Step through every solar eclipse from 1900 to 2200 — about 3,700 events. Eclipse identification and Sun/Moon positions come from astronomy-engine (Don Cross's port of Steve Moshier's ephemeris, sub-arcsecond accurate, MIT-licensed). Path of the Moon's shadow uses the same MoonShadow + GeoidIntersect pipeline as SearchGlobalSolarEclipse — WGS84 geoid intersection for NASA/Espenak parity.
SearchGlobalSolarEclipse/NextGlobalSolarEclipse from the same librarySearchLocalSolarEclipseEclipse times and path geometry match NASA's Five Millennium Canon (Espenak/Meeus) — sub-km on the ground for 1900–2200. The GeoidIntersect pipeline is the same one astronomy-engine uses internally for global eclipse search. For mission-critical planning, cross-check with eclipse.gsfc.nasa.gov.
Step through every solar eclipse from 1900 to 2200. Paths of totality are computed with astronomy-engine (sub-arcsecond ephemeris) and drawn on a rotatable 3D Earth.
?date=2026-08-12 or ?year=2027 jump straight to the eclipse.Sign in with GitHub to share strategies, ask questions, or report a bug.