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| Event type | Gamma-ray burst |
|---|---|
| Constellation | Orion |
| Redshift | 1.02 |
| Other designations | GRB 991216 |
| | |
GRB 991216, nicknamed theBeethoven Burst by Dr. Brad Schaefer ofYale University, was agamma-ray burst observed on December 16, 1999,[1] coinciding with the 229th anniversary ofLudwig van Beethoven's birth.[2] A gamma-ray burst is a highlyluminous flash associated with an explosion in a distant galaxy and producinggamma rays, the most energetic form ofelectromagnetic radiation, and often followed by a longer-lived "afterglow" emitted at longer wavelengths (X-ray,ultraviolet,optical,infrared, andradio).
The optical afterglow of the burst reached anapparent magnitude of 18.7, making the Beethoven Burst one of the brightest bursts ever detected, even though it occurred about 10 billionlight years from Earth.[1] Frank Marshall, aNASA astrophysicist at theGoddard Space Flight Center, commented that "this was by far the brightest burst we have detected in a long time."[3] The burst's peakflux ranked it as the second most powerful burst that theBurst and Transient Source Experiment (BATSE) had ever detected.[4] The analysis of the observations strengthened the theory that gamma-ray bursts are a result of ahypernova,[5] though other possibleprogenitors exist, such as the merger of twoblack holes.
Within four hours of the burst's detection, observations made by BATSE and theRossi X-ray Timing Explorer were able to determine the burst's position ofα = 77.38 ± 0.04,δ = 11.30 ± 0.05.[6] This rapid determination allowed astronomers to conduct follow-up studies using optical and X-ray telescopes. Other instruments which detected GRB 991216 included theChandra X-ray Observatory, theMDM Observatory,[7] and theSpace Telescope Imaging Spectrograph on board theHubble Space Telescope.[8] This was the first use of theChandra X-ray Observatory for the purpose of gamma-ray burst detection.[7]