This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||||
|---|---|---|---|---|
 October 9, 1809 (Saros 121) |
 September 7, 1820 (Saros 122) |
 August 7, 1831 (Saros 123) |
 July 8, 1842 (Saros 124) |
 June 6, 1853 (Saros 125) |
 May 6, 1864 (Saros 126) |
 April 6, 1875 (Saros 127) |
 March 5, 1886 (Saros 128) |
 February 1, 1897 (Saros 129) |
 January 3, 1908 (Saros 130) |
 December 3, 1918 (Saros 131) |
 November 1, 1929 (Saros 132) |
 October 1, 1940 (Saros 133) |
 September 1, 1951 (Saros 134) |
 July 31, 1962 (Saros 135) |
 June 30, 1973 (Saros 136) |
 May 30, 1984 (Saros 137) |
 April 29, 1995 (Saros 138) |
 March 29, 2006 (Saros 139) |
 February 26, 2017 (Saros 140) |
 January 26, 2028 (Saros 141) |
 December 26, 2038 (Saros 142) |
 November 25, 2049 (Saros 143) |
 October 24, 2060 (Saros 144) |
 September 23, 2071 (Saros 145) |
 August 24, 2082 (Saros 146) |
 July 23, 2093 (Saros 147) |
 June 22, 2104 (Saros 148) |
 May 24, 2115 (Saros 149) |
 April 22, 2126 (Saros 150) |
 March 21, 2137 (Saros 151) |
 February 19, 2148 (Saros 152) |
 January 19, 2159 (Saros 153) |
 December 18, 2169 (Saros 154) |
 November 17, 2180 (Saros 155) |
 October 18, 2191 (Saros 156) | ||||