The centerline and totality band are self-computed from public-domain NASA/Espenak Besselian elements — matching NASA’s published path to within ~0.15 km. Lunar-limb relief and local terrain can shift the true edges by ~1–3 km.
See it from your location
Your eclipse type, peak coverage, and contact times — in your local time.
Will you see totality?
Check your current location against the path of totality.
Next steps
Keep building the eclipse plan.
Compare paths, nearby dark-sky stays, protected places, and practical field guides for this event.