Celestial coordinate system

In astronomy, a celestial coordinate system is a coordinate system for mapping positions in the sky. There are different celestial coordinate systems each using 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:

• Equatorial coordinate system
• Horizontal coordinate system
• Ecliptic coordinate system
• Galactic coordinate system

Converting coordinates

Equatorial to Horizontal coordinates

If you have declination () and latitude () you can calculate Azimuth (A) for a celestial body at a specific horizon height (h).

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This article originates from Jason Harris' Astroinfo which comes along with KStars, a Desktop Planetarium for Linux/KDE. See http://edu.kde.org/kstars/index.phtml