Ultra-metal-poor star discovered in Milky Way’s halo

By analyzing the data from ESA’s Gaia satellite, astronomers from the University of Chicago, Illinois and elsewhere, have identified a new ultra-metal-poor star. The newfound star, designated GDR3_526285, turns out to be one of the most metal-poor stars detected so far. The finding was announced in a research paper published August 8 in The Astrophysical Journal Letters.