Solar eclipse of April 16, 1893 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.1764 |
Magnitude | 1.0556 |
Maximum eclipse | |
Duration | 287 s (4 min 47 s) |
Coordinates | 1°18′N 34°36′W / 1.3°N 34.6°W |
Max. width of band | 186 km (116 mi) |
Times (UTC) | |
Greatest eclipse | 14:36:11 |
References | |
Saros | 127 (51 of 82) |
Catalog # (SE5000) | 9264 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, April 16, 1893, with a magnitude of 1.0556. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days before perigee (on April 17, 1893, at 21:50 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of the modern-day countries of Chile, Argentina, Paraguay, Brazil, Senegal, Mauritania, Mali, southern Algeria, Niger, Chad, and Sudan. A partial solar eclipse was also visible for parts of South America, Africa, and Southern Europe.