{ "count": 504, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Laboratory%22", "previous": null, "results": [ { "id": 31386, "url": "https://svs.gsfc.nasa.gov/31386/", "result_type": "Hyperwall Visual", "release_date": "2026-04-02T12:00:00-04:00", "title": "Space Station Research Informs New FDA-Approved Cancer Therapy", "description": "European Space Agency (ESA) astronaut Thomas Pesquet works with Protein Crystallization Facility hardware, used to study protein crystal growth research on the space station.", "hits": 1145 }, { "id": 31377, "url": "https://svs.gsfc.nasa.gov/31377/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "The Fluid Particles Experiment aboard the ISS", "description": "One of the experiments in the Microgravity Science Glovebox (MSG), observing how the particles cluster and form larger structures in microgravity.", "hits": 370 }, { "id": 14979, "url": "https://svs.gsfc.nasa.gov/14979/", "result_type": "Produced Video", "release_date": "2026-03-26T14:00:00-04:00", "title": "Early Testing of Aerogel and Silicon Detectors for TIGERISS", "description": "Nick Cannady, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, examines a block of silica aerogel in May 2025. Cannady uses the light weight material in detectors for the upcoming TIGERISS (Trans-Iron Galactic Element Recorder for the International Space Station) mission, which is designed to study high-speed charged particles called cosmic rays.Credit: NASA/Scott WiessingerAlt text: A man studies a transparent block of aerogel.Image description: A man with glasses wearing a blue checkered shirt examines a block of transparent material resting on a table. He is leaning and rests his right hand on the table. The block glows faintly blue. The table is gray with evenly spaced rows of holes. || Tigeriss-Aerogel__Nick_Cannady-3.jpg (6393x4718) [17.4 MB] || Tigeriss-AerogelNick_Cannady-3-small.jpg (3196x2359) [1.6 MB] || ", "hits": 221 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 720 }, { "id": 5625, "url": "https://svs.gsfc.nasa.gov/5625/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami", "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.", "hits": 552 }, { "id": 5626, "url": "https://svs.gsfc.nasa.gov/5626/", "result_type": "Visualization", "release_date": "2026-03-25T00:00:00-04:00", "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)", "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.", "hits": 193 }, { "id": 14991, "url": "https://svs.gsfc.nasa.gov/14991/", "result_type": "Produced Video", "release_date": "2026-03-20T12:00:00-04:00", "title": "Argonne Assembles, Tests Early ComPair-2 Hardware", "description": "Tim Cundiff, an engineering specialist at Argonne National Laboratory in Lemont, Illinois, monitors the automated wire bond of a ComPair-2 detector layer in April 2025. Image courtesy of Argonne National LaboratoryAlt text: A man in a lab uses a microscope.Image description: A man in a white clean suit, gloves, safety glasses, and a hairnet sits in front of a piece of machinery in a laboratory and peers into a microscope. Behind him is a long bench covered in scientific equipment and computers. In front of him, inside the machinery, are what look like two black treads that loop in and out of frame. || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9.jpg (2000x1125) [1.1 MB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_searchweb.png (320x180) [124.6 KB] || 34340D_0388_PSE_NASA_Goddard_Gamma-Ray_Tracker_Assembly_Process_WEB_16x9_thm.png (80x40) [27.3 KB] || ", "hits": 85 }, { "id": 5618, "url": "https://svs.gsfc.nasa.gov/5618/", "result_type": "Visualization", "release_date": "2026-03-04T11:00:00-05:00", "title": "SWOT River Volume Variations", "description": "SWOT River Volume Variations", "hits": 113 }, { "id": 5619, "url": "https://svs.gsfc.nasa.gov/5619/", "result_type": "Visualization", "release_date": "2026-03-04T11:00:00-05:00", "title": "SWOT River Volume Variations (rivers only)", "description": "No description available.", "hits": 140 }, { "id": 31347, "url": "https://svs.gsfc.nasa.gov/31347/", "result_type": "Hyperwall Visual", "release_date": "2026-03-03T18:59:59-05:00", "title": "Astronaut Don Pettit’s Photos from Space", "description": "hyperwall hwshows for photos from https://www.nasa.gov/gallery/astronaut-don-pettits-photos-from-space/", "hits": 1144 }, { "id": 14982, "url": "https://svs.gsfc.nasa.gov/14982/", "result_type": "Produced Video", "release_date": "2026-02-27T11:00:00-05:00", "title": "Deserts of Africa and the Middle East", "description": "Deserts of North Africa and the Middle East || Africa-Asia_HYPERWALL_PRINT.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_Thumb.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_Thumb.png (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_SearchWeb.jpg (1280x720) [1.9 MB] || Africa-Asia_HYPERWALL_1080.webm (1920x1080) [21.4 MB] || Africa-Asia_HYPERWALL_1080.mp4 (1920x1080) [222.6 MB] || Africa-Asia_HYPERWALL_6K.webm (5760x3240) [7.2 MB] || Africa-MiddleEast_HYPERWALL_4K.mp4 (3840x2160) [1.1 GB] || Africa-Asia_HYPERWALL_6K.mp4 (5760x3240) [5.0 GB] || ", "hits": 148 }, { "id": 14976, "url": "https://svs.gsfc.nasa.gov/14976/", "result_type": "Produced Video", "release_date": "2026-02-20T00:00:00-05:00", "title": "Fermi's 15-year View of the Gamma-Ray Sky", "description": "This image shows the entire sky as seen by Fermi's Large Area Telescope. Lighter colors indicate brighter gamma-ray sources. The map is centered on the center of our galaxy. The most prominent feature is the bright, diffuse glow running along the middle of the map, which marks the central plane of our Milky Way galaxy. The gamma rays there are mostly produced when energetic particles accelerated in the shock waves of supernova remnants collide with gas atoms and even light between the stars. Many of the star-like features above and below the Milky Way plane are distant galaxies powered by supermassive black holes. Many of the bright sources along the plane are pulsars. The image was constructed from 15 years of observations using front-converting gamma rays with energies greater than 1 GeV. Hammer projection with black background.Credit: NASA/DOE/Fermi LAT CollaborationAlt text: Fermi 15-year all-sky gamma-ray mapImage description: A colorful oval map sits in the middle of a black background. The oval is predominantly royal blue, striped with an irregular bright red, orange, and yellow band horizontally across the center, which shows the plane of our Milky Way galaxy. Smaller dots and splotches in red, orange, yellow, and white appear throughout the oval. || intens_ait_180m_gt1000_psf3_gal_0p1.png (3600x1800) [2.9 MB] || intens_ait_180m_gt1000_psf3_gal_0p1_print.jpg (1024x512) [290.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_searchweb.png (320x180) [74.2 KB] || intens_ait_180m_gt1000_psf3_gal_0p1_thm.png (80x40) [4.6 KB] || ", "hits": 188 }, { "id": 14924, "url": "https://svs.gsfc.nasa.gov/14924/", "result_type": "Produced Video", "release_date": "2026-02-18T09:55:00-05:00", "title": "\"Dark Galaxy\" Identified by Hubble", "description": "Master VersionHorizontal version. This is for use on any YouTube or non-YouTube platform where you want to display the video horizontally. || 14924_DARK_WIDE_PRINT.jpg (1920x1080) [759.2 KB] || 14924_DARK_WIDE_THUMB.jpg (1920x1080) [759.2 KB] || 14924_DARK_WIDE_SEARCH.jpg (320x180) [32.1 KB] || 14924_DARK_WIDE_MP4.mp4 (1920x1080) [239.9 MB] || 14924_DARK_WIDE_MP4.en_US.srt [3.6 KB] || 14924_DARK_WIDE_MP4.en_US.vtt [3.6 KB] || ", "hits": 288 }, { "id": 5607, "url": "https://svs.gsfc.nasa.gov/5607/", "result_type": "Visualization", "release_date": "2026-02-04T12:00:00-05:00", "title": "Record Temperature Years: 2025, 2024, and 2023", "description": "2025, 2024, and 2023 were the three warmest years in NASA's 146-year record. This visualization highlights these three years in the context of the full GISTEMP temperature record.", "hits": 1023 }, { "id": 5613, "url": "https://svs.gsfc.nasa.gov/5613/", "result_type": "Visualization", "release_date": "2026-02-04T00:00:00-05:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2025", "description": "The change in the distribution of land temperature anomalies over the years 1951 to 2025.", "hits": 478 }, { "id": 14957, "url": "https://svs.gsfc.nasa.gov/14957/", "result_type": "Produced Video", "release_date": "2026-01-27T10:00:00-05:00", "title": "IMAP Arrives at L1", "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) reached its destination at Lagrange point 1, or L1, approximately 1 million miles from Earth toward the Sun on Jan. 10, 2026.The mission’s operations team sent commands to the spacecraft on