This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
 April 13, 1801 (Saros 145) |
 March 24, 1830 (Saros 146) |
 March 4, 1859 (Saros 147) |
 February 11, 1888 (Saros 148) |
 January 23, 1917 (Saros 149) |
 January 3, 1946 (Saros 150) |
 December 13, 1974 (Saros 151) |
 November 23, 2003 (Saros 152) |
 November 3, 2032 (Saros 153) |
 October 13, 2061 (Saros 154) |
 September 23, 2090 (Saros 155) |
 September 5, 2119 (Saros 156) |
 August 14, 2148 (Saros 157) |
 July 25, 2177 (Saros 158) |
|