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 8, 1823 (Saros 114) |
 June 17, 1852 (Saros 115) |
 May 27, 1881 (Saros 116) |
 May 9, 1910 (Saros 117) |
 April 19, 1939 (Saros 118) |
 March 28, 1968 (Saros 119) |
 March 9, 1997 (Saros 120) |
 February 17, 2026 (Saros 121) |
 January 27, 2055 (Saros 122) |
 January 7, 2084 (Saros 123) |
 December 19, 2112 (Saros 124) |
 November 28, 2141 (Saros 125) |
 November 8, 2170 (Saros 126) |
 October 19, 2199 (Saros 127) |
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