This eclipse is a part of Saros series 132, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146; hybrid eclipses on March 23, 2164 and April 3, 2182; and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. 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 was produced by member 25 at 6 minutes, 56 seconds on May 9, 1641, and the longest duration of totality will be produced by member 61 at 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 34–56 occur between 1801 and 2200: | |||
|---|---|---|---|
| 34 | 35 | 36 | |
 August 17, 1803 |
 August 27, 1821 |
 September 7, 1839 | |
| 37 | 38 | 39 | |
 September 18, 1857 |
 September 29, 1875 |
 October 9, 1893 | |
| 40 | 41 | 42 | |
 October 22, 1911 |
 November 1, 1929 |
 November 12, 1947 | |
| 43 | 44 | 45 | |
 November 23, 1965 |
 December 4, 1983 |
 December 14, 2001 | |
| 46 | 47 | 48 | |
 December 26, 2019 |
 January 5, 2038 |
 January 16, 2056 | |
| 49 | 50 | 51 | |
 January 27, 2074 |
 February 7, 2092 |
 February 18, 2110 | |
| 52 | 53 | 54 | |
 March 1, 2128 |
 March 12, 2146 |
 March 23, 2164 | |
| 55 | 56 | ||
 April 3, 2182 |
 April 14, 2200 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 132". eclipse.gsfc.nasa.gov.