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As seen here, the full extent of the jet and counterjet is 4.16 light-years, smaller than the distance between our sun and the nearest star. The image resolves details as small as 15 light-days across. Undetected between the jets is the galaxy's 55-million-solar-mass black hole. Credit: NASA/TANAMI/Müller et al.", "width": 320, "height": 201, "pixels": 64320 } }, { "id": 330660, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486073, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/Cen_A_inner_jet_English_no_labels_thm.png", "filename": "Cen_A_inner_jet_English_no_labels_thm.png", "media_type": "Image", "alt_text": "No Labels. Left: The giant elliptical galaxy NGC 5128 is the radio source known as Centaurus A. Vast radio-emitting lobes (shown as orange in this optical/radio composite) extend nearly a million light-years from the galaxy. 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Junkes (MPIfR).", "width": 1963, "height": 2570, "pixels": 5044910 } }, { "id": 330665, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486078, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/CenA_radio_optical_gamma_composite_new_no_labels_web.png", "filename": "CenA_radio_optical_gamma_composite_new_no_labels_web.png", "media_type": "Image", "alt_text": "The giant elliptical galaxy NGC 5128 is the radio source known as Centaurus A. Vast radio-emitting lobes (shown as orange in this optical/radio composite) extend nearly a million light-years from the galaxy. Credit: Capella Observatory (optical), with radio data from Ilana Feain, Tim Cornwell, and Ron Ekers (CSIRO/ATNF), R. Morganti (ASTRON), and N. Junkes (MPIfR).", "width": 320, "height": 418, "pixels": 133760 } } ], "extra_data": {} }, { "id": 351853, "url": "https://svs.gsfc.nasa.gov/10770/#media_group_351853", "widget": "Single image", "title": "", "caption": "", "description": "The elliptical galaxy NGC 5128, host of the Centaurus A radio source, as it appears in visible light. The galaxy is located about 12 million light-years away and is one of the closest sporting an active supermassive black hole. Credit: Capella Observatory", "items": [ { "id": 330666, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486079, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/CenA_optical_Capella_Obs.jpg", "filename": "CenA_optical_Capella_Obs.jpg", "media_type": "Image", "alt_text": "The elliptical galaxy NGC 5128, host of the Centaurus A radio source, as it appears in visible light. The galaxy is located about 12 million light-years away and is one of the closest sporting an active supermassive black hole. Credit: Capella Observatory", "width": 2000, "height": 2946, "pixels": 5892000 } }, { "id": 330667, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486080, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/CenA_optical_Capella_Obs_web.png", "filename": "CenA_optical_Capella_Obs_web.png", "media_type": "Image", "alt_text": "The elliptical galaxy NGC 5128, host of the Centaurus A radio source, as it appears in visible light. The galaxy is located about 12 million light-years away and is one of the closest sporting an active supermassive black hole. Credit: Capella Observatory", "width": 320, "height": 471, "pixels": 150720 } } ], "extra_data": {} }, { "id": 351854, "url": "https://svs.gsfc.nasa.gov/10770/#media_group_351854", "widget": "Single image", "title": "", "caption": "", "description": "This composite of visible, microwave (orange) and X-ray (blue) data reveals the jets and radio-emitting lobes emanating from Centaurus A's central black hole. Credit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray)", "items": [ { "id": 330668, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486081, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/eso0903a.jpg", "filename": "eso0903a.jpg", "media_type": "Image", "alt_text": "This composite of visible, microwave (orange) and X-ray (blue) data reveals the jets and radio-emitting lobes emanating from Centaurus A's central black hole. Credit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray)", "width": 1280, "height": 1348, "pixels": 1725440 } }, { "id": 330669, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486082, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/eso0903a_web.png", "filename": "eso0903a_web.png", "media_type": "Image", "alt_text": "This composite of visible, microwave (orange) and X-ray (blue) data reveals the jets and radio-emitting lobes emanating from Centaurus A's central black hole. Credit: ESO/WFI (visible); MPIfR/ESO/APEX/A.Weiss et al. (microwave); NASA/CXC/CfA/R.Kraft et al. (X-ray)", "width": 320, "height": 