{ "count": 80, "next": null, "previous": null, "results": [ { "id": 14974, "url": "https://svs.gsfc.nasa.gov/14974/", "result_type": "Infographic", "release_date": "2026-08-20T09:00:00-04:00", "title": "Infographic: NASA’s Pandora Mission", "description": "Pandora is a NASA small satellite (SmallSat) mission designed to study exoplanet atmospheres and their host stars. In its first year, it will observe about 20 exoplanets using visible and near-infrared light, revisiting each planet 10 times for 24-hour observations to separate the planet’s signal from its star and reveal the composition of the planet’s atmosphere. || ", "hits": 290 }, { "id": 15046, "url": "https://svs.gsfc.nasa.gov/15046/", "result_type": "Infographic", "release_date": "2026-06-05T10:00:00-04:00", "title": "Swift Multitool Infographic", "description": "This infographic highlights some of the achievements of NASA’s Neil Gehrels Swift Observatory, which has become the agency’s astrophysics multitool since launching in 2004. The spacecraft studies a wide range of objects, from those near Earth, to stars, black holes, and gamma-ray bursts — the most powerful explosions in the cosmos. Credit: NASA’s Goddard Space Flight CenterAlt text: Infographic of some of Swift’s science highlightsImage description: This infographic highlighting NASA’s Neil Gehrels Swift Observatory is done mostly in shades of blue except for pops of green, purple, brown and orange. A line of icon-style images, sort of like a film strip, bisects the image. The icons get smaller the further away they are, giving the sense of distance. Furthest to the left is a green Earth and a brown asteroid. Then there is a white comet, an orange star, a blue-and-white neutron star, a purple-and-black black hole, a blue-and-white spiral galaxy, a reddish nebula, and a purple gamma-ray burst.At top left, text reads “Astrophysics Multitool” and “NASA’s Neil Gehrels Swift Observatory.” Below that is a box labeled “Original Objectives,” with text reading “To discover and quickly localize GRBs (gamma-ray bursts) and observe their afterglows in visible, ultraviolet, and X-ray light.” The GRB text is purple, and the rest is blue. Below the box, text reads “Since launching on Nov. 20, 2004, Swift has …” To the right of the film strip are four boxes. The top box is labeled “GRBs” in purple. There are five lines of text below it reading “Detected thousands of GRBs / Discovered the farthest GRB / Pinpointed the afterglows of short GRBs / Helped monitor the brightest GRB ever seen / Assisted in tying short GRBs to neutron star mergers.”The next box down and a little to the left is labeled “Stars” in orange text on a brown background. Five lines of text below it read “Spotted megaflares from red dwarf stars / Monitored the clashing winds of giant binary stars / Caught enormous star quakes on distant magnetars / Discovered a supernova remnant / Surveyed star formation in the nearest galaxies.”The next box down and a little more to the left is labeled “Earth” in green. The five lines of text below it read “Measured water released by comets / Analyzed an asteroid collision / Caught a comet slowing its spin / Tracked a near-Earth asteroid / Studied a Sun-grazing comet.”The last box at bottom right is labeled “Black Holes” in blue. Five lines of text below it read “Discovered new black holes / Observed monster black holes destroying stars / Used X-ray echoes to map gas around a black hole / Showed that galaxy collisions fuel their central black holes / Found a black hole repeatedly nibbling on a star.” || Swift_Multitool_Infographic_Final_half.jpg (3641x2048) [1.3 MB] || Swift_Multitool_Infographic_Final.jpg (7282x4096) [2.8 MB] || Swift_Multitool_Infographic_Final.png (7282x4096) [10.8 MB] || Swift_Multitool_Infographic_Final_half_searchweb.png (320x180) [91.4 KB] || Swift_Multitool_Infographic_Final_half_thm.png (80x40) [7.4 KB] || ", "hits": 277 }, { "id": 15047, "url": "https://svs.gsfc.nasa.gov/15047/", "result_type": "Produced Video", "release_date": "2026-05-28T10:00:00-04:00", "title": "Milky Way Habitable Zone", "description": "This infographic features artist's concept views of our Milky Way galaxy: face-on at the left and edge-on at the right. It highlights different galactic environments that could influence the development of planets and potentially life. The center of the galaxy is rich in the elements that form planets (like silicon, oxygen, and magnesium), which are forged by multiple generations of stars and supernova explosions. Planets there may be more common or larger, but they would also be flooded with radiation from densely packed stars (including massive ones that emit enormous amounts of high-energy ultraviolet light and X-rays). In the outskirts of the galaxy, where stars are much more spread out, radiation is far milder but there are also smaller amounts of planet-building materials. Nestled in between these regions is the galactic habitable zone, a happy medium where radiation levels and planet-forming elements balance out, increasing the likelihood of worlds that could support life. || MilkyWayZONES_Final_half.jpg (2160x1080) [438.6 KB] || MilkyWayZONES_Final.jpg (4320x2160) [1.2 MB] || MilkyWayZONES_Final.png (4320x2160) [5.9 MB] || MilkyWayZONES_Final_searchweb.png (320x180) [66.4 KB] || MilkyWayZONES_Final_thm.png (80x40) [5.1 KB] || ", "hits": 397 }, { "id": 15033, "url": "https://svs.gsfc.nasa.gov/15033/", "result_type": "Produced Video", "release_date": "2026-05-12T00:00:00-04:00", "title": "TESS Finds Possible New Worlds Using Stellar Eclipses", "description": "A gas giant planet looms in the foreground at right, illuminated by a pair of stars, in this artist’s concept of a world in a binary system. NASA’s TESS (Transiting Exoplanet Survey Satellite) has found planets in two binary star systems by looking for stellar dimming as the planets cross in front of one of the stars. Astronomers have now demonstrated a new method of finding planets in these systems by focusing on the timing of the stars’ mutual eclipses. Credit: NASA's Goddard Space Flight Center/Chris Smith (USRA)Alt text: Planet orbiting a binary systemImage description: Against a starry sky suffused with an orange glow, a gas giant planet with purple and white clouds appears in its crescent phase at right. Two bright stars illuminate the scene, one large and whitish at left, the other smaller and more orange near the center. || circumbinary_planet_AC.png (3991x2160) [3.7 MB] || circumbinary_planet_AC_print.jpg (1024x554) [71.5 KB] || circumbinary_planet_no_text.png (3991x2160) [3.7 MB] || ", "hits": 369 }, { "id": 40542, "url": "https://svs.gsfc.nasa.gov/gallery/dark-energy/", "result_type": "Gallery", "release_date": "2026-01-28T00:00:00-05:00", "title": "Dark Energy", "description": "Some 13.8 billion years ago, the universe began with a rapid expansion we call the big bang. After this initial expansion, which lasted a fraction of a second, gravity started to slow the universe down. But the cosmos wouldn’t stay this way. Nine billion years after the universe began, its expansion started to speed up, driven by an unknown force that scientists have named dark energy.\n\nBut what exactly is dark energy?