| Solar eclipse of September 23, 2071 | |
|---|---|
|  Map | |
| Type of eclipse | |
| Nature | Total | 
| Gamma | 0.262 | 
| Magnitude | 1.0333 | 
| Maximum eclipse | |
| Duration | 191 sec (3 m 11 s) | 
| Coordinates | 14°12′N 76°42′W / 14.2°N 76.7°W | 
| Max. width of band | 116 km (72 mi) | 
| Times (UTC) | |
| Greatest eclipse | 17:20:28 | 
| References | |
| Saros | 145 (25 of 77) | 
| Catalog # (SE5000) | 9668 | 
A total solar eclipse will occur on Wednesday, September 23, 2071. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
Related eclipses
Solar eclipses 2069–2072
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.[1]
| 120 | April 21, 2069  Partial | 125 | October 15, 2069  Partial | 
| 130 | April 11, 2070  Total | 135 | October 4, 2070  Annular | 
| 140 | March 31, 2071  Annular | 145 | September 23, 2071  Total | 
| 150 | March 19, 2072  Partial | 155 | September 12, 2072  Total | 
Saros series 145
This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon's ascending node.
| Series members 10–32 occur between 1801 and 2359 | ||
|---|---|---|
| 10 | 11 | 12 | 
|  April 13, 1801 |  April 24, 1819 |  May 4, 1837 | 
| 13 | 14 | 15 | 
|  May 16, 1855 |  May 26, 1873 |  June 6, 1891 | 
| 16 | 17 | 18 | 
|  June 17, 1909 |  June 29, 1927 |  July 9, 1945 | 
| 19 | 20 | 21 | 
|  July 20, 1963 |  July 31, 1981 |  August 11, 1999 | 
| 22 | 23 | 24 | 
|  August 21, 2017 |  September 2, 2035 |  September 12, 2053 | 
| 25 | 26 | 27 | 
|  September 23, 2071 |  October 4, 2089 |  October 16, 2107 | 
| 28 | 29 | 30 | 
|  October 26, 2125 |  November 7, 2143 |  November 17, 2161 | 
| 31 | 32 | 33 | 
|  November 28, 2179 |  December 9, 2197 |  December 21, 2215 | 
| 34 | 35 | 36 | 
|  December 31, 2233 |  January 12, 2252 |  January 22, 2270 | 
| 37 | 38 | 39 | 
|  February 2, 2288 |  February 14, 2306 |  February 25, 2324 | 
| 40 | ||
|  March 8, 2342 | ||
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.
| Inex series members between 1901 and 2100: | ||
|---|---|---|
|  January 3, 1927 (Saros 140) |  December 14, 1955 (Saros 141) |  November 22, 1984 (Saros 142) | 
|  November 3, 2013 (Saros 143) |  October 14, 2042 (Saros 144) |  September 23, 2071 (Saros 145) | 
|  September 4, 2100 (Saros 146) | ||
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.
| 21 eclipse events, progressing from south to north between July 13, 2018, and July 12, 2094 | ||||
|---|---|---|---|---|
| July 12–13 | April 30-May 1 | February 16–17 | December 5–6 | September 22–23 | 
| 117 | 119 | 121 | 123 | 125 | 
|  July 13, 2018 |  April 30, 2022 |  February 17, 2026 |  December 5, 2029 |  September 23, 2033 | 
| 127 | 129 | 131 | 133 | 135 | 
|  July 13, 2037 |  April 30, 2041 |  February 16, 2045 |  December 5, 2048 |  September 22, 2052 | 
| 137 | 139 | 141 | 143 | 145 | 
|  July 12, 2056 |  April 30, 2060 |  February 17, 2064 |  December 6, 2067 |  September 23, 2071 | 
| 147 | 149 | 151 | 153 | 155 | 
|  July 13, 2075 |  May 1, 2079 |  February 16, 2083 |  December 6, 2086 |  September 23, 2090 | 
| 157 | ||||
|  July 12, 2094 | ||||
Notes
- ↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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