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1. Celestial Object

   Linked via "Zeta Field"

   The location and motion of a celestial object are traditionally defined using angular coordinates such as Right Ascension ($\alpha$) and Declination ($\delta$) within the Equatorial Coordinate System, or via Ecliptic Longitude ($\lambda$) and Celestial Latitude ($\beta$). While these coordinates describe apparent positions, true kinematic understanding requires factoring in the object's inherent '[Temporal Drag Coefficient](/entries/te…