On Wednesday, August 12, 2026, the Moon slid directly between the Earth and the Sun, plunging a narrow strip of the Northern Hemisphere into daytime darkness. It was Europe’s first total solar eclipse since 1999, with the Moon’s shadow sweept across Greenland, Iceland, northern Spain, and the Balearic Islands.
For anyone standing in the right spot, day briefly turned to twilight, streetlights may have flickered on, and the Sun’s ghostly outer atmosphere — the corona — became visible for a couple of minutes. Watch it here:
What made this eclipse special
The path of totality crossed Russia, Greenland, and Europe — specifically Iceland, Spain, and Portugal — with a maximum duration of totality of 2 minutes and 18 seconds. Along the way, the shadow passed over the Arctic Ocean, Greenland, Iceland, the Atlantic Ocean, Portugal, and northern Spain.
The eclipse actually began at sunrise on the other side of the globe. The track of totality started at sunrise over the polar permafrost of Russia’s Taymyr Peninsula and the nearby Laptev Sea, touching down on an uninhabited Arctic coastline before continuing on its journey west.
Because so much of the path fell over open water and remote Arctic terrain, two-thirds of the Moon’s shadow path fell over water, making Spain and Mallorca the most promising locations for clear-sky viewing.
Timing: Greatest eclipse occurred at 17:47 UTC, 23:17 IST
What causes a solar eclipse?
A solar eclipse is really just a matter of cosmic geometry – three objects lining up in space. A solar eclipse happens when the Moon passes directly between the Earth and the Sun, casting a shadow onto Earth’s surface. From the ground, it looks like the Moon is “eating” the Sun, because the Moon blocks some or all of the sunlight reaching a given location.
This can only happen during a new moon, when the Moon is positioned between the Earth and the Sun. But new moons happen every month, and we don’t get an eclipse every month — so what’s the missing piece?
Why eclipses don’t happen every month
The Moon’s orbit around Earth is tilted about 5 degrees relative to Earth’s orbit around the Sun. Because of this tilt, the Moon usually passes slightly above or below the Sun during a new moon, and no shadow reaches Earth.
Eclipses can only occur when a new moon happens near one of two points called nodes — the spots where the Moon’s tilted orbital path crosses Earth’s orbital plane. This is exactly why astronomers can pin down eclipses months or years in advance. The August 12, 2026 eclipse occurred at the Moon’s descending node of orbit.
When’s the next one?
Eclipses come in predictable cycles, and this one was no exception — it belonged to Saros series 126, the 48th of 72 eclipses in that particular cycle. If you missed this one, don’t worry: the Moon’s shadow will be back. Every eclipse in a Saros series repeats roughly every 18 years and 11 days, tracing a similar (but shifted) path across the globe.
For now, this eclipse gave much of Europe its long-awaited return to totality — a brief, dramatic reminder of just how precisely the Sun, Moon, and Earth line up so often.
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