Context. The tidal evolution of planets orbiting brown dwarfs (BDs) presents an interesting case study because BDs’ terrestrial planet forming region is located extremely close-in. In fact, the habitable zones of BDs range from roughly 0.001 to 0.03 AU and for the lowest-mass BDs are located interior to the Roche limit.
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Bolmont et al. (2011) studied this question.
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