Eta Carinae
- Type
- Star System (binary)
- Diameter
- 51,874,560 to 761,691,456 miles (a), 12,363,436 to 20,403,992 miles (b)
- Mass
- 100 suns (a), 30 to 80 suns (b)
- Distance
- Around 7,500 light years
- Temperature
- 16,460 to 62,900 °F (a), 66,500 °F (b)
- Star Type
- LBV - Wolf-Rayet Star (a), O(?) (b)
- Date of Discovery
- 17th century
- Other Names
- Foramen, Tseen She, 231 G Carinae, HR 4210, HD 93308
- Eta Carinae is a binary star system, with a massive, very bright star, one of the most luminous (brightest) in the galaxy. It is known for a nebula that has formed around it after a violent eruption in the 19th century.
- Draw a picture of Eta Carinae and its nebula.

- Located in
- Carina, Milky Way
- The combined stars of Eta Carinae are so powerful and bright, that they might be as much as 5 million times or more the brightness of our Sun.
- The primary star is the only star known to produce ultraviolet laster emissions.
- The nebula surrounding the star, called the Homunculus Nebula, is the material that was ejected by the main star during the Great Eruption in 1837.