What is the general upper mass limit defining a low-mass star relative to the Sun?
Answer
Less than about eight times the mass of the Sun ($< 8 M_{\odot}$)
Astronomers generally classify a star as low-mass if its mass is less than about eight times the mass of the Sun ($M < 8 M_{\odot}$).
#Videos
Low Mass Stars: Crash Course Astronomy #29 - YouTube
Related Questions
What is the general upper mass limit defining a low-mass star relative to the Sun?What celestial body results if mass falls below the critical fusion threshold of $0.08 M_{\odot}$?Which primary fusion chain powers stars at the lower end of the low-mass spectrum, such as red dwarfs?What evolutionary phase does a Sun-like star enter after exhausting the hydrogen fuel in its core?What is the final remnant core left behind after a typical Sun-like star sheds its outer layers?What fate do theoretical models suggest awaits the smallest red dwarfs without a significant expansion phase?Where is the Habitable Zone located relative to a low-mass star compared to the Sun?What significant effect is likely to occur to a planet orbiting very closely within a low-mass star's Habitable Zone?What danger do younger red dwarfs present to the atmospheres of closely orbiting planets?What fusion mechanism is primarily used by stars above about $1.3$ solar masses?