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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![]() December 10, 1806 (Saros 129) |
![]() November 20, 1835 (Saros 130) |
![]() October 30, 1864 (Saros 131) |
![]() October 9, 1893 (Saros 132) |
![]() September 21, 1922 (Saros 133) |
![]() September 1, 1951 (Saros 134) |
![]() August 10, 1980 (Saros 135) |
![]() July 22, 2009 (Saros 136) |
![]() July 2, 2038 (Saros 137) |
![]() June 11, 2067 (Saros 138) |
![]() May 22, 2096 (Saros 139) |
![]() May 3, 2125 (Saros 140) |
![]() April 12, 2154 (Saros 141) |
![]() March 23, 2183 (Saros 142) |