🚨 Direct Hit: Monster X5.16 Solar Flare Erupts Facing Earth ☀️ At 10:00 UTC today, sunspot region 4274 unleashed the biggest flare of 2025 so far. The X5.16 blast triggered a strong R3 radio blackout, wiping out HF comms across the daylight side. A double CME impact is already inbound. This flare could be adding a third. ⚠️ We’re monitoring closely and will post updates as new data comes in. #SolarFlare #X5 #SpaceWeather #Sunspot4274 #HFBlackout #AuroraWatch #SolarCycle25 #AboveTheNormNews | Ab

The Sun emitted a strong solar flare on Nov. 30, 2025, peaking at 9:49 p.m. ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X1.9 class: go.nasa.gov/4alXf6P Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. However — when intense enough — they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such sp

614K views · 7.4K reactions | Last Solar Flare of 2025 caught on camera with NASA-Recorded Solar Sound #solarflare #sun #solar #space | Space science | Facebook

#FirstpostNews: Sun Releases Strong Flare, Energy Equivalent to a Billion Bombs The Sun released a powerful solar flare on February 3, following several flares in previous days. NASA confirmed it was an X-class flare, the most intense category of solar flares. The European Space Agency said such flares can release as much energy as a billion atomic bombs. The Space Weather Prediction Center noted that flares of this strength are rare but not unprecedented. These solar flares can trigger geomagne

The Sun just fired off its most powerful kind of flare. At 1:09 p.m. EST on January 18, 2026, the Solar Dynamics Observatory recorded a dramatic burst of light and energy emerging from the Sun’s surface. Classified as an X1.9 flare, this event is part of the most intense category of solar flares — with the potential to disrupt life here on Earth. Solar flares are sudden explosions of energy caused by the tangling, crossing, or reorganizing of magnetic field lines near sunspots. This particular f