This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity will be produced by member 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 1–8 occur between 2058 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
 June 21, 2058 |
 July 1, 2076 |
 July 12, 2094 |
| 4 | 5 | 6 |
 July 23, 2112 |
 August 4, 2130 |
 August 14, 2148 |
| 7 | 8 | |
 August 25, 2166 |
 September 4, 2184 | |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 157". eclipse.gsfc.nasa.gov.