The IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.
Credit: NASA/Princeton/Patrick McPike", "items": [ { "id": 492131, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158444, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_NoLogo_2-002.00001_print.jpg", "filename": "20410_IMAP_5k_Spin_NoLogo_2-002.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 492132, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158445, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_NoLogo_2-002.00001_searchweb.png", "filename": "20410_IMAP_5k_Spin_NoLogo_2-002.00001_searchweb.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492133, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158446, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_NoLogo_2-002.00001_web.png", "filename": "20410_IMAP_5k_Spin_NoLogo_2-002.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492134, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158447, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_NoLogo_2-002.00001_thm.png", "filename": "20410_IMAP_5k_Spin_NoLogo_2-002.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 492080, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158443, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_SPIN_HD_9_17_25.mp4", "filename": "20410_IMAP_SPIN_HD_9_17_25.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492079, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158442, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_NoLogo_2-002.mov", "filename": "20410_IMAP_5k_Spin_NoLogo_2-002.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 378901, "url": "https://svs.gsfc.nasa.gov/20410/#media_group_378901", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation With Logo
The IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.
Credit: NASA/Princeton/Patrick McPike", "items": [ { "id": 492135, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158448, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_print.jpg", "filename": "20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation With LogoThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 492136, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158449, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_web.png", "filename": "20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_web.png", "media_type": "Image", "alt_text": "Conceptual Animation With LogoThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492137, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158450, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_thm.png", "filename": "20410_IMAP_5k_Spin_Logo_9_17_25-001.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual Animation With LogoThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 492112, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158441, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_SPIN_HD_Logo_9_17_25.mp4", "filename": "20410_IMAP_SPIN_HD_Logo_9_17_25.mp4", "media_type": "Movie", "alt_text": "Conceptual Animation With LogoThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492111, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158440, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_5k_Spin_Logo_9_17_25-001.mov", "filename": "20410_IMAP_5k_Spin_Logo_9_17_25-001.mov", "media_type": "Movie", "alt_text": "Conceptual Animation With LogoThe IMAP spacecraft, located at Lagrange Point 1, spins at four revolutions per minute as it surveys the heliosphere.Credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 378902, "url": "https://svs.gsfc.nasa.gov/20410/#media_group_378902", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.
Credit: NASA/Adriana Manrique", "items": [ { "id": 492118, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158397, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_4k_proRes.00001_print.jpg", "filename": "20410_IMAP_BS_S1_30fps_4k_proRes.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 492120, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158398, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_4k_proRes.00001_web.png", "filename": "20410_IMAP_BS_S1_30fps_4k_proRes.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492122, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158399, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_4k_proRes.00001_thm.png", "filename": "20410_IMAP_BS_S1_30fps_4k_proRes.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 492116, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158387, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_1080_h264.mp4", "filename": "20410_IMAP_BS_S1_30fps_1080_h264.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492114, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158388, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_1080_proRes.mov", "filename": "20410_IMAP_BS_S1_30fps_1080_proRes.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492123, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158406, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_4k_proRes.webm", "filename": "20410_IMAP_BS_S1_30fps_4k_proRes.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 492113, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158389, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S1_30fps_4k_proRes.mov", "filename": "20410_IMAP_BS_S1_30fps_4k_proRes.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it can study the heliosphere by measuring particles returning from that boundary and it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way.Credit: NASA/Adriana Manrique", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 378903, "url": "https://svs.gsfc.nasa.gov/20410/#media_group_378903", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.
