{ "count": 633, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Radiation%22", "previous": null, "results": [ { "id": 31388, "url": "https://svs.gsfc.nasa.gov/31388/", "result_type": "Hyperwall Visual", "release_date": "2026-04-08T12:00:00-04:00", "title": "AVATAR: A Virtual Astronaut Tissue Analog Response", "description": "The AVATAR (A Virtual Astronaut Tissue Analog Response) investigation on Artemis II uses organ-on-a-chip devices, or organ chips, to study the effects of increased radiation and microgravity on human health.", "hits": 1158 }, { "id": 14993, "url": "https://svs.gsfc.nasa.gov/14993/", "result_type": "Produced Video", "release_date": "2026-04-08T11:00:00-04:00", "title": "Working on The Nancy Grace Roman Space Telescope - Long Exposure Timelapses", "description": "Building a telescope like the Nancy Grace Roman Space Telescope requires long hours focusing on small regions, repeated with precision day after day. These timelapses capture that slow and steady pace with long-exposure images stitched together to highlight the continuous work behind the scenes.In much the same way, the telescope itself will stitch together vast numbers of exposures into sweeping scientific surveys. By observing millions of stars over time, it will track changes across the cosmos capturing exploding stars, belching black holes, neutron star mergers, and more phenomena as they unfold. || ", "hits": 761 }, { "id": 31380, "url": "https://svs.gsfc.nasa.gov/31380/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "APEX-12 (Advanced Plant EXperiment-12) on the ISS", "description": "The findings of the APEX series of experiments offer insight into the effects of spaceflight on plant chromosomes, and how these findings could impact human health.", "hits": 377 }, { "id": 14988, "url": "https://svs.gsfc.nasa.gov/14988/", "result_type": "Produced Video", "release_date": "2026-03-16T14:00:00-04:00", "title": "Artemis II: Into the Path of Solar Eruptions", "description": "For the first time in half a century, four astronauts are leaving Earth’s protective magnetic field. They’ll enter a realm where massive solar eruptions can unleash more energy than a billion hydrogen bombs. The Artemis II crew will fly through a dangerous environment, but they’re not going it alone. On the voyage, the astronauts and their Orion capsule are outfitted with radiation trackers as ground teams monitor solar eruptions 24/7. Here’s how NASA and the National Oceanic and Atmospheric Administration (NOAA) are protecting explorers from the most powerful eruptions in the solar system. Learn more: https://science.nasa.gov/missions/artemis/artemis-2/to-protect-artemis-ii-astronauts-nasa-experts-keep-eyes-on-sun/ || ", "hits": 2500 }, { "id": 5622, "url": "https://svs.gsfc.nasa.gov/5622/", "result_type": "Visualization", "release_date": "2026-03-05T18:00:00-05:00", "title": "Artemis II: Sending Humans Beyond the Magnetosphere", "description": "Artemis II will be the first time in over 50 years that humans venture beyond Earth's protective magnetic shield, called the magnetosphere. This visualization captures the spacecraft's journey as the Orion spacecraft leaves the safety of the magnetosphere (shown here in green) and travels into open space, where it will encounter the solar wind streaming from the Sun.", "hits": 4323 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 500 }, { "id": 14956, "url": "https://svs.gsfc.nasa.gov/14956/", "result_type": "Produced Video", "release_date": "2026-01-26T16:00:00-05:00", "title": "Space Weather Effects Animations", "description": "Solar flares, coronal mass ejections, solar particle events, and the solar wind form the recipe for space weather that affects life on Earth and astronauts in space. A farmer stops their planting operations due to poor GPS signal for their autonomous tractor. A power grid manager changes the configuration of their network to ensure a blackout doesn’t occur due to voltage instability. A pilot switches to back-up communication equipment due to loss of high-frequency radio. A commercial internet company providing service to the military must change the orbit of their spacecraft to avoid a collision due to increased atmospheric drag.These are a few examples of the ways the Sun influences our everyday lives. This is what we define as space weather – the conditions of the space environment driven by the Sun and it’s impacts on objects in the solar system. Learn more about space weather: https://science.nasa.gov/space-weather-2/ || ", "hits": 554 }, { "id": 14930, "url": "https://svs.gsfc.nasa.gov/14930/", "result_type": "Infographic", "release_date": "2025-12-18T10:00:00-05:00", "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles", "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel", "hits": 147 }, { "id": 14885, "url": "https://svs.gsfc.nasa.gov/14885/", "result_type": "Produced Video", "release_date": "2025-09-12T06:00:00-04:00", "title": "NASA Interview Opportunity: Groundbreaking New NASA Mission Will Give Us The Most Detailed Look Yet At Our Solar System’s Shield", "description": "Scroll down page for associated cut b-roll and pre-recorded soundbites. || IMAP_banner.jpeg (1600x640) [185.0 KB] || IMAP_banner_print.jpg (1024x409) [110.6 KB] || IMAP_banner_searchweb.png (320x180) [73.1 KB] || IMAP_banner_thm.png (80x40) [6.7 KB] || ", "hits": 145 }, { "id": 14892, "url": "https://svs.gsfc.nasa.gov/14892/", "result_type": "Produced Video", "release_date": "2025-08-29T16:00:00-04:00", "title": "Solar Wind Animations", "description": "The Sun releases a constant stream of charged particles, called the solar wind. The solar wind originates in the outermost layer of the Sun’s atmosphere, the corona, when plasma is heated to a point that the Sun’s gravity can’t hold it down. When this plasma escapes – often reaching speeds of over one million miles per hour – it drags the Sun’s magnetic out across the solar system. When the solar wind encounters Earth, it is deflected by our planet's magnetic shield, causing most of the solar wind's energetic particles to flow around and beyond us. However, some of these high-energy particles can sneak past Earth’s natural magnetic defenses and produce hazardous conditions for satellites and astronauts, as well as power grids and infrastructure on Earth.Learn more about the solar wind: https://science.nasa.gov/sun/what-is-the-solar-wind/ || ", "hits": 896 }, { "id": 14888, "url": "https://svs.gsfc.nasa.gov/14888/", "result_type": "Produced Video", "release_date": "2025-08-22T16:00:00-04:00", "title": "IMAP Traveling to L1", "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. Additionally, IMAP will support real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. The IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space. At L1, it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way. || ", "hits": 282 }, { "id": 20406, "url": "https://svs.gsfc.nasa.gov/20406/", "result_type": "Animation", "release_date": "2025-08-22T09:00:00-04:00", "title": "The Heliosphere Within The Milky Way Galaxy", "description": "Our solar system is nestled inside the Milky Way galaxy, home to more than 100 billion stars. Stretching for millions of miles around the solar system is a protective bubble called the heliosphere. Created by particles and magnetic fields from the Sun, the heliosphere separates our solar system from the vast galaxy beyond — and much of its harsh space radiation that can be damaging to life on Earth. || ", "hits": 847 }, { "id": 20410, "url": "https://svs.gsfc.nasa.gov/20410/", "result_type": "Animation", "release_date": "2025-08-14T00:00:00-04:00", "title": "IMAP Beauty Passes", "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) 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.As a modern-day celestial cartographer, IMAP will also explore and chart the vast range of particles in interplanetary space, helping to investigate two of the most important overarching issues in heliophysics — the energization of charged particles from the Sun, and the interaction of the solar wind at its boundary with interstellar space. Additionally, IMAP will support real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. The IMAP spacecraft will be located at Lagrange Point 1, or L1. Lagrange points are positions in space where objects sent there tend to stay put. At L1, which is around 1 million miles from Earth towards the Sun, the gravitational pull of the Sun and Earth are balanced, allowing spacecraft to reduce fuel consumption needed to remain in position. At L1, IMAP will have a clear view of the heliosphere and will also