An article published in “The Astrophysical Journal” reports the detection of a superflare in the V1355 Orionis system, a pair of stars of the variable RS Canum Venaticorum type, which features a more massive and evolved star than its companion. A team of researchers used space and ground-based telescopes to monitor the activity of the V1355 Orionis system, known for its powerful eruptions. This allowed to obtain continuous observations of this phenomenon, which was generated by a process called prominence eruption. This study offers new insights into these stellar phenomena that also occur on the Sun, albeit with a much smaller force.