A total solar eclipse crosses the Arctic and parts of Europe
The Moon's central shadow reaches Greenland, Iceland, northern Spain, a small part of Portugal, and part of Russia while the rest of the world can follow the geometry from home.
The meaning behind the moment
Totality is one of nature's most precise alignments: a small moving patch of Earth briefly enters the Moon's central shadow.
Walk through the Moon's moving shadow
Move through a three-step shadow diagram: the Moon crosses the Sun, its narrow central shadow touches Earth, and most places remain outside that path.
- Start with the physical arrangement.
- Notice what changes from Earth's point of view.
- Connect the geometry to what a person can actually experience.
Useful without a location; richer with one
The global event and indoor experience are complete above. Add a city on This Week for a localized time and an honest easy / possible / not-visible result.
No equipment required
Only observers inside the official path can see totality. Elsewhere, use the NASA map for the local partial phase; location enrichment never guesses across a path boundary.
Where to look: Look toward the Sun only through an approved solar-viewing method.
Except during the brief total phase at a location inside the path, never look directly at the Sun without safe solar viewers that comply with ISO 12312-2. Ordinary sunglasses are not safe.
Source, calculation, and revision
- Primary source
- NASA Eclipses
- Last checked
- 2026-08-11T18:16:09.116566+00:00
- Calculation
- astronomy-engine@2.1.19
- Precision
- exact; weather is not included
- Media
- NASA source evidence; Space Now original explainer · original editorial text with linked first-party evidence
We’ll keep this page current
After the event, this durable page will preserve the result, official replay, or a concise correction without silently rewriting the earlier revision.