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        {
            "id": 20412,
            "url": "https://svs.gsfc.nasa.gov/20412/",
            "result_type": "Animation",
            "release_date": "2026-01-21T11:00:00-05:00",
            "title": "Artemis II Flight Path Animations",
            "description": "Animated Flight Path of Artemis II and comparison with NASA's Lunar Reconnaissance Orbiter and the Apollo mission orbits.",
            "hits": 121802
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        {
            "id": 14922,
            "url": "https://svs.gsfc.nasa.gov/14922/",
            "result_type": "Produced Video",
            "release_date": "2025-12-01T14:00:00-05:00",
            "title": "Anatomy of an Active Galactic Nucleus",
            "description": "An active galactic nucleus, or AGN, is a supermassive black hole at the center of a galaxy that is consuming surrounding matter. Although the black hole itself is not visible, the structures around it emit light across many wavelengths. The artist’s concepts here highlight distinct structures that can accompany an AGN — the photon ring, accretion disk, corona, dusty torus, and relativistic jets. || ",
            "hits": 413
        },
        {
            "id": 14905,
            "url": "https://svs.gsfc.nasa.gov/14905/",
            "result_type": "Produced Video",
            "release_date": "2025-11-28T09:00:00-05:00",
            "title": "Black Hole Environments, Explained",
            "description": "If light can’t escape black holes, how do we know where they are? The regions around them tell an incredible story. From blazing coronas and swirling accretion disks to powerful jets that stretch millions of miles, these extreme environments reveal black holes' secrets and how these mysterious objects shape the universe.Join host Sophia Roberts as she talks with researchers Jenna Cann and Cecilia Chirenti at NASA Goddard about how scientists study these mysterious structures, the challenges of observing the unseeable, and the discoveries that continue to change our understanding of black holes.Credit: NASA’s Goddard Space Flight CenterMusic credits from Universal Production Music:\"Breaking the Barrier,\" David Bertrand Holland\"Dust Spirals,\" Alexandre Prodhomme\"Miniature Universe,\" Geoffrey Wilkinson\"Urban Decay,\" Sarah Natasha Penelope Warne\"Solar Plexus,\" Brandon Seliga\"Polygraph,\" Eric Chevalier\"The Mischief Makers,\" Joaquim Badia\"Maelstrom Dream,\" Lucie Rose\"The Truth Will Out,\" Chris Dony and Beth Perry || 14905_-_BHE_Thumbnail.jpg (1280x720) [947.8 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.srt [15.7 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.vtt [14.8 KB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_1080.mp4 (1920x1080) [1.7 GB] || FINAL_-_14905_Black_Hole_Enviroments_Explained_4k.mp4 (3840x2160) [9.2 GB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_ProRes.mov (3840x2160) [39.3 GB] || ",
            "hits": 187
        },
        {
            "id": 14873,
            "url": "https://svs.gsfc.nasa.gov/14873/",
            "result_type": "Produced Video",
            "release_date": "2025-07-22T17:00:00-04:00",
            "title": "Lagrange Point 1 Animation",
            "description": "Lagrange points are positions in space where objects sent there tend to stay put. At Lagrange points, the gravitational pull of two large masses precisely equals the centripetal force required for a small object to move with them. These points in space can be used by spacecraft to reduce fuel consumption needed to remain in position.Of the five Lagrange points, three are unstable and two are stable. The unstable Lagrange points - labeled L1, L2 and L3 - lie along the line connecting the two large masses. The stable Lagrange points - labeled L4 and L5 - form the apex of two equilateral triangles that have the large masses at their vertices. L4 leads the orbit of earth and L5 follows.The L1 point of the Earth-Sun system affords an uninterrupted view of the Sun and will be home to three new heliophysics missions in 2025 - NASA's Interstellar Mapping and Acceleration Probe (IMAP), NASA's Carruthers Geocorona Observatory, and NOAA's Space Weather Follow On-Lagrange 1 (SWFO-L1). || ",
            "hits": 746
        },
        {
            "id": 14856,
            "url": "https://svs.gsfc.nasa.gov/14856/",
            "result_type": "Infographic",
            "release_date": "2025-06-20T10:00:00-04:00",
            "title": "Roman Space Telescope to Scale with Tyrannosaurus rex",
            "description": "A comparison of the Nancy Grace Roman Space Telescope with a Tyrannosaurus rex. They have the same approximate length and weight.",
            "hits": 57
        },
        {
            "id": 31353,
            "url": "https://svs.gsfc.nasa.gov/31353/",
            "result_type": "Animation",
            "release_date": "2025-06-09T18:59:59-04:00",
            "title": "Supermassive Black Holes",
            "description": "In this video NuSTAR (Nuclear Spectroscopic Telescope Array) lead scientist Peter Boorman explains how the NuSTAR penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)",
            "hits": 239
        },
        {
            "id": 14799,
            "url": "https://svs.gsfc.nasa.gov/14799/",
            "result_type": "Produced Video",
            "release_date": "2025-05-27T20:54:00-04:00",
            "title": "Astrophysics: Observing the Universe Vertical Video",
            "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.",
            "hits": 464
        },
        {
            "id": 14786,
            "url": "https://svs.gsfc.nasa.gov/14786/",
            "result_type": "Animation",
            "release_date": "2025-02-20T00:00:00-05:00",
            "title": "Swift Spacecraft Animations: 2025",
            "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || ",
            "hits": 95
        },
        {
            "id": 14771,
            "url": "https://svs.gsfc.nasa.gov/14771/",
            "result_type": "Produced Video",
            "release_date": "2025-01-24T14:00:00-05:00",
            "title": "PUNCH Instruments",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ",
            "hits": 88
        },
        {
            "id": 14683,
            "url": "https://svs.gsfc.nasa.gov/14683/",
            "result_type": "Produced Video",
            "release_date": "2024-10-15T13:30:00-04:00",
            "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period",
            "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ",
            "hits": 820
        },
        {
            "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": 376
        },
        {
            "id": 31302,
            "url": "https://svs.gsfc.nasa.gov/31302/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-08-02T00:00:00-04:00",
            "title": "NASA's Balloon Program",
            "description": "Scientific Balloon Program Infographic || nasa-scientific-balloon-facts_print.jpg (1024x576) [171.2 KB] || nasa-scientific-balloon-facts.png (3840x2160) [3.0 MB] || nasa-scientific-balloon-facts_searchweb.png (320x180) [58.8 KB] || nasa-scientific-balloon-facts_thm.png (80x40) [6.3 KB] || nasas-balloon-program-infographic.hwshow [280 bytes] || ",
            "hits": 263
        },
        {
            "id": 14584,
            "url": "https://svs.gsfc.nasa.gov/14584/",
            "result_type": "Produced Video",
