Solar eclipses of 2033–2036
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [3]
The partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.
Saros 155
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. [4]
| 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 |
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
| 20 eclipse events between June 10, 1964 and August 21, 2036 |
|---|
| June 10–11 | March 28–29 | January 14–16 | November 3 | August 21–22 |
|---|
| 117 | 119 | 121 | 123 | 125 |
|---|
June 10, 1964 | 
March 28, 1968 | 
January 16, 1972 | 
November 3, 1975 | 
August 22, 1979 |
| 127 | 129 | 131 | 133 | 135 |
|---|
June 11, 1983 | 
March 29, 1987 | 
January 15, 1991 | 
November 3, 1994 | 
August 22, 1998 |
| 137 | 139 | 141 | 143 | 145 |
|---|
June 10, 2002 | 
March 29, 2006 | 
January 15, 2010 | 
November 3, 2013 | 
August 21, 2017 |
| 147 | 149 | 151 | 153 | 155 |
|---|
June 10, 2021 | 
March 29, 2025 | 
January 14, 2029 | 
November 3, 2032 |
August 21, 2036 |
Tritos series
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
The partial solar eclipses on November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.
| Series members between 1801 and 2069 |
|---|
June 6, 1807
(Saros 134) | 
May 5, 1818
(Saros 135) | 
April 3, 1829
(Saros 136) | 
March 4, 1840
(Saros 137) | 
February 1, 1851
(Saros 138) |
December 31, 1861
(Saros 139) | 
November 30, 1872
(Saros 140) | 
October 30, 1883
(Saros 141) | 
September 29, 1894
(Saros 142) | 
August 30, 1905
(Saros 143) |
July 30, 1916
(Saros 144) | 
June 29, 1927
(Saros 145) | 
May 29, 1938
(Saros 146) | 
April 28, 1949
(Saros 147) | 
March 27, 1960
(Saros 148) |
February 25, 1971
(Saros 149) | 
January 25, 1982
(Saros 150) | 
December 24, 1992
(Saros 151) | 
November 23, 2003
(Saros 152) | 
October 23, 2014
(Saros 153) |
September 21, 2025
(Saros 154) |
August 21, 2036
(Saros 155) | 
July 22, 2047
(Saros 156) | 
June 21, 2058
(Saros 157) | 
May 20, 2069
(Saros 158) |
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 |
|---|
January 30, 1805
(Saros 147) | 
January 9, 1834
(Saros 148) | 
December 21, 1862
(Saros 149) |
December 1, 1891
(Saros 150) | 
November 10, 1920
(Saros 151) | 
October 21, 1949
(Saros 152) |
October 2, 1978
(Saros 153) | 
September 11, 2007
(Saros 154) |
August 21, 2036
(Saros 155) |
August 2, 2065
(Saros 156) | 
July 12, 2094
(Saros 157) | 
June 23, 2123
(Saros 158) |
June 3, 2152
(Saros 159) | 
May 13, 2181
(Saros 160) | |
This page is based on this
Wikipedia article Text is available under the
CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.
