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

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This exoplanet was discovered in 2019 and it is a gas giant planet

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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.
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Source Artist's conception of the Epsilon Indi system
Author International Gemini Observatory/NOIRLab/NSF/AURA/Lomberg J.

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Date/TimeThumbnailDimensionsUserComment
current08:44, 28 October 2023Thumbnail for version as of 08:44, 28 October 20233,000 × 2,100 (417 KB)Юрий Д.К. (talk | contribs)original file with an explicit permission in EXIF
06:54, 9 May 2015Thumbnail for version as of 06:54, 9 May 20153,000 × 2,100 (262 KB)Jcpag2012 (talk | contribs)full resolution
16:34, 28 June 2008Thumbnail for version as of 16:34, 28 June 2008600 × 420 (22 KB)NuclearVacuum (talk | contribs){{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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