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 | ||
|---|---|---|
 June 16, 1825 (Saros 134) |
 May 26, 1854 (Saros 135) |
 May 6, 1883 (Saros 136) |
 April 17, 1912 (Saros 137) |
 March 27, 1941 (Saros 138) |
 March 7, 1970 (Saros 139) |
 February 16, 1999 (Saros 140) |
 January 26, 2028 (Saros 141) |
 January 5, 2057 (Saros 142) |
 December 16, 2085 (Saros 143) |
 November 27, 2114 (Saros 144) |
 November 7, 2143 (Saros 145) |
 October 17, 2172 (Saros 146) |
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