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 | ||
|---|---|---|
 October 19, 1808 (Saros 111) |
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 August 20, 1895 (Saros 114) |
 July 31, 1924 (Saros 115) |
 July 11, 1953 (Saros 116) |
 June 21, 1982 (Saros 117) |
 June 1, 2011 (Saros 118) |
 May 11, 2040 (Saros 119) |
 April 21, 2069 (Saros 120) |
 April 1, 2098 (Saros 121) |
 March 13, 2127 (Saros 122) |
 February 21, 2156 (Saros 123) |
 January 31, 2185 (Saros 124) |
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