description NGC 2467 (Skull and Crossbones) Overview
NGC 2467 is an active star-forming region located in the southern constellation of Puppis. The nebula consists of bright emission clouds interspersed with dark dust lanes, creating an appearance that has led to its unofficial nickname, the Skull and Crossbones. It serves as a rich area for astronomical observation, containing massive young stars and stellar groupings.
help NGC 2467 (Skull and Crossbones) FAQ
Where is NGC 2467, and how far away is it?
NGC 2467 lies in the southern constellation of Puppis, within the Milky Way. ESA/Hubble data place it at roughly 13,000 light-years from Earth.
Why is NGC 2467 called the Skull and Crossbones Nebula?
Bright emission clouds are broken up by dark dust lanes that create a skull-like pattern in images. Skull and Crossbones is an informal nickname, not the object's formal astronomical designation.
Is NGC 2467 a nebula or a star cluster?
It is an H II emission region and active stellar nursery, also known as Sharpless 311 or S311. The wider complex includes young stellar groups such as Haffner 18 and Haffner 19, which is why some catalogs describe both nebulosity and clusters.
What makes NGC 2467 glow?
Radiation from massive young stars ionizes the surrounding hydrogen gas and makes the nebula shine. Astronomical studies identify the O6-type star HD 64315 as a major source of that energy.
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