Eta Carinae Nebula (NGC 3372)
Also called the Carina Nebula or the Great Nebula
in Carina, a spectacular diffuse
nebula in the constellation Carina –
one of the largest and brightest in the sky. Indeed, the Eta Carinae Nebula
(NGC 3372) is one of the largest HII regions
in the entire Milky Way Galaxy – four times larger than the Orion
Nebula (which itself is part of the Orion Molecular Cloud Complex).
The only reason the Carina Nebula isn't better known is that it cannot be
seen from most of the northern hemisphere. It was discovered by Abbé
Nicolas Louis de Lacaille during his 2-year
journey to the Cape of Good Hope in 1751–52.
In addition to Eta Carinae itself, the Nebula
contains several stars that are among the hottest and most massive known,
each about 10 times as hot, and 100 times as massive, as our Sun.
Eight catalogued open clusters fall
within the area of the Eta Carinae Nebula. These are Collinder (Cr) 228,
Bochum (Bo) 10, Trumpler (Tr) 14 (also cataloged as Cr 230), Tr 15 (= Cr
231), Cr 232, Tr 16 (= Cr 233), Cr 234, and Bo 11. The star Eta Carinae
is part of the cluster Trumpler 16.
The Keyhole Nebula (NGC 3324) is a dark cloud, whose round
portion is some 7 light-years across, that is silhouetted against the brighter
background near Eta Carinae.
 |
The Keyhole Nebula. Hubble Space
Telescope image |
| visual magnitude |
1.0 |
| angular diameter |
2° |
| linear diameter |
200 light-years |
| distance |
7,500 light-years |
| position |
R.A. 10h 44m;
Dec. -59° 52' |
Related category
• NEBULAE
AND STAR CLUSTERS
Also on this site: Encyclopedia
of Alternative Energy & Sustainable Living
Encyclopedia
of History
BACK TO TOP
|