Scenes from a Supernova

Weizmann Institute scientists examined a particular type of exploding star supernova and gained new insights into why these stars end their lives in an explosion. A new supernova was observed with both Earth- and satellite-based X-ray and radio-wave telescopes. Researchers studied the material thrown off in the blast and analyzed the stages of the explosion. They showed that the exploding star was a white dwarf – an extremely compact star whose diameter is much smaller than that of our sun – which siphons off material from a companion star until it exceeds its stable weight limit, causing an explosion. The scientists set an upper limit on the size of a possible companion, showing it could not have been a particularly large star – excluding, for instance, a red giant scenario.

