{ "count": 390, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Evolution%22", "previous": null, "results": [ { "id": 40549, "url": "https://svs.gsfc.nasa.gov/gallery/interstellar-boundary-explorer-ibex/", "result_type": "Gallery", "release_date": "2026-03-02T00:00:00-05:00", "title": "IBEX – Interstellar Boundary Explorer", "description": "The Interstellar Boundary Explorer (IBEX) is a NASA spacecraft studying how our heliosphere — the protective bubble surrounding the Sun and planets that is inflated by a constant stream of solar particles — interacts with interstellar space. IBEX created the first maps showing the interactions at that border, and how they change over time due to variations in the Sun’s activity. IBEX studies the heliosphere’s boundaries by measuring a type of uncharged particle called energetic neutral atoms.\n\nIBEX launched on Oct. 19, 2008, from the Ronald Reagan Ballistic Missile Defense Test Site, in the Republic of the Marshall Islands. \n\nLearn more: https://science.nasa.gov/mission/ibex/", "hits": 225 }, { "id": 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": 280 }, { "id": 14884, "url": "https://svs.gsfc.nasa.gov/14884/", "result_type": "Produced Video", "release_date": "2026-01-29T11:00:00-05:00", "title": "NASA Supercomputer Probes Tangled Magnetospheres of Merging Neutron Stars", "description": "New supercomputer simulations explore the tangled magnetic structures around merging neutron stars. These structures, called magnetospheres, interact as the city-sized stars enter their final orbits. Magnetic field lines can connect both stars, break, and reconnect, while currents surge through surrounding plasma moving at nearly the speed of light. The simulations show that these systems may produce X-rays and gamma rays that future observatories should be able to detect. Credit: NASA’s Goddard Space Flight CenterAlt text: Narrated video introducing simulations of merging neutron star magnetospheresMusic: “A Theory Develops,” Pip Heywood [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NS_Binary_Sim_Still.jpg (5760x3240) [1.4 MB] || NS_Binary_Sim_Still_searchweb.png (320x180) [67.6 KB] || NS_Binary_Sim_Still_thm.png (80x40) [5.2 KB] || 14884_NeutronStarBinarySim2_good.mp4 (1920x1080) [220.4 MB] || 14884_NeutronStarBinarySim2_best.mp4 (1920x1080) [363.9 MB] || NeutronStarBinarySimulationCaptions.en_US.srt [2.4 KB] || NeutronStarBinarySimulationCaptions.en_US.vtt [2.2 KB] || 14884_NeutronStarBinarySim2_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || ", "hits": 448 }, { "id": 20411, "url": "https://svs.gsfc.nasa.gov/20411/", "result_type": "Animation", "release_date": "2026-01-14T10:00:00-05:00", "title": "A Pathway to Protocells on Titan – Animations", "description": "These animations illustrate how simple protocells could form in the lakes of Titan, Saturn’s largest moon. When rain falls from Titan’s methane clouds into its hydrocarbon lakes, it can transport organic molecules like acrylonitrile that are attracted to both water and oil. Such amphiphile molecules are likely to collect in a thin film on the surface of Titan’s lakes. As large raindrops pelt the lakes, they could stir up this floating “pond scum” to form spherical droplets of methane coated in a bilayer of amphiphiles – structures called vesicles that resemble cell membranes on Earth.Although such vesicles have yet to be detected on Titan, a 2025 study by Christian Mayer and NASA scientist Conor Nixon lays out the process for their formation and evolution, and it proposes a mechanism for their discovery by a future mission to Titan. The paper also proposes that different mixtures of amphiphiles could stabilize vesicles and lead to the evolution of simple protocells on Titan. || ", "hits": 330 }, { "id": 14937, "url": "https://svs.gsfc.nasa.gov/14937/", "result_type": "Produced Video", "release_date": "2025-12-23T11:00:00-05:00", "title": "NASA's Roman Space Telescope: Widening Our Gaze", "description": "The NASA Astrophysics fleet of spacecraft has an impressive range of capabilities. What is the next step in exploring the cosmos? The Nancy Grace Roman Space Telescope, NASA’s upcoming flagship mission, will take Hubble’s resolution and widen its infrared view to more than 100 times the coverage in every single image. Roman is a survey telescope that can peer through the Milky Way’s obscuring dust, and see faint, distant galaxies. Roman’s rigid design allows it to scan large regions of sky very quickly. Hubble would take 1,000 years to observe what Roman can see in one. Roman’s 18 4k x 4k detectors create 300-megapixel images covering an area of sky slightly larger than the full Moon. Roman will also look at the same regions of space repeatedly over time, allowing astronomers to see changes and observe temporary events like supernovae. Roman’s surveys of deep space and the center of our Milky Way galaxy will find thousands of new exoplanets, survey millions of galaxies, help us understand dark matter and dark energy, and learn more about the evolution of the universe. || ", "hits": 366 }, { "id": 14932, "url": "https://svs.gsfc.nasa.gov/14932/", "result_type": "Produced Video", "release_date": "2025-12-02T08:00:00-05:00", "title": "Bio-Essential Sugars Discovered in Samples from Asteroid Bennu", "description": "OSIRIS-REx Project Scientist Daniel Glavin discusses the discovery of ribose and glucose in samples of asteroid Bennu, and the implications for the formation and evolution of life on Earth.Complete transcript available.Watch this video on the NASA.gov Video YouTube channel. || Bennu-Sugars-Thumbnail_print.jpg (1024x576) [175.2 KB] || Bennu-Sugars-Thumbnail.jpg (1280x720) [534.2 KB] || Bennu-Sugars-Thumbnail.png (1280x720) [892.3 KB] || Bennu-Sugars-Thumbnail_searchweb.png (320x180) [77.4 KB] || Bennu-Sugars-Thumbnail_thm.png (80x40) [6.8 KB] || 14932_Bennu_Sugars_Interview_Glavin_720.mp4 (1280x720) [180.6 MB] || 14932_Bennu_Sugars_Interview_Glavin_1080.mp4 (1920x1080) [1011.6 MB] || BennuSugarsGlavinCaptionsV2.en_US.srt [18.4 KB] || BennuSugarsGlavinCaptionsV2.en_US.vtt [17.5 KB] || 14932_Bennu_Sugars_Interview_Glavin_4K.mp4 (3840x2160) [6.2 GB] || 14932_Bennu_Sugars_Interview_Glavin_ProRes.mov (3840x2160) [47.0 GB] || ", "hits": 254 }, { "id": 14920, "url": "https://svs.gsfc.nasa.gov/14920/", "result_type": "Produced Video", "release_date": "2025-11-13T12:00:00-05:00", "title": "Preparing for Martian Explorers: NASA's ESCAPADE Investigates Mars Space Weather", "description": "NASA’s new ESCAPADE mission is launching to Mars to help us better understand the Sun’s influence on Mars’ past and present. Its work could help protect future human explorers from potentially dangerous space weather when they set foot on the Red Planet.For the first time, the 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. Its observations will reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE orbiters build on earlier Mars missions, such as NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) orbiter. The MAVEN mission has one spacecraft that has been studying Mars’ atmospheric loss since arriving at the Red Planet in 2014.ESCAPADE is scheduled to launch no earlier than fall 2025 from Cape Canaveral Space Force Station Launch Complex 36 in Florida.Find out more about the ESCAPADE mission: https://science.nasa.gov/mission/escapade/ || ", "hits": 155 }, { "id": 14906, "url": "https://svs.gsfc.nasa.gov/14906/", "result_type": "Produced Video", "release_date": "2025-09-30T15:00:00-04:00", "title": "Evolution of a Sun-Like Star", "description": "As a star ages, its spin and the number and sizes of its spots decreases as shown in this animation of a Sun-like star. Star spots are tied to local magnetic fields that have been amplified by the star’s rotation, so the phenomena are connected.A version without labels is available for download.Credit: NASA’s Goddard Space Flight Center || ThreeStars_Still.jpg (3840x2160) [586.8 KB] || ThreeStars_Still.png (3840x2160) [3.4 MB] || ThreeStars_Still_searchweb.png (320x180) [65.9 KB] || ThreeStars_Still_thm.png (80x40) [6.3 KB] || 14906_ThreeStars_NoText_1080.mp4 (1920x1080) [53.6 MB] || 14906_ThreeStars_1080.mp4 (1920x1080) [53.8 MB] || 14906_ThreeStars_4k.mp4 (3840x2160) [178.6 MB] || 14906_ThreeStars_NoText_4k.mp4 (3840x2160) [178.3 MB] || 14906_ThreeStars_NoText_ProRes_3840x2160_2997.mov (3840x2160) [1.8 GB] || 14906_ThreeStars_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || ", "hits": 342 }, { "id": 14886, "url": "https://svs.gsfc.nasa.gov/14886/", "result_type": "Produced Video", "release_date": "2025-08-22T11:00:00-04:00", "title": "Artemis Science: Exploring the Moon’s South Pole", "description": "By sending astronauts to collect samples from the Moon’s South Pole, NASA’s Artemis missions may uncover clues to the formation of the solar system.Complete transcript available.Universal Production Music: “Transitions” by Harry Gregson Williams [BMI] and Ben Andrew [PRS]; “Love on the Moon” by Sebastian Barnaby Robertson [BMI] and Yaacov Kobi Hokima [BMI]Watch this video on the NASA Goddard YouTube channel. || Artemis_Sci_Young_S_Pole_Preview_print.jpg (1024x576) [139.2 KB] || Artemis_Sci_Young_S_Pole_Preview.jpg (1920x1080) [721.6 KB] || Artemis_Sci_Young_S_Pole_Preview.png (1920x1080) [1.5 MB] || Artemis_Sci_Young_S_Pole_Preview_searchweb.png (320x180) [84.1 KB] || Artemis_Sci_Young_S_Pole_Preview_thm.png (80x40) [6.7 KB] || 14886_Artemis_Sci_Young_SPole_720.mp4 (1280x720) [37.3 MB] || 14886_Artemis_Sci_Young_SPole_1080.mp4 (1920x1080) [208.1 MB] || ArtemisSciYoungSPoleCaptions.en_US.srt [4.0 KB] || ArtemisSciYoungSPoleCaptions.en_US.vtt [3.8 KB] || 14886_Artemis_Sci_Young_SPole_4K.mp4 (3840x2160) [1.3 GB] || 14886_Artemis_Sci_Young_SPole_ProRes.mov (3840x2160) [7.4 GB] || ", "hits": 1499 }, { "id": 14874, "url": "https://svs.gsfc.nasa.gov/14874/", "result_type": "Produced Video", "release_date": "2025-07-28T10:00:00-04:00", "title": "STORIE Thermal Vacuum Test at NASA Goddard Space Flight Center", "description": "NASA’s STORIE mission, or Storm Time O+ Ring current Imaging Evolution, has completed its design, build, and testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its six-month mission onboard the International Space Station (ISS). From its unique vantage point on the ISS, STORIE will use its onboard neutral atom imager to provide an “inside out” view of Earth’s ring current – a region of the magnetosphere where energetic particles are trapped in near-Earth space. In addition to answering fundamental questions about the ring current’s intensity and composition, STORIE will also provide a more detailed understanding of how geomagnetic storms affect Earth.From NASA’s Goddard Space Flight Center, STORIE will be shipped to NASA’s Johnson Space Center in Houston, Texas, where it will be integrated onto a pallet to be installed outside the ISS’s Columbus Module. STORIE will head to the ISS aboard a SpaceX commercial resupply flight no earlier than spring 2026. || ", "hits": 112 }, { "id": 14869, "url": "https://svs.gsfc.nasa.gov/14869/", "result_type": "Produced Video", "release_date": "2025-07-18T11:00:00-04:00", "title": "STORIE