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 | ||
|---|---|---|
 February 1, 1813 (Saros 118) |
 January 11, 1842 (Saros 119) |
 December 22, 1870 (Saros 120) |
 December 3, 1899 (Saros 121) |
 November 12, 1928 (Saros 122) |
 October 23, 1957 (Saros 123) |
 October 3, 1986 (Saros 124) |
 September 13, 2015 (Saros 125) |
 August 23, 2044 (Saros 126) |
 August 3, 2073 (Saros 127) |
 July 15, 2102 (Saros 128) |
 June 25, 2131 (Saros 129) |
 June 4, 2160 (Saros 130) |
 May 15, 2189 (Saros 131) |
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