_date": "2019-11-20T13:00:00-05:00", "title": "A New Era in Gamma-ray Science", "description": "On Jan. 14, 2019, the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) observatory in the Canary Islands captured the highest-energy light every recorded from a gamma-ray burst. MAGIC began observing the fading burst just 50 seconds after it was detected thanks to positions provided by NASA's Fermi and Swift spacecraft (top left and right, respectively, in this illustration). The gamma rays packed energy up to 10 times greater than previously seen. Credit: NASA/Fermi and Aurore Simonnet, Sonoma State University || GRB190114CbASimonnet.jpg (2475x3300) [4.5 MB] || GRB190114CbASimonnet_searchweb.png (320x180) [106.4 KB] || GRB190114CbASimonnet_thm.png (80x40) [6.6 KB] || ", "hits": 109 }, { "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": 83 }, { "id": 13297, "url": "https://svs.gsfc.nasa.gov/13297/", "result_type": "Produced Video", "release_date": "2019-09-02T00:00:00-04:00", "title": "Animations of TESS's First Exoplanets", "description": "Illustration of the exoplanet LHS 3844 b. It is a rocky planet about 1.3 times Earth’s size located about 49 light-years away in the constellation Indus, making it among the closest transiting exoplanets known. The star is a cool M-type dwarf star about one-fifth the size of our Sun. Completing an orbit every 11 hours, the planet lies so close to its star that some of its rocky surface on the daytime side may form pools of molten lava.Credit: NASA/MIT/TESS || LHS3844b_Still_print.jpg (1024x1023) [170.9 KB] || LHS3844b_Still.png (2144x2142) [6.8 MB] || LHS3844b_Still_searchweb.png (320x180) [83.2 KB] || LHS3844b_Still_thm.png (80x40) [5.5 KB] || LHS3844b_4K_1.mp4 (1080x1080) [49.4 MB] || LHS3844b_4K_1.webm (1080x1080) [4.6 MB] || LHS3844b_4K.mp4 (4096x4096) [482.9 MB] || LHS3844b_4K_2.mp4 (4096x4096) [98.6 MB] || ", "hits": 182 }, { "id": 13236, "url": "https://svs.gsfc.nasa.gov/13236/", "result_type": "Produced Video", "release_date": "2019-08-15T09:50:00-04:00", "title": "Fermi Sees the Moon in Gamma Rays", "description": "These images show the steadily improving view of the Moon’s gamma-ray glow from NASA’s Fermi Gamma-ray Space Telescope. Each 5-by-5-degree image is centered on the Moon and shows gamma rays with energies above 31 million electron volts, or tens of millions of times that of visible light. At these energies, the Moon is actually brighter than the Sun. Brighter colors indicate greater numbers of gamma rays. This image sequence shows how longer exposure, ranging from two to 128 months (10.7 years), improved the view.Credit: NASA/DOE/Fermi LAT Collaboration || MoonvsTimesingleimageen.jpg (4322x2161) [5.2 MB] || ", "hits": 113 }, { "id": 13269, "url": "https://svs.gsfc.nasa.gov/13269/", "result_type": "Produced Video", "release_date": "2019-08-07T00:00:00-04:00", "title": "Exoplanet HD 21749 c Animation", "description": "This animation shows HD 21749 c, an exoplanet about 89% Earth’s diameter. It orbits HD 21749, a K-type star with about 70% of the Sun’s mass located 53 light-years away in the southern constellation Reticulum. A second, bluish exoplanet in the same system, HD 21749 b, appears briefly in the background.Credit: NASA/JPL-Caltech/R. Hurt (IPAC) || HD_21749c_Still.png (1792x1057) [1.7 MB] || HD_21749c_Still_print.jpg (1024x604) [63.4 KB] || HD_21749c_Still_searchweb.png (320x180) [61.0 KB] || HD_21749c_Still_thm.png (80x40) [4.5 KB] || TESS_Exoplanet_HD_21749c_v2.mp4 (1920x1080) [23.8 MB] || TESS_Exoplanet_HD_21749c_v2.webm (1920x1080) [2.3 MB] || TESS_Exoplanet_HD_21749c_v2.mov (1920x1080) [330.6 MB] || Tess_trappist_compiled.hwshow || ", "hits": 269 }, { "id": 13266, "url": "https://svs.gsfc.nasa.gov/13266/", "result_type": "Produced