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 11, 1804 (Saros 137) |
 January 20, 1833 (Saros 138) |
 December 31, 1861 (Saros 139) |
 December 12, 1890 (Saros 140) |
 November 22, 1919 (Saros 141) |
 November 1, 1948 (Saros 142) |
 October 12, 1977 (Saros 143) |
 September 22, 2006 (Saros 144) |
 September 2, 2035 (Saros 145) |
 August 12, 2064 (Saros 146) |
 July 23, 2093 (Saros 147) |
 July 4, 2122 (Saros 148) |
 June 14, 2151 (Saros 149) |
 May 24, 2180 (Saros 150) |
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