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

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Summary

Artist's conception of the <a href="https://en.wikipedia.org/wiki/Epsilon_Indi" class="extiw" title="en:Epsilon Indi">Epsilon Indi</a> 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.

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File history

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Date/TimeThumbnailDimensionsUserComment
current10:07, 8 January 2017Thumbnail for version as of 10:07, 8 January 20173,000 × 2,100 (262 KB)127.0.0.1 (talk)Artist's conception of the <a href="https://en.wikipedia.org/wiki/Epsilon_Indi" class="extiw" title="en:Epsilon Indi">Epsilon Indi</a> 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.
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