            "release_date": "2024-05-08T09:00:00-04:00",
            "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy",
            "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ",
            "hits": 147
        },
        {
            "id": 14574,
            "url": "https://svs.gsfc.nasa.gov/14574/",
            "result_type": "Produced Video",
            "release_date": "2024-05-06T10:00:00-04:00",
            "title": "Black Hole Week 2024 Poster and Media",
            "description": "In this movie-style poster, the viewer gets the feeling of being on a precipice, teetering just on the edge of a black hole’s event horizon.",
            "hits": 235
        },
        {
            "id": 14492,
            "url": "https://svs.gsfc.nasa.gov/14492/",
            "result_type": "Produced Video",
            "release_date": "2024-01-05T08:50:00-05:00",
            "title": "XRISM Reveals Its First Look at X-ray Cosmos",
            "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ",
            "hits": 145
        },
        {
            "id": 20388,
            "url": "https://svs.gsfc.nasa.gov/20388/",
            "result_type": "Animation",
            "release_date": "2023-12-05T14:00:00-05:00",
            "title": "PUNCH Spacecraft Beauty Passes",
            "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in Sun-synchronous, low Earth orbit that will make global, 3D observations of the young solar wind, from the outermost solar atmosphere to the inner heliopshere. Images of unprecedented quality will help to close a 60-year gap in measurements of understanding of what occurs in this region of space. PUNCH will share a ride to space with NASA’s Jet Propulsion Laboratory’s Spectro-Photometer for the History of the Universe, Epoch of Re-ionization, and Ices Explorer (SPHEREx) mission. The missions launched on March 11, 2025, on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.Get the latest updates on NASA's PUNCH blog. || ",
            "hits": 63
        },
        {
            "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": 218
        },
        {
            "id": 14401,
            "url": "https://svs.gsfc.nasa.gov/14401/",
            "result_type": "Produced Video",
            "release_date": "2023-10-31T10:00:00-04:00",
            "title": "NASA’s Eclipse Art",
            "description": "“The greatest scientists are artists as well.” ~Albert EinsteinArt and science have been treated as separate disciplines but have more in common than is often realized. Creativity is critical to making scientific breakthroughs, and art is often an expression (or product) of scientific knowledge. And both art and science begin in the experience of awe, of beholding something grand. The experience of a solar eclipse is a prime example of where these two human endeavors meet.Eclipses are celestial events we can predict with extreme precision, and their occurrence reveals fundamental truths about our place in the universe. Yet, as many eclipse watchers will attest, there is no anticipating how you will feel when experiencing one. The emotional resonance of eclipses is underlined by their presence in artforms in cultures across the world going back millennia.To celebrate the special role of eclipses in connecting art and science, creatives across NASA will be sharing their eclipse-inspired artwork in anticipation of two solar eclipses that will cross the United States on October 14, 2023, and April 8, 2024.The first two pieces in the series are presented below, with short biographies of their creators. || ",
            "hits": 83
        },
        {
            "id": 20378,
            "url": "https://svs.gsfc.nasa.gov/20378/",
            "result_type": "Animation",
            "release_date": "2023-09-19T18:00:00-04:00",
            "title": "Long Gamma-Ray Burst",
            "description": "Complete animation sequence.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GRB_Sequence_Still.jpg (3840x2160) [1.6 MB] || 20378_GRB_Sequence_1080.mp4 (1920x1080) [41.7 MB] || 20378_GRB_Sequence_4k.mp4 (3840x2160) [109.7 MB] || 20378_GRB_Sequence_ProRes_3840x2160_30.mov (3840x2160) [1.4 GB] || ",
            "hits": 328
        },
        {
            "id": 14363,
            "url": "https://svs.gsfc.nasa.gov/14363/",
            "result_type": "Produced Video",
            "release_date": "2023-09-12T09:55:00-04:00",
            "title": "Hubble Science: Expansion Rate: The Hubble Tension",
            "description": "When the Hubble Space Telescope launched, one of its main goals was to measure the rate at which our universe is expanding. That rate is called the “Hubble Constant” – named after the astronomer Edwin Hubble, who contributed to the discovery of the universe’s expansion. However, the expected value of the expansion rate is different depending on what equipment is being used to determine it.In this video, Nobel Laureate Dr. Adam Riess explains this phenomenon known as “Hubble Tension,” and how important this mystery is to our understanding of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Dark Energy Expansion GraphCredit: NASA's Goddard Space Flight Center Dark Energy Expansion Animation Credit: NASA's Goddard Space Flight Center Conceptual Image Lab Hubble Extreme Deep Field Fly ThroughCredit: NASA, ESA, and F. Summers, L. Frattare, T. Davis, Z. Levay, and G. Bacon (Viz3D Team, STScI) James Webb Space Telescope AnimationsCredit: NASA's Goddard Space Flight Center Conceptual Image Lab Music Credit:“Alpha and Omega” by Laurent Parisi [SACEM] via KTSA Publishing [SACEM] and Universal Production Music“Cosmic Call” by Immersive Music (Via Shutterstock Music) || ",
            "hits": 132
        },
        {
            "id": 20381,
            "url": "https://svs.gsfc.nasa.gov/20381/",
            "result_type": "Animation",
            "release_date": "2023-08-30T16:30:00-04:00",
            "title": "OSIRIS-REx Sample Return: Animations",
            "description": "Ride along with OSIRIS-REx on the thrilling finale of its journey to Bennu and back.Universal Production Music: “Rise to the Challenge” by Daniel Marantz and Michael James Burns, Raydia Music library [PRS]; “Fragments of Time” by Timothy Robert Shortell, Scores of Hypersonic Music [BMI]Watch this video on the NASA.gov Video YouTube channel. || Shot11_DivertBurn_Thumbnail_print.jpg (1024x576) [63.3 KB] || Shot11_DivertBurn_Thumbnail.jpg (3840x2160) [1.1 MB] || Shot11_DivertBurn_Thumbnail.png (3840x2160) [9.9 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_720.mp4 (1280x720) [42.8 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_1080.mp4 (1920x1080) [298.0 MB] || 20381_OSIRIS-REx_RETURN_MONTAGE_4K.mp4 (3840x2160) [2.9 GB] || 20381_OSIRIS-REx_RETURN_MONTAGE_ProRes.mov (3840x2160) [20.4 GB] || ",
            "hits": 276
        },
        {
            "id": 14358,
            "url": "https://svs.gsfc.nasa.gov/14358/",
            "result_type": "Produced Video",
            "release_date": "2023-08-17T12:55:00-04:00",
            "title": "Hubble Science: Gravitational Waves: Ripples In Space-Time",
