Template:Solar Saros series 147
Appearance
This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 will be produced by member 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
Series members 11–32 occur between 1801 and 2200: | ||
---|---|---|
11 | 12 | 13 |
January 30, 1805 |
February 11, 1823 |
February 21, 1841 |
14 | 15 | 16 |
March 4, 1859 |
March 15, 1877 |
March 26, 1895 |
17 | 18 | 19 |
April 6, 1913 |
April 18, 1931 |
April 28, 1949 |
20 | 21 | 22 |
May 9, 1967 |
May 19, 1985 |
May 31, 2003 |
23 | 24 | 25 |
June 10, 2021 |
June 21, 2039 |
July 1, 2057 |
26 | 27 | 28 |
July 13, 2075 |
July 23, 2093 |
August 4, 2111 |
29 | 30 | 31 |
August 15, 2129 |
August 26, 2147 |
September 5, 2165 |
32 | ||
September 16, 2183 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 147". eclipse.gsfc.nasa.gov.