{
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    "next": null,
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    "results": [
        {
            "id": 5582,
            "url": "https://svs.gsfc.nasa.gov/5582/",
            "result_type": "Visualization",
            "release_date": "2025-12-18T13:50:00-05:00",
            "title": "OSIRIS-APEX Earth Flyby September 23, 2025",
            "description": "On Sept. 23, 2025, NASA’s OSIRIS-APEX (Origins, Spectral Interpretation, Resource Identification, and Security – Apophis Explorer) mission flew within about 2,100 miles (3,400 kilometers) of Earth, part of its journey to asteroid Apophis.",
            "hits": 137
        },
        {
            "id": 5571,
            "url": "https://svs.gsfc.nasa.gov/5571/",
            "result_type": "Visualization",
            "release_date": "2025-07-22T17:00:00-04:00",
            "title": "NASA's Fleet of Active Satellites (July 2025)",
            "description": "This visualization shows the orbits of NASA satellites considered operational as of July 2025. It includes both NASA-managed missions and those operated by partner organizations.",
            "hits": 1584
        },
        {
            "id": 5419,
            "url": "https://svs.gsfc.nasa.gov/5419/",
            "result_type": "Visualization",
            "release_date": "2025-06-09T00:00:00-04:00",
            "title": "The Carruthers Geocorona Observatory at the Earth-Sun Lagrange Point 1",
            "description": "The Carruthers Geocorona Obervatory observes Earth's exosphere, or geocorona, from the Earth-Sun Lagrange Point 1.",
            "hits": 87
        },
        {
            "id": 5525,
            "url": "https://svs.gsfc.nasa.gov/5525/",
            "result_type": "Visualization",
            "release_date": "2025-04-14T13:00:00-04:00",
            "title": "Lucy Flyby of Asteroid Donaldjohanson Trajectory Visualizations",
            "description": "NASA’s Lucy mission is heading to the Jupiter Trojans – an unexplored population of asteroids considered to be the fossils of planetary formation. Along the way, Lucy is traveling through the main asteroid belt, on course to fly past 52246 Donaldjohanson on April 20, 2025.",
            "hits": 95
        },
        {
            "id": 5429,
            "url": "https://svs.gsfc.nasa.gov/5429/",
            "result_type": "Visualization",
            "release_date": "2024-12-05T10:00:00-05:00",
            "title": "Lucy Earth Gravity Assist 2 Trajectory Visualizations",
            "description": "Ride-along view of Lucy’s second Earth gravity assist (EGA). The camera follows Lucy as the spacecraft approaches the sunlit side of Earth before crossing into Earth’s shadow as it slingshots around the planet. || lucy_ega2_pov-full.02400_print.jpg (1024x576) [73.5 KB] || lucy_ega2_pov-full.02400_searchweb.png (320x180) [55.6 KB] || lucy_ega2_pov-full.02400_thm.png (80x40) [3.5 KB] || lucy_ega2_pov-full_1080p60.mp4 (1920x1080) [8.5 MB] || lucy_ega2_pov-full [0 Item(s)] || lucy_ega2_pov-full_2160p30.mp4 (3840x2160) [36.4 MB] || lucy_ega2_pov-full_2160p60.mp4 (3840x2160) [34.7 MB] || lucy_ega2_pov-full_2160p60_prores.mov (3840x2160) [3.2 GB] || lucy_ega2_pov-full_2160p60.mp4.hwshow || ",
            "hits": 178
        },
        {
            "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": 321
        },
        {
            "id": 5155,
            "url": "https://svs.gsfc.nasa.gov/5155/",
            "result_type": "Visualization",
            "release_date": "2023-10-01T00:00:00-04:00",
            "title": "Lucy - Asteroid Dinkinesh Flyby",
            "description": "A top-down view of the inner solar system, with planets shown in gray, Lucy in teal, and Dinkinesh in pink.  The Lucy/Dinkinesh close approach will occur on November 1, 2023. || lucy_dinkinesh_withDates.00385_print.jpg (1024x576) [66.1 KB] || lucy_dinkinesh_withDates.00385_searchweb.png (320x180) [54.9 KB] || lucy_dinkinesh_withDates.00385_thm.png (80x40) [4.0 KB] || lucy_dinkinesh_withDates_1080p60.mp4 (1920x1080) [3.4 MB] || lucy_dinkinesh_withDates (3840x2160) [64.0 KB] || lucy_dinkinesh_withDates_2160p60.mp4 (3840x2160) [16.0 MB] || lucy_dinkinesh_withDates_2160p30.mp4 (3840x2160) [20.0 MB] || lucy_dinkinesh_withDates.prores.mov (3840x2160) [3.0 GB] || ",
            "hits": 34