be positioned to provide advanced warning of incoming solar storms headed to Earth. Learn more about IMAP.Below are conceptual animations highlighting the IMAP spacecraft. || ", "hits": 287 }, { "id": 14866, "url": "https://svs.gsfc.nasa.gov/14866/", "result_type": "Produced Video", "release_date": "2025-07-15T00:00:00-04:00", "title": "Cosmic Desktop & Phone Wallpapers", "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||", "hits": 30501 }, { "id": 20405, "url": "https://svs.gsfc.nasa.gov/20405/", "result_type": "Animation", "release_date": "2025-07-08T16:00:00-04:00", "title": "Carruthers Atmospheric Layers Animation", "description": "Earth’s atmosphere is divided into five main layers, differentiated by factors such as temperature, chemical composition, and air density. The troposphere is the lowest layer, extending from Earth's surface up to about 10 miles above it, and is where almost all weather phenomena occur. Above the troposphere is the stratosphere, which reaches up to around 31 miles. It contains the ozone layer, which absorbs harmful ultraviolet (UV) radiation from the Sun. Next is the mesosphere, which extends from about 31 to 53 miles above Earth. It is the coldest layer of the atmosphere, and it is where most meteors burn up upon entering. Above the mesosphere is the thermosphere, ranging from about 53 to 375 miles above Earth. Known as the upper atmosphere, this region contains the ionosphere, a region filled with charged particles that enable radio communications and where auroras often occur. The outermost layer is the exosphere, which gradually transitions into outer space. It is extremely thin and composed mainly of hydrogen and helium. Together, these layers form a protective shield that regulates Earth’s energy balance and helps sustain life. || ", "hits": 1772 }, { "id": 31348, "url": "https://svs.gsfc.nasa.gov/31348/", "result_type": "Hyperwall Visual", "release_date": "2025-05-21T18:59:59-04:00", "title": "Exploring the Cosmic Cliffs in 3D", "description": "In July 2022, NASA’s James Webb Space Telescope made history, revealing a breathtaking view of a region now nicknamed the Cosmic Cliffs. This glittering landscape, captured in incredible detail, is part of the nebula Gum 31 — a small piece of the vast Carina Nebula Complex", "hits": 198 }, { "id": 20403, "url": "https://svs.gsfc.nasa.gov/20403/", "result_type": "Animation", "release_date": "2025-05-14T09:00:00-04:00", "title": "Titan science results from James Webb Space Telescope: animation resource page", "description": "Push into JWST to Saturn and Titan. || JWST_Titan_Intro_Final_V001.00957_print.jpg (1024x576) [145.8 KB] || JWST_Titan_Intro_Final_V001.00957_searchweb.png (320x180) [78.0 KB] || JWST_Titan_Intro_Final_V001.00957_thm.png [5.5 KB] || JWST_Titan_Intro_Final_1080.mp4 (1920x1080) [72.8 MB] || JWST_Titan_Intro_Final_V001.mp4 (3840x2160) [38.4 MB] || JWST_Titan_Intro_Final_V001.mov (3840x2160) [6.8 GB] || ", "hits": 147 }, { "id": 14835, "url": "https://svs.gsfc.nasa.gov/14835/", "result_type": "Produced Video", "release_date": "2025-05-09T15:00:00-04:00", "title": "What Happened During the Biggest Geomagnetic Storm in Over 20 Years", "description": "On May 10, 2024, the first G5 or “severe” geomagnetic storm in over two decades hit Earth. The event did not cause any catastrophic damages, but it did produce surprising effects on Earth. The storm, which has been called the best-documented geomagnetic storm in history, spread auroras to unusually low latitudes and produced effects spanning from the ground to near-Earth space. Data captured during this historic event will be analyzed for years to come, revealing new lessons about the nature of geomagnetic storms and how best to weather them.Learn more:• What NASA Is Learning from the Biggest Geomagnetic Storm in 20 Years• How NASA Tracked the Most Intense Solar Storm in Decades || ", "hits": 525 }, { "id": 31390, "url": "https://svs.gsfc.nasa.gov/31390/", "result_type": "Hyperwall Visual", "release_date": "2025-04-08T12:00:00-04:00", "title": "Studying Biological Impacts of Space Radiation", "description": "Researchers developed human brain models in the lab and exposed them to simulated space radiation to study the impacts of space radiation and other spaceflight hazards on the human body.", "hits": 314 }, { "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": 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": 40532, "url": "https://svs.gsfc.nasa.gov/gallery/punch/", "result_type": "Gallery", "release_date": "2025-01-22T00:00:00-05:00", "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch", "hits": 225 }, { "id": 14756, "url": "https://svs.gsfc.nasa.gov/14756/", "result_type": "Produced Video", "release_date": "2025-01-13T16:00:00-05:00", "title": "50 Years of GOES", "description": "Music:“Realms of the Sky” by Frederik Helmut Wiedmann [GMR]; Icon Trailer Music; Universal Production Music“Exoplanet” by Jeff Penny [ASCAP]; Emperia Musicworks; Universal Production Music“Solo Trip” by Nicholas Smith [PRS]; Ideal.e; Universal Production Music“Reaching the Skies” by Ben Hicks [ASCAP]; Emperia Musicworks; Universal Production Music“Aetherion” by Lincoln Dale Davis [BMI]; Emperia Musicworks; Universal Production MusicThis video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by FootageFirm.com, Sebolla74/Pond5 and danr13/Pond5 are obtained through permission and may not be excised or remixed in other products. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html || YouTubeThumbnail_GOES50th_GOESandEarth.jpg (1920x1080) [1.2 MB] || YouTubeThumbnail_GOES50th_GOESandEarth.png (1280x720) [1.5 MB] || 14756_GOES_50th_FINAL_UHD.00500_print.jpg (1024x576) [167.0 KB] || 14756_GOES_50th_FINAL_UHD.00500_searchweb.png (320x180) [95.9 KB] || 14756_GOES_50th_FINAL_UHD.00500_thm.png [7.4 KB] || 14756_GOES_50th_FINAL_1080.mp4 (1920x1080) [178.6 MB] || 14756_GOES_50th_FINAL_UHD.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_UHD.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_1080.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_1080.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_UHD.webm (3840x2160) [20.5 MB] || 14756_GOES_50th_FINAL_UHD.mp4 (3840x2160) [684.3 MB] || ", "hits": 52 }, { "id": 14739, "url": "https://svs.gsfc.nasa.gov/14739/", "result_type": "Produced Video", "release_date": "2025-01-03T12:00:00-05:00", "title": "From the Moon, NASA’s LEXI Will Reveal Earth’s Magnetic Shield", "description": "NASA’s next mission to the Moon will carry an instrument called LEXI (the Lunar Environment Heliospheric X-ray Imager), which will provide the first-ever global view of the magnetic environment that shields Earth from solar radiation.From the surface of the Moon, LEXI will capture wide-field images of Earth's magnetic environment, or magnetosphere, in low-energy (or \"soft\") X-rays. LEXI will study changes in the magnetosphere and help us learn more about how it interacts with a stream of particles from the Sun called the solar wind, which can pose hazards for Artemis astronauts traveling to the Moon.Learn more about LEXI and its CLPS (Commercial Lunar Payload Services) flight to the Moon from Hyunju Connor, LEXI co-investigator at NASA’s Goddard Space Flight Center.More on LEXI: https://science.nasa.gov/science-research/heliophysics/nasas-lexi-will-provide-x-ray-vision-of-earths-magnetosphere/ || ", "hits": 198 }, { "id": 14722, "url": "https://svs.gsfc.nasa.gov/14722/", "result_type": "Produced Video", "release_date": "2024-12-06T15:00:00-05:00", "title": "NASA Interview Opportunity: NASA Spacecraft Days Away From Historic Close Approach to the Sun", "description": "Scroll down the page for associated cut b-roll for the live shots and pre-recorded soundbites.Find out more about NASA's Parker Solar Probe here! nasa.gov/parker || Screenshot_2024-12-06_at_2.24.02 PM.png (1546x606) [1.9 MB] || Screenshot_2024-12-06_at_2.24.02 PM_print.jpg (1024x401) [195.3 KB] || Screenshot_2024-12-06_at_2.24.02 PM_searchweb.png (320x180) [128.7 KB] || Screenshot_2024-12-06_at_2.24.02 PM_thm.png (80x40) [12.2 KB] || ", "hits": 143 }, { "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": 14715, "url": "https://svs.gsfc.nasa.gov/14715/", "result_type": "Produced Video", "release_date": "2024-11-18T00:00:00-05:00", "title": "COBE Celebrates 35th Launch Anniversary", "description": "Technicians work on the COBE (Cosmic Background Explorer) spacecraft in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission launched into an Earth orbit in 1989 to make an all-sky map of the cosmic microwave background, the oldest light in the universe. The conical silver shield protects the scientific instruments from direct radiation from the Sun and Earth, isolates them from radio-frequency interference from the spacecraft transmitters and terrestrial sources, and provides thermal isolation for a dewar containing liquid helium coolant.Credit: NASA/COBE Science Team || COBE_in_gfsc_clean_room_1.jpg (1629x1600) [552.8 KB] || ", "hits": 221 }, { "id": 31323, "url": "https://svs.gsfc.nasa.gov/31323/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GOES East vs GMAO – Global GeoColor Imagery", "description": "gmao-plot-all-colorbars-goes-east-vs-gmao_print.jpg (1024x576) [168.6 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao.png (3840x2160) [6.9 MB] || gmao-plot-all-colorbars-goes-east-vs-gmao_searchweb.png (320x180) [78.