Video", "release_date": "2019-07-31T10:00:00-04:00", "title": "TESS Discovery Leads to Surprising Find of Promising World", "description": "Tour the GJ 357 system, located 31 light-years away in the constellation Hydra. Astronomers confirming a planet candidate identified by NASA’s Transiting Exoplanet Survey Satellite subsequently found two additional worlds orbiting the star. The outermost planet, GJ 357 d, is especially intriguing to scientists because it receives as much energy from its star as Mars does from the Sun. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Music: \"Golden Temple\" from Killer Tracks.Complete transcript available.See the bottom of the page for a version without on-screen text. || tess_gj357_english_thm.jpg (1920x1080) [798.7 KB] || tess_gj357_english_thm_print.jpg (1024x576) [291.4 KB] || tess_gj357_english_thm_searchweb.png (180x320) [79.3 KB] || tess_gj357_english_thm_web.png (320x180) [79.3 KB] || tess_gj357_english_thm_thm.png (80x40) [5.7 KB] || tess_gj357_english_HQ.webm (1920x1080) [15.6 MB] || tess_gj357_english_LQ.mp4 (1920x1080) [139.2 MB] || tess_gj357_english_HQ.mp4 (1920x1080) [259.3 MB] || tess_gj357_english.en_US.srt [2.4 KB] || tess_gj357_english.en_US.vtt [2.4 KB] || tess_gj357_english_prores.mov (1920x1080) [1.4 GB] || ", "hits": 308 }, { "id": 13200, "url": "https://svs.gsfc.nasa.gov/13200/", "result_type": "Produced Video", "release_date": "2019-07-29T10:00:00-04:00", "title": "NASA’s TESS Finds Three New Worlds", "description": "This infographic illustrates key features of the TOI 270 system, located about 73 light-years away in the southern constellation Pictor. The three known planets were discovered by NASA’s Transiting Exoplanet Survey Satellite through periodic dips in starlight caused by each orbiting world. Insets show information about the planets, including their relative sizes, and how they compare to Earth. Temperatures given for TOI 270’s planets are equilibrium temperatures, calculated without the warming effects of any possible atmospheres. Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || TOI_270_Infographic_Final_print.jpg (1024x576) [64.1 KB] || TOI_270_Infographic_Final.png (5760x3240) [17.4 MB] || TOI_270_Infographic_Final.jpg (5760x3240) [2.0 MB] || TOI_270_Infographic_Final-halfsize.png (2880x1620) [5.4 MB] || TOI_270_Infographic_Final-halfsize.jpg (2880x1620) [484.0 KB] || TOI_270_Infographic_Final_searchweb.png (320x180) [47.7 KB] || TOI_270_Infographic_Final_thm.png (80x40) [4.9 KB] || ", "hits": 233 }, { "id": 13127, "url": "https://svs.gsfc.nasa.gov/13127/", "result_type": "Produced Video", "release_date": "2019-05-20T12:00:00-04:00", "title": "Arctic Bubbles", "description": "Methane bubbles up from permafrost beneath Arctic lakes. || bubblesPic2-1.jpeg (1335x738) [601.8 KB] || bubblesPic2-1_1024x576.jpg (1024x576) [456.6 KB] || ", "hits": 117 }, { "id": 13167, "url": "https://svs.gsfc.nasa.gov/13167/", "result_type": "Produced Video", "release_date": "2019-05-07T15:00:00-04:00", "title": "VISIONS-2 Aurora Imagery", "description": "Aurora in Ny-Ålesund, Svalbard on December 6, 2018. A GIF optimized for Twitter. || Aurora.gif (1920x1080) [13.3 MB] || Aurora in Ny-Ålesund, Svalbard on December 6, 2018.Credit: NASA/Joy Ng || Dec6_Aurora_JoyNg_print.jpg (1024x682) [455.2 KB] || Dec6_Aurora_JoyNg.jpg (4104x2736) [4.6 MB] || Dec6_Aurora_JoyNg_searchweb.png (320x180) [67.8 KB] || Dec6_Aurora_JoyNg_web.png (320x213) [82.2 KB] || Dec6_Aurora_JoyNg_thm.png (80x40) [4.6 KB] || ", "hits": 135 }, { "id": 12853, "url": "https://svs.gsfc.nasa.gov/12853/", "result_type": "Produced Video", "release_date": "2019-01-07T17:15:00-05:00", "title": "TESS Rounds Up its