Solar eclipse of April 21, 2088
| Solar eclipse of April 21, 2088 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.4135 |
| Magnitude | 1.0474 |
| Maximum eclipse | |
| Duration | 238 sec (3 m 58 s) |
| Coordinates | 36°00′N 15°06′E / 36°N 15.1°E |
| Max. width of band | 173 km (107 mi) |
| Times (UTC) | |
| Greatest eclipse | 10:31:49 |
| References | |
| Saros | 130 (56 of 73) |
| Catalog # (SE5000) | 9706 |
A total solar eclipse will occur on April 21, 2088. 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.
Related eclipses
Solar eclipses 2087-2090
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 |
Saros 130
It is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619.[1]
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Series members 43-56 between 1853 and 2100
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Notes
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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