        },
        {
            "id": 5133,
            "url": "https://svs.gsfc.nasa.gov/5133/",
            "result_type": "Visualization",
            "release_date": "2023-07-26T00:00:00-04:00",
            "title": "OSIRIS-REx Return Cruise/Extended Mission to Apophis",
            "description": "Top-down view of OSIRIS-REx’s return to Earth after studying asteroid Bennu. A sample of Bennu’s surface carried by the spacecraft will be deposited at Earth on Sept. 24, 2023.  The spacecraft will then begin its extended mission - beginning the long journey towards a rendezvous with Apophis in 2029. || orex_return.02345_print.jpg (1024x576) [37.8 KB] || orex_return.02345_searchweb.png (320x180) [40.7 KB] || orex_return.02345_thm.png (80x40) [2.3 KB] || orex_return (3840x2160) [0 Item(s)] || orex_return_2160p60.mp4 (3840x2160) [125.3 MB] || orex_return_2160p60_prores.mov (3840x2160) [34.9 GB] || ",
            "hits": 176
        },
        {
            "id": 5044,
            "url": "https://svs.gsfc.nasa.gov/5044/",
            "result_type": "Visualization",
            "release_date": "2022-10-13T11:00:00-04:00",
            "title": "Lucy Earth Gravity Assist Trajectory Visualizations",
            "description": "Ride-along view of Lucy’s first Earth gravity assist (EGA).  The camera follows Lucy as the spacecraft approaches the sunlit side of Earth before crossing into Earth’s shadow as it slingshots around the planet. || lucy_ega1_pov-full.6200_print.jpg (1024x576) [64.0 KB] || lucy_ega1_pov-full_1080p60.mp4 (1920x1080) [10.6 MB] || lucy_ega1_pov-full_1080p60.webm (1920x1080) [3.3 MB] || lucy_ega1_pov-full (3840x2160) [0 Item(s)] || lucy_ega1_pov-full_2160p60.mp4 (3840x2160) [38.8 MB] || lucy_ega1_pov-full_2160p60_prores.mov (3840x2160) [4.7 GB] || ",
            "hits": 96
        },
        {
            "id": 5013,
            "url": "https://svs.gsfc.nasa.gov/5013/",
            "result_type": "Visualization",
            "release_date": "2022-08-19T13:00:00-04:00",
            "title": "Artemis III Landing Region Candidates",
            "description": "This narrated movie introduces Artemis III, reveals the mission's 13 candidate landing regions near the lunar South Pole, and briefly discusses some of the criteria that narrowed the selection to these regions.Music provided by Universal Production Music: Best Days to Come – Matteo Pagamici and Max Molling.This video can also be viewed on the NASA Goddard YouTube channel. || ArtemisIII_LandingRegions_print.jpg (1024x576) [130.2 KB] || ArtemisIII_LandingRegions_YouTubeHD.webm (1920x1080) [15.6 MB] || ArtemisIII_LandingRegions_YouTubeHD.mp4 (1920x1080) [230.8 MB] || ArtemisIII_LandingRegions_Captions.en_US.srt [3.0 KB] || ArtemisIII_LandingRegions_Captions.en_US.vtt [2.8 KB] || ArtemisIII_LandingRegions_MASTER.mov (1920x1080) [1.9 GB] || ",
            "hits": 979
        },
        {
            "id": 4957,
            "url": "https://svs.gsfc.nasa.gov/4957/",
            "result_type": "Visualization",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "Parker Solar Probe: The Origins of Switchbacks",
            "description": "Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors).  A switchback occurs when the field changes direction almost 180 degrees for a short period of time.  FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows.  The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line.  The heliospheric magnetic field lines are represented as gold. || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_print.jpg (1024x576) [114.9 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_searchweb.png (320x180) [71.7 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_thm.png (80x40) [4.5 KB] || Switchbacks20181106A (1920x1080) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4 (1920x1080) [25.7 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.webm (1920x1080) [4.4 MB] || Switchbacks20181106A (3840x2160) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.UHD3840_2160p30.mp4 (3840x2160) [100.2 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4.hwshow [229 bytes] || ",
            "hits": 132
        },
        {
            "id": 4958,
            "url": "https://svs.gsfc.nasa.gov/4958/",
            "result_type": "Visualization",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "Parker Solar Probe: Crossing the Alfven Surface",
