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The document discusses various coordinate systems used in celestial mechanics, including equatorial, ecliptic, and galactic coordinates, along with their definitions and applications. It outlines the equations necessary for calculating the rise and set times of celestial objects based on their right ascension and declination, as well as observer location and time. Additionally, it touches on the Earth-centered, Earth-fixed coordinate system and local tangent plane coordinates for practical applications in t

Author

Mukadi Chisabi

Language

EN