Presently, the faint star V Sagittae, V Sge, in the constellation Sagitta, is barely visible, even in mid-sized telescopes.
Nevertheless, around the year 2083, this harmless star will explode, becoming as bright as Sirius, the most shining star seen in the night sky. Throughout this time of the eruption, V Sge will be the most luminous star within the Milky Way galaxy.
This prediction is being displayed for the first time at the 235th American Astronomical Society assembly in Honolulu, by astronomers Bradley E. Schaefer, and Manos Chatzopoulos, with the Louisiana State University Division of Physics & Astronomy.
V Sge is a star community in a big and numerous class known as Cataclysmic Variables, CVs, consisting of a general star in a binary orbit around a white fairy star, where the traditional star’s mass is slowly falling onto the white dwarf.
CVs embrace multiple types of binary stars, usually with spectacular behavior. V Sge is the most excessive of all the CVs, roughly 100 times more luminous than all different known CVs, and is powering a massive stellar wind, equal to the winds of the most huge stars before their demise.
These two extreme properties are brought on by the fact that the traditional star is 3.9 occasions more massive than the white dwarf.
This realization came from regular measures of V Sge’s brightness on old sky photographs now archived at the Harvard College Observatory.