|
March 2006 Lunar Eclipse
A penumbral lunar eclipse took place on 14 March 2006, the first of two lunar eclipses in 2006. This was a relatively rare total penumbral lunar eclipse with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. The tables below contain detailed predictions and additional information on the Penumbral Lunar Eclipse of 14 March 2006. Visibility It was completely visible over Africa and Europe, seen rising over eastern North America, all of South America, and setting over western Asia. A simulated view of the Earth from the center of the Moon at maximum eclipse. Map Relation to other lunar eclipses Eclipses of 2006 * A penumbral lunar eclipse on 14 March. * A total solar eclipse on 29 March. * A partial lunar eclipse on 7 September. * An annular solar eclipse on 22 September. Lunar year series (354 days) Saros series The eclipse belongs to Saros series 113, and is the 63rd of 71 lunar eclipses in the series. The firs ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lunar Eclipse (114948858)
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 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, it takes on a reddish color that is caused by the planet when it completely blocks direct sunlight from reaching the Moon surface, as only the light diffuse reflection, reflected from the lunar surface has been atmospheric refraction, refracted by Earth's atmosphere. This light appears ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
21st-century Lunar Eclipses
The 1st century was the century spanning AD 1 ( I) through AD 100 ( C) according to the Julian calendar. It is often written as the or to distinguish it from the 1st century BC (or BCE) which preceded it. The 1st century is considered part of the Classical era, epoch, or historical period. The 1st century also saw the appearance of Christianity. During this period, Europe, North Africa and the Near East fell under increasing domination by the Roman Empire, which continued expanding, most notably conquering Britain under the emperor Claudius (AD 43). The reforms introduced by Augustus during his long reign stabilized the empire after the turmoil of the previous century's civil wars. Later in the century the Julio-Claudian dynasty, which had been founded by Augustus, came to an end with the suicide of Nero in AD 68. There followed the famous Year of Four Emperors, a brief period of civil war and instability, which was finally brought to an end by Vespasian, ninth Roman emperor, a ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
May 2004 Lunar Eclipse
A total lunar eclipse took place on Tuesday 4 May 2004, the first of two total lunar eclipses in 2004, the second being on October 2004 lunar eclipse, 28 October 2004. Visibility It was visible throughout most of Europe and Asia, eastern Africa, Indian Ocean and western South America including the Pacific Ocean. The eclipse seen in eastern Asia before sunrise and western South America after sunset. The eclipse was seen over and the Philippines at dawn. Mid Eclipse was visible during moonset in Eastern Australia. Related lunar eclipses Eclipse season This is the second eclipse this season. First eclipse this season: Solar eclipse of April 19, 2004, 19 April 2004 Partial Solar Eclipse Eclipses of 2004 * Solar eclipse of April 19, 2004, A partial solar eclipse on 19 April. * A total lunar eclipse on 4 May. * Solar eclipse of October 14, 2004, A partial solar eclipse on 14 October. * October 2004 lunar eclipse, A total lunar eclipse on 28 October. Lunar year series It ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
November 2003 Lunar Eclipse
A total lunar eclipse took place on Sunday, November 9, 2003, the second of two total lunar eclipses in 2003, the first being on May 16, 2003. It is the first total lunar eclipse of 21st century which happened on a micromoon day. The Moon barely edged into total eclipse for 21 minutes and 58 seconds. With the Moon just 1.78% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours, 31 minutes and 25 seconds. Occurring only 1.4 days before apogee (Apogee on Monday, November 10, 2003), the Moon's apparent diameter was 6.4% smaller than average. This was the last of 14 total lunar eclipses of Lunar Saros 126, which started on 19 June 1769 and ended on 9 November 2003. Visibility It was completely visible over Americas, Europe, Africa and central Asia, seen rising over the Americas and setting over central Asia. Photo gallery Image:Eclipse01.jpg, Grand Rapids, MI, ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
May 2003 Lunar Eclipse
A total lunar eclipse took place on Friday, May 16, 2003, the first of two total lunar eclipses in 2003, the other being on November 9, 2003. A shallow total eclipse saw the Moon in relative darkness for 52 minutes and 3.1 seconds. The Moon was 12.938% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 15 minutes and 3.1 seconds in total. Occurring only 0.5 days after perigee (Perigee on Thursday, May 15, 2003), the Moon's apparent diameter was 6.2% larger than average. At greatest eclipse the Moon was only 357,693 km (222,260 mi) from the Earth, making it a Super Full Moon. This lunar eclipse is first of a ''tetrad'', four total lunar eclipses in series. The previous series was in 1985 and 1986, starting with a May 1985 lunar eclipse. The next one was in 2014 and 2015, starting with the April 15, 2014 lunar eclipse. Visibility It was completely visible over central Pacific, North America, Sout ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
List Of 21st-century Lunar Eclipses
There will be 230 lunar eclipses in the 21st century (2001–2100): 87 penumbral, 58 partial and 85 total. Eclipses are listed in sets by lunar years, repeating every 12 months for each node. Ascending node eclipses are given a red background highlight. See also: List of lunar eclipses, List of 20th-century lunar eclipses, and List of 22nd-century lunar eclipses List of lunar eclipses between 1998 and 2100 Eclipses from August 1998 are included to complete the first eclipse set. References This list was compiled with data calculated by Fred Espenak of NASA's GSFC. {{DEFAULTSORT:21st-Century Lunar Eclipses * Lunar eclipses Lunar eclipses A lunar eclipse occurs when the Moon moves into the Earth's shadow. Such alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to the plane of the Earth ... 21 Science timelines Lunar eclipses by time ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
List Of Lunar Eclipses
There are several lists of lunar eclipses On the Moon, by the Earth ; Type * List of central lunar eclipses * Total penumbral lunar eclipse ; Classification * List of saros series for lunar eclipses * Tetrad (astronomy) contains lists of tetrads in the late-20th and 21st centuries ; By era * Lunar eclipses by century * Historically significant lunar eclipses Historically significant lunar eclipses are eclipses of the Moon that are mentioned in historical accounts in connection with a significant event. Lunar eclipses are somewhat rare events, although not as rare as solar eclipses, because unlike sol ... On Earth, by the Moon {{DEFAULTSORT:Lunar eclipses ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Eclipse Season
An eclipse season is the period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axial parallelism of the Moon's tilted orbital plane ( tilted five degrees to the Earth's orbital plane), just as Earth's weather seasons are the result of the axial parallelism of Earth's tilted axis as it orbits around the Sun. During the season, the "lunar nodes" – the line where the Moon's orbital plane intersects with the Earth's orbital plane – aligns with the Sun and Earth, such that a solar eclipse is formed during the new moon phase and a lunar eclipse is formed during the full moon phase. Only two (or occasionally three) eclipse seasons occur during each year, and each season lasts about 35 days and repeats just short of six months later, thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. During the eclipse season, the Moon is at a low ecliptic latitude (less than around 1.5° north or ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
SE2015Mar20T
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 * Sweden, I ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
