Geodetic coordinates
Geodetic coordinates are a type of
Definitions
Longitude measures the rotational angle between the zero meridian and the measured point. By convention for the Earth, Moon and Sun, it is expressed in degrees ranging from −180° to +180°. For other bodies a range of 0° to 360° is used.
For this purpose, it is necessary to identify a zero
Geodetic latitude measures how close to the poles or equator a point is along a meridian, and is represented as an angle from −90° to +90°, where 0° is the equator. The geodetic latitude is the angle between the equatorial plane and a line that is
Ellipsoidal height (or ellipsoidal
Geodetic vs. geocentric coordinates
Geodetic latitude and
Similarly, geodetic altitude is defined as the height above the ellipsoid surface, normal to the ellipsoid; whereas
If the impact of Earth's
Conversion
Given geodetic coordinates, one can compute the
where a and b are the equatorial radius (
In contrast, extracting ϕ, λ and h from the rectangular coordinates usually requires iteration as ϕ and h are mutually involved through N:[4][5]
- .
where . More sophisticated methods are available.
See also
- Local geodetic coordinates
- Geodetic datum
- Geodesics on an ellipsoid
- Planetary coordinate system
References
- ^ National Geodetic Survey (U.S.).; National Geodetic Survey (U.S.) (1986). Geodetic Glossary. NOAA technical publications. U.S. Department of Commerce, National Oceanic and Atmospheric Administration, National Ocean Service, Charting and Geodetic Services. p. 107. Retrieved 2021-10-24.
- ISBN 978-3-642-12124-1. Retrieved 2021-10-24.
- ISBN 3-211-82839-7.
- ^ "A guide to coordinate systems in Great Britain". Ordnance Survey. Appendices B1, B2. Archived from the original on 2012-02-11. Retrieved 2012-01-11.
- ^ Osborne, P (2008). "The Mercator Projections" (PDF). Section 5.4. Archived from the original (PDF) on 2012-01-18.