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What happens when a massive star dies? Nobody knows, because nobody has really observed a supernova in the act. Until now. And they’ve caught it on film.

Susan Lentz, a professor of astronomy at Columbia, has been watching exploding stars since she got her doctorate in 1987. One day, while on a routine monitoring project, she was surprised to see a new supernova on a CCD camera. And it was spectacular.

“It exploded like a full-body atomic bomb, not just with light, but also with high-energy particles,” she says. “The light from the explosion was 10 times brighter than a normal supernova. It looked like an old-style light bulb burning out.”

Teams of astronomers around the world are now trying to unravel the secrets of supernova progenitors, which is to say what types of stars are most likely to go bang. This year’s discovery, by Leon Van Dyk, a graduate student at Harvard, confirms a theory he and Ms. Lentz had been promoting.

Scientists have known for years that at least a few stars more massive than the Sun explode: a dozen or so supernovae have been seen in recent years. But that is the tip of the iceberg. The more events we observe, the more we find that supernovae come in many shapes and sizes. This new trend points toward more kinds of progenitors: it suggests that some supernova explosions are due to exploding stars that form from intermediate-mass stars, like our Sun.

If that is true, there is a message for future astronomers and cosmologists. Supernovae could hold the key to many mysteries of the Universe, including those about the first generation of stars. The more we find out, the more we will learn.

A version of this letter appears in print on January 30, 1998, on Page 2002026 of the National edition with the headline: A BIG BANG. Today’s Paper|SubscribeQ:

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