Scientists have succeeded in dating some of the oldest stars in our galaxy with unprecedented precision by combining data from the stars’ oscillations with information about their chemical composition.
The team led by researchers at the University of Birmingham, surveyed around a hundred red giant stars, and were able to determine 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 results, published in Nature Astronomy, revealed that the group of stars surveyed all have similar ages, or are slightly younger than the majority of the stars known to have started their lives within the Milky Way. 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 Montalbán, lead author on 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 measures the relative frequencies and amplitudes of the natural modes of oscillation of the stars. This enables scientists to assemble information about the star’s size and internal structure, which enables accurate estimations of the star’s age to be made.
In this research, the team used information on the individual oscillation modes of each star, rather than averaged properties of their pulsations. They were also able to use asteroseimology in combination with spectroscopy – which enables the chemical composition of the stars to be measured.
Co-author, Professor Andrea Miglio, at 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.”
The work is the result of the collaborative project, Asterochonometry, funded by the European Research council and hosted by the Università di Bologna and the University of Birmingham. The research was also supported by the Science and Technology Facilities Council through a doctoral studentship.
