- A gamma-ray burst (GRB) is defined as:
A short, extremely high energy burst of gamma radiation emitted by a collapsing supergiant star
Gamma ray burst
Gamma ray burst from a collapsing star
- These bright gamma sources can produce, in a very short period of time, as much energy as the total energy output of the Sun over its 10 billion-year lifespan
- They typically emit energies in the region of 1044 to 1047 J
- This energy is usually highly focused, or collimated, as narrow beams which are ejected from the poles of the exploding star
- Because of this, some astronomers have concerns that the evolution of a supergiant star in the local part of our galaxy could pose a danger to life on Earth
- However, so far, gamma-ray bursts have only ever been detected at great distances, and never in the Milky Way