Fit Test at NASA Goddard Space Flight Center", "description": "NASA’s STORIE mission, or Storm Time O+ Ring current Imaging Evolution, has completed its design, build, and testing campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, ahead of its mission onboard the International Space Station (ISS). From its unique vantage point on the ISS, STORIE will use neutral atom imaging to provide an “inside out” view of Earth’s ring current – a region of the magnetosphere where energetic particles are trapped in near-Earth space. In addition to answering fundamental questions about the ring current’s intensity and composition, STORIE will also provide a more detailed understanding of how geomagnetic storms affect Earth.From NASA’s Goddard Space Flight Center, STORIE will be shipped to NASA’s Johnson Space Center in Houston, Texas, where it will be integrated onto a pallet to be installed outside the ISS’s Columbus Module. STORIE will head to the ISS aboard a SpaceX commercial resupply flight no earlier than spring 2026. || ", "hits": 30 }, { "id": 14863, "url": "https://svs.gsfc.nasa.gov/14863/", "result_type": "Produced Video", "release_date": "2025-07-17T09:00:00-04:00", "title": "Quickshot: New NASA Mission Launching Soon To Study Earth’s Space Weather Shield", "description": "Scroll down page for advisory with suggested questions and anchor intro. You will also find the associated cut b-roll and pre-recorded soundbites below.Click here for more information about TRACERS || Live_Shot_Banner_TRACERS_final.jpg (1800x720) [256.8 KB] || Live_Shot_Banner_TRACERS_final_print.jpg (1024x409) [150.1 KB] || Live_Shot_Banner_TRACERS_final_searchweb.png (320x180) [82.8 KB] || Live_Shot_Banner_TRACERS_final_thm.png (80x40) [6.5 KB] || ", "hits": 78 }, { "id": 14866, "url": "https://svs.gsfc.nasa.gov/14866/", "result_type": "Produced Video", "release_date": "2025-07-15T00:00:00-04:00", "title": "Cosmic Desktop & Phone Wallpapers", "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||", "hits": 30501 }, { "id": 5543, "url": "https://svs.gsfc.nasa.gov/5543/", "result_type": "Visualization", "release_date": "2025-06-11T10:00:00-04:00", "title": "Solar Magnetic Field - from Solar Minimum to Solar Maximum", "description": "Visualizations of the solar magnetic field evolution as a potential-field-source-surface model (PFSS) from solar minimum (2019) to solar maximum (2025).", "hits": 185 }, { "id": 14846, "url": "https://svs.gsfc.nasa.gov/14846/", "result_type": "Produced Video", "release_date": "2025-05-29T11:00:00-04:00", "title": "Is This How Mars Lost Its Atmosphere?", "description": "Mars is losing its atmosphere. Over billions of years, the Red Planet has transformed from a potentially habitable world with lakes, rivers, and a thicker atmosphere into the cold, dry desert we see today. NASA’s MAVEN mission has been tracking this process in real time, catching Mars in the act of slowly sputtering its atmosphere into space.This phenomenon—called “atmospheric sputtering”—happens when high-energy particles from the Sun slam into Mars’s upper atmosphere, knocking atoms and molecules loose. Without a global magnetic field to protect it, Mars is especially vulnerable. MAVEN has shown that this atmospheric escape accelerates during solar storms, offering a powerful view of how the Sun shapes the evolution of planetary atmospheres.The data from MAVEN doesn’t just tell us about Mars—it helps us understand how atmospheres behave across the solar system and beyond. It’s a glimpse into what makes a planet stay habitable—or lose that potential entirely.For more information, visit https://science.nasa.gov/mission/maven/Credit: NASA's Goddard Space Flight Center Dan Gallagher: Lead ProducerPaul Morris: Producer / EditorDr. Shannon Curry: Scientist / IntervieweeWillow Reed: Public AffairsNancy Jones: Public AffairsGreg Shirah: Data VisualizerCindy Starr: Data VisualizerKel Elkins: Data VisualizerWalt Feimer: AnimatorMichael Lentz: AnimatorChris Smith: AnimatorJonathan North: AnimatorBrian Monroe: AnimatorLisa Poje: Graphic DesignerAdriana Manrique Gutierrez: Graphic DesignerKim Dongjae: Graphic DesignerErnie Wright: SupportAaron E. Lepsch: Technical SupportMusic Credit:\"The Greatest Unknown\" by Samuel Sim [PRS] via Abbey Road Masters [PRS] and Universal Production MusicVideo Credits:Periodic Table Focusing On Argon With Properties by S_D_Brath via Pond5Ashes Of A Camp Fire Next To Chair by BlackBoxGuild via Pond5Wood Burning In A Camp Fire by Edb3_16 via Pond5 || ", "hits": 1063 }, { "id": 31349, "url": "https://svs.gsfc.nasa.gov/31349/", "result_type": "Hyperwall Visual", "release_date": "2025-05-28T18:59:59-04:00", "title": "Juno images, 2024 - early 2025", "description": "Several recent images from the JunoCam and Jovian Infrared Auroral Mapper (JIRAM) instruments show volcanic hot spots on IO, polar storms and Jupiter's moon Amalthea.", "hits": 380 }, { "id": 14797, "url": "https://svs.gsfc.nasa.gov/14797/", "result_type": "Produced Video", "release_date": "2025-05-27T20:55:00-04:00", "title": "Exoplanets Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to the topic of exoplanets.", "hits": 64 }, { "id": 20403, "url": "https://svs.gsfc.nasa.gov/20403/", "result_type": "Animation", "release_date": "2025-05-14T09:00:00-04:00", "title": "Titan science results from James Webb Space Telescope: animation resource page", "description": "Push into JWST to Saturn and Titan. || JWST_Titan_Intro_Final_V001.00957_print.jpg (1024x576) [145.8 KB] || JWST_Titan_Intro_Final_V001.00957_searchweb.png (320x180) [78.0 KB] || JWST_Titan_Intro_Final_V001.00957_thm.png [5.5 KB] || JWST_Titan_Intro_Final_1080.mp4 (1920x1080) [72.8 MB] || JWST_Titan_Intro_Final_V001.mp4 (3840x2160) [38.4 MB] || JWST_Titan_Intro_Final_V001.mov (3840x2160) [6.8 GB] || ", "hits": 147 }, { "id": 14819, "url": "https://svs.gsfc.nasa.gov/14819/", "result_type": "Produced Video", "release_date": "2025-05-06T10:45:00-04:00", "title": "NASA's NICER Studies Recurring Cosmic Crashes", "description": "Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" by Lee Groves [PRS] and Peter Geogre Marett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_thumbnail_NICER_QPE.jpg (1280x720) [225.7 KB] || YTframe_thumbnail_NICER_QPE_searchweb.png (320x180) [95.5 KB] || YTframe_thumbnail_NICER_QPE_thm.png [8.7 KB] || 14819_NICER_QPE_Good.mp4 (1920x1080) [70.6 MB] || 14819_NICER_QPE_Best.mp4 (1920x1080) [172.3 MB] || 14819_NICER_QPE_Captions.en_US.srt [2.8 KB] || 14819_NICER_QPE_Captions.en_US.vtt [2.7 KB] || 14819_NICER_QPE_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ", "hits": 140 }, { "id": 14802, "url": "https://svs.gsfc.nasa.gov/14802/", "result_type": "Produced Video", "release_date": "2025-03-28T14:31:59-04:00", "title": "Earth to Space: A National Symphony Orchestra Concert", "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.", "hits": 117 }, { "id": 20398, "url": "https://svs.gsfc.nasa.gov/20398/", "result_type": "Animation", "release_date": "2025-03-19T11:00:00-04:00", "title": "Habitable Worlds Observatory (HWO) EAC 2 Design Animations", "description": "Animations and stills of design concept EAC 2 for the Habitable Worlds Observatory", "hits": 102 }, { "id": 14790, "url": "https://svs.gsfc.nasa.gov/14790/", "result_type": "Produced Video", "release_date": "2025-03-04T10:55:00-05:00", "title": "Hubble Finds Possible Triple System 3.7 Billion Miles Away", "description": "Today, we dive into the mysteries of the Kuiper Belt, home to thousands of icy remnants from the early solar system. Among these objects, scientists have cataloged over 3,000, yet they estimate there could be hundreds of thousands more, each spanning more than 10 miles in diameter, with Pluto being the most famous.Recent research using data from the Keck Observatory and NASA’s Hubble Space Telescope has revealed a potential three-body system in the Kuiper Belt, known as the Altjira system. This discovery challenges traditional collision theories by suggesting that these triple systems might form directly from the gravitational collapse of material in the early solar disk.The Altjira system, located roughly 3.7 billion miles away, demonstrates how even the most distant and faint objects can yield groundbreaking insights when observed over decades. Join us as we explore how these long-term observations are reshaping our understanding of the solar system’s formation and evolution.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerMusic Credit:“Dark Reflection” by Peter William Hall [PRS], via Ninja Tune Production Music [PRS] and Universal Production Music. || ", "hits": 44 }, { "id": 5495, "url": "https://svs.gsfc.nasa.gov/5495/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M7.4 flare from Active Region 13964 - January 17, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13964 (in the upper right quadrant of the disk) launch an M7.4 flare followed by some complex post-flare evolution.", "hits": 10 }, { "id": 14762, "url": "https://svs.gsfc.nasa.gov/14762/", "result_type": "Produced Video", "release_date": "2025-01-16T14:15:00-05:00", "title": "2.5 Billion Pixel Image of Galaxy Shot by Hubble", "description": "The Andromeda galaxy holds over 1 trillion stars and has been a key to unlocking the secrets of the universe. Thanks to NASA’s Hubble Space Telescope, we’re now seeing Andromeda in stunning new detail, revealing its dynamic history and unique structure.Recent Hubble surveys mapped the galaxy’s entire disk—an effort spanning a decade and over 1,000 orbits—showing everything from young stars to remnants of past galactic collisions. Learn how new information about Andromeda is reshaping our understanding of galactic evolution and what it reveals about the fate of our own galaxy. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerMusic Credit:“Vitava From Ma Vlast \"My Country\"” by Bedrich Smetana [PD] and Robert J Walsh [BMI], via First Digital Music [BMI] and Universal Production Music. || ", "hits": 455 }, { "id": 14753, "url": "https://svs.gsfc.nasa.gov/14753/", "result_type": "Produced Video", "release_date": "2025-01-13T10:14:00-05:00", "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole", "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ", "hits": 177 }, { "id": 14750, "url": "https://svs.gsfc.nasa.gov/14750/", "result_type": "Produced Video", "release_date": "2025-01-10T10:00:00-05:00", "title": "NASA to Study the Moon’s Interior", "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Human Behaviour\" and \"Overview Effect\" from Jan Telegra of Universal Production Music. || YT_THUMB_LMS.jpg (1280x720) [171.6 KB] || CLPS_MAIN_LMS_FINAL.01682_searchweb.png (320x180) [63.2 KB] || CLPS_MAIN_LMS_FINAL.mp4 (1440x1080) [22.5 MB] || CLPS_MAIN_LMS_socialversion.mp4 (1440x1080) [27.4 MB] || CLPS_MAIN_LMS.en_US.srt [2.5 KB] || CLPS_MAIN_LMS.en_US.vtt [2.4 KB] || CLPS_MAIN_LMS_FINAL.01682_thm.png [5.2 KB] || ", "hits": 190 }, { "id": 5423, "url": "https://svs.gsfc.nasa.gov/5423/", "result_type": "Visualization", "release_date": "2024-11-27T11:00:00-05:00", "title": "Gravity waves disturbing the stratospheric polar vortex", "description": "Animation 1: Changes in temperature and height on the surface of 850 Kelvin potential temperature. The mountain generated gravity waves create strong cooling  as the gravity waves propagate through the stratosphere, while the polar vortex (the cold blue ring) evolves to become colder. || stratospher850_039_T.02498_print.jpg (1024x576) [108.0 KB] || stratospher850_039_T.02498_searchweb.png (320x180) [50.4 KB] || stratospher850_039_T.02498_thm.png (80x40) [4.2 KB] || stratospher850_039_T_1080p30.mp4 (1920x1080) [52.0 MB] || stratospher850_039_T [0 Item(s)] || stratospher850_039_T.mp4 (3840x2160) [148.7 MB] || stratospher850_039_T.mp4.hwshow || ", "hits": 105 }, { "id": 20394, "url": "https://svs.gsfc.nasa.gov/20394/", "result_type": "Animation", "release_date": "2024-11-12T15:00:00-05:00", "title": "Habitable Worlds Observatory (HWO) Animations and Stills", "description": "This page contains artist's concept computer renderings of a current possible design for the Habitable Worlds Observatory. HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ", "hits": 210 }, { "id": 20395, "url": "https://svs.gsfc.nasa.gov/20395/", "result_type": "Animation", "release_date": "2024-11-12T15:00:00-05:00", "title": "Habitable Worlds Observatory Additional Spacecraft Designs", "description": "The Habitable Worlds Observatory is early in its development. Many designs are under consideration. These artist's concept animations show some of the options.HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ", "hits": 285 }, { "id": 5344, "url": "https://svs.gsfc.nasa.gov/5344/", "result_type": "Visualization", "release_date": "2024-10-15T14:00:00-04:00", "title": "Solar Cycle 25 - the Solar Magnetic Field from Solar Minimum to Pole Flip", "description": "One advantage of long-lived missions like Solar Dynamics Observatory (SDO) is the ability to see slow but significant changes over long periods of time.This view from SDO's Helioseismic and Magnetic Imager (HMI) shows the evolution of sunspots on the solar disk starting from solar minimum (around December 2019) and into the maximum solar activity phase. The video ends in September 2024, however this maximum phase is expected to continue into 2025.", "hits": 561 }, { "id": 40525, "url": "https://svs.gsfc.nasa.gov/gallery/habitable-worlds-observatory/", "result_type": "Gallery", "release_date": "2024-10-01T00:00:00-04:00", "title": "Habitable Worlds Observatory", "description": "The Habitable Worlds Observatory is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.\n\nHabitable Worlds will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.\n\nThis future space observatory will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter and the evolution of cosmic structure.\n\nThe Habitable Worlds Observatory will build on the technological foundations of the Hubble, Webb and Roman Space Telescopes, uniting government, industry, academia, and international partners.", "hits": 293 }, { "id": 14690, "url": "https://svs.gsfc.nasa.gov/14690/", "result_type": "Produced Video", "release_date": "2024-09-23T14:00:00-04:00", "title": "Ten Years at Mars with NASA’s MAVEN Mission", "description": "During its first decade at Mars, MAVEN has helped to explain how the Red Planet evolved from warm and wet into the cold, dry world we see today. Complete transcript available.Universal Production Music: “Executive Deceit” by Samuel Karl Bohn [PRS], Chalk Music [PRS]; “Quasar” by Ross Stephen Gilmartin [PRS], Chappell Recorded Music Library Ltd [PRS]; “Modular Odyssey” and “Synthology” by Laetitia Frenod [SACEM], Koka Media [SACEM]Watch this video on the NASA Goddard YouTube channel. || MAVEN-10th-Anniversary-Preview_print.jpg (1024x576) [160.7 KB] || MAVEN-10th-Anniversary-Preview.jpg (1280x720) [622.5 KB] || MAVEN-10th-Anniversary-Preview.png (1280x720) [1.2 MB] || MAVEN-10th-Anniversary-Preview_searchweb.png (320x180) [80.6 KB] || MAVEN-10th-Anniversary-Preview_thm.png (80x40) [6.3 KB] || 14690_MAVEN_10th_Anniversary_720.mp4 (1280x720) [92.2 MB] || 14690_MAVEN_10th_Anniversary_1080.mp4 (1920x1080) [516.6 MB] || Maven10thAnniversaryCaptionsV3.en_US.srt [8.9 KB] || Maven10thAnniversaryCaptionsV3.en_US.vtt [8.5 KB] || 14690_MAVEN_10th_Anniversary_4K.mp4 (3840x2160) [6.3 GB] || 14690_MAVEN_10th_Anniversary_ProRes.mov (3840x2160) [36.5 GB] || ", "hits": 151 }, { "id": 14672, "url": "https://svs.gsfc.nasa.gov/14672/", "result_type": "Produced Video", "release_date": "2024-09-05T09:55:00-04:00", "title": "Hubble Helps Solve The Mystery of Mars’ Escaping Water", "description": "Mars was once a very wet planet. Scientists know that over the last 3 billion years, some of the water went underground, but what happened to the rest? Now, NASA’s Hubble Space Telescope and the Mars Atmosphere and Volatile Evolution (MAVEN) mission are helping unlock that mystery. To understand how much water there was and what happened to it, scientists need to understand how the atoms escape into space. A team combined data from Hubble and MAVEN to measure the current rate of these atoms escaping into space. This information allowed them to extrapolate the escape rate backwards through time to understand the history of water on the Red Planet.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerDan Gallagher: Producer for Assorted Mars AnimationsMusic Credit:\"Cosmic Overture\" by Sergey Azbel [BMI] via Nova Production Music Ltd [PRS], and Universal Production Music. || ", "hits": 56 }, { "id": 40523, "url": "https://svs.gsfc.nasa.gov/gallery/escapade/", "result_type": "Gallery", "release_date": "2024-09-04T00:00:00-04:00", "title": "ESCAPADE – Escape and Plasma Acceleration and Dynamics Explorer", "description": "Using two identical spacecraft in orbit around Mars, the Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will investigate how a stream of charged particles from the Sun called 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 will use its twin orbiters to 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 ESCAPADE will provide new insight into the evolution of Mars’ climate, helping to understand how Mars began losing its atmosphere and water.\n\nESCAPADE launched on Nov. 13, 2025, from NASA’s Kennedy Space Center in Florida and is expected to reach Mars in September 2027.\n\nLearn more: https://science.nasa.gov/mission/escapade/ ", "hits": 300 }, { "id": 5337, "url": "https://svs.gsfc.nasa.gov/5337/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An M5.0 flare from Active Region 13743 - and an Earth Eclipse - July 17, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13743 launches an M5.0 flare on July 17, 2024. Moments later, the Sun was eclipsed by Earth from SDO so we don't get to enjoy much of the post-flare evolution. SDO's geosynchronous orbit around Earth enables the Sun to occasionally be eclipsed by Earth (Eclipse Season Starts for NASA's SDO). For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 9 }, { "id": 14628, "url": "https://svs.gsfc.nasa.gov/14628/", "result_type": "Produced Video", "release_date": "2024-08-28T11:30:00-04:00", "title": "Discovering Earth’s Third Global Energy Field", "description": "High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed – until now.In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission, and this is its story.To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/ || ", "hits": 374 }, { "id": 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": 67 }, { "id": 14663, "url": "https://svs.gsfc.nasa.gov/14663/", "result_type": "Produced Video", "release_date": "2024-08-23T00:00:00-04:00", "title": "Take a Tour of the Horsehead Nebula", "description": "Dr. Macarena Garcia Marin presents the latest JWST images of the Horsehead Nebula, showcasing the intricate details and structures that were previously unseen. These new observations offer deeper insights into the formation and evolution of this iconic nebula, enriching our understanding of stellar nurseries. The discussion also highlights the scientific significance of these findings, bringing complex astrophysical concepts into clearer focus.For more information, visit https://webb.nasa.gov/. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Thaddeus Cesari: ScriptImage Credits:NASA/Webb, CSA, ESA, ESA/Euclid, Euclid Consortium, ESO, Digitized Sky Survey 2, N. Bartmann (ESA/Webb), E. Slawik, N. Risinger, D. De Martin, M. Zamani (ESA/Webb), K. Misselt (University of Arizona) and A. Abergel (IAS/University Paris-Saclay, CNRS)Music Credit:\"One Way Journey\" by Timothy James Cornick [PRS] and Matthew Jacob Loveridge [PRS] via BBC Production Music [PRS], and Universal Production Music. || ", "hits": 28 }, { "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": 42 }, { "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": 45 }, { "id": 14652, "url": "https://svs.gsfc.nasa.gov/14652/", "result_type": "Produced Video", "release_date": "2024-08-15T17:00:00-04:00", "title": "Exploring Volcanoes with NASA’s GEODES Team", "description": "Enjoy this music video of NASA’s GEODES team exploring lunar-like landscapes.Complete transcript available.Music credit: “Aerial” by Ben Cosgrove” and \"Volcano\" by Ben Cosgrove. Used with permission from the artist.Watch this video on the NASA Goddard YouTube channel. || ExploringVolcanoes_Thumbnail_print.jpg (1024x576) [185.0 KB] || ExploringVolcanoes_Thumbnail.png (1280x720) [1.2 MB] || ExploringVolcanoes_Thumbnail_searchweb.png (320x180) [106.5 KB] || ExploringVolcanoes_Thumbnail_thm.png (80x40) [8.4 KB] || ExploringVolcanoes_720.mp4 (1280x720) [67.0 MB] || EXPLORING_VOLCANOES_Captions_Final.en_US.srt [2.1 KB] || EXPLORING_VOLCANOES_Captions_Final.en_US.vtt [2.0 KB] || ExploringVolcanoes.mp4 (1920x1080) [471.1 MB] || ", "hits": 52 }, { "id": 14645, "url": "https://svs.gsfc.nasa.gov/14645/", "result_type": "Produced Video", "release_date": "2024-08-08T09:55:00-04:00", "title": "Hubble’s Inside the Image: Cat's Eye Nebula", "description": "NASA's Hubble Space Telescope has captured a stunning image of the Cat's Eye Nebula, one of the most complex planetary nebulae known, with its intricate structure of concentric rings and high-density knots.In this video, Dr. Ken Carpenter delves into the beauty of this cosmic jewel and discusses the critical role Hubble plays in unraveling the secrets of stellar evolution and the lifecycle of stars.