Solar eclipse of June 11, 2086 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.7215 |
Magnitude | 1.0174 |
Maximum eclipse | |
Duration | 108 s (1 min 48 s) |
Coordinates | 23°12′S12°30′E / 23.2°S 12.5°E |
Max. width of band | 86 km (53 mi) |
Times (UTC) | |
Greatest eclipse | 11:07:14 |
References | |
Saros | 148 (25 of 75) |
Catalog # (SE5000) | 9701 |
A total solar eclipse will occur on June 11, 2086. 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.
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 eclipse series sets from 2083 to 2087 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
118 | July 15, 2083 Partial | 123 | January 7, 2084 Partial | |
128 | July 3, 2084 Annular | 133 | December 27, 2084 Total | |
138 | June 22, 2085 Annular | 143 | December 16, 2085 Annular | |
148 | June 11, 2086 Total | 153 | December 6, 2086 Partial | |
158 | June 1, 2087 Partial |
Solar saros 148, repeating every about 18 years and 11 days, contains 75 events. The series started with a partial solar eclipse on September 21, 1653. It has annular eclipses on April 29, 2014, and May 9, 2032, and a hybrid eclipse on May 20, 2050. It has total eclipses from May 31, 2068, to August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. The longest total eclipse will be on April 26, 2609, at 5 minutes and 23 seconds. [2]
Series members 15–25 occur between 1901 and 2100: | ||
---|---|---|
15 | 16 | 17 |
February 23, 1906 | March 5, 1924 | March 16, 1942 |
18 | 19 | 20 |
March 27, 1960 | April 7, 1978 | April 17, 1996 |
21 | 22 | 23 |
April 29, 2014 | May 9, 2032 | May 20, 2050 |
24 | 25 | |
May 31, 2068 | June 11, 2086 |
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 |
An annular solar eclipse occurred on Tuesday, April 29, 2014. 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 center of the Moon's shadow missed the Earth's South Pole, but the partial eclipse was visible from parts of Antarctica and Australia, and an annular eclipse was visible from a small part of Antarctica.
A partial solar eclipse occurred on October 13–14, 2004. 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 the 54th eclipse of the 124th Saros cycle, which began with a partial eclipse on March 6, 1049 and will conclude with a partial eclipse on May 11, 2347.
A partial solar eclipse occurred on July 31, 2000. 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 visible from northern Russia, northeastern Scandinavia, northern Greenland, western Canada, and the northwestern United States.
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An annular solar eclipse will occur on Wednesday, January 26, 2028. 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.
An annular solar eclipse will occur on May 9, 2032. 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.
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An annular solar eclipse occurred on September 11, 1969.
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