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Giant star goes supernova and is smothered by its own dust

The supernova released more energy than our Sun could produce in its entire lifetime.
Provided by Ohio State University, Columbus
dusty-supernova
While searching the skies for black holes using the Spitzer Space Telescope Deep Wide Field Survey, Ohio State University astronomers discovered a giant supernova that was smothered in its own dust. In this artist’s rendering, an outer shell of gas and dust — which erupted from the star hundreds of years ago — obscures the supernova within. This event in a distant galaxy hints at one possible future for the brightest star system in our own Milky Way.

A giant star in a faraway galaxy recently ended its life with a dust-shrouded whimper instead of the more typical bang.

Ohio State University researchers suspect that this odd event — the first one of its kind viewed by astronomers — was more common early in the universe. It also hints at what we would see if the brightest star system in our galaxy became a supernova.

Christopher Kochanek from Ohio State University and his colleagues describe how the supernova appeared in late August 2007 as part of the Spitzer Space Telescope Deep Wide Field Survey.

The astronomers were searching the survey data for active galactic nuclei (AGN) — supermassive black holes at the centers of galaxies. AGN radiate enormous amounts of heat as material is sucked into the black hole. In particular, the astronomers were searching for hot spots that varied in temperature because these could provide evidence of changes in how the material was falling into the black hole.

Normally, astronomers wouldn't expect to find a supernova this way, said Szymon Kozlowski from Ohio State. Supernovae release most of their energy as light, not heat.

But one hot spot, which appeared in a galaxy some 3 billion light-years from Earth, didn't match the typical heat signal of an AGN. The visible spectrum of light emanating from the galaxy didn't show the presence of an AGN either.

Enormous heat flared from the object for a little over 6 months, then faded away in early March 2008 — another clue that the object was a supernova. "Over 6 months, it released more energy than our Sun could produce in its entire lifetime," Kozlowski said.

The astronomers knew that if the source were a supernova, the extreme amount of energy it emitted would qualify it as a big one, or a "hypernova." The temperature of the object was around 1,300° Fahrenheit (700° Celsius) — only a little hotter than the surface of the planet Venus. They wondered what could absorb that much light energy and dissipate it as heat?

The answer: Dust, and a lot of it.

Using what they learned from the Spitzer survey, the astronomers worked backward to determine what kind of star could have spawned the supernova, and how the dust was able to partly muffle the explosion. They calculated that the star was probably a giant, at least 50 times more massive than our Sun. Such massive stars typically belch clouds of dust as they near the end of their existence.

This particular star must have had at least two such ejections, they determined — one about 300 years before the supernova, and one only about 4 years before it. The dust and gas from both ejections remained around the star, each in a slowly expanding shell. The inner shell from 4 years ago would be close to the star, while the outer shell from 300 years ago would be farther away.

"We think the outer shell must be nearly opaque, so it absorbed any light energy that made it through the inner shell and converted it to heat," said Kochanek. That's why the supernova showed up on the Spitzer survey as a hot dust cloud.

Krzysztof Stanek from Ohio State said that stars probably choked on their own dust more often in the distant past.

"These events are much more likely to happen in a small, low-metallicity galaxy," Stanek said — meaning a young galaxy that hadn't been around long enough for its stars to fuse hydrogen and helium into the more complex chemicals that astronomers refer to as metals.

Still, Kozlowski added, NASA's Wide-field Infrared Explorer (WISE) will likely find more such supernovae. "I would expect WISE to see 100 of these events in 2 years, now that we know what to look for," he said.

Because of the alignment of the galaxy with Earth and our Sun, astronomers were not able to see what the event looked like to the naked eye while it was happening. But Kochanek believes that we might see the star brighten a decade or so from now. That's how long it will take for the shock wave from the exploding star to reach the inner dust shell and slam it into the outer shell. Then we'll have something to see here on Earth.

We do have at least one chance to see a similar light show closer to home, though. "If Eta Carinae went supernova right now, this is what it would probably look like," Kochanek said, referring to the brightest star system in our Milky Way Galaxy.

The two stars that make up Eta Carinae are 7,500 light-years away, and they host a distinctive dust shell dubbed the Homunculus Nebula. Astronomers believe that the nebula was created when the larger of the two stars underwent a massive eruption around 1840, and that future eruptions are likely.

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