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_thm.png (80x40) [6.4 KB] || gmao-plot-all-colorbars-goes-east-vs-gmao_1080p30.mp4 (1920x1080) [12.9 MB] ||", "hits": 41 }, { "id": 31326, "url": "https://svs.gsfc.nasa.gov/31326/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GMAO South American Wild Fires", "description": "GMAO South American Wild Fires || 3840x2160_16x9_30p [0 Item(s)] || GMAO SOuth American Wild Fires ||", "hits": 19 }, { "id": 31320, "url": "https://svs.gsfc.nasa.gov/31320/", "result_type": "Hyperwall Visual", "release_date": "2024-10-30T00:00:00-04:00", "title": "Antarctic Ozone Hole Maximum, 1979-2024", "description": "Here, the globes show ozone data on the day that the minimum ozone concentration was reached over Antarctica, each year from 1979 and 2024. || annual_minimum_ozone_hole_area_yesColorbar_1080pa.00001_print.jpg (1024x576) [115.6 KB] || annual_minimum_ozone_hole_area_yesColorbar_1080pa.00001_searchweb.png (320x180) [54.4 KB] || annual_minimum_ozone_hole_area_yesColorbar_1080pa.00001_thm.png (80x40) [5.0 KB] || annual_minimum_ozone_hole_area_yesColorbar_1080pa.mp4 (1920x1080) [82.2 MB] || annual_minimum_ozone_hole_area_yesColorbar_1080pa.webm (1920x1080) [7.6 MB] || annual_minimum_ozone_hole_area_yesColorbar_4ka.mp4 (3840x2160) [228.9 MB] || antarctic-ozone-hole-maximum-1979-2024-4k-movie.hwshow [361 bytes] || antarctic-ozone-hole-maximum-1979-2024-1080p-movie.hwshow [370 bytes] || ", "hits": 231 }, { "id": 31319, "url": "https://svs.gsfc.nasa.gov/31319/", "result_type": "Hyperwall Visual", "release_date": "2024-10-23T00:00:00-04:00", "title": "2025 NASA Science Calendar", "description": "Images from the 2025 NASA Science Calendar", "hits": 121 }, { "id": 14685, "url": "https://svs.gsfc.nasa.gov/14685/", "result_type": "Produced Video", "release_date": "2024-10-15T15:00:00-04:00", "title": "What is Solar Maximum?", "description": "The Sun is stirring from its latest slumber. As sunspots and flares bubble from the Sun’s surface, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced on Tuesday, September 24, 2024, the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. || ", "hits": 321 }, { "id": 14683, "url": "https://svs.gsfc.nasa.gov/14683/", "result_type": "Produced Video", "release_date": "2024-10-15T13:30:00-04:00", "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period", "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ", "hits": 836 }, { "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": 14659, "url": "https://svs.gsfc.nasa.gov/14659/", "result_type": "Produced Video", "release_date": "2024-10-01T06:00:00-04:00", "title": "NASA Interview Opportunity: NASA’s Europa Clipper is Ready for Launch to Jupiter’s Moon Europa", "description": "Click here to find out more about Europa Clipper: go.nasa.gov/europaclipperClick here for the Europa Clipper PRESS KITKeep up-to-date on the lastest news about the mission blogs.nasa.gov/europaclipperScroll down page for LIVE SHOT B-ROLL PACKAGE and PRERECORDED INTERVIEWS || Europa_Clipper_Banner-english.png (1800x720) [974.7 KB] || Europa_Clipper_Banner-english_print.jpg (1024x409) [101.8 KB] || Europa_Clipper_Banner-english_searchweb.png (320x180) [77.5 KB] || Europa_Clipper_Banner-english_thm.png (80x40) [5.8 KB] || ", "hits": 161 }, { "id": 5378, "url": "https://svs.gsfc.nasa.gov/5378/", "result_type": "Visualization", "release_date": "2024-09-07T15:30:00-04:00", "title": "Map of the October 2, 2024 Annular Solar Eclipse", "description": "On Wednesday, October 2, 2024, the Moon passes in front of the Sun, casting its shadow across the Pacific Ocean. Observers on Rapa Nui (Easter Island) and in far southern Chile and Argentina are in the path of the annular eclipse. Hawai'i, parts of Antarctica, and the southern half of South America see a partial eclipse.", "hits": 247 }, { "id": 5373, "url": "https://svs.gsfc.nasa.gov/5373/", "result_type": "Visualization", "release_date": "2024-09-03T13:00:00-04:00", "title": "PREFIRE First Light", "description": "Visualization emphasizing two passes of PREFIRE over Greenland. Information about the rates of atmospheric emission can be derived from the change in emission at the intersection of the passes. || prefire_first_light_FINAL_2160p30.00450_print.jpg (1024x576) [224.8 KB] || prefire_first_light_FINAL_2160p30.00450_thm.png (80x40) [6.3 KB] || prefire_first_light_FINAL_2160p30.00450_searchweb.png (320x180) [78.7 KB] || prefire_first_light_FINAL [0 Item(s)] || prefire_first_light_FINAL_1080p30.mp4 (1920x1080) [47.2 MB] || prefire_first_light_FINAL_4K [0 Item(s)] || prefire_first_light_FINAL_2160p30.mp4 (3840x2160) [133.7 MB] || prefire_first_light_FINAL_2160p30.mp4.hwshow [199 bytes] || ", "hits": 81 }, { "id": 14628, "url": "https://svs.gsfc.nasa.gov/14628/", "result_type": "Produced Video", "release_date": "2024-08-28T11:30:00-04:00", "title": "Discovering Earth’s Third Global Energy Field", "description": "High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed – until now.In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission, and this is its story.To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/ || ", "hits": 374 }, { "id": 14657, "url": "https://svs.gsfc.nasa.gov/14657/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Journey into the Orion Nebula (Dome Version)", "description": "Journey into the Orion Nebula || PRINT.jpg (1920x1080) [130.9 KB] || THUMB.jpg (1920x1080) [130.9 KB] || SEARCH.jpg (320x180) [12.7 KB] || 4096x4096_1x1_24p [256.0 KB] || Journey_into_the_Orion_Nebula_Dome_Version.mp4 (1920x1080) [112.2 MB] || ", "hits": 107 }, { "id": 14658, "url": "https://svs.gsfc.nasa.gov/14658/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible Light || PRINT.jpg (1920x1080) [298.3 KB] || THUMB.jpg (1920x1080) [298.3 KB] || SEARCH.jpg (320x180) [27.0 KB] || Flight_Through_the_Orion_Nebula_in_Visible_Light_Dome_Version.mp4 (1920x1080) [225.5 MB] || 3840x3840_1x1_60p [0 Item(s)] || ", "hits": 169 }, { "id": 14661, "url": "https://svs.gsfc.nasa.gov/14661/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Infrared Light || PRINT.jpg (1920x1080) [206.5 KB] || THUMB.jpg (1920x1080) [206.5 KB] || SEARCH.jpg (320x180) [22.2 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.1 MB] || ", "hits": 75 }, { "id": 14662, "url": "https://svs.gsfc.nasa.gov/14662/", "result_type": "Produced Video", "release_date": "2024-08-19T00:00:00-04:00", "title": "Flight Through the Orion Nebula in Visible and Infrared Light (Dome Version)", "description": "Flight Through the Orion Nebula in Visible and Infrared Light || PRINT.jpg (1920x1080) [159.4 KB] || THUMB.jpg (1920x1080) [159.4 KB] || SEARCH.jpg (320x180) [18.5 KB] || 3840x3840_1x1_60p [1.0 MB] || Flight_Through_the_Orion_Nebula_in_Visible_and_Infrared_Light_Dome_Version.mp4 (1920x1080) [237.3 MB] || ", "hits": 156 }, { "id": 31302, "url": "https://svs.gsfc.nasa.gov/31302/", "result_type": "Hyperwall Visual", "release_date": "2024-08-02T00:00:00-04:00", "title": "NASA's Balloon Program", "description": "Scientific Balloon Program Infographic || nasa-scientific-balloon-facts_print.jpg (1024x576) [171.2 KB] || nasa-scientific-balloon-facts.png (3840x2160) [3.0 MB] || nasa-scientific-balloon-facts_searchweb.png (320x180) [58.8 KB] || nasa-scientific-balloon-facts_thm.png (80x40) [6.3 KB] || nasas-balloon-program-infographic.hwshow [280 bytes] || ", "hits": 255 }, { "id": 5238, "url": "https://svs.gsfc.nasa.gov/5238/", "result_type": "Visualization", "release_date": "2024-06-27T11:00:00-04:00", "title": "Our Active Ionosphere", "description": "In this view of Earth on October 7, 2019, just past sunset, GOLD observed an X-shaped structure in the equatorial ionization anomaly. || GOLD_O5S_20191007.00034_print.jpg (1024x576) [76.3 KB] || GOLD_O5S_20191007 [0 Item(s)] || GOLD_O5S_20191007_1080p4.mp4 (1920x1080) [1.8 MB] || ", "hits": 