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 16, 1817 (Saros 125) |
 April 25, 1846 (Saros 126) |
 April 6, 1875 (Saros 127) |
 March 17, 1904 (Saros 128) |
 February 24, 1933 (Saros 129) |
 February 5, 1962 (Saros 130) |
 January 15, 1991 (Saros 131) |
 December 26, 2019 (Saros 132) |
 December 5, 2048 (Saros 133) |
 November 15, 2077 (Saros 134) |
 October 26, 2106 (Saros 135) |
 October 7, 2135 (Saros 136) |
 September 16, 2164 (Saros 137) |
 August 26, 2193 (Saros 138) |
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