The absolute brightness (or luminosity) of a star is related to its mass. Generally, more massive stars tend to be more luminous. According to the mass-luminosity relation, for main sequence stars, the luminosity is approximately proportional to the mass raised to a power (often around 3 to 4).
In the case of the stars you provided:
- Star L: \(10x\)
- Star M: \(2.5x\)
- Star N: \(0.5x\)
- Star O: \(15x\)
Among these stars, Star N has the lowest mass (0.5 times the mass of the sun). As a result of the mass-luminosity relationship, Star N is expected to have the lowest absolute brightness.
Thus, the star that most likely has the lowest absolute brightness is:
N