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 | ||
|---|---|---|
 May 27, 1816 (Saros 115) |
 May 6, 1845 (Saros 116) |
 April 16, 1874 (Saros 117) |
 March 29, 1903 (Saros 118) |
 March 7, 1932 (Saros 119) |
 February 15, 1961 (Saros 120) |
 January 26, 1990 (Saros 121) |
 January 6, 2019 (Saros 122) |
 December 16, 2047 (Saros 123) |
 November 26, 2076 (Saros 124) |
 November 6, 2105 (Saros 125) |
 October 17, 2134 (Saros 126) |
 September 28, 2163 (Saros 127) |
 September 6, 2192 (Saros 128) |
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