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Silverton, Devon
Silverton is a large village and civil parish, about north of Exeter, in the English county of Devon. It is one of the oldest villages in Devon and dates from the first years of the Saxon occupation. It has been suggested that the medieval manor of Burn, within the modern parish of Silverton, may be the estate listed as Mylenburnan (Mill-on-the-Burn or Burn Mill) in the will of King Alfred the Great of 899, now in the British Library, in which it was left to his youngest son Athelweard (c. 880-922). In the year 2001, its population was 1,905, recounted to 1,494 at the United Kingdom Census 2011. The electoral ward with the same name had a population of 1,875 at the above census. The parish has two pubs: The Lamb and The Silverton Inn. The church, dating back to the fourteenth century, is dedicated to St Mary. It has a full set of bells that are rung regularly. Inside, the pews have doors at the end of each row which is unusual in this area. The village also has a further ...
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United Kingdom Census 2011
A Census in the United Kingdom, census of the population of the United Kingdom is taken every ten years. The 2011 census was held in all countries of the UK on 27 March 2011. It was the first UK census which could be completed online via the Internet. The Office for National Statistics (ONS) is responsible for the census in England and Wales, the General Register Office for Scotland (GROS) is responsible for the census in Scotland, and the Northern Ireland Statistics and Research Agency (NISRA) is responsible for the census in Northern Ireland. The Office for National Statistics is the executive office of the UK Statistics Authority, a non-ministerial department formed in 2008 and which reports directly to Parliament. ONS is the UK Government's single largest statistical producer of independent statistics on the UK's economy and society, used to assist the planning and allocation of resources, policy-making and decision-making. ONS designs, manages and runs the census in England an ...
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Silverton Railway Station
There are 22 disused railway stations in the between and , 12 of which have structures that can still be seen from passing trains. Most were closed in the 1960s but four of them, especially around , were replaced by stations on new sites. 13 stations remain open on the line today, but there have been proposals to reopen stations at Cullompton and Wellington. Background The route was opened by the Bristol and Exeter Railway in stages between 1841 and 1844. In 1876 this company was amalgamated with the Great Western Railway which, in turn, was nationalised into British Railways in 1948. It is now owned by Network Rail. Apart from the temporary station at Beam Bridge which was only used for a year, the earliest closures were in the Weston-super-Mare area in order to provide new facilities for the traffic to that town, which was much greater than predicted when the line was planned. The majority of the remaining closures followed Dr Beeching's ''Reshaping of British Railways'' r ...
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Saint-Thégonnec
Saint-Thégonnec (; br, Sant-Tegoneg) is a former commune in the Finistère department in Brittany in northwestern France. On 1 January 2016, it was merged into the new commune Saint-Thégonnec Loc-Eguiner.Arrêté préfectoral
23 December 2015 The village is noted for its very elaborate , one of a number in the area, which include and .


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St Mary's Church, Silverton, Devon 1
ST, St, or St. may refer to: Arts and entertainment * Stanza, in poetry * Suicidal Tendencies, an American heavy metal/hardcore punk band * Star Trek, a science-fiction media franchise * Summa Theologica, a compendium of Catholic philosophy and theology by St. Thomas Aquinas * St or St., abbreviation of "State", especially in the name of a college or university Businesses and organizations Transportation * Germania (airline) (IATA airline designator ST) * Maharashtra State Road Transport Corporation, abbreviated as State Transport * Sound Transit, Central Puget Sound Regional Transit Authority, Washington state, US * Springfield Terminal Railway (Vermont) (railroad reporting mark ST) * Suffolk County Transit, or Suffolk Transit, the bus system serving Suffolk County, New York Other businesses and organizations * Statstjänstemannaförbundet, or Swedish Union of Civil Servants, a trade union * The Secret Team, an alleged covert alliance between the CIA and American indust ...
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Patrick Moore
Sir Patrick Alfred Caldwell-Moore (; 4 March 1923 – 9 December 2012) was an English amateur astronomer who attained prominence in that field as a writer, researcher, radio commentator and television presenter. Moore was president of the British Astronomical Association; co-founder and president of the Society for Popular Astronomy; author of over seventy books on astronomy; and presenter of the world's longest-running television series with the same original presenter, BBC's ''The Sky at Night'' (from 1957). He became known as a specialist in Moon observation and for creating the Caldwell catalogue. Idiosyncrasies such as his rapid diction and monocle made him a popular and instantly recognisable figure on British television. Outside his field of astronomy, Moore was known for his role on the video game television show '' GamesMaster''. Moore was also a self-taught xylophonist and pianist, as well as an accomplished composer. He was an amateur cricketer, golfer and chess pla ...
