What are the final evolutionary stages for low-mass stars (between 0.5 M☉ and 8 M☉)?
Answer
Red Giant phase leading to a Planetary Nebula and then a White Dwarf
Low-mass stars swell into Red Giants, shed their outer layers as a planetary nebula, and their dense, hot core remnant eventually cools as a White Dwarf.
#Videos
How Does Mass Affect a Star's HR Diagram Evolution? - YouTube
Related Questions
What single property dictates nearly every aspect of a star's existence?According to the Initial Mass Function (IMF), which type of star is the most common inhabitant of galaxies?What fate awaits a stellar object beginning its life with less than 0.08 times the mass of the Sun?How does luminosity (L) generally scale with mass (M) for main-sequence stars?Why do massive stars have surprisingly brief lifespans relative to their size?What is the expected lifespan of our Sun on the main sequence?What are the final evolutionary stages for low-mass stars (between 0.5 M☉ and 8 M☉)?In high-mass stars, what causes the fusion furnace to switch off, leading to immediate collapse?What process is responsible for forging elements heavier than iron throughout the cosmos?What type of remnant is formed from a progenitor star between approximately 8 M☉ and 25 M☉?What ultimate gravitational fate awaits the core remnant of the truly most massive stars (exceeding approximately 25 M☉ at birth)?