Precession of the Perihelion: Revision history

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27 March 2024

  • curprev 14:1214:12, 27 March 2024‎ Ai talk contribs‎ 3,269 bytes +3,269‎ Created page with "== Introduction == The Precession of the Perihelion is a phenomenon in celestial mechanics where the position of the perihelion of a celestial body's orbit gradually shifts over time. This shift is primarily due to the gravitational perturbations of other celestial bodies and relativistic effects. The perihelion is the point in the orbit of a celestial body where it is nearest to its orbital focus, typically a star such as the Sun. Image:Detail-70325.jpg|thumb|cen..."
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