On 2 August 2027 the Moon’s shadow crosses the Atlantic, the Strait of Gibraltar, North Africa and parts of the Middle East before ending over the Indian Ocean. Southern Spain is Europe’s total-eclipse gateway for this event.
A worldwide maximum of about 6 minutes 23 seconds
NASA lists the eclipse as total, Saros 136, with a greatest duration of roughly 6 minutes 23 seconds near Egypt. Spain is earlier on the path, so durations are shorter but still exceptional by European standards.
The eclipse phases
First contact begins the partial phase as the Moon starts covering the Sun. Second contact begins totality at locations inside the totality path. Maximum eclipse occurs near the middle of the total phase. Third contact ends totality, and fourth contact ends the final partial phase.
Why totality is fundamentally different
During a partial eclipse, even when almost all of the Sun is covered, the remaining photosphere is still intensely bright. During complete totality the photosphere is hidden, the corona becomes visible and the environment changes rapidly. That is why being a few kilometres inside or outside the path boundary can transform the experience.
Solar safety
Appropriate certified eclipse viewers are required during every partial phase. Ordinary sunglasses are not sufficient. Cameras, binoculars and telescopes require correct solar filters mounted in front of the optics. Direct unaided viewing is only safe during complete totality, and protection must be restored immediately when the bright photosphere returns.
Planning matters because the event is predictable
Astronomy tells us the date and geometry years in advance. The uncertain variables are human: weather, transport, accommodation, crowding and access. Good eclipse planning therefore combines official astronomical data with a flexible travel plan.