query: when does the solar eclipse happen in north america

pos: Solar eclipse of August 21, 2017 coinciding with the eclipse, and at least one wedding was also planned and took place to coincide with the eclipse. Logistical problems were expected with the influx of visitors, especially for smaller communities. The sale of counterfeit eclipse glasses was also anticipated to be a hazard for eye injuries. Future total solar eclipses will cross the United States in April 2024 (12 states) and August 2045 (10 states), and annular solar eclipses—wherein the Moon appears smaller than the Sun—will occur in October 2023 (9 states) and June 2048 (9 states). The total eclipse had a magnitude of 1.0306 and was

neg: Solar eclipse of October 23, 2014 across most of North America. The partial eclipse was visible in most of North America, as well as eastern Siberia. Solar eclipse of October 23, 2014 A partial solar eclipse occurred on October 23, 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. The center of the Moon's shadow missed the Earth, passing above the North Pole, but

neg: Solar eclipse of March 7, 1970 remainder of the southern states. There will not be an eclipse with a greater duration of totality over the contiguous U.S. until April 8, 2024, a period of 54 years. This eclipse slowed a radio transmission of atomic time from North Carolina to Washington, D.C. <BR>Animation of eclipse path (3 minutes per frame) CBS broadcast the first total eclipse in color. "Maps": "News": "Photos and observations" Solar eclipse of March 7, 1970 A total solar eclipse occurred on Saturday, March 7, 1970, visible across most of North America and Central America. A solar eclipse occurs when the Moon passes between

neg: Solar eclipse of September 14, 2099 Canada, and move eastern across Canada (British Columbia, Alberta, and Saskatchewan) and the northern states of the United States (North Dakota, Minnesota, Wisconsin, Illinois, Indiana, Ohio, West Virginia, Virginia and North Carolina). The eclipse will end in the Atlantic ocean, with partial visibility in parts of Europe, West Africa and throughout the entirety of North and South America. The total eclipse will pass through the cities of Madison, Wisconsin, and Grand Rapids, Michigan. The last total solar eclipse over these two cities respectively was May 16, 1379, and April 18, 1558. Although this solar eclipse does pass over a few

neg: Solar eclipse of March 7, 1970 Solar eclipse of March 7, 1970 A total solar eclipse occurred on Saturday, 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. Totality

neg: Solar eclipse of March 30, 2052 southeastern states of the United States. Almost all of North America and the northern edge of South America will see a partial eclipse. It will be the 2nd total eclipse visible from the Florida Panhandle and southwest Georgia in 7 years. Solar eclipse of March 30, 2052 A total solar eclipse will occur on March 30, 2052. 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,

neg: Solar eclipse of June 26, 1824 partial eclipse across much of North America near sunset. It is a part of solar Saros 124. Solar eclipse of June 26, 1824 A total solar eclipse occurred on June 26, 1824. 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

neg: Solar eclipse of February 26, 1979 Solar eclipse of February 26, 1979 A total solar eclipse occurred in North America on Monday, February 26, 1979. A solar eclipse is an astronomical phenomenon that 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 central

neg: Solar eclipse of July 29, 1878 Solar eclipse of July 29, 1878 A total solar eclipse occurred on July 29, 1878, over much of North America including the region of the Rocky Mountains. 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

neg: Solar eclipse of July 9, 1945 Solar eclipse of July 9, 1945 A total solar eclipse occurred on July 9, 1945. 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 northern North America, across Greenland and

neg: Solar eclipse of April 8, 2024 Solar eclipse of April 8, 2024 A total solar eclipse will take place on Monday, April 8, 2024, visible across North 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. With a magnitude of

neg: Solar eclipse of November 22, 1919 Solar eclipse of November 22, 1919 An annular solar eclipse occurred on November 22, 1919. 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 occurred in over half of North America,

neg: Solar eclipse of January 5, 1935 Solar eclipse of January 5, 1935 A partial solar eclipse occurred on January 5, 1935 during summer. 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 one of five eclipses that took place that year, the next one was in the Northern Hemisphere on February 3 and covered much of North America. It was the last eclipse

neg: Solar eclipse August 11, 2018. It was a partial solar eclipse visible from Northern Europe and Northeastern Asia. Solar eclipse A solar eclipse occurs when an observer (on Earth) passes through the shadow cast by the Moon which fully or partially blocks ("occults") the Sun. This can only happen when the Sun, Moon and Earth are nearly aligned on a straight line in three dimensions (syzygy) during a new moon when the Moon is close to the ecliptic plane. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of

neg: Solar eclipse of April 8, 2024 9,000 square mile intersection of the paths of totality of both the 2017 and 2024 eclipses, therefore earning the rare distinction of being witness to two total solar eclipses within a span of seven years. Notable total and annular solar eclipse crossing the United States from 1900 to 2050: Solar eclipse of April 8, 2024 A total solar eclipse will take place on Monday, April 8, 2024, visible across North 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

neg: Solar eclipse of May 10, 1994 Solar eclipse of May 10, 1994 An annular solar eclipse occurred on May 10, 1994. It was visible over a wide swath of North America, from Baja California across the Midwest of the United States up through Ontario and Nova Scotia in Canada. 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. The eclipse is either total or annular. In a total eclipse, the moon's size from earth is large enough to block all of the disk of the sun. An

