description M1-67 Nebula Overview
M1-67 is an emission nebula surrounding the Wolf-Rayet star WR 124 in the constellation Sagitta, roughly 20,000 light-years from Earth. The nebula consists of gas expelled by the massive, evolved star and shaped by its powerful stellar wind. Its irregular knots and clumps are moving outward, providing astronomers with a view of substantial mass loss during a short-lived stage preceding the star's eventual supernova.
help M1-67 Nebula FAQ
Where is the M1-67 nebula located?
The M1-67 nebula is located in the northern sky within the small constellation of Sagitta, roughly 20,000 light-years from Earth. It surrounds a massive central star known as WR 124.
What kind of star sits at the center of the M1-67 nebula?
The nebula surrounds a Wolf-Rayet star, which is an incredibly hot, massive, and evolved star nearing the end of its life cycle. This star emits powerful stellar winds that continuously shape the surrounding gas.
How was the M1-67 nebula formed?
The irregular knots and clumps of gas seen in the nebula were physically expelled by the central star. The intense stellar wind from the massive star pushes this material outward into space at incredible speeds.
What type of nebula is M1-67 classified as?
M1-67 is classified as an emission nebula because the gases within it glow from the intense ultraviolet radiation emitted by the central star. These glowing gases provide a spectacular and colorful target for advanced astrophotography.
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