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April 2013 Lunar Eclipse
A partial lunar eclipse took place on 25 April 2013, the first of three lunar eclipses in 2013. Only a tiny sliver (1.48%) of the Moon was covered by the Earth's umbral shadow at maximum eclipse, but the entire northern half of the Moon was darkened from being inside the penumbral shadow. This was one of the shortest partial eclipses of the Moon for the 21st century, lasting 27 minutes. This was the last of 58 umbral lunar eclipses of Lunar Saros 112. Visibility It was visible over Europe, Africa, Asia, and Australia. Gallery File:April Moon Partial Lunar Eclipse 2013 (8681604874).jpg, From Melbourne, Australia, 18:42 UTC Eclipse parcial de luna (8686734152).jpg, From Las Palmas, Canary Islands, 20:05 UTC Partial Lunar Eclipse (8680925175).jpg, From Essex, England, 20:06 UTC -i---i- (8682223072).jpg, From Arinaga, Canary Islands, 20:07 UTC Lune moon (8683076272).jpg, From Foncquevillers, France, 20:08 UTC 2013-04-25 21-09-18-ecl-lune.gif, From Belfort, France, combined ...
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Rabka-Zdrój
Rabka-Zdrój (, in Goral dialects: ''Robka'', colloquially: ''Rabka'') is a spa town in Lesser Poland Voivodeship, Poland. It is located between Kraków and Zakopane in a valley on the northern slopes of the Gorce Mountains, where the rivers Poniczanka and Słonka join the river Raba. It has about 13,000 inhabitants. There is a substantial population of Gorals in the town. Rabka was always known for its salt-works, and from 1864 became a popular spa town. The first treatment centre for children was established a few years later and continues to this day. Hydrotherapy continues to be utilised in local hospital and sanatoriums. The Władysław Orkan Museum established in a former 17th-century larch-wood church, includes a collection of folk sculpture and paintings on glass. It also houses the "Order of the Smile Museum" (which children award to adults) and hosts events such as a winter carnival, the Carpathian Festival of Children's Regional Ensembles and the Mountain Children's H ...
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SE2004Apr19P
SE, Se, or Sé may refer to: Arts and entertainment * ''Sé'' (album), by Lúnasa, 2006 * Se (instrument), a traditional Chinese musical instrument Businesses and organizations * Sea Ltd (NYSE: SE), tech conglomerate headquartered in Singapore * Slovenské elektrárne, electric utility company in Slovakia * Societas Europaea, a European Union public company * XL Airways France, IATA airline designator SE * Southeastern (train operating company), or SE Trains Limited, in England Places * Sè, Atlantique, Benin * Sè, Mono, Benin *Subprefecture of Sé, São Paulo, Brazil **Sé (district of São Paulo) **Sé (São Paulo Metro), a station *Sé, Hungary *Sé, Macau *Sé (Angra do Heroísmo), Terceira, Azores, Portugal *Sé (Braga), Portugal *Sé (Bragança), Faro, Portugal * Sé (Funchal), Madeira, Portugal *Sé, Lamego, Portugal *Sé (Lisbon), Portugal *Sé, Portalegre, Portugal * Sé (Porto), Portugal * SE postcode area, London, England * Sergipe (SE), a state of Brazil * Swe ...
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Solar Eclipse Of April 30, 2022
A partial solar eclipse took place on April 30, 2022. A solar eclipse occurs when the Moon passes between Earth and the Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ..., 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. Images Animated path Related eclipses Eclipses of 2022 * A total lunar eclipse on May 16. * A partial solar eclipse on October 25. * A total lunar eclipse on November 8. Solar eclipses of 2022–2025 Saros 119 It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 15, 850 AD. It contains total eclipses on Augu ...
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Solar Eclipse Of April 19, 2004
A partial solar eclipse took place on 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 could also be seen in southern Africa at sunset. Considering the magnitude and the solar altitude, South Africa was the best place to observe this eclipse. In Cape Town, the sun was about 40% obscured, while in Pretoria the sun was 29% obscured. Further north, the eclipse remained visible up to Angola, southern DR Congo and Tanzania. Images Animated eclipse path Related eclipses Eclipse season An eclipse season is the period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axi ...
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Solar Saros 119
Saros cycle series 119 for solar eclipse A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six month ...s occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's ascending node. It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012 with a hybrid eclipse on August 31, 1030. It has annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on ...
