A significant space weather event unfolded recently as a powerful X1.9-class solar flare erupted from sunspot AR 4341, unleashing a Coronal Mass Ejection (CME) that reached Earth in an exceptionally short span of just 25 hours. This rapid arrival is notably faster than the typical travel time for CMEs, which generally takes several days, sometimes extending up to four days, to traverse the distance from the Sun to Earth. The impact of this unusually swift CME triggered a severe G4-class geomagnetic storm, as confirmed by NOAA's Space Weather Prediction Center. While solar flares emit radiation that reaches Earth in approximately eight minutes, CMEs involve massive clouds of solar plasma and magnetic fields that travel at varying speeds. The fastest recorded CMEs can arrive in as little as 15-18 hours, making the recent 25-hour transit time a significant and relatively rare occurrence. Geomagnetic storms of this magnitude can have widespread implications, including potential disruptions to power grids, satellite operations, and high-frequency radio communications, particularly in high-latitude regions. Beyond technological impacts, such severe storms also lead to spectacular aurora displays, which were expected to be visible at unusually low latitudes across Canada and potentially parts of the southern United States. This event underscores the dynamic nature of the Sun's activity and the importance of space weather monitoring for global infrastructure.