File:Infrared view of the Rho Ophiuchi star-forming region (eso1234c).tiff
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![File:Infrared view of the Rho Ophiuchi star-forming region (eso1234c).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/3/38/Infrared_view_of_the_Rho_Ophiuchi_star-forming_region_%28eso1234c%29.tiff/lossy-page1-610px-Infrared_view_of_the_Rho_Ophiuchi_star-forming_region_%28eso1234c%29.tiff.jpg?20211203082324)
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DescriptionInfrared view of the Rho Ophiuchi star-forming region (eso1234c).tiff | This image shows the Rho Ophiuchi star-forming region in infrared light, as seen by NASA’s Wide-field Infrared Explorer (WISE). Blue and cyan represent light emitted at wavelengths of 3.4 and 4.6 micrometres, which is predominantly from stars. Green and red represent light from 12 and 22 micrometres, respectively, which is mostly emitted by dust. | ||||||||||||
Date | 29 August 2012, 12:00 | ||||||||||||
Source | https://www.eso.org/public/images/eso1234c/ | ||||||||||||
Author | NASA/JPL-Caltech/WISE Team | ||||||||||||
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current | 08:23, 3 December 2021 | ![]() | 10,282 × 10,100 (123.39 MB) | Junior Jumper (talk | contribs) | {{Information |Description=This image shows the Rho Ophiuchi star-forming region in infrared light, as seen by NASA’s Wide-field Infrared Explorer (WISE). Blue and cyan represent light emitted at wavelengths of 3.4 and 4.6 micrometres, which is predominantly from stars. Green and red represent light from 12 and 22 micrometres, respectively, which is mostly emitted by dust. |Source=https://www.eso.org/public/images/eso1234c/ |Date={{Date|2012|08|29}}, 12:00 |Author=NASA/JPL-Caltech/WISE Team... |
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Height | 10,100 px |
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Compression scheme | LZW |
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Orientation | Normal |
Number of components | 3 |
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Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
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Software used | Adobe Photoshop CS5 Macintosh |
File change date and time | 17:40, 23 August 2012 |
Color space | Uncalibrated |