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 31, 1826 (Saros 111) |
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 August 31, 1913 (Saros 114) |
 August 12, 1942 (Saros 115) |
 July 22, 1971 (Saros 116) |
 July 1, 2000 (Saros 117) |
 June 12, 2029 (Saros 118) |
 May 22, 2058 (Saros 119) |
 May 2, 2087 (Saros 120) |
 April 13, 2116 (Saros 121) |
 March 23, 2145 (Saros 122) |
 March 3, 2174 (Saros 123) |
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