File:Smoke and Mirrors.jpg
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[edit]DescriptionSmoke and Mirrors.jpg |
English: Gemini North, of the international Gemini Observatory (a Program of NSF’s NOIRLab), stands peacefully in the foreground, under a crystal clear sky. The dramatic upward sweep of milky and sooty patches of the Milky Way galaxy is seen in the background. The dark tendrils that permeate the Milky Way are due to enormous clouds of cosmic dust. These clouds of tiny particles absorb and scatter light, making huge patches of the Milky Way appear dark to human eyes from our vantage point here on Earth. Telescopes such as Gemini North, however, see the night sky differently. They are designed to collect far more light that the human eye can, thanks to their large primary mirrors. They can also detect ranges of light that humans cannot, meaning that they can probe areas of cosmic dust, giving us information on things that would otherwise remain obscured.
Español: El telescopio Gemini Norte, parte boreal del Observatorio Gemini (un Programa de NOIRLab de NSF), protagoniza el primer plano de esta imagen, bajo un cielo cristalino. Pero si entrecierras los ojos, da la sensación que el telescopio del fondo estuviese en llamas, enviando columnas de humo hacia el cielo estrellado. Por suerte, el vecino más cercano de Gemini Norte no se está incendiando, y ese espectacular “humo blanco” que se proyecta hacia el cielo, corresponde a nuestra galaxia, la Vía Láctea.
Los filamentos oscuros que se extienden en la Vía Láctea son enormes nubes de polvo cósmico. Estas nubes de pequeñas partículas absorben y dispersan la luz, formando enormes manchas oscuras para los ojos humanos desde nuestra perspectiva aquí en la Tierra. Sin embargo, telescopios como Gemini Norte observan el cielo de forma distinta: Gracias a sus grandes espejos primarios, están diseñados para recoger mucha más luz que el ojo humano. Además, tienen la capacidad de detectar rangos de luz que los ojos humanos no pueden, lo que significa que pueden sondear estas oscuras áreas de polvo cósmico, dándonos información de cosas que de otra forma permanecerían ocultas. |
Date | |
Source | https://noirlab.edu/public/images/iotw2213a/ |
Author | International Gemini Observatory/NOIRLab/NSF/AURA/J. Chu |
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[edit]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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current | 18:05, 22 June 2023 | 5,966 × 3,934 (6.43 MB) | C messier (talk | contribs) | full size | |
21:41, 30 January 2023 | 1,280 × 844 (247 KB) | Yiseth Romero (talk | contribs) | Uploaded a work by International Gemini Observatory/NOIRLab/NSF/AURA/J. Chu from https://noirlab.edu/public/images/iotw2213a/ with UploadWizard |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Author | Jason K. Chu |
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Copyright holder |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA/J. Chu |
Source | NSF's NOIRLab |
Online copyright statement | http://www.jason-chu.artistwebsites.com/ |
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Date and time of data generation | 12:00, 30 March 2022 |
JPEG file comment | Gemini North, of the international Gemini Observatory (a Program of NSF’s NOIRLab), stands peacefully in the foreground, under a crystal clear sky. If you narrow your eyes, however, it looks a little as though the telescope in the background of this image is on fire, sending plumes of smoke up into the starry sky. Fortunately, Gemini North’s near neighbor is not ablaze! The dramatic upward sweep of milky and sooty patches is in fact the Milky Way galaxy. The dark tendrils that permeate the Milky Way are due to enormous clouds of cosmic dust. These clouds of tiny particles absorb and scatter light, making huge patches of the Milky Way appear dark to human eyes from our vantage point here on Earth. Telescopes such as Gemini North, however, see the night sky differently. They are designed to collect far more light that the human eye can, thanks to their large primary mirrors. They can also detect ranges of light that humans cannot, meaning that they can probe areas of cosmic dust, giving us information on things that would otherwise remain obscured. |
Software used | Adobe Photoshop 22.0 (Windows) |
File change date and time | 12:15, 17 January 2021 |
Date metadata was last modified | 13:15, 17 January 2021 |
Date and time of digitizing | 15:14, 1 July 2020 |
Unique ID of original document | B8EE4FC76923FD6B3A5660975F25EEA1 |
Keywords | Gemini North |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |