(Nanowerk News) An international team of scientists led by the University of Birmingham adopted the novel approach of applying the forensic characterisation of a single ancient, bright star called ν Indi as a probe of the history of the Milky Way. Stars carry “fossilized records” of their histories and hence the environments in which they formed. The team used data from satellites and ground-based telescopes to unlock this information from ν Indi.
The animation shows a schematic of the orbits of three stars within our Galaxy the Milky Way – whose extent is marked by the dashed line -- as viewed from above (left) and side-on (right), projected over the next half a billion years. The three stars are: nu Indi, the subject of the Nature Astronomy paper; a star accreted from Gaia-Enceladus (after its collision with the Milky Way); and the Sun. The accreted star came from outside the Galaxy, as part of the Gaia-Enceladus collision, and so has a very elongated orbit. The collision affected the motion and orbit of nu Indi. Notice how its orbit is quite different to that of the Sun.
The star was aged using its natural oscillations (asteroseismology), detected in data collected by NASA's recently launched Transiting Exoplanet Survey Satellite (TESS). Launched in 2018, TESS is surveying stars across most of the sky to search for planets orbiting the stars and to study the stars themselves. When combined with data from the European Space Agency (ESA) Gaia Mission, the detective story revealed that this ancient star was born early in the life of the Milky Way, but the Gaia-Enceladus collision altered its motion through our Galaxy.
Bill Chaplin, Professor of Astrophysics at the University of Birmingham and lead author of the study said: “Since the motion of ν Indi was affected by the Gaia-Enceladus collision, the collision must have happened once the star had formed. That is how we have been able to use the asteroseismically-determined age to place new limits on when the Gaia-Enceladus event occurred.”
Co-author Dr Ted Mackereth, also from Birmingham, said: “Because we see so many stars from Gaia-Enceladus, we think it must have had a large impact on the evolution of our Galaxy. Understanding that is now a very hot topic in astronomy, and this study is an important step in understanding when this collision occurred.”
Bill Chaplin added: “This study demonstrates the potential of asteroseismology with TESS, and what is possible when one has a variety of cutting-edge data available on a single, bright star”
The research clearly shows the strong potential of the TESS programme to draw together rich new insights about the stars that are our closest neighbours in the Milky Way.
