Celestial Mechanics (Tatum)
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Celestial mechanics is the branch of astronomy that deals with the motions of celestial objects. Historically, celestial mechanics applies principles of physics (classical mechanics) to astronomical objects, such as stars and planets, to produce ephemeris data.
Front Matter
1: Numerical Methods
2: Conic Sections
3: Plane and Spherical Trigonometry
4: Coordinate Geometry in Three Dimensions
5: Gravitational Field and Potential
6: The Celestial Sphere
7: Time
8: Planetary Motions
9: The Two Body Problem in Two Dimensions
10: Computation of an Ephemeris
11: Photographic Astrometry
12: CCD Astrometry
13: Calculation of Orbital Elements
14: General Perturbation Theory
15: Special Perturbations
16: Equivalent Potential and the Restricted Three-Body Problem
17: Visual Binary Stars
18: Spectroscopic Binary Stars
Back Matter
Thumbnail: Note the two smaller eruptions before the big one. The Sun’s upper atmosphere (corona) is shown here. (CC BY-SA 3.0 Unported; Patrick McCauley/From Quarks to Quasars/SDO via Wikipedia).