description HR 2562 b Overview
HR 2562 b is a directly imaged substellar companion to the young F-type star HR 2562. It lies at a projected separation of about 20 astronomical units and has a poorly constrained mass, with published estimates spanning roughly 13 to 30 Jupiter masses. The system contains a debris disk, and the companion's mass places it near the boundary between a very massive planet and a brown dwarf, so its classification depends partly on the adopted formation definition.
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