154 }, { "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": 31288, "url": "https://svs.gsfc.nasa.gov/31288/", "result_type": "Hyperwall Visual", "release_date": "2024-06-13T00:00:00-04:00", "title": "Webb, Chandra, Hubble, and Spitzer Together Explore Cassiopeia A", "description": "For the first time astronomers have combined data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the “Green Monster”, first discovered in Webb data in April 2023. The research has also uncovered new details about the explosion that created Cas A about 340 years ago, from Earth’s perspective.A new composite image contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). The outer parts of the image also include infrared data from NASA’s Spitzer Space Telescope (red, green and blue). The outline of the Green Monster can be seen by mousing over the image in the original feature, located here: chandra.cfa.harvard.edu/photo/2024/casa/.The Chandra data reveals hot gas, mostly from supernova debris from the destroyed star, including elements like silicon and iron. In the outer parts of Cas A the expanding blast wave is striking surrounding gas that was ejected by the star before the explosion. The X-rays are produced by energetic electrons spiraling around magnetic field lines in the blast wave. These electrons light up as thin arcs in the outer regions of Cas A, and in parts of the interior. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. The Hubble data shows stars in the field.Detailed analysis by the researchers found that filaments in the outer part of Cas A, from the blast wave, closely matched the X-ray properties of the Green Monster, including less iron and silicon than in the supernova debris. This interpretation is apparent from the color Chandra image, which shows that the colors inside the Green Monster’s outline best match with the colors of the blast wave rather than the debris with iron and silicon. The authors conclude that the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, supporting earlier suggestions from the Webb data alone.The debris from the explosion is seen by Chandra because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris.Read more here: chandra.cfa.harvard.edu/photo/2024/casa/. || 53453268481_e80cfca2d4_o.jpg (4200x3386) [7.1 MB] || 53453268481_e80cfca2d4_o_searchweb.png (320x180) [121.1 KB] || 53453268481_e80cfca2d4_o_thm.png (80x40) [15.9 KB] || webb-chandra-hubble-and-spitzer-all-explore-cassiopeia-a-composite-all-4.hwshow || ", "hits": 320 }, { "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": 31285, "url": "https://svs.gsfc.nasa.gov/31285/", "result_type": "Hyperwall Visual", "release_date": "2024-06-12T00:00:00-04:00", "title": "The Webb Space Telescope Studies the \"Cosmic Cliffs\" in NGC 3324", "description": "The seemingly three-dimensional “Cosmic Cliffs” showcases Webb’s capabilities to peer through obscuring dust and shed new light on how stars form. Webb reveals emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. This landscape of “mountains” and “valleys” is actually the edge of a nearby stellar nursery called NGC 3324 at the northwest corner of the Carina Nebula.So-called mountains — some towering about 7 light-years high — are speckled with glittering, young stars imaged in infrared light. A cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located above the area shown in this image. The blistering, ultraviolet radiation from these stars is sculpting the nebula’s wall by slowly eroding it away. Dramatic pillars rise above the glowing wall of gas, resisting this radiation. The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation.Objects in the earliest, rapid phases of star formation are difficult to capture, but Webb’s extreme sensitivity, spatial resolution and imaging capability can chronicle these elusive events. || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_print.jpg (1024x593) [318.7 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution.png (3840x2224) [10.2 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png (14575x8441) [113.7 MB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_searchweb.png (320x180) [116.3 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R-hw_resolution_thm.png (80x40) [13.5 KB] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png.dzi [179 bytes] || eta-carina-cliffs-webb-STScI-01G8GX1KMWX2XA4PK2EWM7KE3R.png_files [4.0 KB] || the-webb-space-telescope-studies-the-cosmic-cliffs-in-ngc-3324-still.hwshow [430 bytes] || ", "hits": 375 }, { "id": 14592, "url": "https://svs.gsfc.nasa.gov/14592/", "result_type": "Produced Video", "release_date": "2024-05-14T00:00:00-04:00", "title": "Largest Flare yet from Solar Cycle 25", "description": "On May 14, 2024, the Sun emitted a strong solar flare. This solar flare is the largest of Solar Cycle 25 and is classified as an X8.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.A solar flare is an intense burst of radiation, or light, on the Sun. Flares are our solar system’s most powerful explosive events. Light only takes about 8 minutes to travel from the Sun to Earth, so that’s how long it would take the energy from a flare to reach our planet. Stronger solar flares — those rated class M5 or above — can have impacts on technology that depends on Earth’s ionosphere (our electrically charged upper atmosphere), like high-frequency radio used for navigation and GPS.NASA’s Solar Dynamics Observatory (SDO) captured these images of the flare, which peaked at 12:51 p.m. ET on May 14. The X8.7 flare appears on the lower right edge of the Sun. (A small eruption appears afterward in the upper left.) SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. Different wavelengths are shown in this video to highlight different features of the flare.Music credit: “Ethereal Mirrorscape” from the album Reflections written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || X8pt7_flare_May_14_2024.00_00_40_22.Still001.jpg (3840x2160) [3.0 MB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_print.jpg (1024x576) [342.3 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_searchweb.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_web.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_thm.png (80x40) [6.1 KB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.webm (3840x2160) [20.4 MB] || 14592_SDO_X8pt7_flare_May_14_2024_Good_Outro.mp4 (3840x2160) [175.9 MB] || 14592_SDO_X8pt7_flare_May_14_2024_YouTube_Outro.mp4 (3840x2160) [673.0 MB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.mov (3840x2160) [4.2 GB] || ", "hits": 447 }, { "id": 14584, "url": "https://svs.gsfc.nasa.gov/14584/", "result_type": "Produced Video", "release_date": "2024-05-08T09:00:00-04:00", "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy", "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ", "hits": 132 }, { "id": 14524, "url": "https://svs.gsfc.nasa.gov/14524/", "result_type": "Infographic", "release_date": "2024-05-07T10:00:00-04:00", "title": "Primordial Black Holes", "description": "This artist's concept takes a fanciful approach to imagining small primordial black holes. In reality, such tiny black holes would have a difficult time forming the accretion disks that make them visible here.Credit: NASA's Goddard Space Flight Center || Primordial_Black_Hole_Still_1080.jpg (1920x1080) [275.1 KB] || Primordial_Black_Hole_Still_4k_print.jpg (1024x576) [51.1 KB] || Primordial_Black_Hole_Still_4k.jpg (3840x2160) [2.5 MB] || Primordial_Black_Hole_Still_4k.png (3840x2160) [7.3 MB] || Primordial_Black_Hole_Still_4k_searchweb.png (320x180) [61.5 KB] || Primordial_Black_Hole_Still_4k_thm.png (80x40) [5.6 KB] || ", "hits": 929 }, { "id": 5240, "url": "https://svs.gsfc.nasa.gov/5240/", "result_type": "Visualization", "release_date": "2024-04-22T00:00:00-04:00", "title": "Radio Signal Reflection & Refraction on a Simple Ionosphere Model", "description": "A simple animated plotting of radio wave refraction and reflection on a simplified ionosphere model, landscape format. || polar.propagation.basic.sample.1920x1080.png (1920x1080) [178.8 KB] || polar.propagation.basic.sample.1920x1080.1590_print.jpg (1024x576) [69.8 KB] || polar.propagation.basic.sample.1920x1080.1590_searchweb.png (320x180) [20.5 KB] || polar.propagation.basic.sample.1920x1080.1590_thm.png (80x40) [3.2 KB] || polar.propagation.basic.sample.1920x1080_p30.mp4 (1920x1080) [456.4 KB] || polar.propagation.basic.sample.1920x1080 (1920x1080) [0 Item(s)] || ", "hits": 197 }, { "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": 14537, "url": "https://svs.gsfc.nasa.gov/14537/", "result_type": "Produced