This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. 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 totality was produced by member 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 41–62 occur between 1801 and 2200: | ||
|---|---|---|
| 41 | 42 | 43 |
 November 9, 1817 |
 November 20, 1835 |
 November 30, 1853 |
| 44 | 45 | 46 |
 December 12, 1871 |
 December 22, 1889 |
 January 3, 1908 |
| 47 | 48 | 49 |
 January 14, 1926 |
 January 25, 1944 |
 February 5, 1962 |
| 50 | 51 | 52 |
 February 16, 1980 |
 February 26, 1998 |
 March 9, 2016 |
| 53 | 54 | 55 |
 March 20, 2034 |
 March 30, 2052 |
 April 11, 2070 |
| 56 | 57 | 58 |
 April 21, 2088 |
 May 3, 2106 |
 May 14, 2124 |
| 59 | 60 | 61 |
 May 25, 2142 |
 June 4, 2160 |
 June 16, 2178 |
| 62 | ||
 June 26, 2196 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 130". eclipse.gsfc.nasa.gov.