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Starquakes Reveal Pulse of Giant Stars

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Sizes of red giant stars compared to the Sun. Using the Kepler telescope, we have detected oscillations in hundreds of red giant stars. The periods of those oscillations allowed us to study the interiors of these giant stars, which represent the future li
Sizes of red giant stars compared to the Sun. Using the Kepler telescope, we have detected oscillations in hundreds of red giant stars. The periods of those oscillations allowed us to study the interiors of these giant stars, which represent the future life of our Sun. (Image credit: Daniel Huber, University of Sydney)

Astronomers have taken the pulse of red giant stars by measuring their starquakes — stellar shivers that run so deep they can reach a star's core, scientists say.

These new findings can help scientists separate the vastly different types of red giants that would otherwise look virtually identical, which could help shed light on the future of our sun and the history of the galaxy.

Red giants are the swollen fate that awaits stars such as our own sun as they begin to exhaust their primary source of fuel, the hydrogen near their cores. The byproduct of the nuclear fusion that powers the sun — helium — accumulates over time, forcing hydrogen into a shell around the core that burns more vigorously than before.

Approximately 5 billion years from now, this will force our sun to swell to more than 100 times its current size, turning it into a red giant. [Video: How the Sun Will Die]

Stages in the evolution of a star like the sun. The sun is currently fusing hydrogen into helium in its core (lower left). In later stages, when it becomes a red giant, the star will fuse hydrogen in a shell around the helium core (2nd and 3rd figures). Finally, the red giant will begin to fuse helium into carbon in its core (4th figure). (Image credit: Thomas Kallinger, University of British Columbia and University of Vienna)

After red giants age, they should, in principle, start burning the helium in their cores as well. However, although theoretical calculations predicted that this profound transformation should occur, scientists had never actually witnessed it, since the change would be largely invisible from the outside.

Now, by analyzing "starquakes," researchers have uncovered secret differences lurking in the hearts of these red giants.

"In the same way that geologists use earthquakes to explore Earth's interior, we use starquakes to explore the internal structure of stars," said researcher Timothy Bedding, an astronomer at the University of Sydney in Australia.

Stars are turbulent, experiencing violent starquakes that generate sound waves, which zip through the stars and back to their surfaces. The way these sound waves interact with other waves fluctuating on a star can alter its brightness regularly, changes that scientists can observe and which are sensitive to the structure of the cores of the stars — an emerging scientific field known as astroseismology. [Top 10 Star Mysteries]

Using the Kepler spacecraft, researchers observed about 400 red giants over the course of nearly a year.

They discovered that hydrogen-burning stars demonstrated a range of sequences of a kind of gravity-linked vibration that differed from each other in the time they took to complete by up to 50 seconds, while helium-burning ones showed differences of about 100 to 300 seconds. The cores of these latter stars are much hotter and less dense, Bedding explained, meaning that sound travels more slowly through them.

"We were hoping to see a difference in their oscillation properties, but I did not expect it to be so clear-cut," Bedding told SPACE.com.

Now the researchers will scan red giants en masse to see what stages of evolution they have reached, "trying to work out details of the history of the Milky Way," Bedding said.

The scientists detailed their findings in the March 31 issue of the journal Nature.

Follow SPACE.com contributor Charles Q. Choi on Twitter @cqchoi. Visit SPACE.com for the latest in space science and exploration news on Twitter @Spacedotcom and on Facebook.

This story was provided by SPACE.com, a sister site to LiveScience.

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Charles Q. Choi
Charles Q. Choi
Live Science Contributor
Charles Q. Choi is a contributing writer for Live Science and Space.com. He covers all things human origins and astronomy as well as physics, animals and general science topics. Charles has a Master of Arts degree from the University of Missouri-Columbia, School of Journalism and a Bachelor of Arts degree from the University of South Florida. Charles has visited every continent on Earth, drinking rancid yak butter tea in Lhasa, snorkeling with sea lions in the Galapagos and even climbing an iceberg in Antarctica.