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.
The partial solar eclipse on November 4, 2116 (part of Saros 164) is also a part of this series but is not included in the table below.
| Series members between 1801 and 2029 | ||||
|---|---|---|---|---|
 March 24, 1811 (Saros 136) |
 February 21, 1822 (Saros 137) |
 January 20, 1833 (Saros 138) |
 December 21, 1843 (Saros 139) |
 November 20, 1854 (Saros 140) |
 October 19, 1865 (Saros 141) |
 September 17, 1876 (Saros 142) |
 August 19, 1887 (Saros 143) |
 July 18, 1898 (Saros 144) |
 June 17, 1909 (Saros 145) |
 May 18, 1920 (Saros 146) |
 April 18, 1931 (Saros 147) |
 March 16, 1942 (Saros 148) |
 February 14, 1953 (Saros 149) |
 January 14, 1964 (Saros 150) |
 December 13, 1974 (Saros 151) |
 November 12, 1985 (Saros 152) |
 October 12, 1996 (Saros 153) |
 September 11, 2007 (Saros 154) |
 August 11, 2018 (Saros 155) |
 July 11, 2029 (Saros 156) | ||||