the morning of Jan. 9 to begin trajectory maneuvers to enter orbit at L1. Early on the morning of Jan. 10, the team confirmed the spacecraft had successfully entered its final L1 orbit, where it will stay for the duration of its mission.From L1, IMAP will explore and map the very boundaries of our heliosphere — the protective bubble created by the solar wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.Learn more about the milestone: https://science.nasa.gov/blogs/imap/2026/01/12/nasas-imap-mission-reaches-its-destination/ || ", "hits": 383 }, { "id": 5600, "url": "https://svs.gsfc.nasa.gov/5600/", "result_type": "Visualization", "release_date": "2026-01-26T15:00:00-05:00", "title": "23 Years of Sea Surface Temperature (SST) - 2002-2025", "description": "23 Years of Sea Surface Temperature (SST) - 2002-2025", "hits": 127 }, { "id": 5603, "url": "https://svs.gsfc.nasa.gov/5603/", "result_type": "Visualization", "release_date": "2026-01-14T13:00:00-05:00", "title": "Global Temperature Anomalies from 1880 to 2025", "description": "Global surface air temperatures from 1880-2025 as estimated from the GISTEMP analysis.", "hits": 1665 }, { "id": 14945, "url": "https://svs.gsfc.nasa.gov/14945/", "result_type": "Produced Video", "release_date": "2026-01-09T09:00:00-05:00", "title": "NASA’s Pandora Satellite to Explore Exoplanets and Stars", "description": "Artist’s concept of NASA’s Pandora mission, which will help scientists untangle the signals from exoplanets’ atmospheres — worlds beyond our solar system — and their stars.Credit: NASA's Goddard Space Flight CenterAlt text: The Pandora spacecraft with an exoplanet and two stars in the backgroundImage description: A metallic spacecraft takes up most of this image. Its body is made of a cylindrical telescope attached to a square base. Inside the telescope is the reflection of an orange star. A line of three solar panels extends from the right side of the spacecraft at a 45-degree angle. On the right side of the background is a large planet streaked with purple, pink, and white. To the left of the planet are two stars. One is small, yellow, and very close to the planet. The other is white and is almost totally eclipsed by the spacecraft. || Pandora_Graphic_No_Text.jpg (6000x3000) [3.5 MB] || Pandora_Graphic_No_Text.png (6000x3000) [22.7 MB] || ", "hits": 431 }, { "id": 14944, "url": "https://svs.gsfc.nasa.gov/14944/", "result_type": "Produced Video", "release_date": "2026-01-06T16:00:00-05:00", "title": "Black Aurora Rocket Instrument Testing at NASA Goddard", "description": "NASA’s Black and Diffuse Aurora Science Surveyor sounding rocket mission has completed its testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its launch. Sounding rocket missions like this one are suborbital rockets that fly scientific instruments into near-Earth space for short, approximately 15-minute flights. The mission will study so-called “black auroras,” dark patches and stripes that appear within an aurora. Previous research has hinted that they may be formed by electrons going upward escaping back out into space (rather than the absence of any electrons). The visible aurora is formed by an incoming downward stream of electrons. Scientists want to solve the puzzle as to why these patches and stripes form within the visible aurora. From Goddard, the instruments were delivered to Wallops Flight Facility, where they – along with the entire rocket payload – will be shipped to the Poker Flat Research Range in Fairbanks, Alaska, where the team aims to fly their rocket through black aurora. Onboard instruments will survey the electron populations as they fly through them to understand how and why these black patches and stripes form within the visible aurora. The mission is scheduled for launch no earlier than February 2026. || ", "hits": 63 }, { "id": 14666, "url": "https://svs.gsfc.nasa.gov/14666/", "result_type": "Produced Video", "release_date": "2025-11-13T12:00:00-05:00", "title": "ESCAPADE Launch Phase and Deployment Animations", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission will be carried into orbit on the second launch of Blue Origin’s New Glenn rocket. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 110 }, { "id": 14915, "url": "https://svs.gsfc.nasa.gov/14915/", "result_type": "Produced Video", "release_date": "2025-11-13T00:00:00-05:00", "title": "ESCAPADE Trajectory Animations", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, mission will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission is being carried into orbit on the second launch of Blue Origin’s New Glenn rocket (NG-2) and is scheduled to launch in November 2025 from Cape Canaveral, Florida. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin.Below are animations demonstrating the different phases of the mission's trajectory from traveling from Earth to Mars to implementing its science orbits around the Red Planet. || ", "hits": 564 }, { "id": 14918, "url": "https://svs.gsfc.nasa.gov/14918/", "result_type": "Produced Video", "release_date": "2025-11-11T00:00:00-05:00", "title": "ESCAPADE Prepares for Flight (2025)", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission is being carried into orbit on the second launch of Blue Origin’s New Glenn rocket (NG-2) and is scheduled to launch in November 2025 from Cape Canaveral, Florida. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 232 }, { "id": 14895, "url": "https://svs.gsfc.nasa.gov/14895/", "result_type": "Produced Video", "release_date": "2025-09-17T10:00:00-04:00", "title": "Mapping the Boundaries of Our Home in Space with NASA’s IMAP Mission", "description": "NASA’s new 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 solar system — and study how that boundary interacts with the local galactic neighborhood beyond.As a modern-day celestial cartographer, IMAP will 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 with interstellar space. Additionally, IMAP will support near real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. IMAP is launching no earlier than Sept. 23, 2025, aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Learn more about IMAP science: https://science.nasa.gov/missions/nasas-imap-mission-to-study-boundaries-of-our-home-in-space/Find out more about the IMAP mission: https://science.nasa.gov/mission/imap/ || ", "hits": 142 }, { "id": 5576, "url": "https://svs.gsfc.nasa.gov/5576/", "result_type": "Visualization", "release_date": "2025-08-26T09:00:00-04:00", "title": "TROPICS Eyes Hurricane Erin", "description": "This animation tracks Hurricane Erin from August 10 through August 20, 2025. || Erin_v07_L1C_ch12_2025-08-28_121639.02708_print.jpg (1024x576) [138.3 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_searchweb.png (320x180) [86.9 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.02708_thm.png (80x40) [6.2 KB] || Erin_v07_L1C_ch12_2025-08-28_121639.mp4 (1920x1080) [17.4 MB] || channel_12 (1920x1080) [855 Item(s)] ||", "hits": 53 }, { "id": 5558, "url": "https://svs.gsfc.nasa.gov/5558/", "result_type": "Animation", "release_date": "2025-07-11T12:01:00-04:00", "title": "Spread of the Palisades and Eaton Fires - January 2025", "description": "These visualizations show the spread of the Palisades and Eaton fires that occurred near Los Angeles, California in January 2025. This visualization highlights data from a fire detection and tracking approach (Chen et al., 2022) based on near-real time active fire detections from the VIIRS sensor on the Suomi-NPP and NOAA-20 satellites.", "hits": 977 }, { "id": 14861, "url": "https://svs.gsfc.nasa.gov/14861/", "result_type": "Produced Video", "release_date": "2025-07-07T10:00:00-04:00", "title": "NASA's Habitable Worlds Observatory Will Search For Life", "description": "No description available.", "hits": 398 }, { "id": 14792, "url": "https://svs.gsfc.nasa.gov/14792/", "result_type": "Produced Video", "release_date": "2025-05-27T20:57:00-04:00", "title": "Astrophysics Missions Vertical Video", "description": "This page collects vertical videos related to specific Astrophysics missions and their hardware or capabilities.", "hits": 106 }, { "id": 5524, "url": "https://svs.gsfc.nasa.gov/5524/", "result_type": "Interactive", "release_date": "2025-05-22T08:00:59-04:00", "title": "\"Snap It!