            "description": "Split window view illustrating the orbit of Parker with the orbit trail colored based on the Mach number of the solar wind and the magnetic field lines (represented as gold) connecting back to the Sun.  The Mach number drops below unity (one) when a field line transitions between two different coronal hole regions (the blue and red regions marked on the Sun). || Parker_SolarCloseup.combo.HD1080.00480_print.jpg (1024x576) [121.9 KB] || Parker_SolarCloseup.combo.HD1080.00480_searchweb.png (320x180) [74.1 KB] || Parker_SolarCloseup.combo.HD1080.00480_thm.png (80x40) [5.2 KB] || Parker_SolarCloseup.combo.HD1080 (1920x1080) [0 Item(s)] || Parker_SolarCloseup.combo.HD1080_p30.mp4 (1920x1080) [45.8 MB] || Parker_SolarCloseup.combo.HD1080_p30.webm (1920x1080) [5.6 MB] || Parker_SolarCloseup.combo.UHD2160 (3840x2160) [0 Item(s)] || Parker_SolarCloseup.combo.UHD2160_p30.mp4 (3840x2160) [124.5 MB] || Parker_SolarCloseup.combo.HD1080_p30.mp4.hwshow [202 bytes] || ",
            "hits": 337
        },
        {
            "id": 4921,
            "url": "https://svs.gsfc.nasa.gov/4921/",
            "result_type": "Visualization",
            "release_date": "2021-08-11T13:00:00-04:00",
            "title": "Bennu 2135/2182 orbits",
            "description": "Visualization depicting the 2135 Bennu-Earth flyby.  Bennu’s orbit is represented in white.  Earth’s orbit is represented in light blue. || bennu_2135_comp_0000_print.jpg (1024x576) [35.1 KB] || bennu_2135_comp_0000_searchweb.png (320x180) [13.4 KB] || bennu_2135_comp_0000_thm.png (80x40) [4.1 KB] || bennu_2135_comp_1080p30.webm (1920x1080) [3.7 MB] || bennu_2135_comp_1080p30.mp4 (1920x1080) [1.7 MB] || bennu_2135_comp_1080p60.mp4 (1920x1080) [1.7 MB] || bennu_orbit_2135 (3840x2160) [0 Item(s)] || bennu_2135_comp_2160p30.mp4 (3840x2160) [3.4 MB] || bennu_2135_comp_2160p60.mp4 (3840x2160) [3.5 MB] || osiris-rex_animations.hwshow || ",
            "hits": 419
        },
        {
            "id": 4805,
            "url": "https://svs.gsfc.nasa.gov/4805/",
            "result_type": "Visualization",
            "release_date": "2020-12-07T10:00:00-05:00",
            "title": "Coordinated Heliosphere - How Solar Missions Work Together",
            "description": "Using Solar Orbiter, Parker Solar Probe, and other sun-observing missions, in coordinated observations, we can learn far more about the solar atmosphere which surrounds and impacts Earth and other missions in space, crewed and uncrewed. || ",
            "hits": 40
        },
        {
            "id": 4790,
            "url": "https://svs.gsfc.nasa.gov/4790/",
            "result_type": "Visualization",
            "release_date": "2020-03-20T00:00:00-04:00",
            "title": "Orbit Views of our Solar System",
            "description": "A visualization of the inner solar system from a view 25 degrees above the ecliptic.  Versions with and without planet labels. || SolarSystemOverview.oblique.inner.labels.clockSlate_EarthTarget.HD1080i.01000_print.jpg (1024x576) [79.3 KB] || SolarSystemOverview.oblique.inner.labels.clockSlate_EarthTarget.HD1080i.01000_searchweb.png (320x180) [65.7 KB] || SolarSystemOverview.oblique.inner.labels.clockSlate_EarthTarget.HD1080i.01000_thm.png (80x40) [3.1 KB] || InnerSolarSystem.oblique.labels (1920x1080) [0 Item(s)] || InnerSolarSystem.oblique.nolabels (1920x1080) [0 Item(s)] || SolarSystemOverview.oblique.inner.labels.HD1080i_p30.mp4 (1920x1080) [61.3 MB] || SolarSystemOverview.oblique.inner.nolabels.HD1080i_p30.mp4 (1920x1080) [59.3 MB] || SolarSystemOverview.oblique.inner.labels.HD1080i_p30.webm (1920x1080) [14.3 MB] || SolarSystemOverview.oblique.inner.nolabels.HD1080i_p30.webm (1920x1080) [14.0 MB] || InnerSolarSystem.oblique.labels (3840x2160) [0 Item(s)] || InnerSolarSystem.oblique.nolabels (3840x2160) [0 Item(s)] || SolarSystemOverview.oblique.inner.nolabels_2160p30.mp4 (3840x2160) [171.5 MB] || SolarSystemOverview.oblique.inner.labels_2160p30.mp4 (3840x2160) [174.9 MB] || SolarSystemOverview.oblique.inner.nolabels.HD1080i_p30.mp4.hwshow [220 bytes] || ",
            "hits": 1869
        },
        {
            "id": 4748,
            "url": "https://svs.gsfc.nasa.gov/4748/",
            "result_type": "Visualization",
            "release_date": "2019-11-18T13:00:00-05:00",
