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 | ||
|---|---|---|
 November 19, 1816 (Saros 120) |
 October 30, 1845 (Saros 121) |
 October 10, 1874 (Saros 122) |
 September 21, 1903 (Saros 123) |
 August 31, 1932 (Saros 124) |
 August 11, 1961 (Saros 125) |
 July 22, 1990 (Saros 126) |
 July 2, 2019 (Saros 127) |
 June 11, 2048 (Saros 128) |
 May 22, 2077 (Saros 129) |
 May 3, 2106 (Saros 130) |
 April 13, 2135 (Saros 131) |
 March 23, 2164 (Saros 132) |
 March 3, 2193 (Saros 133) |
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