\" Solar Eclipse Photography Game", "description": "The Traveler needs your help! They have come to Earth to study an event we call a total solar eclipse. Can you help the Traveler snap photos of an eclipse?", "hits": 48 }, { "id": 14834, "url": "https://svs.gsfc.nasa.gov/14834/", "result_type": "Produced Video", "release_date": "2025-05-12T00:00:00-04:00", "title": "Cosmic Dawn: The Untold Story of the James Webb Space Telescope", "description": "For more than three decades, NASA and an international team of scientists and engineers pushed the limits of technology, innovation, and perseverance to build and launch the James Webb Space Telescope, the most powerful space observatory ever created. Cosmic Dawn brings audiences behind the scenes with the Webb film crew, and never-before-heard testimonies revealing the real story of how this telescope overcame all odds. ||", "hits": 304 }, { "id": 31343, "url": "https://svs.gsfc.nasa.gov/31343/", "result_type": "Animation", "release_date": "2025-05-01T04:00:00-04:00", "title": "Curiosity Mars rover panoramas", "description": "Animated zoom and pans of two Curiosity Mars rover panoramas from February 7, 2025 and March 9, 2025.", "hits": 814 }, { "id": 14829, "url": "https://svs.gsfc.nasa.gov/14829/", "result_type": "Produced Video", "release_date": "2025-04-25T10:00:00-04:00", "title": "TRACERS Thermal Vacuum Testing at Millennium Space Systems", "description": "NASA’s Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, or TRACERS, is embarking on its integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission. The TRACERS mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Below are clips of Millennium Space Systems’ team members conducting Thermal Vacuum (TVAC) testing at the Boeing Space Systems Laboratory in El Segundo, California.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 130 }, { "id": 14824, "url": "https://svs.gsfc.nasa.gov/14824/", "result_type": "Produced Video", "release_date": "2025-04-24T09:55:00-04:00", "title": "Hubble’s Highlights from its 35th Year in Orbit", "description": "The Hubble Space Telescope celebrated its 35th year in orbit by premiering four stunning new Hubble images.From the planet Mars, to spectacular star forming regions, to a magnificent neighboring galaxy, these new images are the best birthday present anyone could ask for!Even after all these years, Hubble continues to uncover the mysteries of the universe. These are a few science achievements from Hubble’s latest year in orbit.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerVideo Credit:Images/Visualizations: NASA, ESA, STScIFU Orionis Disk Illustration from NASA Jet Propulsion Laboratory via Caltech/T. Pyle (IPAC)Music Credit:“Quartet for Strings in C Major Emperor\" by Franz Joseph Haydn [DP] and Jim Long [ASCAP], via Just Classics [ASCAP] and Universal Production Music. || ", "hits": 95 }, { "id": 14815, "url": "https://svs.gsfc.nasa.gov/14815/", "result_type": "B-Roll", "release_date": "2025-04-09T14:00:00-04:00", "title": "IMAP Testing and Integration at NASA's Goddard Space Flight Center", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which its instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "hits": 35 }, { "id": 14814, "url": "https://svs.gsfc.nasa.gov/14814/", "result_type": "B-Roll", "release_date": "2025-04-09T08:00:00-04:00", "title": "IMAP Testing and Integration at Johns Hopkins Applied Physics Lab", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "hits": 80 }, { "id": 14808, "url": "https://svs.gsfc.nasa.gov/14808/", "result_type": "Produced Video", "release_date": "2025-03-24T15:00:00-04:00", "title": "Largest Organics Yet Discovered on Mars", "description": "Researchers analyzing pulverized rock onboard NASA’s Curiosity rover have found the largest organic compounds on the Red Planet to date.Complete transcript available.Universal Production Music: “Labyrinth of Discovery” by Emma Zarobyan [SOCAN]Watch this video on the NASA Goddard YouTube channel. || Mars_Large_Organics_Thumbnail_V3_print.jpg (1024x576) [234.9 KB] || Mars_Large_Organics_Thumbnail_V3.jpg (1280x720) [810.1 KB] || Mars_Large_Organics_Thumbnail_V3.png (1280x720) [1.3 MB] || Mars_Large_Organics_Thumbnail_V3_searchweb.png (320x180) [103.3 KB] || Mars_Large_Organics_Thumbnail_V3_thm.png [7.1 KB] || Mars_Large_Organics_Thumbnail_V3_web.png (320x180) [103.3 KB] || 14808_Mars_Large_Organics_720.mp4 (1280x720) [23.4 MB] || 14808_Mars_Large_Organics_1080.mp4 (1920x1080) [131.1 MB] || MarsLargeOrganicsCaptions.en_US.srt [2.1 KB] || MarsLargeOrganicsCaptions.en_US.vtt [2.0 KB] || 14808_Mars_Large_Organics_4K.mp4 (3840x2160) [1.6 GB] || 14808_Mars_Large_Organics_ProRes.mov (3840x2160) [9.7 GB] || ", "hits": 461 }, { "id": 14786, "url": "https://svs.gsfc.nasa.gov/14786/", "result_type": "Animation", "release_date": "2025-02-20T00:00:00-05:00", "title": "Swift Spacecraft Animations: 2025", "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || ", "hits": 90 }, { "id": 14432, "url": "https://svs.gsfc.nasa.gov/14432/", "result_type": "Produced Video", "release_date": "2025-01-31T15:00:00-05:00", "title": "How NASA Sees the Air We Breathe", "description": "NASA and NOAA, among other agencies, worked together this summer through the STAQS and AEROMMA missions to calibrate and validate NASA’s new TEMPO satellite. The satellite and missions combined aim to not only better measure air quality, and the major pollutants that impact it, but also to improve air quality, from street to stratosphere. This effort was documented during the August 2023 campaign leg, which took place over the Chicago region. Complete transcript available.Universal Music Production: Night Swimmer Instrumental [PRS], Living In The Light Instrumental [PRS], Nanofiber Instrumental [PRS], Results Take Time Instrumental [PRS], Spin Foam Instrumental [PRS], and Mindful Instrumental [PRS]. \u2028Additional images courtesy of Rafael Méndez Peña Additional images courtesy of Community Research On Climate and Urban Science Department of Energy Integrated Urban Field LaboratoryThis video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by ASF is 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 || STAQS_thumbnail_FINAL.jpg (1280x720) [648.9 KB] || STAQS_thumbnail_FINAL_print.jpg (1024x576) [461.5 KB] || STAQS_thumbnail_FINAL_web.png (320x180) [91.7 KB] || STAQS_Locked_Final.webm (1920x1080) [71.4 MB] || STAQS_transcript_en_US.en_US.srt [11.2 KB] || STAQS_transcript_en_US.en_US.vtt [11.2 KB] || STAQS_Locked_Final.mp4 (1920x1080) [1.3 GB] || ", "hits": 28 }, { "id": 14772, "url": "https://svs.gsfc.nasa.gov/14772/", "result_type": "B-Roll", "release_date": "2025-01-29T11:00:00-05:00", "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics", "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ", "hits": 489 }, { "id": 14757, "url": "https://svs.gsfc.nasa.gov/14757/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman Space Telescope's Coronagraph Instrument Integration into the Instrument Carrier", "description": "The Coronagraph, one of two science instruments, finds it home in NASA's Nancy Grace Roman Telescope Instrument Carrier.Designed and built by NASA’s Jet Propulsion Laboratory, the Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars (exoplanets). Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet. The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star. || ", "hits": 64 }, { "id": 14758, "url": "https://svs.gsfc.nasa.gov/14758/", "result_type": "Produced Video", "release_date": "2025-01-21T00:00:00-05:00", "title": "Roman Space Telescope's Coronagraph Instrument Arrives to Goddard Space Flight Center", "description": "The first of two scientific instruments for NASA's Nancy Grace Roman Space Telescope has arrived to Goddard Space Flight Center.Designed and built by NASA’s Jet Propulsion Laboratory, the Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars (exoplanets). Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet.The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star. || ", "hits": 58 }, { "id": 14754, "url": "https://svs.gsfc.nasa.gov/14754/", "result_type": "Produced Video", "release_date": "2025-01-16T10:14:00-05:00", "title": "NASA’s Pandora Mission Closer To Probing Alien Atmospheres", "description": "Basic overview of NASA's Pandora mission, which will revolutionize the study of exoplanet atmospheres.", "hits": 94 }, { "id": 14749, "url": "https://svs.gsfc.nasa.gov/14749/", "result_type": "Produced Video", "release_date": "2025-01-14T10:00:00-05:00", "title": "OpenUniverse: Simulated Universe Views for Roman", "description": "This video begins with a tiny one-square-degree portion of the full OpenUniverse simulation area (about 70 square degrees, equivalent to an area of sky covered by more than 300 full moons). It spirals in toward a particularly galaxy-dense region, zooming by a factor of 75. This simulation showcases the cosmos as NASA’s Nancy Grace Roman Space Telescope could see it, allowing scientists to preview the next generation of cosmic discovery now. Roman’s real future surveys will enable a deep dive into the universe with highly resolved imaging, as demonstrated in this video.Credit: NASA’s Goddard Space Flight Center and M. Troxel || OpenUniverseFullZoom_4k_Best.00001_print.jpg (1024x576) [111.9 KB] || OpenUniverseFullZoom_4k_Good.mp4 (3840x2160) [101.9 MB] || OpenUniverseFullZoom_4k_Best.mp4 (3840x2160) [249.3 MB] || OpenUniverseFullZoom_ProRes_3840x2160_30.mov (3840x2160) [2.9 GB] || ", "hits": 134 }, { "id": 5376, "url": "https://svs.gsfc.nasa.gov/5376/", "result_type": "Visualization", "release_date": "2025-01-10T11:00:00-05:00", "title": "Record Temperature Years: 2024, 2023, and 2016", "description": "A visualization of global temperature anomalies highlighting the record years of 2024, 2023, and 2016. The visualizations morphs between a data grid showing monthly temperatures and a bar chart of annual temperatures. This version is labeled in English and temperatures are in Celsius. || GISTEMP_Records_English_C.00001_print.jpg (1024x1024) [402.0 KB] || GISTEMP_Records_English_C.00001_searchweb.png (320x180) [105.1 KB] || GISTEMP_Records_English_C.00001_thm.png [7.1 KB] || GISTEMP_Records_English_C.mp4 (2160x2160) [19.3 MB] || climate_compiled_GISTEMP.hwshow || ", "hits": 344 }, { "id": 5450, "url": "https://svs.gsfc.nasa.gov/5450/", "result_type": "Visualization", "release_date": "2025-01-10T11:00:00-05:00", "title": "Global Temperature Anomalies from 1880 to 2024", "description": "This color-coded map in Robinson projection displays a progression of changing global surface temperature anomalies. Normal temperatures are shown in white. Higher than normal temperatures are shown in red and lower than normal temperatures are shown in blue. Normal temperatures are calculated over the 30 year baseline period 1951-1980. The maps are averages over a running 24 month window. The final frame represents global temperature anomalies in 2024.", "hits": 1903 }, { "id": 5451, "url": "https://svs.gsfc.nasa.gov/5451/", "result_type": "Visualization", "release_date": "2025-01-10T11:00:00-05:00", "title": "Zonal Climate Anomalies 1880-2024", "description": "A visualization of zonal temperature anomalies. The latitude zones are 90N-64N, 64N-44N, 44N-24N, 24N-EQU, EQU-24S, 24S-44S, 44S-64S, 64S-90S. The anomalies are calculated relative to a baseline period of 1951-1980. This version is in Celsius, an alternate version in Fahrenheit is also available. || GISTEMP_Zonal_1880-2024_C_2160p30.00850_print.jpg (1024x576) [52.4 KB] || GISTEMP_Zonal_1880-2024_C_2160p30.00850_searchweb.png (320x180) [17.8 KB] || GISTEMP_Zonal_1880-2024_C_2160p30.00850_thm.png [2.4 KB] || GISTEMP_Zonal_1880-2024_C_2160p30.mp4 (3840x2160) [20.3 MB] || ", "hits": 160 }, { "id": 5452, "url": "https://svs.gsfc.nasa.gov/5452/", "result_type": "Visualization", "release_date": "2025-01-10T11:00:00-05:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1964-2024", "description": "The change in the distribution of land temperature anomalies over the years 1964 to 2024. This version is in Celsius, a Fahrenheit version is also available. || GISTEMPDist_2024_C.00850_print.jpg (1024x576) [45.7 KB] || GISTEMPDist_2024_C.00850_searchweb.png (320x180) [13.7 KB] || GISTEMPDist_2024_C.00850_thm.png [2.1 KB] || GISTEMPDist_2024_C.mp4 (3840x2160) [21.1 MB] ||", "hits": 264 }, { "id": 14680, "url": "https://svs.gsfc.nasa.gov/14680/", "result_type": "Produced Video", "release_date": "2025-01-09T00:00:00-05:00", "title": "Astronauts Prepare for NICER Repair Training", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague participated in a training exercise at the NBL (Neutral Buoyancy Laboratory) at NASA’s Johnson Space Center in Houston. They were rehearsing activities related to repairing NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.Before any spacewalk, astronauts practice and refine procedures in the NBL to simulate — as closely as possible on Earth — the conditions under which they’ll complete the task in space.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s X-ray measurements during orbital daytime.The NICER team developed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 62 }, { "id": 14678, "url": "https://svs.gsfc.nasa.gov/14678/", "result_type": "Produced Video", "release_date": "2025-01-07T00:00:00-05:00", "title": "Astronauts Practice NICER Repair", "description": "On May 16, 2024, astronauts Don Pettit and Nick Hague practiced a repair for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station. The training exercise took place in the (NBL) Neutral Buoyancy Laboratory at NASA’s Johnson Space Center in Houston.Before any spacewalk, astronauts rehearse activities in the NBL to simulate — as much as possible — the conditions under which they’ll complete the task in space.In May 2023, NICER developed a “light leak,” where unwanted sunlight began entering the instrument. The damage allows sunlight to reach the detectors during the station’s daytime, saturating sensors and interfering with NICER’s X-ray measurements. The damage does not impact nighttime observations.The NICER team developed a plan to cover the largest areas of damage using five patches, each shaped like a piece of pie, to be inserted into the instrument’s sunshades and locked in place. || ", "hits": 74 }, { "id": 14741, "url": "https://svs.gsfc.nasa.gov/14741/", "result_type": "Produced Video", "release_date": "2024-12-27T13:00:00-05:00", "title": "Parker Solar Probe: Humanity’s Closest Encounter with the Sun", "description": "Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.Breaking its previous record by flying just 3.8 million miles above the surface of the Sun, NASA’s Parker Solar Probe hurtled through the solar atmosphere at a blazing 430,000 miles per hour — faster than any human-made object has ever moved. A beacon tone received in the late evening hours of Dec. 26 confirmed the spacecraft had made it through the encounter safely and is operating normally.This pass, the first of more to come at this distance, allows the spacecraft to conduct unrivaled scientific measurements with the potential to change our understanding of the Sun. || ", "hits": 593 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 293 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 550 }, { "id": 5389, "url": "https://svs.gsfc.nasa.gov/5389/", "result_type": "Visualization", "release_date": "2024-11-14T00:00:00-05:00", "title": "Tracking methane with EMIT and AVIRIS-3", "description": "Methane plumes can now be detected using the airborne AVIRIS-3 spectrometer in addition to EMIT on the International Space Station.", "hits": 174 }, { "id": 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": 114 }, { "id": 5405, "url": "https://svs.gsfc.nasa.gov/5405/", "result_type": "Visualization", "release_date": "2024-10-11T00:00:00-04:00", "title": "TROPICS Monitors Milton", "description": "Hurricane Milton transversing through the Gulf of Mexico, starting October 5, 2024 through October 9, 2024 when it made landfall along the western Florida coast. || Milton_v02_2024-10-11_1120.02500_print.jpg (1024x576) [132.9 KB] || Milton_v02_2024-10-11_1120.02500_searchweb.png (320x180) [85.7 KB] || Milton_v02_2024-10-11_1120.02500_thm.png (80x40) [6.6 KB] || Milton_v02_2024-10-11_1120.mp4 (1920x1080) [12.4 MB] || 1920x1080_16x9_30p [0 Item(s)] || Milton_v02_2024-10-11_1120.webm (1920x1080) [2.9 MB] || tropics-monitors-milton.hwshow || ", "hits": 23 }, { "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": 159 }, { "id": 5390, "url": "https://svs.gsfc.nasa.gov/5390/", "result_type": "Visualization", "release_date": "2024-09-27T00:00:00-04:00", "title": "TROPICS Tracks Hurricane Helene", "description": "This data visualization shows TROPICS tracking Hurricane Helene throughout most of its life cycle. On September 27th Helene rapidly intensified to a category 4 hurricane before making landfall on the Florida bend. Although weakened after landfall it was still a category 1 hurricane as it hit Georgia and a Tropical Strom over western North Carolina. || Helene0927_v93_2024-10-01_1139.02900_print.jpg (1024x576) [125.4 KB] || Helene0927_v93_2024-10-01_1139.02900_searchweb.png (320x180) [81.2 KB] || Helene0927_v93_2024-10-01_1139.02900_thm.png (80x40) [6.2 KB] || Helene0927_v93_2024-10-01_1139.mp4 (1920x1080) [17.4 MB] || final [0 Item(s)] || ", "hits": 100 }, { "id": 31243, "url": "https://svs.gsfc.nasa.gov/31243/", "result_type": "Hyperwall Visual", "release_date": "2024-09-23T00:00:00-04:00", "title": "A New Look at Earth’s Lightning", "description": "Map of lightning frequency showing Lake Maracaibo in northern Venezuela and Lake Kivu between Rwanda and Democratic Republic of Congo are the places with the most lightning. || eob149301_annualdenclim_lis_2020_lrg.png (2704x1352) [2.7 MB] || eob149301_annualdenclim_lis_2020_lrg_print.jpg (1024x512) [153.8 KB] || eob149301_annualdenclim_lis_2020_lrg_searchweb.png (320x180) [72.1 KB] || eob149301_annualdenclim_lis_2020_lrg_thm.png (80x40) [6.3 KB] || eob149301_annualdenclim_lis_2020.hwshow [117 bytes] || ", "hits": 200 }, { "id": 5383, "url": "https://svs.gsfc.nasa.gov/5383/", "result_type": "Visualization", "release_date": "2024-09-17T15:00:00-04:00", "title": "Slow Reveal Graphs: Climate Spiral", "description": "Slow reveal graphs are an instructional routine using scaffolded visuals and discourse to help students (in K-12 and beyond) make sense of data. This is a slow reveal graph of the SVS visualization of NASA Climate Spiral. || ", "hits": 198 }, { "id": 14675, "url": "https://svs.gsfc.nasa.gov/14675/", "result_type": "Produced Video", "release_date": "2024-09-03T17:00:00-04:00", "title": "ESCAPADE Testing and Integration", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The spacecraft were designed, built, integrated, and tested by Rocket Lab at their Spacecraft Production Complex and Headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 73 }, { "id": 14664, "url": "https://svs.gsfc.nasa.gov/14664/", "result_type": "Produced Video", "release_date": "2024-08-23T16:00:00-04:00", "title": "ESCAPADE Mission Trailer", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 73 }, { "id": 5362, "url": "https://svs.gsfc.nasa.gov/5362/", "result_type": "Visualization", "release_date": "2024-08-23T00:00:00-04:00", "title": "TROPICS Tracks Hurricane Debby", "description": "This data visualization starts by showing the constellation of cubesats that make up the TROPICS mission collecting data across the globe. The camera then pushes in tighter to show Tropical Depression Debby over Haiti. We then follow Debby's path over Cuba as it begins to organize into a Tropical Storm. It then strengthens to a category 1 hurricane in the Gulf of Mexico right before hitting Florida, where it quickly weakens back into a Tropical Storm. It then slowly moves over Georgia and South Carolina flooding both those states. || tropics_debbyL1c_v90_2024-08-15_1016.02928_print.jpg (1024x576) [146.7 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_searchweb.png (320x180) [86.0 KB] || tropics_debbyL1c_v90_2024-08-15_1016.02928_thm.png (80x40) [6.4 KB] || tropics_debbyL1c_v90_2024-08-15_1016_1080p30.mp4 (1920x1080) [31.8 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4 (3840x2160) [94.7 MB] || 3840x2160_16x9_30p [0 Item(s)] || tropics_debbyL1c_v90_2024-08-15_1016.webm (3840x2160) [20.4 MB] || tropics_debbyL1c_v90_2024-08-15_1016.mp4.hwshow || ", "hits": 37 }, { "id": 14667, "url": "https://svs.gsfc.nasa.gov/14667/", "result_type": "Produced Video", "release_date": "2024-08-22T14:00:00-04:00", "title": "ESCAPADE Instrument Build and Testing", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 45 }, { "id": 14665, "url": "https://svs.gsfc.nasa.gov/14665/", "result_type": "Produced Video", "release_date": "2024-08-21T09:00:00-04:00", "title": "ESCAPADE Spacecraft Development Images", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ", "hits": 44 }, { "id": 14641, "url": "https://svs.gsfc.nasa.gov/14641/", "result_type": "Infographic", "release_date": "2024-07-30T15:00:00-04:00", "title": "ESCAPADE Mission Posters", "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 57 }, { "id": 14642, "url": "https://svs.gsfc.nasa.gov/14642/", "result_type": "Infographic", "release_date": "2024-07-30T15:00:00-04:00", "title": "ESCAPADE Spacecraft Specifications", "description": "The Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission, led by Rob Lillis at the University of California, Berkeley, Space Sciences Laboratory (UCBSSL), is a twin-spacecraft science mission that will orbit two spacecraft around Mars to understand the structure, composition, variability, and dynamics of Mars' unique hybrid magnetosphere. The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time. ESCAPADE is being developed under NASA’s Small Innovative Missions for Planetary Exploration (SIMPLEx) program in the Science Mission Directorate (SMD). The mission is led by UCBSSL with spacecraft design provided by Rocket Lab.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ", "hits": 177 }, { "id": 14609, "url": "https://svs.gsfc.nasa.gov/14609/", "result_type": "Produced Video", "release_date": "2024-07-30T12:00:00-04:00", "title": "Anodizing NICER’s Patches", "description": "This video shows engineering technician Katrina Harvey anodizing NICER’s patches at the Plating Laboratory at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.0:00 One of the NICER patch bodies hangs from a spiky stick by a wire. 0:05 Patch lids attached to a similar stick are seen submerged in a dark blue liquid. 0:07 Harvey lifts the lids and one patch body from a chemical bath and submerges them in a container of deionized water. 0:24 Several lids have been dyed black. 0:29 Harvey submerges the black lids into a chemical bath covered with white plastic balls. 0:42 Harvey lifts undyed patch bodies from a deionized water rinse. 0:47 Harvey lifts patch bodies from a chemical bath covered in white plastic balls and dunks them in deionized water. 1:07 A wider view of Harvey as she works on the patch bodies in the plating lab. 1:24 The patch bodies are shown submerged in a blue liquid. 1:28 A pan across patch bodies submerged in blue liquid. 1:34 Harvey lifts the patch bodies on their individual wires out of a well where nozzles spray them with deionized water. She then dunks them several times in a container of black dye. 1:54 She adds more patch bodies to the black dye. 2:22 She hangs the dyed bodies in a well where nozzles spray them with deionized water. 2:35 Harvey sprays the patches with deionized water. 2:40 Keith Gendreau (NASA), Steve Kenyon (NASA), and Isiah Holt (NASA) cluster together, looking at one of the dyed NICER patch bodies. 2:48 Harvey rinses dyed patch bodies. 2:58 Harvey holds several dyed patch bodies still on their wires. She lifts them and starts walking through the lab. 3:18 Gendreau and Kenyon help remove plugs from holes in the patch bodies. These protected screw threads during the anodizing process. 3:32: Someone dries one of the patch bodies with compressed air. 3:42 The dyed patch bodies rest on a table. 3:58 Close-ups of various features of the lab, like labels, knobs, readouts, buttons, clamps, and wires.Credit:NASA/Sophia Roberts and Scott Wiessinger || Anondizing_Patches_at_4k.00001_print.jpg (1024x576) [72.4 KB] || Anondizing_Patches_at_4k.00001_searchweb.png (320x180) [61.0 KB] || Anondizing_Patches_at_4k.00001_thm.png (80x40) [5.0 KB] || Anondizing_Patches_at_4k.webm (3840x2160) [99.1 MB] || Anondizing_Patches_at_4k.mp4 (3840x2160) [2.5 GB] || Anondizing_Patches_at_4k_ProRes.mov (3840x2160) [18.3 GB] || ", "hits": 34 }, { "id": 14635, "url": "https://svs.gsfc.nasa.gov/14635/", "result_type": "Produced Video", "release_date": "2024-07-22T12:00:00-04:00", "title": "ESCAPADE Mission Spacecraft Beauty Passes", "description": "NASA’s Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will study the interaction between the solar wind and Martian atmosphere. Two identical spacecraft will orbit around the Red Planet to understand the structure, composition, variability, and dynamics of Mars’ unique hybrid magnetosphere, including its real-time response to space weather.The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time — so much that Mars no longer supports liquid water on its surface. The pair will be the first coordinated multi-spacecraft orbital science mission to Mars.ESCAPADE is part of the NASA Small Innovative Missions for Planetary Exploration (SIMPLEx) program. The mission is managed by the University of California Berkeley’s Space Sciences Laboratory, with key partners Rocket Lab, NASA Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ", "hits": 104 }, { "id": 5311, "url": "https://svs.gsfc.nasa.gov/5311/", "result_type": "Visualization", "release_date": "2024-07-17T06:00:00-04:00", "title": "Twelve consecutive months of global surface temperature records: June 2023 - May 2024", "description": "This visualization shows monthly global surface temperatures from 1880 to May 2024. The last 12 months (June 2023 through May 2024) each set a record as the warmest month in the temperature record. This version of the graph is in Fahrenheit. || GISTEMP_Lines_Rotate_2024_degF.00650_print.jpg (1024x1024) [428.6 KB] || GISTEMP_Lines_Rotate_2024_degF.00650_searchweb.png (320x180) [109.7 KB] || GISTEMP_Lines_Rotate_2024_degF.00650_thm.png (80x40) [7.5 KB] || GISTEMP_Lines_Rotate_2024_degF.mp4 (2160x2160) [57.3 