neg: Lunar phase the times of lunar phases. It might be expected that once every month, when the Moon passes between Earth and the Sun during a new moon, its shadow would fall on Earth causing a solar eclipse, but this does not happen every month. Nor is it true that during every full moon, the Earth's shadow falls on the Moon, causing a lunar eclipse. Solar and lunar eclipses are not observed "every" month because the plane of the Moon's orbit around the Earth is tilted by about 5° with respect to the plane of Earth's orbit around the Sun (the plane

neg: Eclipse cycle a solar eclipse. At full moon, when the Moon is in opposition to the Sun, the Moon may pass through the shadow of the Earth, and a lunar eclipse is visible from the night half of the Earth. Conjunction and opposition of the Moon together have a special name: syzygy (from "Greek" for "junction"), because of the importance of these lunar phases. An eclipse does not happen at every new or full moon, because the plane of the orbit of the Moon around the Earth is tilted with respect to the plane of the orbit of the Earth around the

neg: Solar eclipse of March 20, 2015 that day. The event was visible as a partial eclipse all across Europe including: Norway, Sweden, Denmark, the United Kingdom, Ireland, Portugal, France, Germany, Poland, Czech Republic, Hungary, Austria, Italy, Montenegro, Finland, Western Russia, and Ukraine. A total lunar eclipse followed on April 4, 2015, visible over Australia, and the Pacific coast of Asia and North America. Solar eclipse of March 20, 2015 A total solar eclipse occurred on March 20, 2015. 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.

neg: Solar eclipse of August 11, 2018 China. During the sunset, the eclipse was observed in North and South Korea. Solar eclipse of August 11, 2018 The solar eclipse of August 11, 2018 was a partial solar eclipse that was visible in the north of North America, Greenland, Northern Europe and north-eastern Asia. The maximal phase of the partial eclipse was recorded in East Siberian Sea, near the Wrangel Island. The eclipse was observed in Canada, Greenland, Scotland, most of the Nordic countries (Iceland, Norway, Sweden, Finland), Estonia, Latvia, practically throughout Russia (except for places southwest of the line roughly passing through Pskov, Moscow and Penza, and

neg: Solar eclipse of August 23, 2044 as well as extreme southwestern Saskatchewan in Canada, and will be widely visible in Montana and partially in North Dakota in the United States of America; partiality will be visible throughout the western United States near sunset. The greatest duration of the eclipse can be observed in the Northwest Territories, approximately southeast of Great Bear Lake. <BR>Animated path Solar eclipse of August 23, 2044 A total solar eclipse will occur on August 23, 2044. 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

neg: Solar eclipse of May 10, 1994 and part of Morocco including the capital city Rabat. Niagara Falls was also covered by the path of annularity. Photos: Solar eclipse of May 10, 1994 An annular solar eclipse occurred on May 10, 1994. It was visible over a wide swath of North America, from Baja California across the Midwest of the United States up through Ontario and Nova Scotia in Canada. 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. The eclipse is either total or annular. In a

neg: Solar eclipse of July 29, 1878 the opportunity to make their observations from the higher altitudes provided by the Rocky Mountains. After the 1878 eclipse, astronomers began to build observatories at locations well above sea level, including on the sides and summits of mountains, a scientific trend which extended throughout the twentieth century and into the twenty-first. Solar eclipse of July 29, 1878 A total solar eclipse occurred on July 29, 1878, over much of North America including the region of the Rocky Mountains. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the

neg: Solar eclipse Solar eclipse A solar eclipse occurs when an observer (on Earth) passes through the shadow cast by the Moon which fully or partially blocks ("occults") the Sun. This can only happen when the Sun, Moon and Earth are nearly aligned on a straight line in three dimensions (syzygy) during a new moon when the Moon is close to the ecliptic plane. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of the Sun is obscured. If the Moon were in a perfectly circular orbit, a little closer

neg: Solar eclipse of September 12, 2034 Atlantic Ocean, and enter South America. Countries under the path include northern Chile, southern Bolivia, northern Argentina, southern Paraguay, and southern Brazil. The eclipse will then enter the Pacific Ocean, and terminate approximately southeast of South America. <BR>Animated path Solar eclipse of September 12, 2034 An annular solar eclipse will occur on September 12, 2034. 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

neg: Solar eclipse of June 28, 1908 of North America including a part of Central Mexico around Mexico City and Orlando and Daytona Beach, Florida in the USA which occurred in the morning hours. In Africa, it included Rosso, Mauritania, the northernmost part of Senegal, Bamako and the southwestern French Sudan (now Mali), the southwesternmost part of Upper Volta (now Burkina Faso) and northern British Gold Coast (now Ghana) which occurred before sunset. Solar eclipse of June 28, 1908 An annular solar eclipse occurred on June 28, 1908. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the

neg: Solar eclipse of August 11, 2018 Solar eclipse of August 11, 2018 The solar eclipse of August 11, 2018 was a partial solar eclipse that was visible in the north of North America, Greenland, Northern Europe and north-eastern Asia. The maximal phase of the partial eclipse was recorded in East Siberian Sea, near the Wrangel Island. The eclipse was observed in Canada, Greenland, Scotland, most of the Nordic countries (Iceland, Norway, Sweden, Finland), Estonia, Latvia, practically throughout Russia (except for places southwest of the line roughly passing through Pskov, Moscow and Penza, and the most eastern places of the Far East), in Kazakhstan, Kyrgyzstan, Mongolia and