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer, Director & Editor: James LeighDirector of Photography: James BallExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope Animation:ESA/Hubble - M. Kornmesser & L. L. ChristensenMusic Credits:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music\"The Search\" by Northern Points via PREMIUM BEAT BY SHUTTERSTOCK || ", "hits": 74 }, { "id": 31303, "url": "https://svs.gsfc.nasa.gov/31303/", "result_type": "Hyperwall Visual", "release_date": "2024-08-06T00:00:00-04:00", "title": "25 Images for Chandra's 25th: 25 Images to Celebrate!", "description": "25 images from 25 years, still image || 25th-chandra-hw_print.jpg (1024x576) [248.2 KB] || 25th-chandra-hw.png (5760x3240) [16.0 MB] || 25th-chandra-hw_searchweb.png (320x180) [92.1 KB] || 25th-chandra-hw_thm.png (80x40) [12.7 KB] || 25-images-to-celebrate-chandras-25th.hwshow [290 bytes] || ", "hits": 85 }, { "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": 54 }, { "id": 14607, "url": "https://svs.gsfc.nasa.gov/14607/", "result_type": "Produced Video", "release_date": "2024-07-10T10:55:00-04:00", "title": "Hubble Finds New Evidence for Intermediate-Mass Black Hole in Omega Centauri", "description": "Intermediate-mass black holes are a long-sought “missing link” in black hole evolution. They are smaller than the supermassive black holes that lie at the cores of large galaxies, but larger than stellar-mass black holes formed by the collapse of massive stars. Only a few candidates have been found to date. Now, a team of astronomers analyzed over 500 images from 20 years of NASA's Hubble Space Telescope observations to find evidence of an intermediate-mass black hole by tracking seven fast-moving stars in the Omega Centauri globular star cluster.Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. From the motions of the stars, they estimate it has a mass of at least 8,200 times that of our Sun, the mass range for an Intermediate-Mass Black Hole is between 100 and 100,000 solar masses, therefore the only object that can be so massive is a black hole. For more information, visit https://nasa.gov/hubble. Music Credit:\"A Simpler Time\" by Oskari Nurminen [ASCAP] via Universal Publishing Prod. Music Nordic [STIM], and Universal Production Music. || ", "hits": 64 }, { "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": 58 }, { "id": 14575, "url": "https://svs.gsfc.nasa.gov/14575/", "result_type": "Produced Video", "release_date": "2024-04-26T13:30:00-04:00", "title": "Moving Roman - Propulsion", "description": "Moving Roman: Propulsion. Fuel is a finite resource for NASA's Nancy Grace Roman Space Telescope. Watch this video to learn more about how the tanks for propellent are installed and why they are an essential part of the mission.Credit: NASA's Goddard Space Flight Center.Music Credits: Univeral Production Music: \"Black Nebula\" by Thomas Daniel Bellingham\"Maelstrom Dream\" by Lucie Rose\"Evolution of Life\" by David Stephen Goldsmith\"Maximist\" by Michael Blainey\"Greatness Takes Time\" by Beth Perry and Chris Doney\"Asthma inhaler\" by natty23\"Compressed Air\" by thompsonmanWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Moving_Roman_-_Propulsion-Thumbnail.jpg (1280x720) [979.8 KB] || Moving_Roman_-_Propulsion-Thumbnail_searchweb.png (320x180) [120.8 KB] || Moving_Roman_-_Propulsion-Thumbnail_thm.png (80x40) [8.2 KB] || Moving_Roman_-_Propulsion_1080.mp4 (1920x1080) [727.4 MB] || Moving_Roman_-_Propulsion-4k.webm (3840x2160) [78.9 MB] || Moving_Roman_-_Propulsion.en_US.srt [4.4 KB] || Moving_Roman_-_Propulsion.en_US.vtt [4.2 KB] || Moving_Roman_-_Propulsion-4k.mp4 (3840x2160) [720.5 MB] || Moving_Roman_-_Propulsion4k.mp4 (3840x2160) [2.4 GB] || Moving_Roman_-_Propulsion_ProRes.mov (3840x2160) [16.6 GB] || ", "hits": 59 }, { "id": 14498, "url": "https://svs.gsfc.nasa.gov/14498/", "result_type": "Produced Video", "release_date": "2024-01-11T11:05:00-05:00", "title": "Finding A New Galactic 'Fossil'", "description": "Some 5 million years ago, a black hole eruption in the galaxy NGC 4945 set off a star-formation frenzy and shot a vast cloud of gas into intergalactic space. Watch and learn how two X-ray telescopes revealed the story.Music Credits: Universal Production Music\"Planetary Horizons\" by Jia Lee\"Eyes Peeled\" by Bard\"Sprinkle of Mischief\" by Ash and HaroldWatch this video on the NASA Goddard YouTube channel.Credit: NASA’s Goddard Space Flight Center", "hits": 124 }, { "id": 5200, "url": "https://svs.gsfc.nasa.gov/5200/", "result_type": "Visualization", "release_date": "2023-12-11T12:00:00-05:00", "title": "Mars Disappearing Solar Wind: MAVEN Visualizations", "description": "This data visualization depicts a period of decreased solar wind at Mars that occurred on December 25, 2022, causing the planet’s magnetosphere to expand outward. Ion velocity and density data collected by the MAVEN spacecraft is presented using a color-mapped satellite orbit tail and vectors along MAVEN’s orbit. || maven_solar_wind_comp.02715_print.jpg (1024x576) [84.4 KB] || maven_solar_wind_comp.02715_searchweb.png (320x180) [47.3 KB] || maven_solar_wind_comp.02715_thm.png (80x40) [4.3 KB] || maven_solar_wind_comp (3840x2160) [0 Item(s)] || maven_solar_wind_comp_2160p60.mp4 (3840x2160) [187.6 MB] || maven_solar_wind_comp_prores.mov (3840x2160) [10.1 GB] || ", "hits": 271 }, { "id": 14477, "url": "https://svs.gsfc.nasa.gov/14477/", "result_type": "Produced Video", "release_date": "2023-12-11T12:00:00-05:00", "title": "The Day the Solar Wind Disappeared from Mars", "description": "Learn about the “disappearance” of the solar wind at Mars that was witnessed by MAVEN – an event last seen nearly a quarter-century ago at Earth.Complete transcript available.Universal Production Music: “Space Museum” by Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]; “Currents and Crime Scenes” by Dylan Matthew Love and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || MAVEN_Solar_Wind_Disappear_V4_print.jpg (1024x576) [142.7 KB] || MAVEN_Solar_Wind_Disappear_V4.jpg (1280x720) [459.3 KB] || MAVEN_Solar_Wind_Disappear_V4.png (1280x720) [800.2 KB] || MAVEN_Solar_Wind_Disappear_V4_searchweb.png (320x180) [69.9 KB] || MAVEN_Solar_Wind_Disappear_V4_thm.png (80x40) [6.5 KB] || 14477_MAVEN_Solar_Wind_Disappear_720.mp4 (1280x720) [43.4 MB] || 14477_MAVEN_Solar_Wind_Disappear_1080.mp4 (1920x1080) [243.1 MB] || MavenSolarWindCaptionsV2.en_US.srt [3.8 KB] || MavenSolarWindCaptionsV2.en_US.vtt [3.6 KB] || 14477_MAVEN_Solar_Wind_Disappear_4K.mp4 (3840x2160) [3.0 GB] || 14477_MAVEN_Solar_Wind_Disappear_ProRes.mov (3840x2160) [20.7 GB] || ", "hits": 164 }, { "id": 14434, "url": "https://svs.gsfc.nasa.gov/14434/", "result_type": "Produced Video", "release_date": "2023-11-28T09:20:00-05:00", "title": "NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars", "description": "This visualization shows 294 gamma-ray pulsars, first plotted on an image of the entire starry sky as seen from Earth and then transitioning to a view from above our galaxy. The symbols show different types of pulsars. Young pulsars blink in real time except for the Crab, which pulses slower because its rate is only slightly lower than the video frame rate. Millisecond pulsars remain steady, pulsing too quickly to see. The Crab, Vela, and Geminga were among the 11 gamma-ray pulsars known before Fermi launched. Other notable objects are also highlighted. Distances are shown in light-years (abbreviated ly).Credit: NASA’s Goddard Space Flight CenterMusic: \"Fascination\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Pulsar_Still.jpg (3840x2160) [3.5 MB] || Pulsar_Still_searchweb.png (320x180) [105.5 KB] || Pulsar_Still_thm.png (80x40) [7.0 KB] || 14434_Fermi_Pulsar_Locations_1080.mp4 (1920x1080) [93.9 MB] || 14434_Fermi_Pulsar_Locations_1080.webm (1920x1080) [10.0 MB] || Pulsar_Captions.en_US.srt [46 bytes] || Pulsar_Captions.en_US.vtt [56 bytes] || 14434_Fermi_Pulsar_Locations_4k_Good.mp4 (3840x2160) [112.8 MB] || 14434_Fermi_Pulsar_Locations_4k_Best.mp4 (3840x2160) [689.2 MB] || 14434_Fermi_Pulsar_Locations_ProRes_3840x2160_2997.mov (3840x2160) [4.5 GB] || ", "hits": 215 }, { "id": 5179, "url": "https://svs.gsfc.nasa.gov/5179/", "result_type": "Visualization", "release_date": "2023-10-25T09:50:00-04:00", "title": "Worldview Tour: Journey of Iceberg B-22", "description": "Iceberg B-22 calved from Thwaites Glacier, located in Antarctica in early 2002. From the vantage point of space we track its journey and evolution during the last 21 years. || Worldview_IcebergJourney.png (3548x1824) [5.8 MB] || Worldview_IcebergJourney_print.jpg (1024x526) [176.1 KB] || Worldview_IcebergJourney_searchweb.png (320x180) [107.3 KB] || Worldview_IcebergJourney_thm.png (80x40) [7.1 KB] || Worldview_IcebergJourney.mov (3548x1824) [146.2 MB] || ", "hits": 18 }, { "id": 14442, "url": "https://svs.gsfc.nasa.gov/14442/", "result_type": "Animation", "release_date": "2023-10-24T11:00:00-04:00", "title": "STAQS Air Quality Conceptual Illustrations", "description": "While poor air quality affects everyone, there are pollution hotspots that can adversely affect those nearest. For example, neighborhoods located near highways and warehouses can be hotspots of nitrogen dioxide (NO2) and hazardous particles called PM2.5, which are more than 35 times smaller in diameter than a grain of sand.For other residents, such as those located downwind from major cities like Chicago and New York, ozone can be an issue. While ozone high in the atmosphere protects Earth from dangerous solar radiation, at the ground level it can cause respiratory diseases and drive smog. Ozone ‘brewed’ in cities can travel to rural communities.Ground-level ozone along with another hazardous pollutant – tiny particles called PM2.5 – lead to over 100,000 premature deaths each year in the U.S. || ", "hits": 23 }, { "id": 5158, "url": "https://svs.gsfc.nasa.gov/5158/", "result_type": "Visualization", "release_date": "2023-09-11T15:00:00-04:00", "title": "Hurriances Idalia and Franklin Wind Flows", "description": "Particles released in the wind field mark the trajectory and evolution of Hurricanes Idalia and Franklin. The particles are color coded based on the magnitude of the wind velocity vectors from blue to red indicating low to high wind speeds. || hurricane_idalia_winds.4k_p60.02200_print.jpg (1024x576) [365.2 KB] || hurricane_idalia_winds.4k_p60.02200_searchweb.png (320x180) [117.4 KB] || hurricane_idalia_winds.4k_p60.02200_thm.png (80x40) [6.6 KB] || 1920x1080_16x9_60p (1920x1080) [256.0 KB] || 3840x2160_16x9_60p (3840x2160) [256.0 KB] || hurricane_idalia_winds_1920x1080_p60.mp4 (1920x1080) [355.1 MB] || hurricane_idalia_winds.4k_p60.mp4 (3840x2160) [1.4 GB] || ", "hits": 37 }, { "id": 5145, "url": "https://svs.gsfc.nasa.gov/5145/", "result_type": "Visualization", "release_date": "2023-08-30T00:00:00-04:00", "title": "Franklin Re-intensifies over the Western Atlantic", "description": "Hurricane Franklin in the Atlantic on August 29, 2023 at 2:41Z || Franklin_001.4300_print.jpg (1024x576) [237.7 KB] || Franklin_001.4300_searchweb.png (320x180) [108.1 KB] || Franklin_001.4300_thm.png (80x40) [8.4 KB] || Franklin_001_1080p30_2.mp4 (1920x1080) [52.