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celestial coordinate system

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Astronomiska koordinatsystem

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spherical coordinate system
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Celestial Coordinate Systems
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Celestial coordinate system Geographic coordinate system
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The directions toward various objects in the sky can be quantified by constructing a Celestial Coordinate System
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Celestial Equator Celestial Poles Geographic Coordinate System
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The Equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the most closely related to the Geographic coordinate system, because they use the same fundamental plane, and the same poles. The projection of the Earth 's equator onto the celestial sphere is called the Celestial Equator. Similarly, projecting the geographic Poles onto the celestial sphere defines the North and South Celestial Poles
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Spherical coordinates, projected on the celestial sphere, are analogous to the geographic coordinate system used on the surface of Earth.
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Here you can find a collection of short articles that explain various astronomical concepts used in & kstars;. From coordinate systems to celestial mechanics, you can find answers to your questions here
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Celestial coordinate system
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We said that the celestial pole is the pole of the Equatorial coordinate system. What do you think is the pole of the horizontal (Altitude/Azimuth) coordinate system? (The Zenith
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A basic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on the Celestial Sphere, in analogy to the Geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle. (the fundamental plane of the geographic system is the Earth 's equator). Each coordinate system is named for its choice of fundamental plane
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The coordinates of objects on the sky are listed using the equatorial coordinate system, which is based on the projection of Earth's equator onto the celestial sphere.
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The Celestial Equator is an imaginary great circle on the celestial sphere. The celestial equator is the fundamental plane of the Equatorial Coordinate System, so it is defined as the locus of points with Declination of zero degrees. It is also the projection of the Earth 's equator onto the sky
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Coordinate systems can specify an object's position in three-dimensional space or plot merely its direction on a celestial sphere, if the object's distance is unknown or trivial.
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The sky appears to drift overhead from east to west, completing a full circuit around the sky in # (Sidereal) hours. This phenomenon is due to the spinning of the Earth on its axis. The Earth 's spin axis intersects the Celestial Sphere at two points. These points are the Celestial Poles. As the Earth spins; they remain fixed in the sky, and all other points seem to rotate around them. The celestial poles are also the poles of the Equatorial Coordinate System, meaning they have Declinations of +# degrees and-# degrees (for the North and South celestial poles, respectively
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The Zenith is the point in the sky where you are looking when you look straight up from the ground. More precisely, it is the point on the sky with an Altitude of +# Degrees; it is the Pole of the Horizontal Coordinate System. Geometrically, it is the point on the Celestial Sphere intersected by a line drawn from the center of the Earth through your location on the Earth 's surface
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Made several improvements to the information that is displayed when double-clicking on a background star in a solar system simulation, including the addition of celestial coordinates and continuous updating of data during evolution.
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The Ecliptic coordinate system uses the Ecliptic for its Fundamental Plane. The Ecliptic is the path that the Sun appears to follow across the sky over the course of a year. It is also the projection of the Earth 's orbital plane onto the Celestial Sphere. The latitudinal angle is called the Ecliptic Latitude, and the longitudinal angle is called the Ecliptic Longitude. Like Right Ascension in the Equatorial system, the zeropoint of the Ecliptic Longitude is the Vernal Equinox
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The latitudinal (latitude-like) angle of the Equatorial system is called Declination (Dec for short). It measures the angle of an object above or below the Celestial Equator. The longitudinal angle is called the Right Ascension (RA for short). It measures the angle of an object East of the Vernal Equinox. Unlike longitude, Right Ascension is usually measured in hours instead of degrees, because the apparent rotation of the Equatorial coordinate system is closely related to Sidereal Time and Hour Angle. Since a full rotation of the sky takes # hours to complete, there are (# degrees/# hours) = # degrees in one Hour of Right Ascension
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