neg: Solar eclipse of November 3, 2013 Coast and Ghana. Places with partial darkening were the Eastern coast of North America, southern Greenland, Bermuda, the Caribbean islands, Costa Rica, Panama, Northern South America, almost all the African continent, the Iberian Peninsula, Italy, Greece, Malta, Southern Russia, the Caucasus, Turkey and the Middle East. This solar eclipse happened simultaneously with the 2013 Abu Dhabi Grand Prix, and it was possible to observe a partial solar eclipse in Abu Dhabi before the sunset while the F1 race took place, as shown briefly during its broadcast. Solar eclipse of November 3, 2013 A total solar eclipse occurred on 3 November

neg: Solar eclipse of May 20, 2012 Solar eclipse of May 20, 2012 The solar eclipse of May 20, 2012 (May 21, 2012 local time in the Eastern Hemisphere) was an annular solar eclipse that was visible in a band spanning through Eastern Asia, the Pacific Ocean, and North America. As a partial solar eclipse, it was visible from northern Greenland to Hawaii, and from eastern Indonesia at sunrise to northwestern Mexico at sunset. The annular eclipse was the first visible from the contiguous United States since the solar eclipse of May 10, 1994, and the first in Asia since the solar eclipse of January 15, 2010.

neg: Solar eclipse of June 8, 1918 Solar eclipse of June 8, 1918 A total solar eclipse occurred on June 8, 1918. The eclipse was observed by a U.S. Naval Observatory team at Baker City in Oregon. The painting below shows totality when the Moon prevented the Sun's rays from hitting that part of Oregon. The track of the eclipse was a band across the entire contiguous United States, which would not happen again until 99 years later in 2017. The path of the eclipse started south of Japan, went across the Pacific Ocean, passing northern part of Kitadaitō, Okinawa and the whole Tori-shima in Izu Islands

neg: Solar eclipse of July 11, 1991 down through Central America and across South America ending over Brazil. It lasted for 6 minutes and 53 seconds at the point of maximum eclipse. There will not be a longer total eclipse until June 13, 2132. This eclipse was the most central total eclipse in 800 years, with a gamma of -.0041. There will not be a more central eclipse for another 800 years. Its magnitude was also greater than any eclipse since the 6th century. Photos: Videos: Solar eclipse of July 11, 1991 A total solar eclipse occurred on July 11, 1991. A solar eclipse occurs when the

neg: March 2007 lunar eclipse the first of two lunar eclipses to occur in 2007, the second being on 28 August 2007. The whole event was visible from Europe, Africa, parts of South America, and some areas of North America, Asia, and Western Australia. In North America, part of the event was visible at moonrise. It last occurred on February 20, 1989 and will next occur on March 14, 2025. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 130. March

neg: Solar eclipse of December 1, 1891 Solar eclipse of December 1, 1891 A partial solar eclipse occurred on December 1, 1891, during late spring. 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 only partial eclipse that took place that year. It was part of solar saros 150. The eclipse took place in South America including Argentina and Chile (along with its

neg: Solar eclipse of February 21, 1803 Solar eclipse of February 21, 1803 A total solar eclipse occurred on February 21, 1803. 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 eclipse was visible in Pacific Ocean and Central America, while

neg: Solar eclipse of August 21, 1914 this solar eclipse. However, World War I broke out and he was interned in Russia, unable to carry out the necessary measurements. William Wallace Campbell, from neutral America, was permitted to continue with his plans, but cloud cover obscured the eclipse. Solar eclipse of August 21, 1914 A total solar eclipse occurred on August 21, 1914. 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

neg: Eclipse the Earth, a solar eclipse occurs when the Moon passes in front of the Sun. The type of solar eclipse event depends on the distance of the Moon from the Earth during the event. A total solar eclipse occurs when the Earth intersects the umbra portion of the Moon's shadow. When the umbra does not reach the surface of the Earth, the Sun is only partially occulted, resulting in an annular eclipse. Partial solar eclipses occur when the viewer is inside the penumbra. The eclipse magnitude is the fraction of the Sun's diameter that is covered by the Moon. For

neg: Solar eclipse of June 8, 1918 other eclipses that year. The first was a partial lunar eclipse, during which the shadow of the earth can be seen on the moon, and another solar eclipse that took place on December 3 over South America. The other solar eclipse, however, was an annular eclipse, which occurs when the moon has a smaller apparent diameter and therefore never fully obscures the sun. Solar eclipse of June 8, 1918 A total solar eclipse occurred on June 8, 1918. The eclipse was observed by a U.S. Naval Observatory team at Baker City in Oregon. The painting below shows totality when the

neg: Solar eclipse of May 12, 1706 Solar eclipse of May 12, 1706 The solar eclipse on May 12, 1706 was a total eclipse. The eclipse was visible in north and west Africa along with all Europe and its islands, Asia including the most of Middle East and almost all of Siberia and a small part of northeastern North America and the northern islands. It was also visible in the Atlantic. A very small portion occurred in the Southern Hemisphere almost entirely over the ocean. It was part of solar saros 133. The umbral portion which was as far as 242 km (150 km), it included areas

