An international team of astronomers from Australia, the United States and Europe has for the first-time unlocked the interior structure of Beta Crucis - a bright blue giant star that features on the flags of Australia, Brazil, New Zealand, Papua New Guinea and Samoa.

With an entirely new approach, the team led by Dr Daniel Cotton, found the star to be 14.5 times as massive as the Sun and as young as 11 million years old, making it the heaviest star with an age determined from asteroseismology ever.

The findings will provide new detail on how stars live and die, and how they impact the Galaxy's chemical evolution.

To crack the star's age and mass, the research team combined asteroseismology, the study of a star's regular movements, with polarimetry, the measurement of the orientation of light waves.

Asteroseismology relies on seismic waves bouncing around the interior of a star and producing measurable changes in its light. Probing the interiors of heavy stars that will later explode as supernovae has traditionally been difficult.

"I wanted to investigate an old idea," lead author Dr Cotton, from The Australian National University (ANU), and Monterey Institute for Research in Astronomy in the USA, said.

"It was predicted in 1979 that polarimetry had the potential to measure the interiors of massive stars, but it's not been possible until now."

Study co-author Professor Jeremy Bailey from the University of New South Wales (UNSW) said: "The size of the effect is quite small. We needed the world's best precision of the polarimeter we designed and built at UNSW for the project to succeed."

The study of Beta Crucis, also known as Mimosa, combines three different types of measurements of its light: space-based measurements of light intensity from NASA's WIRE and TESS satellites, 13 years of ground-based high-resolution spectroscopy from the European Southern Observatory, and ground-based polarimetry gathered from Siding Spring Observatory and Western Sydney University's Penrith Observatory.

"It was a lucky circumstance that we could use the world's most precise astronomical polarimeter to make so many observations of Mimosa at the Anglo-Australian Telescope while TESS was also observing the star," second author Professor Derek Buzasi from Florida Gulf Coast University said.

"Analysing the three types of long-term data together allowed us to identify Mimosa's dominant mode geometries. This opened the road to weighing and age-dating the star using seismic methods."

Professor Conny Aerts of KU Leuven said: "This polarimetric study of Mimosa opens a new avenue for asteroseismology of bright massive stars. While these stars are the most productive chemical factories of our galaxy, they are so far the least analysed asteroseismically, given the degree of difficulty of such studies. The heroic efforts by the Australian;polarimetrists are to be admired."

Research Report: "The dawn of polarimetric asteroseismology and its application to blue giant star ss Crucis"

Related Links
Australian National University,
Stellar Chemistry, The Universe And All Within It

Thanks for being there; We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain. With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords. Our news coverage takes time and effort to publish 365 days a year. If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Monthly Supporter $5+ Billed Monthly		SpaceDaily Contributor $5 Billed Once credit card or paypal

Unique look at the self-destruction of a star is presented in 3D
Stockholm, Sweden (SPX) Dec 08, 2021
The new study authored by Josefin Larsson, an astrophysicist at KTH Royal Institute of Technology in Stockholm, in collaboration with researchers at Stockholm University, the University of Warwick and at ESO, was published in the Astrophysical Journal. The supernova that the researchers studied, known as SNR 0540-69.3, is a familiar subject. For those observing the remnants of exploded stars, it's one of the sky's go-to supernovae, thanks to its relative proximity in the Large Magellanic Cloud, a ... read more

Read more from original source...