During the lifetime of our Milky Way galaxy, there have been something like
100 million supernova explosions, which have enriched the Galaxy with the
oxygen we breathe, the iron in our cars, the calcium in our bones and the s
ilicon in the rocks beneath our feet. These exploding stars also influence
the birth of new stars and are the source of the energetic cosmic rays that
irradiate us on the Earth. The prodigious amount of energy (similar to 10(
51), Or similar to 2.5 x 10(28) megatonnes of TNT equivalent) and momentum
associated with each supernova may even have helped to shape galaxies as th
ey formed in the early Universe. Supernovae are now being used to measure t
he geometry of the Universe, and have recently been implicated in the decad
es-old mystery of the origin of the gamma-ray bursts. Together with major c
onceptual advances in our theoretical understanding of supernovae, these de
velopments have made supernovae the centre of attention in astrophysics.