Carina nebula

From Simple English Wikipedia, the free encyclopedia
An image of the Carina nebula taken by the European Southern Observatory's Very Large Telescope (Ultra high image available by clicking)
The Cosmic Cliffs at the edge of NGC 3324, one of the first images taken by the James Webb Space Telescope

The Carina nebula (NGC 3372 or the Great Nebula in Carina, the Eta Carina nebula) is a large, bright nebula. It is around 7,500 light years from Earth and has over 14,000 stars.[1][2] It appears in the constellation of Carina in the Carina–Sagittarius Arm of the Milky Way. The Carina nebula was discovered by Nicolas Louis de Lacaille in 1751 from the Cape of Good Hope.[3] The French astronomer had made an astronomical expedition to record objects in the southern sky.

From the description in WP Commons:

"Trumpler 16 is an open cluster that contains the massive luminous blue variable Eta Carinae, one of the brightest stars in the galaxy. It is possibly as much as 120 times the mass of the Sun, and emits the light of 4,000,000 Suns. Eta Carinae is nearing the end of its life, and is surrounded by a huge nebula, cast off by numerous eruptions of the star over the last several centuries. It is expected to explode into a supernova at any time. Trumpler 14 (annotated) contains the huge double star HD 93129 A/B. The young O3 class star HD 93129 A is one of the brightest stars in the galaxy that is still on the main sequence, and with a luminosity equivalent to 3,000,000 Suns. It is very nearly as bright as Eta Carinae, but this is not obvious in the photo due to obscuring nebulosities".

References[change | change source]

  1. "The Carina Nebula", How it Works, no. 34, Imagine Publishing, p. 47, 2012-05-17
  2. "Carina Nebula". NASA. Archived from the original on 2012-05-24. Retrieved 2012-05-18.
  3. Coffey, Jerry (2009-12-14). "Carina Nebula". Universe Today. Retrieved 2012-05-18.