Discontinued due to lack of motivation and citing. Sorry.
BASIC INFO
Eta Carinae A, the primary star in the Eta Carinae system, is one of the most massive and luminous stars known in the Milky Way galaxy. Classified as a luminous blue variable (LBV) star, it exhibits dramatic variability in brightness attributed to its unstable outer layers and episodic mass loss. Eta Carinae A is famous for its Great Eruption, a spectacular outburst event in the mid-19th century that briefly made it one of the brightest objects in the night sky. As part of a binary system with Eta Carinae B, it generates powerful stellar winds and plays a crucial role in shaping the surrounding nebula.
ADVANCED INFO
Size: 346.15 million miles across
Mass: 120 solar masses
Distance from Earth: 7,502 light-years
Galaxy: Milky Way
Age: Less than 3 million years old
Luminosity: 4.6 million L
Type: Luminous blue variable
Temperature: 26,540 Fahrenheit (14,727 Celsius) (At surface)
SOME RANDOM FACTS
Despite its extreme properties, the future evolution of Eta Carinae A remains uncertain.
Like other LBVs, Eta Carinae A exhibits significant variability in its brightness over time. These fluctuations in luminosity are thought to be caused by instability in the star's outer layers and episodic mass loss.
Eta Carinae A is famous for its Great Eruption, a colossal outburst event that occurred in the mid-19th century (around 1837-1856). During this event, the star briefly became one of the brightest objects in the night sky, rivaling even Sirius, the brightest star visible from Earth.