The total luminosity of the main feature is 101 L and;.

The total luminosity varied widely from hour to hour, but not simultaneously in all wavelengths.

As a result of the steady accumulation of helium at the Sun's core, the star's total luminosity will slowly increase.

Its X-ray output is 2.3x10 W, about 60,000 times the total luminosity of the Sun.

The total luminosity is about 2,500 times that of the Sun, and it has estimated 180 times the Sun's radius.

Its temperature is approximately 13,000 K giving it a total luminosity that is 2,400 times solar.

At about 5,000 days post-supernova (November of 2000), however, the predicted decline stopped, and the total luminosity started to rise again.

The magnitude varies by about 0.03, or about 3% of the total luminosity.

The total luminosity of this cluster is around 120,000 times that of the Sun, the absolute magnitude being -8.04.

At present its total luminosity equals 280 Sols; and this is slowly, inexorably rising.