Credit: NASA/Adriana Manrique", "items": [ { "id": 492127, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158400, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_4k_proRes.00001_print.jpg", "filename": "20410_IMAP_BS_S2_30fps_4k_proRes.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 492128, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158401, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_4k_proRes.00001_web.png", "filename": "20410_IMAP_BS_S2_30fps_4k_proRes.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492129, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158402, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_4k_proRes.00001_thm.png", "filename": "20410_IMAP_BS_S2_30fps_4k_proRes.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 492126, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158390, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_1080_h264.mp4", "filename": "20410_IMAP_BS_S2_30fps_1080_h264.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492125, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158391, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_1080_proRes.mov", "filename": "20410_IMAP_BS_S2_30fps_1080_proRes.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492130, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158407, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_4k_proRes.webm", "filename": "20410_IMAP_BS_S2_30fps_4k_proRes.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 492124, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158392, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_BS_S2_30fps_4k_proRes.mov", "filename": "20410_IMAP_BS_S2_30fps_4k_proRes.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP mission will use 10 scientific instruments to chart a comprehensive picture of what’s roiling in space, from high-energy particles originating at the Sun, to magnetic fields in interplanetary space, to remnants of exploded stars in interstellar space.Credit: NASA/Adriana Manrique", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 378907, "url": "https://svs.gsfc.nasa.gov/20410/#media_group_378907", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.
Credit: NASA/Adriana Manrique/Jonathan North", "items": [ { "id": 492105, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158403, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_print.jpg", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 492106, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158404, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_web.png", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 492107, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158405, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_thm.png", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 492104, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158394, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_1080_V002.mp4", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_1080_V002.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 492102, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158395, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.mp4", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 492108, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158408, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.webm", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_h264_4K_V002.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 492103, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158393, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020410/20410_IMAP_ZouttoHelio_Clouds_Final_QT_V002.mov", "filename": "20410_IMAP_ZouttoHelio_Clouds_Final_QT_V002.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP spacecraft is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun. There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space.Credit: NASA/Adriana Manrique/Jonathan North", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 378908, "url": "https://svs.gsfc.nasa.gov/20410/#media_group_378908", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
This is a turntable animation with an alpha channel of the IMAP spacecraft.
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There, it will collect and measure particles that have traveled from the Sun, the heliosphere’s boundary 6 to 9 billion miles away, and interstellar space. At L1, it can also provide about a half hour's warning to voyaging astronauts and spacecraft near Earth of harmful radiation coming their way. || ", "release_date": "2025-08-22T16:00:00-04:00", "update_date": "2025-08-22T16:25:50.287771-04:00", "main_image": { "id": 1157904, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014888/14888_IMAP_Trajectory_to_L1_1080_H264.00001_print.jpg", "filename": "14888_IMAP_Trajectory_to_L1_1080_H264.