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 | ||
|---|---|---|
 December 9, 1825 (Saros 139) |
 November 20, 1854 (Saros 140) |
 October 30, 1883 (Saros 141) |
 October 10, 1912 (Saros 142) |
 September 21, 1941 (Saros 143) |
 August 31, 1970 (Saros 144) |
 August 11, 1999 (Saros 145) |
 July 22, 2028 (Saros 146) |
 July 1, 2057 (Saros 147) |
 June 11, 2086 (Saros 148) |
 May 24, 2115 (Saros 149) |
 May 3, 2144 (Saros 150) |
 April 12, 2173 (Saros 151) |
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