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New View of the Great Nebula in Carina
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Name: Carina Nebula, NGC 3372, Eta Carinae
Description: Star Formation nebula, Wolf-Rayet type star
Position (J2000): RA 10h 45m 4.8s Dec -59° 48' 34.8"
Constellation: Carina
Distance: 10,000 Light Years
Field of View: 1.0 x 1.0 degrees
Image Credit: NASA/JPL-Caltech/M. Povich (Penn State Univ.)
Release Date: May 24, 2011

Other:  2000  2007  2009a  2009b  2010  2011a  2011b  2012a  2012b  2018
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Eta Carinae is one of the most massive and brightest stars in the Milky Way. Compared to our own Sun, it is about 100 times as massive and a million times as bright. This famed variable hypergiant star (upper center) is surrounded by the Carina Nebula. In this composite image spanning the visible and infrared parts of the spectrum, areas that appear blue are not obscured by dust, while areas that appear red are hidden behind dark clouds of dust in visible light. A study combining X-ray and Infrared observations has revealed a new population of massive stars lurking in regions of the nebula that are highly obscured by dust. Adding these new massive stars to the known massive stars suggests that the Carina Nebula will produce twice as many supernova explosions as previously supposed.

Visible light in the blue part of the spectrum from the Digital Sky Survey is represented as blue, near infrared light with a wavelength of 2.2 microns from the Two Micron All Sky Survey (2MASS) is green, and infrared observations from the Infrared Array Camera on NASA's Spitzer Space telescope at 3.6 microns is red