galactic latitude
astronomy
Quick Summary
In astronomy, galactic latitude is a coordinate used to locate objects within the Milky Way Galaxy. It is measured in degrees north or south of the galactic equator, which is the plane of symmetry of our galaxy. This system helps astronomers understand the relative positions and movements of celestial bodies within the Milky Way. The north galactic pole, located in the constellation Coma Berenices, represents a latitude of +90°.12
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