neg: Solar eclipse of November 12, 1966 Solar eclipse of November 12, 1966 A total solar eclipse occurred on November 12, 1966. 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 cut a swath across South America from

neg: Solar eclipse of June 8, 1956 ended west of South America on June 8th. Solar eclipse of June 8, 1956 A total solar eclipse occurred on June 8–9, 1956. 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 began near

neg: Solar eclipse of 1 May 1185 the Scottish Highlands, the Western Isles and Orkney. Solar eclipse of 1 May 1185 The solar eclipse of 1 May 1185 was a total solar eclipse visible in Central America, Northern Europe, Eastern Europe, and Kazakhstan. The eclipse is number 30 in the Solar Saros 115 series. The eclipse shadow on the Earth's surface was at its greatest at 13:18:02 Universal Time. The sun was in Taurus at this time. The shadow axis passed between the Earth's center and the north pole. The minimum distance from the center of the Earth to the Moon's shadow cone axis was 3,357 kilometers.

neg: Solar eclipse of 1 May 1185 Solar eclipse of 1 May 1185 The solar eclipse of 1 May 1185 was a total solar eclipse visible in Central America, Northern Europe, Eastern Europe, and Kazakhstan. The eclipse is number 30 in the Solar Saros 115 series. The eclipse shadow on the Earth's surface was at its greatest at 13:18:02 Universal Time. The sun was in Taurus at this time. The shadow axis passed between the Earth's center and the north pole. The minimum distance from the center of the Earth to the Moon's shadow cone axis was 3,357 kilometers. The average length of the Moon's shadow was

neg: Solar Eclipse (video game) Solar Eclipse (video game) Solar Eclipse is a 1995 space flight simulation video game developed and published by Crystal Dynamics, released exclusively for the Sega Saturn in North America and Japan. "Solar Eclipse" was developed under the title ""Titan"", but the American marketing team decided it would sell better if published as a sequel to the 1994 video game "Total Eclipse", especially as the two featured similar gameplay and graphical style. A port called Titan Wars was released in Europe for the PlayStation, in November 1996. "Solar Eclipse" is a hybrid of rail shooter and free-roaming space combat simulation; the

neg: Solar Eclipse (video game) but that these problems would discourage repeat plays. Solar Eclipse (video game) Solar Eclipse is a 1995 space flight simulation video game developed and published by Crystal Dynamics, released exclusively for the Sega Saturn in North America and Japan. "Solar Eclipse" was developed under the title ""Titan"", but the American marketing team decided it would sell better if published as a sequel to the 1994 video game "Total Eclipse", especially as the two featured similar gameplay and graphical style. A port called Titan Wars was released in Europe for the PlayStation, in November 1996. "Solar Eclipse" is a hybrid of

neg: Solar eclipse of February 26, 2017 Solar eclipse of February 26, 2017 An annular solar eclipse took place on February 26, 2017. 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 was visible across southern South America

neg: June 1964 lunar eclipse 5 days alternating between each saros series. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 136. June 1964 lunar eclipse A total lunar eclipse took place on June 25, 1964. The moon passed through the center of the Earth's shadow. It was completely visible from South America and Africa, seen as rising over North America, and setting over Europe and Western Asia. This is the 35th member of Lunar Saros 129. The previous event was

neg: Solar eclipse of April 8, 2005 beginning and ending as an annular eclipse. It was visible within a narrow corridor in the Pacific Ocean. The path of the eclipse started south of New Zealand and crossed the Pacific Ocean in a diagonal path and ended in the extreme northwestern part of South America. The total solar eclipse was not visible on any land, while the annular solar eclipse was visible in Southern tip of Puntarenas Province of Costa Rica, Panama, Colombia and Venezuela. <BR>Animated path Photos: Solar eclipse of April 8, 2005 A total solar eclipse occurred on April 8, 2005. A solar eclipse occurs when

neg: August 2036 lunar eclipse August 2036 lunar eclipse A total lunar eclipse will take place on August 7, 2036. The moon will pass through the center of the Earth's shadow. This is the second eclipse this season. First eclipse this season: Partial solar eclipse of July 23, 2036 Third eclipse this season: Partial solar eclipse of August 21, 2036 It will be completely visible over South America, seen as rising over North America, and setting over Africa and Europe. This is the 39th member of Lunar Saros 129. The previous event was the July 2018 lunar eclipse. The next event is the August 2054

neg: Solar eclipse of September 2, 2035 Beijing, China and Pyongyang, North Korea, and will pass north of a third, Tokyo, Japan. Solar eclipse of September 2, 2035 A total solar eclipse will occur on September 2, 2035. 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

neg: Solar eclipse of December 15, 2039 Ocean, passing over much of Antartica and closely reaching the South Pole. A partial eclipse will be visible in the southern extremities of South America and Africa. It will terminate in the southern Indian Ocean several hours later. <BR>Animated path Solar eclipse of December 15, 2039 A total solar eclipse will occur on December 15, 2039. 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

neg: Solar eclipse of June 21, 2001 narrow corridor in the southern Atlantic Ocean and southern Africa, including Angola, Zambia, Zimbabwe, Mozambique, the southern tip of Malawi, and Madagascar. A partial eclipse was seen from the much broader path of the Moon's penumbra, including eastern South America and most of Africa. Photos: Solar eclipse of June 21, 2001 A total solar eclipse took place on June 21, 2001, with a magnitude of 1.0495. 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

