Earlier quoted context omitted.
Does this also hold for rogue planets? I was under the impression that some rogue planets could form outside of any star's accretion disk.
My understanding is that smaller rouge plants do not form in isolation and are always the product of ejection. However, the categorization again is fuzzy, with definitional overlap between "planet", "sub-brown-dwarf", and "brown dwarfs" Planets cover spherical objects ranging from 0.001 Jupiter masses to stars at ~80 Jupiter masses. Brown dwarfs range from 3-80 Jupiter masses. Brown Dwarfs are planets and can form ou…
Wikipedia says "Rogue planets may originate from planetary systems in which they are formed and later ejected, or they can also form on their own, outside a planetary system."