Star-quake vibrations lead to new estimate for Milky Way age

Data gathered by NASA’s now defunct Kepler telescope provides a solution to an astronomical mystery.

An artist impression of the Milky Way, showing the thick and thin discs.
Credit: NASA/JPL Caltech/R.Hurt/SSC

Star-quakes recorded by NASA’s Kepler space telescope have helped answer a long-standing question about the age of the “thick disc” of the Milky Way.

In a paper published in the journal Monthly Notices of the Royal Astronomical Society, a team of 38 scientists led by researchers from Australia’s ARC Centre of Excellence for All Sky Astrophysics in Three Dimensions (ASTRO-3D) use data from the now-defunct probe to calculate that the disc is about 10 billion years old.

“This finding clears up a mystery,” says lead author Dr Sanjib Sharma from ASTRO 3D and Australia’s University of Sydney.

“Earlier data about the age distribution of stars in the disc didn’t agree with the models constructed to describe it, but no one knew where the error lay – in the data or the models. Now we’re pretty sure we’ve found it.”

The Milky Way-like many other spiral galaxies – consists of two disc-like structures, known as thick and thin. The thick disc contains only about 20 per cent of the Galaxy’s total stars, and, based on its vertical puffiness and composition, is thought to be the older of the pair.

To find out just how much older, Dr Sharma and colleagues used a method known as asteroseismology – a way of identifying the internal structures of stars by measuring their oscillations from starquakes.

“The quakes generate soundwaves inside the stars that make them ring, or vibrate,” explains co-author Associate Professor Dennis Stello from ASTRO-3D and the University of New South Wales.

“The frequencies produced tell us things about the stars’ internal properties, including their age. It’s a bit like identifying a violin as a Stradivarius by listening to the sound it makes.”

This age-dating allows researchers to essentially look back in time and discern the period in the Universe’s history when the Milky Way formed; a practice known as Galactic-archaeology.

Not that the researchers actually hear the sound generated by star-quakes. Instead, they look for how the internal movement is reflected in changes to brightness.

“Stars are just spherical instruments full of gas,” says Sharma, “but their vibrations are tiny, so we have to look very carefully.

“The exquisite brightness measurements made by Kepler were ideal for that. The telescope was so sensitive it would have been able to detect the dimming of a car headlight as a flea walked across it.”

The data delivered by the telescope during the four years after it was launched in 2009 presented a problem for astronomers. The information suggested there were more younger stars in the thick disc than models predicted.

The question confronting scientists was stark: were the models wrong, or was the data incomplete?

In 2013, however, Kepler broke down, and NASA reprogrammed it to continue working on a reduced capacity – a period that became known as the K2 mission. The project involved observing many different parts of the sky for 80 days at a time.

The first tranche of this data represented a rich new source for Dr Sharma and colleagues from Macquarie University, Australian National University, University of New South Wales and the University of Western Australia. They were joined in their analysis by others from institutions in the US, Germany, Austria, Italy, Denmark, Slovenia and Sweden.

A fresh spectroscopic analysis revealed that the chemical composition incorporated in the existing models for stars in the thick disc was wrong, which affected the prediction of their ages.  Taking this into account, the researchers found that the observed asteroseismic data now fell into “excellent agreement” with model predictions.

The results provide a strong indirect verification of the analytical power of asteroseismology to estimate ages, says Professor Stello.

He added that additional data still to be analysed from K2, combined with new information gathered by NASA’s Transiting Exoplanet Survey Satellite (TESS), will result in accurate estimates for the ages of even more stars within the disc and this will help us to unravel the formation history of the Milky Way.

A pre-print version of the paper is available here: https://arxiv.org/abs/1904.12444

The Monthly Notices of the Royal Astronomical Society abstract is here: https://academic.oup.com/mnras/article-abstract/490/4/5335/5586605?redirectedFrom=fulltext

More information:

Andrew Masterson: andrew@scienceinpublic.com.au

Sanjib Sharma is available for interview: +61 434 191 346

Dennis Stello is available for interview: +61 424 234 550

More about ASTRO-3D

ASTRO 3D is a seven-year $40 million Centre of Excellence project funded by the Australian Government through the Australian Research Council. The Centre began in June 2017 and will end in June 2024. It hosts around 200 investigators and professional staff, mostly based at six nodes: the Australian National University, Curtin University, Swinburne University of Technology, University of Melbourne, University of Sydney, and University of Western Australia. https://astro3d.org.au/

The K2-HERMES Survey: Age and Metallicity of the Thick Disc

Sanjib Sharma,1,2 Dennis Stello,3,1,4,2 Joss Bland-Hawthorn,1,2 Michael R. Hayden,1,2 Joel C. Zinn,5 Thomas Kallinger,Marc Hon,3 Martin Asplund,7,2 Sven Buder,8,9 Gayandhi M. De Silva,10 Valentina D’orazi,11 Ken Freeman,7 Janez Kos,12 Geraint F. Lewis,1 Jane Lin,7 Karin Lind,8,13 Sarah Martell,3 Jeffrey D. Simpson,3 Rob A. Wittenmyer,14 Daniel B. Zucker,10,15 Tomaz Zwitter,12 Timothy R. Bedding,1 Boquan Chen,1 Klemen Cotar,12 James Esdaile,3 Jonathan Horner,14 Daniel Huber,16,17,18 Prajwal R. Kafle,19 Shourya Khanna,1 Tanda Li,1 Yuan-Sen Ting,20,21 David M. Nataf,22 Thomas Nordlander,7,2 Hafiz Saddon,3 Gregor Traven,12 Duncan Wright,14 and Rosemary F. G. Wyse,23

  1. Sydney Institute for Astronomy, School of Physics, The University of Sydney, NSW 2006, Australia
  2. ARC Centre of Excellence for All Sky Astrophysics in Three Dimensions (ASTRO-3D)
  3. School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
  4. Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark
  5. Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA
  6. Institute of Astrophysics, University of Vienna, TÃijrkenschanzstrasse 17, Vienna 1180, Austria
  7. Research School of Astronomy & Astrophysics, Australian National University, ACT 2611, Australia
  8. Max Planck Institute for Astronomy (MPIA), Koenigstuhl 17, D-69117 Heidelberg
  9. Fellow of the International Max Planck Research School for Astronomy & Cosmic Physics at the University of Heidelberg
  10. Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia
  11. INAF -Osservatorio Astronomico di Padova
  12. Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana, Slovenia
  13. Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
  14. Centre for Astrophysics, University of Southern Queensland, Toowoomba, Queensland 4350, Australia
  15. Research Centre in Astronomy, Astrophysics & Astrophotonics, Macquarie University, Sydney, NSW 2109, Australia
  16. Institute for Astronomy, University of Hawai‘i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
  17. SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA
  18. Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
  19. International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
  20. Institute for Advanced Study, Princeton, NJ 08540, USA
  21. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA
  22. Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA
  23. Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, US