Revealing the history of the Milky Way Galaxy through precision stellar spectroscopy

点击翻译按钮获取中文摘要

How did the Milky Way Galaxy form? The answer to this fundamental question lies in the chemical compositions of stars. Enormous investments by the Australian and international community into state-of-the-art facilities and surveys will yield a 1 million star sample for chemical analysis. To fully harvest the information from those surveys requires stellar chemical composition measurements of the highest possible precision. This project aims to use recently pioneered analysis techniques that have led the field of chemical abundance measurements in stars to the unprecedented precision level of 2 per cent (a five-fold improvement) to chart the evolution of our Galaxy over cosmic time.