Homunculus Nebula

The Homunculus Nebula is a bipolar emission and reflection nebula surrounding the massive star system Eta Carinae, about 7,500 light-years (2,300 parsecs) from Earth. The nebula is embedded within the much larger Carina Nebula, a large star-forming H II region. From the Latin homunculus meaning Little Man, the nebula consists of gas which was ejected from Eta Carinae during the Great Eruption, which occurred ~7,500 years before it was observed on Earth, from 1838 to 1845. It also contains dust which absorbs much of the light from the extremely luminous central stellar system and re-radiates it as infra-red (IR). It is the brightest object in the sky at mid-IR wavelengths.

Homunculus Nebula
Emission nebula
Reflection nebula
Observation data: J2000 epoch
Right ascension10h 45m 03.6s
Declination−59° 41 04
Distance7,500 ly
Apparent magnitude (V)6.21 (-0.8–7.9) (including the central star)
Apparent dimensions (V)18"
ConstellationCarina
Physical characteristics
Radius0.29 ly
Notable featuresBipolar nebula

Within the Homunculus is a smaller Little Homunculus, and within that a shell of shocked material from stellar winds that has been called Baby Homunculus.

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