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 | |||||
|---|---|---|---|---|---|
| 1811 Sep 02 (Saros 115) |
1840 Aug 13 (Saros 116) |
1869 Jul 23 (Saros 117) | |||
| 1898 Jul 03 (Saros 118) |
1927 Jun 15 (Saros 119) |
1956 May 24 (Saros 120) | |||
|
|
|
| ||
| 1985 May 04 (Saros 121) |
2014 Apr 15 (Saros 122) |
2043 Mar 25 (Saros 123) | |||
|
|
|
|
|
|
| 2072 Mar 04 (Saros 124) |
2101 Feb 14 (Saros 125) |
2130 Jan 24 (Saros 126) | |||
| 2159 Jan 04 (Saros 127) |
2187 Dec 15 (Saros 128) | ||||