The Early Flash of an Exploding Star

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The brilliant flash of an exploding star’s shockwave—what astronomers call the “shock breakout”—has been captured for the first time in the optical wavelength or visible light by NASA’s planet-hunter, the Kepler space telescope.

An international science team led by Peter Garnavich, an astrophysics professor at the University of Notre Dame in Indiana, analyzed light captured by Kepler every 30 minutes over a three-year period from 500 distant galaxies, searching some 50 trillion stars.

They were hunting for signs of massive stellar death explosions known as supernovae.

In 2011, two of these massive stars, called red supergiants, exploded while in Kepler’s view.

The first behemoth, KSN 2011a, is nearly 300 times the size of our sun and a mere 700 million light years from Earth. The second, KSN 2011d, is roughly 500 times the size of our sun and around 1.2 billion light years away.

To put their size into perspective, Earth’s orbit about our sun would fit comfortably within these colossal stars, said Garnavich.

Whether it’s a plane crash, car wreck or supernova, capturing images of sudden, catastrophic events is extremely difficult but tremendously helpful in understanding root cause.

Just as widespread deployment of mobile cameras has made forensic videos more common, the steady gaze of Kepler allowed astronomers to see, at last, a supernova shockwave as it reached the surface of a star.

The shock breakout itself lasts only about 20 minutes, so catching the flash of energy is an investigative milestone for astronomers.

In order to see something that happens on timescales of minutes, like a shock breakout, you want to have a camera continuously monitoring the sky, said Garnavich.

You don’t know when a supernova is going to go off, and Kepler’s vigilance allowed us to be a witness as the explosion began.

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