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        {
            "id": 14667,
            "url": "https://svs.gsfc.nasa.gov/14667/",
            "result_type": "Produced Video",
            "release_date": "2024-08-22T14:00:00-04:00",
            "title": "ESCAPADE Instrument Build and Testing",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
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        {
            "id": 14665,
            "url": "https://svs.gsfc.nasa.gov/14665/",
            "result_type": "Produced Video",
            "release_date": "2024-08-21T09:00:00-04:00",
            "title": "ESCAPADE Spacecraft Development Images",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ",
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        },
        {
            "id": 14641,
            "url": "https://svs.gsfc.nasa.gov/14641/",
            "result_type": "Infographic",
            "release_date": "2024-07-30T15:00:00-04:00",
            "title": "ESCAPADE Mission Posters",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 51
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        {
            "id": 14642,
            "url": "https://svs.gsfc.nasa.gov/14642/",
            "result_type": "Infographic",
            "release_date": "2024-07-30T15:00:00-04:00",
            "title": "ESCAPADE Spacecraft Specifications",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission, led by Rob Lillis at the University of California, Berkeley, Space Sciences Laboratory (UCBSSL), is a twin-spacecraft science mission that will orbit two spacecraft around Mars to understand the structure, composition, variability, and dynamics of Mars' unique hybrid magnetosphere. The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time. ESCAPADE is being developed under NASA’s Small Innovative Missions for Planetary Exploration (SIMPLEx) program in the Science Mission Directorate (SMD). The mission is led by UCBSSL with spacecraft design provided by Rocket Lab.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ",
            "hits": 187
        },
        {
            "id": 14635,
            "url": "https://svs.gsfc.nasa.gov/14635/",
            "result_type": "Produced Video",
            "release_date": "2024-07-22T12:00:00-04:00",
            "title": "ESCAPADE Mission Spacecraft Beauty Passes",
            "description": "NASA’s Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will study the interaction between the solar wind and Martian atmosphere. Two identical spacecraft will orbit around the Red Planet to understand the structure, composition, variability, and dynamics of Mars’ unique hybrid magnetosphere, including its real-time response to space weather.The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time — so much that Mars no longer supports liquid water on its surface. The pair will be the first coordinated multi-spacecraft orbital science mission to Mars.ESCAPADE is part of the NASA Small Innovative Missions for Planetary Exploration (SIMPLEx) program. The mission is managed by the University of California Berkeley’s Space Sciences Laboratory, with key partners Rocket Lab, NASA Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 142
        },
        {
            "id": 13655,
            "url": "https://svs.gsfc.nasa.gov/13655/",
            "result_type": "Produced Video",
            "release_date": "2020-07-23T06:00:00-04:00",
            "title": "Countdown to Mars! NASA's Perseverance Rover Launch Live Shots",
            "description": "Click HERE for quick link to b-roll. For more about the Mars 2020 Perseverance Rover, including quick facts, interviews, and additional images and videos check out https://mars.nasa.gov/mars2020/.Count down is on! Check out b-roll of the rocket being rolled out to the launch pad here.And more images of the rocket on the launchpad as well as other file material can be found on https://images.nasa.gov/And don't miss the latest podcast release from NASA's Curious Universe: \"We're Going To Mars!\" || banner.png (2438x346) [970.2 KB] || banner_print.jpg (1024x145) [41.5 KB] || banner_searchweb.png (320x180) [85.4 KB] || banner_thm.png (80x40) [9.1 KB] || ",
