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 1844 and 2200 | ||
|---|---|---|
 November 10, 1844 (Saros 111) |
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 September 12, 1931 (Saros 114) |
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 July 13, 2018 (Saros 117) |
 June 23, 2047 (Saros 118) |
 June 1, 2076 (Saros 119) |
 May 14, 2105 (Saros 120) |
 April 24, 2134 (Saros 121) |
 April 3, 2163 (Saros 122) |
 March 13, 2192 (Saros 123) |
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