File:Infrared view of the Rho Ophiuchi star-forming region (eso1234c).tiff

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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.
Date 29 August 2012, 12:00
Source https://www.eso.org/public/images/eso1234c/
Author NASA/JPL-Caltech/WISE Team
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Date/TimeThumbnailDimensionsUserComment
current08:23, 3 December 2021Thumbnail for version as of 08:23, 3 December 202110,282 × 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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