Solar eclipse of October 1, 1921
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| Solar eclipse of October 1, 1921 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | -0.9383 |
| Magnitude | 1.0293 |
| Maximum eclipse | |
| Duration | 1m 52s |
| Coordinates | 66.1S 56.1W |
| Max. width of band | 291 km |
| Times (UTC) | |
| Greatest eclipse | 12:35:58 |
| References | |
| Saros | 123 (48 of 70) |
| Catalog # (SE5000) | 9331 |
A total solar eclipse occurred on October 1, 1922. 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 1921-1924 [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 | |||
|---|---|---|---|---|
| 118 | April 8, 1921 Annular |
123 | October 1, 1921 Total |
|
| 128 | March 28, 1922 Annular |
133 | September 21, 1922 Total |
|
| 138 | March 17, 1923 Annular |
143 | September 10, 1923 Total |
|
| 148 | March 5, 1924 Partial |
153 | August 30, 1924 Partial |
|
Notes [edit]
References [edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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