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, 1805 (Saros 114) |
 June 7, 1834 (Saros 115) |
 May 17, 1863 (Saros 116) |
 April 26, 1892 (Saros 117) |
 April 8, 1921 (Saros 118) |
 March 18, 1950 (Saros 119) |
 February 26, 1979 (Saros 120) |
 February 7, 2008 (Saros 121) |
 January 16, 2037 (Saros 122) |
 December 27, 2065 (Saros 123) |
 December 7, 2094 (Saros 124) |
 November 18, 2123 (Saros 125) |
 October 28, 2152 (Saros 126) |
 October 8, 2181 (Saros 127) |
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