IC 2599

IC 2599 (Gabriela Mistral Nebula) is an emission nebula (hydrogen or HII region) excited by an open star cluster (OCL 819) in its center. It is in the constellation Carina and located northwest of the Eta Carina Nebula (NGC 3372). The nebula lies at a distance of 7,560 ly (2,317 pc) from Earth.

IC 2599 is associated with the open cluster NGC 3324. A rich deposit of gas and dust in the NGC 3324 region fuelled a burst of starbirth millions of years ago and led to the creation of several extremely massive and very hot stars. The intense ultraviolet radiation from these hot young stars causes the gas cloud to glow and has carved out a cavity in the surrounding gas and dust. In fact the stars are slowly eroding the gas cloud away.

NGC 3324 is an open cluster in the constellation Carina, located northwest of the Eta Carina Nebula (NGC 3372) at a distance of 7,560 ly (2,317 pc) from Earth.

IC 2599 (aka Gum 31) is sometimes called the "Gabriela Mistral Nebula" due to its resemblance to the Nobel Prize-winning poet from Chile. NGC 3324 was first catalogued by James Dunlop in 1826. See Wikipedia for more details.

This image captures IC 2599 through a Hydrogen Alpha filter.

Technical Details



Return to: Chile Remote Obs






AstroPixels Links

| Open Clusters | Globular Clusters | Diffuse Nebulae | Planetary Nebulae | Supernovae | Galaxies |
 | 
Messier Catalog Photo Gallery | 
Messier Catalog | 
Caldwell Catalog Photo Gallery | 
Caldwell Catalog | 
 | 
AstroPixels Photo Index | 
Recent Images | 
Images with ASA N12 |
 | 
Chile Remote Obs |
Southern Sky |
Southern Sky 2018 |