A supernova is a powerful and luminous stellar explosion. This transient astronomical event occurs during the last evolutionary stages of a massive star or when a white dwarf is triggered into runaway nuclear fusion. The explosion marks the ultimate demise of the star and briefly outshines an entire galaxy, radiating as much energy as the Sun is expected to emit over its entire lifespan.
The details of a supernova explosion are still clouded in mystery and subject to vigorous debate. What exactly happens when they explode? What underlying mechanisms are involved? New observations of a supernova with the European Southern Observatory's Very Large Telescope are removing some of the mystery.

