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 4, 1810 (Saros 126) |
 March 15, 1839 (Saros 127) |
 February 23, 1868 (Saros 128) |
 February 1, 1897 (Saros 129) |
 January 14, 1926 (Saros 130) |
 December 25, 1954 (Saros 131) |
 December 4, 1983 (Saros 132) |
 November 13, 2012 (Saros 133) |
 October 25, 2041 (Saros 134) |
 October 4, 2070 (Saros 135) |
 September 14, 2099 (Saros 136) |
 August 25, 2128 (Saros 137) |
 August 5, 2157 (Saros 138) |
 July 16, 2186 (Saros 139) |
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