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 | ||
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![]() October 9, 1809 (Saros 121) |
![]() September 18, 1838 (Saros 122) |
![]() August 29, 1867 (Saros 123) |
![]() August 9, 1896 (Saros 124) |
![]() July 20, 1925 (Saros 125) |
![]() June 30, 1954 (Saros 126) |
![]() June 11, 1983 (Saros 127) |
![]() May 20, 2012 (Saros 128) |
![]() April 30, 2041 (Saros 129) |
![]() April 11, 2070 (Saros 130) |
![]() March 21, 2099 (Saros 131) |
![]() March 1, 2128 (Saros 132) |
![]() February 9, 2157 (Saros 133) |
![]() January 20, 2186 (Saros 134) |