Video", "release_date": "2024-02-29T12:00:00-05:00", "title": "One Month Out From The Total Solar Eclipse Live Shots", "description": "Included on this resource page are cut broll for the live shots and pre-recorded soundbites with Gina DiBraccio / Deputy Director of Heliophysics, NASA GSFC and Nicholeen Viall / NASA Mission Scientist for PUNCH. Also check out NASA's podcast nasa.gov/curiousuniverse. New episodes coming soon including one about the April 2024 solar eclipse. || Unknown.jpeg (1600x640) [86.5 KB] || Unknown_print.jpg (1024x409) [53.1 KB] || Unknown_searchweb.png (320x180) [35.3 KB] || Unknown_thm.png (80x40) [5.1 KB] || ", "hits": 29 }, { "id": 14494, "url": "https://svs.gsfc.nasa.gov/14494/", "result_type": "Produced Video", "release_date": "2024-01-08T10:00:00-05:00", "title": "Atmospheric Waves Experiment (AWE) Installation", "description": "On Saturday, Nov. 18, at 2 p.m. EST, installation of NASA’s Atmospheric Waves Experiment (AWE) was completed on the International Space Station.By remotely controlling the Canadarm2 robotic arm, engineers first extracted AWE from SpaceX’s Dragon cargo spacecraft a couple days after it arrived at the station on Nov. 11. Then, on Saturday, using the Canadarm2 robotic arm again, engineers completed AWE’s installation onto the EXPRESS Logistics Carrier 1, a platform designed to support external payloads mounted to the International Space Station.AWE is led by Ludger Scherliess at Utah State University in Logan, and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Utah State University’s Space Dynamics Laboratory built the AWE instrument and provides the mission operations center.To learn more visit science.nasa.gov/mission/awe || ", "hits": 92 }, { "id": 14493, "url": "https://svs.gsfc.nasa.gov/14493/", "result_type": "Produced Video", "release_date": "2024-01-05T09:55:00-05:00", "title": "Hubble’s Inside The Image: The Eagle Nebula", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of The Pillars of Creation.The Pillars of Creation in the Eagle Nebula, situated in the Serpens constellation, stand as celestial marvels. Composed of interstellar gas and dust, these towering structures captivate astronomers and stargazers alike. Shaped by the potent forces of stellar winds and radiation, the pillars, resembling cosmic sentinels, showcase vibrant hues. Functioning as crucibles for stellar birth, they facilitate the creation of new stars in a delicate dance of destruction and formation. The Pillars of Creation in the Eagle Nebula offer a captivating spectacle, inviting observers to contemplate the profound dynamics at play within our ever-evolving cosmic tapestry.In this video, Dr. Jennifer Wiseman explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationESA/Hubble (M. Kornmesser & L. L. Christensen) Light Echo AnimationNASA/ESA/Hubble - M. KornmesserMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Transitions” by Ben Niblett [PRS] and Jon Cotton [PRS] via Atmosphere Music Ltd [PRS] and Universal Production Music. || ", "hits": 110 }, { "id": 5144, "url": "https://svs.gsfc.nasa.gov/5144/", "result_type": "Interactive", "release_date": "2023-11-28T09:20:00-05:00", "title": "Fermi Gamma-ray Pulsar Catalog WorldWide Telescope Interactive", "description": "Before NASA’s Fermi Gamma-ray Space Telescope launched in 2008, only a handful of pulsars, including the Crab, Vela, and Geminga, were known to emit gamma-rays, the highest-energy form of light. Shown here are 294 gamma-ray pulsars detected by Fermi. Young pulsars, formed when massive stars explode, are the slowest rotators, typically spinning about 10 times a second. Paradoxically, their older siblings, called millisecond pulsars (MSPs), spin much faster, up to hundreds of times a second, thanks to the effects of a stream of matter pulled from a companion star. In spider systems, the companion is all but consumed. The most energetic spiders may fully evaporate their companions, leaving behind only an isolated MSP. Studying pulsars provides insights into the interplay of gravity, radiation, and magnetic fields with matter in the most extreme state we can observe directly.The WorldWide Telescope is a tool for showcasing astronomical data and knowledge. It’s not a physical telescope — it’s a suite of free and open source software and data sets that combine to create stunning scientific visualizations and stories. || ", "hits": 126 }, { "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": 14457, "url": "https://svs.gsfc.nasa.gov/14457/", "result_type": "Produced Video", "release_date": "2023-11-24T09:55:00-05:00", "title": "Hubble’s Inside The Image: M87 Jet", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the incredible image of galaxy M87 and its giant jet.M87, a massive elliptical galaxy in the Virgo Cluster, is famous for its prominent jet of high-energy particles and radiation that extends for thousands of light-years from its central supermassive black hole.In this video, Dr. Padi Boyd explains this breathtaking image and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationESA/Hubble (M. Kornmesser & L. L. Christensen) Black Hole AnimationsGoddard Space Flight CenterMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Cognition” by Lorenzo Ferrara [SIAE] via Hyperscore Productions [ASCAP] and Universal Production Music || ", "hits": 73 }, { "id": 14464, "url": "https://svs.gsfc.nasa.gov/14464/", "result_type": "Produced Video", "release_date": "2023-11-17T14:00:00-05:00", "title": "NASA Mission Catching AWEsome Waves in Earth’s Airglow", "description": "Attached to the International Space Station, NASA’s Atmospheric Waves Experiment, or AWE, is studying airglow, an ethereal radiance at the boundary between Earth’s atmosphere and space, to look for an invisible phenomenon called atmospheric gravity waves.Caused by winds rushing over mountain ranges or severe weather events such as hurricanes, thunderstorms, and tornadoes, atmospheric gravity waves can grow and reach all the way to space, where it interacts with space weather. Find out more about the AWE mission and how it will help us better understand the connection between weather on Earth and weather in space. || ", "hits": 137 }, { "id": 14442, "url": "https://svs.gsfc.nasa.gov/14442/", "result_type": "Animation", "release_date": "2023-10-24T11:00:00-04:00", "title": "STAQS Air Quality Conceptual Illustrations", "description": "While poor air quality affects everyone, there are pollution hotspots that can adversely affect those nearest. For example, neighborhoods located near highways and warehouses can be hotspots of nitrogen dioxide (NO2) and hazardous particles called PM2.5, which are more than 35 times smaller in diameter than a grain of sand.For other residents, such as those located downwind from major cities like Chicago and New York, ozone can be an issue. While ozone high in the atmosphere protects Earth from dangerous solar radiation, at the ground level it can cause respiratory diseases and drive smog. Ozone ‘brewed’ in cities can travel to rural communities.Ground-level ozone along with another hazardous pollutant – tiny particles called PM2.5 – lead to over 100,000 premature deaths each year in the U.S. || ", "hits": 23 }, { "id": 31253, "url": "https://svs.gsfc.nasa.gov/31253/", "result_type": "Hyperwall Visual", "release_date": "2023-10-18T00:00:00-04:00", "title": "Ozone Minimum Concentrations, 1979-2023", "description": "Here, the globes show ozone data on the day that the minimum ozone concentration was reached over Antarctica, each year from 1979 and 2023. || annual_ozone_min_v2_4k.00001_print.jpg (1024x574) [109.7 KB] || annual_ozone_min_v2_4k.00001_searchweb.png (320x180) [52.9 KB] || annual_ozone_min_v2_4k.00001_thm.png (80x40) [5.0 KB] || annual_ozone_min_v2_1080p30_2.mp4 (1920x1080) [7.5 MB] || annual_ozone_min_v2_1080p30_2.webm (1920x1080) [5.2 MB] || annual_ozone_min_v2 (4104x2304) [128.0 KB] || annual_ozone_min_v2_2160p30.mp4 (3840x2160) [18.2 MB] || ", "hits": 117 }, { "id": 5173, "url": "https://svs.gsfc.nasa.gov/5173/", "result_type": "Visualization", "release_date": "2023-10-10T00:00:00-04:00", "title": "Earth's Radiation Balance, 2000-2023", "description": "A plotted view of planetary heat uptake since the beginning of the CERES data record showing an oscillating, monthly mean (yellow) and twelve-month running average (red line). These data show how much energy is added (absorbed) by Earth during the CERES period. || planetary_heat_anomaly.1800_print.jpg (1024x576) [69.7 KB] || planetary_heat_anomaly.1800_searchweb.png (320x180) [21.2 KB] || planetary_heat_anomaly.1800_thm.png (80x40) [3.0 KB] || phu_2023 (3840x2160) [0 Item(s)] || planetary_heat_anomaly_2160p60.mp4 (3840x2160) [4.2 MB] || ", "hits": 317 }, { "id": 20383, "url": "https://svs.gsfc.nasa.gov/20383/", "result_type": "Animation", "release_date": "2023-10-05T14:35:00-04:00", "title": "Clouds 101", "description": "Climate Feedback || ClimateFeedback_Final_ProRes422LT.00100_print.jpg (1024x576) [200.6 KB] || ClimateFeedback_Final_ProRes422LT.00100_searchweb.png (320x180) [90.7 KB] || ClimateFeedback_Final_ProRes422LT.00100_web.png (320x180) [90.7 KB] || ClimateFeedback_Final_ProRes422LT.00100_thm.png (80x40) [6.1 KB] || ClimateFeedback_Final_1080p.mov (1920x1080) [504.7 MB] || ClimateFeedback_Final_web.mp4 (1920x1080) [58.3 MB] || ClimateFeedback_Final_ProRes422LT.mov (3840x2160) [1.4 GB] || ClimateFeedback_Final_ProRes422LT.webm (3840x2160) [13.5 MB] || ", "hits": 25 }, { "id": 31248, "url": "https://svs.gsfc.nasa.gov/31248/", "result_type": "Hyperwall Visual", "release_date": "2023-09-29T00:00:00-04:00", "title": "How Do Space Weather Effects & Solar Storms Affect Earth?", "description": "Technological and infrastructure affected by space weather events. || space-weather-effects_print.jpg (1024x953) [307.6 KB] || space-weather-effects.png (3480x3240) [8.3 MB] || space-weather-effects_searchweb.png (320x180) [77.3 KB] || space-weather-effects_thm.png (80x40) [6.2 KB] || how-do-space-weather-effects-solar-storms-affect-earth.hwshow [320 bytes] || ", "hits": 431 }, { "id": 5152, "url": "https://svs.gsfc.nasa.gov/5152/", "result_type": "Visualization", "release_date": "2023-09-26T17:00:00-04:00", "title": "Near surface Ozone (O3)", "description": "Near surface concentration of ozone (O3) estimated by NASA’s GEOS-CF model.", "hits": 87 }, { "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": 14358, "url": "https://svs.gsfc.nasa.gov/14358/", "result_type": "Produced Video", "release_date": "2023-08-17T12:55:00-04:00", "title": "Hubble Science: Gravitational Waves: Ripples In Space-Time", "description": "Gravitational waves are invisible ripples in the fabric of space-time. They are caused by some of the most violent and energetic events in the universe. These include colliding black holes, collapsing stellar cores, merging neutron stars or white dwarf stars, the wobble of neutron stars that are not perfect spheres and possibly even the remnants of gravitational radiation created by the birth of the universe.In this video, Dr. Padi Boyd explains gravitational waves and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSF. LIGO Interferometer IllustrationCredit: LIGO/T. Pyle Gravitational Wave AnimationCredit: NASA GSFC Conceptual Image Lab Kilonova AnimationCredit: NASA GSFC Conceptual Image Lab Ripples In Space Time AnimationCredit: LIGO/T. Pyle LIGO Hanford Aerial & InteriorCredit: Caltech/MIT/LIGO LabMusic Credit:“Alpha and Omega” by Laurent Parisi [SACEM] via KTSA Publishing [SACEM] and Universal Production Music“Cosmic Call” by Immersive Music (Via Shutterstock Music) || ", "hits": 248 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 45 }, { "id": 14328, "url": "https://svs.gsfc.nasa.gov/14328/", "result_type": "Produced Video", "release_date": "2023-07-28T09:55:00-04:00", "title": "Hubble Science: Multiwavelength Astronomy, The Big Picture", "description": "Until the 20th century, astronomers learned virtually all they knew about sources in the sky from only the tiny fraction of electromagnetic radiation that is visible to the eye. However, as astronomers have discovered how to collect radiation outside this part of the spectrum, they have been able to learn much more about the universe. Many objects reveal different aspects of their composition and behavior at different wavelengths. Other objects are completely invisible at one wavelength, yet are clearly visible at another.In this video, Dr. Padi Boyd explains the exciting future of multiwavelength astronomy and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Electromagnetic Spectrum GraphicCredit: NASA GSFC Conceptual Image Lab James Webb Space Telescope AnimationCredit: NASA GSFC Conceptual Image LabMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Cosmic Call” by Immersive Music (Via Shutterstock Music) || ", "hits": 41 }, { "id": 31234, "url": "https://svs.gsfc.nasa.gov/31234/", "result_type": "Hyperwall Visual", "release_date": "2023-07-22T00:00:00-04:00", "title": "Column Carbon Monoxide (CO) from Canada Wildfires", "description": "Column CO from Canada Wildfires || goes-fp-cobbna-nam-jun2023_00000_print.jpg (1024x576) [154.9 KB] || goes-fp-cobbna-nam-jun2023_00000_searchweb.png (320x180) [85.6 KB] || goes-fp-cobbna-nam-jun2023_00000_thm.png (80x40) [6.3 KB] || goes-fp-cobbna-nam-jun2023_1080p30.mp4 (1920x1080) [11.6 MB] || goes-fp-cobbna-nam-jun2023_1080p30.webm (1920x1080) [2.4 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || goes-fp-cobbna-nam-jun2023_2160p30.mp4 (3840x2160) [35.4 MB] || earth_observations_5x3.hwshow [570 bytes] || ", "hits": 151 }, { "id": 31223, "url": "https://svs.gsfc.nasa.gov/31223/", "result_type": "Hyperwall Visual", "release_date": "2023-04-03T00:00:00-04:00", "title": "A Daily View of Earth", "description": "A year-long true color global animation of MODIS corrected reflectance. || MODIS_combined_CorrRefl_TrueColor_2023-02-20_print.jpg (1024x576) [276.9 KB] || MODIS_combined_CorrRefl_TrueColor_2023-02-20_searchweb.png (320x180) [127.8 KB] || MODIS_combined_CorrRefl_TrueColor_2023-02-20_thm.png (80x40) [19.9 KB] || modis_truecolor_labeled_2022-2023_1080p10.webm (1920x1080) [8.7 MB] || MODIS_combined_CorrRefl_TrueColor_2023-02-20.tif (3840x2160) [14.0 MB] || modis_truecolor_labeled (3840x2160) [32.0 KB] || modis_truecolor_labeled_2022-2023_1080p10.mp4 (1920x1080) [176.9 MB] || modis_truecolor_labeled_2022-2023_2160p10.mp4 (3840x2160) [799.1 MB] || modis_truecolor_labeled_2022-2023_1080p10.hwshow [123 bytes] || modis_truecolor_labeled_2022-2023_2160p10.hwshow [123 bytes] || ", "hits": 203 }, { "id": 14317, "url": "https://svs.gsfc.nasa.gov/14317/", "result_type": "Produced Video", "release_date": "2023-03-28T13:50:00-04:00", "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst", "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ", "hits": 121 }, { "id": 40457, "url": "https://svs.gsfc.nasa.gov/gallery/cube-sats/", "result_type": "Gallery", "release_date": "2023-02-03T00:00:00-05:00", "title": "CubeSats", "description": "CubeSats are a class of nanosatellites that use a standard size and form factor. The standard CubeSat size uses a \"one unit\" or \"1U\" measuring 10x10x10 cms and is extendable to larger sizes; 1.5, 2, 3, 6, and even 12U. Originally developed in 1999 by California Polytechnic State University at San Luis Obispo (Cal Poly) and Stanford University to provide a platform for education and space exploration. The development of CubeSats has advanced into it's own industry with government, industry and academia collaborating for ever increasing capabilities. CubeSats now provide a cost effective platform for science investigations, new technology demonstrations and advanced mission concepts using constellations, swarms disaggregated systems.", "hits": 266 }, { "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": 14272, "url": "https://svs.gsfc.nasa.gov/14272/", "result_type": "Produced Video", "release_date": "2023-01-12T17:15:00-05:00", "title": "Hubble Finds Hungry Black Hole Twisting Captured Star Into Donut Shape", "description": "Black holes are gatherers, not hunters. They lie in wait until a hapless star wanders by. When the star gets close enough, the black hole's gravitational grasp violently rips it apart and sloppily devours its gasses while belching out intense radiation. Astronomers using NASA's Hubble Space Telescope have recorded a star's final moments in detail as it gets gobbled up by a black hole.For more information, visit https://nasa.gov/hubble. Music Credit“Solar Eclipse” by Alexander Ryder Mcnair [ASCAP] and Harry Gregson Williams [BMI] via Atmosphere Music Ltd. [PRS] and Universal Production Music. || ", "hits": 40 }, { "id": 14253, "url": "https://svs.gsfc.nasa.gov/14253/", "result_type": "Produced Video", "release_date": "2022-12-14T09:55:00-05:00", "title": "Hubble’s Inside The Image: Carina Nebula", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the past 32 years. One of them is the breathtaking image of the Carina Nebula.Hubble's view of the nebula shows star birth in a new level of detail. The fantasy-like landscape of the nebula is sculpted by the action of outflowing winds and scorching ultraviolet radiation from the monster stars that