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 | |||||
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| 1810 Apr 19 (Saros 138) |
1839 Mar 30 (Saros 139) |
1868 Mar 08 (Saros 140) | |||
| 1897 Feb 17 (Saros 141) |
1926 Jan 28 (Saros 142) |
1955 Jan 08 (Saros 143) | |||
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| 1983 Dec 20 (Saros 144) |
2012 Nov 28 (Saros 145) |
2041 Nov 08 (Saros 146) | |||
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| 2070 Oct 19 (Saros 147) |
2099 Sep 29 (Saros 148) |
2128 Sep 09 (Saros 149) | |||
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| 2157 Aug 20 (Saros 150) |
2186 Jul 31 (Saros 151) | ||||