Almost a decade ago, on February 23, 1987, astronomers noticed that a star 167,000 light-years from Earth in the Large Magellanic Cloud had blown apart. This blazing act of self-destruction released an amount of energy equivalent to that of 100 suns over their lifetime. Ever since, scientists have watched the fading aftermath of supernova 1987A--and the second act of the show is now beginning: An immense shockwave from the explosion is smashing into a mysterious ring of gas that surrounds the dead star, causing it to light up once again.
Supernova 1987A was the brightest stellar cataclysm seen since Johannes Kepler recorded his observations of a supernova in the year 1604. At its brightest, Supernova 1987A glowed as intensely as the stars in the Big Dipper constellation. And it is the first supernova observed clearly over a long period with modern instruments. "This is the first time we have been able to observe these events in the span of a human lifetime," says Ann Kinney of the Space Telescope Science Institute, which manages the orbiting Hubble Space Telescope for the National Aeronautics and Space Administration.
Indeed, observing the supernova is like watching a nuclear bomb detonate in extreme slow motion. Because of its vast scale, events that would take a fraction of a second in an explosion on Earth are played out over decades in space. The most recent Hubble observations show that the physical shockwave from the giant blast is just now reaching the innermost of three mysterious gas rings circling the dead star at a distance of two-thirds of a light year.
Jolted by the 40-million mile per hour sledgehammer blow, one knot of gas--100 billion miles in diameter in a piece of the ring--has already begun to glow brightly, as its temperature surges from a few thousand degrees to a million degrees Fahrenheit. Astronomers predict it's only a matter of years before the complete ring becomes ablaze with light as it absorbs the full force of the impact. "Ten years from now, the entire ring will be hundreds of times brighter than today," says Robert Kirshner of the Harvard-Smithsonian Center for Astrophysics, which made the recent images of the supernova ring.
Astronomers do not think that this inner ring is simply debris from the explosion. Rather, they believe that it likely formed about 20,000 years before the star exploded. But it only became visible when it was heated by the burst of x-ray and light energy from the explosion; since then, it has been slowly fading as the gas cools. "This material used to be part of the star--its not shrapnel, its surface stuff that puffed off before the star exploded," says Kirshner.
Image: HUBBLE SPACE TELESCOPE
The outer two rings are even more puzzling. Hubble images recorded in 1994 revealed that the exploding star had assumed a shape resembling two wine glasses placed base to base. The supernova is located where the stems of the two glasses would intersect. The inner ring of gas is dispersed around the edges of the bases. Then, there are two more, fainter. rings of gas that would be on the edges of the flutes of the glasses.
Because the outer rings appear to be mirror images, astronomers speculate that they were "painted" on the expanding envelope of gas by twin jets of high-energy. A rapidly rotating but unseen companion star--one that collapsed as a neutron star or black hole at the time of the supernova--could have produced these jets. Material falling from the exploded star onto the compact companion would have been heated and blasted back into space in two narrow jets, along with a beam of radiation.