V1355 Orionis (also known as HD 291095) is an RS CVn-type binary star system located 400 light-years away in the constellation of Orion. An artist’s impression of the superflare from the main member of the V1355 Orionis binary system. Image credit: NAOJ. “Solar flares are explosive phenomena wherein magnetic energy stored around sunspots is suddenly released through magnetic reconnection. Generally, a solar flare releases about 1026-1032 erg,”...
