This eclipse is a part of Saros series 150, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no hybrid or total eclipses in this set. The series ends at member 71 as a partial eclipse on September 29, 2991. 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 45 at 9 minutes, 58 seconds on December 19, 2522. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 5–27 occur between 1801 and 2200: | ||
|---|---|---|
| 5 | 6 | 7 |
 October 7, 1801 |
 October 19, 1819 |
 October 29, 1837 |
| 8 | 9 | 10 |
 November 9, 1855 |
 November 20, 1873 |
 December 1, 1891 |
| 11 | 12 | 13 |
 December 12, 1909 |
 December 24, 1927 |
 January 3, 1946 |
| 14 | 15 | 16 |
 January 14, 1964 |
 January 25, 1982 |
 February 5, 2000 |
| 17 | 18 | 19 |
 February 15, 2018 |
 February 27, 2036 |
 March 9, 2054 |
| 20 | 21 | 22 |
 March 19, 2072 |
 March 31, 2090 |
 April 11, 2108 |
| 23 | 24 | 25 |
 April 22, 2126 |
 May 3, 2144 |
 May 14, 2162 |
| 26 | 27 | |
 May 24, 2180 |
 June 4, 2198 | |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 150". eclipse.gsfc.nasa.gov.