NGC 3372 Carina Nebula
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NGC 3372 Carina Nebula
The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun.
The circular 'keyhole' structure contains both bright filaments of hot gas and dark silhouetted clouds of cold molecules and dust, all of which are in rapid, chaotic motion. Two striking large, sharp-edged dust clouds are located near the bottom centre and upper-left edges of the image. These large dark clouds may eventually evaporate or, if there are sufficiently dense condensations within them, give birth to small star clusters.
The Carina Nebula, with an overall diameter of more than 200 light-years, is one of the outstanding features of the southern-hemisphere part of the Milky Way.
The circular 'keyhole' structure contains both bright filaments of hot gas and dark silhouetted clouds of cold molecules and dust, all of which are in rapid, chaotic motion. Two striking large, sharp-edged dust clouds are located near the bottom centre and upper-left edges of the image. These large dark clouds may eventually evaporate or, if there are sufficiently dense condensations within them, give birth to small star clusters.
The Carina Nebula, with an overall diameter of more than 200 light-years, is one of the outstanding features of the southern-hemisphere part of the Milky Way.
SPECIFICATIONS
Telescope
CHI-2
Camera
FLI PL 16803
Location
Rio Hurtado valley, Chile
Date of observation
2020-04-01
Filters
Halpha, SII, OIII
Processing
Processing 3X600s Halpha, 3X600s SII, 3X600s OIII aligned, integreted and comined then edited all in pixinsight.
Credits
79 credits
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