Discoveries


Recent Discoveries Stories

This image shows the gas disc in a computer simulation of a Milky Way-like galaxy from the Auriga suite. Colours represent the ratio of magnesium (Mg) to iron (Fe), revealing that the galactic centre (pink) is poor in Mg, while the outskirts (green) are Mg-rich. These chemical patterns provide important clues about how the galaxy formed.
New simulations show why the Milky Way’s stars split into two chemical groups and reveal a new view of galactic evolution.
Joseph Shavitupda