MB] || ", "hits": 133 }, { "id": 5327, "url": "https://svs.gsfc.nasa.gov/5327/", "result_type": "Visualization", "release_date": "2024-07-17T06:00:00-04:00", "title": "Slow Reveal Graphs: Twelve consecutive months of global surface temperature records (June 2023 - May 2024)", "description": "Slow reveal graphs are an instructional routine using scaffolded visuals and discourse to help students (in K-12 and beyond) make sense of data. This is a slow reveal graph of the SVS visualization of Twelve consectutive months of global surface temperature records. || ", "hits": 56 }, { "id": 31295, "url": "https://svs.gsfc.nasa.gov/31295/", "result_type": "Hyperwall Visual", "release_date": "2024-06-21T00:00:00-04:00", "title": "Hubble Observes a Cosmic Fossil", "description": "Credits: ESA/Hubble & NASA, F. Niederhofer, L. Girardi || 31295-hubble-ngc2005-potw2424a-hw.jpg (3840x2160) [4.1 MB] || 31295-hubble-ngc2005-potw2424a-hw_searchweb.png (320x180) [108.5 KB] || 31295-hubble-ngc2005-potw2424a-hw_thm.png (80x40) [12.8 KB] || hubble-observes-a-cosmic-fossil.hwshow [321 bytes] || ", "hits": 52 }, { "id": 14604, "url": "https://svs.gsfc.nasa.gov/14604/", "result_type": "Produced Video", "release_date": "2024-06-12T10:00:00-04:00", "title": "NASA’s Roman Mission Gets Cosmic ‘Sneak Peek’ From Supercomputers", "description": "This graphic highlights part of a new simulation of what NASA’s Nancy Grace Roman Space Telescope could see when it launches by May 2027. The background spans about 0.11 square degrees (roughly equivalent to half of the area of sky covered by a full Moon), representing less than half the area Roman will see in a single snapshot. The inset zooms in to a region 300 times smaller, showcasing a swath of brilliant synthetic galaxies at Roman’s full resolution. Having such a realistic simulation helps scientists study the physics behind cosmic images –– both synthetic ones like these and future real ones. Researchers will use the observations for many types of science, including testing our understanding of the origin, evolution, and ultimate fate of the universe.Credit: C. Hirata and K. Cao (OSU) and NASA’s Goddard Space Flight Center || Roman_Simulation_Popout_2k_deg.jpg (2048x2048) [979.2 KB] || ", "hits": 59 }, { "id": 14591, "url": "https://svs.gsfc.nasa.gov/14591/", "result_type": "Produced Video", "release_date": "2024-05-16T12:00:00-04:00", "title": "Quickshot: Twin NASA Spacecraft Headed To Ends Of The Earth Launching May 22", "description": "Scroll down page to see pre-recorded soundbites available for download + animations of the satellites.Check out 5 Things to Know About NASA’s Tiny Twin Polar Satellites ! || Screenshot_2024-05-14_at_4.19.48_PM.png (3360x844) [4.6 MB] || Screenshot_2024-05-14_at_4.19.48_PM_print.jpg (1024x257) [95.7 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_print.jpg (1024x257) [53.8 KB] || Screenshot_2024-05-14_at_4.19.48_PM_web.png (320x80) [53.4 KB] || Screenshot_2024-05-14_at_4.19.48_PM_thm.png (80x40) [10.8 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_searchweb.png (320x180) [94.5 KB] || Screenshot_2024-05-14_at_4.19.48_PM_print_thm.png (80x40) [10.3 KB] || ", "hits": 31 }, { "id": 14552, "url": "https://svs.gsfc.nasa.gov/14552/", "result_type": "Produced Video", "release_date": "2024-03-27T10:00:00-04:00", "title": "Volunteers Help ESA & NASA Mission to Discover 5,000 Comets", "description": "The Solar and Heliospheric Observatory (SOHO), a joint mission of ESA (European Space Agency) and NASA, has discovered its 5,000th comet, thanks to the help of volunteer comet hunters participating in the NASA-funded Sungrazer Project.The sungrazing comet was spotted in SOHO images on March 25, 2024, by Hanjie Tan in the Czech Republic, who has participated in the Sungrazer Project since he was 13 years old. The comet is small and has a short orbital period around the Sun. It belongs to the “Marsden group” of comets, which are thought to be related to the larger comet 96P/Machholz. The group is named after the late scientist Brian Marsden, who first recognized the group using SOHO observations.To learn more about the discovery and SOHO, visit: https://science.nasa.gov/science-research/heliophysics/esa-nasa-solar-observatory-discovers-its-5000th-comet/Since the early 2000s, the Sungrazer Project has allowed anyone with a computer to search for comets in images taken by the SOHO spacecraft.To learn more about the Sungrazer Project, visit: https://science.nasa.gov/citizen-science/the-sungrazer-project/ || ", "hits": 58 }, { "id": 5234, "url": "https://svs.gsfc.nasa.gov/5234/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "AIRS Global Carbon Dioxide (CO₂) measurements (2002-October 2023)", "description": "Data visualization showing the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft over a 20 year timespan.", "hits": 172 }, { "id": 14542, "url": "https://svs.gsfc.nasa.gov/14542/", "result_type": "Produced Video", "release_date": "2024-03-05T10:00:00-05:00", "title": "EZIE – Electrojet Zeeman Imaging Explorer", "description": "Slated to launch in 2025, NASA’s Electrojet Zeeman Imaging Explorer (EZIE) will be the first mission to image the magnetic fingerprint of the auroral electrojets — intense electric currents flowing high above Earth’s poles that are central to the electrical circuit coupling the planet’s magnetosphere to its atmosphere.Led by the Johns Hopkins Applied Physics Laboratory (APL), EZIE will use a trio of small satellites to characterize and record the electrojets’ structure over space and time. It will fill gaps in our understanding of this space weather phenomenon and provide findings that scientists can apply to other magnetized planets, both within and outside our solar system.Learn more:https://science.nasa.gov/mission/ezie/ || ", "hits": 98 }, { "id": 14534, "url": "https://svs.gsfc.nasa.gov/14534/", "result_type": "Produced Video", "release_date": "2024-02-27T11:00:00-05:00", "title": "NASA's Heliophysics Division Director Joe Westlake", "description": "Meet NASA’s new heliophysics division director, Joe Westlake.Joe has more than 18 years of scientific, technical, management, and programmatic experience in heliophysics, astrophysics, and planetary science. Throughout his career he has made several significant contributions to NASA missions including the Magnetospheric Multiscale mission, the Van Allen Probes, Parker Solar Probe, the Interstellar Boundary Explorer mission, the Juno mission, Cassini, and the European Space Agency’s Jupiter Icy Moons Explorer mission.Prior to joining NASA, Joe served as a researcher and project scientist for the Interstellar Mapping and Acceleration Probe mission and principal investigator for the Plasma Instrument for Magnetic Sounding instrument at the Johns Hopkins Applied Physics Laboratory. || ", "hits": 99 }, { "id": 14530, "url": "https://svs.gsfc.nasa.gov/14530/", "result_type": "Produced Video", "release_date": "2024-02-21T08:00:00-05:00", "title": "Goldstone Apple Valley Radio Telescope (GAVRT) Solar Patrol", "description": "The Goldstone Apple Valley Radio Telescope (GAVRT) is located in Goldstone, California. It is a reconfigured antenna used for teaching purposes.The GAVRT program teaches K-12 students how to calibrate this 34-meter antenna (known as Deep Space Station-28), collect and distribute science data through the Internet and get excited about radio astronomy. Students collaborate with scientists who are working on the same mission and are recognized as part of the science team. Data collected and analyzed by the students is used by NASA in their studies of the solar system.During the April 8, 2024, total solar eclipse, NASA’s Jet Propulsion Laboratory, educators at the Lewis Center for Education Research in Southern California, and participants in the center’s Solar Patrol citizen science program will observe solar “active regions” – the magnetically complex regions that form over sunspots – as the Moon moves over them. The Moon’s gradual passage across the Sun blocks different portions of the active region at different times, allowing scientists to distinguish light signals coming from one portion versus another. The technique, first used during the May 2012 annular eclipse, revealed details on the Sun the telescope couldn’t otherwise detect. || ", "hits": 66 }, { "id": 31276, "url": "https://svs.gsfc.nasa.gov/31276/", "result_type": "Hyperwall Visual", "release_date": "2024-02-08T00:00:00-05:00", "title": "Curiosity's Hazcams Capture a Day on Mars", "description": "A hyperwall ready version of animation publised at https://photojournal.jpl.nasa.gov/catalog/PIA26209NASA's Curiosity Mars rover recorded two 25-frame videos showing the