Template:Solar Saros series 116
Appearance
This eclipse is a part of Saros series 116, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 23, 727 AD. It contains annular eclipses from October 10, 907 AD through May 6, 1845. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on July 22, 1971. 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 51 at 12 minutes, 2 seconds on December 25, 1628. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
Series members 61–70 occur between 1801 and 1971: | ||
---|---|---|
61 | 62 | 63 |
![]() April 14, 1809 |
![]() April 26, 1827 |
![]() May 6, 1845 |
64 | 65 | 66 |
![]() May 17, 1863 |
![]() May 27, 1881 |
![]() June 8, 1899 |
67 | 68 | 69 |
![]() June 19, 1917 |
![]() June 30, 1935 |
![]() July 11, 1953 |
70 | ||
![]() July 22, 1971 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 116". eclipse.gsfc.nasa.gov.