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 17, 1803 (Saros 132) |
 July 27, 1832 (Saros 133) |
 July 8, 1861 (Saros 134) |
 June 17, 1890 (Saros 135) |
 May 29, 1919 (Saros 136) |
 May 9, 1948 (Saros 137) |
 April 18, 1977 (Saros 138) |
 March 29, 2006 (Saros 139) |
 March 9, 2035 (Saros 140) |
 February 17, 2064 (Saros 141) |
 January 27, 2093 (Saros 142) |
 January 8, 2122 (Saros 143) |
 December 19, 2150 (Saros 144) |
 November 28, 2179 (Saros 145) |
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