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Franklin_001_1080p30_2.webm (1920x1080) [5.7 MB] || Franklin_001_1080p30_2.mp4.hwshow [188 bytes] || ", "hits": 62 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 255 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 339 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 331 }, { "id": 31228, "url": "https://svs.gsfc.nasa.gov/31228/", "result_type": "Hyperwall Visual", "release_date": "2023-06-29T00:00:00-04:00", "title": "Landsat Tracks Brunt Ice Shelf Evolution 1986-2023", "description": "Data from 30 January 1986 - 12 February 2023 || ForAmy_BruntHyperwall-selected.v2.0000_print.jpg (1024x576) [115.7 KB] || ForAmy_BruntHyperwall-selected.v2.0000_searchweb.png (320x180) [52.8 KB] || ForAmy_BruntHyperwall-selected.v2.0000_thm.png (80x40) [4.3 KB] || ForAmy_BruntHyperwall-selected.v2_1080p30_2.mp4 (1920x1080) [26.6 MB] || ForAmy_BruntHyperwall-selected.v2_1080p30_2.webm (1920x1080) [4.1 MB] || v2 (3840x2160) [128.0 KB] || ForAmy_BruntHyperwall-selected.v2_2160p30_2.mp4 (3840x2160) [114.1 MB] || ", "hits": 98 }, { "id": 31231, "url": "https://svs.gsfc.nasa.gov/31231/", "result_type": "Hyperwall Visual", "release_date": "2023-06-07T00:00:00-04:00", "title": "Monitoring California Groundwater", "description": "GRACE California Terrestrial Water Storage from 2002-04 to 2023-03. || grace_ca_water_black_v3_20230316_1200_print.jpg (1024x574) [149.5 KB] || grace_ca_water_black_v3_20230316_1200_searchweb.png (320x180) [66.6 KB] || grace_ca_water_black_v3_20230316_1200_thm.png (80x40) [12.5 KB] || grace_ca_water_2002-2023_seasonal_1080p.mp4 (1920x1080) [7.0 MB] || grace_ca_water_2002-2023_seasonal_1080p.webm (1920x1080) [4.2 MB] || grace_ca_water_2002-2023_seasonal_2160p.mp4 (3840x2160) [23.1 MB] || grace_ca_water_black_v3_20230316_1200.tif (4104x2304) [4.7 MB] || grace_ca_water_2002-2023 (4104x2304) [0 Item(s)] || grace_ca_water_2002-2023_seasonal_1080p.hwshow [112 bytes] || ", "hits": 45 }, { "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": 347 }, { "id": 14323, "url": "https://svs.gsfc.nasa.gov/14323/", "result_type": "Produced Video", "release_date": "2023-05-11T15:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "This video includes music from a synthesized orchestra provided by composer Henry Dehlinger.Music credit: “Echoes of the Big Bang\" from Cosmic Cycles: A Space Symphony by Henry Dehlinger. Courtesy of the composer.Complete list of footage usedHERE. Watch this video on the NASA Goddard YouTube channel. || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_print.jpg (1024x576) [73.5 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2.jpg (3840x2160) [511.8 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_searchweb.png (320x180) [40.4 KB] || Cosmic_Cycles_Echoes_of_the_Big_Bang_V2_thm.png (80x40) [5.4 KB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.webm (1920x1080) [130.2 MB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_1080.mp4 (1920x1080) [1.7 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_50mbps.mp4 (1920x1080) [4.1 GB] || Cosmic_Cycles-Echoes_of_the_Big_Bang_Online_ProRes_1920x1080_2997.mov (1920x1080) [14.7 GB] || ", "hits": 114 }, { "id": 40461, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles7-echoesofthe-big-bang/", "result_type": "Gallery", "release_date": "2023-03-27T00:00:00-04:00", "title": "Cosmic Cycles 7: Echoes of the Big Bang", "description": "NASA studies the makeup and workings of the universe, from the smallest particles of matter and energy to its large-scale structure and evolution. Scientists look far back in space and time to learn the full cosmic history of stars and galaxies. They tease out details of the environments around black holes and observe the most powerful explosions since the big bang. NASA is discovering numerous planets beyond our solar system, decoding how planetary systems form, and learning how environments hospitable for life develop.\n\nWant to know more?\nNASA Universe Webb Space Telescope images Hubble Space Telescope", "hits": 56 }, { "id": 14297, "url": "https://svs.gsfc.nasa.gov/14297/", "result_type": "Produced Video", "release_date": "2023-03-01T10:00:00-05:00", "title": "How NASA's Roman Space Telescope Will Rewind the Universe", "description": "In this simulated view of the deep cosmos, each dot represents a galaxy. The three small squares show Hubble's field of view, and each reveals a different region of the synthetic universe. Roman will be able to quickly survey an area as large as the whole zoomed-out image, which will give us a glimpse of the universe’s largest structures.Credits: NASA’s Goddard Space Flight Center/A. Yung || Yung_Stucture_Survey-Hubble.gif (800x800) [10.9 MB] || Yung_Structure_Survey-Hubble_ProRes.mov (800x800) [36.3 MB] || Yung_Structure_Survey-Hubble_800.mp4 (800x800) [6.4 MB] || Yung_Structure_Survey-Hubble_800.webm (800x800) [1.6 MB] || ", "hits": 93 }, { "id": 5063, "url": "https://svs.gsfc.nasa.gov/5063/", "result_type": "Visualization", "release_date": "2023-02-10T00:00:00-05:00", "title": "An X1.9 Class Solar Flare and its Aftermath - January 9, 2023", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Here, Active Region 13164 (near the lower left limb of the solar disk) fires off a hefty X-class flare (X1.9). (Solar Flares: What does it take to be X-class?). The region continues some active evolution with loops and filaments more visible in the 171A and 304A filters. Smaller M-Class flares erupt later in this sequence, an M 5.1 at the upper left limb and an M 2.6 in the lower right center. The point-spread function correction (PSF) has been applied to all the imagery on this page. || ", "hits": 21 }, { "id": 14278, "url": "https://svs.gsfc.nasa.gov/14278/", "result_type": "Produced Video", "release_date": "2023-01-17T16:00:00-05:00", "title": "SpaceBack", "description": "SpaceBack is a series of shorts that pairs an archival clip of NASA Goddard's history with a current and related science or mission effort. These videos are formatted for viewing in vertical platforms. || ", "hits": 100 }, { "id": 14203, "url": "https://svs.gsfc.nasa.gov/14203/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Simulations of Weak Black Hole Jets", "description": "This sequence shows the simulated evolution of weak jets (orange, pink, and purple) formed by a supermassive black hole as they interact with stars and gas clouds (green, yellow) at the center of a galaxy. The jet is angled about 15 degrees toward the plane of its galaxy and is shown in 12 time steps, with each interval representing 50,000 years. The image at bottom right shows the jets 600,000 years after they formed. Each step is available as a 4K video and as frames by selecting \"Download Options.\"Credit: NASA's Goddard Space Flight Center/R. Tanner and K. Weaver || AGN_time_series_Numbered_print.jpg (1024x576) [109.6 KB] || AGN_time_series_Numbered.jpg (3840x2160) [982.9 KB] || Step1 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.webm (4000x4000) [3.2 MB] || Step12 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step12_4k_30.mp4 (4000x4000) [15.0 MB] || Step11 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step11_4k_30.mp4 (4000x4000) [15.0 MB] || Step10 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step10_4k_30.mp4 (4000x4000) [14.9 MB] || Step9 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step9_4k_30.mp4 (4000x4000) [15.0 MB] || Step8 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step8_4k_30.mp4 (4000x4000) [15.0 MB] || Step7 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step7_4k_30.mp4 (4000x4000) [15.0 MB] || Step6 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step1_4k_30.mp4 (4000x4000) [15.1 MB] || Step5 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step5_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step2_4k_30.mp4 (4000x4000) [15.0 MB] || Step4 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step4_4k_30.mp4 (4000x4000) [15.0 MB] || Step2 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step6_4k_30.mp4 (4000x4000) [14.9 MB] || Step3 (4000x4000) [16.0 KB] || AGNwinds_TimeEvolution_Step3_4k_30.mp4 (4000x4000) [15.0 MB] || AGNwinds_TimeEvolution_Step10_ProRes_4k_30.mov (4000x4000) [3.1 GB] || AGNwinds_TimeEvolution_Step1_ProRes_4k_30.mov (4000x4000) [387.2 MB] || AGNwinds_TimeEvolution_Step2_ProRes_4k_30.mov (4000x4000) [864.7 MB] || AGNwinds_TimeEvolution_Step12_ProRes_4k_30.mov (4000x4000) [3.3 GB] || AGNwinds_TimeEvolution_Step3_ProRes_4k_30.mov (4000x4000) [1.4 GB] || AGNwinds_TimeEvolution_Step11_ProRes_4k_30.mov (4000x4000) [3.2 GB] || AGNwinds_TimeEvolution_Step4_ProRes_4k_30.mov (4000x4000) [1.9 GB] || AGNwinds_TimeEvolution_Step9_ProRes_4k_30.mov (4000x4000) [2.9 GB] || AGNwinds_TimeEvolution_Step5_ProRes_4k_30.mov (4000x4000) [2.4 GB] || AGNwinds_TimeEvolution_Step8_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step7_ProRes_4k_30.mov (4000x4000) [2.8 GB] || AGNwinds_TimeEvolution_Step6_ProRes_4k_30.mov (4000x4000) [2.7 GB] || ", "hits": 183 }, { "id": 14217, "url": "https://svs.gsfc.nasa.gov/14217/", "result_type": "Produced Video", "release_date": "2022-11-15T13:00:00-05:00", "title": "Creating Black Hole Jets With a NASA Supercomputer", "description": "New simulations carried out on the NASA Center for Climate Simulation’s Discover supercomputer show how weaker, low-luminosity jets produced by a galaxy's monster black hole interact with their galactic environment. Because these jets are more difficult to detect, the simulations help astronomers link these interactions to features they can observe, such as various gas motions and optical and X-ray emissions.Credit: NASA's Goddard Space Flight CenterMusic credit: \"Lost Time;\" \"Ascension;\" \"Flowing Cityscape;\" \"Jupiter's Eye;\" \"Pizzicato Piece;\" \"Facts;\" \"Final Words\" all from Universal Production MusicVideo Descriptive Text available.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || 14217_AGN_OUtflow_Still.jpg (1920x1080) [1.0 MB] || 14217_AGN_OUtflow_Still_searchweb.png (320x180) [92.9 KB] || 14217_AGN_OUtflow_Still_thm.png (80x40) [6.7 KB] || 14217_AGN_Outflow_FINAL_1080.webm (1920x1080) [67.5 MB] || AGN_Outflow_SRT_Captions.en_US.srt [11.4 KB] || 14217_AGN_Outflow_FINAL_1080.mp4 (1920x1080) [632.4 MB] || 14217_AGN_Outflow_FINAL_1080_Best.mp4 (1920x1080) [1.5 GB] || 14217_AGN_Outflow_FINAL_ProRes_1920x1080_24.mov (1920x1080) [6.4 GB] || ", "hits": 171 }, { "id": 31197, "url": "https://svs.gsfc.nasa.gov/31197/", "result_type": "Hyperwall Visual", "release_date": "2022-10-26T00:00:00-04:00", "title": "Carina Nebula Webb vs Hubble", "description": "Carina Nebula comparison of James Web vs HubbleThese comparison photos of a young star-forming region called NGC 3324 in the Carina Nebula, taken by Webb, (left) and Hubble, (right), showcase Webb’s abilities to peer through cosmic dust and unveil hundreds of previously hidden stars and background galaxies. Taken by NASA’s James Webb Space Telescope, this image reveals for the first time areas of stellar birth captured in infrared light by the Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). Webb’s NIRCam – with its crisp resolution and unparalleled sensitivity – unveils emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. In MIRI’s view, young stars and their planet-forming disks shine brightly in the mid-infrared, appearing pink and red. Hot dust, hydrocarbons, and other chemical compounds on the surface of the ridges glow, giving the appearance of jagged rocks.Webb’s detailed image captured in infrared light (left) is juxtaposed with a color composite image (right) of separate exposures made by Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Planetary Camera 2 (WFPC2). In Hubble’s image on the right, sulfur is represented by red, oxygen by blue, and hydrogen by green.Webb’s new observations of NGC 3324 will shed light on stellar processes