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 | ||
|---|---|---|
 August 5, 1804 (Saros 142) |
 July 17, 1833 (Saros 143) |
 June 27, 1862 (Saros 144) |
 June 6, 1891 (Saros 145) |
 May 18, 1920 (Saros 146) |
 April 28, 1949 (Saros 147) |
 April 7, 1978 (Saros 148) |
 March 19, 2007 (Saros 149) |
 February 27, 2036 (Saros 150) |
 February 5, 2065 (Saros 151) |
 January 16, 2094 (Saros 152) |
 December 28, 2122 (Saros 153) |
 December 8, 2151 (Saros 154) |
 November 17, 2180 (Saros 155) |
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