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Saros (astronomy)
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. One saros period after an eclipse, the Sun, Earth, and Moon return to approximately the same relative geometry, a near straight line, and a nearly identical eclipse will occur, in what is referred to as an eclipse cycle. A sar is one half of a saros. A series of eclipses that are separated by one saros is called a ''saros series''. It corresponds to: *6,585.321347 solar days *18.029 years *223 synodic months *241.999 draconic months *18.999 eclipse years (38 eclipse seasons) *238.992 anomalistic months The 19 eclipse years means that if there is a solar eclipse (or lunar eclipse), then after one saros a new moon will take place at the same node of the orbit of the Moon, and under these circumstances another eclipse can occur. History The earliest disco ...
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Lunar Year
A lunar calendar is a calendar based on the monthly cycles of the Moon's phases (synodic months, lunations), in contrast to solar calendars, whose annual cycles are based only directly on the solar year. The most commonly used calendar, the Gregorian calendar, is a solar calendar system that originally evolved out of a lunar calendar system. A purely lunar calendar is also distinguished from a lunisolar calendar, whose lunar months are brought into alignment with the solar year through some process of intercalation. The details of when months begin vary from calendar to calendar, with some using new, full, or crescent moons and others employing detailed calculations. Since each lunation is approximately  days, (which gives a mean synodic month as 29.53059 days or 29 days 12 hours 44 minutes and 3 seconds) it is common for the months of a lunar calendar to alternate between 29 and 30 days. Since the period of 12 such lunations, a lunar year, is 354 days, 8 ho ...
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Solar Eclipse Of November 3, 2013
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. In this particular case the eclipse path starts out as annular and ends as total. It was the 23rd eclipse of the 143rd Saros cycle, which began with a partial eclipse on March 7, 1617, and will conclude with a partial eclipse on April 23, 2897. Viewing Totality was visible from the northern Atlantic Ocean (east of Florida) to Africa (Gabon (landfall), R. Con ...
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October 2013 Lunar Eclipse
A penumbral lunar eclipse took place on 18–19 October 2013, the last of three lunar eclipses in 2013. Visibility It was visible from the Americas (for the end), Europe, Africa, and most of Asia (the beginning of the eclipse was visible in east Asia). The western part of the Philippines (including western Luzon and Palawan) could see the penumbral eclipse at moonset. Photo Penumbral Eclipse in very cloudy skies. (10354279925).jpg, Kennesaw, Georgia, 0:16 UTC Related eclipses Eclipses of 2013 * A partial lunar eclipse on 25 April. * An annular solar eclipse on 10 May. * A penumbral lunar eclipse on 25 May. * A penumbral lunar eclipse on 18 October. * A hybrid solar eclipse on 3 November. This eclipse is the one of four lunar eclipses in a short-lived series at the descending node of the moon's orbit. 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 ...
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May 2013 Lunar Eclipse
A penumbral lunar eclipse took place on 24–25 May 2013, the second of three lunar eclipses in 2013. It was visually imperceptible due to the small entry into the penumbral shadow. This event marked the beginning of Saros series 150. Visibility A simulated view of the earth from the center of the moon at maximal eclipse. Map Gallery File:Penumbral eclipse of May 25, 2013 from lunar south pole.gif, Animation of the eclipse viewed from South pole of the Moon Related eclipses Eclipses of 2013 * A partial lunar eclipse on 25 April. * An annular solar eclipse on 10 May. * A penumbral lunar eclipse on 25 May. * A penumbral lunar eclipse on 18 October. * A hybrid solar eclipse on 3 November. Lunar year (354 days) 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 i ...
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Solar Eclipse Of May 10, 2013
An annular solar eclipse took place at the Moon's descending node of the orbit on Friday, May 10, 2013 (Thursday, May 9, 2013 if observed east of International Date Line), with a magnitude of 0.9544. 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 the 31st eclipse of the 138th Saros cycle, which began with a partial eclipse on June 6, 1472 and will conclude with a partial eclipse on July 11, 2716. Visibility Annularity was visible from a 171 to 225 kilometre-wide track that traversed Australia, eastern Papua New Guinea, the Solomon Islands, and the Gilbert Islands, with the maximum of 6 minut ...
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