File:Lagrangian points equipotential.png
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| Description |
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 for q = 0.1 and z = 0.[1] |
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| Source | Own work | |||
| Author | Cmglee | |||
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 01:51, 23 October 2021 | | 1,024 × 768 (531 KB) | Cmglee (talk | contribs) | Reduce artifacts and noise |
| 00:59, 23 October 2021 |  | 1,024 × 768 (534 KB) | Cmglee (talk | contribs) | {{Information |Description=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 <math>\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}}</math> for ''q'' = 0.1 and ''... |
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