{ "id": 13661, "url": "https://svs.gsfc.nasa.gov/13661/", "page_type": "Produced Video", "title": "NASA Missions Spot Comet NEOWISE", "description": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO || wide.00250_print.jpg (1024x576) [164.4 KB] || wide.mp4 (3840x2160) [72.2 MB] || wide.webm (3840x2160) [6.2 MB] || ", "release_date": "2020-07-10T09:50:00-04:00", "update_date": "2023-05-03T13:44:51.300653-04:00", "main_image": { "id": 384086, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wisprinnerneowise20200705T020949E1_print.jpg", "filename": "wisprinnerneowise20200705T020949E1_print.jpg", "media_type": "Image", "alt_text": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "width": 1024, "height": 1092, "pixels": 1118208 }, "main_video": { "id": 384081, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wide.mp4", "filename": "wide.mp4", "media_type": "Movie", "alt_text": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO", "width": 3840, "height": 2160, "pixels": 8294400 }, "main_credits": { "Written by": [ { "name": "Sarah Frazier", "employer": "SGT" } ] }, "progress": "Complete", "media_groups": [ { "id": 319552, "url": "https://svs.gsfc.nasa.gov/13661/#media_group_319552", "widget": "Video player", "title": "", "caption": "", "description": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE.

Credit: ESA/NASA/SOHO", "items": [ { "id": 227178, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384082, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wide.00250_print.jpg", "filename": "wide.00250_print.jpg", "media_type": "Image", "alt_text": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 227177, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384081, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wide.mp4", "filename": "wide.mp4", "media_type": "Movie", "alt_text": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 227179, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384083, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wide.webm", "filename": "wide.webm", "media_type": "Movie", "alt_text": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO", "width": 3840, "height": 2160, "pixels": 8294400 } } ], "extra_data": {} }, { "id": 319551, "url": "https://svs.gsfc.nasa.gov/13661/#media_group_319551", "widget": "Basic text with HTML", "title": "", "caption": "", "description": "NASA’s Parker Solar Probe was at the right place at the right time to capture a unique view of comet NEOWISE on July 5, 2020. Parker Solar Probe’s position in space gave the spacecraft an unmatched view of the comet’s twin tails when it was particularly active just after its close approach to the Sun, called perihelion. \r
\r
The comet was discovered by NASA’s Near-Earth Object Wide-field Infrared Survey Explorer, or NEOWISE, on March 27. Since then, the comet — called comet C/2020 F3 NEOWISE and nicknamed comet NEOWISE — has been spotted by several NASA spacecraft, including Parker Solar Probe, NASA’s Solar and Terrestrial Relations Observatory, the ESA/NASA Solar and Heliospheric Observatory, and astronauts aboard the Space Station.", "items": [], "extra_data": {} }, { "id": 319553, "url": "https://svs.gsfc.nasa.gov/13661/#media_group_319553", "widget": "Single image", "title": "", "caption": "", "description": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens.

Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "items": [ { "id": 227180, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384085, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wisprinnerneowise20200705T020949E1.png", "filename": "wisprinnerneowise20200705T020949E1.png", "media_type": "Image", "alt_text": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "width": 937, "height": 1000, "pixels": 937000 } }, { "id": 227181, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384086, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wisprinnerneowise20200705T020949E1_print.jpg", "filename": "wisprinnerneowise20200705T020949E1_print.jpg", "media_type": "Image", "alt_text": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "width": 1024, "height": 1092, "pixels": 1118208 } }, { "id": 227182, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384087, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wisprinnerneowise20200705T020949E1_searchweb.png", "filename": "wisprinnerneowise20200705T020949E1_searchweb.png", "media_type": "Image", "alt_text": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 227183, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384084, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/wisprinnerneowise20200705T020949E1_thm.png", "filename": "wisprinnerneowise20200705T020949E1_thm.png", "media_type": "Image", "alt_text": "An unprocessed image from the WISPR instrument on board NASA’s Parker Solar Probe shows comet NEOWISE on July 5, 2020, shortly after its closest approach to the Sun. The Sun is out of frame to the left. The white streak near the upper left corner of the image is light reflected off a grain of dust that passed through the instrument’s field of view during the observation. The faint grid pattern near the center of the image is an artifact of the way the image is created. The small black structure near the lower left of the image is caused by a grain of dust resting on the imager’s lens. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Brendan Gallagher", "width": 80, "height": 40, "pixels": 3200 } } ], "extra_data": {} }, { "id": 319554, "url": "https://svs.gsfc.nasa.gov/13661/#media_group_319554", "widget": "Single image", "title": "", "caption": "", "description": "Processed data from the WISPR instrument on NASA’s Parker Solar Probe shows greater detail in the twin tails of comet NEOWISE, as seen on July 5, 2020. The lower, broader tail is the comet’s dust tail, while the thinner, upper tail is the comet’s ion tail.

Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Guillermo Stenborg", "items": [ { "id": 227184, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384088, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/20200705T020949BW.png", "filename": "20200705T020949BW.png", "media_type": "Image", "alt_text": "Processed data from the WISPR instrument on NASA’s Parker Solar Probe shows greater detail in the twin tails of comet NEOWISE, as seen on July 5, 2020. The lower, broader tail is the comet’s dust tail, while the thinner, upper tail is the comet’s ion tail. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Guillermo Stenborg", "width": 2000, "height": 1322, "pixels": 2644000 } }, { "id": 227185, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384089, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/20200705T020949BW_print.jpg", "filename": "20200705T020949BW_print.jpg", "media_type": "Image", "alt_text": "Processed data from the WISPR instrument on NASA’s Parker Solar Probe shows greater detail in the twin tails of comet NEOWISE, as seen on July 5, 2020. The lower, broader tail is the comet’s dust tail, while the thinner, upper tail is the comet’s ion tail. Credit: NASA/Johns Hopkins APL/Naval Research Lab/Parker Solar Probe/Guillermo Stenborg", "width": 1024, "height": 676, "pixels": 692224 } } ], "extra_data": {} }, { "id": 319555, "url": "https://svs.gsfc.nasa.gov/13661/#media_group_319555", "widget": "Single image", "title": "", "caption": "", "description": "This image of comet NEOWISE was captured by NASA’s Solar and Terrestrial Relations Observatory, or STEREO, on June 24, 2020, as the comet approached the Sun. The comet was visible in the field of view of STEREO’s Heliospheric Imager because of a special observing campaign: STEREO underwent a 180-degree roll on June 24 in order to observe the star Betelgeuse, whose brightness variations over the past several months have intrigued scientists. This image has been processed to increase contrast.\r

\r

Credit: NASA/STEREO/William Thompson\r

", "items": [ { "id": 227187, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384091, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/neowise_print.jpg", "filename": "neowise_print.jpg", "media_type": "Image", "alt_text": "This image of comet NEOWISE was captured by NASA’s Solar and Terrestrial Relations Observatory, or STEREO, on June 24, 2020, as the comet approached the Sun. The comet was visible in the field of view of STEREO’s Heliospheric Imager because of a special observing campaign: STEREO underwent a 180-degree roll on June 24 in order to observe the star Betelgeuse, whose brightness variations over the past several months have intrigued scientists. This image has been processed to increase contrast.\r\rCredit: NASA/STEREO/William Thompson\r", "width": 1024, "height": 762, "pixels": 780288 } }, { "id": 227186, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 384090, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013661/neowise.gif", "filename": "neowise.gif", "media_type": "Image", "alt_text": "This image of comet NEOWISE was captured by NASA’s Solar and Terrestrial Relations Observatory, or STEREO, on June 24, 2020, as the comet approached the Sun. The comet was visible in the field of view of STEREO’s Heliospheric Imager because of a special observing campaign: STEREO underwent a 180-degree roll on June 24 in order to observe the star Betelgeuse, whose brightness variations over the past several months have intrigued scientists. This image has been processed to increase contrast.\r\rCredit: NASA/STEREO/William Thompson\r", "width": 602, "height": 448, "pixels": 269696 } } ], "extra_data": {} } ], "studio": "gms", "funding_sources": [ "NASA Heliophysics" ], "credits": [ { "role": "Science writer", "people": [ { "name": "Sarah Frazier", "employer": "SGT" } ] }, { "role": "Project support", "people": [ { "name": "Scott Wiessinger", "employer": "USRA" } ] } ], "missions": [ "Parker Solar Probe", "SOHO" ], "series": [ "Heliophysics Breaking News" ], "tapes": [], "papers": [], "datasets": [], "nasa_science_categories": [ "Sun" ], "keywords": [ "Comet", "Parker Solar Probe", "SOHO" ], "recommended_pages": [], "related": [ { "id": 13030, "url": "https://svs.gsfc.nasa.gov/13030/", "page_type": "Produced Video", "title": "NASA's Planet-Hunting TESS Catches a Comet Before Starting Science", "description": "This video is compiled from a series of images taken on July 25 by the Transiting Exoplanet Survey Satellite. The angular extent of the widest field of view is six degrees. Visible in the images are the comet C/2018 N1, asteroids, variable stars, asteroids and reflected light from Mars. TESS is expected to find thousands of planets around other nearby stars. Credit: Massachusetts Institute of Technology/NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Comet_Still.jpg (1920x1080) [409.0 KB] || TESS_Comet_Still_print.jpg (1024x576) [112.2 KB] || TESS_Comet_Still_searchweb.png (320x180) [50.8 KB] || TESS_Comet_Still_thm.png (80x40) [3.8 KB] || 13030_TESS_Comet_ProRes_1080_2997.mov (1920x1080) [1.7 GB] || 13030_TESS_Comet_1080.mp4 (1920x1080) [118.6 MB] || 13030_TESS_Comet_H264_1080_Best.mov (1920x1080) [173.0 MB] || 13030_TESS_Comet_H264_1080_Good.m4v (1920x1080) [114.8 MB] || 13030_TESS_Comet_ProRes_1080_2997.webm (1920x1080) [10.8 MB] || 13030_TESS_Comet_SRT_Captions.en_US.srt [1.3 KB] || 13030_TESS_Comet_SRT_Captions.en_US.vtt [1.3 KB] || ", "release_date": "2018-08-06T10:00:00-04:00", "update_date": "2023-05-03T13:46:32.882979-04:00", "main_image": { "id": 401281, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013000/a013030/TESS_Comet_Still.jpg", "filename": "TESS_Comet_Still.jpg", "media_type": "Image", "alt_text": "This video is compiled from a series of images taken on July 25 by the Transiting Exoplanet Survey Satellite. The angular extent of the widest field of view is six degrees. Visible in the images are the comet C/2018 N1, asteroids, variable stars, asteroids and reflected light from Mars. TESS is expected to find thousands of planets around other nearby stars. Credit: Massachusetts Institute of Technology/NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available.", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }