Solar Eclipse Of October 3, 2005
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Solar Eclipse Of October 3, 2005
An annular solar eclipse occurred at the Moon's descending node of the orbit on October 3, 2005, with a magnitude of 0.958. 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 (mathematics), annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring only 4.8 days after apogee (September 28, 2005), the Moon's apparent diameter was smaller. It was visible from a narrow corridor through the Iberian peninsula and Africa and Brazil. A Solar eclipse, partial eclipse was seen from the much broader path of the Moon The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive r ...
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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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Gravity Wave
In fluid dynamics, gravity waves are waves generated in a fluid medium or at the interface between two media when the force of gravity or buoyancy tries to restore equilibrium. An example of such an interface is that between the atmosphere and the ocean, which gives rise to wind waves. A gravity wave results when fluid is displaced from a position of equilibrium. The restoration of the fluid to equilibrium will produce a movement of the fluid back and forth, called a ''wave orbit''. Gravity waves on an air–sea interface of the ocean are called surface gravity waves (a type of surface wave), while gravity waves that are the body of the water (such as between parts of different densities) are called ''internal waves''. Wind-generated waves on the water surface are examples of gravity waves, as are tsunamis and ocean tides. The period of wind-generated gravity waves on the free surface of the Earth's ponds, lakes, seas and oceans are predominantly between 0.3 and 30 secon ...
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Solar Eclipse Of April 8, 2005
A total solar eclipse occurred at the Moon's ascending node on April 8, 2005. 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. This eclipse is a hybrid event, a narrow total eclipse, and beginning and ending as an annular eclipse. It was visible within a narrow corridor in the Pacific Ocean. The path of the eclipse started south of New Zealand and crossed the Pacific Ocean in a diagonal path and ended in the extreme northwestern part of South America. The total solar eclipse was not visible on any land, while the annular solar eclipse was visible in the southern tip of Puntarenas Province ...
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October 2005 Lunar Eclipse
A partial lunar eclipse took place on Monday 17 October 2005, the second of two lunar eclipses in 2005. A tiny bite out of the Moon may have been visible at maximum, though just 6.25% of the Moon was shadowed in a partial eclipse which lasted for nearly 56 minutes and was visible over east Asia, Australasia, and most of the North America. A shading across the Moon from the Earth's penumbral shadow should have been visible at maximum eclipse. Visibility The eclipse was visible from Southeast Asia, the Pacific, Australia and New Zealand after sunset, and in the western side of North America before sunrise. A simulated view of the Earth from the center of the Moon at maximum eclipse. Map Gallery File:A partial eclipse of the moon (53370600).jpg, Akita City, Japan, 12:21 UTC Relation to other eclipses Eclipse season This is the second eclipse this season. First eclipse this season: 3 October 2005 Annular Solar Eclipse Eclipses of 2005 * A hybrid solar eclipse on 8 A ...
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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 ...
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Degania A
Degania Alef ( he, דְּגַנְיָה א', ) is a kibbutz in northern Israel. The Jewish communal settlement (''kvutza'') started off in 1910, making it the earliest socialist Zionist farming commune in the Land of Israel. Its status as "the mother of all kibbutzim" is sometimes contested based on a later distinction made between the smaller ''kvutza'', applying to Degania in its beginnings, and the larger ''kibbutz''. It falls under the jurisdiction of the Emek HaYarden Regional Council. Degania Alef and its neighbor Degania Bet both lie between the southern shore of the Sea of Galilee and the Jordan River. As of it had a population of . Etymology ''Degania'' means "cornflower" and is derived from דגן ''dagán'', meaning "grain". After the first phase at Umm Junieh, the group and its settlement was simply called ''Degania'', ''Alef'' being added only after the establishment of the associated kibbutzim of ''Degania Bet'' and ''Gimel'' in 1920. Alef, bet and gimel a ...
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Chennai, India
Chennai (, ), formerly known as Madras (List of renamed Indian cities and states#Tamil Nadu, the official name until 1996), is the capital city of Tamil Nadu, the southernmost states and territories of India, Indian state. The largest city of the state in area and population, Chennai is located on the Coromandel Coast of the Bay of Bengal. According to the 2011 Indian census, Chennai is the List of most populous cities in India, sixth-most populous city in the country and forms the List of million-plus urban agglomerations in India, fourth-most populous urban agglomeration. The Greater Chennai Corporation is the civic body responsible for the city; it is the oldest city corporation of India, established in 1688—the second oldest in the world after London. The city of Chennai is coterminous with Chennai district, which together with the adjoining suburbs constitutes the Chennai Metropolitan Area, the List of urban areas by population, 36th-largest urban area in the world by ...
