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 is then computed from Besselian elements and traced where the shadow axis pierces Earth's surface.
Controls
← / → — previous / next eclipse (or arrow keys)
JUMP TO — type a year to jump to the nearest cataloged eclipse
PLAY — auto-advance every 2 seconds
Drag the globe to rotate; scroll to zoom
Hover a 3D landmark to see its name
What you see
Red ribbon: path of totality / annularity (umbra centerline as Earth rotates beneath the Moon's shadow)
Yellow dot: point of greatest eclipse (where shadow axis comes closest to Earth's center)
Sun & Moon positions from astronomy-engine (Moshier's port of JPL DE-style theories) — sub-arcsecond accurate
Eclipse search via SearchGlobalSolarEclipse/NextGlobalSolarEclipse from the same library
Besselian elements (x, y, d, μ, ℓ1, ℓ2) computed from geocentric Sun & Moon vectors
Central path = trace of where the shadow axis pierces Earth's surface, sampled every 30 s for ±3 hours around greatest eclipse
Accuracy
Eclipse times match NASA's catalog to seconds. Path positions are accurate to roughly ±1–2 km on the ground for the entire 1900–2200 range — effectively NASA-precision for a single-file browser tool. For mission-critical use, cross-check with eclipse.gsfc.nasa.gov.
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TOTAL
Date (UTC)—
Greatest eclipse—
Magnitude—
Gamma—
Central duration—
Max location—
Sun altitude—
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Computed live via astronomy-engine (Moshier ephemeris) + Besselian path · sub-km accuracy