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 | ||
|---|---|---|
 October 29, 1818 (Saros 140) |
 October 9, 1847 (Saros 141) |
 September 17, 1876 (Saros 142) |
 August 30, 1905 (Saros 143) |
 August 10, 1934 (Saros 144) |
 July 20, 1963 (Saros 145) |
 June 30, 1992 (Saros 146) |
 June 10, 2021 (Saros 147) |
 May 20, 2050 (Saros 148) |
 May 1, 2079 (Saros 149) |
 April 11, 2108 (Saros 150) |
 March 21, 2137 (Saros 151) |
 March 2, 2166 (Saros 152) |
 February 10, 2195 (Saros 153) |
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