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 | ||
|---|---|---|
 September 28, 1810 (Saros 131) |
 September 7, 1839 (Saros 132) |
 August 18, 1868 (Saros 133) |
 July 29, 1897 (Saros 134) |
 July 9, 1926 (Saros 135) |
 June 20, 1955 (Saros 136) |
 May 30, 1984 (Saros 137) |
 May 10, 2013 (Saros 138) |
 April 20, 2042 (Saros 139) |
 March 31, 2071 (Saros 140) |
 March 10, 2100 (Saros 141) |
 February 18, 2129 (Saros 142) |
 January 30, 2158 (Saros 143) |
 January 9, 2187 (Saros 144) |
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