File:Cerro Tololo Light Show.jpg
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DescriptionCerro Tololo Light Show.jpg |
English: Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF's NOIRLab, is depicted here with the Milky Way and several nebulae within it, including the Lagoon Nebula and Rho Ophiuchi cloud complex. A number of CTIO telescopes are captured in this 360-degree panorama, including, from left to right: the UBC Southern Observatory, the SMARTS 1.0-meter Telescope, the Curtis Schmidt Telescope, the Víctor M. Blanco 4-meter Telescope, the SMARTS 1.5-meter Telescope and the SMARTS 0.9-meter Telescope. Various other, more unusual night sky phenomena are also visible. The white glow on the left of the image is zodiacal light, arising from interplanetary dust illuminated by the Sun. The green, orange, and reddish “clouds” near the horizon are airglow, caused by trace gasses in the upper atmosphere.
Español: El Observatorio Cerro Tololo (CTIO), un Programa de NOIRLab de NSF y AURA, se muestra aquí con la Vía Láctea y muchas nebulosas dentro de ella, incluyendo la Nebulosa de la Laguna y el complejo de formación estelar Rho Ophiuchi. En esta panorámica de 360 grados aparecen varios telescopios de CTIO, incluyendo, de izquierda a derecha: el UBC Southern Observatory, el Telescopio SMARTS de 1 metro, el Telescopio Curtis Schmidt, el Telescopio de 4 metros Víctor M. Blanco, el Telescopio SMARTS de 1,5 metros y el Telescopio SMARTS de 0,9 metros.
En la fotografía también podemos ver otros fenómenos más inusuales en el cielo nocturno: El resplandor blanco a la izquierda de la imagen es la luz zodiacal que se genera por el reflejo del Sol sobre el polvo interplanetario. Las “nubes” verdes, anaranjadas y rojizas cerca del horizonte son ejemplos del fenómeno conocido como luminiscencia nocturna o airglow, causado por los gases presentes en la atmósfera superior. |
Date | |
Source | https://noirlab.edu/public/images/iotw2218a/ |
Author | CTIO/NOIRLab/NSF/AURA/B. Tafreshi |
Licensing
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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Items portrayed in this file
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4 May 2022
image/jpeg
084d5b230d2d5c8e1cd6bbb843bdee4469e9041e
32,610,475 byte
5,891 pixel
18,296 pixel
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:10, 22 June 2023 | 18,296 × 5,891 (31.1 MB) | C messier | full size | |
19:26, 28 March 2023 | 1,280 × 412 (164 KB) | Yiseth Romero | Uploaded a work by CTIO/NOIRLab/NSF/AURA/B. Tafreshi from https://noirlab.edu/public/images/iotw2218a/ with UploadWizard |
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Metadata
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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, 4 May 2022 |
JPEG file comment | Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF's NOIRLab, is depicted here with the Milky Way and several nebulae within it, including the Lagoon Nebula and Rho Ophiuchi cloud complex. A number of CTIO telescopes are captured in this 360-degree panorama, including, from left to right: the UBC Southern Observatory, the SMARTS 1.0-meter Telescope, the Curtis Schmidt Telescope, the Víctor M. Blanco 4-meter Telescope, the SMARTS 1.5-meter Telescope and the SMARTS 0.9-meter Telescope. Various other, more unusual night sky phenomena are also visible. The white glow on the left of the image is zodiacal light, arising from interplanetary dust illuminated by the Sun. The green, orange, and reddish “clouds” near the horizon are airglow, caused by trace gasses in the upper atmosphere. |
Software used | Adobe Photoshop 22.0 (Windows) |
File change date and time | 08:40, 24 September 2021 |
Date and time of digitizing | 09:26, 18 July 2015 |
Date metadata was last modified | 01:40, 24 September 2021 |
Unique ID of original document | xmp.did:f713a2ce-c733-4b4e-a859-8db437276709 |
Keywords | CTIO |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |
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