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Lunar Saros 124
Saros cycle series 124 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 73 member events, with 28 total eclipses, starting in 1657 and ending in 2144. The order is 20 penumbral, 8 partial, 28 total, 8 partial, 9 penumbral. This lunar saros is linked to Solar Saros 131. See also * List of lunar eclipses ** List of Saros series for lunar eclipses Notes External links www.hermit.org: Saros 124 {{Lunar eclipses Lunar saros series ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Eclipse Lunar Total 21
An eclipse is an astronomical event which occurs when an astronomical object or spacecraft is temporarily obscured, by passing into the shadow of another body or by having another body pass between it and the viewer. This alignment of three celestial objects is known as a syzygy (astronomy), ''syzygy''. An eclipse is the result of either an ''occultation'' (completely hidden) or a transit (astronomy), ''transit'' (partially hidden). A "deep eclipse" (or "deep occultation") is when a small astronomical object is behind a bigger one. "What is a deep eclipse? The smaller star is behind the bigger star" The term ''eclipse'' is most often used to describe either a solar eclipse, when the Moon's shadow crosses the Earth's surface, or a lunar eclipse, when the Moon moves into the Earth's shadow. However, it can also refer to such events beyond the Earth–Moon system: for example, a planet moving into the shadow cast by one of its moons, a moon passing into the shadow cast by its hos ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
December 1963 Lunar Eclipse
A total lunar eclipse occurred at the Moon’s Lunar node, ascending node of orbit on Monday, December 30, 1963, with an umbral Magnitude of eclipse, magnitude of 1.3350. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's Umbra, penumbra and antumbra, shadow is smaller. Occurring about 1.5 days after Apsis, perigee (on December 29, 1963, at 0:10 UTC), the Moon's apparent diameter was larger. Visibility The eclipse was completely visible over northeast Asia and much of North America, seen rising over much of Asia and Australi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
List Of Lunar Eclipses
__NOTOC__ A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. By type * List of central lunar eclipses * Total penumbral lunar eclipse By classification * List of saros series for lunar eclipses – counts by saros (astronomy), saros number * Tetrad (astronomy), Tetrad – four total lunar eclipses within two years By era * Lunar eclipses by century * Historically significant lunar eclipses * List of lunar eclipses in the 19th century * List of lunar eclipses in the 20th century * List of lunar eclipses in the 21st century * List of lunar eclipses in the 22nd century See also * Lists of solar eclipses {{DEFAULTSORT:Lunar eclipses Lists of lunar eclipses, ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
May 2198 Lunar Eclipse
May is the fifth month of the year in the Julian and Gregorian calendars. Its length is 31 days. May is a month of spring in the Northern Hemisphere, and autumn in the Southern Hemisphere. Therefore, May in the Southern Hemisphere is the seasonal equivalent of November in the Northern Hemisphere and vice versa. Late May typically marks the start of the summer vacation season in the United States (Memorial Day) and Canada (Victoria Day) that ends on Labor Day, the first Monday of September. May (in Latin, ''Maius'') was named for the Greek goddess Maia, who was identified with the Roman era goddess of fertility, Bona Dea, whose festival was held in May. Conversely, the Roman poet Ovid provides a second etymology, in which he says that the month of May is named for the ''maiores,'' Latin for "elders", and that the following month (June) is named for the ''iuniores,'' or "young people" (''Fasti VI.88''). Eta Aquariids meteor shower appears in May. It is visible from about A ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