            "title": "LISA Pathfinder vs Solar System Dust",
            "description": "Trajectory of the LISA Pathfinder mission from Earth orbit to its L1 halo orbit including impacts with inner solar system dust (yellow points) and time windows along the orbit when this capability is enabled (purple).  With labels. || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_print.jpg (1024x576) [44.6 KB] || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_searchweb.png (320x180) [49.9 KB] || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_thm.png (80x40) [3.1 KB] || LISAGSE.L1View.impacts.labelfade.HD1080i_p30.mp4 (1920x1080) [47.9 MB] || L1View.impacts.labels (1920x1080) [0 Item(s)] || LISAGSE.L1View.impacts.labelfade.HD1080i_p30.webm (1920x1080) [8.5 MB] || L1View.impacts.labels (3840x2160) [0 Item(s)] || LISAGSE.L1View.impacts.labelfade_2160p30.mp4 (3840x2160) [151.6 MB] || LISAGSE.L1View.impacts.labelfade.HD1080i_p30.mp4.hwshow [210 bytes] || ",
            "hits": 29
        },
        {
            "id": 4749,
            "url": "https://svs.gsfc.nasa.gov/4749/",
            "result_type": "Visualization",
            "release_date": "2019-11-18T13:00:00-05:00",
            "title": "LISA Pathfinder Trajectory to L1",
            "description": "Trajectory of the LISA Pathfinder mission from Earth orbit to its L1 halo orbit.  With labels. || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_print.jpg (1024x576) [42.7 KB] || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_searchweb.png (320x180) [47.9 KB] || LISAGSE.L1View.GSE.AU.clockSlate_EarthTarget.UHD3840.01000_thm.png (80x40) [2.1 KB] || L1View.labels (1920x1080) [0 Item(s)] || LISAGSE.L1View.noimpacts.labelfade.HD1080i_p30.mp4 (1920x1080) [47.3 MB] || LISAGSE.L1View.noimpacts.labelfade.HD1080i_p30.webm (1920x1080) [8.5 MB] || L1View.labels (3840x2160) [0 Item(s)] || LISAGSE.L1View.noimpacts.labelfade_2160p30.mp4 (3840x2160) [148.3 MB] || LISAGSE.L1View.noimpacts.labelfade.HD1080i_p30.mp4.hwshow [212 bytes] || ",
            "hits": 43
        },
        {
            "id": 4719,
            "url": "https://svs.gsfc.nasa.gov/4719/",
            "result_type": "Visualization",
            "release_date": "2019-10-21T10:00:00-04:00",
            "title": "Lucy mission trajectory",
            "description": "Jupiter's swarms of Trojan asteroids may be remnants of the primordial material that formed the outer planets, and serve as time capsules from the birth of our Solar System more than 4 billion years ago. The Trojans orbit in two loose groups that orbit the Sun, with one group always ahead of Jupiter in its path, the other always behind. At these two Lagrange points the bodies are stabilized by the Sun and Jupiter in a gravitational balancing act.  These primitive bodies hold vital clues to deciphering the history of the solar system, and perhaps even the origins of life and organic material on Earth.Lucy will be the first space mission to study the Trojans. The mission takes its name from the fossilized human ancestor (called “Lucy” by her discoverers) whose skeleton provided unique insight into humanity's evolution. Likewise, the Lucy mission will revolutionize our knowledge of planetary origins and the formation of the solar system.Lucy will launch in October 2021 and, with boosts from Earth's gravity, will complete a twelve-year journey to eight different asteroids — a Main Belt asteroid and seven Jupiter Trojans, the last two members of a “two-for-the-price-of-one” binary system. Lucy’s complex path will take it to both clusters of Trojans and give us our first close-up view of all three major types of bodies in the swarms (so-called C-, P- and D-types). || ",
            "hits": 181
        },
        {
            "id": 4702,
            "url": "https://svs.gsfc.nasa.gov/4702/",
            "result_type": "Infographic",
            "release_date": "2019-02-11T06:00:00-05:00",
            "title": "MAVEN Aerobraking to Achieve Science and Relay Orbit",
