☀️ The Sun today — not as quiet as it looks. What you see here are sunspot groups AR4444, AR4447, AR4455 and AR4464. Dark patches on a star 1.4 million km across. Each one a region of intense, twisted magnetic fields suppressing the surface plasma from below — that's why they appear darker: they're "only" around 3,500 K, while the surrounding photosphere burns at ~5,778 K.
AR4447 has been the quite active of the bunch lately, leading flare production with several C-class events. And AR4455 — just rotating into view from the far left side — has already been firing prominences and jets, with astronomers watching closely to see what it brings.
Solar Cycle 25 peaked around October 2024 and activity has been gradually declining 📉 since early 2026 — so catching a disk this busy, YEAH, is still worth documenting. 🔭😉
Shot in white light through my Takahashi TOA-130NFB telescope Sony A7RV Sony FE 2× teleconverter. The granulation texture across the photosphere — that subtle "orange peel" surface — is convection cells, each roughly the size of Greece 🇬🇷, churning beneath you.
#SolarObserving