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 | ||
|---|---|---|
 March 4, 1821 (Saros 127) |
 February 12, 1850 (Saros 128) |
 January 22, 1879 (Saros 129) |
 January 3, 1908 (Saros 130) |
 December 13, 1936 (Saros 131) |
 November 23, 1965 (Saros 132) |
 November 3, 1994 (Saros 133) |
 October 14, 2023 (Saros 134) |
 September 22, 2052 (Saros 135) |
 September 3, 2081 (Saros 136) |
 August 15, 2110 (Saros 137) |
 July 25, 2139 (Saros 138) |
 July 5, 2168 (Saros 139) |
 June 15, 2197 (Saros 140) |
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