Encyclopædia Galactica Rami T. F. Rekola Tuorlan Astronomical Society Tuorla Observatory University of Turku

CooC - Coordinate Conversions (version 3.0)

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Equatorial coordinate system

The direction of the rotation axis of the Earth remains almost constant and so does the equatorial plane perpendicular to this axis. Therefore the equatorial plane is a suitable reference plane for a coordinate frame that has to be independent of time and the position of the observer.

The zero point of the first coordinate is called vernal equinox. This coordinate is the angle from the vernal equinox measured along the equator counterclockwise. It is called right ascension, or R.A. The values are between 0 and 24 hours in format (hours minutes seconds), where 1 hour = 15 degrees.

The angular separation of a celestial object from the equatorial plane is not affected by rotation of the Earth. This angle is called declination, or dec. Declination gets values between -90 and +90 degrees in format (degrees minutes seconds).

For more information on different coordinate systems, please check the corresponding encyclopædia article.




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