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 | ||
|---|---|---|
 June 16, 1806 (Saros 124) |
 May 27, 1835 (Saros 125) |
 May 6, 1864 (Saros 126) |
 April 16, 1893 (Saros 127) |
 March 28, 1922 (Saros 128) |
 March 7, 1951 (Saros 129) |
 February 16, 1980 (Saros 130) |
 January 26, 2009 (Saros 131) |
 January 5, 2038 (Saros 132) |
 December 17, 2066 (Saros 133) |
 November 27, 2095 (Saros 134) |
 November 6, 2124 (Saros 135) |
 October 17, 2153 (Saros 136) |
 September 27, 2182 (Saros 137) |
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