inhabit this inferno. In the process, these stars are shredding the surrounding material that is the last vestige of the giant cloud from which the stars were born.In this video, Dr. Ken Carpenter takes us on a journey through the Nebula, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSFMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Moving Headlines” by Immersive Music via Shutterstock Music || ", "hits": 84 }, { "id": 14228, "url": "https://svs.gsfc.nasa.gov/14228/", "result_type": "Produced Video", "release_date": "2022-10-31T11:00:00-04:00", "title": "Clouds 101", "description": "Complete transcript available. || Screen_Shot_2022-10-19_at_1.52.39_PM_print.jpg (1024x578) [66.1 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM.png (2844x1607) [3.9 MB] || Clouds_101_Lock.00001_searchweb.png (320x180) [34.8 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_searchweb.png (320x180) [66.0 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_web.png (320x180) [66.4 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_thm.png (80x40) [8.7 KB] || Clouds_101_audio_otter_ai.en_US.srt [9.6 KB] || Clouds_101_audio_otter_ai.en_US.vtt [9.6 KB] || Clouds_101_Lock.mp4 (1920x1080) [974.5 MB] || ", "hits": 34 }, { "id": 31203, "url": "https://svs.gsfc.nasa.gov/31203/", "result_type": "Hyperwall Visual", "release_date": "2022-10-28T00:00:00-04:00", "title": "Ozone Minimum Concentrations, 1979-2022", "description": "Here, the globes show ozone data on the day that the minimum ozone concentration was reached over Antarctica, each year from 1979 and 2022. || annual_ozone_min_v2_00000_print.jpg (1024x574) [107.9 KB] || annual_ozone_min_v2_00000_searchweb.png (320x180) [50.6 KB] || annual_ozone_min_v2_00000_thm.png (80x40) [5.0 KB] || annual_ozone_min_v2_1080p30_3.mp4 (1920x1080) [7.1 MB] || annual_ozone_min_v2_1080p30_3.webm (1920x1080) [4.7 MB] || annual_ozone_min_v2_2160p30_3.mp4 (3840x2160) [17.4 MB] || 3840x2160_16x9_30p (4104x2304) [128.0 KB] || ", "hits": 179 }, { "id": 14227, "url": "https://svs.gsfc.nasa.gov/14227/", "result_type": "Produced Video", "release_date": "2022-10-13T15:30:00-04:00", "title": "NASA Missions Detect Record-Breaking Burst", "description": "Swift’s X-Ray Telescope captured the afterglow of GRB 221009A about an hour after it was first detected. The bright rings form as a result of X-rays scattered by otherwise unobservable dust layers within our galaxy that lie in the direction of the burst. The dark vertical line is an artifact of the imaging system.Credit: NASA/Swift/A. Beardmore (University of Leicester) || XRT_image_crop.jpg (1084x1080) [629.3 KB] || XRT_image_crop_print.jpg (1024x1020) [657.0 KB] || XRT_image_crop_searchweb.png (320x180) [133.7 KB] || XRT_image_crop_web.png (320x318) [191.7 KB] || XRT_image_crop_thm.png (80x40) [26.1 KB] || ", "hits": 266 }, { "id": 31193, "url": "https://svs.gsfc.nasa.gov/31193/", "result_type": "Hyperwall Visual", "release_date": "2022-09-23T00:00:00-04:00", "title": "NASA's Biological & Physical Sciences Fleet", "description": "Current BPS Fleet || BPS_FLEET-2024-04-09_print.jpg (1024x576) [148.2 KB] || BPS_FLEET-2024-04-09.png (4000x2250) [5.1 MB] || BPS_FLEET-2024-04-09_searchweb.png (320x180) [84.1 KB] || BPS_FLEET-2024-04-09_thm.png (80x40) [6.5 KB] || nasas-biological-physical-sciences-fleet.hwshow [304 bytes] ||", "hits": 42 }, { "id": 14189, "url": "https://svs.gsfc.nasa.gov/14189/", "result_type": "Produced Video", "release_date": "2022-08-19T12:45:00-04:00", "title": "50th Anniversary of NASA's Copernicus Mission", "description": "Watch: This vintage segment on Copernicus comes from a 1973 edition of “The Science Report,” a long-running film series produced by the U.S. Information Agency. Credit: National Archives (306-SR-138B)Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || OAO-CopernicusFilm.02735_print.jpg (1024x768) [108.8 KB] || OAO-CopernicusFilm.mov (1440x1080) [2.1 GB] || OAO-CopernicusFilm.mp4 (1440x1080) [235.2 MB] || OAO-CopernicusFilm.webm (1440x1080) [24.5 MB] || OAO-CopernicusFilm.en_US.srt [3.8 KB] || OAO-CopernicusFilm.en_US.vtt [3.8 KB] || ", "hits": 96 }, { "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": 31186, "url": "https://svs.gsfc.nasa.gov/31186/", "result_type": "Hyperwall Visual", "release_date": "2022-08-09T00:00:00-04:00", "title": "Webb's Science Mission Begins: First Light Images", "description": "The Cartwheel Galaxy, a rare ring galaxy once shrouded in dust and mystery, has been unveiled by the imaging capabilities of NASA’s James Webb Space Telescope. The galaxy, which formed as a result of a collision between a large spiral galaxy and another smaller galaxy, not only retained a lot of its spiral character, but has also experienced massive changes throughout its structure. Webb’s high-precision instruments resolved individual stars and star-forming regions within the Cartwheel, and revealed the behavior of the black hole within its galactic center. These new details provide a renewed understanding of a galaxy in the midst of a slow transformation. || cartwheel_348_print.jpg (1024x576) [152.0 KB] || cartwheel_348.png (3840x2160) [9.1 MB] || webbs-science-mission-begins-first-light-images-cartwheel-galaxy.hwshow [314 bytes] || ", "hits": 94 }, { "id": 14134, "url": "https://svs.gsfc.nasa.gov/14134/", "result_type": "Produced Video", "release_date": "2022-05-02T13:00:00-04:00", "title": "NASA Simulation Suggests Some Volcanoes Might Warm Climate, Destroy Ozone Layer", "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Good Omens\" by Count Zero and Rohan Stevenson and \"Blue Moons\" by Gresby Race Nash of Universal Production Music || 14134_thumb.jpg (1920x1080) [450.5 KB] || volcanism_14134.00242_searchweb.png (320x180) [71.1 KB] || volcanism_14134.00242_thm.png (80x40) [5.5 KB] || volcanism_14134.mp4 (1920x1080) [377.7 MB] || volcanism_14134.webm (1920x1080) [27.0 MB] || volcanism_14134_caption.en_US.srt [4.9 KB] || volcanism_14134_caption.en_US.vtt [4.7 KB] || ", "hits": 99 }, { "id": 14131, "url": "https://svs.gsfc.nasa.gov/14131/", "result_type": "Produced Video", "release_date": "2022-04-12T00:00:00-04:00", "title": "Black Hole Week: Traveler and Friends GIFs", "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. The world of Black Hole Week is populated by a fun bunch of characters, including a little blue explorer (called the Traveler) and their cosmic friends.Below, you'll find tons of GIFs to download and use if you want to join in! || ", "hits": 119 }, { "id": 14130, "url": "https://svs.gsfc.nasa.gov/14130/", "result_type": "Produced Video", "release_date": "2022-04-07T14:00:00-04:00", "title": "Fermi Searches for Gravitational Waves From Monster Black Holes", "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ", "hits": 104 }, { "id": 20363, "url": "https://svs.gsfc.nasa.gov/20363/", "result_type": "Animation", "release_date": "2022-03-09T18:00:00-05:00", "title": "Animation: Heliosphere", "description": "The sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium. This forms a giant bubble around the sun and its planets, known as the heliosphere. NASA studies the heliosphere to better understand the fundamental physics of the space surrounding us - which, in turn, provides information regarding space throughout the rest of the universe, as well as regarding what makes planets habitable.The solar wind is a gas of charged particles known as plasma, a state of matter governed by its own set physical laws just as the more common solids, liquids, and gases are. As the solar wind sweeps out into space, it creates a space environment filled with radiation as well as magnetic fields that trail all the way back to the sun. This space environment is augmented by interstellar cosmic rays and occasional concentrated clouds of solar material that burst off the sun, known as coronal mass ejections.This complex environment surrounds the planets and ultimately has a crucial effect on the formation, evolution, and destiny of planetary systems. For one thing, our heliosphere acts as a giant shield, protecting the planets from galactic cosmic radiation. Earth is additionally shielded by its own magnetic field, the magnetosphere, which protects us not only from solar and cosmic particle radiation but also from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to such processes and have evolved differently.NASA's studies of the heliosphere include research into: how the solar wind behaves near Earth; what causes and sustains magnetic and electric fields around other planets; how does the heliosphere interact with the interstellar medium; what do the boundaries of