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 | ||
|---|---|---|
 August 16, 1822 (Saros 142) |
 July 28, 1851 (Saros 143) |
 July 7, 1880 (Saros 144) |
 June 17, 1909 (Saros 145) |
 May 29, 1938 (Saros 146) |
 May 9, 1967 (Saros 147) |
 April 17, 1996 (Saros 148) |
 March 29, 2025 (Saros 149) |
 March 9, 2054 (Saros 150) |
 February 16, 2083 (Saros 151) |
 January 29, 2112 (Saros 152) |
 January 8, 2141 (Saros 153) |
 December 18, 2169 (Saros 154) |
 November 28, 2198 (Saros 155) |
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