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 | ||
|---|---|---|
 April 14, 1809 (Saros 116) |
 March 25, 1838 (Saros 117) |
 March 6, 1867 (Saros 118) |
 February 13, 1896 (Saros 119) |
 January 24, 1925 (Saros 120) |
 January 5, 1954 (Saros 121) |
 December 15, 1982 (Saros 122) |
 November 25, 2011 (Saros 123) |
 November 4, 2040 (Saros 124) |
 October 15, 2069 (Saros 125) |
 September 25, 2098 (Saros 126) |
 September 6, 2127 (Saros 127) |
 August 16, 2156 (Saros 128) |
 July 26, 2185 (Saros 129) |
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