Solar eclipse of September 23, 2090
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| Solar eclipse of September 23, 2090 | |
|---|---|
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.9157 |
| Magnitude | 1.0562 |
| Maximum eclipse | |
| Duration | 3m 36s |
| Coordinates | 60.7N 40.5W |
| Max. width of band | 463 km |
| Times (UTC) | |
| Greatest eclipse | 16:56:36 |
| References | |
| Saros | 155 (10 of 71) |
| Catalog # (SE5000) | 9711 |
A total solar eclipse will occur on September 23, 2090. 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 2087-2090 [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.
| 120 | May 2, 2087 Partial |
125 | October 26, 2087 Partial |
| 130 | April 21, 2088 Total |
135 | October 14, 2088 Annular |
| 140 | April 10, 2089 Annular |
145 | October 4, 2089 Total |
| 150 | March 31, 2090 Partial |
155 | September 23, 2090 Total |
Notes [edit]
References [edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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