The findings are an important contribution to the overall understanding of what goes on inside trillions of stars across the cosmos.
Institute for Astronomy Assistant Professor Daniel Huber and School of Ocean and Earth Science and Technology Professor Eric Gaidos co-authored the study recently published in the science journal Nature.
“The signals from these stars have been a mystery for over a hundred years. We knew that brightness variations in these stars are caused by sound waves traveling in their interior, but we just couldn’t make any sense of them,” Huber said.
The international team led by Professor Tim Bedding at the University of Sydney used data from NASA’s Transiting Exoplanet Survey Satellite (TESS), a space telescope used to detect planets around nearby stars. It provided the team with brightness measurements of thousands of stars, allowing them to find 60 whose pulsations made sense.
“NASA’s TESS data has delivered precise detections in a much larger number of these stars than we had before. This has now finally cleared up the picture, and we were able to identify regular structures. It’s like notes of a song finally falling into place to play a beautiful melody,” Huber explained.
The stars analyzed in the study are about 1.5 to 2.5 times more massive than the Sun and are known as Delta Scuti stars. Within the past few decades, astronomers have been able to detect the internal oscillations of stars, revealing their structure by studying stellar pulsations using careful and precise measurements of changes in light output.
Over periods of time, brightness variations reveal intricate — and often regular- patterns, allowing researchers to stare into the very heart of the massive nuclear furnaces that light the universe.
This branch of science, known as asteroseismology, enables astronomers to understand the insides of distant stars similar to how earthquakes are used to decipher the interior structure of our planet.
The research team’s identification of regular patterns in Delta Scuti stars will dramatically expand the reach of asteroseismology.
“Young stars like these are among the most intriguing and important objects in astronomy. They allow us to see how stars and their planets form and change with time much as the solar system did more than 4 billion years ago. They are a window into our past,” said Huber.
Observations from the W. M. Keck Observatory on Maunakea provided critical information during the study to explain the brightness variations of the stars recorded by TESS.
“Our observations with Keck showed that most Delta Scuti stars with regular patterns appear to be spinning slower than normal,” Huber said. “We believe that this is one of the key pieces to explain their clear frequency patterns, and this will be critical to find more of them in the future.”