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 | ||
|---|---|---|
 September 19, 1819 (Saros 112) |
 August 28, 1848 (Saros 113) |
 August 9, 1877 (Saros 114) |
 July 21, 1906 (Saros 115) |
 June 30, 1935 (Saros 116) |
 June 10, 1964 (Saros 117) |
 May 21, 1993 (Saros 118) |
 April 30, 2022 (Saros 119) |
 April 11, 2051 (Saros 120) |
 March 21, 2080 (Saros 121) |
 March 1, 2109 (Saros 122) |
 February 9, 2138 (Saros 123) |
 January 21, 2167 (Saros 124) |
 December 31, 2195 (Saros 125) |
|
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 | ||
|---|---|---|
|
September 19, 1819 (Saros 112) |
August 28, 1848 (Saros 113) |
August 9, 1877 (Saros 114) |
|
July 21, 1906 (Saros 115) |
June 30, 1935 (Saros 116) |
June 10, 1964 (Saros 117) |
|
May 21, 1993 (Saros 118) |
April 30, 2022 (Saros 119) |
April 11, 2051 (Saros 120) |
|
March 21, 2080 (Saros 121) |
March 1, 2109 (Saros 122) |
February 9, 2138 (Saros 123) |
|
January 21, 2167 (Saros 124) |
December 31, 2195 (Saros 125) |
|