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 | ||
|---|---|---|
 February 21, 1803 (Saros 127) |
 February 1, 1832 (Saros 128) |
 January 11, 1861 (Saros 129) |
 December 22, 1889 (Saros 130) |
 December 3, 1918 (Saros 131) |
 November 12, 1947 (Saros 132) |
 October 23, 1976 (Saros 133) |
 October 3, 2005 (Saros 134) |
 September 12, 2034 (Saros 135) |
 August 24, 2063 (Saros 136) |
 August 3, 2092 (Saros 137) |
 July 14, 2121 (Saros 138) |
 June 25, 2150 (Saros 139) |
 June 5, 2179 (Saros 140) |
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