            "description": "Aerobraking plan for MAVEN.  (left) Current MAVEN orbit around Mars — 6200-km highest altitude, and an orbit period of ~4.5 hours.  (center) Aerobraking process — MAVEN performs a series of “deep dip” orbits approaching to within ~125 km of Mars at lowest altitude, causing drag from the atmosphere slow down the spacecraft.  Over roughly three-hundred and sixty orbits spanning about two months, this slowing reduces the spacecraft’s highest altitude to ~4500 km and its orbit period to ~3.5 hours.  (right) Post-aerobraking orbit, with reduced altitude and shorter orbit period. || maven_aerobraking_comp_03_print.jpg (1024x576) [90.4 KB] || MavenAerobrakingDiagram.jpg (3840x2160) [679.4 KB] || maven_aerobraking_comp_03_searchweb.png (320x180) [38.7 KB] || maven_aerobraking_comp_03_thm.png (80x40) [4.9 KB] || maven_aerobraking_comp_03.tif (3840x2160) [23.8 MB] || ",
            "hits": 56
        },
        {
            "id": 4680,
            "url": "https://svs.gsfc.nasa.gov/4680/",
            "result_type": "Visualization",
            "release_date": "2018-10-04T00:00:00-04:00",
            "title": "Space Weather to the Edge of the Solar System - Revisited",
            "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_print.jpg (1024x576) [97.2 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_searchweb.png (320x180) [79.1 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_thm.png (80x40) [5.0 KB] || TopView (1920x1080) [0 Item(s)] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4 (1920x1080) [41.0 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.webm (1920x1080) [6.6 MB] || TopView (3840x2160) [0 Item(s)] || NewHorizons.topfixed_HAE.UHD3840_2160p30.mp4 (3840x2160) [125.3 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4.hwshow [202 bytes] || ",
            "hits": 67
        },
        {
            "id": 4653,
            "url": "https://svs.gsfc.nasa.gov/4653/",
            "result_type": "Visualization",
            "release_date": "2018-06-05T10:00:00-04:00",
            "title": "Parker Solar Probe and Solar Orbiter Trajectories",
            "description": "This visualization opens near Earth for the launch of Parker Solar Probe August 12,  2018.  Then the camera moves around the Sun to match of with Earth again for the launch of Solar Orbiter in 2020.  After that, the camera moves in a slow drift around the Sun as the orbits evolve.  The Parker Solar Probe orbit fades out after the nominal end of mission in 2025.  This version has longer orbit trails to better view orbit changes, and the red along the orbits indicate the nominal science operations portions of the missions. || ParkerAndSolarOrbiter.InnerTourDeluxe.HAE.AU.clockSlate_EarthTarget.HD1080i.02000_print.jpg (1024x576) [100.7 KB] || DeluxeTour (1920x1080) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.webm (1920x1080) [17.6 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4 (1920x1080) [179.8 MB] || DeluxeTour (3840x2160) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4 (3840x2160) [489.0 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4.hwshow [270 bytes] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4.hwshow [211 bytes] || ",
            "hits": 259
        },
        {
            "id": 4549,
            "url": "https://svs.gsfc.nasa.gov/4549/",
            "result_type": "Visualization",
            "release_date": "2017-02-09T10:00:00-05:00",
            "title": "MMS Phase 2b: Transitioning to Magnetosphere Science on the Darkside",
            "description": "Visualization of the spacecraft orbit transition from apogee at the dayside magnetopause to the nightside magnetopause. || MMSPhase2b_Pole_Jan2May2017_RE_GSE.slate_GSEtour.UHD3840.3660_print.jpg (1024x576) [103.1 KB] || MMSPhase2b_Pole_Jan2May2017_RE_GSE.slate_GSEtour.UHD3840.3660_searchweb.png (320x180) [72.9 KB] || MMSPhase2b_Pole_Jan2May2017_RE_GSE.slate_GSEtour.UHD3840.3660_thm.png (80x40) [5.2 KB] || MMSPhase2b_Pole_Jan2May2017_Fast.HD1080i_p30.webm (1920x1080) [23.0 MB] || FastVersion (1920x1080) [0 Item(s)] || MMSPhase2b_Pole_Jan2May2017_Fast.HD1080i_p30.mp4 (1920x1080) [140.4 MB] || FastVersion (3840x2160) [0 Item(s)] || MMSPhase2b_Pole_Jan2May2017.UHD3840_2160p30.mp4 (3840x2160) [449.6 MB] || MMSPhase2b_Pole_Jan2May2017_Fast.HD1080i_p30.mp4.hwshow [210 bytes] || ",
            "hits": 16
        },
        {
            "id": 4392,
            "url": "https://svs.gsfc.nasa.gov/4392/",
            "result_type": "Visualization",
            "release_date": "2015-12-08T10:00:00-05:00",
            "title": "Space Weather to the Edge of the Solar System",