neg: Solar eclipse of February 4, 1981 and southern Stewart Island of New Zealand near sunrise on February 5th, and ended at sunset over western South America. Solar eclipse of February 4, 1981 An annular solar eclipse occurred on February 4–5, 1981. 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

neg: Solar eclipse of May 20, 2012 The eclipse continued to travel southeast, passing 30 miles (48 km) north of Las Vegas, Nevada, over St. George, Utah, and reaching the Grand Canyon by approximately 6:35 p.m MST. After passing over Albuquerque, New Mexico and Lubbock, Texas, the eclipse terminated above central Texas at sunset, 8:39 p.m. CST. An estimated 6.6 million people lived under the path of the antumbra. The penumbra was visible throughout most of North America, including the islands of Hawaii. Solar eclipse of May 20, 2012 The solar eclipse of May 20, 2012 (May 21, 2012 local time in the Eastern Hemisphere) was an

neg: Solar eclipse of July 1, 2011 Solar eclipse of July 1, 2011 A partial solar eclipse occurred on July 1, 2011. 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 is the first solar eclipse of Saros series 156, only visible as a partial solar eclipse in a small area south of South Africa and north of Antarctica. At greatest eclipse, the magnitude was

neg: Solar eclipse of April 8, 2024 1.0566, its longest duration of totality will be of four minutes and 28 seconds near the town of Nazas, Durango, Mexico, and the nearby city of Torreón, Coahuila. This eclipse will be the first total solar eclipse to be visible from Canada since February 26, 1979, the first in Mexico since July 11, 1991, and the first in the U.S. since August 21, 2017. It will be the only total solar eclipse in the 21st century where totality is visible in Mexico, the United States of America, and Canada. Totality will be visible in a narrow strip in North America,

neg: Solar eclipse of August 21, 2017 clouds, prolonging the observation time spent in the umbra. A partial solar eclipse was seen from the much broader path of the Moon's penumbra, including all of North America, particularly areas just south of the totality pass, where the eclipse lasted about 3–5 hours, northern South America, Western Europe, and some of Africa and north-east Asia. At one location in Wyoming, a small group of astronomers used telescopic lenses to photograph the sun as it was in partial eclipse, while the ISS was also seen to briefly transit the sun. Similar images were captured by NASA from a location in

neg: August 2053 lunar eclipse of North and South America, Oceania, far-eastern Asia, western Africa, and far-western Europe. This lunar eclipse is part of Lunar Saros 119. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two solar eclipses of Solar Saros 126. August 2053 lunar eclipse A penumbral lunar eclipse will take place on August 29, 2053. This eclipse is a relatively rare total penumbral lunar eclipse wherein the entire moon passes through the Earth's penumbra without any portion entering the umbra. This eclipse will be the

neg: April 1986 lunar eclipse eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 138. April 1986 lunar eclipse A total lunar eclipse took place on April 24, 1986. It is seen rising over eastern Asia, the Pacific Ocean, and western North America and South America, the eclipse is also seen setting over the whole of Europe, Africa and Western Asia. The eclipse was seen very visible over the Philippines, it becomes the first lunar eclipse after the EDSA Revolution since the two lunar eclipses happened between May 4, 1985 and

neg: Solar eclipse of December 14, 2001 Costa Rica, northern Nicaragua and San Andrés Island, Colombia. The central shadow passed just south of Hawaii in early morning and ended over Central America near sunset. Photos: Solar eclipse of December 14, 2001 An annular solar eclipse occurred on December 14, 2001. 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

neg: Eclipse happen during an "eclipse season", the two times of each year when the plane of the Earth's orbit around the Sun crosses with the plane of the Moon's orbit around the Earth. The type of solar eclipse that happens during each season (whether total, annular, hybrid, or partial) depends on apparent sizes of the Sun and Moon. If the orbit of the Earth around the Sun, and the Moon's orbit around the Earth were both in the same plane with each other, then eclipses would happen each and every month. There would be a lunar eclipse at every full moon,

neg: Solar eclipse of May 22, 1724 Solar eclipse of May 22, 1724 A total solar eclipse occurred on May 22, 1724. 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 solar eclipse crossed Ireland and Great Britain near sunset, north-west

neg: Solar eclipse of August 16, 1841 of Antarctica at 61.9 S & 158 E at 21:20:24 UTC (8:20 AM local time). The subsolar marking was in the Pacific north of the 10th parallel north. Solar eclipse of August 16, 1841 A partial solar eclipse occurred on August 16, 1841 during winter. 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 last of four

neg: July 1982 lunar eclipse between 1910 and 2090. Solar Saros 136 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 136. July 1982 lunar eclipse A total lunar eclipse took place on July 6, 1982. The moon passed through the center of the Earth's shadow. It was seen completely over North and South America, seen rising over Australia, and setting over

neg: Solar eclipses on the Moon at 43.31°S) where the temperatures remains high. Some craters are slightly cooler but as warm as the surface and warmer than areas outside the mares (basins) such as Copernicus and Langrenus. On the Moon, when there is a partial eclipse, one example is when half of the Sun is blocked (north or south), a part of the Moon has a partial eclipse (north or south). In some partial eclipses when the center of the Earth's shadow misses the Moon, one example is one hemisphere has a partial eclipse and the other does not. In some eclipses when the center of

neg: Solar eclipse of August 12, 2026 Solar eclipse of August 12, 2026 A total solar eclipse will occur on August 12, 2026, in North America and 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 50 km off the western coast of Iceland by 65°10.3' N and 25°12.3' W, where the totality will last 2m 18s. It will be the first total eclipse visible in Iceland since June 30, 1954 and the only one to occur in the 21st century as the next one will be in 2196.

