Solar eclipse of November 26, 2076 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.1401 |
Magnitude | 0.7315 |
Maximum eclipse | |
Coordinates | 63°42′N40°06′E / 63.7°N 40.1°E |
Times (UTC) | |
Greatest eclipse | 11:43:01 |
References | |
Saros | 124 (58 of 73) |
Catalog # (SE5000) | 9680 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Thursday, November 26, 2076, with a magnitude of 0.7315. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
This will be the last of four solar eclipses in 2076, with the others occurring on January 6, June 1, and July 1.
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]
The partial solar eclipses on January 6, 2076 and July 1, 2076 occur in the previous lunar year eclipse set.
Solar eclipse series sets from 2076 to 2079 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | June 1, 2076 ![]() Partial | −1.3897 | 124 | November 26, 2076 ![]() Partial | 1.1401 | |
129 | May 22, 2077 ![]() Total | −0.5725 | 134 | November 15, 2077 ![]() Annular | 0.4705 | |
139 | May 11, 2078 ![]() Total | 0.1838 | 144 | November 4, 2078 ![]() Annular | −0.2285 | |
149 | May 1, 2079 ![]() Total | 0.9081 | 154 | October 24, 2079 ![]() Annular | −0.9243 |
This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit. [2]
Series members 43–64 occur between 1801 and 2200: | ||
---|---|---|
43 | 44 | 45 |
![]() June 16, 1806 | ![]() June 26, 1824 | ![]() July 8, 1842 |
46 | 47 | 48 |
![]() July 18, 1860 | ![]() July 29, 1878 | ![]() August 9, 1896 |
49 | 50 | 51 |
![]() August 21, 1914 | ![]() August 31, 1932 | ![]() September 12, 1950 |
52 | 53 | 54 |
![]() September 22, 1968 | ![]() October 3, 1986 | ![]() October 14, 2004 |
55 | 56 | 57 |
![]() October 25, 2022 | ![]() November 4, 2040 | ![]() November 16, 2058 |
58 | 59 | 60 |
![]() November 26, 2076 | ![]() December 7, 2094 | ![]() December 19, 2112 |
61 | 62 | 63 |
![]() December 30, 2130 | ![]() January 9, 2149 | ![]() January 21, 2167 |
64 | ||
![]() January 31, 2185 |
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 April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) are also a part of this series but are not included in the table below.
Series members between 2000 and 2200 | ||||
---|---|---|---|---|
![]() July 1, 2000 (Saros 117) | ![]() June 1, 2011 (Saros 118) | ![]() April 30, 2022 (Saros 119) | ![]() March 30, 2033 (Saros 120) | ![]() February 28, 2044 (Saros 121) |
![]() January 27, 2055 (Saros 122) | ![]() December 27, 2065 (Saros 123) | ![]() November 26, 2076 (Saros 124) | ![]() October 26, 2087 (Saros 125) | ![]() September 25, 2098 (Saros 126) |
![]() August 26, 2109 (Saros 127) | ![]() July 25, 2120 (Saros 128) | ![]() June 25, 2131 (Saros 129) | ![]() May 25, 2142 (Saros 130) | ![]() April 23, 2153 (Saros 131) |
![]() March 23, 2164 (Saros 132) | ![]() February 21, 2175 (Saros 133) | ![]() January 20, 2186 (Saros 134) | ![]() December 19, 2196 (Saros 135) |
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 descending node.
22 eclipse events between July 3, 2065 and November 26, 2152 | ||||
---|---|---|---|---|
July 3–4 | April 21–23 | February 7–8 | November 26–27 | September 13–15 |
118 | 120 | 122 | 124 | 126 |
![]() July 3, 2065 | ![]() April 21, 2069 | ![]() February 7, 2073 | ![]() November 26, 2076 | ![]() September 13, 2080 |
128 | 130 | 132 | 134 | 136 |
![]() July 3, 2084 | ![]() April 21, 2088 | ![]() February 7, 2092 | ![]() November 27, 2095 | ![]() September 14, 2099 |
138 | 140 | 142 | 144 | 146 |
![]() July 4, 2103 | ![]() April 23, 2107 | ![]() February 8, 2111 | ![]() November 27, 2114 | ![]() September 15, 2118 |
148 | 150 | 152 | 154 | 156 |
![]() July 4, 2122 | ![]() April 22, 2126 | ![]() February 8, 2130 | ![]() November 26, 2133 | ![]() September 15, 2137 |
158 | 160 | 162 | 164 | |
![]() July 3, 2141 | ![]() November 26, 2152 |
A partial solar eclipse occurred at the Moon’s descending node of orbit on Saturday, February 5, 2000, with a magnitude of 0.5795. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. It was only visible over Antarctica.
A partial solar eclipse will occur at the Moon's descending node of orbit on Wednesday, February 27, 2036, with a magnitude of 0.6286. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, September 13, 2080, with a magnitude of 0.8743. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, August 31, 1989, with a magnitude of 0.6344. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of orbit on Friday, April 7, 1978, with a magnitude of 0.7883. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse will occur at the Moon's descending node of orbit on Monday, July 22, 2047, with a magnitude of 0.3604. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, November 15, 2077, with a magnitude of 0.9371. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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 path of annularity will cross North America and South America. This will be the 47th solar eclipse of Saros cycle 134. A small annular eclipse will cover only 93.71% of the Sun in a very broad path, 262 km wide at maximum, and will last 7 minutes and 54 seconds. Occurring only 4 days after apogee, the Moon's apparent diameter is smaller.
A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, December 26, 2057, with a magnitude of 1.0348. 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.
A partial solar eclipse will occur at the Moon's descending node of orbit on Saturday, November 16, 2058, with a magnitude of 0.7644. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, August 2, 2065, with a magnitude of 0.4903. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse will occur at the Moon's descending node of orbit on Monday, May 20, 2069, with a magnitude of 0.0879. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, with a magnitude of 0.967. 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.
A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, July 1, 2076, with a magnitude of 0.2746. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A total solar eclipse will occur at the Moon's descending node of orbit on Monday, January 6, 2076, with a magnitude of 1.0342. 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.
A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, May 22, 2077, with a magnitude of 1.029. 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.
An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, November 4, 2078, with a magnitude of 0.9255. 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 path of annularity will cross the Pacific Ocean, South America, and the Atlantic Ocean.
An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 24, 2079, with a magnitude of 0.9484. 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.
A partial solar eclipse will occur at the Moon's ascending node of orbit on Friday, December 6, 2086, with a magnitude of 0.9271. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, August 10, 1934, with a magnitude of 0.9436. 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.
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, June 1, 2087, with a magnitude of 0.2146. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.