The sun has been quite busy lately. It recently unleashed several powerful solar flares that sent hot solar material hurtling into space. On May 13, a sunspot named AR4086 erupted, releasing an X1.2-class solar flare, which is one of the most intense types of flares. The following day, another sunspot, AR4087, produced an M5.3 flare, followed by an even stronger X2.7 flare and an M7.7 flare shortly after.
These flares resulted in radio blackouts on the sunlit side of Earth, affecting North and South America, Europe, Africa, the Middle East, and Southeast Asia. When solar flares occur, they can disrupt radio communications due to the intense X-ray and ultraviolet radiation affecting the atmosphere.
Solar flares are bursts of electromagnetic radiation caused by intense magnetic activity on the sun’s surface. The sun’s surface has powerful magnetic fields that can twist and tangle. When the strain on these fields becomes too much, they snap and realign, releasing a surge of energy in the form of a solar flare. Not all flares have the same strength. The NOAA’s Space Weather Prediction Center categorizes them into classes: A, B, C, M, and X. Each class is ten times stronger than the last. For instance, an X2.7 flare is significantly more powerful than an M1 flare. The recent X1.2 and X2.7 flares were notable but among the weaker end of the X-class spectrum.
In fact, the strongest flare recorded in recent years was an X9 flare back in 2024. These recent solar flares were the first of their kind since March 2025.
The impacts of solar flares can extend beyond simple radio issues. When a flare occurs, it often coincides with a coronal mass ejection (CME), a massive eruption of solar material. While solar flares travel at the speed of light, CMEs can take longer to reach Earth. They can cause geomagnetic storms when they interact with Earth’s magnetic field. These storms can produce stunning auroras but can also lead to satellite and power grid disruptions.
Interestingly, the recent CME was aimed at Mars, not Earth, due to the sunspot’s position. NASA models predict that this CME will reach Mars on May 18, potentially creating auroras in its atmosphere.
As sunspot AR4087 continues its journey across the sun, it may produce more flares. NOAA predicts a significant chance for both M-class and potentially X-class solar flares in the coming days. They estimate a 65% chance for M-class activity and a 30% chance for X-class flares through May 17.
Solar activity is closely monitored because of its impact on technology and communication. As we learn more about the sun, understanding these events becomes increasingly vital.