Template:Solar Tritos series 2008 February 7
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 1866 and 2200 | ||||
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March 16, 1866 (Saros 108) |
December 13, 1898 (Saros 111) |
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September 12, 1931 (Saros 114) |
August 12, 1942 (Saros 115) |
July 11, 1953 (Saros 116) |
June 10, 1964 (Saros 117) | |
May 11, 1975 (Saros 118) |
April 9, 1986 (Saros 119) |
March 9, 1997 (Saros 120) |
February 7, 2008 (Saros 121) |
January 6, 2019 (Saros 122) |
December 5, 2029 (Saros 123) |
November 4, 2040 (Saros 124) |
October 4, 2051 (Saros 125) |
September 3, 2062 (Saros 126) |
August 3, 2073 (Saros 127) |
July 3, 2084 (Saros 128) |
June 2, 2095 (Saros 129) |
May 3, 2106 (Saros 130) |
April 2, 2117 (Saros 131) |
March 1, 2128 (Saros 132) |
January 30, 2139 (Saros 133) |
December 30, 2149 (Saros 134) |
November 27, 2160 (Saros 135) |
October 29, 2171 (Saros 136) |
September 27, 2182 (Saros 137) |
August 26, 2193 (Saros 138) |