neg: Solar eclipse of May 28, 1900 loaded several railroad cars with scientific equipment and headed to Wadesboro, North Carolina. Scientists had determined that this small town would be the best location in North America for viewing an expected total solar eclipse, and the "Smithsonian Solar Eclipse Expedition" hoped to capture photographic proof of the solar corona during the event for further study. The team included Smithsonian photographer Thomas Smillie, who headed up the missions photographic component. Smillie rigged cameras to seven telescopes and successfully made eight glass-plate negatives, ranging in size from eleven by fourteen inches to thirty by thirty inches. At the time, Smillie's work

neg: August 2072 lunar eclipse August 2072 lunar eclipse A total lunar eclipse will take place on August 28, 2072. It will be completely visible over North America, Europe, Africa, Asia, and Australia, seen rising over Europe, Africa, and Asia and setting over North America. In South America the eclipse will be not visible over invisible. This is the 41st member of Lunar Saros 129. The previous event was the August 2054 lunar eclipse. The next event is the September 2090 lunar eclipse. Lunar Saros 129 contains 11 total lunar eclipses between 1910 and 2090. Solar Saros 136 interleaves with this lunar saros with an

neg: August 2053 lunar eclipse August 2053 lunar eclipse A penumbral lunar eclipse will take place on August 29, 2053. This eclipse is a relatively rare total penumbral lunar eclipse wherein the entire moon passes through the Earth's penumbra without any portion entering the umbra. This eclipse will be the first total penumbral lunar eclipse since the March 2006 lunar eclipse. This lunar eclipse will be followed by the solar eclipse of September 12, 2053. The entire eclipse will be visible in most of North America, Central America, and the western half of South America. Part of the eclipse will be visible in the remainder

neg: Solar eclipse of April 3, 1848 and 20% at the Antarctic peninsula. The greatest eclipse was at the Antarctic Peninsula at 71.8 S, 89 W at 22:49 UTC (4:49 PM local time). The subsolar marking was north of the 5th parallel north in the Pacific around the Palmyra Atoll. Solar eclipse of April 3, 1848 A partial solar eclipse occurred on April 3, 1848 during fall. 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

neg: Solar eclipse of September 23, 1699 Solar eclipse of September 23, 1699 A total solar eclipse occurred on September 23, 1699. 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 narrow path of totality just clipped the north-east corner of

neg: Solar eclipse of February 14, 1934 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

neg: Solar eclipse of August 6, 1823 Montt in the early morning hours and ended near another part of northern Antarctica east of the peninsula in the afternoon. The greatest eclipse was in the Pacific Ocean west of the ocean line and halfway between South America and Antarctica which happened at 13:45 UTC (08:19 local time) at 62.5 S and 79.3 W. The sub-solar marking was northwest of the island of Santiago in Cape Verde, nearly midway with the other islands. Solar eclipse of August 6, 1823 A partial solar eclipse occurred on August 6, 1823 in the midwinter season. A solar eclipse occurs when the Moon

neg: June 2012 lunar eclipse eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 147. June 2012 lunar eclipse A partial lunar eclipse took place on June 4, 2012. It was the first of two lunar eclipses occurring in 2012, the second eclipse set to happen on November 28. The moon was about one third covered by the Earth's northern umbral shadow at maximum eclipse. The portion of the moon inside the umbral shadow was illuminated by sunlight refracted through the Earth's atmosphere,

neg: Solar eclipse of November 23, 2003 corridor in the Antarctic region. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the southern tip of South America and most of Australia. For most solar eclipses the path of totality moves eastwards. In this case the path moved south and then west round Antarctica. <BR>Animated map Photos: Solar eclipse of November 23, 2003 A total solar eclipse took place on November 23, 2003 with a magnitude of 1.0379. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for

neg: Solar eclipse of April 26, 1892 experienced heavy cloud cover and the eclipse was thus not visible. The subsolar marking was at around the 15th parallel north southeast of Hawai'i and northeast of the Palmyra Atoll. Solar eclipse of April 26, 1892 The solar eclipse on April 26, 1892 was a total 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 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

neg: Solar eclipse of April 29, 1976 Solar eclipse of April 29, 1976 An annular solar eclipse occurred on April 29, 1976. 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. Totality was visible from North Africa, Greece, Turkey,

neg: Solar eclipse of October 30, 1845 was also around 90% in the shores of Western Antarctica and around the 180th meridian. The rim of the eclipse included the area south of Cairns, Queensland, the Coral Sea and Cook Islands. The eclipse started at sunrise in Western Australia and finished at sunset in the Antarctic Peninsula and southwest of Patagonia in South America. Solar eclipse of October 30, 1845 A hybrid (annular/total) solar eclipse occurred on October 30, 1845 during winter. 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

