| To expand on this, as stated in your source: > [270B solar masses] is the maximum mass of a black hole that models predict, at least for luminous accreting SMBHs. as well as: > The limit is only 5×10^10 M [50B solar masses] for black holes with typical properties, but can reach 2.7×10^11 M [270B solar masses] at maximal prograde spin (a = 1). However in the chapter before, it's stated: > New discoveries suggest that many black holes, dubbed 'stupendously large', may exceed 100 billion or even 1 trillion M. |