Template:Solar Tritos series 2000 February 5
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 2087 | ||||
---|---|---|---|---|
August 17, 1803 (Saros 132) |
July 17, 1814 (Saros 133) |
June 16, 1825 (Saros 134) |
May 15, 1836 (Saros 135) |
April 15, 1847 (Saros 136) |
March 15, 1858 (Saros 137) |
February 11, 1869 (Saros 138) |
January 11, 1880 (Saros 139) |
December 12, 1890 (Saros 140) |
November 11, 1901 (Saros 141) |
October 10, 1912 (Saros 142) |
September 10, 1923 (Saros 143) |
August 10, 1934 (Saros 144) |
July 9, 1945 (Saros 145) |
June 8, 1956 (Saros 146) |
May 9, 1967 (Saros 147) |
April 7, 1978 (Saros 148) |
March 7, 1989 (Saros 149) |
February 5, 2000 (Saros 150) |
January 4, 2011 (Saros 151) |
December 4, 2021 (Saros 152) |
November 3, 2032 (Saros 153) |
October 3, 2043 (Saros 154) |
September 2, 2054 (Saros 155) |
August 2, 2065 (Saros 156) |
July 1, 2076 (Saros 157) |
June 1, 2087 (Saros 158) |