passage of 12 hours on Nov. 8, 2023, the 4,002nd Martian day, or sol, of the mission. The images were captured with Curiosity's front and rear Hazard-Avoidance Cameras, or Hazcams. A long series of images can be put together to create a video so that scientists can look for passing clouds or dust devils, which teach them more about the Martian environment. The perfect time for doing this type of work is when Curiosity is less active for long stretches, as it was during Mars solar conjunction. The lack of robotic arm motion and driving during conjunction allowed the Hazcams to image for 12 hours of a day for the first time. While these Hazcam videos didn't reveal any clouds or dust activity, they did capture the passage of time as the Sun rose and set. || ", "hits": 116 }, { "id": 5207, "url": "https://svs.gsfc.nasa.gov/5207/", "result_type": "Visualization", "release_date": "2024-01-12T11:00:00-05:00", "title": "Global Temperature Anomalies from 1880 to 2023", "description": "This color-coded map in Robinson projection displays a progression of changing global surface temperature anomalies. Normal temperatures are shown in white. Higher than normal temperatures are shown in red and lower than normal temperatures are shown in blue. Normal temperatures are calculated over the 30 year baseline period 1951-1980. The maps are averages over a running 24 month window. The final frame represents global temperature anomalies in 2023. || 2023GISTEMP_Map.00899_print.jpg (1024x576) [138.7 KB] || 2023GISTEMP_Map.00899_searchweb.png (320x180) [66.6 KB] || 2023GISTEMP_Map.00899_thm.png (80x40) [6.4 KB] || 2023GISTEMP_Map.00899_web.png (320x180) [65.9 KB] || 2023GISTEMP_Map_HD.mp4 (1920x1080) [57.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 2023GISTEMP_Map.mp4 (3840x2160) [114.3 MB] || earth_observations_5x3.hwshow || ", "hits": 693 }, { "id": 5209, "url": "https://svs.gsfc.nasa.gov/5209/", "result_type": "Visualization", "release_date": "2024-01-12T11:00:00-05:00", "title": "Zonal Climate Anomalies 1880-2023", "description": "A visualization of zonal temperature anomalies. The latitude zones are 90N-64N, 64N-44N, 44N-24N, 24N-EQU, EQU-24S, 24S-44S, 44S-64S, 64S-90S. The anomalies are calculated relative to a baseline period of 1951-1980. This version is in Celsius, an alternate version in Fahrenheit is also available. || GISTEMP_Zonal_1880-2023_C.00840_print.jpg (1024x576) [43.1 KB] || GISTEMP_Zonal_1880-2023_C.00840_searchweb.png (320x180) [18.0 KB] || GISTEMP_Zonal_1880-2023_C.00840_thm.png (80x40) [2.5 KB] || GISTEMP_Zonal_1880-2023_C.mp4 (3840x2160) [20.2 MB] || degC (3840x2160) [0 Item(s)] || GISTEMP_Zonal_1880-2023_C.mp4.hwshow || ", "hits": 125 }, { "id": 5211, "url": "https://svs.gsfc.nasa.gov/5211/", "result_type": "Visualization", "release_date": "2024-01-12T11:00:00-05:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1963-2023", "description": "The change in the distribution of land temperature anomalies over the years 1963 to 2023. This version is in Celsius, a Fahrenheit version is also available. || 2023_GISTEMP_Dist_C.00899_print.jpg (1024x576) [38.5 KB] || 2023_GISTEMP_Dist_C.00899_searchweb.png (320x180) [13.9 KB] || 2023_GISTEMP_Dist_C.00899_thm.png (80x40) [2.3 KB] || 2023_GISTEMP_Dist_C.mp4 (3840x2160) [22.3 MB] || 2023_GISTEMP_Dist_C.mp4.hwshow || ", "hits": 107 }, { "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": 83 }, { "id": 14399, "url": "https://svs.gsfc.nasa.gov/14399/", "result_type": "Produced Video", "release_date": "2023-12-20T11:00:00-05:00", "title": "Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky", "description": "From solar flares to black hole jets: NASA’s Fermi Gamma-ray Space Telescope has produced a unique time-lapse tour of the dynamic high-energy sky. Fermi Deputy Project Scientist Judy Racusin narrates this movie, which compresses 14 years of gamma-ray observations into 6 minutes. Credit: NASA’s Goddard Space Flight Center and NASA/DOE/LAT CollaborationMusic: \"Expanding Shell\" written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Video descriptive text available. || Fermi_14Year_Narrated_Still_print.jpg (1024x576) [157.6 KB] || Fermi_14Year_Narrated_Still.jpg (3840x2160) [891.9 KB] || Fermi_14Year_Narrated_Still_searchweb.png (320x180) [39.2 KB] || Fermi_14Year_Narrated_Still_thm.png (80x40) [4.2 KB] || 14399_Fermi_14Year_Narrated_sub100.mp4 (1920x1080) [90.5 MB] || 14399_Fermi_14Year_Narrated_1080.webm (1920x1080) [49.4 MB] || 14399_Fermi_14Year_Narrated_1080.mp4 (1920x1080) [908.7 MB] || Fermi_14Year_Narrated_SRT_Captions.en_US.srt [8.4 KB] || Fermi_14Year_Narrated_SRT_Captions.en_US.vtt [8.0 KB] || 14399_Fermi_14Year_Narrated_4k.mp4 (3840x2160) [2.2 GB] || 14399_Fermi_14Year_Narrated_ProRes_3840x2160_2997.mov (3840x2160) [19.4 GB] || ", "hits": 132 }, { "id": 14489, "url": "https://svs.gsfc.nasa.gov/14489/", "result_type": "Produced Video", "release_date": "2023-12-18T11:00:00-05:00", "title": "BurstCube Completes Thermal Vacuum Testing", "description": "BurstCube is a mission developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The spacecraft is slated for takeoff in March 2024 from NASA’s Kennedy Space Center in Florida aboard a resupply mission to the International Space Station. This CubeSat will detect short gamma-ray bursts, brief flashes of the highest-energy form of light. Dense stellar remnants called neutron stars create these bursts when they collide with other neutron stars or black holes. Short gamma-ray bursts, which last less than 2 seconds, are important sources for gravitational wave discoveries and multimessenger astronomy. As BurstCube orbits, it will experience major temperature swings every 90 minutes as it passes in and out of daylight. The team evaluated how the spacecraft will operate in these new conditions using a thermal vacuum chamber at Goddard, shown in these images and video, where temperatures ranged from minus 4 to 113 degrees Fahrenheit (minus 20 to 45 Celsius). || ", "hits": 49 }, { "id": 20388, "url": "https://svs.gsfc.nasa.gov/20388/", "result_type": "Animation", "release_date": "2023-12-05T14:00:00-05:00", "title": "PUNCH Spacecraft Beauty Passes", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in Sun-synchronous, low Earth orbit that will make global, 3D observations of the young solar wind, from the outermost solar atmosphere to the inner heliopshere. Images of unprecedented quality will help to close a 60-year gap in measurements of understanding of what occurs in this region of space. PUNCH will share a ride to space with NASA’s Jet Propulsion Laboratory’s Spectro-Photometer for the History of the Universe, Epoch of Re-ionization, and Ices Explorer (SPHEREx) mission. The missions launched on March 11, 2025, on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.Get the latest updates on NASA's PUNCH blog. || ", "hits": 70 }, { "id": 5191, "url": "https://svs.gsfc.nasa.gov/5191/", "result_type": "Visualization", "release_date": "2023-11-16T00:00:00-05:00", "title": "Global Temperature Graph 1880-2024", "description": "The seasonal cycle of average temperature variation on the earth's surface.", "hits": 453 }, { "id": 5190, "url": "https://svs.gsfc.nasa.gov/5190/", "result_type": "Visualization", "release_date": "2023-11-15T00:00:00-05:00", "title": "NASA Climate Spiral 1880-Present", "description": "The NASA climate spiral visualization of the GISTEMP global temperature record.", "hits": 1570 }, { "id": 31263, "url": "https://svs.gsfc.nasa.gov/31263/", "result_type": "Hyperwall Visual", "release_date": "2023-11-15T00:00:00-05:00", "title": "ECOSTRESS observes Summer 2023 heatwaves", "description": "ECOSTRESS image of Houston, Texas heatwave || ecostress_00109_Houston_13Jun2023_print.jpg (1024x724) [400.0 KB] || ecostress_00109_Houston_13Jun2023.png (3507x2480) [7.2 MB] || ecostress_00109_Houston_13Jun2023_searchweb.png (320x180) [129.1 KB] || ecostress_00109_Houston_13Jun2023_thm.png (80x40) [8.4 KB] || ecostress_00109_Houston_13Jun2023.hwshow [115 bytes] || ", "hits": 31 }, { "id": 14440, "url": "https://svs.gsfc.nasa.gov/14440/", "result_type": "Produced Video", "release_date": "2023-10-25T08:00:00-04:00", "title": "Atmospheric Waves Experiment (AWE) Media Resources", "description": "From its unique vantage point on the International Space Station, NASA’s Atmospheric Waves Experiment (AWE) will look directly down into Earth’s atmosphere to study how gravity waves travel through the upper atmosphere. Data collected by AWE will enable scientists to determine the physics and characteristics of atmospheric gravity waves and how terrestrial weather influences the ionosphere, which can affect communication with satellites.AWE is led by Michael Taylor 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 will provide the mission operations center.Visit https://science.nasa.gov/mission/awe/ to learn more. Watch AWE launch aboard NASA's SpaceX Cargo Dragon. Download isolated launch views of NASA's SpaceX CRS-29 mission. || ", "hits": 89 }, { "id": 40513, "url": "https://svs.gsfc.nasa.gov/gallery/awe/", "result_type": "Gallery", "release_date": "2023-10-25T00:00:00-04:00", "title": "AWE – Atmospheric Waves Experiment", "description": "From its unique vantage point on the International Space Station, NASA’s Atmospheric Waves Experiment (AWE) looks directly down into Earth’s atmosphere to study how atmospheric gravity waves — naturally occurring waves often caused by weather disturbances — travel through the upper atmosphere. Data collected by AWE enables scientists to determine the physics and characteristics of atmospheric gravity waves and how terrestrial weather influences the ionosphere, which can affect communication with satellites.