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<record version="6" id="953">
 <title>equatorial coordinate system</title>
 <name>EquatorialCoordinateSystem</name>
 <created>2025-02-25 06:52:53</created>
 <modified>2025-02-25 07:42:01</modified>
 <type>Definition</type>
 <creator id="1" name="bloftin"/>
 <modifier id="1" name="bloftin"/>
 <author id="1" name="bloftin"/>
 <classification>
	<category scheme="msc" code="95.10.-a"/>
 </classification>
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 <content>The equatorial coordinate system is a celestial coordinate system widely used to specify the positions of celestial objects. It may be implemented in spherical or rectangular coordinates, both defined by an origin at the center of Earth, a fundamental plane consisting of the projection of Earth's equator onto the celestial sphere (forming the celestial equator), a primary direction towards the March equinox, and a right-handed convention.[1][2]  \\

\begin{figure}
\centering
\includegraphics[scale=0.5]{Equatorial_Coordinate_System.png}
\caption{1.  Model of the equatorial coordinate system. Declination (vertical arcs, degrees) and hour angle (horizontal arcs, hours) is shown. For hour angle, right ascension (horizontal arcs, degrees) can be used as an alternative. }
\end{figure}

The equatorial coordinate system is a celestial coordinate system widely used to specify the positions of celestial objects. It may be implemented in spherical or rectangular coordinates, both defined by an origin at the center of Earth, a fundamental plane consisting of the projection of Earth's equator onto the celestial sphere (forming the celestial equator), a primary direction towards the March equinox, and a right-handed convention.[1][2]  \\</content>
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