Solar eclipse of May 19, 1928
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| Solar eclipse of May 19, 1928 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | 1.0048 |
| Magnitude | 1.014 |
| Maximum eclipse | |
| Duration | - |
| Coordinates | 63.3S 22.5E |
| Max. width of band | - km |
| Times (UTC) | |
| Greatest eclipse | 13:24:20 |
| References | |
| Saros | 117 (64 of 71) |
| Catalog # (SE5000) | 9347 |
A total solar eclipse occurred on May 19, 1928. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.
Contents |
Related eclipses[edit]
Solar eclipses 1928-1931[edit]
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.
| Ascending node | Descending node | |||
|---|---|---|---|---|
| 117 | May 19, 1928 Total |
122 | November 12, 1928 Partial |
|
| 127 | May 9, 1929 Total |
132 | November 1, 1929 Annular |
|
| 137 | April 28, 1930 Hybrid |
142 | October 21, 1930 Total |
|
| 147 | April 18, 1931 Partial |
152 | October 11, 1931 Partial |
|
Notes[edit]
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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