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 | ||
|---|---|---|
 March 24, 1811 (Saros 136) |
 March 4, 1840 (Saros 137) |
 February 11, 1869 (Saros 138) |
 January 22, 1898 (Saros 139) |
 January 3, 1927 (Saros 140) |
 December 14, 1955 (Saros 141) |
 November 22, 1984 (Saros 142) |
 November 3, 2013 (Saros 143) |
 October 14, 2042 (Saros 144) |
 September 23, 2071 (Saros 145) |
 September 4, 2100 (Saros 146) |
 August 15, 2129 (Saros 147) |
 July 25, 2158 (Saros 148) |
 July 6, 2187 (Saros 149) |
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