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October 2052 Lunar Eclipse
A partial lunar eclipse will occur at the Moon’s Lunar node, descending node of orbit on Tuesday, October 8, 2052, with an umbral Magnitude of eclipse, magnitude of 0.0821. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 2.1 days before Apsis, perigee (on October 10, 2052, at 11:35 UTC), the Moon's apparent diameter will be larger. Visibility The eclipse will be completely visible over northeast Asia, eastern Australia, and western North America, seen rising over east Asia, east and south Asia and western Australia and setting over eastern North America and much of South America. Eclipse details Shown below is a tab ...
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Lunar Eclipse
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. Such an alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to Ecliptic, the plane of the Earth's orbit. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy (astronomy), syzygy) with Earth between the other two, which can happen only on the night of a full moon when the Moon is near either lunar node. The type and length of a lunar eclipse depend on the Moon's proximity to the lunar node. When the Moon is totally eclipsed by the Earth (a "deep eclipse"), "What is a deep eclipse? The smaller star is behind the bigger star" it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon's surface, as the only light that is diffuse reflection, reflected from ...
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Fortnight
A fortnight is a unit of time equal to 14 days (two weeks). The word derives from the Old English term , meaning "" (or "fourteen days", since the Anglo-Saxons counted by nights). Astronomy and tides In astronomy, a ''lunar fortnight'' is half a lunar synodic month, which is equivalent to the mean period between a full moon and a new moon (and vice versa). This is equal to 14.77 days. It gives rise to a lunar fortnightly tidal constituent (see: Long-period tides). Analogs and translations In many languages, there is no single word for a two-week period, and the equivalent terms "two weeks", "14 days", or "15 days" ( counting inclusively) have to be used. * Celtic languages: in Welsh, the term ''pythefnos'', meaning "15 nights", is used. This is in keeping with the Welsh term for a week, which is ''wythnos'' ("eight nights"). In Irish, the term is ''coicís''. * Similarly, in Greek, the term δεκαπενθήμερο (''dekapenthímero''), meaning "15 days", is used. * ...
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November 2041 Lunar Eclipse
A partial lunar eclipse will occur at the Moon’s ascending node of orbit on Friday, November 8, 2041, with an umbral magnitude of 0.1714. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 2.7 days after perigee (on November 5, 2041, at 10:50 UTC), the Moon's apparent diameter will be larger. Visibility The eclipse will be completely visible over North and South America, western Europe, and west Africa, seen rising over the central Pacific Ocean and setting over much of Africa, eastern Europe, the Middle East, and central Asia. Eclipse details Shown below is a table displaying details about this particular eclipse. It ...
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Solar Eclipse Of October 13, 2061
An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, October 13, 2061, with a magnitude of 0.9469. 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. Occurring about 1.1 days before apogee (on April 21, 2061, at 4:00 UTC), the Moon's apparent diameter will be smaller. The path of annularity will be visible from parts of southern Chile, southern Argentina, the Falkland Islands, and Antarctica. A partial solar eclipse will also be visible for much of South America and Antarctica. Eclipse details Shown below are two tables displaying details about this particular solar ...
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Solar Eclipse Of October 3, 2043
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, October 3, 2043, with a magnitude of 0.9497. 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. Occurring about 4.8 days before apogee (on October 7, 2043, at 23:20 UTC), the Moon's apparent diameter will be smaller. It will be unusual in that while it is an annular solar eclipse, it is not a central solar eclipse. A ''non-central'' eclipse is one where the center-line of annularity does not intersect the surface of the Earth (when the gamma is between 0.9972 and 1.0260). Instead, the center line passes just above the ...
