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.
Series members between 1801 and 2200 | ||||
---|---|---|---|---|
March 14, 1801 (Saros 107) |
February 12, 1812 (Saros 108) |
January 12, 1823 (Saros 109) |
November 10, 1844 (Saros 111) | |
August 9, 1877 (Saros 114) |
July 9, 1888 (Saros 115) |
June 8, 1899 (Saros 116) | ||
May 9, 1910 (Saros 117) |
April 8, 1921 (Saros 118) |
March 7, 1932 (Saros 119) |
February 4, 1943 (Saros 120) |
January 5, 1954 (Saros 121) |
December 4, 1964 (Saros 122) |
November 3, 1975 (Saros 123) |
October 3, 1986 (Saros 124) |
September 2, 1997 (Saros 125) |
August 1, 2008 (Saros 126) |
July 2, 2019 (Saros 127) |
June 1, 2030 (Saros 128) |
April 30, 2041 (Saros 129) |
March 30, 2052 (Saros 130) |
February 28, 2063 (Saros 131) |
January 27, 2074 (Saros 132) |
December 27, 2084 (Saros 133) |
November 27, 2095 (Saros 134) |
October 26, 2106 (Saros 135) |
September 26, 2117 (Saros 136) |
August 25, 2128 (Saros 137) |
July 25, 2139 (Saros 138) |
June 25, 2150 (Saros 139) |
May 25, 2161 (Saros 140) |
April 23, 2172 (Saros 141) |
March 23, 2183 (Saros 142) |
February 21, 2194 (Saros 143) |