Astronomers have for the first time have captured the early death throes of supernovae and found the initial stages of the explosion don’t quite fit with existing theories.
The scientists used the Kepler space telescope to photograph three type 1a supernovae in the earliest stages of ignition.
They then tracked the explosions in detail to full brightness around three weeks later and the subsequent decline over the next few months.
“The stars all blow up uniquely. It doesn’t make sense,” says Dr Brad Tucker from the Australian National University (ANU).
“It’s particularly weird for these supernovae because even though their initial shock waves are very different, they end up doing the same thing.”
Before this study, the earliest type 1a supernovae had been glimpsed was more than 2.5 hours after ignition, after which the explosions all followed an identical pattern.
This led astronomers to theorise that supernovae, the brilliant explosions of dying stars, all occurred through an identical process.
Astronomers had thought supernovae all happened when a dense star steadily sucked in material from a large nearby neighbour until it became so dense that carbon in the star’s core ignited.
“Somewhat to our surprise the results suggest an alternative hypothesis, that a violent collision between two smallish white dwarf stars sets off the explosion,” says lead researcher Dr Robert Olling, from the University of Maryland in the United States.
At the peak of their brightness, supernovae are brighter than the billions of stars in their galaxy. Because of their brightness, astronomers have been able to use them to calculate distances to distant galaxies.
Measurements of distant supernovae led to the discovery that some unknown force, now called dark energy, is causing the accelerated expansion of the universe.
Brian Schmidt from the ANU, Saul Perlmutter (Berkeley) and Adam Reiss (Johns Hopkins) were awarded the Nobel prize in 2011 for this discovery.
The latest findings are published in the journal Nature.
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