|
Explanation: Why would a gamma ray burst fade so slowly? This behavior, recorded last October, is considered a new clue into the cause of gamma-ray bursts, the most powerful explosions known in the universe. The burst, first detected by the orbiting HETE satellite and later tracked by numerous ground-based telescopes, showed an unusually slow and tumultuous decay in visible light. Speculations on the cause of the unusual light curve include a blast wave striking a windy circumburst medium, a blast wave energetically refreshed by a faster outgoing shock, and non-uniformity in a fast moving jet. Pictured above is the massive Wolf-Rayet star WR124, a star itself undergoing a slow explosion by producing a very powerful but tumultuous wind. Popular candidate progenitor sources for GRBs include supernova or hypernova explosions from massive stars, possibly ones with similarities to Wolf-Rayet stars.
|
January February March April May June July August September October November December |
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: GRB - Wolf-Rayet star
Publications with words: GRB - Wolf-Rayet star
See also:
- APOD: 2025 February 3 Á Wolf Rayet Star 124: Stellar Wind Machine
- APOD: 2025 January 29 Á Dust Shells around WR 140 from Webb
- Sharpless 308: The Dolphin Head Nebula
- APOD: 2024 January 9 Á Thors Helmet
- APOD: 2023 March 29 Á Sh2-308: A Dolphin Shaped Star Bubble
- Wolf Rayet 124
- APOD: 2023 February 8 Á Stellar Wind Shaped Nebula RCW 58