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 9, 1828 (Saros 131) |
 September 18, 1857 (Saros 132) |
 August 29, 1886 (Saros 133) |
 August 10, 1915 (Saros 134) |
 July 20, 1944 (Saros 135) |
 June 30, 1973 (Saros 136) |
 June 10, 2002 (Saros 137) |
 May 21, 2031 (Saros 138) |
 April 30, 2060 (Saros 139) |
 April 10, 2089 (Saros 140) |
 March 22, 2118 (Saros 141) |
 March 2, 2147 (Saros 142) |
 February 10, 2176 (Saros 143) |
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