            "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons2015_40AU.NoSTEREO_1080p30.01000_print.jpg (1024x576) [72.7 KB] || NewHorizons2015_40AU.NoSTEREO_1080p30.mp4 (1920x1080) [27.9 MB] || NewHorizons2015_40AU.NoSTEREO_1080p30.webm (1920x1080) [6.6 MB] || NewHorizons2015_40AU.NoSTEREO.3840x2160_p30.mp4 (3840x2160) [82.5 MB] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || NoSTEREO (3840x2160) [0 Item(s)] || space-weather-to-the-edge-of-the-solar-system-hd1080-movie.hwshow [336 bytes] || ",
            "hits": 44
        },
        {
            "id": 4342,
            "url": "https://svs.gsfc.nasa.gov/4342/",
            "result_type": "Visualization",
            "release_date": "2015-09-15T10:00:00-04:00",
            "title": "Sixteen Comets Touring the Inner Solar System",
            "description": "This visualization presents a small sample of the 9 years of comets seen by SOHO from the perspective a an observer at a fixed point above the ecliptic plane with the Sun at the center. || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [109.1 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [72.2 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_thm.png (80x40) [4.3 KB] || SixteenComets-oblique.HD1080.webm (1920x1080) [11.3 MB] || SixteenComets-oblique.HD1080.mov (1920x1080) [109.2 MB] || Oblique (1920x1080) [512.0 KB] || SixteenComets-oblique_1080p30.mp4 (1920x1080) [64.2 MB] || ",
            "hits": 48
        },
        {
            "id": 4322,
            "url": "https://svs.gsfc.nasa.gov/4322/",
            "result_type": "Visualization",
            "release_date": "2015-06-24T00:00:00-04:00",
            "title": "The Multiple CMEs of June, 2015",
            "description": "A view of multiple CMEs which erupted from the Sun in the latter half of June 2015.  Their trajectories, and potential impacts on Earth and space assets, are propagated with the Enlil model. || 2015June20_high2AU.full.0006_print.jpg (1024x576) [48.8 KB] || 2015June20_high2AU.full.0006_searchweb.png (320x180) [38.5 KB] || 2015June20_high2AU.full.0006_thm.png (80x40) [4.7 KB] || 2015June20_high2AU.full.HD1080.webm (1920x1080) [406.6 KB] || 2015June20_high2AU.full.HD1080.mov (1920x1080) [1.8 MB] || 1920x1080_16x9_10p (1920x1080) [4.0 KB] || ",
            "hits": 34
        },
        {
            "id": 4064,
            "url": "https://svs.gsfc.nasa.gov/4064/",
            "result_type": "Visualization",
            "release_date": "2013-04-12T12:00:00-04:00",
            "title": "The CME of April 11, 2013",
            "description": "The CME launched from the Sun on April 11, 2013 was modelled at the Community-Coordinated Modeling Center (CCMC) at NASA's Goddard Space Flight Center. These model runs are used for testing various space weather models and for protecting NASA assets (spacecraft AND astronauts) throughout the Solar System.Different colors of a red, green, blue color palette are used to designate different physical variables from the simulation. When the three colors combine, they create a dramatic example of how the coronal mass ejection (CME) is different from the solar wind. || ",
            "hits": 30
        },
        {
            "id": 4058,
            "url": "https://svs.gsfc.nasa.gov/4058/",
            "result_type": "Visualization",
            "release_date": "2013-03-27T00:00:00-04:00",
            "title": "Space Weather @ Mars: The CME of March 5, 2013",
            "description": "These images were produced from a space weather model known as ENLIL named after the Sumerian storm god. It shows the way a coronal mass ejection (CME) on March 5, 2013, was expected to travel. The view on the left is top down, while the one on the right shows Earth from the side.To protect their space assets from excessive radiation, NASA and other organizations research the fundamental processes behind space weather such as CMEs, integrating them into research models, which are run continuously at the Community-Coordinated Modeling Center (CCMC) at NASA Goddard.When CMEs occur on the sun, models are generated with the best event information available at the time and propagated forward to estimate regions in the solar system that might be affected. The models take about an hour or two to run. The CMEs themselves usually take one or two days to reach other planets or spacecraft.The March 5 CME moved towards Mars and the STEREO-B spacecraft (blue spacecraft icon). This allowed mission operators to take steps to protect STEREO-B as well as spacecraft operating around and on Mars. || ",