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November 2059 Lunar Eclipse
November is the eleventh and penultimate month of the year in the Julian and Gregorian calendars. Its length is 30 days. November was the ninth month of the calendar of Romulus . November retained its name (from the Latin ''novem'' meaning "nine") when January and February were added to the Roman calendar. November is a month of late spring in the Southern Hemisphere and late autumn in the Northern Hemisphere. Therefore, November in the Southern Hemisphere is the seasonal equivalent of May in the Northern Hemisphere and vice versa. In Ancient Rome, Ludi Plebeii was held from November 4–17, Epulum Jovis was held on November 13 and Brumalia celebrations began on November 24. These dates do not correspond to the modern Gregorian calendar. November was referred to as Blōtmōnaþ by the Anglo-Saxons. Brumaire and Frimaire were the months on which November fell in the French Republican calendar. Astronomy November meteor showers include the Andromedids, which occurs from ...
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August 2045 Lunar Eclipse
A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, August 27, 2045, with an umbral magnitude of −0.3899. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 1.6 days after apogee (on August 26, 2045, at 0:10 UTC), the Moon's apparent diameter will be smaller. Visibility The eclipse will be completely visible over east Asia and Australia, seen rising over east Africa and west, central, and south Asia and setting over western North America. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse. Eclipse ...
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July 2056 Lunar Eclipse
July is the seventh month of the year in the Julian and Gregorian calendars. Its length is 31 days. It was named by the Roman Senate in honour of Roman general Julius Caesar in 44 B.C., being the month of his birth. Before then it was called Quintilis, being the fifth month of the calendar that started with March. It is on average the warmest month in most of the Northern Hemisphere, where it is the second month of summer, and the coldest month in much of the Southern Hemisphere, where it is the second month of winter. The second half of the year commences in July. In the Southern Hemisphere, July is the seasonal equivalent of January in the Northern hemisphere. "Dog days" are considered to begin in early July in the Northern Hemisphere, when the hot sultry weather of summer usually starts. Spring lambs born in late winter or early spring are usually sold before 1 July. Symbols July's birthstone is the ruby, which symbolizes contentment. Its birth flowers are the lar ...
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December 2048 Lunar Eclipse
A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, December 20, 2048, with an umbral magnitude of −0.1420. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 13 hours before apogee (on December 20, 2048, at 19:30 UTC), the Moon's apparent diameter will be smaller. Visibility The eclipse will be completely visible over North America and much of South America, seen rising over northeast Asia and the western Pacific Ocean and setting over west and central Africa and Europe. Eclipse details Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pe ...
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April 2052 Lunar Eclipse
A penumbral lunar eclipse will occur at the Moon’s Lunar node, ascending node of orbit on Sunday, April 14, 2052, with an umbral Magnitude of eclipse, magnitude of −0.1294. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 2.4 days before Apsis, apogee (on April 16, 2052, at 13:00 UTC), the Moon's apparent diameter will be smaller. Visibility The eclipse will be completely visible over eastern North America, South America, western Europe, and west Africa, seen rising over western and central North America and setting over east Africa, eastern Europe, and west Asia, west, central Asia, central, and south Asia. Eclipse details Shown below i ...
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Solar Eclipse Of March 30, 2052
A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, March 30, 2052, with a magnitude of 1.0466. 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 about 1.5 days before perigee (on April 1, 2052, at 6:30 UTC), the Moon's apparent diameter will be larger. The path of totality will be visible from parts of central Mexico, the extreme southern tip of Texas, southeastern Louisiana, southeastern Alabama, Florida, Georgia, and South Carolina. A partial solar eclipse will also be visible for parts of Hawaii, North America, Central America, the Caribbean, ...
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Lunar Eclipse
A lunar eclipse is an astronomical event that occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. Such an alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to Ecliptic, the plane of the Earth's orbit. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy (astronomy), syzygy) with Earth between the other two, which can happen only on the night of a full moon when the Moon is near either lunar node. The type and length of a lunar eclipse depend on the Moon's proximity to the lunar node. When the Moon is totally eclipsed by the Earth (a "deep eclipse"), "What is a deep eclipse? The smaller star is behind the bigger star" it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon's surface, as the only light that is diffuse reflection, reflected from ...
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