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Comment by delta_p_delta_x

Worth noting that the artist's impression is... not accurate. Both CD-35 2722 b (the brown dwarf orbiting the primary star) and CD-35 2722 b I (the exomoon orbiting the secondary) should be much closer in size. It is estimated that Jupiter is essentially the largest any gas giant can get; adding more mass will simply increase density and interior temperature until deuterium and lithium fusion and brown dwarfdom, and then at around 80 Jupiter masses, protium fusion and stardom.

Look at Barnard's Star[1], which is actually a fusing red dwarf star: it is not much bigger than Jupiter.

[1]: https://en.wikipedia.org/wiki/Barnard%27s_Star

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