\n\nAWE launched on Nov. 9, 2023, from NASA’s Kennedy Space Center in Florida.\n\nLearn more: https://science.nasa.gov/mission/awe/", "hits": 146 }, { "id": 5176, "url": "https://svs.gsfc.nasa.gov/5176/", "result_type": "Visualization", "release_date": "2023-10-16T00:00:00-04:00", "title": "Sea Surface Temperature (SST) Anomaly - Near Real Time", "description": "An equirectangular view of sea surface temperature (SST) anomaly data for the past two and half years, updated daily to include the latest available data. || sst_mur_anomaly_print.jpg (1024x512) [246.1 KB] || sst_mur_anomaly_searchweb.png (320x180) [101.7 KB] || sst_mur_anomaly_20231014_thm.png (80x40) [7.4 KB] || sst_mur_anomaly (4096x2048) [0 Item(s)] || sst_anomaly_30_sec_4096x2048_2x1_30p.mp4 (4096x2048) [338.0 MB] ||", "hits": 0 }, { "id": 20385, "url": "https://svs.gsfc.nasa.gov/20385/", "result_type": "Animation", "release_date": "2023-10-04T15:00:00-04:00", "title": "Atmospheric Waves Experiment (AWE) Beauty Pass", "description": "AWE aboard the ISS || ISS_AWE_ProRes.00420_print.jpg (576x1024) [133.9 KB] || ISS_AWE_ProRes.00420_searchweb.png (180x320) [81.4 KB] || ISS_AWE_ProRes.00420_thm.png (80x40) [6.7 KB] || ISS_AWE_1080_h264.mov (1920x1080) [27.7 MB] || ISS_AWE_ProRes.mov (3840x2160) [1.7 GB] || ISS_AWE_h264.mov (3840x2160) [66.2 MB] || AWE_frames (3840x2160) [32.0 KB] || ISS_AWE_ProRes.webm (3840x2160) [9.6 MB] || ", "hits": 87 }, { "id": 14412, "url": "https://svs.gsfc.nasa.gov/14412/", "result_type": "Produced Video", "release_date": "2023-09-22T09:00:00-04:00", "title": "How NASA Will Study the Asteroid Bennu Samples", "description": "Learn more about how NASA will curate and study samples of asteroid Bennu that were collected by OSIRIS-REx.Complete transcript available.Universal Production Music: “Mirage” and “Manifest” by Ben Niblett and Jonathan David Cotton, Chappell Recorded Music Library Ltd [PRS]; “Lumos” by Ben Niblett and Jonathan David Cotton, Nova Production Music Ltd [PRS]Watch this video on the NASA Goddard YouTube channel. || 14412_OREX_ScienceGoals_Thumbnail_print.jpg (1024x576) [203.8 KB] || 14412_OREX_ScienceGoals_Thumbnail.jpg (1280x720) [376.7 KB] || 14412_OREX_ScienceGoals_Thumbnail.png (1280x720) [1.5 MB] || 14412_OREX_ScienceGoals_Thumbnail_searchweb.png (320x180) [108.5 KB] || 14412_OREX_ScienceGoals_Thumbnail_thm.png (80x40) [6.9 KB] || 14412_OSIRIS-REx_Science_Goals_720.mp4 (1280x720) [59.1 MB] || 14412_OSIRIS-REx_Science_Goals_1080.mp4 (1920x1080) [330.5 MB] || OsirisRexScienceGoals_Captions.en_US.srt [6.0 KB] || OsirisRexScienceGoals_Captions.en_US.vtt [5.7 KB] || 14412_OSIRIS-REx_Science_Goals_4K.mp4 (3840x2160) [4.0 GB] || 14412_OSIRIS-REx_Science_Goals_ProRes.mov (3840x2160) [28.2 GB] || ", "hits": 101 }, { "id": 5161, "url": "https://svs.gsfc.nasa.gov/5161/", "result_type": "Visualization", "release_date": "2023-09-14T11:00:00-04:00", "title": "Summer 2023 Record High Global Temperatures", "description": "This 'map shows monthly temperature anomalies measure from 1880 to August 2023 measured with respect to a the baseline period 1951-1980.Versions are provided in both English and Spanish. || GISTEMP_Summer2023_English_2160p30.00899_print.jpg (1024x576) [191.0 KB] || GISTEMP_Summer2023_English_2160p30.00899_searchweb.png (320x180) [74.2 KB] || GISTEMP_Summer2023_English_2160p30.00899_thm.png (80x40) [7.1 KB] || GISTEMP_Summer2023_English_1080p30.mp4 (1920x1080) [35.8 MB] || GISTEMP_Summer2023_Spanish_2160p30.mp4 (3840x2160) [36.2 MB] || gistemp-summer2023-english (3840x2160) [901 Item(s)] || GISTEMP_Summer2023_English_2160p30.mp4 (3840x2160) [106.5 MB] || GISTEMP_Summer2023_Spanish_2160p30.mp4.hwshow [113 bytes] || GISTEMP_Summer2023_English_2160p30.hwshow || GISTEMP_Summer2023_English_1080p30.mp4.hwshow [137 bytes] || ", "hits": 185 }, { "id": 5137, "url": "https://svs.gsfc.nasa.gov/5137/", "result_type": "Visualization", "release_date": "2023-08-14T11:05:00-04:00", "title": "July 2023 Record High Global Temperatures", "description": "Monthly temperature anomalies measure from 1880 to July 2023 measured with respect to a the baseline period 1951-1980. This graph includes the seasonal cycle (from MERRA2) showing that July 2023 was the warmest month on record. Temperatures measured in Celsius, a Fahrenheit version of this graph is also available. || GISTEMP_Curves_July2023_1080p60.01800_print.jpg (1024x576) [164.8 KB] || GISTEMP_Curves_July2023_1080p60.01800_searchweb.png (320x180) [48.1 KB] || GISTEMP_Curves_July2023_1080p60.01800_thm.png (80x40) [4.1 KB] || GISTEMP_Curves_July2023_1080p60.mp4 (1920x1080) [38.8 MB] || GISTEMP_Curves_July2023_C_2160p60.mp4 (3840x2160) [105.6 MB] || ", "hits": 143 }, { "id": 14373, "url": "https://svs.gsfc.nasa.gov/14373/", "result_type": "Infographic", "release_date": "2023-08-08T10:00:00-04:00", "title": "ComPair Infographic", "description": "Explore this infographic to learn more about ComPair and scientific ballooning.Credit: NASA’s Goddard Space Flight CenterMachine-readable PDF copy || ComPair_Infographic_Final.jpg (5100x6600) [3.3 MB] || ComPair_Infographic_Final.png (5100x6600) [11.7 MB] || ComPair_Infographic_Final-half.jpg (2550x3300) [1.3 MB] || ComPair_Infographic_Final-half.png (2550x3300) [3.8 MB] || ", "hits": 42 }, { "id": 14388, "url": "https://svs.gsfc.nasa.gov/14388/", "result_type": "Produced Video", "release_date": "2023-07-28T00:00:00-04:00", "title": "OSIRIS-REx Sample Curation Rehearsals", "description": "OSIRIS-REx team members practice extracting samples of asteroid Bennu from the Touch-and-Go Sample Acquisition Mechanism (TAGSAM) on June 8, 2023. Teflon spheres were used to represent material from Bennu. || JSC_Cleanroom_Preview_20230608_print.jpg (1024x576) [153.6 KB] || JSC_Cleanroom_Preview_20230608.png (3840x2160) [12.7 MB] || JSC_Cleanroom_Preview_20230608_searchweb.png (320x180) [105.0 KB] || JSC_Cleanroom_Preview_20230608_thm.png (80x40) [7.5 KB] || JSC_OSIRIS-REx_Cleanroom_20230608_720.mp4 (1280x720) [57.7 MB] || JSC_OSIRIS-REx_Cleanroom_20230608_1080.mp4 (1920x1080) [323.1 MB] || JSC_OSIRIS-REx_Cleanroom_20230608_4K.mp4 (3840x2160) [2.0 GB] || ", "hits": 39 }, { "id": 14372, "url": "https://svs.gsfc.nasa.gov/14372/", "result_type": "B-Roll", "release_date": "2023-07-20T10:00:00-04:00", "title": "ComPair Thermal Vacuum Photos", "description": "Team members work on the ComPair balloon instrument before it begins testing in a thermal vacuum chamber at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. ComPair project manager Regina Caputo (front right), graduate student Nicholas Kirschner (George Washington University, left), and research scientist Nicholas Cannady (University of Maryland Baltimore County, rear) examine ComPair's various components to determine what needs to be “harnessed,” or connected via cable to power systems and the onboard computer.Credit: NASA/Scott Wiessinger || ComPair_TVac_IMG_2141.png (5319x3546) [30.9 MB] || ComPair_TVac_IMG_2141.jpg (5319x3546) [6.0 MB] || ComPair_TVac_IMG_2141_half.jpg (2659x1773) [1.4 MB] || ", "hits": 51 }, { "id": 5065, "url": "https://svs.gsfc.nasa.gov/5065/", "result_type": "Visualization", "release_date": "2023-05-31T00:00:00-04:00", "title": "Shifting Distribution of Land Temperature Anomalies, 1962-2022", "description": "The change in the distribution of land temperature anomalies over the years 1962 to 2022. This version is in Celsius, a Fahrenheit version is also available. || GISTEMPDist2022_C.00890_print.jpg (1024x576) [49.0 KB] || GISTEMPDist2022_C.00890_searchweb.png (320x180) [18.8 KB] || GISTEMPDist2022_C.00890_thm.png (80x40) [2.5 KB] || GISTEMPDist2022_C.mp4 (3840x2160) [17.1 MB] || GISTEMPDist2022_C.webm (3840x2160) [4.2 MB] || ", "hits": 351 } ] }