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 | ||
|---|---|---|
 June 6, 1807 (Saros 134) |
 May 15, 1836 (Saros 135) |
 April 25, 1865 (Saros 136) |
 April 6, 1894 (Saros 137) |
 March 17, 1923 (Saros 138) |
 February 25, 1952 (Saros 139) |
 February 4, 1981 (Saros 140) |
 January 15, 2010 (Saros 141) |
 December 26, 2038 (Saros 142) |
 December 6, 2067 (Saros 143) |
 November 15, 2096 (Saros 144) |
 October 26, 2125 (Saros 145) |
 October 7, 2154 (Saros 146) |
 September 16, 2183 (Saros 147) |
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