and reveal the impact of star formation on the evolution of gigantic clouds of gas and dust.For more information: https://www.nasa.gov/image-feature/goddard/2022/nasa-s-webb-reveals-cosmic-cliffs-glittering-landscape-of-star-birth || carina_nebula_00000_print.jpg (1024x576) [202.8 KB] || carina_nebula_00000_searchweb.png (320x180) [96.5 KB] || carina_nebula_00000_web.png (320x180) [96.5 KB] || carina_nebula_00000_thm.png (80x40) [6.9 KB] || carina_nebula_720p30.mp4 (1280x720) [22.5 MB] || carina_nebula_720p30.webm (1280x720) [9.4 MB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || carina_nebula_2160p30_h265.mp4 (3840x2160) [57.7 MB] || ", "hits": 136 }, { "id": 5037, "url": "https://svs.gsfc.nasa.gov/5037/", "result_type": "Visualization", "release_date": "2022-09-28T00:00:00-04:00", "title": "Hurricane Ian Forms South of Cuba", "description": "Hurricane Ian off the Cuban Coast on September 26, 2022 at 20:29Z. || Ian0926_001.4300_print.jpg (1024x576) [277.8 KB] || Ian0926_001.4300_searchweb.png (320x180) [128.0 KB] || Ian0926_001.4300_thm.png (80x40) [8.8 KB] || Ian0926_001_1080p30_3.mp4 (1920x1080) [74.2 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Ian0926_001_1080p30_3.webm (1920x1080) [5.9 MB] || Ian0926_001_1080p30_3.mp4.hwshow [187 bytes] || ", "hits": 71 }, { "id": 5023, "url": "https://svs.gsfc.nasa.gov/5023/", "result_type": "Visualization", "release_date": "2022-09-19T09:30:00-04:00", "title": "Lunar Polar Wander", "description": "The wandering path of the lunar South Pole is shown over a period from 4.25 billion years ago to the present.This video can also be viewed on the SVS YouTube channel. || tpw.0750_print.jpg (1024x576) [250.9 KB] || tpw.0750_searchweb.png (320x180) [109.2 KB] || tpw.0750_thm.png (80x40) [7.6 KB] || tpw_1080p30.mp4 (1920x1080) [46.9 MB] || tpw_720p30.mp4 (1280x720) [22.5 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || tpw_720p30.webm (1280x720) [5.6 MB] || tpw_360p30.mp4 (640x360) [8.1 MB] || tpw_1080p30.mp4.hwshow [177 bytes] || ", "hits": 129 }, { "id": 5018, "url": "https://svs.gsfc.nasa.gov/5018/", "result_type": "Visualization", "release_date": "2022-09-14T13:00:00-04:00", "title": "BAMS Cover: Mapping Global Precipitation", "description": "BAMS cover as published, showing the evolution of the coverage of precipitation observations provided by passive microwave satellite sensors from 1985-2015. || Aug22_cover_proof3_print.jpg (1024x1353) [370.4 KB] || Aug22_cover_proof3_searchweb.png (320x180) [88.5 KB] || Aug22_cover_proof3_thm.png (80x40) [7.5 KB] || Aug22_cover_proof3.tiff (2450x3238) [9.8 MB] || ", "hits": 30 }, { "id": 14089, "url": "https://svs.gsfc.nasa.gov/14089/", "result_type": "Produced Video", "release_date": "2022-09-05T10:00:00-04:00", "title": "A Box of Treasure from Asteroid Ryugu", "description": "NASA scientist Heather Graham receives a shipment of asteroid Ryugu samples from her colleagues at the Japan Aerospace Exploration Agency (JAXA). Transcript available.Universal Production Music: “The Ocean and the Moon” & “On Your Game” by Andy Blythe and Marten JoustraWatch this video on the NASA Goddard YouTube channel. || Ryugu_Treasure_Preview_V7_print.jpg (1024x576) [110.4 KB] || Ryugu_Treasure_Preview_V7.png (3840x2160) [6.0 MB] || Ryugu_Treasure_Preview_V7.jpg (3840x2160) [1.2 MB] || Ryugu_Treasure_Preview_V7_searchweb.png (320x180) [62.7 KB] || Ryugu_Treasure_Preview_V7_thm.png (80x40) [5.7 KB] || 14089_Ryugu_Sample_V4_Twitter.mp4 (1280x720) [33.5 MB] || 14089_Ryugu_Sample_V2_Twitter.webm (1280x720) [16.2 MB] || 14089_Ryugu_Sample_V4_Facebook.mp4 (1920x1080) [189.1 MB] || 14089_Ryugu_Sample_V2_Captions.en_US.srt [3.7 KB] || 14089_Ryugu_Sample_V2_Captions.en_US.vtt [3.5 KB] || 14089_Ryugu_Sample_V4_YouTube.mp4 (3840x2160) [1.8 GB] || 14089_Ryugu_Sample_V4_MASTER.mov (3840x2160) [7.7 GB] || ", "hits": 162 }, { "id": 14204, "url": "https://svs.gsfc.nasa.gov/14204/", "result_type": "Produced Video", "release_date": "2022-08-31T09:00:00-04:00", "title": "Mars Patchy Proton Aurora", "description": "NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission and the United Arab Emirates’ Emirates Mars Mission (EMM) have released joint observations of dynamic proton aurora events at Mars. Remote auroral observations by EMM paired with in-situ plasma observations made by MAVEN open new avenues for understanding the Martian atmosphere. This collaboration was made possible by recent data-sharing between the two missions and highlights the value of multi-point observations in space.Learn more about this discovery by MAVEN and EMM. || ", "hits": 63 }, { "id": 14172, "url": "https://svs.gsfc.nasa.gov/14172/", "result_type": "Produced Video", "release_date": "2022-07-05T00:00:00-04:00", "title": "Dominic Benford 2022 AAS Roman Hyperwall Talk", "description": "Static title card.Credit: NASA's Goddard Space Flight Center || dominic_benford_roman_title_slide_print.jpg (1024x576) [262.4 KB] || dominic_benford_roman_title_slide.png (3840x2160) [10.2 MB] || dominic_benford_roman_title_slide_searchweb.png (320x180) [113.1 KB] || dominic_benford_roman_title_slide_thm.png (80x40) [7.9 KB] || ", "hits": 21 }, { "id": 14124, "url": "https://svs.gsfc.nasa.gov/14124/", "result_type": "Produced Video", "release_date": "2022-03-23T06:00:00-04:00", "title": "NASA’s Hubble Space Telescope Makes Record-Breaking Discovery Live Shots", "description": "Quick link to cut B-ROLL for the live shotsQuick link to canned interview with Dr. Michelle ThallerClick here for the release: Record Broken: Hubble Spots Farthest Star Ever SeenClick here for the release in Spanish: Un nuevo récord: Hubble detecta la estrella más lejana jamás vistaQuick link to canned interview with Dr Jennifer WisemanQuick link to first canned interview with Brian Welch Quick link to second canned interview with Brian WelchQuick link too canned interview in Spanish with Dr. Rosa Diaz || HubbleBanner.png (3125x1042) [2.6 MB] || HubbleBanner_print.jpg (1024x341) [101.4 KB] || HubbleBanner_searchweb.png (320x180) [98.3 KB] || HubbleBanner_thm.png (80x40) [6.3 KB] || ", "hits": 107 }, { "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": 238 }, { "id": 14116, "url": "https://svs.gsfc.nasa.gov/14116/", "result_type": "Produced Video", "release_date": "2022-03-18T00:00:00-04:00", "title": "Two Scientists Have a Frank and Honest Discussion about Antarctica", "description": "NASA Glaciologists Kelly Brunt and Alex Gardner discuss the history, challenges and evolution of mapping the Antarctic continent and what it means for science and society. || ", "hits": 32 }, { "id": 20363, "url": "https://svs.gsfc.nasa.gov/20363/", "result_type": "Animation", "release_date": "2022-03-09T18:00:00-05:00", "title": "Animation: Heliosphere", "description": "The sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium. This forms a giant bubble around the sun and its planets, known as the heliosphere. NASA studies the heliosphere to better understand the fundamental physics of the space surrounding us - which, in turn, provides information regarding space throughout the rest of the universe, as well as regarding what makes planets habitable.The solar wind is a gas of charged particles known as plasma, a state of matter governed by its own set physical laws just as the more common solids, liquids, and gases are. As the solar wind sweeps out into space, it creates a space environment filled with radiation as well as magnetic fields that trail all the way back to the sun. This space environment is augmented by interstellar cosmic rays and occasional concentrated clouds of solar material that burst off the sun, known as coronal mass ejections.This complex environment surrounds the planets and ultimately has a crucial effect on the formation, evolution, and destiny of planetary systems. For one thing, our heliosphere acts as a giant shield, protecting the planets from galactic cosmic radiation. Earth is additionally shielded by its own magnetic field, the magnetosphere, which protects us not only from solar and cosmic particle radiation but also from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to such processes and have evolved differently.NASA's studies of the heliosphere include research into: how the solar wind behaves near Earth; what causes and sustains magnetic and electric fields around other planets; how does the heliosphere interact with the interstellar medium; what do the boundaries of the heliosphere look like; what is the origin and evolution of the solar wind and the interstellar cosmic rays; and what contributes to the habitability of exoplanets.The field is, therefore, intensely cross-disciplinary. Heliospheric research often works hand in hand with planetary scientists, astrophysicists, astrobiologists, and space weather researchers.NASA heliophysics missions contributing to heliospheric research are: the Advanced Composition Explorer; NOAA's Deep Space Climate Observatory, the Interstellar Boundary Explorer, the Solar Terrestrial Relations Observatory; Voyager, and Wind. || ", "hits": 503 }, { "id": 20345, "url": "https://svs.gsfc.nasa.gov/20345/", "result_type": "Animation", "release_date": "2022-03-01T00:00:00-05:00", "title": "TROPICS Mission Animations", "description": "The NASA Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats (TROPICS) mission is a constellation of state-of-the-science observing platforms that will measure temperature and humidity soundings and precipitation with spatial resolution comparable to current operational passive microwave sounders but with unprecedented temporal resolution (median revisit time of 50 minutes).Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || Tropics_Beauty_Shot_ProRes.00540_print.jpg (1024x576) [95.4 KB] || Tropics_Beauty_Shot_H264_1080.mp4 (1920x1080) [76.4 MB] || Tropics_Beauty_Shot_H264_1080.webm (1920x1080) [3.4 MB] || Tropics_Beauty_Shot_H264_4k.mp4 (3840x2160) [309.1 MB] || Tropics_Beauty_Shot_ProRes.mov (3840x2160) [3.1 GB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || Tropics_Beauty_Shot_ProRes.webm (3840x2160) [10.3 MB] || ", "hits": 36 }, { "id": 31177, "url": "https://svs.gsfc.nasa.gov/31177/", "result_type": "Hyperwall Visual", "release_date": "2022-02-15T00:00:00-05:00", "title": "Monitoring California Groundwater 2002-2022", "description": "California land water storage, 2002-2022 || grace_ca_water_title1_202202_print.jpg (1024x576) [139.6 KB] || grace_ca_water_title1_202202_searchweb.png (320x180) [64.0 KB] || grace_ca_water_title1_202202_thm.png (80x40) [12.3 KB] || grace_ca_water_200205-202202_title1_1080p6.mp4 (1920x1080) [4.4 MB] || grace_ca_water_200205-202202_title1_1080p6.webm (1920x1080) [3.9 MB] || grace_ca_water_200205-202202_title1_2160p6.mp4 (3840x2160) [14.4 MB] || grace_ca_water_title1_202202.tif (3840x2160) [4.3 MB] || grace_ca_water_200205-202202_title1_2160.hwshow [125 bytes] || ", "hits": 35 }, { "id": 4959, "url": "https://svs.gsfc.nasa.gov/4959/", "result_type": "Visualization", "release_date": "2021-12-13T00:00:00-05:00", "title": "Reduction in Tropospheric NOx and Ozone Corresponding to Worldwide COVID-19 Lockdowns", "description": "When the world went into lockdown to slow the spread of COVID-19, air pollution emissions started to rapidly decrease leaving a global atmospheric fingerprint detected by a team of scientists at NASA’s Jet Propulsion Laboratory using satellite measurements. These traces provided an unexpected window into what low-emissions world could look like, thus providing a means for identifying effective environmental policies. While many countries in the last few decades have implemented environmental policies to reduce human health risk from air pollution by controlling emissions, the impacts of those policies have not always been clear. The global lockdowns in response to COVID-19 represent a well-observed “scenario-of-opportunity” that allows us to assess how atmospheric emission and composition responds to reduced human activity. COVID-19 lockdowns effectively showed how reducing NOx emissions affects the global atmosphere. Its identifying signature shows up as in the atmosphere’s altered ability to produce harmful ozone pollution and ozone’s reduced influence on Earth’s heat balance that affects climate. These effects are not uniform across the world and depend on the location and season of the emission reductions.The results of this research indicate that in order to design effective environmental policies which benefit both air quality and climate, decision-makers need to carefully consider the complex relationships between emissions and atmospheric composition. || ", "hits": 40 }, { "id": 40435, "url": "https://svs.gsfc.nasa.gov/gallery/davinci/", "result_type": "Gallery", "release_date": "2021-12-07T00:00:00-05:00", "title": "DAVINCI", "description": "Launching in 2029, NASA’s Deep Atmosphere Venus Investigation of Noble gases, Chemistry and Imaging (DAVINCI) mission will bring a rich suite of instruments to Venus to address long standing questions about Earth’s sister planet. Some scientists think Venus may once have been more Earth-like in the past, with oceans and pleasant surface temperatures -- DAVINCI data will help us determine if this intriguing possibility is true. Clues to Venus’ mysterious past may be hidden in atmospheric gases or in surface rocks formed in association with ancient water in the planet’s mountainous highlands.", "hits": 104 }, { "id": 40431, "url": "https://svs.gsfc.nasa.gov/gallery/fulldome-gallery/", "result_type": "Gallery", "release_date": "2021-11-23T00:00:00-05:00", "title": "Fulldome Gallery", "description": "Visualizations in fulldome format for display in digital planetariums.", "hits": 227 }, { "id": 40433, "url": "https://svs.gsfc.nasa.gov/gallery/science-ona-sphere-gallery/", "result_type": "Gallery", "release_date": "2021-11-23T00:00:00-05:00", "title": "Science On a Sphere Gallery", "description": "Content for NOAA's Science on a Sphere and related spherical display platforms.", "hits": 300 }, { "id": 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": 91 }, { "id": 13945, "url": "https://svs.gsfc.nasa.gov/13945/", "result_type": "Produced Video", "release_date": "2021-10-14T10:00:00-04:00", "title": "Lucy L-2 Science and Instrument Briefing", "description": "NASA will hold a virtual media briefing at 1 p.m. EDT Thursday, October 14th, to preview the launch of the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun.The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Participants in Thursday's briefing will include:• Alana Johnson, Senior Communications Specialist, NASA Planetary Science Division• Adriana Ocampo, Lucy Program Executive, NASA Headquarters• Cathy Olkin, Lucy Deputy Principal Investigator, Southwest Research Institute • Keith Noll, Lucy Project Scientist, NASA's Goddard Space Flight Center• Hal Weaver, L’LORRI Instrument PI, Johns Hopkins University Applied Physics Laboratory • Phil Christensen, L’TES Instrument PI, Arizona State University • Dennis Reuter, L’RALPH Instrument PI, NASA's Goddard Space Flight Center Over its 12-year primary mission, Lucy will explore a record number of asteroids in separate orbits around the Sun. The spacecraft will fly by one asteroid in the solar system’s main belt, located between the orbits of Mars and Jupiter, followed by seven Trojans. In addition, Lucy’s path will circle back to Earth three times for gravity assists, making it the first spacecraft ever to travel out to the distance of Jupiter and return to the vicinity of Earth.The Lucy mission is named after the fossilized skeleton of an early hominin (pre-human ancestor) discovered in Ethiopia in 1974 and named “Lucy” by the team of paleoanthropologists who discovered it. Just as the Lucy fossil provided unique insights into humanity’s evolution, the Lucy mission promises to revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida.Southwest Research Institute is the home institution of the principal investigator. NASA Goddard Space provides overall mission management, systems engineering, plus safety and mission assurance. Lockheed Martin Space built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the Science Mission Directorate. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida.For more information about Lucy, visit: http://www.nasa.gov/lucy || ", "hits": 19 }, { "id": 13948, "url": "https://svs.gsfc.nasa.gov/13948/", "result_type": "Produced Video", "release_date": "2021-10-05T09:00:00-04:00", "title": "Designing Lucy’s Path to the Trojan Asteroids", "description": "Explore Lucy’s journey to one main-belt asteroid and seven Jupiter Trojans.Complete transcript available.Universal Production Music: “Ocean Simulation” & “The Sequencer Paradox” by Laetitia Frenod; “The Chess Game” by David James Elliott & Martin Gratton; “Tale of Time” by Markus GleissnerWatch this video on the NASA Goddard YouTube channel. || DesigningLucyPreview_print.jpg (1024x576) [277.3 KB] || DesigningLucyPreview.png (3840x2160) [11.6 MB] || DesigningLucyPreview.jpg (3840x2160) [3.2 MB] || DesigningLucyPreview_searchweb.png (320x180) [105.7 KB] || DesigningLucyPreview_thm.png (80x40) [7.2 KB] || 13948_Designing_Lucy_Twitter.webm (1280x720) [50.5 MB] || 13948_Designing_Lucy_Twitter.mp4 (1280x720) [101.0 MB] || 13948_Designing_Lucy_Facebook.mp4 (1920x1080) [559.4 MB] || 13948_Designing_Lucy_Captions.en_US.srt [10.8 KB] || 13948_Designing_Lucy_Captions.en_US.vtt [10.4 KB] || 13948_Designing_Lucy_YouTube.mp4 (3840x2160) [4.4 GB] || 13948_Designing_Lucy_MASTER.mov (3840x2160) [21.6 GB] || ", "hits": 57 }, { "id": 13950, "url": "https://svs.gsfc.nasa.gov/13950/", "result_type": "Produced Video", "release_date": "2021-10-05T06:00:00-04:00", "title": "NASA Just Days Away From Launching Probe To Mysterious Asteroid Belt To Explore \"Fossils\" Of The Early Solar System Live Shots", "description": "Quick link to edited B-ROLL for the live shotsQuick link to canned interview with Donya Douglas-Bradshaw Lucy Project ManagerQuick link to canned interview with Cory Prykull, Lockheed Martin Space, Lucy Assembly, Test & Launch Operations Lead || Lucy_banner.png (1550x464) [1.3 MB] || Lucy_banner_print.jpg (1024x306) [134.8 KB] || Lucy_banner_searchweb.png (320x180) [139.1 KB] || Lucy_banner_thm.png (80x40) [12.5 KB] || ", "hits": 34 }, { "id": 13933, "url": "https://svs.gsfc.nasa.gov/13933/", "result_type": "Produced Video", "release_date": "2021-09-28T13:00:00-04:00", "title": "Lucy L-20 Briefing", "description": "NASA will hold a virtual media briefing at 2 p.m. EDT Tuesday, Sept. 28, to preview the launch of the agency’s first spacecraft to study Jupiter’s Trojan asteroids. The Trojan asteroids are remnants of the early solar system clustered in two “swarms” leading and following Jupiter in its path around the Sun.The live briefing will stream on NASA Television, the agency's website, NASA’s Twitter account and the NASA App.Participants in Tuesday's briefing will include:• Alana Johnson, Senior Communications Specialist, NASA Planetary Science Division• Lori Glaze, director of NASA's Planetary Science Division at NASA Headquarters in Washington.• Hal Levison, Lucy Principal Investigator, Southwest Research Institute in Boulder, Colorado.• Keith Noll, Lucy Project Scientist, NASA’s Goddard Space Flight Center in Greenbelt, Maryland. • Rich Lipe, Lockheed Marin Spacecraft Program Manager, Denver, Colorado. • Donya Douglas-Bradshaw, Lucy Project Manager, NASA Goddard Space Flight Center in Greenbelt, Maryland.Over its 12-year primary mission, Lucy will explore a record number of asteroids in separate orbits around the Sun. The spacecraft will fly by one asteroid in the solar system’s main belt, located between the orbits of Mars and Jupiter, followed by seven Trojans. In addition, Lucy’s path will circle back to Earth three times for gravity assists, making it the first spacecraft ever to travel out to the distance of Jupiter and return to the vicinity of Earth.The Lucy mission is named after the fossilized skeleton of an early hominin (pre-human ancestor) discovered in Ethiopia in 1974 and named “Lucy” by the team of paleoanthropologists who discovered it. Just as the Lucy fossil provided unique insights into humanity’s evolution, the Lucy mission promises to revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy is scheduled to launch no earlier than Saturday, Oct. 16, on a United Launch Alliance Atlas V 401 rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station, Florida.Southwest Research Institute is the home institution of the principal investigator. NASA Goddard Space provides overall mission management, systems engineering, plus safety and mission assurance. Lockheed Martin Space built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the Science Mission Directorate. The launch is managed by NASA’s Launch Services Program based at Kennedy Space Center in Florida.For more information about Lucy, visit: http://www.nasa.gov/lucy || ", "hits": 28 }, { "id": 13902, "url": "https://svs.gsfc.nasa.gov/13902/", "result_type": "Produced Video", "release_date": "2021-08-02T09:55:00-04:00", "title": "The Hubble Deep Field: Looking Back In Time", "description": "The Hubble Space Telescope has made over 1.5 million observations since its launch in 1990, capturing stunning subjects such as the Eagle Nebula and producing data that has been featured in almost 18,000 scientific articles. But no image has revolutionized the way we understand the universe as much as the Hubble Deep Field.Taken over the course of 10 days in 1995, the Hubble Deep Field captured roughly 3,000 distant galaxies varying in their stages of evolution, stunning the world. This video features some of the scientists and engineers that work on Hubble, and how the Hubble Deep Field changed everything.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Compact galaxies in the Hubble Ultra Deep Field: Credit: ESA/Hubble (M. Kornmesser & L. L. Christensen)Pan of GOODS field containing distant dwarf galaxies forming stars at an incredible rate: Credit: NASA & ESAHubble: Galaxies Across Space and Time: Credit: NASA, ESA and F. Summers (STScI)Speedthrough of galaxies added to deep field image: Credit: NASA/CXC/SAO/K.Arcand; Sonification: @SYSTEMSounds (M. Russo, A. Santaguida)Music Credits: \"Earth’s Orbit\" by Andreas Andreas Bolldén [STIM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music.