Solar eclipses of 2062–2065
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 eclipses on July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.
Saros 121
This eclipse is a part of Saros series 121, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 25, 944 AD. It contains total eclipses from July 10, 1070 through October 9, 1809; hybrid eclipses on October 20, 1827 and October 30, 1845; and annular eclipses from November 11, 1863 through February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. 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 was produced by member 39 at 6 minutes, 20 seconds on June 21, 1629, and the longest duration of annularity will be produced by member 62 at 2 minutes, 27 seconds on February 28, 2044. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]
| Series members 49–70 occur between 1801 and 2200: |
|---|
| 49 | 50 | 51 |
|---|
October 9, 1809 | 
October 20, 1827 | 
October 30, 1845 |
| 52 | 53 | 54 |
|---|
November 11, 1863 | 
November 21, 1881 | 
December 3, 1899 |
| 55 | 56 | 57 |
|---|
December 14, 1917 | 
December 25, 1935 | 
January 5, 1954 |
| 58 | 59 | 60 |
|---|
January 16, 1972 | 
January 26, 1990 | 
February 7, 2008 |
| 61 | 62 | 63 |
|---|
February 17, 2026 | 
February 28, 2044 | 
March 11, 2062 |
| 64 | 65 | 66 |
|---|
March 21, 2080 | 
April 1, 2098 | 
April 13, 2116 |
| 67 | 68 | 69 |
|---|
April 24, 2134 | 
May 4, 2152 | 
May 16, 2170 |
| 70 |
|---|
May 26, 2188 |
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.
| 23 eclipse events between August 3, 2054 and October 16, 2145 |
|---|
| August 3–4 | May 22–24 | March 10–11 | December 27–29 | October 14–16 |
|---|
| 117 | 119 | 121 | 123 | 125 |
|---|
August 3, 2054 | 
May 22, 2058 |
March 11, 2062 | 
December 27, 2065 | 
October 15, 2069 |
| 127 | 129 | 131 | 133 | 135 |
|---|
August 3, 2073 | 
May 22, 2077 | 
March 10, 2081 | 
December 27, 2084 | 
October 14, 2088 |
| 137 | 139 | 141 | 143 | 145 |
|---|
August 3, 2092 | 
May 22, 2096 | 
March 10, 2100 | 
December 29, 2103 | 
October 16, 2107 |
| 147 | 149 | 151 | 153 | 155 |
|---|
August 4, 2111 | 
May 24, 2115 | 
March 11, 2119 | 
December 28, 2122 | 
October 16, 2126 |
| 157 | 159 | 161 | 163 | 165 |
|---|
August 4, 2130 | 
May 23, 2134 | | | 
October 16, 2145 |
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.
| Series members between 2018 and 2200 |
|---|
July 13, 2018
(Saros 117) | 
June 12, 2029
(Saros 118) | 
May 11, 2040
(Saros 119) | 
April 11, 2051
(Saros 120) |
March 11, 2062
(Saros 121) |
February 7, 2073
(Saros 122) | 
January 7, 2084
(Saros 123) | 
December 7, 2094
(Saros 124) | 
November 6, 2105
(Saros 125) | 
October 6, 2116
(Saros 126) |
September 6, 2127
(Saros 127) | 
August 5, 2138
(Saros 128) | 
July 5, 2149
(Saros 129) | 
June 4, 2160
(Saros 130) | 
May 5, 2171
(Saros 131) |
April 3, 2182
(Saros 132) | 
March 3, 2193
(Saros 133) |
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 |
|---|
September 8, 1801
(Saros 112) | 
August 18, 1830
(Saros 113) | 
July 29, 1859
(Saros 114) |
July 9, 1888
(Saros 115) | 
June 19, 1917
(Saros 116) | 
May 30, 1946
(Saros 117) |
May 11, 1975
(Saros 118) | 
April 19, 2004
(Saros 119) | 
March 30, 2033
(Saros 120) |
March 11, 2062
(Saros 121) | 
February 18, 2091
(Saros 122) | 
January 30, 2120
(Saros 123) |
January 9, 2149
(Saros 124) | 
December 20, 2177
(Saros 125) | |
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