Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

Jump to content

Blue Ring Nebula

From Wikipedia, the free encyclopedia
Blue Ring Nebula
Nebula
Composite image of the Blue Ring Nebula.
Observation data: J2000[1] epoch
Right ascension16h 48m 37.41s
Declination+35° 12' 09.44"
Distance6,300 ly
ConstellationHercules
See also: Lists of nebulae

The Blue Ring Nebula is a cosmic object located approximately 6,300 light years away in the constellation Hercules.[2] It was formed when two stars merged, creating a debris cloud that eventually cooled down and produced hydrogen molecules that collided with the interstellar medium. The collisions made the molecules radiate far-ultraviolet light, allowing GALEX to discover the object in 2004.[3] The merging of the two stars resulted into a new star designated as TYC 2597-735-1.[4][5]

References

[edit source]
  1. "TYC 2597-735-1". SIMBAD. CDS. Retrieved 3 August 2026.
  2. "Blue Ring Nebula". GALEX. Caltech. Retrieved 3 August 2026.
  3. "The Blue Ring Nebula". NASA Jet Propulsion Laboratory. NASA. Retrieved 3 August 2026.
  4. "X-Ray Emission from Candidate Stellar Merger Remnant TYC 2597-735-1 and Its Blue Ring Nebula". The Astronomical Journal. 163 (4): 173. April 2022. doi:10.3847/1538-3881/ac54a2. Retrieved 3 August 2026.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  5. "The dazzling Blue Ring Nebula puzzled scientists for 16 years — and now they finally understand why". Space.com. Future plc. 18 November 2020. Retrieved 3 August 2026.