Template:Solar Saros series 133
This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
Series members 34–55 occur between 1801 and 2200: | ||
---|---|---|
34 | 35 | 36 |
July 17, 1814 |
July 27, 1832 |
August 7, 1850 |
37 | 38 | 39 |
August 18, 1868 |
August 29, 1886 |
September 9, 1904 |
40 | 41 | 42 |
September 21, 1922 |
October 1, 1940 |
October 12, 1958 |
43 | 44 | 45 |
October 23, 1976 |
November 3, 1994 |
November 13, 2012 |
46 | 47 | 48 |
November 25, 2030 |
December 5, 2048 |
December 17, 2066 |
49 | 50 | 51 |
December 27, 2084 |
January 8, 2103 |
January 19, 2121 |
52 | 53 | 54 |
January 30, 2139 |
February 9, 2157 |
February 21, 2175 |
55 | ||
March 3, 2193 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.