The IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.
Animation credit: NASA/Princeton/Patrick McPike
", "items": [ { "id": 468803, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154074, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.00001_print.jpg", "filename": "14811_IMAP-Lo_Scanning_H264.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 468804, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154075, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.00001_searchweb.png", "filename": "14811_IMAP-Lo_Scanning_H264.00001_searchweb.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468805, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154076, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.00001_web.png", "filename": "14811_IMAP-Lo_Scanning_H264.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468806, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154077, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.00001_thm.png", "filename": "14811_IMAP-Lo_Scanning_H264.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 468494, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153805, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.mp4", "filename": "14811_IMAP-Lo_Scanning_H264.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468817, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154088, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_H264.webm", "filename": "14811_IMAP-Lo_Scanning_H264.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468495, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153806, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Lo_Scanning_Prores422.mov", "filename": "14811_IMAP-Lo_Scanning_Prores422.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Lo instrument measures low-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the low-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 377758, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_377758", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.
Animation credit: NASA/Princeton/Patrick McPike
", "items": [ { "id": 468808, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154079, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.00001_print.jpg", "filename": "14811_IMAP-Hi_Scanning_H264.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 468809, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154080, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.00001_searchweb.png", "filename": "14811_IMAP-Hi_Scanning_H264.00001_searchweb.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468810, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154081, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.00001_web.png", "filename": "14811_IMAP-Hi_Scanning_H264.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468811, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154082, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.00001_thm.png", "filename": "14811_IMAP-Hi_Scanning_H264.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 468496, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153807, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.mp4", "filename": "14811_IMAP-Hi_Scanning_H264.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468818, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154089, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_H264.webm", "filename": "14811_IMAP-Hi_Scanning_H264.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468497, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153808, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Hi_Scanning_Prores422.mov", "filename": "14811_IMAP-Hi_Scanning_Prores422.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Hi instrument measures high-energy energetic neutral atoms, or ENAs, as it spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 377759, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_377759", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.
Animation credit: NASA/Princeton/Patrick McPike
", "items": [ { "id": 468813, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154084, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.00001_print.jpg", "filename": "14811_IMAP-ULTRA_Scanning_H264.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 468814, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154085, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.00001_searchweb.png", "filename": "14811_IMAP-ULTRA_Scanning_H264.00001_searchweb.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468815, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154086, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.00001_web.png", "filename": "14811_IMAP-ULTRA_Scanning_H264.00001_web.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 468816, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154087, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.00001_thm.png", "filename": "14811_IMAP-ULTRA_Scanning_H264.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 468499, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153809, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.mp4", "filename": "14811_IMAP-ULTRA_Scanning_H264.mp4", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468819, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1154090, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_H264.webm", "filename": "14811_IMAP-ULTRA_Scanning_H264.webm", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 468500, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1153810, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-ULTRA_Scanning_Prores422.mov", "filename": "14811_IMAP-ULTRA_Scanning_Prores422.mov", "media_type": "Movie", "alt_text": "Conceptual AnimationThe IMAP-Ultra instrument is a pair of imagers that measure ultra high-energy energetic neutral atoms, or ENAs, as the spacecraft spins along its orbital path at Lagrange Point 1. This data is used to create maps that show the amount and origin location of the high-energy ENAs coming from the heliosphere’s boundary.Animation credit: NASA/Princeton/Patrick McPike", "width": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 378740, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_378740", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation
The 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", "items": [ { "id": 503025, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "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": 503026, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1195042, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_H264.00001_searchweb.png", "filename": "14811_IMAP_ScanningFOV2_H264.00001_searchweb.png", "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": 320, "height": 180, "pixels": 57600 } }, { "id": 503027, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1195043, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_H264.00001_web.png", "filename": "14811_IMAP_ScanningFOV2_H264.00001_web.png", "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": 320, "height": 180, "pixels": 57600 } }, { "id": 503028, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1195044, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_H264.00001_thm.png", "filename": "14811_IMAP_ScanningFOV2_H264.00001_thm.png", "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": 80, "height": 40, "pixels": 3200 } }, { "id": 503023, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1195039, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_H264.mp4", "filename": "14811_IMAP_ScanningFOV2_H264.mp4", "media_type": "Movie", "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": 5760, "height": 3240, "pixels": 18662400 } }, { "id": 503024, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1195040, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP_ScanningFOV2_ProRes422.mov", "filename": "14811_IMAP_ScanningFOV2_ProRes422.mov", "media_type": "Movie", "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": 5760, "height": 3240, "pixels": 18662400 } } ], "extra_data": {} }, { "id": 378785, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_378785", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation - Version 1
Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike
", "items": [ { "id": 490899, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157930, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_1080.00001_print.jpg", "filename": "14811_IMAP-Heliosphere-ENA_1080.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 490900, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157931, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_1080.00001_web.png", "filename": "14811_IMAP-Heliosphere-ENA_1080.00001_web.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 490901, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157932, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_1080.00001_thm.png", "filename": "14811_IMAP-Heliosphere-ENA_1080.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 490898, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157929, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_1080.mp4", "filename": "14811_IMAP-Heliosphere-ENA_1080.mp4", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 1Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 490910, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157942, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_1080.webm", "filename": "14811_IMAP-Heliosphere-ENA_1080.webm", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 1Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 378786, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_378786", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation - Version 2 (No Solar Particle)
Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike
", "items": [ { "id": 491185, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158079, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_print.jpg", "filename": "14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2 (No Solar Particle)Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 491186, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158080, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_web.png", "filename": "14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_web.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2 (No Solar Particle)Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 491187, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158081, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_thm.png", "filename": "14811_IMAP-Heliosphere-ENA_NoParticle_1080.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2 (No Solar Particle)Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 491184, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158078, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_NoParticle_1080.mp4", "filename": "14811_IMAP-Heliosphere-ENA_NoParticle_1080.mp4", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 2 (No Solar Particle)Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 491188, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1158082, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_IMAP-Heliosphere-ENA_NoParticle_1080.webm", "filename": "14811_IMAP-Heliosphere-ENA_NoParticle_1080.webm", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 2 (No Solar Particle)Charged solar particles travel toward the boundary of the heliosphere while following magnetic field lines. When some of the solar particles collide with the interstellar medium, they become energetic neutral atoms (ENAs) that have no charge and are not influenced by the magnetic fields. This allows ENAs to travel in straight lines and in all directions throughout our solar system. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 378787, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_378787", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation - Version 1
An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "items": [ { "id": 491175, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157933, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V1_1080.00001_print.jpg", "filename": "14811_ENA-hole-in-one_V1_1080.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 491176, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157934, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V1_1080.00001_web.png", "filename": "14811_ENA-hole-in-one_V1_1080.00001_web.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 491177, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157935, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V1_1080.00001_thm.png", "filename": "14811_ENA-hole-in-one_V1_1080.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 1An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 491178, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157943, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V1_1080.webm", "filename": "14811_ENA-hole-in-one_V1_1080.webm", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 1An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 491174, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157926, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V1_1080.mp4", "filename": "14811_ENA-hole-in-one_V1_1080.mp4", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 1An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 378821, "url": "https://svs.gsfc.nasa.gov/14811/#media_group_378821", "widget": "Video player", "title": "", "caption": "", "description": "Conceptual Animation - Version 2
An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "items": [ { "id": 491180, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157936, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V2_1080.00001_print.jpg", "filename": "14811_ENA-hole-in-one_V2_1080.00001_print.jpg", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 491181, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157938, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V2_1080.00001_web.png", "filename": "14811_ENA-hole-in-one_V2_1080.00001_web.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 491182, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157940, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V2_1080.00001_thm.png", "filename": "14811_ENA-hole-in-one_V2_1080.00001_thm.png", "media_type": "Image", "alt_text": "Conceptual Animation - Version 2An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 491179, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157928, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V2_1080.mp4", "filename": "14811_ENA-hole-in-one_V2_1080.mp4", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 2An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 491183, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1157944, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014800/a014811/14811_ENA-hole-in-one_V2_1080.webm", "filename": "14811_ENA-hole-in-one_V2_1080.webm", "media_type": "Movie", "alt_text": "Conceptual Animation - Version 2An energetic neutral atom, or ENA, travels toward the boundary of the heliosphere. Since they are not charged, ENAs travel in a straight line, unaffected by the twists, turns and turbulences in a magnetic field. The IMAP mission will use the ENAs it collects near Earth to trace back their origins and construct cosmic maps of the boundaries of the heliosphere, which would otherwise be invisible from such a distance. Credit: NASA/Princeton/Patrick McPike", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} } ], "studio": "gms", "funding_sources": [ "PAO" ], "credits": [ { "role": "Animator", "people": [ { "name": "Patrick McPike", "employer": null } ] }, { "role": "Producer", "people": [ { "name": "Joy Ng", "employer": "eMITS" } ] } ], "missions": [], "series": [], "tapes": [], "papers": [], "datasets": [], "nasa_science_categories": [ "Sun" ], "keywords": [ "Imap" ], "recommended_pages": [], "related": [ { "id": 14888, "url": "https://svs.gsfc.nasa.gov/14888/", "page_type": "Produced Video", "title": "IMAP Traveling to L1", "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. Additionally, IMAP will support real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. 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. 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": 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": 20410, "url": "https://svs.gsfc.nasa.gov/20410/", "page_type": "Animation", "title": "IMAP Beauty Passes", "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) 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.As a modern-day celestial cartographer, IMAP will also explore and 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 at its boundary with interstellar space. Additionally, IMAP will support real-time observations of the solar wind and energetic particles, which can produce hazardous conditions in the space environment near Earth. The IMAP spacecraft will be located at Lagrange Point 1, or L1. Lagrange points are positions in space where objects sent there tend to stay put. At L1, which is around 1 million miles from Earth towards the Sun, the gravitational pull of the Sun and Earth are balanced, allowing spacecraft to reduce fuel consumption needed to remain in position. At L1, IMAP will have a clear view of the heliosphere and will also be positioned to provide advanced warning of incoming solar storms headed to Earth. Learn more about IMAP.Below are conceptual animations highlighting the IMAP spacecraft. || ", "release_date": "2025-08-14T00:00:00-04:00", "update_date": "2025-09-17T16:58:27.554849-04:00", "main_image": { "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 } } ], "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 } } ], "newer_versions": [], "older_versions": [], "alternate_versions": [] }