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft launches from Cape Canaveral, Florida, to space. The mission is situated at the first Earth-Sun Lagrange point (L1), at around one million miles from Earth toward the Sun.Credit: Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 20406, "url": "https://svs.gsfc.nasa.gov/20406/", "page_type": "Animation", "title": "The Heliosphere Within The Milky Way Galaxy", "description": "Our solar system is nestled inside the Milky Way galaxy, home to more than 100 billion stars. Stretching for millions of miles around the solar system is a protective bubble called the heliosphere. Created by particles and magnetic fields from the Sun, the heliosphere separates our solar system from the vast galaxy beyond — and much of its harsh space radiation that can be damaging to life on Earth. || ", "release_date": "2025-08-22T09:00:00-04:00", "update_date": "2025-08-22T16:32:28.946043-04:00", "main_image": { "id": 1157626, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020406/MilkyWayZoom_30fps_proRes_wStars.00001_print.jpg", "filename": "MilkyWayZoom_30fps_proRes_wStars.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThis conceptual animation highlights the Milky Way Galaxy only.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 20408, "url": "https://svs.gsfc.nasa.gov/20408/", "page_type": "Animation", "title": "Solar Particle Acceleration", "description": "The Sun constantly emits a stream of high energy particles that can be accelerated by magnetic fields and other processes to nearly the speed of light. These particles, made of protons, ions and electrons, can be damaging at Earth where they can impede the function of satellites and telecommunications. NASA’s IMAP (Interstellar Mapping and Acceleration Probe) studies particle acceleration to better understand the fundamental processes driving these particles. This information will help scientists better understand and prepare for their effects at Earth, collectively called space weather. || ", "release_date": "2025-08-22T09:00:00-04:00", "update_date": "2025-08-06T15:47:40.086270-04:00", "main_image": { "id": 1157638, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020408/H_AccParticle_main_h264_wIMAP_V10.00504_print.jpg", "filename": "H_AccParticle_main_h264_wIMAP_V10.00504_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation With IMAPAt Lagrange Point 1, NASA's IMAP mission will detect solar particle acceleration to better understand the fundamental processes driving these particles that can cause space weather.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 20409, "url": "https://svs.gsfc.nasa.gov/20409/", "page_type": "Animation", "title": "The Heliosphere and Galactic Cosmic Rays", "description": "Surrounding our solar system is a giant protective bubble created by particles and magnetic fields from the Sun called the heliosphere. Every 11 years, the Sun’s activity ramps up and down in what’s known as the solar cycle. As the Sun reaches its peak activity level, called solar maximum, the heliosphere expands. During this time, the heliosphere’s protective shield is strengthened by the increase in particles and magnetic fields from the Sun. As a result, fewer damaging particles from the galaxy, such as galactic cosmic rays, are able to penetrate into the heliosphere. As the Sun ramps down into a low level of activity, called solar minimum, the heliosphere shrinks and more cosmic rays are able to enter the heliosphere. || ", "release_date": "2025-08-22T09:00:00-04:00", "update_date": "2025-08-22T16:38:50-04:00", "main_image": { "id": 1157621, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020400/a020409/Cosmic_rays_Anim_V002_1080_Final.00543_print.jpg", "filename": "Cosmic_rays_Anim_V002_1080_Final.00543_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationAs the heliosphere expands with the natural 11-year solar cycle, the number of galactic cosmic rays that penetrate the heliosphere decreases. As the heliosphere shrinks, more galactic cosmic rays can penetrate the heliosphere.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 5567, "url": "https://svs.gsfc.nasa.gov/5567/", "page_type": "Visualization", "title": "New Missions to L1", "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.", "release_date": "2025-07-21T18:59:59-04:00", "update_date": "2025-07-11T10:20:17.384003-04:00", "main_image": { "id": 1156845, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005500/a005567/Geospace2025.New2L1.GSE.RE.clockSlate_CRTT.HD1080.00900.jpg", "filename": "Geospace2025.New2L1.GSE.RE.clockSlate_CRTT.HD1080.00900.jpg", "media_type": "Image", "alt_text": "A visualization depicting 3 missions: SWFO, IMAP, and Carruthers' orbits. The Earth and its magnetosphere are depicted at the left of the visualization, and there is a large arrow pointing to the right. The missions orbits are all centered at a point on the arrow, which is marked with a large plus shape, and labeled \"L1\".", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 14816, "url": "https://svs.gsfc.nasa.gov/14816/", "page_type": "Produced Video", "title": "IMAP Testing and Integration at NASA's Marshall Space Flight Center", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, arrived at NASA’s Marshall Space Flight Center on March 18, 2025, to undergo testing