Solar eclipse of August 2, 2027 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.1421 |
Magnitude | 1.079 |
Maximum eclipse | |
Duration | 383 s (6 min 23 s) |
Coordinates | 25°30′N33°12′E / 25.5°N 33.2°E |
Max. width of band | 258 km (160 mi) |
Times (UTC) | |
Greatest eclipse | 10:07:50 |
References | |
Saros | 136 (38 of 71) |
Catalog # (SE5000) | 9568 |
A total solar eclipse will occur over much of the central Eastern Hemisphere on Monday, August 2, 2027. 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.
Totality will commence over the eastern Atlantic Ocean and travel across the Strait of Gibraltar between Spain and Morocco, and continue across parts of North Africa and the Middle East. Major cities and locations under the path of totality will include: [1]
The maximum duration of totality will be observed in Egypt, approximately 37 miles (60 km) southeast of Luxor, and will last 6 minutes and 22 seconds. [2]
A partial solar eclipse will be visible from the extreme east tip of Maine, United States, far eastern Quebec and the Atlantic Provinces in Canada, southern Greenland, Iceland, Ireland, Great Britain, nearly the entirety of the European continent, all but the southern quarter of Africa, the Middle East, and from South and Southeast Asia. [1]
It will be the first of three total solar eclipses that are observable in Tunisia in the 21st century, passing over the central part of the country. [3] It will be the second total eclipse in Spain within less than a year (after August 2026). Furthermore, an annular eclipse will appear in Spain in January 2028, less than half a year afterwards. National eclipse committee has been established to coordinate eclipse-related activities. [4]
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. [5]
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | 2026 February 17 Annular | −0.97427 | 126 | 2026 August 12 Total | 0.89774 | |
131 | 2027 February 6 Annular | −0.29515 | 136 | 2027 August 2 Total | 0.14209 | |
141 | 2028 January 26 Annular | 0.39014 | 146 | 2028 July 22 Total | −0.60557 | |
151 | 2029 January 14 Partial | 1.05532 | 156 | 2029 July 11 Partial | −1.41908 |
Partial solar eclipses on June 12, 2029, and December 5, 2029, occur in the next lunar year eclipse set.
Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node. [6]
Series members 29–43 occur between 1865 and 2117 | ||
---|---|---|
29 | 30 | 31 |
Apr 25, 1865 | May 6, 1883 | May 18, 1901 |
32 | 33 | 34 |
May 29, 1919 | Jun 8, 1937 | Jun 20, 1955 |
35 | 36 | 37 |
Jun 30, 1973 | Jul 11, 1991 | Jul 22, 2009 |
38 | 39 | 40 |
Aug 2, 2027 | Aug 12, 2045 | Aug 24, 2063 |
41 | 42 | 43 |
Sep 3, 2081 | Sep 14, 2099 | Sep 26, 2117 |
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. [7]
Octon series with 21 events between May 21, 1993 and August 2, 2065 | ||||
---|---|---|---|---|
May 20–21 | March 8–9 | December 25–26 | October 13–14 | August 1–2 |
98 | 100 | 102 | 104 | 106 |
May 21, 1955 | March 9, 1959 | December 26, 1962 | October 14, 1966 | August 2, 1970 |
108 | 110 | 112 | 114 | 116 |
May 21, 1974 | March 9, 1978 | December 26, 1981 | October 14, 1985 | August 1, 1989 |
118 | 120 | 122 | 124 | 126 |
May 21, 1993 | March 9, 1997 | December 25, 2000 | October 14, 2004 | August 1, 2008 |
128 | 130 | 132 | 134 | 136 |
May 20, 2012 | March 9, 2016 | December 26, 2019 | October 14, 2023 | August 2, 2027 |
138 | 140 | 142 | 144 | 146 |
May 21, 2031 | March 9, 2035 | December 26, 2038 | October 14, 2042 | August 2, 2046 |
148 | 150 | 152 | 154 | 156 |
May 20, 2050 | March 9, 2054 | December 26, 2057 | October 13, 2061 | August 2, 2065 |
158 | 160 | 162 | 164 | 166 |
May 20, 2069 | March 8, 2073 | December 26, 2076 | October 13, 2080 | August 1, 2084 |
An annular solar eclipse occurred at the Moon's ascending node of the orbit on Monday, January 26, 2009. 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. It had a magnitude of 0.9282 and was visible from a narrow corridor beginning in the south Atlantic Ocean and sweeping eastward 900 km south of Africa, slowly curving northeast through the Indian Ocean. Its first landfall was in the Cocos Islands followed by southern Sumatra and western Java. It continued somewhat more easterly across central Borneo, across the northwestern edge of Celebes, then ending just before Mindanao, Philippines. The duration of annularity at greatest eclipse lasted 7 minutes, 53.58 seconds, but at greatest duration lasted 7 minutes, 56.05 seconds.
A total solar eclipse took place at the Moon's descending node of the orbit on March 8–9, 2016. If viewed from east of the International Date Line, the eclipse took place on March 8 (Tuesday) and elsewhere on March 9 (Wednesday). A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The eclipse of March 8–9, 2016 had a magnitude of 1.0450 visible across an area of Pacific Ocean, which started in the Indian Ocean, and ended in the northern Pacific Ocean.
A total solar eclipse occurred at the Moon's ascending node on 3 November 2013. It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse, and the rest of the path as a narrow total solar eclipse. 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.
An annular solar eclipse occurred on September 1, 2016. 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. In this case, annularity was observed in Gabon, Congo, Democratic Republic of the Congo, Tanzania, Mozambique, Madagascar, and Reunion.
A total solar eclipse occurred at the Moon’s descending node of the orbit on Thursday, February 26, 1998. 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. Totality was visible in the Galápagos Islands, Panama, Colombia, the Paraguaná Peninsula in northwestern Venezuela, all of Aruba, most of Curaçao and the northwestern tip of Bonaire, all of Montserrat, Guadeloupe and Antigua and Barbuda.
An annular solar eclipse occurred at the Moon’s ascending node of the orbit on August 22, 1998. 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. Annularity was visible in Indonesia, Malaysia, Papua New Guinea, Solomon Islands and Vanuatu. Occurring only 5.2 days before apogee, the Moon’s apparent diameter was 3.6% smaller than average.
A total solar eclipse occurred at the Moon's descending node of the orbit on February 16, 1980. 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. The path of totality crossed central Africa, southern India, and into China at sunset. The southern part of Mount Kilimanjaro, the highest mountain in Africa, also lies in the path of totality. Occurring only about 24 hours before perigee, the Moon's apparent diameter was larger. This was a Supermoon Total Solar Eclipse because the Moon was just a day before perigee.
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A total solar eclipse will occur at the Moon's descending node of the orbit on Wednesday, August 12, 2026, two days past perigee, in parts of North America and almost all of Europe. The total eclipse will pass over the Arctic, Greenland, Iceland, Atlantic Ocean and northern Spain. The points of greatest duration and greatest eclipse will be just 45 km (28 mi) off the western coast of Iceland by 65°10.3' N and 25°12.3' W, where the totality will last 2m 18.21s. It will be the first total eclipse visible in Iceland since June 30, 1954, also Solar Saros series 126, and the only one to occur in the 21st century as the next one visible over Iceland will be in 2196. As lunar perigee will occur on August 10, 2026, two days before the total solar eclipse, the Moon's apparent diameter will be larger.
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A total solar eclipse occurred at the Moon's ascending node of the orbit on June 11, 1983. 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. Occurring only 48 hours before perigee, the Moon's apparent diameter was larger.
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