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 | ||
|---|---|---|
 April 14, 1828 (Saros 126) |
 March 25, 1857 (Saros 127) |
 March 5, 1886 (Saros 128) |
 February 14, 1915 (Saros 129) |
 January 25, 1944 (Saros 130) |
 January 4, 1973 (Saros 131) |
 December 14, 2001 (Saros 132) |
 November 25, 2030 (Saros 133) |
 November 5, 2059 (Saros 134) |
 October 14, 2088 (Saros 135) |
 September 26, 2117 (Saros 136) |
 September 6, 2146 (Saros 137) |
 August 16, 2175 (Saros 138) |
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