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            "description": "See [ESCAPADE Mission Page](https://science.nasa.gov/mission/escapade/)",
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                    "name": "Beth Anthony",
                    "employer": "eMITS"
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            "title": "ESCAPADE Launch Phase and Deployment Animations",
            "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.The ESCAPADE mission will be carried into orbit on the second launch of Blue Origin’s New Glenn rocket. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.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. || ",
            "release_date": "2025-11-13T12:00:00-05:00",
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                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014666/14666_NewGlenn_ESCAPADE_4K_ProRes.00075_print.jpg",
                "filename": "14666_NewGlenn_ESCAPADE_4K_ProRes.00075_print.jpg",
                "media_type": "Image",
                "alt_text": "Credit: Blue Origin",
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            "title": "ESCAPADE Trajectory Animations",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, mission will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. 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.The ESCAPADE mission is being carried into orbit on the second launch of Blue Origin’s New Glenn rocket (NG-2) and is scheduled to launch in November 2025 from Cape Canaveral, Florida. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.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.Below are animations demonstrating the different phases of the mission's trajectory from traveling from Earth to Mars to implementing its science orbits around the Red Planet. || ",
            "release_date": "2025-11-13T00:00:00-05:00",
            "update_date": "2026-03-03T15:00:18-05:00",
            "main_image": {
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                "filename": "14915_ESCAPADE_ScienceOrbitA_Thumb_print.jpg",
                "media_type": "Image",
                "alt_text": "ESCAPADE - Science Orbit AAfter ESCAPADE reaches Mars, the two spacecraft will arrange themselves in their first science formation, in which the twin spacecraft will follow each other in the same orbit, passing through the same areas at different times to uncover when and where changes are happening at Mars. This science campaign will last for six months.Credit: Matt Bollinger/Advanced Space",
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        {
            "id": 14910,
            "url": "https://svs.gsfc.nasa.gov/14910/",
            "page_type": "Produced Video",
            "title": "Mars ESCAPADE! Duo of NASA spacecraft launching next week to solve a cosmic cold case",
            "description": "Associated cut b-roll will be posted by 3 p.m. EST on Thursday, Nov. 6. || ESCAPADE_banner.jpeg (1800x720) [138.2 KB] || ESCAPADE_banner_print.jpg (1024x409) [69.7 KB] || ESCAPADE_banner_searchweb.png (320x180) [57.1 KB] || ESCAPADE_banner_thm.png (80x40) [5.5 KB] || ",
            "release_date": "2025-11-07T00:00:00-05:00",
            "update_date": "2025-10-29T12:30:26.787353-04:00",
            "main_image": {
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                "alt_text": "Associated cut b-roll will be posted by 3 p.m. EST on Thursday, Nov. 6.",
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            "url": "https://svs.gsfc.nasa.gov/14675/",
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            "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 spacecraft were designed, built, integrated, and tested by Rocket Lab at their 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.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. || ",
            "release_date": "2024-09-03T17:00:00-04:00",
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            "main_image": {
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                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014675/ESCAPADE_Spacecraft_Full_Integration_01_print.jpg",
                "filename": "ESCAPADE_Spacecraft_Full_Integration_01_print.jpg",
                "media_type": "Image",
                "alt_text": "Image of the fully integrated ESCAPADE spacecraft in the clean room at Rocket Lab’s Space Systems Production Complex and Headquarters in Long Beach, California, before they are shipped to Astrotech Space Operations for pre-launch preparations.Photo Credit: Rocket Lab USA",
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        {
            "id": 14664,
            "url": "https://svs.gsfc.nasa.gov/14664/",
            "page_type": "Produced Video",
            "title": "ESCAPADE Mission Trailer",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "release_date": "2024-08-23T16:00:00-04:00",
            "update_date": "2025-03-01T08:44:19.389963-05:00",
            "main_image": {
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                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014664/ESCAPADE_Trailer_thumb.png",
                "filename": "ESCAPADE_Trailer_thumb.png",
                "media_type": "Image",
                "alt_text": "Music Credit: \"Inviolable\" by Bob E. Thole [BUMA] via Universal Production MusicAnimation Credits: James Rattray/Rocket Lab USA; Blue Origin",
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                "height": 720,
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        {
            "id": 14667,
            "url": "https://svs.gsfc.nasa.gov/14667/",
