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File:Artist's Conception of Epsilon Indi System (labelled).jpg

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Summary

Description
English: Artist's conception of the Epsilon Indi system showing Epsilon Indi and the brown-dwarf binary companions. Due to the perspective of the brown dwarf companions, the relative sizes are not represented in this illustration. Brown dwarfs have a radius close to Jupiter. The more massive brown dwarf would be denser and brighter in the Near-IR.
Date
Source http://www.gemini.edu/science/epsilonindi.html
Author Jon Lomberg

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Public domain This work has been released into the public domain by its author, Jon Lomberg. This applies worldwide.
In some countries this may not be legally possible; if so:
Jon Lomberg grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

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Date/TimeThumbnailDimensionsUserComment
current06:54, 9 May 2015Thumbnail for version as of 06:54, 9 May 20153,000 × 2,100 (262 KB)Jcpag2012full resolution
16:34, 28 June 2008Thumbnail for version as of 16:34, 28 June 2008600 × 420 (22 KB)NuclearVacuum{{Information |Description={{en|1=Artist's conception of the Epsilon Indi system showing Epsilon Indi and the brown-dwarf binary companions. Due to the perspective of the brown dwarf companions, the relative sizes are not represented
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