            "description": "Gravitational waves are invisible ripples in the fabric of space-time. They are caused by some of the most violent and energetic events in the universe. These include colliding black holes, collapsing stellar cores, merging neutron stars or white dwarf stars, the wobble of neutron stars that are not perfect spheres and possibly even the remnants of gravitational radiation created by the birth of the universe.In this video, Dr. Padi Boyd explains gravitational waves and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSF. LIGO Interferometer IllustrationCredit: LIGO/T. Pyle Gravitational Wave AnimationCredit: NASA GSFC Conceptual Image Lab Kilonova AnimationCredit: NASA GSFC Conceptual Image Lab Ripples In Space Time AnimationCredit: LIGO/T. Pyle LIGO Hanford Aerial & InteriorCredit: Caltech/MIT/LIGO LabMusic Credit:“Alpha and Omega” by Laurent Parisi [SACEM] via KTSA Publishing [SACEM] and Universal Production Music“Cosmic Call” by Immersive Music (Via Shutterstock Music) || ",
            "hits": 243
        },
        {
            "id": 14328,
            "url": "https://svs.gsfc.nasa.gov/14328/",
            "result_type": "Produced Video",
            "release_date": "2023-07-28T09:55:00-04:00",
            "title": "Hubble Science: Multiwavelength Astronomy, The Big Picture",
            "description": "Until the 20th century, astronomers learned virtually all they knew about sources in the sky from only the tiny fraction of electromagnetic radiation that is visible to the eye. However, as astronomers have discovered how to collect radiation outside this part of the spectrum, they have been able to learn much more about the universe. Many objects reveal different aspects of their composition and behavior at different wavelengths. Other objects are completely invisible at one wavelength, yet are clearly visible at another.In this video, Dr. Padi Boyd explains the exciting future of multiwavelength astronomy and how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credit:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Electromagnetic Spectrum GraphicCredit: NASA GSFC Conceptual Image Lab James Webb Space Telescope AnimationCredit: NASA GSFC Conceptual Image LabMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Cosmic Call” by Immersive Music (Via Shutterstock Music) || ",
            "hits": 37
        },
        {
            "id": 14335,
            "url": "https://svs.gsfc.nasa.gov/14335/",
            "result_type": "Produced Video",
            "release_date": "2023-05-01T10:45:00-04:00",
            "title": "NASA Animation Sizes Up the Universe’s Biggest Black Holes",
            "description": "All monster black holes are not equal. Watch this video to see how they compare to each other and to our solar system. The black holes shown, which range from 100,000 to more than 60 billion times our Sun’s mass, are scaled according to the sizes of their shadows – a circular zone about twice the size of their event horizons. Only one of these colossal objects resides in our own galaxy, and it lies 26,000 light-years away. Smaller black holes are shown in bluish colors because their gas is expected to be hotter than that orbiting larger ones. Scientists think all of these objects shine most intensely in ultraviolet light. Credit: NASA's Goddard Space Flight Center Conceptual Image LabMusic: \"In the Stars\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SMBH_Scale_Still_1.jpg (3840x2160) [3.0 MB] || SMBH_Scale_Still_1_searchweb.png (180x320) [71.4 KB] || SMBH_Scale_Still_1_thm.png (80x40) [4.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.mp4 (1920x1080) [166.0 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080.mp4 (1920x1080) [102.7 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_1080_Best.webm (1920x1080) [13.3 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_ProRes_3840x2160_60.mov (3840x2160) [12.6 GB] || 14335_Supermassive_Black_Hole_Scale_Comparison_V2_4k_Best.mp4 (3840x2160) [314.2 MB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.srt [2.2 KB] || 14335_Supermassive_Black_Hole_Scale_Comparison_SRT_Captions.en_US.vtt [2.2 KB] || ",
            "hits": 1755
        },
        {
            "id": 14267,
            "url": "https://svs.gsfc.nasa.gov/14267/",
            "result_type": "Produced Video",
            "release_date": "2023-01-19T09:55:00-05:00",
            "title": "Hubble Science: Planetary Missions, Fossils of our Solar System",
            "description": "When the Hubble Space Telescope launched, one of its main goals was to learn more about our incredible universe.While we’re used to Hubble images coming from thousands of light-years away, Hubble is also capable of looking at objects in our solar system. Using Hubble, astronomers have been able to help planetary missions, like New Horizons and Lucy, plan out their own discoveries. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationsCredit: M. Kornmesser (ESA/Hubble)  Lucy Mission AnimationsCredit: NASA GSFC Conceptual Image Lab & NASA’s Scientific Visualization Studio New Horizons AnimationsCredit: NASA/JHUAPLMusic Credits:“Cosmic Call” by Immersive Music via Shutterstock Music“Night Call” by Timothy Paul Handels [SABAM] via Pedigree Cuts [PRS] and Universal Production Music || ",
            "hits": 28
        },
        {
            "id": 20374,
            "url": "https://svs.gsfc.nasa.gov/20374/",
            "result_type": "Animation",
            "release_date": "2022-12-12T00:00:00-05:00",
            "title": "XRISM Beauty Shots",
            "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ",
            "hits": 52
        },
        {
            "id": 14243,
            "url": "https://svs.gsfc.nasa.gov/14243/",
            "result_type": "Produced Video",
            "release_date": "2022-11-18T10:00:00-05:00",
            "title": "Hubble Science: Hubble Constant, An Expanding Universe",
            "description": "When the Hubble Space Telescope launched, one of its main goals was to measure the rate at which our universe is expanding. That rate is called the “Hubble Constant” – named after the astronomer Edwin Hubble, who contributed to the discovery of the universe’s expansion. Using the Hubble Space Telescope, astronomers have been able to measure the Hubble Constant and even found out that the expansion rate of our universe is accelerating due to a mysterious force known as dark energy.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Video Credits:Hubble Space Telescope AnimationCredit: M. Kornmesser (ESA/Hubble) Dark Energy Expansion GraphCredit: NASA's Goddard Space Flight Center Dark Energy Expansion Animation Credit: NASA's Goddard Space Flight Center Conceptual Image Lab Hubble Extreme Deep Field Fly ThroughCredit: NASA, ESA, and F. Summers, L. Frattare, T. Davis, Z. Levay, and G. Bacon (Viz3D Team, STScI) James Webb Space Telescope AnimationsCredit: NASA's Goddard Space Flight Center Conceptual Image LabMusic Credits:“Cosmic Call” by Immersive Music via Shutterstock Music“Alpha and Omega” by Laurent Parisi [SACEM] via KTSA Publishing [SACEM] and Universal Production Music || ",
            "hits": 212
        },
        {
            "id": 20371,
            "url": "https://svs.gsfc.nasa.gov/20371/",
            "result_type": "Animation",
            "release_date": "2022-10-28T14:00:00-04:00",
            "title": "BurstCube Animations",
            "description": "BurstCube is a mission under development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. This CubeSat will detect short gamma-ray bursts, which are important sources for gravitational wave discoveries and multimessenger astronomy. The satellite is expected to launch in 2023. || ",
            "hits": 35
        },
        {
            "id": 20372,
            "url": "https://svs.gsfc.nasa.gov/20372/",
            "result_type": "Animation",
