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 | ||
|---|---|---|
 July 6, 1815 (Saros 143) |
 June 16, 1844 (Saros 144) |
 May 26, 1873 (Saros 145) |
 May 7, 1902 (Saros 146) |
 April 18, 1931 (Saros 147) |
 March 27, 1960 (Saros 148) |
 March 7, 1989 (Saros 149) |
 February 15, 2018 (Saros 150) |
 January 26, 2047 (Saros 151) |
 January 6, 2076 (Saros 152) |
 December 17, 2104 (Saros 153) |
 November 26, 2133 (Saros 154) |
 November 7, 2162 (Saros 155) |
 October 18, 2191 (Saros 156) |
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