For the First Time Astronomers Identify a Rhythm of Life in Pulsating Stars

High Frequency Pulsation Modes in Stars

Still image from animation showing a simulation of pulsations in the delta Scuti variable star called HD 31901, based on brightness measurements by NASA’s Transiting Exoplanet Survey Satellite (TESS). Credit: Produced by Dr. Chris Boshuizen with assistance from Dr. Simon Murphy and Prof. Tim Bedding

Through the noise, a class of stars reveals its inner workings; poor ‘social distancing’ identified using NASA space telescope.

By listening to the beating hearts of stars, astronomers have for the first time identified a rhythm of life for a class of stellar objects that had until now puzzled scientists.

Their findings are reported today (May 13, 2020) in the journal Nature.

“Previously we were finding too many jumbled up notes to understand these pulsating stars properly,” said lead author Professor Tim Bedding from the University of Sydney. “It was a mess, like listening to a cat walking on a piano.”

The international team used data from NASA’s Transiting Exoplanet Survey Satellite (TESS), a space telescope mainly used to detect planets around some of the nearest stars to Earth. It provided the team with brightness measurements of thousands of stars, allowing them to find 60 whose pulsations made sense.

“The incredibly precise data from NASA’s TESS mission have allowed us to cut through the noise. Now we can detect structure, more like listening to nice chords being played on the piano,” Professor Bedding said.

Professor Tim Bedding University of Sydney

This is lead author Professor Tim Bedding. Credit: University of Sydney

The findings are an important contribution to our overall understanding of what goes on inside the countless trillions of stars across the cosmos.

The intermediate-sized stars in question — about 1.5 to 2.5 times the mass of our Sun — are known as delta Scuti stars, named after a variable star in the constellation Scutum. When studying the pulsations of this class of stars, astronomers had previously detected many pulsations, but had been unable to determine any clear patterns.

The Australian-led team of astronomers has reported the detection of remarkably regular high-frequency pulsation modes in 60 delta Scuti stars, ranging from 60 to 1400 light-years away.

“This definitive identification of pulsation modes opens up a new way by which we can determine the masses, ages and internal structures of these stars,” Professor Bedding said.

Daniel Hey, a Ph.D. student at the University of Sydney and co-author on the paper, designed the software that allowed the team to process the TESS data.

“We needed to process all 92,000 light curves, which measure a star’s brightness over time. From here we had to cut through the noise, leaving us with the clear patterns of the 60 stars identified in the study,” he said.

“Using the open-source Python library, Lightkurve, we managed to process all of the light curve data on my university desktop computer in a just few days.”


The insides of stars were once a mystery to science. But in the past few decades, astronomers have been able to detect the internal oscillations of stars, revealing their structure. They do this by studying stellar pulsations using precise measurements of changes in light output.

Over periods of time, variations in the data reveal intricate — and often regular — patterns, allowing us to stare into the very heart of the massive nuclear furnaces that power the universe.

Isabel Colman Professor Tim Bedding

Co-author Isabel Colman (left), Ph.D. candidate, University of Sydney, with lead author Professor Tim Bedding. Credit: University of Sydney

This branch of science, known as asteroseismology, allows us to not only understand the workings of distant stars, but to fathom how our own Sun produces sunspots, flares, and deep structural movement. Applied to the Sun, it gives highly accurate information about its temperature, chemical make-up, and even the production of neutrinos, which could prove important in our hunt for dark matter.

“Asteroseismology is a powerful tool by which we can understand a broad range of stars,” Professor Bedding said. “This has been done with great success for many classes of pulsators including low-mass Sun-like stars, red giants, high-mass stars, and white dwarfs.

“The delta Scuti stars had perplexed us until now.”

Isabel Colman, a co-author and Ph.D. student at the University of Sydney, said: “I think it’s incredible that we can use techniques like this to look at the insides of stars.

“Some of the stars in our sample host planets, including beta Pictoris, just 60 light-years from Earth and which is visible to the naked eye from Australia. The more we know about stars, the more we learn about their potential effects on their planets.”

Poor ‘social distancing’

The identification of regular patterns in these intermediate-mass stars will expand the reach of asteroseismology to new frontiers, Professor Bedding said. For example, it will allow us to determine the ages of young moving groups, clusters, and stellar streams.

“Our results show that this class of stars is very young and some tend to hang around in loose associations. They haven’t got the idea of ‘social distancing’ rules yet,” Professor Bedding said.

Dr. George Ricker from the MIT Kavli Institute for Astrophysics and Space Research is Principal Investigator for NASA’s Transiting Exoplanet Sky Survey, from which the study took its data.

He said: “We are thrilled that TESS data is being used by astronomers throughout the world to deepen our knowledge of stellar processes. The findings in this exciting new paper led by Tim Bedding have opened up entirely new horizons for better understanding a whole class of stars.”

For more on this discovery:

Reference: “Very regular high-frequency pulsation modes in young intermediate-mass stars” by Timothy R. Bedding, Simon J. Murphy, Daniel R. Hey, Daniel Huber, Tanda Li, Barry Smalley, Dennis Stello, Timothy R. White, Warrick H. Ball, William J. Chaplin, Isabel L. Colman, Jim Fuller, Eric Gaidos, Daniel R. Harbeck, J. J. Hermes, Daniel L. Holdsworth, Gang Li, Yaguang Li, Andrew W. Mann, Daniel R. Reese, Sanjay Sekaran, Jie Yu, Victoria Antoci, Christoph Bergmann, Timothy M. Brown, Andrew W. Howard, Michael J. Ireland, Howard Isaacson, Jon M. Jenkins, Hans Kjeldsen, Curtis McCully, Markus Rabus, Adam D. Rains, George R. Ricker, Christopher G. Tinney and Roland K. Vanderspek, 13 May 2020, Nature.
DOI: 10.1038/s41586-020-2226-8

Funding bodies include the Australian Research Council, the US National Science Foundation, NASA, Lithuanian Science Council and the Danish National Research Foundation.

For full funding information please see the acknowledgements in the research paper in Nature.

The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the Indigenous Hawai’ian community; we are most fortunate to have the opportunity to conduct observations from this mountain. We also acknowledge the traditional owners of the land on which the Anglo-Australian Telescope stands, the Gamilaraay people, and pay our respects to elders past, present, and emerging.

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