            "release_date": "2022-10-19T00:00:00-04:00",
            "title": "Lucy Earth Gravity Assist One: Animations",
            "description": "NASA’s Lucy mission is heading to the Jupiter Trojans – two swarms of primitive asteroids trapped in Jupiter’s orbit that may hold clues to the formation of the planets. Lucy launched on October 16, 2021, spent a year in orbit around the Sun, and returned home on its launch anniversary for the first of three Earth gravity assists. The maneuver boosted Lucy’s speed and elongated its orbit around the Sun, setting it track for a second flyby of Earth in December 2024. This page provides artist concept animations depicting Lucy’s first Earth gravity assist.Learn more about Lucy's first Earth gravity assist. || ",
            "hits": 75
        },
        {
            "id": 20362,
            "url": "https://svs.gsfc.nasa.gov/20362/",
            "result_type": "Animation",
            "release_date": "2022-07-07T15:20:00-04:00",
            "title": "Gravity on the Moon vs. Asteroid Bennu: Animation",
            "description": "The lunar surface is better at resisting impacts than the loose surface of asteroid Bennu – thanks to the Moon’s much stronger gravity. || OREX-MoonvsBennuMograph-ProRes.00240_print.jpg (1024x576) [74.2 KB] || OREX-MoonvsBennuMograph-ProRes.00240_searchweb.png (320x180) [60.3 KB] || OREX-MoonvsBennuMograph-ProRes.00240_thm.png (80x40) [4.3 KB] || OREX-MoonvsBennuMograph-ProRes_1080.mp4 (1920x1080) [58.2 MB] || 3840x2160_16x9_30p (3840x2160) [128.0 KB] || OREX-MoonvsBennuMograph-ProRes.webm (3840x2160) [8.7 MB] || OREX-MoonvsBennuMograph-ProRes.mov (3840x2160) [3.2 GB] || OREX-MoonvsBennuMograph-ProRes_4K.mp4 (3840x2160) [238.1 MB] || ",
            "hits": 271
        },
        {
            "id": 20360,
            "url": "https://svs.gsfc.nasa.gov/20360/",
            "result_type": "Animation",
            "release_date": "2022-07-07T14:30:00-04:00",
            "title": "Thirty Seconds on Asteroid Bennu: Animation",
            "description": "Data-driven animation showing how the OSIRIS-REx spacecraft impacted asteroid Bennu's surface when it touched down and collected a sample. || 20360_Orex_tag_h264_1080.00111_print.jpg (576x1024) [160.5 KB] || 20360_Orex_tag_h264_1080.00111_searchweb.png (320x180) [97.3 KB] || 20360_Orex_tag_h264_1080.00111_thm.png (80x40) [6.1 KB] || 20360_Orex_tag_h264_1080.webm (1920x1080) [13.2 MB] || 20360_Orex_tag_h264_1080.mp4 (1920x1080) [175.4 MB] || 20360_Orex_tag_h264_4K.mp4 (3840x2160) [86.5 MB] || OREx_Tag_PNG (3840x2160) [0 Item(s)] || 20360_Orex_Prores_4k.mov (3840x2160) [4.4 GB] || ",
            "hits": 187
        },
        {
            "id": 14146,
            "url": "https://svs.gsfc.nasa.gov/14146/",
            "result_type": "Produced Video",
            "release_date": "2022-05-04T00:00:00-04:00",
            "title": "Black Hole Desktop & Phone Wallpapers",
            "description": "While black holes can’t emit their own light, matter surrounding and falling toward it can create quite a light show. Here you’ll find a collection of data visualizations, illustrations, and telescope images of black hole environments. Download these phone and desktop wallpapers for your screens. || ",
            "hits": 9666
        },
        {
            "id": 20367,
            "url": "https://svs.gsfc.nasa.gov/20367/",
            "result_type": "Animation",
            "release_date": "2022-04-28T00:00:00-04:00",
            "title": "Gravitational Wave",
            "description": "Two black holes orbit around each other and generate space-time ripples called gravitational waves in this animation. As the black holes get closer, the waves increase in frequency. Eventually, the event horizons merge into a peanut-shaped object, generating one very high-frequency wave. Within a rotation, the black holes merge completely. One lower-frequency wave, called the ring down, ripples out after the merger.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || A_Gravitational_Wave_ProRes.00450_print.jpg (1024x576) [119.9 KB] || A_Gravitational_Wave_ProRes.00450_searchweb.png (320x180) [78.6 KB] || A_Gravitational_Wave_ProRes.00450_thm.png (80x40) [6.8 KB] || A_Gravitational_Wave_ProRes.mov (3840x2160) [2.2 GB] || A_Gravitational_Wave_h264.mp4 (3840x2160) [40.4 MB] || A_Gravitational_Wave (3840x2160) [128.0 KB] || A_Gravitational_Wave_ProRes.webm (3840x2160) [15.0 MB] || ",
            "hits": 267
        },
        {
            "id": 14132,
            "url": "https://svs.gsfc.nasa.gov/14132/",
            "result_type": "Produced Video",
            "release_date": "2022-04-12T00:00:00-04:00",
            "title": "Black Hole Week: Black Hole GIFs",
            "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ",
            "hits": 505
        },
        {
            "id": 14130,
            "url": "https://svs.gsfc.nasa.gov/14130/",
            "result_type": "Produced Video",
            "release_date": "2022-04-07T14:00:00-04:00",
            "title": "Fermi Searches for Gravitational Waves From Monster Black Holes",
            "description": "The length of a gravitational wave, or ripple in space-time, depends on its source, as shown in this infographic. Scientists need different kinds of detectors to study as much of the spectrum as possible.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || GravWav_Infographic_MILES_10k_vFinal_print.jpg (1024x576) [158.7 KB] || GravWav_Infographic_MILES_10k_vFinal.png (10000x5625) [2.1 MB] || GravWav_Infographic_MILES_10k_vFinal.jpg (10000x5625) [4.1 MB] || GravWav_Infographic_MILES_10k_vFinal_searchweb.png (320x180) [55.8 KB] || GravWav_Infographic_MILES_10k_vFinal_thm.png (80x40) [5.4 KB] || ",
            "hits": 98
        },
        {
            "id": 14115,
            "url": "https://svs.gsfc.nasa.gov/14115/",
            "result_type": "Produced Video",
            "release_date": "2022-03-08T13:00:00-05:00",
            "title": "NASA's NICER Tracks a Magnetar's Hot Spots",
            "description": "Explore how NASA’s Neutron star Interior Composition Explorer (NICER) tracked brilliant hot spots on the surface of an erupting magnetar – from 13,000 light-years away. Credit: NASA's Goddard Space Flight CenterMusic: \"Particles and Fields\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_Still.jpg (1920x1080) [574.3 KB] || Magnetar_Still_print.jpg (1024x576) [229.0 KB] || Magnetar_Still_searchweb.png (320x180) [66.1 KB] || Magnetar_Still_thm.png (80x40) [5.2 KB] || 14115_Merging_Magnetar_HotSpots_1080_Best.webm (1920x1080) [17.4 MB] || 14115_Merging_Magnetar_HotSpots_1080.mp4 (1920x1080) [158.9 MB] || 14115_Merging_Magnetar_HotSpots_1080_Best.mp4 (1920x1080) [382.0 MB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.srt [2.1 KB] || 14115_Migrating_Magnetar_HotSpots_1080.en_US.vtt [2.1 KB] || 14115_Merging_Magnetar_HotSpots_ProRes_1920x1080_2997.mov (1920x1080) [2.1 GB] || ",
            "hits": 202
        },
        {
            "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": 34
        },
        {
            "id": 20359,
            "url": "https://svs.gsfc.nasa.gov/20359/",
            "result_type": "Animation",
            "release_date": "2022-02-08T13:00:00-05:00",
            "title": "Migrating Magnetar Hot Spot Animations",
            "description": "Animation showing a wide view of SGR 1830, a magnetar that underwent an outburst in October 2020. NICER measurements from the first day of the event show that the X-ray emission exhibited three close peaks with every rotation. Astronomers think the triple peak occurred  when three individual surface regions much hotter than their surroundings spun into and out of our view from Earth. NICER tracked the magnetar nearly every day for more than a month. Over that time, the hot spots dimmed, drifted relative to each other, and two even merged – a phenomenon not seen before. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || 02_MAGNETAR_Wide_view_BlipOnly_Still.png (1920x1080) [2.3 MB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_print.jpg (1024x576) [44.5 KB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_searchweb.png (320x180) [52.6 KB] || 02_MAGNETAR_Wide_view_BlipOnly_Still_thm.png (80x40) [4.4 KB] || 02_MAGNETAR_Wide_view_BlipOnly_1080.mp4 (1920x1080) [36.0 MB] || 02_MAGNETAR_Wide_view_BlipOnly_web.webm (1920x1080) [3.5 MB] || 02_Magnetar_Wide_BlipOnly1 (1920x1080) [0 Item(s)] || 02_MAGNETAR_Wide_view_BlipOnly_ProRes_1920x1080_2997.mov (1920x1080) [502.4 MB] || ",
            "hits": 118
        },
        {
            "id": 13969,
            "url": "https://svs.gsfc.nasa.gov/13969/",
            "result_type": "Produced Video",
            "release_date": "2021-10-21T00:00:00-04:00",
            "title": "Geospace Dynamics Constellation",
            "description": "\"Moonstone,\" by Rainman [PRS]; Atmosphere; Universal Production Music || 13969_GDC_Mission_FINAL.mov (1920x1080) [4.9 GB] || GDC_MissionVideo_Still.png (1920x1080) [3.7 MB] || GDC_Mission_SITLL.jpg (1920x1080) [441.3 KB] || 13969_GDC_Mission_FINAL_lowres.mp4 (1280x720) [62.3 MB] || TWITTER_720_13969_GDC_Mission_FINAL_twitter_720.mp4 (1280x720) [42.8 MB] || 13969_GDC_Mission_FINAL.webm (960x540) [94.7 MB] || YOUTUBE_1080_13969_GDC_Mission_FINAL_youtube_1080.mp4 (1920x1080) [339.8 MB] || 13969_GDC_Mission_FINAL.en_US.srt [4.8 KB] || 13969_GDC_Mission_FINAL.en_US.vtt [4.6 KB] || YOUTUBE_4K_13969_GDC_Mission_FINAL_youtube_4k.mp4 (3840x2160) [1.4 GB] || ",
            "hits": 46
        },
        {
            "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": 25
        },
        {
            "id": 20356,
            "url": "https://svs.gsfc.nasa.gov/20356/",
            "result_type": "Animation",
            "release_date": "2021-08-11T00:00:00-04:00",
            "title": "Asteroid Bennu Impact Hazard: Animations",
            "description": "On September 25, 2135, an asteroid called Bennu will make a close flyby of Earth. Our planet’s gravity will tweak Bennu’s path, making it a challenge to calculate its future trajectory and the odds of a potential impact late in the 22nd century. This media resource page provides broadcast-quality animations related to asteroid Bennu’s impact hazard. Learn more from NASA.Watch the produced video on the NASA Goddard YouTube Channel. || ",
            "hits": 103
        },
        {
            "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": 93
        },
        {
            "id": 20326,
            "url": "https://svs.gsfc.nasa.gov/20326/",
            "result_type": "Animation",
            "release_date": "2020-10-20T00:00:00-04:00",
            "title": "OSIRIS-REx TAG Event: Real-time Animation",
            "description": "Real-time animation of the OSIRIS-REx Touch-And-Go (TAG) Event. This animation accurately depicts the spacecraft's journey to the surface of Bennu. || OrexTagRealtimePreview2_print.jpg (1024x576) [94.4 KB] || OrexTagRealtimePreview2.png (1920x1080) [1.5 MB] || OrexTagRealtimePreview2_searchweb.png (320x180) [58.3 KB] || OrexTagRealtimePreview2_thm.png (80x40) [4.2 KB] || Orex_Tag_1080_29.97fps.webm (1920x1080) [515.7 MB] || Slew_to_TAG_Attitude (3840x2160) [0 Item(s)] || Y_Wing (3840x2160) [0 Item(s)] || Checkpoint (3840x2160) [0 Item(s)] || Matchpoint (3840x2160) [0 Item(s)] || Slew_to_Pegasus_Attitude (3840x2160) [0 Item(s)] || Orex_Tag_4K_30fps.webm (3840x2160) [893.7 MB] || Orex_Tag_4K_30fps.mp4 (3840x2160) [5.6 GB] || Orex_Tag_1080_29.97fps.mp4 (1920x1080) [9.1 GB] || Orex_Tag_4K_ProRes_30fps.mov (3840x2160) [275.1 GB] || ",
            "hits": 103
        },
        {
            "id": 13636,
            "url": "https://svs.gsfc.nasa.gov/13636/",
            "result_type": "Produced Video",
            "release_date": "2020-09-30T10:00:00-04:00",
            "title": "Join the Hunt for New Worlds Through Planet Patrol",
            "description": "Want to hunt the skies for uncharted worlds from home? Join Planet Patrol! Watch to learn how you can collaborate with professional astronomers and analyze images from NASA's Transiting Exoplanet Survey Satellite (TESS) on your own. You'll answer questions about each TESS image and help scientists figure out if they contain signals from new worlds or planetary imposters.Credit: NASA's Goddard Space Flight Center/Conceptual Image LabMusic: \"A Wonderful Loaf\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Planet_Patrol_Still-logo_print.jpg (1024x576) [111.4 KB] || Planet_Patrol_Still-logo.jpg (3840x2160) [1.1 MB] || Planet_Patrol_Still-logo_searchweb.png (320x180) [61.9 KB] || Planet_Patrol_Still-logo_thm.png (80x40) [9.8 KB] || 13636_Planet_Patrol_Best_1080.mp4 (1920x1080) [100.9 MB] || 13636_Planet_Patrol_1080.mp4 (1920x1080) [39.6 MB] || 13636_Planet_Patrol_Best_1080.webm (1920x1080) [7.9 MB] || 13636_Planet_Patrol_ProRes_3840x2160_2997.mov (3840x2160) [3.6 GB] || 13636_Planet_Patrol_4k.mp4 (3840x2160) [114.2 MB] || 13636_Planet_Patrol_SRT_Captions.en_US.srt [878 bytes] || 13636_Planet_Patrol_SRT_Captions.en_US.vtt [890 bytes] || ",
            "hits": 79
        },
        {
            "id": 13714,
            "url": "https://svs.gsfc.nasa.gov/13714/",
            "result_type": "Produced Video",
            "release_date": "2020-09-15T13:00:00-04:00",
            "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means",
            "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ",
            "hits": 273
        },
        {
            "id": 20323,
            "url": "https://svs.gsfc.nasa.gov/20323/",
            "result_type": "Animation",
            "release_date": "2020-09-09T12:00:00-04:00",
            "title": "OSIRIS-REx Sampling Area to Scale: Animations",
            "description": "OSIRIS-REx is NASA’s first asteroid sample return mission. Its main science goal is to collect a sample of near-Earth asteroid Bennu for return to Earth in 2023. These animations show a size comparison of the planned sample collection area before arriving at Bennu (orange), and after arriving at Bennu (blue). The original mission plan envisioned a sample site with a diameter of 164 feet (50 m). However, the sampling region for site Nightingale is approximately 26 ft (8 m) in diameter. The area safe enough for the spacecraft to touch is the width of a few parking spaces. || ",
            "hits": 36
        },
        {
            "id": 20311,
            "url": "https://svs.gsfc.nasa.gov/20311/",
            "result_type": "Animation",
            "release_date": "2020-02-25T16:00:00-05:00",
            "title": "Dragonfly Animation Resource Page",
            "description": "Dragonfly on Titan || DF_End_Pan_4K_Prores.00420_print.jpg (1024x576) [77.6 KB] || DF_End_Pan_H264_1080.mp4 (1920x1080) [27.1 MB] || DF_End_Pan_4K_H264.mp4 (3840x2160) [15.4 MB] || DF_End_Pan_4K_Prores_PNG (3840x2160) [0 Item(s)] || DF_End_Pan_4K_Prores.webm (3840x2160) [7.0 MB] || DF_End_Pan_4K_Prores.mov (3840x2160) [1.7 GB] || ",
            "hits": 317
        },
        {
            "id": 13535,
