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 | ||
|---|---|---|
 September 28, 1829 (Saros 141) |
 September 7, 1858 (Saros 142) |
 August 19, 1887 (Saros 143) |
 July 30, 1916 (Saros 144) |
 July 9, 1945 (Saros 145) |
 June 20, 1974 (Saros 146) |
 May 31, 2003 (Saros 147) |
 May 9, 2032 (Saros 148) |
 April 20, 2061 (Saros 149) |
 March 31, 2090 (Saros 150) |
 March 11, 2119 (Saros 151) |
 February 19, 2148 (Saros 152) |
 January 29, 2177 (Saros 153) |
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