The star is roughly 33 million years old and is spinning with a projected rotational velocity of 50 km/s. It is radiating 8,442 times the solar luminosity from its outer atmosphere at an effective temperature of around 20,815 K.
The star in question is estimated to be roughly 33 million years old and has a significant rotational velocity of approximately 50 km/s. It emits an enormous amount of energy, significantly greater than the sun's, from its outer atmosphere at an effective temperature around 20,815 K.