            "url": "https://svs.gsfc.nasa.gov/13535/",
            "result_type": "Produced Video",
            "release_date": "2020-02-07T14:30:00-05:00",
            "title": "Solar Orbiter Science Press Briefing",
            "description": "NASA and the European Space Agency (ESA) will present Solar Orbiter, the ESA/NASA mission to the Sun, during a science press briefing on Friday, Feb. 7. 2020, at 2.30 p.m. EST. Solar Orbiter will observe the Sun with high spatial resolution telescopes and capture observations in the environment directly surrounding the spacecraft to create a one-of-a-kind picture of how the Sun can affect the space environment throughout our solar system. The spacecraft also will provide the first-ever images of the Sun’s poles and the never-before-observed magnetic environment there, which helps drive the Sun’s 11-year solar cycle and its periodic outpouring of solar storms.The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:European Space Agency• Daniel Müller, Solar Orbiter Project Scientist• Günther Hasinger, Director of ScienceNASA• Nicky Fox, Heliophysics Division Director, NASA HQ• Thomas Zurbuchen, Associate Administrator for the Science Mission Directorate, NASA HQ || ",
            "hits": 32
        },
        {
            "id": 20307,
            "url": "https://svs.gsfc.nasa.gov/20307/",
            "result_type": "Animation",
            "release_date": "2020-01-28T11:00:00-05:00",
            "title": "NASA's Conceptual Image Lab 2020 Demo Reel",
            "description": "Conceptual Image Lab Demo Reel with Text discriptions. || CILDemoReel2020Text4K.00420_print.jpg (1024x576) [33.3 KB] || CILDemoReel2020Text4K.00420_searchweb.png (320x180) [51.3 KB] || CILDemoReel2020Text4K.00420_thm.png (80x40) [4.7 KB] || CILDemoReel2020Text1080.mov (1920x1080) [362.8 MB] || CILDemoReel2020Text4K.webm (3840x2160) [87.7 MB] || CILDemoReel2020Text4K.mov (3840x2160) [867.6 MB] || ",
            "hits": 69
        },
        {
            "id": 20302,
            "url": "https://svs.gsfc.nasa.gov/20302/",
            "result_type": "Animation",
            "release_date": "2019-12-12T14:00:00-05:00",
            "title": "Mars Wind Currents Reveal a Surprising Feature - Animations",
            "description": "By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below. || 20302_MarsUpperWinds_Preview_print.jpg (1024x576) [131.1 KB] || 20302_MarsUpperWinds_Preview.jpg (3840x2160) [676.6 KB] || 20302_MarsUpperWinds_Preview_searchweb.png (320x180) [86.0 KB] || 20302_MarsUpperWinds_Preview_thm.png (80x40) [6.4 KB] || TWITTER_720_MAVEN_Mars_Terrain_Winds_twitter_720.mp4 (1280x720) [16.4 MB] || MAVEN_Mars_Terrain_Winds.webm (960x540) [39.0 MB] || YOUTUBE_1080_MAVEN_Mars_Terrain_Winds_youtube_1080.mp4 (1920x1080) [135.6 MB] || FACEBOOK_720_MAVEN_Mars_Terrain_Winds_facebook_720.mp4 (1280x720) [104.1 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4 (3840x2160) [595.8 MB] || MAVEN_Mars_Terrain_Winds.mov (3840x2160) [10.6 GB] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4.hwshow [143 bytes] || ",
            "hits": 118
        },
        {
            "id": 13303,
            "url": "https://svs.gsfc.nasa.gov/13303/",
            "result_type": "Produced Video",
            "release_date": "2019-09-05T17:00:00-04:00",
            "title": "Albedo Animation",
            "description": "This is a conceptual animation showing how polar ice reflects light from the sun. || ",
            "hits": 203
        },
        {
            "id": 13078,
            "url": "https://svs.gsfc.nasa.gov/13078/",
            "result_type": "Produced Video",
            "release_date": "2019-04-15T11:00:00-04:00",
            "title": "Water Released from Moon During Meteor Showers",
            "description": "Data from the LADEE spacecraft reveal that the lunar surface is periodically releasing water.Music provided by Killer Tracks: Virtual MemoryComplete transcript available. Watch this video on the NASA Goddard YouTube channel. || LADEE_Moon_Earth_Preview_V4_print.jpg (1024x576) [181.9 KB] || LADEE_Moon_Earth_Preview_V4.jpg (1280x720) [281.6 KB] || LADEE_Moon_Earth_Preview_V4_searchweb.png (180x320) [46.5 KB] || LADEE_Moon_Earth_Preview_V4_thm.png (80x40) [3.9 KB] || TWITTER_720_13078_LADEE_Water_Short_MASTER_twitter_720.mp4 (1280x720) [21.1 MB] || 13078_LADEE_Water_Short_MASTER.webm (960x540) [48.9 MB] || YOUTUBE_1080_13078_LADEE_Water_Short_MASTER_youtube_1080.mp4 (1920x1080) [176.0 MB] || FACEBOOK_720_13078_LADEE_Water_Short_MASTER_facebook_720.mp4 (1280x720) [134.7 MB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.srt [2.6 KB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.vtt [2.6 KB] || 13078_LADEE_Water_Short_MASTER.mp4 (3840x2160) [940.5 MB] || 13078_LADEE_Water_Short_MASTER.mov (3840x2160) [5.5 GB] || ",
            "hits": 96
        },
        {
            "id": 13112,
            "url": "https://svs.gsfc.nasa.gov/13112/",
            "result_type": "Animation",
            "release_date": "2018-12-03T10:00:00-05:00",
            "title": "Why Bennu?",
            "description": "The goal of the OSIRIS-REx mission is to collect a sample from an asteroid and bring it back to Earth. But just how did the OSIRIS-REx team choose Bennu from the over 500,000 known asteroids in the solar system? Watch this cartoon to find out!Music provided by Killer Tracks: \"Cheeky Chappy\" - James Patrick Kaleth & Ross Andrew McLean.Watch this video on the NASA Goddard YouTube channel. || WHYBENNUThumbnail.jpg (1920x1080) [462.1 KB] || WHYBENNUThumbnail_searchweb.png (320x180) [70.0 KB] || WHYBENNUThumbnail_thm.png (80x40) [6.9 KB] || 13112_WhyBennu_YouTubeHD.mp4 (1920x1080) [317.6 MB] || 13112_WhyBennu_Facebook.mp4 (1920x1080) [237.6 MB] || 13112_WhyBennu_MASTER.mov (1920x1080) [5.6 GB] || 13112_WhyBennu_YouTubeHD.webm (1920x1080) [22.3 MB] || WhyBennu_Captions.en_US.srt [4.0 KB] || WhyBennu_Captions.en_US.vtt [4.1 KB] || ",
            "hits": 39
        },
        {
            "id": 12969,
            "url": "https://svs.gsfc.nasa.gov/12969/",
            "result_type": "Produced Video",
            "release_date": "2018-06-11T10:00:00-04:00",
            "title": "Fermi Satellite Celebrates 10 Years of Discoveries",
            "description": "Watch a two-minute video on how NASA's Fermi Gamma-ray Space Telescope has revolutionized our understanding of the high-energy sky over its first 10 years in space. Credit: NASA's Goddard Space Flight CenterMusic: \"Unseen Husband\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Fermi_10_Still.jpg (1920x1080) [134.3 KB] || 12969_Fermi_10th_Short_ProRes_1920x1080_2997.mov (1920x1080) [2.3 GB] || 12969_Fermi_10th_Short_1080.m4v (1920x1080) [172.3 MB] || 12969_Fermi_10th_Short_1080p.mov (1920x1080) [259.5 MB] || 12969_Fermi_10th_Short.mp4 (1920x1080) [174.7 MB] || 12969_Fermi_10th_Short_ProRes_1920x1080_2997.webm (1920x1080) [18.7 MB] || 12969_Fermi_10th_Short_SRT_Captions.en_US.srt [3.3 KB] || 12969_Fermi_10th_Short_SRT_Captions.en_US.vtt [3.3 KB] || ",
            "hits": 104
        },
        {
            "id": 12901,
            "url": "https://svs.gsfc.nasa.gov/12901/",
            "result_type": "Produced Video",
            "release_date": "2018-05-09T13:00:00-04:00",
            "title": "NASA Spacecraft Finds New Magnetic Process in Turbulent Space",
