Emission nebula | |
---|---|
Reflection nebula | |
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Observation data: J2000 epoch | |
Right ascension | 10h 45m 03.6s[1] |
Declination | −59° 41′ 04″[1] |
Distance | 7,500 ly |
Apparent magnitude (V) | 6.21 (-0.8–7.9) (including the central star) |
Apparent dimensions (V) | 18"[2] |
Constellation | Carina |
Physical characteristics | |
Radius | 0.29[2] ly |
Notable features | Bipolar 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.[3] 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.[4]
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.[2]