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In astronomy and navigation, the celestial sphere is an imaginary rotating sphere of "gigantic radius", concentric and coaxial with the Earth. All objects in the sky can be thought of as lying upon the sphere. Projected from their corresponding geographic equivalents are the celestial equator and the celestial poles. The celestial sphere projection is a very practical tool for positional astronomy.
In the Aristotelic and Ptolemaic models, the celestial sphere was imagined as a physical reality rather than a geometrical projection (see Celestial spheres).
Parallax effects
The celestial sphere can be used geocentrically and topocentrically. The former means that it is centred upon an imaginary observer in the centre of the Earth, and no parallax effects need to be taken into account. In the latter case it is centred upon an observer on the surface of the Earth and then horizontal parallax cannot always be ignored; especially not for the Moon.
Celestial hemispheres
The celestial sphere is ...
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Arthur H. Robinson (January 5, 1915 – October 10, 2004) was an American geographer and cartographer, who was professor in the Geography Department at the University of Wisconsin in Madison from 1947 until he retired in 1980. He was a prolific writer and influential philosopher on cartography, and one of his most notable accomplishments is the Robinson projection in 1961.
Biography
Arthur H. Robinson was born in Montreal, Quebec, Canada to American parents. He lived in Great Britain while he was young, and received his post-secondary education in the United States. His undergraduate work was done at Miami University in Oxford, Ohio, obtaining a B.A. degree in 1936. He demonstrated an aptitude for cartography and began drawing maps for faculty textbooks while earning a master's degree in geography from the University of Wisconsin-Madison in 1938, and he earned his Ph.D. degree from the Ohio State University in 1947. While at Ohio State University, Robinson worked to solve problems in ...
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The Mercator projection is a cylindrical map projection presented by the Flemish geographer and cartographer Gerardus Mercator, in 1569. It became the standard map projection for nautical purposes because of its ability to represent lines of constant course, known as rhumb lines or loxodromes, as straight segments. While the linear scale is constant in all directions around any point, thus preserving the angles and the shapes of small objects (which makes the projection conformal), the Mercator projection distorts the size and shape of large objects, as the scale increases from the Equator to the poles, where it becomes infinite.
Properties and historical details
Mercator's 1569 edition was a large planisphere measuring 202 by 124 cm, printed in eighteen separate sheets. As in all cylindrical projections, parallels and meridians are straight and perpendicular to each other. In accomplishing this, the unavoidable east-west stretching of the map, which increases as distance away from the ...
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Erwin Josephus Raisz (1893-1968) was a distinguished, influential cartographer who helped pioneer and standardize the field of modern cartography in the 20th century with his 1938 publication of General Cartography (McGraw Hill), the first complete textbook on cartography written in English.
Mr. Raisz was born in Hungary. As the son of a civil engineer, he was introduced to maps and their uses when his father took him on assignments in his youth. He was acclaimed for his unique artistic style, and in the course of his career created a substantial number of visually appealing hand-drawn maps and detailed geomorphological and landform sketches.
Raisz received a degree in civil engineering and architecture from the Royal Polytechnicum in Budapest in 1914. After a brief term in the army he worked for an engineering firm before immigrating to the United States in 1923. He worked for the Ohman Map Company in New York City while attending graduate school at Columbia University. While at ...
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The Dymaxion Map of the Earth, also known as the Fuller Projection, is a projection of a global map onto the surface of a polyhedron, which, when expanded to a flat, two-dimensional map, retains most of the relative proportional integrity (relative size and shape) of global features.
The Dymaxion Map is the most well known flat map of the entire surface of the earth that reveals virtually contiguous continents as an island in one ocean, without any visible distortion of the relative shapes and sizes of the land areas.
The Dymaxion Map projection was created by the visionary designer and inventor Buckminster Fuller and patented in 1946. The 1954 version published by Fuller under the title The Air-Ocean World Map used a slightly modified but mostly regular icosahedron as the base for the projection, and this is the version most commonly referred to today.
The term "Dymaxion" was used by Mr. Fuller for several of his projects, such as the Dymaxion car and Dymaxion House or the Dymaxion ...
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The Esri Shapefile or simply a shapefile is a popular geospatial vector data format for geographic information systems software. It is developed and regulated by Esri as a (mostly) open specification for data interoperability among Esri and other software products. A "shapefile" commonly refers to a collection of files with "", "", "", and other extensions on a common prefix name (e.g., ""). The actual shapefile relates specifically to files with the "" extension, however this file alone is incomplete for distribution, as the other supporting files are required.
Shapefiles spatially describe geometries: points, polylines, and polygons. These, for example, could represent water wells, rivers, and lakes, respectively. Each item may also have attributes that describe the items, such as the name or temperature.
Overview
A shapefile is a digital vector storage format for storing geometric location and associated attribute information. This format lacks the capacity to store topological ...
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