            "description": "Though close to home, the space immediately around Earth is full of hidden secrets and invisible processes. In a new discovery reported in the journal Nature, scientists working with NASA’s Magnetospheric Multiscale spacecraft — MMS — have uncovered a new type of magnetic event in our near-Earth environment by using an innovative technique to squeeze extra information out of the data.Magnetic reconnection is one of the most important processes in the space — filled with charged particles known as plasma — around Earth. This fundamental process dissipates magnetic energy and propels charged particles, both of which contribute to a dynamic space weather system that scientists want to better understand, and even someday predict, as we do terrestrial weather.  Reconnection occurs when crossed magnetic field lines snap, explosively flinging away nearby particles at high speeds. The new discovery found reconnection where it has never been seen before — in turbulent plasma. || ",
            "hits": 72
        },
        {
            "id": 40344,
            "url": "https://svs.gsfc.nasa.gov/gallery/the-nasascientific-visualization-studio/",
            "result_type": "Gallery",
            "release_date": "2017-12-22T00:00:00-05:00",
            "title": "The NASA Scientific Visualization Studio",
            "description": "Explore data brought to life by NASA’s artists and scientists",
            "hits": 220
        },
        {
            "id": 12498,
            "url": "https://svs.gsfc.nasa.gov/12498/",
            "result_type": "Produced Video",
            "release_date": "2017-02-15T12:55:00-05:00",
            "title": "Join the Search for New Nearby Worlds",
            "description": "Join the search for new worlds in the outer reaches of our solar system and in nearby interstellar space at Backyard Worlds: Planet 9. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab/Krystofer D.J. KimMusic: \"Novelty Act\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Backyard_Worlds_Still_2.png (1920x1080) [2.1 MB] || Backyard_Worlds_Still_2.jpg (1920x1080) [303.6 KB] || Backyard_Worlds_Still_2_print.jpg (1024x576) [104.8 KB] || Backyard_Worlds_Still_2_searchweb.png (320x180) [49.5 KB] || Backyard_Worlds_Still_2_thm.png (80x40) [4.8 KB] || 12498_BackyardWorlds_FINAL_ProRes_1920x1080.mov (1920x1080) [679.1 MB] || 12498_BackyardWorlds_FINAL_youtube_hq.mov (1920x1080) [176.5 MB] || 12498_BackyardWorlds_FINAL_1080p.mov (1920x1080) [76.4 MB] || 12498_BackyardWorlds_FINAL_Compatible.m4v (960x540) [16.4 MB] || 12498_BackyardWorlds_FINAL_Good_1080.m4v (1920x1080) [51.3 MB] || 12498_BackyardWorlds_FINAL_720p.mov (1280x720) [46.9 MB] || 12498_BackyardWorlds_FINAL_Compatible.webm (960x540) [5.5 MB] || 12498_BackyardWorlds_New_SRT_Captions.en_US.srt [531 bytes] || 12498_BackyardWorlds_New_SRT_Captions.en_US.vtt [544 bytes] || ",
            "hits": 70
        },
        {
            "id": 12182,
            "url": "https://svs.gsfc.nasa.gov/12182/",
            "result_type": "Produced Video",
            "release_date": "2016-03-31T13:00:00-04:00",
            "title": "Why Do Raindrop Sizes Matter In Storms?",
            "description": "Not all raindrops are created equal. The size of falling raindrops depends on several factors, including where the cloud producing the drops is located on the globe and where the drops originate in the cloud. For the first time, scientists have three-dimensional snapshots of raindrops and snowflakes around the world from space, thanks to the joint NASA and Japan Aerospace Exploration Agency Global Precipitation Measurement (GPM) mission. With the new global data on raindrop and snowflake sizes this mission provides, scientists can improve rainfall estimates from satellite data and in numerical weather forecast models, helping us better understand and prepare for extreme weather events.Watch this video on the NASA Goddard YouTube Channel. || ",
            "hits": 138
        },
        {
            "id": 20234,
            "url": "https://svs.gsfc.nasa.gov/20234/",
            "result_type": "Animation",
            "release_date": "2016-03-07T11:00:00-05:00",
            "title": "Conceptual Image Lab Demo Reel",
            "description": "CI Lab Demo Reel || CI_Labs_Demo_-_APR_Master_print.00105.jpg (1024x576) [14.7 KB] || CI_Labs_Demo_-_APR_Master_searchweb.png (320x180) [6.0 KB] || CI_Labs_Demo_-_APR_Master_thm.png (80x40) [954 bytes] || CI_Labs_Demo_-_APR_Master.mov (1920x1080) [2.4 GB] || CI_Labs_Demo_-_H264_Master.mov (1920x1080) [119.5 MB] || CI_Labs_Demo.mp4 (1920x1074) [94.8 MB] || CI_Labs_Demo_-_H264_Master.webm (1920x1080) [20.7 MB] || CILab_demo.en_US.vtt [384 bytes] || CILab_demo.en_US.srt [370 bytes] || ",
            "hits": 33
        },
        {
            "id": 12153,
            "url": "https://svs.gsfc.nasa.gov/12153/",
            "result_type": "Produced Video",
            "release_date": "2016-02-18T11:00:00-05:00",
            "title": "WFIRST: The Best of Both Worlds",
            "description": "With a view 100 times bigger than that of NASA’s Hubble Space Telescope, the Wide Field Infrared Survey Telescope WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life.  Scientists participating in the mission discuss the spacecraft, the science, and its potential.  Slated to launch in the mid-2020s, the observatory will operate at a gravitational balance point known as Earth-sun L2, which is located about 930,000 miles from Earth and directly opposite the sun.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WfirstAfta-PrintStill2_print.jpg (1024x576) [79.3 KB] || WfirstAfta-PrintStill2.png (3840x2160) [4.7 MB] || WfirstAfta-PrintStill2_searchweb.png (320x180) [59.2 KB] || WfirstAfta-PrintStill2_thm.png (80x40) [4.6 KB] || 12153_WFIRST_Best_Both_Worlds_ProRes_1280x720_5994.mov (1280x720) [3.1 GB] || 12153_WFIRST_Best_Both_Worlds_H264_Best_1280x720_5994.mov (1280x720) [1.7 GB] || 12153_WFIRST_Best_Both_Worlds_FINAL_youtube_hq.mov (1280x720) [671.5 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.mov (1280x720) [174.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv.m4v (1280x720) [122.3 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.webm (1280x720) [25.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv_subtitles.m4v (1280x720) [122.4 MB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.srt [4.6 KB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.vtt [4.4 KB] || NASA_PODCAST_12153_WFIRST_Best_Both_Worlds_FINAL_ipod_sm.mp4 (320x240) [41.6 MB] || ",
            "hits": 68
        },
        {
            "id": 4361,
            "url": "https://svs.gsfc.nasa.gov/4361/",
            "result_type": "Visualization",
            "release_date": "2015-09-28T14:00:00-04:00",
            "title": "Does What Happens in the Arctic Stay in the Arctic?",