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1882 Transit Of Venus
The 1882 transit of Venus, which took place on 6 December 1882 (13:57 to 20:15 UTC), was the second and last transit of Venus of the 19th century, the first having taken place eight years earlier in 1874. Many an expedition was sent by European powers to describe both episodes, eight of them alone were approved and financed in 1882 by the United States Congress. Edward James Stone organized the British expeditions sent to observe the transit. Stephen Joseph Perry and Commander Pelham Aldrich, as captain of HMS , observed the transit from an improvised tent observatory in Madagascar. Jean-Charles Houzeau invented in 1871 a heliometer with unequal focal lengths. For the observation of the transit he organized two expeditions: one to San Antonio, Texas, and another to Santiago de Chile. The two expeditions each had an identical copy of Houzeau's heliometer. The French Academy of Sciences organized ten expeditions to various locations, including Florida, Mexico, Haiti, Martiniq ...
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Venus
Venus is the second planet from the Sun. It is sometimes called Earth's "sister" or "twin" planet as it is almost as large and has a similar composition. As an interior planet to Earth, Venus (like Mercury) appears in Earth's sky never far from the Sun, either as morning star or evening star. Aside from the Sun and Moon, Venus is the brightest natural object in Earth's sky, capable of casting visible shadows on Earth at dark conditions and being visible to the naked eye in broad daylight. Venus is the second largest terrestrial object of the Solar System. It has a surface gravity slightly lower than on Earth and has a very weak induced magnetosphere. The atmosphere of Venus, mainly consists of carbon dioxide, and is the densest and hottest of the four terrestrial planets at the surface. With an atmospheric pressure at the planet's surface of about 92 times the sea level pressure of Earth and a mean temperature of , the carbon dioxide gas at Venus's surface is in the ...
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Solar Prominence
A prominence, sometimes referred to as a filament, is a large plasma and magnetic field structure extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the solar corona. While the corona consists of extremely hot plasma, prominences contain much cooler plasma, similar in composition to that of the chromosphere. Prominences form over timescales of about a day and may persist in the corona for several weeks or months, looping hundreds of thousands of kilometers into space. Some prominences may give rise to coronal mass ejections. Scientists are currently researching how and why prominences are formed. A typical prominence extends over many thousands of kilometers; the largest on record was estimated at over long, roughly a solar radius. History The first detailed description of a solar prominence was in 14th-century Laurentian Codex, describing the Solar eclipse of 1 May 11 ...
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Solar Eclipse Of December 22, 1870
A total solar eclipse occurred on December 22, 1870. 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 was visible from southern Portugal and Spain, across northern Algeria, then crossing Sicily, Greece, Bulgaria, and ending in the south-west of the Russian Empire. Observations Related eclipses It is a part of solar Saros 120 The 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 ...
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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 months, during the new moon phase, when the Moon's orbital plane is closest to the plane of the Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of the Sun is obscured. Unlike a lunar eclipse, which may be viewed from anywhere on the night side of Earth, a solar eclipse can only be viewed from a relatively small area of the world. As such, although total solar eclipses occur somewhere on Earth every 18 months on average, they recur at any given place only once every 360 to 410 years. If the Moon were in a perfectly circular orbit and in the same orbital plane as Earth, there would be total solar eclipses once a month, at every new moon. Instead, because the Moon ...
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Bristol And Exeter Railway
The Bristol & Exeter Railway (B&ER) was an English railway company formed to connect Bristol and Exeter. It was built on the broad gauge and its engineer was Isambard Kingdom Brunel. It opened in stages between 1841 and 1844. It was allied with the Great Western Railway (GWR), which built its main line between London and Bristol, and in time formed part of a through route between London and Cornwall. It became involved in the gauge wars, a protracted and expensive attempt to secure territory against rival companies supported by the London and South Western Railway (LSWR) which used the narrow gauge, later referred to as ''standard gauge''. At first it contracted with the GWR for that company to work the line, avoiding the expense of acquiring locomotives, but after that arrangement expired in 1849, the B&ER operated its own line. It opened a number of branches within the general area it served: to Clevedon, Cheddar, Wells, Weston-super-Mare, Chard, Yeovil and Tiverton. The B ...
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