neg: Solar eclipse of October 23, 2014 Solar eclipse of October 23, 2014 A partial solar eclipse occurred on October 23, 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. The center of the Moon's shadow missed the Earth, passing above the North Pole, but a partial eclipse was visible at sunrise (October 24 local time) in far eastern Russia, and before sunset (October 23)

neg: Sign prayer were superstitious minds of the occurrence of natural disasters. For example, when Abraham, the son of Prophet died, the solar eclipse occurred. People thought that the solar eclipse happened because of the death of the son of the Prophet. There is narration about it. When the prophet was informed of these words, he went pulpit and said: “Oh people! Surely the sun and moon are signs of Allah that are moving by Verdict of Allah. Lunar eclipse or Solar eclipse does not occur by the birth or death of any person. So that when one of them or both is

neg: Solar eclipse of April 19, 2004 Solar eclipse of April 19, 2004 A partial solar eclipse took place on Monday, 19 April 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 largely visible over the south Atlantic Ocean and north shores of Antarctica, most prominently the Antarctic Peninsula. The eclipse was deep enough to be seen from a large portion of southern

neg: Eclipse season Eclipse season An eclipse season is one of only two periods during a year when eclipses can occur, due to the orbital inclination of the Moon. Each season lasts for approximately 35 days and repeats just short of six months, thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. During the eclipse season, the inclination of the Moon's orbit is low, hence the Sun, Moon, and Earth become aligned straight enough (in syzygy) for an eclipse to occur. During each season, the type of solar eclipse (whether total or annular, as

neg: August 1989 lunar eclipse two annular solar eclipses of Solar Saros 135. August 1989 lunar eclipse A total lunar eclipse took place at 0308 UT (GMT) on August 17, 1989, the second of two total lunar eclipses in 1989. The moon passed through the center of the Earth's shadow. It was seen completely over South America, and rising over North America, and setting over Africa, and Europe. This eclipse is the second of four lunar year eclipses occurring at the moon's ascending node. The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of

neg: Solar eclipse of April 9, 2043 total solar eclipse, it is not a central solar eclipse. A non-central eclipse is one where the center-line of totality does not intersect the surface of the Earth. Instead, the center line passes just above the Earth's surface. This rare type occurs when totality is only visible at sunset or sunrise in a polar region. It will be seen fully from Russia's Kamchatka Peninsula. It will be visible partially throughout Canada, Greenland and Iceland. It will be also partially visible from the western part United States including Alaska and Hawaii. <BR>Animated path Solar eclipse of April 9, 2043 A total

neg: December 2010 lunar eclipse and 5.5 days (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 132. December 2010 lunar eclipse The December 2010 lunar eclipse occurred from 5:27 to 11:06 UTC on December 21, 2010, coinciding with the date of the December solstice. It was visible in its entirety as a total lunar eclipse in North and South America, Iceland, Ireland, Britain and northern Scandinavia. The eclipse of December 2010 was the first total lunar eclipse in almost three years, since the February 2008 lunar eclipse. It is the second of two lunar eclipses in 2010.

neg: Solar Saros 139 it will produce the longest total eclipse calculated for the ten millennia from 3999 BCE to 6000 CE. The last eclipse to occur was a total eclipse on March 29, 2006, lasting 4 minutes 7 seconds and passing over portions of Africa and western Asia. The next eclipse will occur on April 8, 2024, lasting 4 minutes 28 seconds over central North America, entering in Mexico, crossing the United States, and leaving in eastern Canada. Solar Saros 139 Solar Saros 139 repeats every 18 years, 11 days. Saros 139 contains 71 events of which 16 will be partial eclipses, 12

neg: Solar eclipse of February 3, 1859 Indian and the Atlantic oceans. It showed about up to 1% obscurity in Antarctica and 4-5% in a part of the Pacific. The greatest eclipse was nearly about a third between Antarctica and South America at 62.4 S and 72.1 W at 1:22 UTC (8:36 PM local time on February 2). The subsolar marking was in the Pacific Ocean about a third of the way between New Caledonia and the Solomon Islands. Solar eclipse of February 3, 1859 A partial solar eclipse occurred on February 3, 1859 during summer. A solar eclipse occurs when the Moon passes between Earth and

neg: Solar eclipse of November 13, 2012 Solar eclipse of November 13, 2012 A total solar eclipse took place on 13–14 November 2012 (UTC). Because it crossed the International Date Line it began in local time on November 14 west of the date line over northern Australia, and ended in local time on November 13 east of the date line near the west coast of South America. Its greatest magnitude was 1.0500, occurring only 12 hours before perigee, with greatest eclipse totality lasting just over four minutes. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image

neg: Solar eclipse of July 11, 2010 the sun by about 98 percent. The path of totality of this eclipse barely missed some significant inhabited islands, including passing just about 20 km north of the northern end of Tahiti. This eclipse was the first one to happen over French Polynesia in 350 years. An estimated 5,000 tourists visited various islands in the archipelago to observe the event. Nearly 120,000 pairs of special glasses were distributed for observers. Eclipse chasers were also able to observe the eclipse at El Calafate, near the southern tip of Argentina, before the sun set just two minutes later. Several hours after the

neg: Solar eclipse of March 25, 1819 in the Pacific at 61.2 S, 87.9 W at 23:44 UTC (5:15 PM local time). The subsolar marking was in the Pacific just north of the Equator. Solar eclipse of March 25, 1819 A partial solar eclipse occurred on March 25, 1819 in the first days of fall. 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

