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 | |||||
|---|---|---|---|---|---|
| 1825 Jan 04 (Saros 141) |
1853 Dec 15 (Saros 142) |
1882 Nov 25 (Saros 143) | |||
| 1911 Nov 06 (Saros 144) |
1940 Oct 16 (Saros 145) |
1969 Sep 25 (Saros 146) | |||
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| 1998 Sep 06 (Saros 147) |
2027 Aug 17 (Saros 148) |
2056 Jul 26 (Saros 149) | |||
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| 2085 Jul 07 (Saros 150) |
2114 Jun 18 (Saros 151) |
2143 May 28 (Saros 152) | |||
| 2172 May 08 (Saros 153) | |||||