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 | ||
|---|---|---|
 January 1, 1824 (Saros 119) |
 December 11, 1852 (Saros 120) |
 November 21, 1881 (Saros 121) |
 November 2, 1910 (Saros 122) |
 October 12, 1939 (Saros 123) |
 September 22, 1968 (Saros 124) |
 September 2, 1997 (Saros 125) |
 August 12, 2026 (Saros 126) |
 July 24, 2055 (Saros 127) |
 July 3, 2084 (Saros 128) |
 June 13, 2113 (Saros 129) |
 May 25, 2142 (Saros 130) |
 May 5, 2171 (Saros 131) |
 April 14, 2200 (Saros 132) |
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