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 5, 1826 (Saros 144) |
 May 16, 1855 (Saros 145) |
 April 25, 1884 (Saros 146) |
 April 6, 1913 (Saros 147) |
 March 16, 1942 (Saros 148) |
 February 25, 1971 (Saros 149) |
 February 5, 2000 (Saros 150) |
 January 14, 2029 (Saros 151) |
 December 26, 2057 (Saros 152) |
 December 6, 2086 (Saros 153) |
 November 16, 2115 (Saros 154) |
 October 26, 2144 (Saros 155) |
 October 7, 2173 (Saros 156) |
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