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 | ||
|---|---|---|
 February 21, 1822 (Saros 137) |
 February 1, 1851 (Saros 138) |
 January 11, 1880 (Saros 139) |
 December 23, 1908 (Saros 140) |
 December 2, 1937 (Saros 141) |
 November 12, 1966 (Saros 142) |
 October 24, 1995 (Saros 143) |
 October 2, 2024 (Saros 144) |
 September 12, 2053 (Saros 145) |
 August 24, 2082 (Saros 146) |
 August 4, 2111 (Saros 147) |
 July 14, 2140 (Saros 148) |
 June 25, 2169 (Saros 149) |
 June 4, 2198 (Saros 150) |
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