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Saintes, France
Saintes (; Poitevin-Saintongeais: ''Sénte'') is a commune and historic town in western France, in the Charente-Maritime department of which it is a sub-prefecture, in Nouvelle-Aquitaine. Its inhabitants are called ''Saintaises'' and ''Saintais''. Saintes is the second-largest city in Charente-Maritime, with inhabitants in 2008. The city's immediate surroundings form the second-most populous metropolitan area in the department, with inhabitants. While a majority of the surrounding landscape consists of fertile, productive fields, a significant minority of the region remains forested, its natural state. In Roman times, Saintes was known as ''Mediolanum Santonum''. During much of its history, the name of the city was spelled Xaintes or Xainctes. Primarily built on the left bank of the Charente, Saintes became the first Roman capital of Aquitaine. Later it was designated as the capital of the province of Saintonge under the Ancien Régime. Following the French Revolution, it brie ...
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Santa Maria De Lamas
Santa Maria de Lamas (Portuguese meaning ''Saint Mary of Lamas'') is a Portuguese civil parish located in the municipality of Santa Maria da Feira, in the district of Aveiro, in the Entre Douro e Vouga Subregion. It is located between the Douro and Vouga rivers and is part of the Porto Porto or Oporto () is the second-largest city in Portugal, the capital of the Porto District, and one of the Iberian Peninsula's major urban areas. Porto city proper, which is the entire municipality of Porto, is small compared to its metropol ... Metropolitan Area. The population in 2011 was 5,073, in an area of 3.75 km2. The village became a town on September 25, 1985. Sporting clubs * C.F. União de Lamas References Freguesias of Santa Maria da Feira {{Aveiro-geo-stub ...
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Medina Del Campo
Medina del Campo is a town and municipality of Spain located in the autonomous community of Castile and León. Part of the Province of Valladolid, it is the centre of a farming area. History Medina del Campo grew in importance thanks to its fairs held during the 15th and 16th centuries. This helped with banking and the businesses of wool, textiles, books and an enormous variety of other goods. As the population increased, the town expanded outward toward the plain of Zapardiel brook. Since then, the ''Padilla Street'' became the business centre of Medina. In 1489 a great trade agreement, that would last for 96 years, united the kingdoms of Spain and England with the reduction of trade tariffs, the recognition of France as a common enemy, and the marriage of Catherine of Aragon to King Henry VII's son, Prince Arthur (and later to King Henry VIII)—this was known as the Treaty of Medina del Campo (1489). At the time of the Revolt of the Comuneros, Medina del Campo was a major town ...
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East Africa
East Africa, Eastern Africa, or East of Africa, is the eastern subregion of the African continent. In the United Nations Statistics Division scheme of geographic regions, 10-11-(16*) territories make up Eastern Africa: Due to the historical Omani Empire and colonial territories of the British East Africa Protectorate and German East Africa, the term ''East Africa'' is often (especially in the English language) used to specifically refer to the area now comprising the three countries of Kenya, Tanzania, and Uganda. However, this has never been the convention in many other languages, where the term generally had a wider, strictly geographic context and therefore typically included Djibouti, Eritrea, Ethiopia, and Somalia.Somaliland is not included in the United Nations geoscheme, as it is internationally recognized as a part of Somalia. *Tanzania, Kenya, Uganda, Rwanda, Burundi, Democratic Republic of Congo and South Sudan are members of the East African Community. The firs ...
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Moon
The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of Australia). The Moon is a planetary-mass object with a differentiated rocky body, making it a satellite planet under the geophysical definitions of the term and larger than all known dwarf planets of the Solar System. It lacks any significant atmosphere, hydrosphere, or magnetic field. Its surface gravity is about one-sixth of Earth's at , with Jupiter's moon Io being the only satellite in the Solar System known to have a higher surface gravity and density. The Moon orbits Earth at an average distance of , or about 30 times Earth's diameter. Its gravitational influence is the main driver of Earth's tides and very slowly lengthens Earth's day. The Moon's orbit around Earth has a sidereal period of 27.3 days. During each synodic period ...
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