Where the Moon's shadow lands, and when it next reaches you
Drag to turn the globe; click anywhere to compute that spot's eclipses
directly from the Besselian elements of every eclipse between 2000 and 2200.
Shading shows how often the shadow has swept each point over five millennia — it is
markedly uneven.
1.0×Drag to rotate · scroll to zoom · click to inspect · double-click to centre
path of totality or annularity
central line
edge of the partial zone, hour by hour
Click the globe
Pick any point on Earth
—
between total eclipses, long-run average
—
between annular eclipses
Every eclipse visible from the point you choose, with contact
times computed on the spot — not looked up from a table.