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    "results": [
        {
            "id": 14957,
            "url": "https://svs.gsfc.nasa.gov/14957/",
            "result_type": "Produced Video",
            "release_date": "2026-01-27T10:00:00-05:00",
            "title": "IMAP Arrives at L1",
            "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) reached its destination at Lagrange point 1, or L1, approximately 1 million miles from Earth toward the Sun on Jan. 10, 2026.The mission’s operations team sent commands to the spacecraft on the morning of Jan. 9 to begin trajectory maneuvers to enter orbit at L1. Early on the morning of Jan. 10, the team confirmed the spacecraft had successfully entered its final L1 orbit, where it will stay for the duration of its mission.From L1, IMAP will explore and map the very boundaries of our heliosphere — the protective bubble created by the solar wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.Learn more about the milestone: https://science.nasa.gov/blogs/imap/2026/01/12/nasas-imap-mission-reaches-its-destination/ || ",
            "hits": 158
        },
        {
            "id": 14921,
            "url": "https://svs.gsfc.nasa.gov/14921/",
            "result_type": "Produced Video",
            "release_date": "2025-11-21T09:00:00-05:00",
            "title": "IMAP Testing and Integration at NASA’s Kennedy Space Center",
            "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) spacecraft arrived May 10, 2025, for processing at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The mission will study how the Sun shapes the boundaries of the heliosphere, the bubble around our solar system.  A semitrailer transported the spacecraft from NASA’s Marshall Space Flight Center in Huntsville, Alabama, after completing thermal vacuum testing, which simulates the harsh conditions of space, at the X-ray and Cryogenic Facility. Astrotech provides the facility and technicians to prepare the spacecraft for launch, including fueling and encapsulation.  The IMAP spacecraft launched Sept. 24, 2025, on a SpaceX Falcon 9 rocket from Launch Complex 39A at NASA Kennedy. || ",
            "hits": 74
        },
        {
            "id": 14904,
            "url": "https://svs.gsfc.nasa.gov/14904/",
            "result_type": "Produced Video",
            "release_date": "2025-09-24T12:00:00-04:00",
            "title": "NASA, NOAA Launch Three Spacecraft to Map Sun’s Influence Across Space",
            "description": "NASA and the National Oceanic and Atmospheric Administration (NOAA) launched three new missions Wednesday, Sept. 24, 2025, to investigate the Sun’s influence across the solar system.At 7:30 a.m. EDT, a SpaceX Falcon 9 rocket lifted off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida carrying the agency’s IMAP (Interstellar Mapping and Acceleration Probe), Carruthers Geocorona Observatory, and NOAA’s SWFO-L1 (Space Weather Follow On-Lagrange 1) spacecraft.Learn more about IMAP: https://science.nasa.gov/mission/imap/Learn more about Carruthers Geocorona Observatory: https://science.nasa.gov/mission/carruthers-geocorona-observatory/Learn more about SWFO-L1: https://science.nasa.gov/mission/swfo-l1/ || ",
            "hits": 178
        },
        {
            "id": 14895,
            "url": "https://svs.gsfc.nasa.gov/14895/",
            "result_type": "Produced Video",
            "release_date": "2025-09-17T10:00:00-04:00",
            "title": "Mapping the Boundaries of Our Home in Space with NASA’s IMAP Mission",
            "description": "NASA’s new Interstellar Mapping and Acceleration Probe, or IMAP, will explore and map the very boundaries of our heliosphere — a huge bubble created by the Sun's wind that encapsulates our solar system — and study how that boundary interacts with the local galactic neighborhood beyond.As a modern-day celestial cartographer, IMAP will chart the vast range of particles in interplanetary space, helping to investigate two of the most important overarching issues in heliophysics — the energization of charged particles from the Sun, and the interaction of the solar wind with interstellar space. Additionally, IMAP will support near real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. IMAP is launching no earlier than Sept. 23, 2025, aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Learn more about IMAP science: https://science.nasa.gov/missions/nasas-imap-mission-to-study-boundaries-of-our-home-in-space/Find out more about the IMAP mission: https://science.nasa.gov/mission/imap/ || ",
            "hits": 113
        },
        {
            "id": 14898,
            "url": "https://svs.gsfc.nasa.gov/14898/",
            "result_type": "Produced Video",
            "release_date": "2025-09-15T15:00:00-04:00",
            "title": "Our Home In Space Series",