“Planetary Exploration” by Richard Andrew Canavan [PRS] via Sound Pocket Music [PRS], and Universal Production Music. || ", "hits": 235 }, { "id": 13876, "url": "https://svs.gsfc.nasa.gov/13876/", "result_type": "Produced Video", "release_date": "2021-07-12T10:00:00-04:00", "title": "TESS Finds Related Stars Have Young Exoplanets", "description": "Stellar siblings over 130 light-years away host two systems of teenage planets. Watch to learn how NASA’s Transiting Exoplanet Survey Satellite discovered these young worlds and what they might tell us about the evolution of planetary systems everywhere, including our own.Music Credit: \"Building Ideas\" from Universal Production MusicCredit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || tess_stellar_siblings_label.jpg (1920x1080) [572.8 KB] || stellar_siblings_still_01.jpg (1920x1080) [536.3 KB] || stellar_siblings_still_01_print.jpg (1024x576) [179.0 KB] || stellar_siblings_still_01_searchweb.png (320x180) [57.0 KB] || stellar_siblings_still_01_web.png (320x180) [57.0 KB] || stellar_siblings_still_01_thm.png (80x40) [4.7 KB] || TESS_stellar_siblings_HQ.mp4 (1920x1080) [286.2 MB] || TESS_stellar_siblings_LQ.mp4 (1920x1080) [150.7 MB] || TESS_stellar_siblings_prores.mov (1920x1080) [1.6 GB] || TESS_stellar_siblings_LQ.webm (1920x1080) [16.0 MB] || TESS_stellar_siblings_prores.en_US.srt [2.0 KB] || TESS_stellar_siblings_prores.en_US.vtt [2.0 KB] || ", "hits": 135 }, { "id": 13872, "url": "https://svs.gsfc.nasa.gov/13872/", "result_type": "Produced Video", "release_date": "2021-06-17T10:55:00-04:00", "title": "Mystery of Galaxy's Missing Dark Matter Deepens", "description": "When astronomers using NASA’s Hubble Space Telescope uncovered an oddball galaxy that looks like it doesn’t have much dark matter, some thought the finding was hard to believe and looked for a simpler explanation. Dark matter, after all, is the invisible glue that makes up the bulk of the universe’s contents. All galaxies are dominated by it; in fact, galaxies are thought to form inside immense halos of dark matter. So, finding a galaxy lacking the invisible stuff is an extraordinary claim that challenges conventional wisdom. It would have the potential to upset theories of galaxy formation and evolution.For more information, visit https://nasa.gov/hubble. Additional Visualizations:Galaxy Motion Simulation: Credit: ESO/L. Calçada.Dark Matter Simulation: Credit: Additional Visualizations:Galaxy Motion Simulation: Credit: ESO/L. Calçada.Dark Matter Simulation: Credit: Wu, Hahn, Wechsler, Abel(KIPAC), Visualization: Kaehler (KIPAC)Music Credits: \"Aphelion Horizon\" by Alistair Hetherington [PRS] via Atmosphere Music Ltd. [PRS], and Universal Production Music. || ", "hits": 226 }, { "id": 10662, "url": "https://svs.gsfc.nasa.gov/10662/", "result_type": "Produced Video", "release_date": "2021-04-14T00:00:00-04:00", "title": "Webb Science Simulations: Planetary Systems and Origins of Life", "description": "Supercomputer simulations of planeratry evolution. Part 1: Turbulent Molecular Cloud Nebula with Protostellar ObjectsThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Drs. Alexei Kritsuk and Michael Norman to visualize a computational data set of a turbulent molecular cloud nebula forming protostellar objects and accretion disks approximately 100 AU in diameter, on the order of the size of our solar system. AVL used its Amore software to interpolate and render the Adaptive Mesh Refinement (AMR) simulation generated from ENZO code for cosmology and astrophysics. The AMR simulation was developed by Drs. Kritsuk and Norman at the Laboratory for Computational Astrophysics. The AMR simulation generated more than 2 terabytes of data and follows star formation processes in a self-gravitating turbulent molecular cloud with a dynamic range of half-a-million in linear scale, resolving both the large-scale filamentary structure of the molecular cloud (~5 parsec) and accretion disks around emerging young protostellar objects (down to 2 AU). Part 2: Protoplanetary Disk and Planet FormationThe Advanced Visualization Laboratory (AVL) at the National Center for Supercomputing Applications (NCSA) collaborated with NASA and Dr. Aaron Boley to visualize the 16,000 year evolution of a young, isolated protoplanetary disk which surrounds a newly-formed protostar. The disk forms spiral arms and a dense clump as a result of gravitational collapse. Dr. Aaron Boley developed this computational model to investigate the response of young disks to mass accretion from their surrounding envelopes, including the direct formation of planets and brown dwarfs through gravitational instability. The main formation mechanism for gas giant planets has been debated within the scientific community for over a decade. One of these theories is 'direct formation through gravitational instability.' If the self-gravity of the gas overwhelms the disk's thermal pressure and the stabilizing effect of differential rotation, the gas closest to the protostar rotates faster than gas farther away. In this scenario, regions of the gaseous disk collapse and form a planet directly. The study, presented in Boley (2009), explores whether mass accretion in the outer regions of disks can lead to such disk fragmentation. The simulations show that clumps can form in situ at large disk radii. If the clumps survive, they can become gas giants on wide orbits, e.g., Fomalhaut b, or even more massive objects called brown dwarfs. Whether a disk forms planets at large radii and, if so, the number of planets that form, depend on how much of the envelope mass is distributed at large distances from the protostar. The results of the simulations suggest that there are two modes of gas giant planet formation. The first mode occurs early in the disk's lifetime, at large radii, and through the disk instability mechanism. After the main accretion phase is over, gas giants can form in the inner disk, over a period of a million years, through the core accretion mechanism, which researchers are addressing in other studies.Thanks to R. H. Durisen, L. Mayer, and G. Lake for comments and discussions relating to this research. This study was supported in part by the University of Zurich, Institute for Theoretical Physics, and by a Swiss Federal Grant. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.AVL at NCSA, University of Illinois. || ", "hits": 218 }, { "id": 4839, "url": "https://svs.gsfc.nasa.gov/4839/", "result_type": "Animation", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Interplanetary Dust: Visualizations", "description": "This visualization depicts a region of interplanetary dust that was detected by the Juno spacecraft. The visualization begins with a solar system view of Juno departing Earth and heading to Jupiter. The camera rotates down and a region of dust is revealed between Earth and Mars. Two distinct regions of density are represented using different colors. As the camera pushes into the volume, a portion of the volume is removed to show the interior shape and how it corresponds to the orbit of Mars. || juno_22.3000_print.jpg (1024x576) [69.0 KB] || juno_22.3000_searchweb.png (320x180) [53.2 KB] || juno_22.3000_thm.png (80x40) [3.6 KB] || juno_dust_1080p30.mp4 (1920x1080) [32.3 MB] || juno_dust_1080p60.mp4 (1920x1080) [34.5 MB] || juno_dust_1080p30.webm (1920x1080) [5.9 MB] || juno_dust (3840x2160) [0 Item(s)] || juno_dust_2160p30.mp4 (3840x2160) [170.8 MB] || juno_dust_2160p60.mp4 (3840x2160) [185.7 MB] || juno_dust_1080p30.mp4.hwshow [183 bytes] || ", "hits": 63 }, { "id": 13821, "url": "https://svs.gsfc.nasa.gov/13821/", "result_type": "Produced Video", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Discovers Mars’ Dust Storms Fill Solar System", "description": "NASA’s Juno spacecraft has made a serendipitous discovery: Mars may be ejecting dust into space, creating an interplanetary dust cloud that reflects sunlight, and which can be seen from Earth as the zodiacal light. Complete transcript available.Original musical score by Vangelis, used with permission.Watch this video on the NASA Goddard YouTube channel. || JunoDustCloudPreview_print.jpg (1024x576) [80.3 KB] || JunoDustCloudPreview.png (3840x2160) [8.3 MB] || JunoDustCloudPreview_searchweb.png (320x180) [47.0 KB] || JunoDustCloudPreview_thm.png (80x40) [3.5 KB] || YOUTUBE_1080_13821_Juno_Dust_MASTER_youtube_1080.mp4 (1920x1080) [147.0 MB] || FACEBOOK_720_13821_Juno_Dust_MASTER_facebook_720.mp4 (1280x720) [116.1 MB] || TWITTER_720_13821_Juno_Dust_MASTER_twitter_720.mp4 (1280x720) [19.5 MB] || 13821_Juno_Dust_MASTER.webm (960x540) [41.5 MB] || 13821_Juno_Dust_MASTER.mov (3840x2160) [10.4 GB] || 13821_Juno_Dust_MASTER.mp4 (3840x2160) [888.4 MB] || 13821_Juno_Dust_Captions.en_US.srt [1.8 KB] || 13821_Juno_Dust_Captions.en_US.vtt [1.7 KB] || ", "hits": 138 }, { "id": 20321, "url": "https://svs.gsfc.nasa.gov/20321/", "result_type": "Animation", "release_date": "2021-03-09T14:00:00-05:00", "title": "Juno Interplanetary Dust: Animations", "description": "Juno during its outbound cruise to Jupiter. Available with and without text. || Juno_Animation_Shot01.00090_print.jpg (1024x576) [53.0 KB] || Juno_Animation_Shot01.00090_searchweb.png (320x180) [40.0 KB] || Juno_Animation_Shot01.00090_thm.png (80x40) [2.4 KB] || Juno_Animation_Shot01.mp4 (3840x2160) [10.3 MB] || Juno_Animation_Shot01 (3840x2160) [0 Item(s)] || Juno_Animation_Shot01_Textless (3840x2160) [0 Item(s)] || Juno_Animation_Shot01.webm (3840x2160) [1.6 MB] || Juno_Animation_Shot01_.mov (3840x2160) [963.3 MB] || Juno_Animation_Shot01_Textless.mov (3840x2160) [962.7 MB] || ", "hits": 100 }, { "id": 13805, "url": "https://svs.gsfc.nasa.gov/13805/", "result_type": "Produced Video", "release_date": "2021-02-22T11:00:00-05:00", "title": "Swift Links Neutrino to Star-destroying Black Hole", "description": "Watch how a monster black hole ripping apart a star may have launched a ghost particle toward Earth. Astronomers have long predicted that tidal disruption events could produce high-energy neutrinos, nearly massless particles from outside our galaxy traveling close to the speed of light. One recent event, named AT2019dsg, provides the first proof this prediction is true but has challenged scientists’ assumptions of where and when these elusive particles might form during these destructive outbursts. Credit: NASA’s Goddard Space Flight CenterMusic: \"Diagnostic Report\" from Universal Production MusicComplete transcript available. || AT2019dsg_prores_still.jpg (1920x1080) [299.2 KB] || AT2019dsg_prores_still_print.jpg (1024x576) [119.5 KB] || AT2019dsg_prores_still_searchweb.png (180x320) [42.6 KB] || AT2019dsg_prores_still_web.png (320x180) [42.6 KB] || AT2019dsg_prores_still_thm.png (80x40) [4.1 KB] || AT2019dsg_HQ.mp4 (1920x1080) [347.5 MB] || AT2019dsg_LQ.mp4 (1920x1080) [191.3 MB] || AT2019dsg_prores.mov (1920x1080) [1.7 GB] || AT2019dsg_LQ.webm (1920x1080) [21.5 MB] || AT2019dsg_LQ.en_US.srt [3.7 KB] || AT2019dsg_LQ.en_US.vtt [3.7 KB] || ", "hits": 95 }, { "id": 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": 360 } ] }