            "hits": 81
        },
        {
            "id": 13625,
            "url": "https://svs.gsfc.nasa.gov/13625/",
            "result_type": "Produced Video",
            "release_date": "2020-05-25T11:00:00-04:00",
            "title": "First Map of Mars Electric Currents",
            "description": "MAVEN data have enabled the first map of the electric current systems (blue and red arrows) that shape the induced magnetic field surrounding Mars.Credit: NASA/Goddard/MAVEN/CU Boulder/SVSUniversal Production Music: “A Lucid Dream” and “Shimmer Oscillations” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MarsElectricCurrentsPreview6_print.jpg (1024x576) [305.8 KB] || MarsElectricCurrentsPreview6.jpg (1920x1080) [853.6 KB] || MarsElectricCurrentsPreview6_searchweb.png (320x180) [50.6 KB] || MarsElectricCurrentsPreview6_thm.png (80x40) [5.3 KB] || 13625_Mars_Electric_Currents_Twitter.mp4 (1280x720) [63.8 MB] || 13625_Mars_Electric_Currents_Facebook.mp4 (1920x1080) [359.1 MB] || 13625_Mars_Electric_Currents_YouTube.webm (3840x2160) [91.7 MB] || 13625_Mars_Electric_Currents_Captions.en_US.srt [7.2 KB] || 13625_Mars_Electric_Currents_Captions.en_US.vtt [6.8 KB] || 13625_Mars_Electric_Currents_YouTube.mp4 (3840x2160) [2.8 GB] || 13625_Mars_Electric_Currents_MASTER.mov (3840x2160) [14.2 GB] || 13625_Mars_Electric_Currents_Facebook.mp4.hwshow [134 bytes] || ",
            "hits": 126
        },
        {
            "id": 4824,
            "url": "https://svs.gsfc.nasa.gov/4824/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN Observes Solar Particle Velocities and the Induced Magnetic Field",
            "description": "MAVEN orbits Mars and measures solar particle velocities and variations in the solar wind’s magnetic field. || maven_vels_magField.03000_print.jpg (1024x576) [92.5 KB] || maven_vels_magField.03000_searchweb.png (320x180) [63.5 KB] || maven_vels_magField.03000_thm.png (80x40) [4.2 KB] || maven_vels_magField_1080p30.mp4 (1920x1080) [83.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || maven_vels_magField_1080p30.webm (1920x1080) [19.0 MB] || 4824_MAVEN_Solar_Wind_Data_1080_30p.mov (1920x1080) [2.6 GB] || maven_vels_magField_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 103
        },
        {
            "id": 4825,
            "url": "https://svs.gsfc.nasa.gov/4825/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN – Mars and Solar Wind Simulation",
            "description": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded. || maven_cme44.03600_print.jpg (1024x512) [253.9 KB] || maven_cme44.03600_searchweb.png (320x180) [92.7 KB] || maven_cme44.03600_thm.png (80x40) [5.2 KB] || 1920x1080_16x9_30p (2048x1024) [0 Item(s)] || maven_cme44_1024p30.webm (2048x1024) [5.9 MB] || maven_cme44_1024p30.mp4 (2048x1024) [195.1 MB] || maven_cme44_1024p30.mp4.hwshow [58 bytes] || ",
            "hits": 64
        },
        {
            "id": 13342,
            "url": "https://svs.gsfc.nasa.gov/13342/",
            "result_type": "Produced Video",
            "release_date": "2020-02-03T11:00:00-05:00",
            "title": "MAVEN Explores Mars to Understand Radio Interference at Earth",
