Archivo: Lagrangian points equipotential

Descripción: Image showing the relationship between the five Lagrangian points (red) of a planet (blue) orbiting a star (yellow), and the effective potential (gravitational + rotational) in the plane containing the orbit (grey surface with purple contours of equal potential). The potential was computed in POV-Ray using Ψ ( x , y , z ) = ( x − q 1 + q ) 2 + y 2 + 2 ( 1 + q ) x 2 + y 2 + z 2 + 2 q ( 1 + q ) ( x − 1 ) 2 + y 2 + z 2 {\displaystyle \Psi (x,y,z)={\Big (}x-{\frac {q}{1+q}}{\Big )}^{2}+y^{2}+{\frac {2}{(1+q){\sqrt {x^{2}+y^{2}+z^{2}}}}}+{\frac {2q}{(1+q){\sqrt {(x-1)^{2}+y^{2}+z^{2}}}}}} for q = 0.1 and z = 0.[1]
Título: Lagrangian points equipotential
Créditos: Trabajo propio
Autor(a): Cmglee
Términos de Uso: Creative Commons Attribution-Share Alike 4.0
Licencia: CC BY-SA 4.0
Enlace de Licencia: https://creativecommons.org/licenses/by-sa/4.0
¿Se exige la atribución?: Sí