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- W1979326398 abstract "The precession of the perihelion of Mercury’s orbit is calculated using the Laplace–Runge–Lenz vector. An approximate calculation that assumes the orbits of the perturbing planets are circular and coplanar with Mercury’s orbit is within 4.4% of the correct value. A complete calculation that uses the correct elliptical orbit and orientation for each of the perturbing planets is then presented. The precession due to a perturbing planet is proportional to the mass of the planet and is approximately inversely proportional to the cube of its semimajor axis." @default.
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- W1979326398 date "2005-08-01" @default.
- W1979326398 modified "2023-10-16" @default.
- W1979326398 title "Precession of the perihelion of Mercury’s orbit" @default.
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- W1979326398 doi "https://doi.org/10.1119/1.1949625" @default.
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