            "description": "The MAVEN mission explores Mars’ atmosphere to better study a phenomenon observed at Earth, known as “Sporadic-E Layers.” They are concentrations of plasma that form in the ionosphere and interfere with radio waves. This video is animated in a comic book style.Music from Universal Production Music. Songs include: \"Alpha and Omega,\" \"Break the News,\" and \"Waiting for a Sensation.\" || MAVEN_thumb.jpg (3840x2160) [801.1 KB] || MAVEN_thumb_searchweb.png (320x180) [106.4 KB] || MAVEN_thumb_thm.png (80x40) [5.2 KB] || 13342_SPORADIC_MAVEN_MASTER.webm (960x540) [63.4 MB] || 13342_SPORADIC_MAVEN_MASTER_twitter_720.mp4 (1280x720) [29.9 MB] || 13342_SPORADIC_MAVEN_MASTER_facebook_720.mp4 (1280x720) [178.5 MB] || 13442_MAVEN_caption.en_US.srt [4.4 KB] || 13442_MAVEN_caption.en_US.vtt [4.4 KB] || 13342_SPORADIC_MAVEN_MASTER.mov (3840x2160) [10.8 GB] || ",
            "hits": 97
        },
        {
            "id": 4755,
            "url": "https://svs.gsfc.nasa.gov/4755/",
            "result_type": "Visualization",
            "release_date": "2019-12-12T14:00:00-05:00",
            "title": "Mars Upper Level Winds Observed by MAVEN - Visualizations",
            "description": "MAVEN observes upper level Martian winds over the course of about two years. || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_print.jpg (1024x576) [42.9 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_searchweb.png (320x180) [49.1 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_thm.png (80x40) [4.0 KB] || maven_upper_winds_campaigns_1080p60.mp4 (1920x1080) [51.0 MB] || maven_upper_winds_campaigns_1080p30.mp4 (1920x1080) [46.4 MB] || maven_upper_winds.0104_cam_mainShape_190909182423_beauty_1080p30.webm (1920x1080) [9.6 MB] || campaigns (3840x2160) [0 Item(s)] || maven_upper_winds_campaigns_2160p60.mp4 (3840x2160) [162.2 MB] || maven_upper_winds_campaigns_2160p30.mp4 (3840x2160) [146.8 MB] || 4755_MAVEN_Wind_Currents_Full.mov (3840x2160) [9.7 GB] || maven_upper_winds_campaigns_1080p30.mp4.hwshow [201 bytes] || ",
            "hits": 59
        },
        {
            "id": 12986,
            "url": "https://svs.gsfc.nasa.gov/12986/",
            "result_type": "Produced Video",
            "release_date": "2018-07-23T11:00:00-04:00",
            "title": "Mars Proton Aurora",
            "description": "On Earth, the northern and southern lights occur when the solar wind (electrically charged particles from the Sun) follow our planet's geomagnetic field lines to the poles and collide with the upper atmosphere. Mars lacks a global magnetic field, so instead the solar wind piles up in front of Mars in a bow shock, which blocks charged particles from reaching the bulk of the atmosphere. However, in a process first observed by the MAVEN mission, some solar wind protons can slip past the bow shock by first bonding with electrons from the Mars upper atmosphere to form hydrogen atoms. Because these hydrogen atoms are electrically neutral, they can pass through the bow shock and go on to create an ultraviolet proton aurora on the dayside of Mars.Learn more about MAVEN's observation of a proton aurora at Mars. || ",
            "hits": 115
        },
        {
            "id": 12045,
            "url": "https://svs.gsfc.nasa.gov/12045/",
            "result_type": "Produced Video",
            "release_date": "2015-11-06T19:00:00-05:00",
            "title": "NASA On Air: NASA Solves Mars Mystery Of Lost Atmosphere (11/6/2015)",
            "description": "LEAD: NASA scientists have identified the process that changed Mars from a warm and wet Earth-like planet to a cold, arid world. 1. New results from NASA’s MAVEN mission show the Martian atmosphere has been stripped away by a stream of particles, known as the solar wind, flowing from the sun at a speed of about one million miles per hour. 2. The Martian atmosphere has escaped from different regions of the Red Planet, including down the \"tail,\" where the solar wind flows behind Mars, and above the Martian poles in a \"polar plume.