Dating of Milky Way stars ‘sharpens view on early years of galaxy’
Researchers surveyed around 100 red giant stars, and found some of these were originally part of a satellite galaxy called Gaia-Enceladus.
Some of the oldest stars in our galaxy have been dated with unprecedented precision, scientists say.
Researchers surveyed around 100 red giant stars, and determined that some of these were originally part of a satellite galaxy called Gaia-Enceladus, which collided with the Milky Way early in its history.
The study revealed that the group of stars observed all have similar ages, or are slightly younger than the majority of the stars known to have started their lives within the Milky Way.
Researchers, led by the University of Birmingham, say this corroborates existing theories suggesting the Milky Way had already started forming a significant fraction of its stars when the merger with the Gaia-Enceladus (also known as the Gaia Sausage) occurred.
By the time of the collision, the Milky Way was already efficiently forming stars, most of which now reside within its thick disc, one of two disc-like structures that make up the galaxy.
Josefina Montalban, lead author of the paper, said: “The chemical composition, location and motion of the stars we can observe today in the Milky Way contain precious information about their origin.
“As we increase our knowledge of how and when these stars were formed, we can start to better understand how the merger of Gaia-Enceladus with the Milky Way affected the evolution of our galaxy.”
In making the calculations, the team used asteroseismology data from the Kepler satellite in combination with data from the Gaia and Apogee instruments.
All three are set up to gather data to help scientists map and characterise stars in the Milky Way.
Asteroseismology is a relatively new technique which involves measuring the oscillations caused by sound waves trapped inside the star.
This enables scientists to assemble information about the star’s size and internal structure, which allows accurate estimations of the star’s age to be made.
In the study published in Nature Astronomy, the team used information on the individual oscillation modes of each star, rather than averaged properties of their pulsations.
Researchers were able to use the technique in combination with spectroscopy – which enables the chemical composition of the stars to be measured.
Co-author Professor Andrea Miglio, from the University of Bologna, said: “We have shown the huge potential of asteroseismology in combination with spectroscopy to deliver precise, accurate relative ages for individual, very old, stars.
“Taken together, these measurements contribute to sharpen our view on the early years of our galaxy and promise a bright future for galactic archeoastronomy.
