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 27, 1821 (Saros 132) |
 August 7, 1850 (Saros 133) |
 July 19, 1879 (Saros 134) |
 June 28, 1908 (Saros 135) |
 June 8, 1937 (Saros 136) |
 May 20, 1966 (Saros 137) |
 April 29, 1995 (Saros 138) |
 April 8, 2024 (Saros 139) |
 March 20, 2053 (Saros 140) |
 February 27, 2082 (Saros 141) |
 February 8, 2111 (Saros 142) |
 January 20, 2140 (Saros 143) |
 December 29, 2168 (Saros 144) |
 December 9, 2197 (Saros 145) |
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