\" (Note: Atmospheric losses in the “tail” and “polar plume” region are rainbow-colored in the video.) TAG: Fortunately, Earth's atmosphere is protected from the solar wind effects because it has a magnetic field, which acts as a shield and deflects the stream of particles blowing off the sun. || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1920x1080_print.jpg (1024x576) [141.2 KB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1920x1080_searchweb.png (320x180) [80.4 KB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1920x1080_thm.png (80x40) [5.1 KB] || WEATHER_CENTRAL-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_WEA_CEN.wmv (1280x720) [40.4 MB] || NASAONAIR-Maven_mars_atmosphere_5_accuweather.avi (1280x720) [9.2 MB] || BARON_SERVICE-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_baron.mp4 (1920x1080) [16.5 MB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_960x540.m4v (960x540) [19.8 MB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1280x720.m4v (1280x720) [37.8 MB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1920x1080.m4v (1920x1080) [60.4 MB] || IPAD_DELIVERABLES-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_iPad_1920x1080.webm (1920x1080) [3.9 MB] || NBC_TODAY-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_NBC_Today.mov (1920x1080) [140.5 MB] || WC_PRORES_422-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_prores.mov (1920x1080) [395.0 MB] || WSI_WEATHER_CHANNEL-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_1920x1080.mov (1920x1080) [638.4 MB] || WSI_WEATHER_CHANNEL-NASAONAIR-Maven_mars_atmosphere_1920_MASTER_1280x720.mov (1280x720) [699.4 MB] || ",
            "hits": 460
        },
        {
            "id": 12042,
            "url": "https://svs.gsfc.nasa.gov/12042/",
            "result_type": "Produced Video",
            "release_date": "2015-11-05T14:00:00-05:00",
            "title": "MAVEN Results Live Shot Page",
            "description": "Interview with MAVEN Principal Investigator Dr. Bruce Jakosky || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_print.jpg (1024x576) [109.3 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_searchweb.png (320x180) [93.0 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq_thm.png (80x40) [6.5 KB] || YOUTUBE_HQ_Bruce_Jakosky_MAVEN_LS_Canned_youtube_hq.mov (1280x720) [649.6 MB] || Bruce_Jakosky_MAVEN_LS_Canned.mov (1280x720) [2.1 GB] || WEBM_Bruce_Jakosky_MAVEN_LS_Canned.webm (960x540) [89.8 MB] || Bruce_Jakosky_MAVEN_LS_Canned.en_US.srt [4.7 KB] || Bruce_Jakosky_MAVEN_LS_Canned.en_US.vtt [4.5 KB] || ",
            "hits": 78
        },
        {
            "id": 11992,
            "url": "https://svs.gsfc.nasa.gov/11992/",
            "result_type": "Produced Video",
            "release_date": "2015-09-02T11:00:00-04:00",
            "title": "Mapping Mars' Upper Atmosphere",
            "description": "Principal Investigator Bruce Jakosky talks about MAVEN’s science observations at Mars.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Bruce_Jakosky_G2015-007_thumbnail.png (1920x1080) [1.8 MB] || Bruce_Jakosky_G2015-007_thumbnail_print.jpg (1024x576) [100.6 KB] || Bruce_Jakosky_G2015-007_thumbnail_searchweb.png (320x180) [90.5 KB] || Bruce_Jakosky_G2015-007_thumbnail_thm.png (80x40) [7.2 KB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv.m4v (1280x720) [123.4 MB] || WEBM_G2015-007_MAVEN_Early_Sci_MASTER.webm (960x540) [101.9 MB] || APPLE_TV_G2015-007_MAVEN_Early_Sci_MASTER_appletv_subtitles.m4v (1280x720) [123.5 MB] || NASA_TV_G2015-007_MAVEN_Early_Sci_MASTER.mpeg (1280x720) [846.9 MB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.srt [4.1 KB] || G2015-007_MAVEN_Early_Sci_MASTER_Captions.en_US.vtt [4.2 KB] || G2015-007_MAVEN_Early_Sci_MASTER_H264.mov (1920x1080) [1.7 GB] || NASA_PODCAST_G2015-007_MAVEN_Early_Sci_MASTER_ipod_sm.mp4 (320x240) [44.1 MB] || PRORES_B-ROLL_G2015-007_MAVEN_Early_Sci_MASTER_prores.mov (1280x720) [3.4 GB] || G2015-007_MAVEN_Early_Sci_MASTER.mov (1920x1080) [6.5 GB] || ",
            "hits": 59
        }
    ]
}