This eclipse is a part of Saros series 155, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 17, 1928. It contains total eclipses from September 12, 2072 through August 30, 2649; hybrid eclipses from September 10, 2667 through October 2, 2703; and annular eclipses from October 13, 2721 through May 8, 3064. The series ends at member 71 as a partial eclipse on July 24, 3190. 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 totality will be produced by member 14 at 4 minutes, 5 seconds on November 6, 2162, and the longest duration of annularity will be produced by member 63 at 5 minutes, 31 seconds on April 28, 3046. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 1–16 occur between 1928 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
 June 17, 1928 |
 June 29, 1946 |
 July 9, 1964 |
| 4 | 5 | 6 |
 July 20, 1982 |
 July 31, 2000 |
 August 11, 2018 |
| 7 | 8 | 9 |
 August 21, 2036 |
 September 2, 2054 |
 September 12, 2072 |
| 10 | 11 | 12 |
 September 23, 2090 |
 October 5, 2108 |
 October 16, 2126 |
| 13 | 14 | 15 |
 October 26, 2144 |
 November 7, 2162 |
 November 17, 2180 |
| 16 | ||
 November 28, 2198 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 155". eclipse.gsfc.nasa.gov.