Astronomers have discovered a binary star system known as D9, surprisingly close to the supermassive black hole Sagittarius A* at the center of the Milky Way.
Binary stars are not expected to form or survive near black holes due to tidal forces, but the D9 system is young and estimated to merge into a single star within a million years.
The discovery of D9 was made using data from the Enhanced Resolution Imager and Spectrograph (ERIS) and the Spectrograph for INtegral Field Observations in the Near Infrared (SINFONI).
Finding binary stars near Sagittarius A* could provide insights into the formation of such systems in the vicinity of supermassive black holes.