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 eclipses on April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.
| Series members between 2000 and 2200 | ||||
|---|---|---|---|---|
 July 1, 2000 (Saros 117) |
 June 1, 2011 (Saros 118) |
 April 30, 2022 (Saros 119) |
 March 30, 2033 (Saros 120) |
 February 28, 2044 (Saros 121) |
 January 27, 2055 (Saros 122) |
 December 27, 2065 (Saros 123) |
 November 26, 2076 (Saros 124) |
 October 26, 2087 (Saros 125) |
 September 25, 2098 (Saros 126) |
 August 26, 2109 (Saros 127) |
 July 25, 2120 (Saros 128) |
 June 25, 2131 (Saros 129) |
 May 25, 2142 (Saros 130) |
 April 23, 2153 (Saros 131) |
 March 23, 2164 (Saros 132) |
 February 21, 2175 (Saros 133) |
 January 20, 2186 (Saros 134) |
 December 19, 2196 (Saros 135) | |