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 19, 1808 (Saros 111) |
 September 19, 1819 (Saros 112) |
 August 18, 1830 (Saros 113) |
 July 18, 1841 (Saros 114) |
 June 17, 1852 (Saros 115) |
 May 17, 1863 (Saros 116) |
 April 16, 1874 (Saros 117) |
 March 16, 1885 (Saros 118) |
 February 13, 1896 (Saros 119) |
 January 14, 1907 (Saros 120) |
 December 14, 1917 (Saros 121) |
 November 12, 1928 (Saros 122) |
 October 12, 1939 (Saros 123) |
 September 12, 1950 (Saros 124) |
 August 11, 1961 (Saros 125) |
 July 10, 1972 (Saros 126) |
 June 11, 1983 (Saros 127) |
 May 10, 1994 (Saros 128) |
 April 8, 2005 (Saros 129) |
 March 9, 2016 (Saros 130) |
 February 6, 2027 (Saros 131) |
 January 5, 2038 (Saros 132) |
 December 5, 2048 (Saros 133) |
 November 5, 2059 (Saros 134) |
 October 4, 2070 (Saros 135) |
 September 3, 2081 (Saros 136) |
 August 3, 2092 (Saros 137) |
 July 4, 2103 (Saros 138) |
 June 3, 2114 (Saros 139) |
 May 3, 2125 (Saros 140) |
 April 1, 2136 (Saros 141) |
 March 2, 2147 (Saros 142) |
 January 30, 2158 (Saros 143) |
 December 29, 2168 (Saros 144) |
 November 28, 2179 (Saros 145) |
 October 29, 2190 (Saros 146) | ||||