(Updated) Sun emits powerful solar flare; NASA telescope captures image

On May 2, 2024, at 10:22 p.m. ET, the Sun released a powerful solar flare, classified as an X1.6 by NASA, indicating an intense burst of radiation. NASA's Solar Dynamics Observatory (SDO), which constantly monitors the Sun, successfully captured an image of this solar event.

Solar flares are intense bursts of radiation emanating from releasing magnetic energy associated with sunspots. Flares are classified into three categories: C, M, and X, with X-class flares being the most powerful. The numerical value denotes the flare's strength, with X1.6 reflecting a powerful flare.

The effects of such flares are far-reaching, impacting not only Earth's space environment but also our technological infrastructure. The intense energy released can disrupt radio communications, navigation systems, and even pose risks to electric power grids. In addition to this, exposure to increased radiation during these events can also be dangerous for spacecraft and astronauts.

The Sun emitted a strong solar flare on May 2, peaking at 10:22pm ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X1.6. https://t.co/FmdiOR2kP9 pic.twitter.com/NaE62YWeS1

— NASA Sun & Space (@NASASun) May 3, 2024

Solar flares and Coronal Mass Ejections (CMEs) frequently occur during the solar maximum - a period of intense solar activity in the 11-year solar cycle of the Sun. The current solar cycle, known as Solar Cycle 25 is expected to peak around 2025.

Update 1

The Sun released two X1.0 solar flares, one peaking at 9:41 p.m. ET on May 7, 2024, and another at 1:09 a.m. ET on May 8, 2024.

Update 2

Two more strong solar flares were unleashed by the Sun on May 8 and May 9, 2024. The first flare is classified as an X1.0 flare and the second flare is classified as an X2.2 flare, NASA said on Thursday.