Solar Saros 139
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Solar Saros 139
Saros cycle series 139 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. It has 16 partial solar eclipses, 12 will be hybrid and 43 will be total. The first total eclipse occurred on December 21, 1843 over southern Asia and lasted 1 minute and 43 seconds. The last total eclipse will occur on March 26, 2601 over Antarctica and the southern ocean lasting 35 seconds. This series is currently producing total eclipses over 4 minutes long, with each one gradually increasing in length. It will continue to do so until July 16, 2186 when it will produce the longest total eclipse calculated for the ten millennia from 3999 BCE to 6000 CE. Starting on May 11, 2078, Saros 139 will begin producing the longest total eclipses of any series, surpassing those of Solar Saros 136 (whose eclipses are getting slightly shorter). The last eclipse in this series to occur was a total eclipse on March 29, 2006, lasting 4 minutes 7 seconds ...
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Gamma (eclipse)
Gamma (denoted as γ) of an eclipse describes how centrally the shadow of the Moon or Earth strikes the other body. This distance, measured at the moment when the axis of the shadow cone passes closest to the center of the Earth or Moon, is stated as a fraction of the equatorial radius of the Earth or Moon. Sign The sign of gamma defines, for a solar eclipse, if the axis of the shadow passes north or south of the center of the Earth; a positive value means north. The Earth is defined as that half which is exposed to the Sun (this changes with the seasons and is not related directly to the Earth's poles or equator; thus, the Earth's center is wherever the Sun is directly overhead). For a lunar eclipse, it defines whether the axis of the Earth's shadow passes north or south of the Moon; a positive value means south. Gamma changes monotonically throughout any single saros series. The change in gamma is larger when Earth is near its aphelion (June to July) than when it is near pe ...
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Solar Eclipse Of June 13, 2132
A total solar eclipse will occur at the Moon's ascending node of the orbit on June 13, 2132. 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 is one of the solar eclipses occurring on Friday the 13th. Duration Lasting a maximum of 6 minutes, 55.02 seconds, it will be the longest solar eclipse since the solar eclipse of July 11, 1991 A total solar eclipse occurred at the Moon’s descending node of the orbit on Thursday, July 11, 1991. 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 ..., ...
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Solar Eclipse Of June 3, 2114
There will be a total solar eclipse on June 3, 2114. 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 The angular diameter, angular size, apparent diameter, or apparent size is an angular distance describing how large a sphere or circle appears from a given point of view. In the vision sciences, it is called the visual angle, and in optics, it is ... 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 Saros 139 References NASA Solar eclipses: 2101 to 2200NASA graphicsNASA googlemap of eclipse path 2114 06 03 2114 06 03 2114 06 03 2110s {{Solar-eclipse-stub ...
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Solar Eclipse Of May 22, 2096
A total solar eclipse will occur on Tuesday, May 22, 2096. 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 The angular diameter, angular size, apparent diameter, or apparent size is an angular distance describing how large a sphere or circle appears from a given point of view. In the vision sciences, it is called the visual angle, and in optics, it is ... 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 will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing. Related eclipses Solar eclipses 2094–20 ...
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Solar Eclipse Of April 30, 2060
A total solar eclipse will occur on Friday, April 30, 2060. 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 The angular diameter, angular size, apparent diameter, or apparent size is an angular distance describing how large a sphere or circle appears from a given point of view. In the vision sciences, it is called the visual angle, and in optics, it is ... 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 2059–2061 Saros 139 Metonic series All eclipses in this table occur at the Moon's ascending node. Notes References 2060 04 30 2060 in science 2060 04 30 2060 04 30 {{Solar-ec ...
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Solar Eclipse Of April 20, 2042
A total solar eclipse will occur on Sunday, April 20, 2042. 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. It will be seen significantly in Western Indonesia (particularly in Sumatra), Eastern Malaysia, Brunei and the Philippines The Philippines (; fil, Pilipinas, links=no), officially the Republic of the Philippines ( fil, Republika ng Pilipinas, links=no), * bik, Republika kan Filipinas * ceb, Republika sa Pilipinas * cbk, República de Filipinas * hil, Republ .... Images Animated path Related eclipses Solar eclipses of 2040–2043 Saros 139 Inex series ...
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Solar Eclipse Of March 18, 1988
A total solar eclipse occurred on March 18, 1988. 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 Indonesia and southern Philippines. Observation The General Santos City Tourism Office of the Philippines promoted it as a big tourism event. Hordes of scientists, astronomers, journalists, TV crews and tourists from all over the globe observed the totality from there. Then president of the Philippines and the first female president in Asia, Corazon Aquino Maria Corazon "Cory" Sumulong Cojuangco-Aquino (; ; January 25, 1933 – August 1, 2009) was a Filipina ...
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Solar Eclipse Of March 7, 1970
A total solar eclipse occurred on March 7, 1970, visible across most of North America and Central America. 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 1.3 days after perigee (Perigee on March 6, 1970 at 09:32 UTC), the Moon's apparent diameter was larger than the Sun and thus fulfilled this condition. Totality was visible across southern Mexico and the Gulf of Mexico, the southeast Atlantic coast of the United States, northeast to the Maritimes of eastern Canada, and northern Miquelon-Langlade in the French overseas collectivity of Saint Pierre and Miquelon. Gre ...
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Solar Eclipse Of February 25, 1952
A total solar eclipse occurred on February 25, 1952. 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 Africa, the Middle East, and Asia Asia (, ) is one of the world's most notable geographical regions, which is either considered a continent in its own right or a subcontinent of Eurasia, which shares the continental landmass of Afro-Eurasia with Africa. Asia covers an are .... Related eclipses Solar eclipses of 1950–1953 Saros 139 Metonic series Notes References Solar eclipse of February 25, 1952 in Russia {{DEFAULTSORT:Solar ...
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Solar Eclipse Of February 14, 1934
A total solar eclipse occurred on February 14, 1934. 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 from the Dutch East Indies (today's Indonesia), North Borneo (now belonging to Malaysia Malaysia ( ; ) is a country in Southeast Asia. The federation, federal constitutional monarchy consists of States and federal territories of Malaysia, thirteen states and three federal territories, separated by the South China Sea into two r ...), and the South Seas Mandate of Japan (the part now belonging to FS Micronesia). Related eclipses Solar eclipses 1931– ...
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Solar Eclipse Of February 3, 1916
A total solar eclipse occurred on February 3, 1916. 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 Colombia, Venezuela, and the whole Guadeloupe except Marie-Galante, Saint Martin and Saint Barthélemy Saint Barthélemy (french: Saint-Barthélemy, ), officially the Collectivité territoriale de Saint-Barthélemy, is an overseas collectivity of France in the Caribbean. It is often abbreviated to St. Barth in French, and St. Barts in English .... Related eclipses Solar eclipse 1913–1917 Saros 139 Tritos series Notes References Eclipse d ...
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