            "hits": 31
        },
        {
            "id": 4057,
            "url": "https://svs.gsfc.nasa.gov/4057/",
            "result_type": "Visualization",
            "release_date": "2013-03-25T00:00:00-04:00",
            "title": "LEND Looks for Water at the South Pole",
            "description": "Since Lunar Reconnaissance Orbiter (LRO) entered lunar orbit in 2009, its neutron detector, LEND, has been counting the neutrons coming from the Moon's surface.Neutrons are created when galactic cosmic rays strike atoms in the lunar regolith. These neutrons bounce from atom to atom like billiard balls, losing energy with each collision. Along the way, some of these neutrons escape into space, where LEND can detect them.The presence of hydrogen in the lunar soil reduces the number of neutrons that escape. To map out likely deposits of water ice, LEND scientists look for this deficit of neutrons in the epithermal (medium) energy range.If the deficit were simply due to random fluctuations, the hydrogen map would never coalesce into a sharp image, but as this animation shows, the map of epithermal neutron deficit at the south pole of the Moon improves over time and converges on particular spots. These include especially strong signals in the permanently shadowed parts of Cabeus and Shoemaker craters, where ice would be completely shielded from the sun. But LEND and other missions have found signs of water in places that aren't permanently shadowed while apparently excluding some places that are, both of which are surprising and exciting discoveries. || ",
            "hits": 336
        },
        {
            "id": 4054,
            "url": "https://svs.gsfc.nasa.gov/4054/",
            "result_type": "Visualization",
            "release_date": "2013-03-19T13:00:00-04:00",
            "title": "LAMP Observes GRAIL Impact",
            "description": "The Gravity Recovery and Interior Laboratory (GRAIL) mission comprised a pair of satellites that together measured the gravity field of the Moon. GRAIL ended its mission with a planned impact into the side of a lunar mountain on December 17, 2012. Lunar Reconnaissance Orbiter (LRO) maneuvered into an orbit that would allow it to observe the impact. One of LRO's instruments, the Lyman-Alpha Mapping Project (LAMP), looked for the chemical signatures of a number of elements, including hydrogen and mercury, in the dust plume kicked up by the impact.This animation shows the relative positions of GRAIL and LRO at the time of the impact, as well as the view from LAMP as it scanned for the dust plume. The LAMP sensor is a 6.0° x 0.3° slit that was positioned to look over the limb of the Moon, so that it would be pointed into the tenuous dust plume with only the sky in the background. This observation was possible, in part, because GRAIL impacted on the night side of the Moon, where there was no concern that LAMP's sensitive detector could be blinded by sunlit terrain. From Earth, the Moon was a waxing crescent at the time of the impact. || ",
            "hits": 37
        },
        {
            "id": 4056,
            "url": "https://svs.gsfc.nasa.gov/4056/",
            "result_type": "Visualization",
            "release_date": "2013-03-18T00:00:00-04:00",
            "title": "The CME of March 15, 2013",
            "description": "The CME launched from the Sun on March 15, 2013 was modelled at the Community-Coordinated Modeling Center (CCMC) at NASA's Goddard Space Flight Center. These model runs are used for testing various space weather models and for protecting NASA assets (spacecraft AND astronauts) throughout the Solar System.Different colors of a red, green, blue color palette are used to designate different physical variables from the simulation. When the three colors combine, they create a dramatic example of how the coronal mass ejection (CME) is different from the solar wind. || ",
            "hits": 21
        },
        {
            "id": 4010,
            "url": "https://svs.gsfc.nasa.gov/4010/",
            "result_type": "Visualization",
            "release_date": "2012-12-20T09:00:00-05:00",
            "title": "Space Weather Research: The CME of March 2012",
