File:Artist's Conception of Epsilon Indi System (labelled).jpg
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Captions
This exoplanet was discovered in 2019 and it is a gas giant planet
Summary
[edit]DescriptionArtist's Conception of Epsilon Indi System (labelled).jpg |
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 | Artist's conception of the Epsilon Indi system |
Author | International Gemini Observatory/NOIRLab/NSF/AURA/Lomberg J. |
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current | 08:44, 28 October 2023 | 3,000 × 2,100 (417 KB) | Юрий Д.К. (talk | contribs) | original file with an explicit permission in EXIF | |
06:54, 9 May 2015 | 3,000 × 2,100 (262 KB) | Jcpag2012 (talk | contribs) | full resolution | ||
16:34, 28 June 2008 | 600 × 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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Image title |
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Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA/Lomberg J. |
Source | NSF's NOIRLab |
Short title |
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Usage terms |
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Date and time of data generation | 05:00, 27 October 2004 |
Keywords | Epsilon Indi |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |