List Of Solar Eclipses In The 19th Century
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List Of Solar Eclipses In The 19th Century
This is a list of solar eclipses in the 19th century. During the period 1801 to 1900 there were 242 solar eclipses of which 87 were partial, 77 were annular, 63 were total, and 15 were hybrids. The greatest number of eclipses in one year was five, in 1805, and two months, January 1805 and December 1880, had two eclipses. References {{DEFAULTSORT:Solar eclipses in the 19th century * 19th century-related lists +19 ...
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The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research. NASA was established in 1958, succeeding the National Advisory Committee for Aeronautics (NACA), to give the U.S. space development effort a distinctly civilian orientation, emphasizing peaceful applications in space science. NASA has since led most American space exploration, including Project Mercury, Project Gemini, the 1968-1972 Apollo Moon landing missions, the Skylab space station, and the Space Shuttle. NASA supports the International Space Station and oversees the development of the Orion spacecraft and the Space Launch System for the crewed lunar Artemis program, Commercial Crew spacecraft, and the planned Lunar Gateway space station. The agency is also responsible for the Launch Services Program, which provides oversight of launch operations and countdown management f ...
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Solar Eclipse Of July 28, 1851
The earliest scientifically useful photograph of a total solar eclipse was made by Julius Berkowski at the Royal Observatory in Königsberg, Prussia, on July 28, 1851. This was the first occasion that an accurate photographic image of a solar eclipse was recorded. Background A solar eclipse occurs when the Moon passes between the Earth and the Sun, casting a shadow on Earth that temporarily obscures part or all of the Sun's disc. Eclipses can occur only when all three bodies are properly aligned. Partial eclipses, in which only a portion of the Sun's surface is obscured, are relatively common due to the width of the Moon's outer shadow, or penumbra, which may be several hundred miles wide. Total eclipses occur when the Moon's inner shadow, or umbra, reaches the surface of the Earth, completely obscuring the Sun over a much narrower portion of the ground. If the Moon is too far away at the time of an eclipse, its umbra may not reach the Earth's surface, and only a partial eclip ...
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Solar Eclipse Of August 18, 1868
A total solar eclipse occurred on August 18, 1868, also known as "The King of Siam's 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 in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Observations Solar eclipse 1868Aug18-Bullock.png, Bullock sketch of the eclipse, ''Total Eclipses of the Sun'', 1900. Sketches of the total solar eclipse, 1868 (19745966082).jpg, M. Stephan sketches of the eclipse, ''Archives des missions scientifiques et littéraires'', 1868. Map of the solar eclipse of August 18, 1868 (19757912091).jpg, Map of the forecast path of the total eclipse, ''Archives des missions scientifiques et littéraires'', ...
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Solar Eclipse Of August 29, 1867
A total solar eclipse occurred on August 29, 1867. 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 occurred across central Argentina and the southern Atlantic ocean. Observations José J. Vergara and Luis Grosch observed the eclipse from a small hill close to Santiago. Related eclipses It is a part of solar Saros 123 Saros cycle The saros () is a period of exactly 223 synodic months, approximately 6585.3211 days, or 18 years, 10, 11, or 12 days (depending on the number of leap years), and 8 hours, that can be used to predict eclipses of the Sun and Moon. On .... Refer ...
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Solar Eclipse Of October 19, 1865
An annular solar eclipse occurred on October 19, 1865. 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 (mathematics), annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Description The greatest eclipse was at 16:21:14 UTC (12:21 local time) at 21.3°N 60.2°W northeast of Antigua and Barbuda and lasted 9 min 27 sec. The maximum width of band was 326 km (203 mi). The eclipse was visible in North America (except for the Yukon, Alaska and the northernmost part of Greenland), Central America, the Caribbean South America including, the northern parts of Peru and Bolivia and most of Brazil, the westernmost parts of Africa and Europe (westernmost Sp ...