337, "pixels": 107840 } } ], "extra_data": {} }, { "id": 351855, "url": "https://svs.gsfc.nasa.gov/10770/#media_group_351855", "widget": "Single image", "title": "", "caption": "", "description": "The TANAMI array consists of nine radio telescopes located on four continents. By combining data from the individual telescopes, astronomers can acquire images with the sharpness of a single telescope some 6,200 miles (10,000 km) across — about 80 percent of Earth's diameter. Credit: Matthias Kadler, Univ. of Würzburg ", "items": [ { "id": 330670, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486083, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/tanami_world_labeled.jpg", "filename": "tanami_world_labeled.jpg", "media_type": "Image", "alt_text": "The TANAMI array consists of nine radio telescopes located on four continents. By combining data from the individual telescopes, astronomers can acquire images with the sharpness of a single telescope some 6,200 miles (10,000 km) across — about 80 percent of Earth's diameter. Credit: Matthias Kadler, Univ. of Würzburg ", "width": 2499, "height": 1425, "pixels": 3561075 } }, { "id": 330671, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 486084, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010700/a010770/tanami_world_labeled_web.png", "filename": "tanami_world_labeled_web.png", "media_type": "Image", "alt_text": "The TANAMI array consists of nine radio telescopes located on four continents. By combining data from the individual telescopes, astronomers can acquire images with the sharpness of a single telescope some 6,200 miles (10,000 km) across — about 80 percent of Earth's diameter. Credit: Matthias Kadler, Univ. of Würzburg ", "width": 320, "height": 182, "pixels": 58240 } } ], "extra_data": {} }, { "id": 351856, "url": "https://svs.gsfc.nasa.gov/10770/#media_group_351856", "widget": "Basic text", "title": "For More Information", "caption": "", "description": "See [http://www.nasa.gov/topics/universe/features/radio-particle-jets.html](http://www.nasa.gov/topics/universe/features/radio-particle-jets.html)", "items": [], "extra_data": {} } ], "studio": "gms", "funding_sources": [ "NASA Astrophysics" ], "credits": [ { "role": "Video editor", "people": [ { "name": "Scott Wiessinger", "employer": "UMBC" } ] }, { "role": "Narrator", "people": [ { "name": "Scott Wiessinger", "employer": "UMBC" } ] }, { "role": "Producer", "people": [ { "name": "Scott Wiessinger", "employer": "UMBC" } ] }, { "role": "Science writer", "people": [ { "name": "Francis Reddy", "employer": "University of Maryland College Park" } ] }, { "role": "Graphics", "people": [ { "name": "Francis Reddy", "employer": "University of Maryland College Park" } ] } ], "missions": [], "series": [ "Astrophysics Features", "Astrophysics Stills", "Astrophysics Visualizations", "Goddard Shorts", "Narrated Movies" ], "tapes": [ "Best Ever view of Black Hole's Jets (Produced by: Robert Crippen)" ], "papers": [], "datasets": [], "nasa_science_categories": [ "Universe" ], "keywords": [ "Active Galaxy", "Ast", "Astrophysics", "Black Hole", "Earth Science", "Edited Feature", "Galaxy", "HDTV", "Narrated", "Radio Wave", "Space science", "Spectral/Engineering" ], "recommended_pages": [], "related": [ { "id": 10987, "url": "https://svs.gsfc.nasa.gov/10987/", "page_type": "Produced Video", "title": "Black Hole Snapshot", "description": "Although it seems improbable to use radio frequencies to see anything—let alone the high-speed particle jets of a supermassive black hole—astronomers have done just that. Using a global array of radio telescopes, a team including NASA-funded scientists has created a fine-resolution radio image that reveals the innermost jets at the center of galaxy Centaurus A, 12 million light-years from Earth. The detail in the image is equivalent to spotting a quarter from 5,000 miles away. As gases fall into the black hole at Centaurus A's core, the material gets accelerated outward, creating huge plumes of matter in a process not fully understood. Watch the video to see the vast size of the galaxy's plumes compared to the relative smallness of the black-hole-powered jet that created them. || ", "release_date": "2012-06-28T00:00:00-04:00", "update_date": "2023-05-03T13:52:59.085411-04:00", "main_image": { "id": 476245, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010900/a010987/Cover-eso0903a_iPad_Cover_1024_576.jpg", "filename": "Cover-eso0903a_iPad_Cover_1024_576.jpg", "media_type": "Image", "alt_text": "Telescopes look deep into a galaxy to snap a detailed view of a black hole's jets.\n", "width": 1024, "height": 576, "pixels": 589824 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }