Solar eclipse of April 28, 1911
| Solar eclipse of April 28, 1911 | |
|---|---|
Map
|
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| Type of eclipse | |
| Nature | Total |
| Gamma | -0.2294 |
| Magnitude | 1.0562 |
| Maximum eclipse | |
| Duration | 297 sec (4 m 57 s) |
| Coordinates | 1°54′N 151°54′W / 1.9°N 151.9°W |
| Max. width of band | 190 km (120 mi) |
| Times (UTC) | |
| Greatest eclipse | 22:27:22 |
| References | |
| Saros | 127 (52 of 82) |
| Catalog # (SE5000) | 9306 |
A total solar eclipse occurred on April 28, 1911. 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.
Each member in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532.
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