First Planets, Snares Far-flung Supernovae", "description": "This visualization shows TESS's first field image and information about three early exoplanet detections. The locations of Pi Mensae c, LHS 3844b, and HD21749b appear, as well as information about the systems and animations of what the planets might look like. || TESS_First_Planets_Still_print.jpg (1024x576) [174.7 KB] || TESS_First_Planets_Still.jpg (3840x2160) [2.1 MB] || TESS_First_Planets_Still_searchweb.png (320x180) [92.2 KB] || TESS_First_Planets_Still_thm.png (80x40) [6.5 KB] || TESS_First_Planet_Locations-1080p.mov (1920x1080) [90.9 MB] || TESS_First_Planet_Locations-1080p.webm (1920x1080) [5.8 MB] || TESS_First_Planet_Locations-4k.mp4 (3840x2160) [114.1 MB] || TESS_First_Planet_Locations-4K.mov (3840x2160) [118.8 MB] || TESS_First_Planet_Locations_ProRes_3840x2160.mov (3840x2160) [3.4 GB] || TESS_First_Planet_Locations-4k.hwshow [490 bytes] || ", "hits": 144 }, { "id": 13112, "url": "https://svs.gsfc.nasa.gov/13112/", "result_type": "Animation", "release_date": "2018-12-03T10:00:00-05:00", "title": "Why Bennu?", "description": "The goal of the OSIRIS-REx mission is to collect a sample from an asteroid and bring it back to Earth. But just how did the OSIRIS-REx team choose Bennu from the over 500,000 known asteroids in the solar system? Watch this cartoon to find out!Music provided by Killer Tracks: \"Cheeky Chappy\" - James Patrick Kaleth & Ross Andrew McLean.Watch this video on the NASA Goddard YouTube channel. || WHYBENNUThumbnail.jpg (1920x1080) [462.1 KB] || WHYBENNUThumbnail_searchweb.png (320x180) [70.0 KB] || WHYBENNUThumbnail_thm.png (80x40) [6.9 KB] || 13112_WhyBennu_YouTubeHD.mp4 (1920x1080) [317.6 MB] || 13112_WhyBennu_Facebook.mp4 (1920x1080) [237.6 MB] || 13112_WhyBennu_MASTER.mov (1920x1080) [5.6 GB] || 13112_WhyBennu_YouTubeHD.webm (1920x1080) [22.3 MB] || WhyBennu_Captions.en_US.srt [4.0 KB] || WhyBennu_Captions.en_US.vtt [4.1 KB] || ", "hits": 33 }, { "id": 4644, "url": "https://svs.gsfc.nasa.gov/4644/", "result_type": "Visualization", "release_date": "2018-10-10T11:00:00-04:00", "title": "Pulsar Current Sheets - Bulk Particle Trajectories", "description": "This movie presents a basic tour around the simulation magnetic field including motion of the bulk particles. This version is generated with some simple reference objects for more general use. || PulsarParticles_grid_bulk_tour_inertial.HD1080i.01001_print.jpg (1024x576) [112.0 KB] || tour-glyph (1920x1080) [0 Item(s)] || PulsarParticles_grid_bulk_tour.HD1080i_p30.mp4 (1920x1080) [67.7 MB] || PulsarParticles_grid_bulk_tour.HD1080i_p30.webm (1920x1080) [5.3 MB] || tour-glyph (3840x2160) [0 Item(s)] || PulsarParticles_grid_bulk_tour_2160p30.mp4 (3840x2160) [129.1 MB] || PulsarParticles_grid_bulk_tour.HD1080i_p30.mp4.hwshow [208 bytes] || ", "hits": 111 }, { "id": 4645, "url": "https://svs.gsfc.nasa.gov/4645/", "result_type": "Visualization", "release_date": "2018-10-10T11:00:00-04:00", "title": "Pulsar Current Sheets - Electron flows", "description": "This movie presents a basic tour around the simulation magnetic field including motion of the high-energy electrons. This version is generated with some simple reference objects for more general use. || PulsarParticles_grid_electrons_tour_inertial.HD1080i.01001_print.jpg (1024x576) [100.3 KB] || tour-glyph (1920x1080) [0 Item(s)] || PulsarParticles_grid_electrons_tour.HD1080i_p30.mp4 (1920x1080) [78.4 MB] || PulsarParticles_grid_electrons_tour.HD1080i_p30.webm (1920x1080) [5.4 MB] || tour-glyph (3840x2160) [0 Item(s)] || PulsarParticles_grid_electrons_tour_2160p30.mp4 (3840x2160) [187.4 MB] || PulsarParticles_grid_electrons_tour.HD1080i_p30.mp4.hwshow [213 bytes] || ", "hits": 43 } ] }