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 | ||
|---|---|---|
 September 17, 1811 (Saros 141) |
 August 27, 1840 (Saros 142) |
 August 7, 1869 (Saros 143) |
 July 18, 1898 (Saros 144) |
 June 29, 1927 (Saros 145) |
 June 8, 1956 (Saros 146) |
 May 19, 1985 (Saros 147) |
 April 29, 2014 (Saros 148) |
 April 9, 2043 (Saros 149) |
 March 19, 2072 (Saros 150) |
 February 28, 2101 (Saros 151) |
 February 8, 2130 (Saros 152) |
 January 19, 2159 (Saros 153) |
 December 29, 2187 (Saros 154) |
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