            "description": "Forecasting space weather is of vital importance in protecting NASA assets around the solar system. For this reason, NASA routinely tests various space weather models at the Community-Coordinated Modeling Center (CCMC).This visualization is constructed from a computer model run of a coronal mass ejection (CME) launched from the sun in early March, 2012. The preliminary CME parameters were measured from instruments on the STEREO (the red and blue satellite icons) and SDO (in Earth orbit) satellites. The Enlil model was used to propagate those parameters through the solar system. From this model, they can estimate the strength and time of arrival of the CME at various locations around the solar system. This allows other missions to either safe-mode their satellites for protection, or allow them to conduct measurements to test the accuracy of the model. || ",
            "hits": 53
        },
        {
            "id": 3966,
            "url": "https://svs.gsfc.nasa.gov/3966/",
            "result_type": "Visualization",
            "release_date": "2012-09-20T00:00:00-04:00",
            "title": "Heliospheric Future: Parker Solar Probe (formerly Solar Probe Plus) & Solar Orbiter",
            "description": "Two future missions scheduled for detailed studies of the Sun and solar atmosphere are Parker Solar Probe and Solar Orbiter.Parker Solar Probe  will move in a highly-elliptical orbit, using gravity-assists from Venus to move it closer to the Sun with each pass. The goal is to get the spacecraft to fly through the corona at a distance of 9.5 solar radii.Solar Orbiter will use Earth and Venus gravity assists to move into a relatively circular orbit, inside the orbit of Mercury for monitoring the Sun. || ",
            "hits": 47
        },
        {
            "id": 3969,
            "url": "https://svs.gsfc.nasa.gov/3969/",
            "result_type": "Visualization",
            "release_date": "2012-09-20T00:00:00-04:00",
            "title": "The 2012 Earth-Orbiting Heliophysics Fleet",
            "description": "Since Sentinels of the Heliosphere in 2008, there have been a few new missions, and a few missions have been shut down. As of Fall of 2012, here's a tour of the NASA Near-Earth Heliophysics fleet, covering the space from near-Earth orbit out to the orbit of the Moon.Revision (November 9, 2012): The RBSP mission has been renamed the Van Allen Probes. NASA Press Release.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observationsNear-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. SORCE: Monitors solar intensity across a broad range of the electromagnetic spectrum.AIM: Images and measures noctilucent clouds. SVS pageRBSP: (Renamed the Van Allen Probes) Designed to study the impact of space weather on Earth's radiation belts. SVS pageGeosynchronous Fleet:SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution.GOES: The newest GOES satellites include a solar X-ray imager operated by NOAA.Geospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of three satellites to study how magnetospheric instabilities produce substorms. Two of the original five satellites were moved into lunar orbit to become ARTEMIS. SVS page IBEX: The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause.Lunar Orbiting FleetARTEMIS: Two of the THEMIS satellites were moved into lunar orbit to study the interaction of the Earth's magnetosphere with the Moon.Note: A number of near-Earth missions had their orbits generated from Two-Line orbital elements valid in July 2012. Orbit perturbations since then may result in significant deviation from the actual satellite position for the time frame of this visualization. || ",
            "hits": 48
        },
        {
            "id": 3993,
            "url": "https://svs.gsfc.nasa.gov/3993/",
            "result_type": "Visualization",
            "release_date": "2012-09-20T00:00:00-04:00",
            "title": "STEREO's Ongoing Mission to See the Sun from All Sides",
            "description": "In 2012, the two STEREO spacecraft, Ahead (STEREO-A) and Behind (STEREO-B) continue on their orbits around the Sun. For the next several years, the spacecraft will be positioned to observe the side of the Sun not visible from the Earth. || ",
            "hits": 33
        }
    ]
}