Which of these measurements is the lower limit for a main-sequence star that will eventually form a black hole?
A) 50 solar masses
B) 25 solar masses
C) 3 solar masses
D) 1.4 solar masses

Question

Quizplus · Accepted Answer

The lower limit for a main-sequence star to eventually form a black hole is generally considered to be around 25 solar masses. Stars with this mass or greater can undergo a supernova explosion and leave behind a black hole.

Which of These Measurements Is the Lower Limit for a Main-Sequence