File:Starry Night, Laser Light.jpg
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DescriptionStarry Night, Laser Light.jpg |
English: Gemini South, one half of the International Gemini Observatory, a Program of NSF’s NOIRLab, is seen here with its laser guide star in action. Both of the Gemini telescopes use laser guide stars to provide data for the calibration of their adaptive optics, systems of deformable mirrors that compensate for fluctuations in the upper atmosphere which can blur the images of distant stars and galaxies. The laser excites trace gas particles high in Earth’s upper atmosphere. Software then analyzes feedback from the laser to provide a model for the adaptive optics to map against. The laser guide stars can also be augmented by additional adaptive optics systems that use imagesof real stars from the telescope itself, such as the Natural Guide Star Next Generation Sensor (NGS-2). This photo was taken as part of the recent NOIRLab 2022 Photo Expedition to all the NOIRLab sites.
аԥсшәа: Gemini Sur, la mitad austral del Observatorio Gemini, un Programa de NOIRLab de NSF, protagoniza esta fotografía junto con su sistema de guía láser en acción. Ambos telescopios Gemini utilizan estrellas guía láser para calibrar sus ópticas adaptativas, que consisten en sistemas de espejos deformables que compensan las fluctuaciones de la atmósfera superior y que pueden distorsionar las imágenes de estrellas y galaxias distantes. El láser estimula las partículas de gas que están en la parte superior de la atmósfera terrestre. Luego, un software analiza la respuesta del láser para proporcionar un modelo con el que la óptica adaptativa puede proveer una imagen sin la distorsión que provoca la atmósfera terrestre. Las estrellas guía láser también pueden aumentarse con sistemas de óptica adaptativa adicionales que utilizan imágenes de estrellas reales creadas por el mismo telescopio, como el Sensor de Próxima Generación de Estrellas Guía Naturales (NGS-2).
Esta fotografía fue tomada como parte de la reciente Expedición Fotográfica de NOIRLab 2022 a todos los sitios de NOIRLab. |
Date | |
Source | https://noirlab.edu/public/images/iotw2223a/?nocache=true |
Author | International Gemini Observatory/NOIRLab/NSF/AURA/T. Slovinský |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:20, 22 June 2023 | 13,000 × 9,199 (26.97 MB) | C messier (talk | contribs) | full size | |
14:37, 29 March 2023 | 1,280 × 906 (252 KB) | Yiseth Romero (talk | contribs) | Uploaded a work by International Gemini Observatory/NOIRLab/NSF/AURA/T. Slovinský from https://noirlab.edu/public/images/iotw2223a/?nocache=true with UploadWizard |
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ISO speed rating | 6,400 |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA/T. Slovinský |
Source | NSF's NOIRLab |
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Date and time of data generation | 12:00, 8 June 2022 |
JPEG file comment | Gemini South, one half of the International Gemini Observatory, a Program of NSF’s NOIRLab, is seen here with its laser guide star in action. Both of the Gemini telescopes use laser guide stars to provide data for the calibration of their adaptive optics, systems of deformable mirrors that compensate for fluctuations in the upper atmosphere which can blur the images of distant stars and galaxies. The laser excites trace gas particles high in Earth’s upper atmosphere. Software then analyzes feedback from the laser to provide a model for the adaptive optics to map against. The laser guide stars can also be augmented by additional adaptive optics systems that use images of real stars from the telescope itself, such as the Natural Guide Star Next Generation Sensor (NGS-2). This photo was taken as part of the recent NOIRLab 2022 Photo Expedition to all the NOIRLab sites. |
Software used | Adobe Photoshop 23.0 (Windows) |
File change date and time | 17:07, 3 May 2022 |
Date and time of digitizing | 02:53, 7 April 2022 |
Date metadata was last modified | 19:07, 3 May 2022 |
Unique ID of original document | xmp.did:12989a41-cd21-4f62-979b-e2d4a4e1a391 |
Keywords | Gemini South |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |
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