\n\nThe short answer is: We don't know. But we do know that it exists, it’s making the universe expand at an accelerating rate, and approximately 68.3 to 70% of the universe is dark energy.", "hits": 1095 }, { "id": 14718, "url": "https://svs.gsfc.nasa.gov/14718/", "result_type": "Infographic", "release_date": "2026-01-09T10:00:00-05:00", "title": "NASA's Heliophysics Fleet Graphics (2025)", "description": "NASA has a fleet of spacecraft strategically placed throughout our heliosphere—from Parker Solar Probe at the Sun observing the very start of the solar wind, to satellites around Earth, to the farthest human-made object, Voyager, which is sending back observations on interstellar space. Each mission is positioned at a critical, well-thought out vantage point to observe and understand the flow of energy and particles throughout the solar system—all helping us untangle the effects of the star we live with.The graphics below show the Heliophysics Division fleet as of December 2025. Green indicates missions in operation and blue indicates missions in extended operation. Numbers in parentheses indicate how many spacecraft the mission currently includes. || ", "hits": 136 }, { "id": 14935, "url": "https://svs.gsfc.nasa.gov/14935/", "result_type": "Infographic", "release_date": "2025-12-18T13:00:00-05:00", "title": "Milky Way Anatomy", "description": "This infographic with artist’s concept views of our Milky Way galaxy highlights its main components: the disk, bulge, stellar halo, and dark matter halo. Scientists have a pretty good idea of the Milky Way’s overall structure, but since we’re nestled inside it, fine details are hard to see. Astronomers have used observations from different telescopes to piece together our galaxy's anatomy, and future observatories like NASA's Nancy Grace Roman Space Telescope will make the picture even clearer. || Milky_Way_Anatomy_Infographic_Simple_Final_print.jpg (1024x512) [118.4 KB] || Milky_Way_Anatomy_Infographic_Simple_Final.jpg (4320x2160) [1.2 MB] || Milky_Way_Anatomy_Infographic_Simple_Final.png (4320x2160) [6.5 MB] || Milky_Way_Anatomy_Infographic_Simple_Final_searchweb.png (320x180) [68.0 KB] || Milky_Way_Anatomy_Infographic_Simple_Final_thm.png (80x40) [5.1 KB] || ", "hits": 2084 }, { "id": 14917, "url": "https://svs.gsfc.nasa.gov/14917/", "result_type": "Infographic", "release_date": "2025-12-12T10:00:00-05:00", "title": "Roman Galactic Plane Survey", "description": "No description available.", "hits": 257 }, { "id": 14931, "url": "https://svs.gsfc.nasa.gov/14931/", "result_type": "Infographic", "release_date": "2025-12-04T00:00:00-05:00", "title": "Roman By The Numbers Infographic", "description": "NASA's Nancy Grace Roman Space Telescope will survey vast swaths of sky during its five-year primary mission. During that time, scientists expect it to see an incredible number of new object, including stars, galaxies, black holes and planets outside our solar system, known as exoplanets. This infographic previews some of the discoveries scientists anticipate from Roman's data deluge. || Roman_ByTheNumbers_Infographic_half.jpg (2000x1125) [498.6 KB] || Roman_ByTheNumbers_Infographic_print.jpg (1024x576) [223.6 KB] || Roman_ByTheNumbers_Infographic.png (4000x2250) [2.0 MB] || Roman_ByTheNumbers_Infographic.jpg (4000x2250) [1.0 MB] || Roman_ByTheNumbers_Infographic_searchweb.png (320x180) [75.1 KB] || Roman_ByTheNumbers_Infographic_thm.png (80x40) [7.1 KB] || ", "hits": 197 }, { "id": 14836, "url": "https://svs.gsfc.nasa.gov/14836/", "result_type": "Infographic", "release_date": "2025-05-07T00:00:00-04:00", "title": "Roman Systems Infographic", "description": "This infographic shows the two major subsystems that make up NASA’s Nancy Grace Roman Space Telescope. The subsystems are each undergoing testing prior to being joined together this fall. || Roman_Systems_Infographic_V1_Final_print.jpg (1024x576) [160.5 KB] || Roman_Systems_Infographic_V1_Final_16bit.png (3840x2160) [30.7 MB] || Roman_Systems_Infographic_V1_Final_8bit.png (3840x2160) [8.2 MB] || Roman_Systems_Infographic_V1_Final.jpg (3840x2160) [1.2 MB] || Roman_Systems_Infographic_V1_Final_searchweb.png (320x180) [88.8 KB] || Roman_Systems_Infographic_V1_Final_thm.png [6.4 KB] || ", "hits": 316 }, { "id": 14820, "url": "https://svs.gsfc.nasa.gov/14820/", "result_type": "Infographic", "release_date": "2025-04-24T12:00:00-04:00", "title": "Roman's Core Surveys Infographics", "description": "NASA’s Nancy Grace Roman Space Telescope’s three main observing programs, highlighted in this infographic, will enable astronomers to view the universe as never before, revealing billions of cosmic objects strewn across enormous swaths of space-time.Credit: NASA’s Goddard Space Flight Center || Roman_CoreSurveys_Infographic_print.jpg (1024x640) [155.3 KB] || Roman_CoreSurveys_Infographic.png (8000x5000) [28.6 MB] || Roman_CoreSurveys_Infographic.jpg (8000x5000) [2.5 MB] || Roman_CoreSurveys_Infographic_Half.jpg (4000x2500) [1.3 MB] || Roman_CoreSurveys_Infographic_searchweb.png (320x180) [72.9 KB] || Roman_CoreSurveys_Infographic_thm.png [6.6 KB] || ", "hits": 237 }, { "id": 11738, "url": "https://svs.gsfc.nasa.gov/11738/", "result_type": "Infographic", "release_date": "2024-11-20T00:00:00-05:00", "title": "Infographic: NASA's Neil Gehrels Swift Observatory", "description": "This infographic summarizes key aspects of NASA's Swift mission, from its instruments to scientific results gleaned from 20 years of operations. Swift is still going strong, and the observatory remains a key part of NASA’s strategy to monitor the changing sky with multiple telescopes using different approaches for studying the cosmos.Credit: NASA's Goddard Space Flight CenterClick the download button to select from a range of sizes. || Swift_20_Infographic_Quarter.jpg (1550x1991) [1.2 MB] || Swfit_20_Poster_CMYK.jpg (6200x7965) [19.2 MB] || Swift_20_Infographic_Full.jpg (6200x7965) [7.4 MB] || Swift_20_Infographic_Full.png (6200x7965) [34.2 MB] || Swift_20_Infographic_Half.jpg (3100x3983) [3.2 MB] || Swift_20_Infographic_Half.png (3100x3983) [10.5 MB] || Swift_20_Infographic_Full.jpg.dzi [178 bytes] || Swift_20_Infographic_Full.jpg_files [4.0 KB] || ", "hits": 325 }, { "id": 31302, "url": "https://svs.gsfc.nasa.gov/31302/", "result_type": "Hyperwall Visual", "release_date": "2024-08-02T00:00:00-04:00", "title": "NASA's Balloon Program", "description": "Scientific Balloon Program Infographic || nasa-scientific-balloon-facts_print.jpg (1024x576) [171.2 KB] || nasa-scientific-balloon-facts.png (3840x2160) [3.0 MB] || nasa-scientific-balloon-facts_searchweb.png (320x180) [58.8 KB] || nasa-scientific-balloon-facts_thm.png (80x40) [6.3 KB] || nasas-balloon-program-infographic.hwshow [280 bytes] || ", "hits": 384 }, { "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": 70 }, { "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": 184 }, { "id": 14524, "url": "https://svs.gsfc.nasa.gov/14524/", "result_type": "Infographic", "release_date": "2024-05-07T10:00:00-04:00", "title": "Primordial Black Holes", "description": "This artist's concept takes a fanciful approach to imagining small primordial black holes. In reality, such tiny black holes would have a difficult time forming the accretion disks that make them visible here.Credit: NASA's Goddard Space Flight Center || Primordial_Black_Hole_Still_1080.jpg (1920x1080) [275.1 KB] || Primordial_Black_Hole_Still_4k_print.jpg (1024x576) [51.1 KB] || Primordial_Black_Hole_Still_4k.jpg (3840x2160) [2.5 MB] || Primordial_Black_Hole_Still_4k.png (3840x2160) [7.3 MB] || Primordial_Black_Hole_Still_4k_searchweb.png (320x180) [61.5 KB] || Primordial_Black_Hole_Still_4k_thm.png (80x40) [5.6 KB] || ", "hits": 1106 }, { "id": 14400, "url": "https://svs.gsfc.nasa.gov/14400/", "result_type": "Infographic", "release_date": "2023-10-31T10:00:00-04:00", "title": "Annular Solar Eclipse Flyers", "description": "On Oct. 14, 2023, an annular solar eclipse will cross North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere can experience this eclipse. || ", "hits": 113 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 313 }, { "id": 40495, "url": "https://svs.gsfc.nasa.gov/gallery/small-missions/", "result_type": "Gallery", "release_date": "2023-08-10T00:00:00-04:00", "title": "Small Missions", "description": "Not every NASA mission is the size and cost of Hubble or Webb. Many important instruments and missions are quite small and use less expensive methods to reach space or even simply get above most of the atmosphere.", "hits": 188 }, { "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": 37 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 777 }, { "id": 40491, "url": "https://svs.gsfc.nasa.gov/gallery/balloons/", "result_type": "Gallery", "release_date": "2023-08-02T00:00:00-04:00", "title": "Balloons", "description": "Since its establishment more than 30 years ago, the NASA Balloon Program has provided high-altitude scientific balloon platforms for scientific and technological investigations, including fundamental scientific discoveries that contribute to our understanding of the Earth, the solar system, and the universe.\n\nBalloons have been used for decades to conduct scientific studies. They can be launched from locations across the globe and are a low-cost method to carry payloads with instruments that conduct scientific observations.\n\nThe primary objective of the NASA Balloon Program is to provide high altitude scientific balloon platforms for scientific and technological investigations.\n\nThese investigations include fundamental scientific discoveries that contribute to our understanding of the Earth, the solar system, and the universe. Scientific balloons also provide a platform for the demonstration of promising new instrument and spacecraft technologies that enable or enhance the objectives for the Science Mission Directorate Strategic Plan.", "hits": 75 }, { "id": 14375, "url": "https://svs.gsfc.nasa.gov/14375/", "result_type": "Infographic", "release_date": "2023-06-27T10:00:00-04:00", "title": "NASA’s Roman and ESA’s Euclid Will Team Up To Investigate Dark Energy", "description": "Euclid (left) is a medium-class ESA mission. The Nancy Grace Roman Space Telescope (right) is an upcoming NASA flagship mission. Both will study the history of the universe and bring new insight to the mystery of dark energy.Credit: NASA's Goddard Space Flight Center; ESA/ATG medialab || Euclid-Roman_Graphic_Final.jpg (1920x1080) [476.1 KB] || Euclid-Roman_Graphic_Final_searchweb.png (320x180) [101.4 KB] || Euclid-Roman_Graphic_Final_thm.png (80x40) [7.9 KB] || ", "hits": 162 }, { "id": 31194, "url": "https://svs.gsfc.nasa.gov/31194/", "result_type": "Hyperwall Visual", "release_date": "2022-10-04T00:00:00-04:00", "title": "DART: Double Asteroid Redirection Test", "description": "The DART mission is NASA's demonstration of kinetic impactor technology, impacting an asteroid to adjust its speed and path. DART was the first-ever space mission to demonstrate asteroid deflection by kinetic impactor. It impacted the moonlet Dimorphos on September 26, 2022. || ", "hits": 456 }, { "id": 14130, "url": "https://svs.gsfc.nasa.gov/14130/", "result_type": "Produced Video", "release_date": "2022-04-07T14:00:00-04:00", "title": "Fermi Searches for Gravitational Waves From Monster Black Holes", "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ", "hits": 136 }, { "id": 14107, "url": "https://svs.gsfc.nasa.gov/14107/", "result_type": "Infographic", "release_date": "2022-03-22T10:00:00-04:00", "title": "Roman Space Telescope Redshift Infographic", "description": "This graphic illustrates how cosmological redshift works and how it offers information about the universe’s evolution. The universe is expanding, and that expansion stretches light traveling through space. The more it has stretched, the greater the redshift and the greater the distance the light has traveled. As a result, we need telescopes with infrared detectors to see light from the first, most distant galaxies.Credit: NASA, ESA, Leah Hustak (STScI) || Roman_CosmologicalRedshift_Vertical_v3.png (1920x4843) [1.3 MB] || Roman_CosmologicalRedshift_Vertical_v3_print.jpg (1024x2582) [361.6 KB] || ", "hits": 250 }, { "id": 14001, "url": "https://svs.gsfc.nasa.gov/14001/", "result_type": "Infographic", "release_date": "2021-11-09T10:00:00-05:00", "title": "Roman Space Telescope High Latitude Wide Area Survey", "description": "This illustration compares the relative sizes of the areas of sky covered by two surveys: Roman’s High Latitude Wide Area Survey, outlined in blue, and the largest mosaic led by Hubble, the Cosmological Evolution Survey (COSMOS), shown in red. In current plans, the Roman survey will be more than 1,000 times broader than Hubble’s. Roman will also explore more distant realms of space than most other telescopes have probed in previous efforts to study why the expansion of the universe is speeding up. Credit: NASA's Goddard Space Flight Center || Roman_HLS_FINAL_1080.png (2160x1080) [9.8 MB] || Roman_HLS_FINAL_1080.jpg (2160x1080) [800.5 KB] || Roman_HLS_FINAL_1080_print.jpg (1024x512) [224.7 KB] || Roman_HLS_Final_Full.jpg (8000x4000) [3.8 MB] || Roman_HLS_FINAL_Half.png (4000x2000) [31.6 MB] || Roman_HLS_FINAL_Half.jpg (4000x2000) [1.7 MB] || Roman_HLS_FINAL_Full.png (8000x4000) [114.3 MB] || Roman_HLS_FINAL_1080_searchweb.png (320x180) [90.3 KB] || Roman_HLS_FINAL_1080_thm.png (80x40) [6.9 KB] || ", "hits": 143 }, { "id": 4934, "url": "https://svs.gsfc.nasa.gov/4934/", "result_type": "Infographic", "release_date": "2021-09-01T09:00:00-04:00", "title": "Explore Auroras", "description": "One-page poster version. || Aurora_Infographic_print.jpg (1024x1592) [691.3 KB] || Aurora_Infographic.jpg (3859x6000) [4.7 MB] || Infographics and source components explaining auroras.PDF versions suitable for printing are linked below. || Long poster version. || Aurora_Infographic_Skinny.jpg (1185x9000) [2.1 MB] || Aurora_Infographic_Skinny_print.jpg (1024x7832) [2.0 MB] || ", "hits": 114 }, { "id": 4922, "url": "https://svs.gsfc.nasa.gov/4922/", "result_type": "Infographic", "release_date": "2021-08-25T00:00:00-04:00", "title": "Plasma Waves", "description": "Where various types of plasma waves are found in the magnetosphere. || PlasmaWavesGraphic_print.jpg (1024x788) [190.2 KB] || PlasmaWavesGraphic.png (3280x2527) [3.8 MB] || PlasmaWavesGraphic_searchweb.png (320x180) [50.1 KB] || PlasmaWavesGraphic_thm.png (80x40) [6.2 KB] || Locator graphic for plasma waves in the magnetosphere || ", "hits": 217 }, { "id": 4923, "url": "https://svs.gsfc.nasa.gov/4923/", "result_type": "Infographic", "release_date": "2021-08-25T00:00:00-04:00", "title": "Space Weather Infographics", "description": "Space and earth-based impacts of space weather. || SpaceWeatherIllustration_print.jpg (1024x791) [154.3 KB] || SpaceWeatherIllustration.png (3300x2550) [2.5 MB] || SpaceWeatherIllustration_searchweb.png (320x180) [56.2 KB] || SpaceWeatherIllustration_thm.png (80x40) [6.2 KB] || Multiple infographics illustrating the science and impact of space weather. || ", "hits": 116 }, { "id": 4904, "url": "https://svs.gsfc.nasa.gov/4904/", "result_type": "Infographic", "release_date": "2021-04-28T00:00:00-04:00", "title": "Heliophysics Background Images for MS-Teams & PowerPoint", "description": "Upper atmosphere & ionosphere theme. || Helio_Teams_Bkgrd_1.jpg (1920x1080) [218.8 KB] || Helio_Teams_Bkgrd_1_with_Logos.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_with_Logos_and_Txt.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_print.jpg (1024x576) [151.3 KB] || Helio_Teams_Bkgrd_PPT_1.pptx [520.0 KB] || Six theme images for NASA Heliophysics - image, image+logos, image+logos+text, and PowerPoint files. Suitable as background images for MS-Teams and PowerPoint presentations. || ", "hits": 43 }, { "id": 13806, "url": "https://svs.gsfc.nasa.gov/13806/", "result_type": "Produced Video", "release_date": "2021-03-12T11:00:00-05:00", "title": "Scientists Build a Detailed Image of U Mon Binary", "description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ", "hits": 47 }, { "id": 13794, "url": "https://svs.gsfc.nasa.gov/13794/", "result_type": "Infographic", "release_date": "2021-02-12T14:00:00-05:00", "title": "NASA’s TESS Finds New Worlds in a River of Stars", "description": "This illustration sketches out the main features of TOI 451, a triple-planet system located 400 light-years away in the constellation Eridanus.Credit: NASA’s Goddard Space Flight Center || TOI_451_infographic_1920.png (1920x1080) [2.6 MB] || TOI_451_infographic_1920_print.jpg (1024x576) [129.4 KB] || TOI_451_infographic_3840.png (3840x2160) [8.2 MB] || TOI_451_infographic_1920_searchweb.png (320x180) [73.0 KB] || TOI_451_infographic_1920_thm.png (80x40) [6.5 KB] || ", "hits": 40 }, { "id": 13771, "url": "https://svs.gsfc.nasa.gov/13771/", "result_type": "Infographic", "release_date": "2020-11-13T12:00:00-05:00", "title": "MAVEN Infographic: Martian Dust Storms Accelerate Water Loss", "description": "This illustration shows how water is lost on Mars normally vs. during regional or global dust storms. Text-readable PDF version.Credits: NASA/Goddard/CI Lab/Adriana Manrique Gutierrez/Krystofer Kim || MAVEN_ILLO_v7_print.jpg (1024x575) [117.4 KB] || MAVEN_ILLO_v7.png (6667x3750) [1.5 MB] || MAVEN_ILLO_v7.jpg (6667x3750) [1.4 MB] || MAVEN_ILLO_v7_searchweb.png (320x180) [53.3 KB] || MAVEN_ILLO_v7_thm.png (80x40) [5.9 KB] || ", "hits": 193 }, { "id": 13667, "url": "https://svs.gsfc.nasa.gov/13667/", "result_type": "Produced Video", "release_date": "2020-07-24T16:00:00-04:00", "title": "The Roman Space Telescope's Immense Data Volume", "description": "This infographic showcases the difference in data volume between the Nancy Grace Roman, Webb and Hubble space telescopes. Each day, Roman will send over 500 times more data back to Earth than Hubble.Credit: NASA's Goddard Space Flight Center || Roman_Data_Scale_Final_1080.png (1920x1080) [9.7 MB] || Roman_Data_Scale_Final_1080.jpg (1920x1080) [515.8 KB] || Roman_Data_Scale_Final_1080_print.jpg (1024x576) [99.3 KB] || Roman_Data_Scale_Final.png (3840x2160) [38.9 MB] || Roman_Data_Scale_Final.jpg (3840x2160) [1.9 MB] || ", "hits": 360 }, { "id": 13583, "url": "https://svs.gsfc.nasa.gov/13583/", "result_type": "Infographic", "release_date": "2020-04-20T10:00:00-04:00", "title": "Hubble, Roman and Webb Space Telescopes Infographic", "description": "This infographic shows the complementary capabilities of select instruments on three of NASA's flagship missions: the Hubble Space Telescope and the currently under development Nancy Grace Roman Space Telescope and James Webb Space Telescope. Hubble views the cosmos in infrared, visible and ultraviolet light, providing a more comprehensive, high-resolution view of individual objects. The Roman Space Telescope will expand on Hubble’s infrared observations specifically, using a much larger field of view to create enormous panoramas of the universe with the same high resolution. Webb will also conduct high-resolution infrared observations, peering across farther stretches of space with a narrower field of view.Credit: NASA's Goddard Space Flight Center || HRJ_Infographic_Final2.png (4560x6680) [20.0 MB] || HRJ_Infographic_Final2.jpg (4560x6680) [5.2 MB] || HRJ_Infographic_Final2_HalfSize.jpg (2280x3340) [2.1 MB] || HRJ_Infographic_Final2_HalfSize.png (2280x3340) [8.8 MB] || HRJ_Infographic_Final2.png.hwshow [119 bytes] || ", "hits": 705 }, { "id": 13526, "url": "https://svs.gsfc.nasa.gov/13526/", "result_type": "Infographic", "release_date": "2020-01-24T10:00:00-05:00", "title": "What Makes an Exoplanet Habitable?", "description": "Explore this infographic to learn more about the many different factors that make a planet potentially habitable. Complete text transcript available.Machine readable version available.Credit: NASA Goddard Space Flight Center || Infographic_24x70_inset.jpg (1920x1080) [201.2 KB] || Habitability_Infographic_CROP_print.jpg (1024x702) [120.2 KB] || Habitability_Infographic_CROP.png (6667x4573) [1.7 MB] || Habitability_Infographic_FULL_24x70_2024Update.png (6667x19500) [5.4 MB] || Habitability_Infographic_CROP_searchweb.png (320x180) [47.0 KB] || Habitability_Infographic_CROP_thm.png (80x40) [5.7 KB] || ", "hits": 328 }, { "id": 13200, "url": "https://svs.gsfc.nasa.gov/13200/", "result_type": "Produced Video", "release_date": "2019-07-29T10:00:00-04:00", "title": "NASA’s TESS Finds Three New Worlds", "description": "This infographic illustrates key features of the TOI 270 system, located about 73 light-years away in the southern constellation Pictor. The three known planets were discovered by NASA’s Transiting Exoplanet Survey Satellite through periodic dips in starlight caused by each orbiting world. Insets show information about the planets, including their relative sizes, and how they compare to Earth. Temperatures given for TOI 270’s planets are equilibrium temperatures, calculated without the warming effects of any possible atmospheres. Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger || TOI_270_Infographic_Final_print.jpg (1024x576) [64.1 KB] || TOI_270_Infographic_Final.png (5760x3240) [17.4 MB] || TOI_270_Infographic_Final.jpg (5760x3240) [2.0 MB] || TOI_270_Infographic_Final-halfsize.png (2880x1620) [5.4 MB] || TOI_270_Infographic_Final-halfsize.jpg (2880x1620) [484.0 KB] || TOI_270_Infographic_Final_searchweb.png (320x180) [47.7 KB] || TOI_270_Infographic_Final_thm.png (80x40) [4.9 KB] || ", "hits": 125 }, { "id": 40363, "url": "https://svs.gsfc.nasa.gov/gallery/sounding-rockets/", "result_type": "Gallery", "release_date": "2019-05-09T00:00:00-04:00", "title": "Sounding Rockets", "description": "\nFor over 40 years, NASA's Sounding Rocket Program has provided critical scientific, technical, and educational contributions to the nation's space program and is one of the most robust, versatile, and cost-effective flight programs at NASA. \n\nSounding rockets carry scientific instruments into space along a parabolic trajectory. Their overall time in space is brief, typically 5-20 minutes, and at lower vehicle speeds for a well-placed scientific experiment. The short time and low vehicle speeds are more than adequate (in some cases they are ideal) to carry out a successful scientific experiments. Furthermore, there are some important regions of space that are too low for satellites and thus sounding rockets provide the only platforms that can carry out measurements in these regions.\n\nGo to NASA.gov for the latest sounding rocket news.", "hits": 216 }, { "id": 4707, "url": "https://svs.gsfc.nasa.gov/4707/", "result_type": "Infographic", "release_date": "2019-02-22T00:00:00-05:00", "title": "Solar Wind Infographic", "description": "Large image version. PDF for posters linked below. || Solar_Wind_Infographic_Final.jpg (2418x3000) [1.3 MB] || Solar_Wind_Infographic_Final_searchweb.png (320x180) [97.7 KB] || Solar_Wind_Infographic_Final_thm.png (80x40) [7.6 KB] || ", "hits": 101 }, { "id": 4702, "url": "https://svs.gsfc.nasa.gov/4702/", "result_type": "Infographic", "release_date": "2019-02-11T06:00:00-05:00", "title": "MAVEN Aerobraking to Achieve Science and Relay Orbit", "description": "Aerobraking plan for MAVEN. (left) Current MAVEN orbit around Mars — 6200-km highest altitude, and an orbit period of ~4.5 hours. (center) Aerobraking process — MAVEN performs a series of “deep dip” orbits approaching to within ~125 km of Mars at lowest altitude, causing drag from the atmosphere slow down the spacecraft. Over roughly three-hundred and sixty orbits spanning about two months, this slowing reduces the spacecraft’s highest altitude to ~4500 km and its orbit period to ~3.5 hours. (right) Post-aerobraking orbit, with reduced altitude and shorter orbit period. || maven_aerobraking_comp_03_print.jpg (1024x576) [90.4 KB] || MavenAerobrakingDiagram.jpg (3840x2160) [679.4 KB] || maven_aerobraking_comp_03_searchweb.png (320x180) [38.7 KB] || maven_aerobraking_comp_03_thm.png (80x40) [4.9 KB] || maven_aerobraking_comp_03.tif (3840x2160) [23.8 MB] || ", "hits": 64 }, { "id": 13068, "url": "https://svs.gsfc.nasa.gov/13068/", "result_type": "Infographic", "release_date": "2018-09-11T15:00:00-04:00", "title": "ICESat-2 Infographic", "description": "Infographic || infographic_thumb_print.jpg (1024x532) [141.4 KB] || ICESat2_Infographic.png (2625x3375) [6.8 MB] || infographic_thumb_searchweb.png (320x180) [87.7 KB] || infographic_thumb_thm.png (80x40) [6.3 KB] || Downloadable high-resolution infographic illustrating the major technology and science objectives of the Ice, Cloud and land Elevation Satellite-2. || ", "hits": 39 }, { "id": 12968, "url": "https://svs.gsfc.nasa.gov/12968/", "result_type": "Infographic", "release_date": "2018-09-11T10:00:00-04:00", "title": "PIPER Infographic", "description": "The Primordial Inflation Polarization Explorer (PIPER) is a NASA scientific balloon mission that will fly to the edge of Earth’s atmosphere to study twisty patterns of light in the universe’s “baby picture.” This infographic highlights some facts about PIPER’s instruments, capabilities and goals.Credit: NASA's Goddard Space Flight CenterMachine-readable PDF copy || PIPER_Infographic_FINAL_Medium.jpg (1500x1941) [902.2 KB] || PIPER_Infographic_FINAL_Small.jpg (1000x1294) [469.6 KB] || PIPER_Infographic_FINAL.jpg (5100x6600) [6.6 MB] || PIPER_Infographic_FINAL.png (5100x6600) [15.3 MB] || PIPER_Infographic_FINAL_half.jpg (2550x3300) [1.7 MB] || PIPER_Infographic_FINAL_half.png (2550x3300) [6.9 MB] || ", "hits": 59 }, { "id": 4671, "url": "https://svs.gsfc.nasa.gov/4671/", "result_type": "Infographic", "release_date": "2018-08-07T14:00:00-04:00", "title": "Parker Solar Probe - Close to the Sun", "description": "Image representing Parker Solar Probe's distance from the Sun. || Parker_Close_to_Sun_Infographic_print.jpg (1024x662) [60.0 KB] || Parker_Close_to_Sun_Infographic.jpg (5100x3300) [1001.2 KB] || Parker_Close_to_Sun_Infographic_borderless.jpg (4628x2572) [1.0 MB] || Parker_Close_to_Sun_Infographic_searchweb.png (320x180) [86.8 KB] || Parker_Close_to_Sun_Infographic_thm.png (80x40) [7.1 KB] || parker-solar-probe-close-to-the-sun.hwshow [306 bytes] || ", "hits": 249 }, { "id": 4672, "url": "https://svs.gsfc.nasa.gov/4672/", "result_type": "Infographic", "release_date": "2018-08-07T14:00:00-04:00", "title": "Solar Corona Science Timeline", "description": "A timeline of science of the solar wind and corona. || Solar_Wind_and_Corona_Timeline_print.jpg (1024x1448) [521.5 KB] || Solar_Wind_and_Corona_Timeline.jpg (4193x5931) [3.4 MB] || Solar_Wind_and_Corona_Timeline_searchweb.png (320x180) [97.1 KB] || Solar_Wind_and_Corona_Timeline_thm.png (80x40) [7.6 KB] || ", "hits": 79 }, { "id": 4673, "url": "https://svs.gsfc.nasa.gov/4673/", "result_type": "Infographic", "release_date": "2018-08-07T14:00:00-04:00", "title": "Parker Solar Probe", "description": "Specifications on the Parker Solar Probe mission and its science questions. || Parker_Solar_Probe_Infographic_print.jpg (1024x950) [474.3 KB] || Parker_Solar_Probe_Infographic.jpg (3479x3230) [2.1 MB] || Parker_Solar_Probe_Infographic_searchweb.png (320x180) [115.9 KB] || Parker_Solar_Probe_Infographic_thm.png (80x40) [7.5 KB] || ", "hits": 313 }, { "id": 20282, "url": "https://svs.gsfc.nasa.gov/20282/", "result_type": "Animation", "release_date": "2018-07-30T11:00:00-04:00", "title": "Terraforming the Martian Atmosphere", "description": "One of the challenges of terraforming Mars is to increase its atmospheric pressure, which is currently less than 1% that of Earth. The Martian polar caps, minerals, and soil could all provide sources of carbon dioxide and water to thicken the atmosphere. Unfortunately, a new study by the MAVEN science team finds that processing all sources available on Mars would only increase the pressure to about 7% that of Earth, far short of what is needed.Learn more about this finding. || ", "hits": 303 }, { "id": 4668, "url": "https://svs.gsfc.nasa.gov/4668/", "result_type": "Infographic", "release_date": "2018-07-12T00:00:00-04:00", "title": "Mind-Melting Facts About the Sun", "description": "Image of poster. See link below for PDF version. || MM_FATS_Infographic_w_NASA_ID_print.jpg (1024x1481) [343.3 KB] || MM_FATS_Infographic_w_NASA_ID.jpg (2966x4291) [1.7 MB] || MM_FATS_Infographic_w_NASA_ID.png (2966x4291) [10.3 MB] || MM_FATS_Infographic_w_NASA_ID_searchweb.png (320x180) [100.6 KB] || MM_FATS_Infographic_w_NASA_ID_thm.png (80x40) [6.6 KB] || Fascinating Facts about the Sun. || ", "hits": 170 }, { "id": 12973, "url": "https://svs.gsfc.nasa.gov/12973/", "result_type": "Infographic", "release_date": "2018-06-01T23:00:00-04:00", "title": "NASA's Heliophysics Fleet", "description": "Heliophysics encompasses science that improves our un­derstanding of fundamental physical processes throughout the solar system, and enables us to understand how the Sun, as the major driver of the energy throughout the solar system, impacts our technological society. The scope of heliophysics is vast, spanning from the Sun’s interior to Earth’s upper atmosphere, throughout interplanetary space, to the edges of the heliosphere, where the solar wind interacts with the local interstellar medium. Heliophysics incorporates studies of the interconnected elements in a single system that produces dynamic space weather and that evolves in response to solar, planetary, and interstellar conditions. || ", "hits": 80 }, { "id": 12960, "url": "https://svs.gsfc.nasa.gov/12960/", "result_type": "Infographic", "release_date": "2018-05-31T19:00:00-04:00", "title": "Ionosphere Graphics", "description": "Stretching from roughly 50 to 400 miles above Earth’s surface, the ionosphere is an electrified layer of the upper atmosphere, generated by extreme ultraviolet radiation from the Sun. It’s neither fully Earth nor space, and instead, reacts to both terrestrial weather below and solar energy streaming in from above, forming a complex space weather system of its own. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. Positioned on the edge of space and intermingled with the neutral atmosphere, the ionosphere’s response to conditions on Earth and in space is difficult to pin down. || ", "hits": 481 }, { "id": 12961, "url": "https://svs.gsfc.nasa.gov/12961/", "result_type": "Produced Video", "release_date": "2018-05-24T19:00:00-04:00", "title": "ICON Graphics", "description": "The Ionospheric Connection Explorer, or ICON, is a low-Earth orbiting satellite that will give us new information about how Earth’s atmosphere interacts with near-Earth space — a give-and-take that plays a major role in the safety of our satellites and reliability of communications signals. Specifically, ICON investigates the connections between the neutral atmosphere — which extends from here near the surface to far above us, at the edge of space — and the electrically charged part of the atmosphere, called the ionosphere. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. || ", "hits": 27 }, { "id": 4641, "url": "https://svs.gsfc.nasa.gov/4641/", "result_type": "Infographic", "release_date": "2018-05-03T00:00:00-04:00", "title": "Terrestrial Atmosphere ITM (Ionosphere, Thermosphere, Mesosphere) Processes", "description": "Large image version || Terrestrial_Atmos_ITM_Processes.jpg (3355x2205) [1.2 MB] || Terrestrial_Atmos_ITM_Processes_searchweb.png (320x180) [65.0 KB] || Terrestrial_Atmos_ITM_Processes_thm.png (80x40) [7.1 KB] || This graphic presents an overview of the physical processes that have been identified in Earth's upper atmosphere. || ", "hits": 128 }, { "id": 12825, "url": "https://svs.gsfc.nasa.gov/12825/", "result_type": "Infographic", "release_date": "2018-01-24T12:00:00-05:00", "title": "GOLD Resources", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. The more we know about the fundamental physics of this region of space, the more we can protect our assets there.Gathering observations from geostationary orbit above the Western Hemisphere, GOLD measures the temperature and composition of neutral gases in Earth’s thermosphere. This part of the atmosphere co-mingles with the ionosphere, which is made up of charged particles. Both the Sun from above and terrestrial weather from below can change the types, numbers, and characteristics of the particles found here — and GOLD helps track those changes.Activity in this region is responsible for a variety of key space weather events. GOLD scientists are particularly interested in the cause of dense, unpredictable bubbles of charged gas that appear over the equator and tropics, sometimes causing communication problems. As we discover the very nature of the Sun-Earth interaction in this region, the mission could ultimately lead to ways to improve forecasts of such space weather and mitigate its effects. || ", "hits": 129 }, { "id": 12833, "url": "https://svs.gsfc.nasa.gov/12833/", "result_type": "Produced Video", "release_date": "2018-01-24T12:00:00-05:00", "title": "GOLD Media Telecon", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. On January 25, 2018, the mission will launch as NASA's first-ever hosted payload.Speakers for the January 24, 2018 media telecon about the mission include:Richard Eastes, Principal Investigator, Laboratory for Atmospheric and Space Physics at the University of Colorado BoulderElsayed Talaat, Heliophysics Chief Scientist, NASA HeadquartersSusan Batiste, Systems Engineer, LASP/CUKatelynn Greer, Research Scientist, LASP/CUReplay information will be available until January 31, 2018 noon ET, via: Toll free, from within the U.S.: 1-866-469-5761 \u2028Toll: 203-369-1460 || ", "hits": 30 }, { "id": 4611, "url": "https://svs.gsfc.nasa.gov/4611/", "result_type": "Infographic", "release_date": "2018-01-19T14:00:00-05:00", "title": "2018 Poker Flat Sounding Rocket Infographic", "description": "Image of poster || 2018_Poker_Flat_Sounding_Rocket_Quick_Look_Infographic.jpg (3378x6000) [2.4 MB] || 2018_Poker_Flat_Sounding_Rocket_Quick_Look_Infographic_searchweb.png (320x180) [64.9 KB] || 2018_Poker_Flat_Sounding_Rocket_Quick_Look_Infographic_thm.png (80x40) [6.0 KB] || For More Information || See [NASA.gov](https://www.nasa.gov/feature/goddard/2018/nasa-alaska-launched-rockets-to-study-space-x-ray-emissions-and-create-polar-mesospheric) || ", "hits": 19 }, { "id": 4612, "url": "https://svs.gsfc.nasa.gov/4612/", "result_type": "Infographic", "release_date": "2018-01-19T14:00:00-05:00", "title": "Magnetospheric Multiscale (MMS) Mission", "description": "Image of MMS Poster || MMS_Poster.jpg (2857x4000) [1.4 MB] || MMS_Poster_searchweb.png (320x180) [85.9 KB] || MMS_Poster_thm.png (80x40) [7.0 KB] || For More Information || See [NASA.gov](https://www.nasa.gov/mms) || ", "hits": 21 }, { "id": 12783, "url": "https://svs.gsfc.nasa.gov/12783/", "result_type": "Infographic", "release_date": "2017-12-06T12:45:00-05:00", "title": "SuperTIGER Ready to Fly Again in Study of Heavy Cosmic Rays", "description": "SuperTIGER team members Brian Rauch, Jason Link and Nathan Walsh join NASA Blueshift's Sara Mitchell for a Skype conversation in November 2017 about the instrument's science, technology and upcoming launch from McMurdo Station, Antarctica. Credit: NASA's Goddard Space Flight CenterComplete transcript available. || SuperTIGER_Skype_Still.png (1280x720) [1.2 MB] || SuperTIGER_Skype2.webm (1280x720) [135.1 MB] || SuperTIGER_Skype2.mp4 (1280x720) [608.6 MB] || SuperTIGER_Skype2_SRT_Captions.en_US.srt [22.5 KB] || SuperTIGER_Skype2_SRT_Captions.en_US.vtt [22.5 KB] || SuperTIGER_Skype2_best.mp4 (1280x720) [1.2 GB] || ", "hits": 61 }, { "id": 4598, "url": "https://svs.gsfc.nasa.gov/4598/", "result_type": "Infographic", "release_date": "2017-11-24T00:00:00-05:00", "title": "Juno Infographic", "description": "TIFF image of the PDF poster (linked below). || Juno_Infographic_print.jpg (1024x975) [242.5 KB] || Juno_Infographic_searchweb.png (320x180) [76.7 KB] || Juno_Infographic_thm.png (80x40) [6.7 KB] || Juno_Infographic.tiff (4743x4517) [12.1 MB] || Some graphics and facts about the Juno mission at Jupiter. || ", "hits": 37 }, { "id": 4599, "url": "https://svs.gsfc.nasa.gov/4599/", "result_type": "Infographic", "release_date": "2017-11-17T00:00:00-05:00", "title": "Magnetic Reconnection Infographic", "description": "TIFF image of the PDF poster (linked below). || Magnetic_Reconnection_Infographic_print.jpg (1024x3054) [456.7 KB] || Magnetic_Reconnection_Infographic_searchweb.png (320x180) [35.6 KB] || Magnetic_Reconnection_Infographic_thm.png (80x40) [4.3 KB] || Magnetic_Reconnection_Infographic.tiff (1259x3756) [3.1 MB] || Where magnetic reconnections is thought to operate. || ", "hits": 20 }, { "id": 12646, "url": "https://svs.gsfc.nasa.gov/12646/", "result_type": "Produced Video", "release_date": "2017-06-21T13:00:00-04:00", "title": "2017 Solar Eclipse Press Conference", "description": "For the first time in 99 years, a total solar eclipse will cross the entire nation Aug. 21. Representatives from NASA, other federal agencies, and science organizations, will provide important viewing safety, travel and science information during two briefings at the Newseum in Washington starting at 1 p.m. EDT Wednesday, June 21.The event will air live on NASA Television and stream on the agency’s website.Over the course of 100 minutes, 14 states across the United States will experience more than two minutes of darkness in the middle of the day. Additionally, a partial eclipse will be viewable across all of North America. The eclipse will provide a unique opportunity to study the sun, Earth, moon and their interaction because of the eclipse’s long path over land coast to coast. Scientists will be able to take ground-based and airborne observations over a period of an hour and a half to complement the wealth of data and images provided by space assets.The June 21 briefings are:Logistics Briefing: 1 to 2 p.m.Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate at the agency’s headquarters in WashingtonVanessa Griffin, director of the National Oceanic and Atmospheric Administration’s Office of Satellite and Product Operations in Suitland, MarylandBrian Carlstrom, deputy associate director of Natural Resource Stewardship and Science at the National Park Service in WashingtonMartin Knopp, associate administrator of the Office of Operations in the Federal Highway Administration at the U.S. Department of Transportation in WashingtonScience Briefing: 2:30 to 3:30 p.m.Thomas ZurbuchenAngela Des Jardins, principal investigator of the Eclipse Ballooning Project at Montana State University, BozemanAngela Speck, professor of astrophysics and director of astronomy at the University of Missouri, ColumbiaDave Boboltz, program director of solar physics in the Division of Astronomical Sciences at the National Science Foundation in Arlington, VirginiaLinda Shore, executive director of the Astronomical Society of the Pacific in San FranciscoMatt Penn, astronomer at the National Solar Observatory in Tucson, Arizona || ", "hits": 88 }, { "id": 12557, "url": "https://svs.gsfc.nasa.gov/12557/", "result_type": "Produced Video", "release_date": "2017-03-30T14:00:00-04:00", "title": "MAVEN Reveals Mars Argon Loss to Space", "description": "Infographic explaining the MAVEN argon results. Enlarge or click \"download\" for print-resolution versions. Also available in text-readable PDF for the visually impaired. || MAVEN_Argon_Infographic_print.jpg (1024x450) [159.1 KB] || MAVEN_Argon_Infographic.jpg (7500x3300) [4.1 MB] || MAVEN_Argon_Infographic.png (7500x3300) [27.0 MB] || MAVEN_Argon_Infographic_searchweb.png (320x180) [72.3 KB] || MAVEN_Argon_Infographic_thm.png (80x40) [5.0 KB] || MAVEN_Argon_Infographic.tif (7500x3300) [27.2 MB] || maven-reveals-mars-argon-loss-to-space.hwshow || ", "hits": 144 }, { "id": 12504, "url": "https://svs.gsfc.nasa.gov/12504/", "result_type": "Produced Video", "release_date": "2017-02-09T13:00:00-05:00", "title": "Searching for Earth's Trojan Asteroids", "description": "Trojan asteroids accompany several of our solar system's planets, leading or trailing the planet in its orbit at the L4 and L5 Lagrange points. Detecting our own planet's Trojan asteroids from Earth is difficult because they appear close to the sun from our perspective. In mid-February 2017, NASA's OSIRS-REx mission will search for these elusive objects when the spacecraft passes by Earth's L4 Lagrange point, en route to asteroid Bennu in 2018.Learn more about OSIRIS-REx's search for Earth Trojans.Visit OSIRIS-REx at NASA and the University of Arizona. || ", "hits": 103 }, { "id": 12494, "url": "https://svs.gsfc.nasa.gov/12494/", "result_type": "Produced Video", "release_date": "2017-02-07T00:00:00-05:00", "title": "GPM Has Best Calibrated Microwave Imager in the World", "description": "This is an infographic describing how the GPM Microwave Imager works and maintains its high degree of calibration, as well as how it contributes to the precipitation rates produced by the mission. || GMI_Calibration_Infographic_10_Final.jpg (1275x5978) [2.9 MB] || GMI_thumbnail_searchweb.png (320x180) [39.4 KB] || GMI_thumbnail_thm.png (80x40) [4.2 KB] || ", "hits": 19 }, { "id": 4526, "url": "https://svs.gsfc.nasa.gov/4526/", "result_type": "Infographic", "release_date": "2017-01-12T00:00:00-05:00", "title": "Ye Olde Tyme Heliophysics Map", "description": "Basic Olde Tyme Heliophysics Map. || OldeTimeHelioMapv4_print.jpg (1024x574) [245.1 KB] || OldeTimeHelioMapv4_searchweb.png (180x320) [110.2 KB] || OldeTimeHelioMapv4_thm.png (80x40) [7.6 KB] || OldeTimeHelioMapv4.pptx [6.5 MB] || OldeTimeHelioMapv4.tif (7819x4386) [98.1 MB] || OldeTimeHelioMapv4.key [98.8 MB] || ye-olde-tyme-heliophysics-map.hwshow || ", "hits": 88 }, { "id": 30822, "url": "https://svs.gsfc.nasa.gov/30822/", "result_type": "Infographic", "release_date": "2016-12-06T00:00:00-05:00", "title": "NASA's Heliophysics Fleet", "description": "The current Heliophysics fleet || hpd-fleet-chart-jan-2024_print.jpg (1024x576) [180.0 KB] || hpd-fleet-chart-jan-2024.png (3840x2160) [7.3 MB] || hpd-fleet-chart-jan-2024_searchweb.png (320x180) [91.3 KB] || hpd-fleet-chart-jan-2024_thm.png (80x40) [7.2 KB] || nasas-fleets-by-division-helio-jewel.hwshow [228 bytes] ||", "hits": 89 }, { "id": 40305, "url": "https://svs.gsfc.nasa.gov/gallery/roman/", "result_type": "Gallery", "release_date": "2016-07-21T00:00:00-04:00", "title": "Nancy Grace Roman Space Telescope", "description": "NASA’s Nancy Grace Roman Space Telescope will pair a large field of view with crisp infrared vision to scan vast, deep swaths of sky. This flagship mission is designed to help astronomers explore dark matter, dark energy, and exoplanets. Since each of Roman’s surveys will sample such a large volume of the cosmos, the mission will also offer practically limitless opportunities for astronomers to conduct a broad range of additional science. From objects in our outer solar system and exploding stars to growing black holes and galaxies by the billions, very little will be beyond Roman’s reach. Roman’s data will be made public as soon as it’s processed so many teams will be able to analyze it simultaneously. The mission is targeting an August 30, 2026, launch from NASA’s Kennedy Space Center in Florida. \nMore information about the Roman Space Telescope", "hits": 0 }, { "id": 12239, "url": "https://svs.gsfc.nasa.gov/12239/", "result_type": "Produced Video", "release_date": "2016-05-12T13:00:00-04:00", "title": "MMS First Results", "description": "This short video outlines the MMS mission and its first results. Since it launched, MMS has made more than 4,000 trips through the magnetic boundaries around Earth, each time gathering information about the way the magnetic fields and particles move. A surprising result was that at the moment of interconnection between the sun’s magnetic field lines and those of Earth the crescents turned abruptly so that the electrons flowed along the field lines. By watching these electron tracers, MMS made the first observation of the predicted breaking and interconnection of magnetic fields in space. Credit: NASA/GSFCWatch this video on the NASA Goddard YouTube channel. || mmsthumb.jpg (1280x720) [139.4 KB] || mmsthumb_print.jpg (1024x576) [161.8 KB] || mmsthumb_searchweb.png (320x180) [104.3 KB] || mmsthumb_web.png (320x180) [104.3 KB] || mmsthumb_thm.png (80x40) [6.8 KB] || 12239_MMS_First_ResultsV2_appletv.m4v (1280x720) [76.9 MB] || 12239_MMS_First_ResultsV2.webm (1920x1080) [18.1 MB] || 12239_MMS_First_ResultsV2_appletv_subtitles.m4v (1280x720) [77.0 MB] || 12239_MMS_First_ResultsV2.en_US.srt [3.0 KB] || 12239_MMS_First_ResultsV2.en_US.vtt [3.0 KB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov (1920x1080) [1.1 GB] || 12239_MMS_First_ResultsV2_lowres.mp4 (480x272) [21.6 MB] || 12239_MMS_First_ResultsV2_ipod_sm.mp4 (320x240) [26.3 MB] || PRORES_B-ROLL_12239_MMS_First_ResultsV2_prores.mov (1280x720) [2.2 GB] || 12239_MMS_First_ResultsV2.mov (1920x1080) [4.2 GB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov.hwshow [100 bytes] || ", "hits": 119 }, { "id": 12052, "url": "https://svs.gsfc.nasa.gov/12052/", "result_type": "Produced Video", "release_date": "2015-12-01T10:00:00-05:00", "title": "SOHO Celebrates 20 Years of Space-based Science", "description": "Dr. Joe Gurman of NASA's Goddard Space Flight Center provides commentary on selected shots from SOHO's 20 years in space.Watch this video on YouTube || SOHO20thumb.jpg (1280x720) [108.1 KB] || SOHO20thumb_searchweb.png (320x180) [119.7 KB] || SOHO20thumb_thm.png (80x40) [19.1 KB] || APPLE_TV_12952_SOHO_20th_anniversary_ws_appletv.m4v (1280x720) [199.6 MB] || YOUTUBE_HQ_12952_SOHO_20th_anniversary_ws_youtube_hq.mov (1920x1080) [2.5 GB] || 12952_SOHO_20th_anniversary_ws-H264_Best_1920x1080_59.94.mov (1920x1080) [4.0 GB] || YOUTUBE_HQ_12952_SOHO_20th_anniversary_ws_youtube_hq.webm (1920x1080) [45.1 MB] || SOHO20.en_US.srt [7.6 KB] || 12952_SOHO_20th_anniversary_ws.key [200.0 MB] || 12952_SOHO_20th_anniversary_ws.pptx [199.8 MB] || 12952_SOHO_20th_anniversary_ws_lowres.mp4 (480x272) [52.9 MB] || NASA_PODCAST_12952_SOHO_20th_anniversary_ws_ipod_sm.mp4 (320x240) [67.5 MB] || ", "hits": 44 }, { "id": 40110, "url": "https://svs.gsfc.nasa.gov/gallery/astro-galaxy/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Galaxy Listing", "description": "No description available.", "hits": 110 }, { "id": 40111, "url": "https://svs.gsfc.nasa.gov/gallery/astro-star/", "result_type": "Gallery", "release_date": "2015-09-18T00:00:00-04:00", "title": "Astrophysics Star Listing", "description": "No description available.", "hits": 155 }, { "id": 40249, "url": "https://svs.gsfc.nasa.gov/gallery/rising-seas/", "result_type": "Gallery", "release_date": "2015-08-25T00:00:00-04:00", "title": "Sea Level Rise", "description": "Earth’s seas are rising, a direct result of a changing climate. Ocean temperatures are increasing, leading to ocean expansion. And as ice sheets and glaciers melt, they add more water. A fleet of increasingly sophisticated instruments deployed by NASA across the oceans, on polar ice and in orbit, reveals significant changes among globally interlocking factors that are driving sea levels higher.", "hits": 218 }, { "id": 30582, "url": "https://svs.gsfc.nasa.gov/30582/", "result_type": "Infographic", "release_date": "2015-02-05T16:00:00-05:00", "title": "SMAP applications infographic", "description": "SMAP applications infographic || smap_inforgraphic_title_slide_print.jpg (1024x576) [234.1 KB] || smap_inforgraphic_title_slide_web.jpg (320x180) [70.5 KB] || smap_inforgraphic_title_slide_searchweb.png (320x180) [115.9 KB] || smap_inforgraphic_title_slide_thm.png (80x40) [24.6 KB] || smap_inforgraphic_title_slide.tif (5760x3240) [11.0 MB] || smap_inforgraphic_title_slide.hwshow [163 bytes] || ", "hits": 23 }, { "id": 40217, "url": "https://svs.gsfc.nasa.gov/gallery/swift/", "result_type": "Gallery", "release_date": "2014-11-18T00:00:00-05:00", "title": "Neil Gehrels Swift Observatory", "description": "NASA's Neil Gehrels Swift Observatory provides astronomers with a unique tool for exploring many different classes of astronomical phenomena, from gamma-ray bursts and supernovae to spinning neutron stars, outbursts from black holes, and even exoplanets, comets and asteroids. These pages gather together media products associated with Swift news releases.For more information about the Swift mission, visit its NASA webpage.", "hits": 727 }, { "id": 40179, "url": "https://svs.gsfc.nasa.gov/gallery/icesat2/", "result_type": "Gallery", "release_date": "2014-10-15T00:00:00-04:00", "title": "ICESat-2", "description": "The Ice, Cloud and land Elevation Satellite-2 will measure the height of Earth from space, creating a record of the planet’s elevation in unprecedented detail and precision. With high-resolution data from ICESat-2’s laser altimeter, scientists will track changes to Earth’s polar ice caps – regions that are a harbinger of warming temperatures worldwide. The mission will also take stock of forests, map ocean surfaces, track the rise of cities and measure everything in between. ICESat-2 continues key elevation observations begun by ICESat-1 (2003 to 2009) and Operation IceBridge (2009 through present), to provide a portrait of change in the beginning of the 21st century.\n\nFor more information, please visit the ICESat-2 website.", "hits": 575 }, { "id": 11499, "url": "https://svs.gsfc.nasa.gov/11499/", "result_type": "Produced Video", "release_date": "2014-03-06T14:00:00-05:00", "title": "Beta Pictoris: Icy Debris Suggests 'Shepherd' Planet", "description": "An international team of astronomers exploring the disk of gas and dust the bright star Beta Pictoris have uncovered a compact cloud of poisonous gas formed by ongoing rapid-fire collisions among a swarm of icy, comet-like bodies. The researchers suggest the comet swarm may be frozen debris trapped and concentrated by the gravity of an as-yet-unseen planet.Using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, astronomers mapped millimeter-wavelength light from dust and carbon monoxide (CO) molecules in a disk surrounding the star. Located about 63 light-years away and only 20 million years old, Beta Pictoris hosts one of the closest, brightest and youngest debris disks known, making it an ideal laboratory for studying the early development of planetary systems. The ALMA images reveal a vast belt of carbon monoxide located at the fringes of the system. Much of the gas is concentrated in a single clump located about 8 billion miles (13 billion kilometers) from the star, or nearly three times the distance between the planet Neptune and the sun. The total amount of CO observed, the scientists say, exceeds 200 million billion tons, equivalent to about one-sixth the mass of Earth’s oceans.The presence of all this gas is a clue that something interesting is going on because ultraviolet starlight breaks up CO molecules in about 100 years, much faster than the main cloud can complete a single orbit around the star. Scientists calculate that a large comet must be completely destroyed every five minutes to offset the destruction of CO molecules. Only an unusually massive and compact swarm of comets could support such an astonishingly high collision rate.The researchers think these comet swarms formed when a as-yet-undetected planet migrated outward, sweeping icy bodies into resonant orbits. When the orbital periods of the comets matched the planet's in some simple ratio – say, two orbits for every three of the planet – the comets received a nudge from the planet at the same location each orbit. Like the regular push of a child's swing, these accelerations amplify over time and work to confine the comets in a small region. || ", "hits": 258 }, { "id": 30481, "url": "https://svs.gsfc.nasa.gov/30481/", "result_type": "Infographic", "release_date": "2013-12-02T10:00:00-05:00", "title": "Heliophysics and Space Weather", "description": "The sun and its atmosphere consist of several zones, or layers, from the inner core to the outer corona. Beyond the corona is the solar wind, which is an outward expansion of coronal plasma that extends well beyond the orbit of Pluto. This entire region of space influenced by the sun is called the heliosphere. Controlled by the Earth’s magnetic field, the magnetosphere acts as a shield protecting the planet from solar wind. The shape of the Earth's magnetosphere is the direct result of being impacted by solar wind, compressed on its sunward side and elongated on the night-side, the magnetotail. The shock wave where the solar wind encounters Earth's magnetosphere is called the bow shock, which slows and diverts the solar wind. Solar activity lead to solar eruptions, which includes such phenomena as sunspots, flares, prominences, and coronal mass ejections that influence space weather, or near-Earth environmental conditions. Modern society depends heavily on a variety of technologies that are susceptible to space weather. CMEs for example can cause geomagnetic storms that can disrupt satellite communications and navigational equipment, and even cause blackouts. || ", "hits": 172 }, { "id": 40152, "url": "https://svs.gsfc.nasa.gov/gallery/maven/", "result_type": "Gallery", "release_date": "2013-11-01T00:00:00-04:00", "title": "MAVEN", "description": "NASA's Mars Atmosphere and Volatile Evolution (MAVEN) is the first mission devoted to understanding the Martian upper atmosphere. Today Mars is cold and dry, but ancient Mars was warm, wet, and possibly hospitable to life. Scientists think that the loss of Mars' early atmosphere caused the planet to dry up, and MAVEN is testing this hypothesis by observing present-day interactions of the Martian atmosphere with the solar wind. Learn more about MAVEN from\n NASA and CU Boulder.", "hits": 222 }, { "id": 40122, "url": "https://svs.gsfc.nasa.gov/gallery/mars/", "result_type": "Gallery", "release_date": "2012-06-28T00:00:00-04:00", "title": "Mars Missions and Science", "description": "This multimedia gallery assembles and organizes Mars content on the Scientific Visualization Studio website. Highlights of NASA Goddard Space Flight Center’s animations, visualizations, videos, images and graphics relating to Mars science and missions can be found here.", "hits": 393 }, { "id": 40073, "url": "https://svs.gsfc.nasa.gov/gallery/astro/", "result_type": "Gallery", "release_date": "2010-07-12T00:00:00-04:00", "title": "Goddard's Astrophysics Gallery", "description": "This multimedia gallery assembles and organizes the astrophysics content on the Scientific Visualization Studio website. All of NASA's Goddard Space Flight Center's animations, visualizations, videos and still images relating to the universe beyond our Solar System are here. Browse through the basic categories or find Goddard's most recent releases under each specific astronomical feature. Find all the content relating to a particular satellite under \"Missions.\" Most entries have multiple downloadable formats and several resolutions.", "hits": 364 }, { "id": 40238, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-themes/", "result_type": "Gallery", "release_date": "2005-09-15T12:00:00-04:00", "title": "Hyperwall Stories for specific event", "description": "The hyperwall gallery features visualizations that have been selected for use at NASA's hyperwall at event\nReturn to Main Hyperwall Gallery.", "hits": 167 } ] }