Template:Solar Saros series 156
Appearance
This eclipse is a part of Saros series 156, repeating every 18 years, 11 days, and containing 69 events. The series started with a partial solar eclipse on July 1, 2011. It contains annular eclipses from September 26, 2155 through April 7, 3075. There are no hybrid or total eclipses in this set. The series ends at member 69 as a partial eclipse on July 14, 3237. 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 29 at 8 minutes, 28 seconds on May 3, 2516. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
Series members 1–11 occur between 2011 and 2200: | ||
---|---|---|
1 | 2 | 3 |
July 1, 2011 |
July 11, 2029 |
July 22, 2047 |
4 | 5 | 6 |
August 2, 2065 |
August 13, 2083 |
August 24, 2101 |
7 | 8 | 9 |
September 5, 2119 |
September 15, 2137 |
September 26, 2155 |
10 | 11 | |
October 7, 2173 |
October 18, 2191 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 156". eclipse.gsfc.nasa.gov.