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Solar Eclipse Of April 25, 1865
A total solar eclipse occurred on April 25, 1865. 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. Observations The total eclipse was also witnessed by the passengers and crew of the SS Great Britain SS ''Great Britain'' is a museum ship and former passenger steamship that was advanced for her time. She was the largest passenger ship in the world from 1845 to 1854. She was designed by Isambard Kingdom Brunel (1806–1859), for the Great W ..., passing the coastline of Brazil en route from Australia to England; they were able to observe stars in the daytime. Related eclipses Sar ...
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Solar Eclipse Of November 11, 1863
An annular solar eclipse occurred on November 11, 1863, during 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. 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. Parts of the areas near the Indian Ocean occurred where the solar eclipse occurred on November 21, 1862. It was part of the solar saros 121 Description The eclipse took place in Africa including Namacqualand (then also South-West Africa, now Namibia), Bechuanaland (now Botswana) South Africa (which included the British colonies and the Boer states at the time), Basutoland (parts now Lesotho), Zululand (now part of KwaZulu-Natal, South Africa) and portions of Swaziland. The rest too ...
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Solar Eclipse Of July 18, 1860
A total solar eclipse occurred on July 18, 1860. 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. Coronal Mass Ejection The first coronal mass ejection may have been observed as coronal loops progressing during this total eclipse. Related eclipses It is a part of solar Saros 124. Tritos series See also *Solar storm of 1859 The Carrington Event was the most intense geomagnetic storm in recorded history, peaking from 1 to 2 September 1859 during solar cycle 10. It created strong auroral displays that were reported globally and caused sparking and even fires in mult ... Refe ...
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Solar Eclipse Of January 23, 1860
An annular solar eclipse occurred on January 23, 1860 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. 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. Description The eclipse was visible in much of the South Island and the southernmost portion of North Island around Wellington in New Zealand, it was also visible in all of Antarctica (much of the areas had a 24-hour daylight), South America's Patagonia and Oceanian islands such as Macquarrie, Chatham, Antipodes, Tahiti and Tuamotu It was part of solar saros 119. On the other side as the Moon from the Earth headed towards the left at New Zealand, as the umbral path was outside the South ...
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Solar Eclipse Of September 7, 1858
A total solar eclipse occurred on September 7, 1858. 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 was visible across South America. Observations Emmanuel Liais from Brazil Brazil ( pt, Brasil; ), officially the Federative Republic of Brazil (Portuguese: ), is the largest country in both South America and Latin America. At and with over 217 million people, Brazil is the world's fifth-largest country by area ... Related eclipses Saros series 142 Notes References NASA graphic*Googlemap*NASA Besselian elementsby Lieut. J. M. Gillis, Published by the Smithsonian Ins ...
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Solar Eclipse Of March 25, 1857
A total solar eclipse occurred on March 25, 1857. 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 began at sunrise over southeastern Australia on March 26 (Thursday), crossing the Pacific ocean, and ended near sunset across Mexico on March 25 (Wednesday). Related eclipses Saros series 127 Notes References NASA graphic*Googlemap*NASA Besselian elements* Observations made at Sydney during the Eclipse of the Sun, March 26, 1857Clarke, W. B., Monthly Notices of the Royal Astronomical Society ''Monthly Notices of the Royal Astronomical Society'' (MNRAS) is a peer-reviewed ...
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Solar Eclipse Of November 9, 1855
A partial solar eclipse occurred on November 9, 1855 during 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 eighth solar saros 150 cycle of eclipses Description The eclipse was visible in Tasmania and the southeasternmost areas of Australia, New Zealand and its surrounding islands such as Chatham and Cook and much of Antarctica which most areas had a 24-hour daylight with the exception of the northernmost peninsular area (from the areas south of the Antarctic Circie) and its surrounding islands and the northernmost area at the 50th meridian east. It included a tiny southeast area of the Indian Ocean, the southwesternmost of the Pacific and the tiny portion of the southernmost Atlantic. The eclipse started at sunrise west of New Zealand and e ...
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