Back انفجار أشعة غاما 970508 Arabic GRB 970508 AST GRB 970508 Azerbaijani GRB 970508 Catalan GRB 970508 Spanish جیآربی ۹۷۰۵۰۸ Persian GRB 970508 French GRB 970508 ID GRB 970508 Japanese GRB 970508 Polish
 Image of the optical afterglow of GRB 970508 taken one month after the burst was detected | |
| Event type | Gamma-ray burst |
|---|---|
| Date | c. 7.4 billion years ago (detected 8 May 1997, 21:42 UTC) |
| Instrument | BeppoSAX |
| Constellation | Camelopardalis |
| Right ascension | 06h 53m 49s[1] |
| Declination | +79° 16′ 19.6″[1] |
| Distance | c. 6 billion ly |
| Redshift | 0.835 ≤ z ≤ 2.3 |
| Peak apparent magnitude | 19.6 |
| Total energy output | 5 × 1050 erg (5 × 1043 J) |
| Other designations | GRB 970508 |
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GRB 970508 was a gamma-ray burst (GRB) detected on May 8, 1997, at 21:42 UTC; it is historically important as the second GRB (after GRB 970228) with a detected afterglow at other wavelengths, the first to have a direct redshift measurement of the afterglow, and the first to be detected at radio wavelengths.
A gamma-ray burst is a highly luminous flash associated with an explosion in a distant galaxy and producing gamma rays, the most energetic form of electromagnetic radiation, and often followed by a longer-lived "afterglow" emitted at longer wavelengths (X-ray, ultraviolet, optical, infrared, and radio).
GRB 970508 was detected by the Gamma Ray Burst Monitor on the Italian–Dutch X-ray astronomy satellite BeppoSAX. Astronomer Mark Metzger determined that GRB 970508 occurred at least 6 billion light years from Earth; this was the first measurement of the distance to a gamma-ray burst.
Until this burst, astronomers had not reached a consensus regarding how far away GRBs occur from Earth. Some supported the idea that GRBs occur within the Milky Way, but are visibly faint because they are not highly energetic. Others concluded that GRBs occur in other galaxies at cosmological distances and are extremely energetic. Although the possibility of multiple types of GRBs meant that the two theories were not mutually exclusive, the distance measurement unequivocally placed the source of the GRB outside the Milky Way, effectively ending the debate.
GRB 970508 was also the first burst with an observed radio frequency afterglow. By analyzing the fluctuating strength of the radio signals, astronomer Dale Frail calculated that the source of the radio waves had expanded almost at the speed of light. This provided strong evidence that GRBs are relativistically expanding explosions.