Template:Solar Tritos series 2004 October 14
Appearance
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 25, 1819 (Saros 107) |
February 23, 1830 (Saros 108) |
January 22, 1841 (Saros 109) |
November 21, 1862 (Saros 111) | |
August 20, 1895 (Saros 114) |
July 21, 1906 (Saros 115) |
June 19, 1917 (Saros 116) | ||
May 19, 1928 (Saros 117) |
April 19, 1939 (Saros 118) |
March 18, 1950 (Saros 119) |
February 15, 1961 (Saros 120) |
January 16, 1972 (Saros 121) |
December 15, 1982 (Saros 122) |
November 13, 1993 (Saros 123) |
October 14, 2004 (Saros 124) |
September 13, 2015 (Saros 125) |
August 12, 2026 (Saros 126) |
July 13, 2037 (Saros 127) |
June 11, 2048 (Saros 128) |
May 11, 2059 (Saros 129) |
April 11, 2070 (Saros 130) |
March 10, 2081 (Saros 131) |
February 7, 2092 (Saros 132) |
January 8, 2103 (Saros 133) |
December 8, 2113 (Saros 134) |
November 6, 2124 (Saros 135) |
October 7, 2135 (Saros 136) |
September 6, 2146 (Saros 137) |
August 5, 2157 (Saros 138) |
July 5, 2168 (Saros 139) |
June 5, 2179 (Saros 140) |
May 4, 2190 (Saros 141) |