This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 10–31 occur between 1801 and 2200: | ||
|---|---|---|
| 10 | 11 | 12 |
 December 30, 1815 |
 January 9, 1834 |
 January 21, 1852 |
| 13 | 14 | 15 |
 January 31, 1870 |
 February 11, 1888 |
 February 23, 1906 |
| 16 | 17 | 18 |
 March 5, 1924 |
 March 16, 1942 |
 March 27, 1960 |
| 19 | 20 | 21 |
 April 7, 1978 |
 April 17, 1996 |
 April 29, 2014 |
| 22 | 23 | 24 |
 May 9, 2032 |
 May 20, 2050 |
 May 31, 2068 |
| 25 | 26 | 27 |
 June 11, 2086 |
 June 22, 2104 |
 July 4, 2122 |
| 28 | 29 | 30 |
 July 14, 2140 |
 July 25, 2158 |
 August 4, 2176 |
| 31 | ||
 August 16, 2194 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 148". eclipse.gsfc.nasa.gov.