Solar eclipse of November 5, 2059 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.4454 |
Magnitude | 0.9417 |
Maximum eclipse | |
Duration | 420 s (7 min 0 s) |
Coordinates | 8°42′N47°06′E / 8.7°N 47.1°E |
Max. width of band | 238 km (148 mi) |
Times (UTC) | |
Greatest eclipse | 9:18:15 |
References | |
Saros | 134 (46 of 71) |
Catalog # (SE5000) | 9641 |
An annular solar eclipse will occur on Wednesday, November 5, 2059. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The Sun will be 94% covered in a moderate annular eclipse, lasting 7 minutes exactly and covering a broad path up to 238 km wide.
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]
Solar eclipses 2059 to 2061 | |||||
---|---|---|---|---|---|
119 | May 22, 2058 Partial | 124 | November 16, 2058 Partial | ||
129 | May 11, 2059 Total | 134 | November 5, 2059 Annular | ||
139 | April 30, 2060 Total | 144 | October 24, 2060 Annular | ||
149 | April 20, 2061 Total | 154 | October 13, 2061 Annular |
It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428. All eclipses in this series occur at the Moon’s descending node. [2]
Series members 32–48 occur between 1801 and 2100: | ||
---|---|---|
32 | 33 | 34 |
June 6, 1807 | June 16, 1825 | June 27, 1843 |
35 | 36 | 37 |
July 8, 1861 | July 19, 1879 | July 29, 1897 |
38 | 39 | 40 |
August 10, 1915 | August 21, 1933 | September 1, 1951 |
41 | 42 | 43 |
September 11, 1969 | September 23, 1987 | October 3, 2005 |
44 | 45 | 46 |
October 14, 2023 | October 25, 2041 | November 5, 2059 |
47 | 48 | |
November 15, 2077 | November 27, 2095 |
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).
21 eclipse events between June 12, 2029 and June 12, 2105 | ||||
---|---|---|---|---|
June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
118 | 120 | 122 | 124 | 126 |
June 12, 2029 | March 30, 2033 | January 16, 2037 | November 4, 2040 | August 23, 2044 |
128 | 130 | 132 | 134 | 136 |
June 11, 2048 | March 30, 2052 | January 16, 2056 | November 5, 2059 | August 24, 2063 |
138 | 140 | 142 | 144 | 146 |
June 11, 2067 | March 31, 2071 | January 16, 2075 | November 4, 2078 | August 24, 2082 |
148 | 150 | 152 | 154 | |
June 11, 2086 | March 31, 2090 | January 16, 2094 | November 4, 2097 |
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