total solar eclipse
Total solar eclipse of 30 April 2041
At greatest eclipse the Moon's disc spans 0.5313° against the Sun's 0.5295° — a ratio of 1.0034. Because the Moon appears larger, it covers the Sun completely and totality is possible.
Where you can see it
The shadow crosses South America, the South Atlantic, Africa and the Indian Ocean. Only along the central line does the Moon cover the Sun completely; a few hundred kilometres either side and it is a partial eclipse, which looks nothing like the same event.
How much is covered, and where
Sorted by how much of the Sun disappears. Below about 40% nothing looks wrong to the naked eye — the Sun is so bright that losing a third of it changes very little. Never look without a proper solar filter regardless.
| City | Covered | Maximum (UTC) | Sun altitude |
|---|---|---|---|
| Nairobi | 93% | 13:02 | 35° |
| Buenos Aires | 40% | 10:07 | below horizon |
| Cape Town | 33% | 11:26 | 40° |
| Johannesburg | 33% | 12:01 | 40° |
| Jeddah | 27% | 13:20 | 33° |
| Mumbai | 18% | 13:33 | below horizon |
| São Paulo | 16% | 10:10 | 9° |
| Luxor | 14% | 13:14 | 40° |
| Dubai | 12% | 13:31 | 16° |
| Cairo | 4% | 13:14 | 41° |
Not visible at all from Brussels, Antwerp, Ghent, Bruges, Liège, Leuven, Charleroi, Amsterdam, Rotterdam, The Hague, Utrecht, Eindhoven, Luxembourg, London, Manchester, Birmingham, Glasgow, Edinburgh, Cardiff, Belfast, Dublin, Paris, Lyon, Marseille, Berlin, Munich, Hamburg, Cologne, Zurich, Vienna, Prague, Warsaw, Copenhagen, Stockholm, Oslo, Helsinki, Reykjavík, Madrid, Barcelona, Lisbon, Rome, Milan, Athens, Istanbul, New York, Boston, Washington, D.C., Miami, Atlanta, Chicago, Houston, Dallas, Denver, Phoenix, Los Angeles, San Francisco, Seattle, Toronto, Montreal, Vancouver, Mexico City, Santiago, Cádiz, Málaga, Tangier, Benghazi, Delhi, Singapore, Hong Kong, Tokyo, Seoul, Sydney, Melbourne, Brisbane, Perth, Auckland.
Greatest eclipse falls at -9.63°, 12.20° — the point where the axis passes closest to Earth's centre. The central line is computed from the Sun–Moon axis intersected with the geoid, and agrees with the reference coordinates to within a tenth of a kilometre.
Why eclipses come in seasons
The Moon's orbit is tilted about 5° to the ecliptic, so at most new and full moons it passes above or below the alignment. An eclipse needs the syzygy to coincide with the Moon being near one of the two nodes where the orbits cross. At this eclipse the Moon's ecliptic latitude was -0.435° — close enough to zero for the shadow to connect.
Times computed from VSOP87 and an ELP-derived lunar theory, validated against NOVAS and JPL Horizons to within one arcminute. See the alignment for yourself in the live simulation.