prior to launch. At Marshall, IMAP will be exposed to extreme temperature changes during a 28-day-long test inside a thermal vacuum chamber (TVAC). By simulating the harsh conditions in space, scientists and engineers can identify any potential issues before launch.To learn more about the testing visit: https://science.nasa.gov/blogs/imap/2025/05/07/nasas-imap-completes-thermal-vacuum-testing-campaign/After thermal vacuum testing concluded at NASA's Marshall Space Flight Center, IMAP was transported to Florida: https://science.nasa.gov/blogs/imap/2025/05/10/nasas-interstellar-mapping-mission-arrives-in-florida/ || ", "release_date": "2025-04-11T11:00:00-04:00", "update_date": "2025-05-14T09:19:34.984553-04:00", "main_image": { "id": 1154848, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014816/Thumbnail01.jpg", "filename": "Thumbnail01.jpg", "media_type": "Image", "alt_text": "Produced Video - Horizontal: NASA’s IMAP Endures Extreme Conditions During Pre-Launch TestingWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: \"Nico's Journey\" by Nicholas Smith [PRS] from Universal Production Music", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 14815, "url": "https://svs.gsfc.nasa.gov/14815/", "page_type": "B-Roll", "title": "IMAP Testing and Integration at NASA's Goddard Space Flight Center", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which its instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "release_date": "2025-04-09T14:00:00-04:00", "update_date": "2025-04-24T13:02:12.421021-04:00", "main_image": { "id": 1154183, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014815/Lift_to_shipping_container_base-1046_print.jpg", "filename": "Lift_to_shipping_container_base-1046_print.jpg", "media_type": "Image", "alt_text": "PhotoSuzie Kellogg, Jackie Kilheffer, Luke Boggs, Pierce Brown, Tyler Radomsky, Emory Toomey, Anthony Fanelli, Anna Shin, Hunter Reeling, and Joe Minty lift the Interstellar Mapping and Acceleration Probe onto the shipping container base at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland.Credit: NASA/Johns Hopkins APL/Princeton/Ed Whitman", "width": 1024, "height": 683, "pixels": 699392 } }, { "id": 14814, "url": "https://svs.gsfc.nasa.gov/14814/", "page_type": "B-Roll", "title": "IMAP Testing and Integration at Johns Hopkins Applied Physics Lab", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "release_date": "2025-04-09T08:00:00-04:00", "update_date": "2025-05-14T14:27:15.080758-04:00", "main_image": { "id": 1154132, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014814/Sep-Shock_Firing_1-1204-Enhanced-NR_searchweb.png", "filename": "Sep-Shock_Firing_1-1204-Enhanced-NR_searchweb.png", "media_type": "Image", "alt_text": "PhotoThe Interstellar Mapping and Acceleration Probe is lifted off of the vibration table after completing vibration testing at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland.Credit: NASA/Johns Hopkins APL/Princeton/Ed Whitman", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 14811, "url": "https://svs.gsfc.nasa.gov/14811/", "page_type": "Produced Video", "title": "IMAP: Mapping The Heliosphere & Sun", "description": "The 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 entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.The mission’s investigation of the boundaries of the heliosphere will be primarily done with energetic neutral atoms, or ENAs. An ENA is a type of uncharged particle formed when an energetic positively charged ion runs into a slow-moving neutral atom. The ion picks up an extra negatively charged electron in the collision, making it neutral — hence the name energetic neutral atom. This process frequently happens wherever there is plasma in space, such as throughout the heliosphere, including its boundary.The IMAP-Lo, IMAP-HI, and IMAP-Ultra instruments on IMAP are imaging the energies and composition of ENAs.Learn more about IMAP: https://science.nasa.gov/mission/imap/ || ", "release_date": "2025-04-02T00:00:00-04:00", "update_date": "2025-12-11T13:45:55.604580-05:00", "main_image": { "id": 1195041, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_H264.00001_print.jpg", "filename": "14811_IMAP_ScanningFOV2_H264.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP spacecraft consists of 10 instruments monitor space weather and study and map the heliosphere, a vast magnetic bubble surrounding the Sun protecting our solar system from radiation. Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 20363, "url": "https://svs.gsfc.nasa.gov/20363/", "page_type": "Animation", "title": "Animation: Heliosphere", "description": "The sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium. This forms a giant bubble around the sun and its planets, known as the heliosphere. NASA studies the heliosphere to better understand the fundamental physics of the space surrounding us - which, in turn, provides information regarding space throughout the rest of the universe, as well as regarding what makes planets habitable.The solar wind is a gas of charged particles known as plasma, a state of matter governed by its own set physical laws just as the more common solids, liquids, and gases are. As the solar wind sweeps out into space, it creates a space environment filled with radiation as well as magnetic fields that trail all the way back to the sun. This space environment is augmented by interstellar cosmic rays and occasional concentrated clouds of solar material that burst off the sun, known as coronal mass ejections.This complex environment surrounds the planets and ultimately has a crucial effect on the formation, evolution, and destiny of planetary systems. For one thing, our heliosphere acts as a giant shield, protecting the planets from galactic cosmic radiation. Earth is additionally shielded by its own magnetic field, the magnetosphere, which protects us not only from solar and cosmic particle radiation but also from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to such processes and have evolved differently.NASA's studies of the heliosphere include research into: how the solar wind behaves near Earth; what causes and sustains magnetic and electric fields around other planets; how does the heliosphere interact with the interstellar medium; what do the boundaries of the heliosphere look like; what is the origin and evolution of the solar wind and the interstellar cosmic rays; and what contributes to the habitability of exoplanets.The field is, therefore, intensely cross-disciplinary. Heliospheric research often works hand in hand with planetary scientists, astrophysicists, astrobiologists, and space weather researchers.NASA heliophysics missions contributing to heliospheric research are: the Advanced Composition Explorer; NOAA's Deep Space Climate Observatory, the Interstellar Boundary Explorer, the Solar Terrestrial Relations Observatory; Voyager, and Wind. || ", "release_date": "2022-03-09T18:00:00-05:00", "update_date": "2025-06-23T00:18:39.136923-04:00", "main_image": { "id": 372595, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020300/a020363/H_0322_HeliopauseCycle_v01.00680_print.jpg", "filename": "H_0322_HeliopauseCycle_v01.00680_print.jpg", "media_type": "Image", "alt_text": "A conceptual animation showing the heliosphere — the vast bubble that is generated by the Sun’s magnetic field and envelops all the planets. ", "width": 1024, "height": 576, "pixels": 589824 } } ], "sources": [], "products": [ { "id": 14895, "url": "https://svs.gsfc.nasa.gov/14895/", "page_type": "Produced Video", "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/ || ", "release_date": "2025-09-17T10:00:00-04:00", "update_date": "2025-09-15T14:21:58.200579-04:00", "main_image": { "id": 1158230, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014895/14895_Thumbnail.jpg", "filename": "14895_Thumbnail.jpg", "media_type": "Image", "alt_text": "Produced VideoWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: \"Soaring Dreams” by Klas Johan Wahl and Anders Paul Niska [STIM], “Electric Works” by Philippe Lhommet [SACEM], and “Mercurial Temperment” by Christian Telfold [ASCAP] from Universal Production Music", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 14893, "url": "https://svs.gsfc.nasa.gov/14893/", "page_type": "Produced Video", "title": "Three Missions Launch to Track Space Weather (Official NASA Trailer)", "description": "Soon, there will be three new ways to study the Sun’s influence across the solar system with the launch of a trio of NASA and National Oceanic and Atmospheric Administration (NOAA) spacecraft. Launching September 23, 2025, from NASA’s Kennedy Space Center in Florida, the missions include NASA’s IMAP (Interstellar Mapping and Acceleration Probe), NASA’s Carruthers Geocorona Observatory, and NOAA’s SWFO-L1 (Space Weather Follow On-Lagrange 1) spacecraft.The missions will each study different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system. Research from the missions will help us better understand the Sun’s influence on Earth’s habitability, map our home in space, and protect satellites and voyaging astronauts from space weather threats.Watch the launch with NASA from anywhere in the world. We will provide live broadcast coverage on September 23 from 6:40 a.m. to about 9:15 a.m. EDT (1040 to 1415 UTC) on NASA+, Amazon Prime, Twitch, YouTube, and more. Learn how to watch NASA content through a variety of platforms, including social media.Media Resources• Interstellar Mapping and Acceleration Probe (IMAP)• Carruthers Geocorona Observatory• Space Weather Follow On-Lagrange 1 (SWFO-L1) || ", "release_date": "2025-09-04T12:00:00-04:00", "update_date": "2025-09-04T09:29:58.434941-04:00", "main_image": { "id": 1158098, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014893/IMAPSWFOCarruthersTrailer_Thumbnail.jpg", "filename": "IMAPSWFOCarruthersTrailer_Thumbnail.jpg", "media_type": "Image", "alt_text": "Music credit: “Emergence” by Aaron Albert Srdoc [BMI] via Universal Production MusicComplete transcript available.Watch this video on the NASA Goddard YouTube channel.", "width": 1280, "height": 720, "pixels": 921600 } } ], "newer_versions": [], "older_versions": [], "alternate_versions": [] }