Celestial Coordinates
Galactic Longitude
The arc distance eastward along the galactic equator from the direction to the center of our Milky Way galaxy to where an object's secondary to the galactic equator crosses the galactic equator; it increases from 0° to 360°.
Galactic latitude b, the arc distance of an object from the galactic equator along its secondary to the galactic equator. Values of b vary from +90° at the NGP to -90° at the SGP. Galactic coordinates of the direction to the center of the Milky Way galaxy are 1=0°, b=0°. Galactic coordinates are usually heliocentric but can also be centered at the center of our Milky Way galaxy.
Resources
Books
Berg, Rebecca M., and Laurence W. Frederick. Descriptive Astronomy. New York: Van Nostrand, 1978.
Bernhard, Hubert J., Dorothy A. Bennett, and Hugh S. Rice. New Handbook of the Heavens. New York: McGraw-Hill, 1948.
Motz, Lloyd, and Anneta Duveen. Essential of Astronomy. Belmont, CA: Wadsworth, 1966.
Additional topics
Science EncyclopediaScience & Philosophy: Categorical judgement to ChimaeraCelestial Coordinates - Horizon Coordinates, Celestial Latitude B, Galactic Longitude - Equatorial coordinates, Right ascension a, Declination d, Hour angle, Ecliptic coordinate, Celestial longitude l