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 | ||
|---|---|---|
 June 26, 1824 (Saros 124) |
 June 6, 1853 (Saros 125) |
 May 17, 1882 (Saros 126) |
 April 28, 1911 (Saros 127) |
 April 7, 1940 (Saros 128) |
 March 18, 1969 (Saros 129) |
 February 26, 1998 (Saros 130) |
 February 6, 2027 (Saros 131) |
 January 16, 2056 (Saros 132) |
 December 27, 2084 (Saros 133) |
 December 8, 2113 (Saros 134) |
 November 17, 2142 (Saros 135) |
 October 29, 2171 (Saros 136) |
 October 9, 2200 (Saros 137) |
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