            "description": "The heliosphere, the massive bubble created by our Sun, is like our “house” in space. It shelters us from harsh weather outside and regulates the environment inside. Without our heliosphere, Earth may never have developed life at all.  But there’s a lot we still don’t know about our cosmic home. How big is it, and what is it shaped like? How does it compare to the “houses” created by other stars? A new NASA mission will soon unlock answers to these questions and more.  Launching as early as Sept. 23, NASA’s Interstellar Mapping and Acceleration Probe will help us construct the “blueprints” or our home in space. This three-part series explores how we learn about our heliosphere, how it protects us, and how it advances the search for life elsewhere in the Universe. || ",
            "hits": 141
        },
        {
            "id": 5567,
            "url": "https://svs.gsfc.nasa.gov/5567/",
            "result_type": "Visualization",
            "release_date": "2025-07-21T18:59:59-04:00",
            "title": "New Missions to L1",
            "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.",
            "hits": 99
        },
        {
            "id": 13642,
            "url": "https://svs.gsfc.nasa.gov/13642/",
            "result_type": "Produced Video",
            "release_date": "2020-06-11T10:00:00-04:00",
            "title": "11 Years Charting The Edge of The Solar System",
            "description": "Watch this video on the NASA Goddard YouTube channel.Music credits: “End of Days - Joe Mason Remix” by Connor Shambrook [BMI], Cyrus Reynolds [BMI], Flynn Hase Spence [ASCAP], Joseph Scott Mason [APRA]; “Brainstorming” by Laurent Dury [SACEM]; “Flight of the Leaf Remix” by Julie Gruss [GEMA], Laurent Dury [SAXEM]; “Ticks and Thoughts” by Laurent Dury [SACEM]; “Intimate Journey” by Laurent Vernerey [SACEM], Nicolas de Ferran [SACEM] from Universal Production MusicComplete transcript available. || 13642_IBEX11years_YouTube.00214_print.jpg (1024x576) [239.3 KB] || 13642_IBEX11years_YouTube.00214_searchweb.png (320x180) [98.0 KB] || 13642_IBEX11years_YouTube.00214_thm.png (80x40) [6.7 KB] || 13642_IBEX11years_Prores-2.mov (1920x1080) [4.2 GB] || 13642_IBEX11years_YouTube.mp4 (1920x1080) [489.0 MB] || 13642_IBEX11years_Facebook.mp4 (1920x1080) [366.4 MB] || 13642_IBEX11years_Twitter.mp4 (1920x1080) [66.4 MB] || 13642_IBEX11years_YouTube.webm (1920x1080) [33.9 MB] || IBEX11years.en_US.srt [5.8 KB] || IBEX11years.en_US.vtt [5.8 KB] || ",
            "hits": 76
        },
        {
            "id": 11382,
            "url": "https://svs.gsfc.nasa.gov/11382/",
            "result_type": "Produced Video",
            "release_date": "2013-10-30T10:00:00-04:00",
            "title": "Five Years of Great Discoveries for NASA's IBEX",
            "description": "Launched on Oct. 19, 2008, the Interstellar Boundary Explorer, or IBEX, spacecraft, is unique to NASA's heliophysics fleet: it images the outer boundary of the heliosphere, a boundary at the furthest edges of the solar system, far past the planets, some 8 million miles away. There, the constant stream of solar particles flowing off the sun, the solar wind, pushes up against the interstellar material flowing in from the local galactic neighborhood.IBEX is also different because it creates images from particles instead of light. IBEX, scientists create maps from the observed neutral atoms. Some are of non-solar origin, others were created by collisions of solar wind particles with other neutral atoms far from the sun. Observing where these energetic neutral atoms, or ENAs, come from describes what's going on in these distant regions. Over the course of six months and many orbits around Earth, IBEX can paint a picture of the entire sky in ENAs.During its first five years, IBEX has made some astounding discoveries.IBEX is a NASA Heliophysics Small Explorer mission. The Southwest Research Institute in San Antonio, Texas, leads IBEX with teams of national and international partners. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program for the agency's Science Mission Directorate in Washington. || ",
            "hits": 39
        },
        {
            "id": 4087,
            "url": "https://svs.gsfc.nasa.gov/4087/",
            "result_type": "Visualization",
            "release_date": "2013-07-10T13:00:00-04:00",
            "title": "IBEX Heliotail Observations",
            "description": "The IBEX (Interstellar Boundary EXplorer) continues to collect data on the flux of neutral atoms from the boundary of the solar wind with the interstellar medium.Starting with the IBEX satellite in orbit around the Earth, we zoom out to beyond the orbit of Neptune, illustrating the direction of the Sun relative to the local stars (red arrow) and relative to the local interstellar medium (violet arrow). These directions are different because the local interstellar medium (mostly gas and dust) move relative to the local stars.The boundaries of the termination shock (red ellipsoidal surface) and heliopause (green) created by the interaction of the solar wind with the interstellar medium is displayed. The camera rotates to a view 'nose on' with the heliopause, and a sphere is faded in representing the region where the neutral atoms detected by IBEX originate. The sphere around the Sun is 'unwrapped' to reproject the IBEX data into an approximately Aitoff projection. || ",
            "hits": 70
        }
    ]
}