This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. 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 20 at 12 minutes, 9 seconds on December 14, 1955. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 12–33 occur between 1801 and 2200: | ||
|---|---|---|
| 12 | 13 | 14 |
 September 17, 1811 |
 September 28, 1829 |
 October 9, 1847 |
| 15 | 16 | 17 |
 October 19, 1865 |
 October 30, 1883 |
 November 11, 1901 |
| 18 | 19 | 20 |
 November 22, 1919 |
 December 2, 1937 |
 December 14, 1955 |
| 21 | 22 | 23 |
 December 24, 1973 |
 January 4, 1992 |
 January 15, 2010 |
| 24 | 25 | 26 |
 January 26, 2028 |
 February 5, 2046 |
 February 17, 2064 |
| 27 | 28 | 29 |
 February 27, 2082 |
 March 10, 2100 |
 March 22, 2118 |
| 30 | 31 | 32 |
 April 1, 2136 |
 April 12, 2154 |
 April 23, 2172 |
| 33 | ||
 May 4, 2190 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 141". eclipse.gsfc.nasa.gov.