neg: Historically significant lunar eclipses resident of Hartford, Connecticut, after a blow to the head, awakens to find himself inexplicably transported back in time to early medieval England at the time of the legendary King Arthur. When Morgan is about to be burned at the stake, he pretends to conjure a solar eclipse that he knew was about to happen; this prediction saves Morgan's life. Another novel that used a solar-eclipse scene modeled after Columbus' lunar eclipse was Bolesław Prus' historical novel, "Pharaoh". A similar plot also features in "The Adventures of Tintin" comic "Prisoners of the Sun". The Ross Sea party was a component

neg: June 2011 lunar eclipse Philippines, the lunar eclipse was visible just before sunrise. It was very visible in the clear and cloudless night sky throughout eastern and southeast Asia. Africa, far eastern Russia and Europe witnessed the whole event even in the late stages (as in partial lunar eclipse). The Americas (including North and northwestern South America) missed the eclipse completely (except in most areas) because it occurred at moonset. It was preceded by the partial solar eclipse of January 4, 2011, and the partial solar eclipse of June 1, 2011. This eclipse is the center of nine lunar eclipses in a short-lived series.

neg: Solar eclipse of April 5, 1837 at 61.3 S, 145.6 E at 7:36 UTC (4:36 PM local time). The subsolar marking was in the Indian Ocean north of the Equator. Solar eclipse of April 5, 1837 A partial solar eclipse occurred on April 5, 1837 during fall. 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 first of three partial eclipses that

neg: Solar eclipse of April 19, 1939 path of annularity passed over the North Pole. Land covered in the path include part of Alaska, Canada, and Franz Josef Land, Ushakov Island and Vize Island in the Soviet Union (today's Russia). Solar eclipse of April 19, 1939 An annular solar eclipse occurred on April 19, 1939. 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

neg: Solar eclipse of August 18, 1868 line even without the need for an eclipse. The same result was found independently by British astronomer Norman Lockyer, and both Janssen's and Lockyer's communications were presented to the French Academy of Sciences on October 26, 1868. King Mongkut, also known as Rama IV of Siam, was able to calculate and predict the solar eclipse two years earlier. The calculations were correct as to the place, the time and the type of the solar eclipse that would happen. The eclipse took place precisely as the king had predicted, the total phase lasting six minutes and 46 seconds. In fact, his

neg: June 2010 lunar eclipse seen before sunrise on Saturday morning setting over western North and South America: This eclipse is the one of five lunar eclipses in a short-lived series. The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of the date shift, the Earth's shadow will be about 11 degrees west in sequential events. A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 127. Photos: June 2010 lunar

neg: Solar eclipse of February 7, 2008 significant partial eclipse was visible over New Zealand and a minor partial eclipse was seen from southeastern Australia. For most solar eclipses the path of centrality moves eastwards. In this case the path moved west round Antarctica and then north. The best land-based visibility outside of Antarctica was from New Zealand. Professional astronomer and eclipse-chaser Jay Pasachoff observed it from Nelson, New Zealand, 60% coverage, under perfect weather. <BR>Animated path Solar eclipse of February 7, 2008 An annular solar eclipse occurred on February 7, 2008. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally

neg: July 1953 lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 135. July 1953 lunar eclipse A total lunar eclipse took place on July 26, 1953. The Moon passed through the very center of the Earth's shadow. It could be completely seen from Australia, seen rising over eastern Asia, and seen setting over North and South America. Lunar Saros 128 contains 15 total lunar eclipses between 1845 and 2097 (in years 1845, 1867, 1881, 1899, 1917, 1935, 1953, 1971, 1989, 2007,

neg: Solar eclipse of October 23, 1976 border with Burundi, with the path of totality passing just north of the large Tanzanian city of Dar es Salaam. It then crossed the Indian Ocean, passing St. Pierre Island, Providence Atoll and Farquhar Atoll of Seychelles before making landfall in southeastern Australia. The largest city that saw totality was Melbourne. After leaving the Australian mainland, the path of totality left the Earth's surface just north of the north island of New Zealand. Solar eclipse of October 23, 1976 A total solar eclipse occurred on October 23, 1976. A solar eclipse occurs when the Moon passes between Earth and the

neg: Solar eclipse of August 7, 1812 at sunset in northeastern Antarctica. It showed about up to 10% obscurity in one part of the Indian Ocean, and up to 30% obscurity of the sun in Antarctica. The greatest eclipse was in the southwest portion of Indian Ocean just north of Antarctica. Solar eclipse of August 7, 1812 A partial solar eclipse occurred on August 7, 1812 during winter. 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

neg: Solar eclipse of May 9, 1948 of the Nicobar Islands, and Burma, Thailand including Bangkok, French Indochina (the part now belonging to Laos), North Vietnam (now belonging to Vietnam), China, South Korea, Rebun Island in Japan, Kuril Islands in the Soviet Union (now belonging to Russia), and Alaska. It was the first central solar eclipse visible from Bangkok from 1948 to 1958, where it is rare for a large city to witness 4 central solar eclipses in just 10 years. Solar eclipse of May 9, 1948 An annular solar eclipse occurred on May 9, 1948. A solar eclipse occurs when the Moon passes between Earth and