the heliosphere look like; what is the origin and evolution of the solar wind and the interstellar cosmic rays; and what contributes to the habitability of exoplanets.The field is, therefore, intensely cross-disciplinary. Heliospheric research often works hand in hand with planetary scientists, astrophysicists, astrobiologists, and space weather researchers.NASA heliophysics missions contributing to heliospheric research are: the Advanced Composition Explorer; NOAA's Deep Space Climate Observatory, the Interstellar Boundary Explorer, the Solar Terrestrial Relations Observatory; Voyager, and Wind. || ", "hits": 503 }, { "id": 31175, "url": "https://svs.gsfc.nasa.gov/31175/", "result_type": "Hyperwall Visual", "release_date": "2022-02-10T00:00:00-05:00", "title": "New Climate for a better (?) tomorrow", "description": "Nadya Vinogradova Shiffer's COP26 presentation \"New climate for a better(?) tomorrow\" || COP26_nadya_vinogradova_shiffer_title_slide_3840x2160_print.jpg (1024x576) [195.6 KB] || COP26_nadya_vinogradova_shiffer_title_slide_3840x2160.png (3840x2160) [8.8 MB] || COP26_nadya_vinogradova_shiffer_title_slide_3840x2160_searchweb.png (320x180) [99.5 KB] || COP26_nadya_vinogradova_shiffer_title_slide_3840x2160_thm.png (80x40) [7.3 KB] || nadya_vinogradova_shiffer_2021_cop26_talk_720p30.webm (1280x720) [58.6 MB] || nadya_vinogradova_shiffer_2021_cop26_talk_720p30.mp4 (1280x720) [113.3 MB] || nadya_vinogradova_shiffer_2021_cop26_talk_1080p30.mp4 (1920x1080) [225.4 MB] || nadya_vinogradova_shiffer_2021_cop26_talk_2160p30.mp4 (1920x1080) [225.3 MB] || ", "hits": 18 }, { "id": 31172, "url": "https://svs.gsfc.nasa.gov/31172/", "result_type": "Hyperwall Visual", "release_date": "2022-01-13T00:00:00-05:00", "title": "First Light from Landsat 9", "description": "The first image collected by Landsat 9, on Oct. 31, 2021, shows remote coastal islands and inlets of the Kimberly region of Western Australia. In the top middle section of the image, the Mitchell River carves through sandstone, while to the left Bigge Island and the Coronation Islands stand out in the Indian Ocean. Australia is a major international partner of the Landsat 9 program, and operates one of the Landsat Ground Network stations in Alice Springs. || l9_australia_hyperwall_rgb_nolabels.jpg (5760x3240) [10.7 MB] || l9_australia_hyperwall_rgb_nolabels_thm.png (80x40) [7.7 KB] || l9_australia_hyperwall_rgb_nolabels_searchweb.png (320x180) [124.3 KB] || first-light-from-landsat-9-western-australia.hwshow [338 bytes] || ", "hits": 56 }, { "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": 4917, "url": "https://svs.gsfc.nasa.gov/4917/", "result_type": "Visualization", "release_date": "2021-11-29T11:00:00-05:00", "title": "ICON Snaps a Peek at the Ionospheric Dynamo", "description": "Visualization of ICON in Earth orbit, camera ahead of the spacecraft looking back on spacecraft and limb of Earth. Magenta curves are lines of Earth's geomagnetic field. Field-of-view (FOV) of MIGHTI imagers (green frustums) and the longitudinal wind vectors (green arrows) it measures are shown. MIGHTI imagers FOV eventually fades out. Vertical plasma speed (red arrows) is measured at the spacecraft. Magnetic field lines turn yellow as measurements of winds by MIGHT provide a connection to influence the plasma velocity measured at the spacecraft, redirecting the plasma flow from upward to downward. || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_print.jpg (1024x576) [135.0 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_searchweb.png (320x180) [79.4 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_thm.png (80x40) [5.7 KB] || ICONSyncView+x (1920x1080) [0 Item(s)] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4 (1920x1080) [36.4 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.webm (1920x1080) [5.1 MB] || ICONSyncView+x (3840x2160) [0 Item(s)] || ICONDataView.ICONSyncView+x.2160p30.mp4 (3840x2160) [114.3 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4.hwshow || ", "hits": 52 }, { "id": 40016, "url": "https://svs.gsfc.nasa.gov/gallery/climate-essentials/", "result_type": "Gallery", "release_date": "2021-11-10T00:00:00-05:00", "title": "Climate Essentials", "description": "This Climate Essentials multimedia gallery brings together the latest and most popular climate-related images, data visualizations and video features from Goddard Space Flight Center. For more multimedia resources on climate and other topics, search the Scientific Visualization Studio. To learn more about NASA's contribution to understanding Earth's climate, visit the Global Climate Change site.", "hits": 331 }, { "id": 13987, "url": "https://svs.gsfc.nasa.gov/13987/", "result_type": "Produced Video", "release_date": "2021-11-05T17:00:00-04:00", "title": "Landsat 9 First Light Images", "description": "The first data from Landsat 9, of Australia's Kimberley Coast in Western Australia, shows off the capabilities of the two instruments on the spacecraft. This image, from the Operational Land Imager 2, or OLI-2, was acquired on Oct. 31, 2021. Although similar in design to its predecessor Landsat 8, the improvements to Landsat 9 allow it to detect more subtle differences, especially over darker areas like water or the dense mangrove forests along the coast. || L9_Australia_20211031_p109r070-lrg.jpg (7621x7811) [24.2 MB] || L9_Australia_20211031_p109r070-lrg_searchweb.png (320x180) [106.1 KB] || L9_Australia_20211031_p109r070-lrg_thm.png (80x40) [7.1 KB] || L9_Australia_20211031_p109r070-lrg.tif (7621x7811) [340.6 MB] || ", "hits": 72 }, { "id": 13982, "url": "https://svs.gsfc.nasa.gov/13982/", "result_type": "Produced Video", "release_date": "2021-10-28T14:00:00-04:00", "title": "Active October Sun Emits X-class Flare", "description": "Brighter than a shimmering ghost, faster than the flick of a black cat’s tail, the Sun cast a spell in our direction, just in time for Halloween. This imagery captured by NASA’s Solar Dynamics Observatory covers a busy few days of activity between Oct. 25-28 that ended with a significant solar flare. From late afternoon Oct. 25 through mid-morning Oct. 26, an active region on the left limb of the Sun flickered with a series of small flares and petal-like eruptions of solar material. Meanwhile, the Sun was sporting more active regions at its lower center, directly facing Earth. On Oct. 28, the biggest of these released a significant flare, which peaked at 11:35 a.m. EDT. Credit: NASA/GSFC/SDOMusic: \"Immersion\" from Above and Below. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ActiveOctober_Still.jpg (1920x1080) [956.2 KB] || 13982_ActiveOctober_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || 13982_ActiveOctober_1080_Best.mp4 (1920x1080) [436.2 MB] || 13982_ActiveOctober_1080.mp4 (1920x1080) [188.1 MB] || 13982_ActiveOctober_1080_Best.webm (1920x1080) [19.7 MB] || 13982_ActiveOctober_SRT_Captions.en_US.srt [574 bytes] || 13982_ActiveOctober_SRT_Captions.en_US.vtt [587 bytes] || ", "hits": 74 }, { "id": 4929, "url": "https://svs.gsfc.nasa.gov/4929/", "result_type": "Visualization", "release_date": "2021-08-30T14:00:00-04:00", "title": "Comparing Atomic Oxygen Emission Observed by GOLD with Ionospheric Total Electron Content (TEC)", "description": "At 23:00UTC on November 19, 2018, we see the maxima of TEC values (red dots) closely aligned with the maxima of OI 135.6nm emission (black dots) || GOLD_TEC_anomalies_inset.00034_print.jpg (1024x576) [121.4 KB] || ", "hits": 33 }, { "id": 13886, "url": "https://svs.gsfc.nasa.gov/13886/", "result_type": "Produced Video", "release_date": "2021-07-26T11:00:00-04:00", "title": "NASA's Fermi Spots 'Fizzled' Burst from Collapsing Star", "description": "Astronomers combined data from NASA's Fermi Gamma-ray Space Telescope, other space missions, and ground-based observatories to reveal the origin of GRB 200826A, a brief but powerful burst of radiation. It’s the shortest burst known to be powered by a collapsing star – and almost didn’t happen at all. Credit: NASA's Goddard Space Flight CenterMusic: \"Inducing Waves\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Fizzled_GRB_Still.jpg (1920x1080) [740.9 KB] || Fizzled_GRB_Still_print.jpg (1024x576) [286.8 KB] || Fizzled_GRB_Still_searchweb.png (320x180) [72.2 KB] || Fizzled_GRB_Still_thm.png (80x40) [4.9 KB] || 13886_Fizzled_GRB_1080.mp4 (1920x1080) [147.2 MB] || 13886_Fizzled_GRB_1080_Best.mp4 (1920x1080) [453.2 MB] || 13886_Fizzled_GRB_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || 13886_Fizzled_GRB_1080.webm (1920x1080) [22.5 MB] || ", "hits": 110 }, { "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 } ] }