Template:Solar Tritos series 2000 July 31
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.
The partial solar eclipse on October 24, 2098 (part of Saros 164) is also a part of this series but is not included in the table below.
Series members between 1801 and 2011 | ||||
---|---|---|---|---|
February 11, 1804 (Saros 137) |
January 10, 1815 (Saros 138) |
December 9, 1825 (Saros 139) |
November 9, 1836 (Saros 140) |
October 9, 1847 (Saros 141) |
September 7, 1858 (Saros 142) |
August 7, 1869 (Saros 143) |
July 7, 1880 (Saros 144) |
June 6, 1891 (Saros 145) |
May 7, 1902 (Saros 146) |
April 6, 1913 (Saros 147) |
March 5, 1924 (Saros 148) |
February 3, 1935 (Saros 149) |
January 3, 1946 (Saros 150) |
December 2, 1956 (Saros 151) |
November 2, 1967 (Saros 152) |
October 2, 1978 (Saros 153) |
August 31, 1989 (Saros 154) |
July 31, 2000 (Saros 155) |
July 1, 2011 (Saros 156) |