Stellar mass

Stellar mass is a phrase that is used by astronomers to describe the mass of a star. It is usually enumerated in terms of the Sun's mass as a proportion of a solar mass (M_☉). Hence, the bright star Sirius has around 2.02 M_☉.^[1] A star's mass will vary over its lifetime as mass is lost with the stellar wind or ejected via pulsational behavior, or if additional mass is accreted, such as from a companion star.

^ Cite error: The named reference Liebert2005 was invoked but never defined (see the help page).

[Liebert2005-1] Cite error: The named reference Liebert2005 was invoked but never defined (see the help page).

[1]