GRB 990510 Sky Region
The object of study is the remnant of a mysterious cosmic explosion far out in space, first detected as a gigantic outburst of gamma rays on May 10. Gamma-Ray Bursters (GRBs) are brief flashes of very energetic radiation — they represent by far the most powerful type of explosion known in the Universe and their afterglow in optical light can be 10 million times brighter than the brightest supernovae. The May 10 event ranks among the brightest one hundred of the over 2500 GRB''s detected in the last decade. To the left is a reproduction of a short (30 sec) centering exposure in the V-band (green-yellow light), obtained with VLT ANTU and the multi-mode FORS1 instrument on May 11, 1999, at 03:48 UT under mediocre observing conditions (image quality 1.0 arcsec).The optical image of the afterglow of GRB 990510 is easily seen in the box, by comparison with an exposure of the same sky field before the explosion, made with the ESO Schmidt Telescope in 1986 (right).The exposure time was 120 min on IIIa-F emulsion behind a R(ed) filter. The field shown measures about 6.2 x 6.2 arcmin 2. North is up and East is left.
About the Image
|Release date:||18 May 1999|
|Size:||2732 x 1332 px|
About the Object
|Type:||• Early Universe : Cosmology : Phenomenon : Gamma Ray Burst|
• X - Stars
Colours & filters
|Very Large Telescope|
|ESO 1-metre Schmidt telescope|
Notes: Right image obtained by the 1-metre Schmidt telescope, the left was taken using the VLT.