            "description": "This gallery was created for Earth Science Week 2015 and beyond. It includes a quick start guide for educators and first-hand stories (blogs) for learners of all ages by NASA visualizers, scientists and educators. We hope that your understanding and use of NASA's visualizations will only increase as your appreciation grows for the beauty of the science they portray, and the communicative power they hold. Read all the blogs and find educational resources for all ages at: the Earth Science Week 2015 page.It all began with my fourth grade teacher, Mrs. Benner. Back then my school had a weather station and one day she had asked me to collect wind speed and temperature data. I soon found myself in charge of the morning weather forecast and soon this was my favorite part of the day. Little did I know that in the years that would follow, I’d pursue my passion for clouds and meteorology to become a research scientist at NASA. Working at NASA is every bit as cool as it sounds! Everyday is different and I always find myself working with new scientific tools to uncover mysteries about our planet Earth. Lately I’ve been studying the cryosphere, or the world’s frozen places, where I’m using scientific visualizations to understand the impacts of climate change in the Arctic. In particular I’m focusing on melting sea ice to understand how it affects Arctic cloud formation.Arctic clouds are made up of tiny liquid droplets and ice particles that form from condensation and then freezing of water vapor. Water vapor is a necessary ingredient for Arctic cloud formation, and evaporation from the Arctic Ocean can serve as an important source of water vapor. But when sea ice sits on the Arctic Ocean it acts as a lid that prevents evaporation and may limit Arctic cloud formation. Over the past decade the amount of Arctic sea ice has declined dramatically and we think this trend may be influencing Arctic cloud formation.I created a visualization showing the hypothesized response of clouds to melting in sea ice (below). The difference between the left panel, \"Current Conditions,\" and the right panel, \"Future Conditions,\" is that less sea ice in the future leads to more evaporation, and more evaporation leads to more water vapor and increased cloudiness. This hypothesis is where I base my research, using state-of-the-art NASA satellite instruments including CALIPSO and CloudSAT. || ",
            "hits": 50
        },
        {
            "id": 11804,
            "url": "https://svs.gsfc.nasa.gov/11804/",
            "result_type": "Produced Video",
            "release_date": "2015-05-14T14:00:00-04:00",
            "title": "RXTE Data Link Pulsar Pulses with a QPO",
            "description": "This animation illustrates the direct relationship between a pulsar's X-ray pulses and its quasi-periodic oscillation (QPO), a flickering signal that hovers around certain frequencies. The QPO is shown here as a bright patch near the inner edge of the disk of gas that feeds matter to the pulsar at the center, called SAX J1808. Guided by magnetic fields, gas streaming onto the neutron star forms bright hot spots. As the pulsar spins 401 times a second, telescopes detect X-ray pulses as these locations swing into view from Earth. When the QPO orbits more slowly than the pulsar’s spin, the neutron star’s magnetic field holds back flowing gas, dimming the X-ray pulses. But during an outburst, the inner edge of the disk is forced closer to the pulsar, resulting in a faster-moving QPO and compression of the pulsar's magnetic field. When the QPO matches or bests the pulsar’s spin, more gas streams onto the neutron star, and the pulses brighten. Gas may even flow directly onto the pulsar's equatorial region, producing extra hot spots. NASA’s Rossi X-ray Timing Explorer observed this relationship during outbursts in 2002, 2005, and 2008. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || QPO_16bit_00728_print.jpg (1024x576) [96.1 KB] || QPO_16bit_00728_web.jpg (320x180) [16.6 KB] || QPO_16bit_00728_thm.png (80x40) [7.1 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || 11804_RXTE_QPO_H264_Good_1920x1080_2997.mov (1920x1080) [45.4 MB] || 11804_RXTE_QPO_MPEG4_1920X1080_2997.mp4 (1920x1080) [28.0 MB] || QPO_16bit_00728.tif (1920x1080) [11.9 MB] || 11804_RXTE_QPO_H264_Good_1920x1080_2997.webm (1920x1080) [3.9 MB] || 11804_RXTE_QPO_H264_Best_1920x1080_2997.mov (1920x1080) [240.9 MB] || 11804_RXTE_QPO_ProRes_1920x1080_2997.mov (1920x1080) [416.6 MB] || ",
            "hits": 60
        },
        {
            "id": 20192,
            "url": "https://svs.gsfc.nasa.gov/20192/",
            "result_type": "Animation",
            "release_date": "2012-09-20T00:01:00-04:00",
            "title": "Space Weather",
            "description": "This movie takes us on a space weather journey from the center of the sun to solar eruptions in the sun's atmosphere all the way to the effects of that activity near Earth. The view starts in the core of the sun where atoms fuse together to create light and energy. Next we travel toward the sun's surface, watching loops of magnetic fields rise up to break through the sun's atmosphere, the corona. In the corona is where we witness giant bursts of radiation and energy known as solar flares, as well as gigantic eruptions of solar material called coronal mass ejections or CMEs. The movie follows one of these CME's toward Earth where it impacts and compresses Earth's own protective magnetic bubble, the magnetosphere. As energy and particles from the sun funnel along magnetic field lines near Earth, they ultimately produce aurora at Earth's poles. || ",
            "hits": 63
        },
        {
            "id": 10747,
            "url": "https://svs.gsfc.nasa.gov/10747/",
            "result_type": "Produced Video",
            "release_date": "2011-04-28T09:00:00-04:00",
            "title": "Swift and Hubble Probe an Asteroid Crash",
            "description": "Late last year, astronomers noticed that an asteroid named Scheila had unexpectedly brightened and it was sporting short-lived plumes. Data from NASA's Swift satellite and Hubble Space Telescope show that these changes likely occurred after Scheila was struck by a much smaller asteroid. On Dec. 11, 2010, images from the University of Arizona's Catalina Sky Survey, a project of NASA's Near Earth Object Observations Program, revealed the Scheila to be twice as bright as expected and immersed in a faint comet-like glow. Looking through the survey's archived images, astronomers inferred the outburst began between Nov. 11 and Dec. 3. Three days after the outburst was announced, Swift's Ultraviolet/Optical Telescope (UVOT) captured multiple images and a spectrum of the asteroid. Ultraviolet sunlight breaks up the gas molecules surrounding comets; water, for example, is transformed into hydroxyl (OH) and hydrogen (H). But none of the emissions most commonly identified in comets — such as hydroxyl or cyanogen (CN) — show up in the UVOT spectrum. The absence of gas around Scheila led the Swift team to reject scenarios where exposed ice accounted for the activity.Images show the asteroid was flanked in the north by a bright dust plume and in the south by a fainter one. The dual plumes formed as small dust particles excavated by the impact were pushed away from the asteroid by sunlight. Hubble observed the asteroid's fading dust cloud on Dec. 27, 2010, and Jan. 4, 2011.The two teams found the observations were best explained by a collision with a small asteroid impacting Scheila's surface at an angle of less than 30 degrees, leaving a crater 1,000 feet across. Laboratory experiments show a more direct strike probably wouldn't have produced two distinct dust plumes. The researchers estimated the crash ejected more than 660,000 tons of dust—equivalent to nearly twice the mass of the Empire State Building.For the collision animation go to #10759. || ",
            "hits": 39
        },
        {
            "id": 1605,
            "url": "https://svs.gsfc.nasa.gov/1605/",
            "result_type": "Visualization",
            "release_date": "2000-05-03T12:00:00-04:00",
            "title": "Hurricanes as Heat Engines",
            "description": "See Conceptual Image Lab animation #10049 for additional Hurricane Heat Engines material. || ",
            "hits": 80
        }
    ]
}