            "page_type": "Produced Video",
            "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. || ",
            "release_date": "2024-08-22T14:00:00-04:00",
            "update_date": "2024-08-22T14:48:19.968157-04:00",
            "main_image": {
                "id": 1097135,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014667/ESCAPADE_Berkeley_1080_001.00001_print.jpg",
                "filename": "ESCAPADE_Berkeley_1080_001.00001_print.jpg",
                "media_type": "Image",
                "alt_text": "Dr. Phyllis Whittlesey (EESA-e instrument lead) is demonstrating the subsystem components of an Electrostatic Analyser, and how the components interface with each other.Footage Credit: University of California, Berkeley/Patrick Farrell",
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                "height": 576,
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        },
        {
            "id": 14665,
            "url": "https://svs.gsfc.nasa.gov/14665/",
            "page_type": "Produced Video",
            "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. || ",
            "release_date": "2024-08-21T09:00:00-04:00",
            "update_date": "2024-08-20T15:12:13.941642-04:00",
            "main_image": {
                "id": 1096827,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014665/ESCAPADE_001_print.jpg",
                "filename": "ESCAPADE_001_print.jpg",
                "media_type": "Image",
                "alt_text": "ESCAPADE spacecraft development at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California.Image Credit: Rocket Lab",
                "width": 1024,
                "height": 768,
                "pixels": 786432
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        },
        {
            "id": 14641,
            "url": "https://svs.gsfc.nasa.gov/14641/",
            "page_type": "Infographic",
            "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. || ",
            "release_date": "2024-07-30T15:00:00-04:00",
            "update_date": "2024-07-30T14:58:03.792202-04:00",
            "main_image": {
                "id": 1095814,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014641/ESCAPADE-FINAL-Horizontal-Front_Web.jpg",
                "filename": "ESCAPADE-FINAL-Horizontal-Front_Web.jpg",
                "media_type": "Image",
                "alt_text": "ESCAPADE Horizontal Poster FRONTCredit: NASA/Kristen Perrin",
                "width": 2100,
                "height": 1421,
                "pixels": 2984100
            }
        },
        {
            "id": 14642,
            "url": "https://svs.gsfc.nasa.gov/14642/",
            "page_type": "Infographic",
            "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. || ",
            "release_date": "2024-07-30T15:00:00-04:00",
            "update_date": "2025-11-03T13:47:58.870680-05:00",
            "main_image": {
                "id": 1096043,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014600/a014642/Mars_ESC_Diagram_white_print.jpg",
                "filename": "Mars_ESC_Diagram_white_print.jpg",
                "media_type": "Image",
                "alt_text": "Credit: Rocket Lab USA",
                "width": 1024,
                "height": 866,
                "pixels": 886784
            }
        },
        {
            "id": 5200,
            "url": "https://svs.gsfc.nasa.gov/5200/",
            "page_type": "Visualization",
            "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] || ",
            "release_date": "2023-12-11T12:00:00-05:00",
            "update_date": "2024-08-22T05:26:59.974355-04:00",
            "main_image": {
                "id": 1088031,
                "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005200/a005200/maven_solar_wind_vertical.02715_print.jpg",
                "filename": "maven_solar_wind_vertical.02715_print.jpg",
                "media_type": "Image",
                "alt_text": "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.   This version does not include a date stamp or legend and is in a vertical orientation. ",
                "width": 1024,
                "height": 1820,
                "pixels": 1863680
            }
        },
        {
            "id": 13771,
            "url": "https://svs.gsfc.nasa.gov/13771/",
            "page_type": "Infographic",
            "title": "MAVEN Infographic: Martian Dust Storms Accelerate Water Loss",
            "description": "This illustration shows how water is lost on Mars normally vs. during regional or global dust storms. Text-readable PDF version.Credits: NASA/Goddard/CI Lab/Adriana Manrique Gutierrez/Krystofer Kim || MAVEN_ILLO_v7_print.jpg (1024x575) [117.4 KB] || MAVEN_ILLO_v7.png (6667x3750) [1.5 MB] || MAVEN_ILLO_v7.jpg (6667x3750) [1.4 MB] || MAVEN_ILLO_v7_searchweb.png (320x180) [53.3 KB] || MAVEN_ILLO_v7_thm.png (80x40) [5.9 KB] || ",
            "release_date": "2020-11-13T12:00:00-05:00",
            "update_date": "2024-10-15T14:52:53.320638-04:00",
            "main_image": {
                "id": 381390,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013700/a013771/MAVEN_ILLO_v7_print.jpg",
                "filename": "MAVEN_ILLO_v7_print.jpg",
                "media_type": "Image",
                "alt_text": "This illustration shows how water is lost on Mars normally vs. during regional or global dust storms. Text-readable PDF version.Credits: NASA/Goddard/CI Lab/Adriana Manrique Gutierrez/Krystofer Kim",
                "width": 1024,
                "height": 575,
                "pixels": 588800
            }
        },
        {
            "id": 4730,
            "url": "https://svs.gsfc.nasa.gov/4730/",
            "page_type": "Visualization",
            "title": "MAVEN – Mars Electric Current Systems",
            "description": "The current systems formed around Mars as a result of a solar wind driven convective electric field(Note: These frame sets were converted to the sRGB color space on 6/16/2020)This video is also available on our YouTube channel. || ideal_currents_1080.00600_print.jpg (1024x576) [71.1 KB] || ideal_currents_1080.00600_searchweb.png (320x180) [21.7 KB] || ideal_currents_1080.00600_thm.png (80x40) [2.0 KB] || ideal_currents_1080p30.mp4 (1920x1080) [74.0 MB] || ideal_currents_1080.webm (1920x1080) [9.9 MB] || ideal_curr (1920x1080) [0 Item(s)] || ideal_curr (3840x2160) [0 Item(s)] || captions_silent.25991.en_US.srt [43 bytes] || ideal_currents_4k_2160p30.mp4 (3840x2160) [170.1 MB] || idealized_currents_prores.mov (1920x1080) [2.9 GB] || Mars_idealized_currents_4k_prores.mov (3840x2160) [3.5 GB] || ideal_currents_1080p30.mp4.hwshow || ",
            "release_date": "2020-05-25T11:00:00-04:00",
            "update_date": "2025-06-23T00:09:41.420680-04:00",
            "main_image": {
                "id": 384922,
                "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004730/ideal_currents_1080.00600_print.jpg",
                "filename": "ideal_currents_1080.00600_print.jpg",
                "media_type": "Image",
                "alt_text": "The current systems formed around Mars as a result of a solar wind driven convective electric field(Note: These frame sets were converted to the sRGB color space on 6/16/2020)This video is also available on our YouTube channel.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 13625,
            "url": "https://svs.gsfc.nasa.gov/13625/",
            "page_type": "Produced Video",
            "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] || ",
            "release_date": "2020-05-25T11:00:00-04:00",
            "update_date": "2025-03-16T23:22:36.981129-04:00",
            "main_image": {
                "id": 384966,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013625/MarsElectricCurrentsPreview6.jpg",
                "filename": "MarsElectricCurrentsPreview6.jpg",
                "media_type": "Image",
                "alt_text": "MAVEN data have enabled the first map of the electric current systems (blue and red arrows) that shape the induced magnetic field surrounding Mars.\r\rCredit: 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.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 4825,
            "url": "https://svs.gsfc.nasa.gov/4825/",
            "page_type": "Visualization",
            "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] || ",
            "release_date": "2020-05-25T00:00:00-04:00",
            "update_date": "2025-03-16T22:46:51.857817-04:00",
            "main_image": {
                "id": 384913,
                "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004800/a004825/maven_cme44.03600_print.jpg",
                "filename": "maven_cme44.03600_print.jpg",
                "media_type": "Image",
                "alt_text": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded.",
                "width": 1024,
                "height": 512,
                "pixels": 524288
            }
        },
        {
            "id": 20302,
            "url": "https://svs.gsfc.nasa.gov/20302/",
            "page_type": "Animation",
            "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] || ",
            "release_date": "2019-12-12T14:00:00-05:00",
            "update_date": "2023-11-09T12:29:07.544223-05:00",
            "main_image": {
                "id": 389340,
                "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020300/a020302/20302_MarsUpperWinds_Preview_print.jpg",
                "filename": "20302_MarsUpperWinds_Preview_print.jpg",
                "media_type": "Image",
                "alt_text": "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.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 20297,
            "url": "https://svs.gsfc.nasa.gov/20297/",
            "page_type": "Animation",
            "title": "Magnetospheres of our Solar System",
            "description": "A magnetosphere is the magnetic field shields a planet against the Sun's dangerous radiation. Not all magnetospheres are alike. This animation depicts the unique magnetospheres around Earth, Mars, and Jupiter. To demonstrate their strength, each planet's magnetosphere receives a direct hit from a coronal mass ejection (CME) - a cloud of dense radiation and magnetic field from the Sun. The impact of the CME on the planet depends on the strength of the magnetosphere. On Mars, the magnetosphere is weak and patchy, resulting in some loss of the planet's atmosphere. At Earth, the magnetosphere acts as a buffer, deforming from the impact, but protecting the planet. For Jupiter, the punch of the CME is barely felt by the massive magnetic field. || ",
            "release_date": "2019-09-16T00:00:00-04:00",
            "update_date": "2023-05-03T13:45:38.848251-04:00",
            "main_image": {
                "id": 392915,
                "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020200/a020297/H_0219_VC_Animation_Full.00600_print.jpg",
                "filename": "H_0219_VC_Animation_Full.00600_print.jpg",
                "media_type": "Image",
                "alt_text": "Animation of a coronal mass ejection impacting Mars, Earth, and Jupiter. Credit: NASA GSFC/CIL/Bailee DesRocher",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        }
    ],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}