File:A Sky Aglow.jpg
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Summary
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DescriptionA Sky Aglow.jpg |
English: The sky above Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, is aglow with color in this image. The bright region at the center of this image is the heart of the Milky Way galaxy, which lies approximately 26,000 light-years from Earth. As well as stars and dark dust lanes, our home galaxy’s heart contains a colossal black hole, roughly 4 million times as massive as the Sun. Though the heart of the Milky Way is a spectacular sight, the majority of the colors in this image arise much closer to home. As well as the tint of airglow around the horizon of the image, zodiacal light stretches from the horizon towards the center of the image. Zodiacal light — also called false dawn — is caused by sunlight reflecting from small particles in the Solar System’s interplanetary dust cloud. The combination of airglow, zodiacal light, and other atmospheric phenomena means that the night sky is never truly dark — even at professional observatories such as CTIO. |
Date | |
Source | https://noirlab.edu/public/images/iotw2144a/ |
Author | CTIO/NOIRLab/NSF/AURA/B. Tafreshi |
Licensing
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This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. |
![]() ![]() This file is licensed under the Creative Commons Attribution 4.0 International license.
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3 November 2021
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 16:58, 2 December 2021 | ![]() | 8,638 × 9,466 (22.49 MB) | Pandreve | Uploaded a work by CTIO/NOIRLab/NSF/AURA/B. Tafreshi from https://noirlab.edu/public/images/iotw2144a/ with UploadWizard |
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Credit/Provider | CTIO/NOIRLab/NSF/AURA/B. Tafreshi |
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Source | NSF's NOIRLab |
Short title |
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Image title |
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Usage terms |
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Date and time of data generation | 12:00, 3 November 2021 |
JPEG file comment | The sky above Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, is aglow with color in this image. The bright region at the center of this image is the heart of the Milky Way galaxy, which lies approximately 26,000 light-years from Earth. As well as stars and dark dust lanes, our home galaxy’s heart contains a colossal black hole, roughly 4 million times as massive as the Sun. Though the heart of the Milky Way is a spectacular sight, the majority of the colors in this image arise much closer to home. As well as the tint of airglow around the horizon of the image, zodiacal light stretches from the horizon towards the center of the image. Zodiacal light — also called false dawn — is caused by sunlight reflecting from small particles in the Solar System’s interplanetary dust cloud. The combination of airglow, zodiacal light, and other atmospheric phenomena means that the night sky is never truly dark — even at professional observatories such as CTIO. |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 04:29, 28 June 2021 |
Date and time of digitizing | 08:44, 18 July 2015 |
Date metadata was last modified | 06:29, 28 June 2021 |
Unique ID of original document | xmp.did:d1e29de0-7303-ca4b-a948-f2616cb2aa52 |
Keywords | CTIO |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |
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