Wolf-Rayet stars like WR 134 are massive stars that burn through their nuclear fuel rapidly and emit powerful stellar winds that sweep material into complex shells, eventually ending in supernova explosions that enrich the interstellar medium with heavy elements for future star formation.
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The Nebulous Realm of WR 134 dazzled with glowing arcs and cosmic winds #NASA #SpaceAdded:
Welcome to NASA's Astronomy Picture of the Day for May 22nd, 2026, titled The Nebulous Realm of WR 134.
This cosmic snapshot covered a field of view over twice as wide as the full moon within the boundaries of the high-flying constellation Cygnus.
Made using astronomical narrow-band filters, >> [music] >> the image highlighted the bright edge of a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas.
Embedded in the region's expanse of interstellar clouds, the complex glowing arcs were sections of shells of material swept up by the wind from Wolf-Rayet star WR 134, [music] the brightest star near image center.
Distance estimates put WR 134 about 6,000 light-years away, >> [music] >> making this telescopic frame over 100 light-years across.
Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars had burned through their nuclear fuel at a prodigious rate and ended their final phase of massive star evolution in a spectacular supernova.
Their stellar winds and final supernova explosion enriched the interstellar material with heavy elements to be incorporated in future generations of stars.
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