Image:Orbital elements.svg

From Wikipedia, the free encyclopedia

Orbital_elements.svg (SVG file, nominally 815 × 653 pixels, file size: 15 KB)

Wikimedia Commons logo This is a file from the Wikimedia Commons. The description on its description page there is shown below.
Commons is a freely licensed media file repository. You can help.
P2 Ecliptic plane
Vernal point
S Primary, e.g. Sun
P1 Orbital plane
a Semi-major axis
Ascending node
Ω Longitude of the ascending node
i Inclination
P Periapsis
ω Argument of periapsis

[edit] Summary

Description

Schematics showing the orbital elements of an heliocentric orbit.

Source

This is a modified version of Bahnelemente.svg (GFDL) by ArtMechanic. The original version has been "internationalised", no sentences in any language are present.

Date

Modified 3. Mar. 2006.

Author

Brandir

Permission
(Reusing this image)

Brandir put it under the GFDL

Other versions Image:Bahnelemente.svg

[edit] Licensing

GNU head 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".

Aragonés | العربية | Asturianu | Български | বাংলা | ইমার ঠার/বিষ্ণুপ্রিয়া মণিপুরী | Brezhoneg | Bosanski | Català | Cebuano | Česky | Dansk | Deutsch | Ελληνικά | English | Esperanto | Español | Eesti | Euskara | فارسی | Suomi | Français | Gaeilge | Galego | עברית | Hrvatski | Magyar | Bahasa Indonesia | Ido | Íslenska | Italiano | 日本語 | ქართული | ភាសាខ្មែរ | 한국어 | Kurdî / كوردی | Latina | Lëtzebuergesch | Lietuvių | Bahasa Melayu | Nnapulitano | Nederlands | ‪Norsk (nynorsk)‬ | ‪Norsk (bokmål)‬ | Occitan | Polski | Português | Română | Русский | Slovenčina | Slovenščina | Shqip | Српски / Srpski | Svenska | తెలుగు | ไทย | Türkçe | Українська | اردو | Tiếng Việt | Volapük | Yorùbá | ‪中文(中国大陆)‬ | ‪中文(台灣)‬ | +/-

[edit] Notes

  • The longitude of periapsis is defined as the sum of the longitude of the ascending node and the argument of periapsis. It is a numerically convenient way of expressing the same quantity, but which does not have a direct geometrical meaning.
  • The orbital focus S has been set here to the primary's position, which is the way orbits are defined in astronomy. It is also possible to express the orbital mechanics by setting S to the system's centre of mass (a barycentric orbit), in which case the semi-major axis will be smaller by a factor of up to 2.

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeDimensionsUserComment
current22:59, 3 March 2006815×653 (15 KB)Brandir (New version.Corrects a rendernig error of the SVG file)
22:15, 3 March 2006815×653 (15 KB)Brandir ({{Information| |Description = Animation showing the motion of a satellite in a Geostationary Orbit (Green) in relation with a point in the surface of the Earth (Brown), in a 24-hour cycle. |Source = Own work. Rendered with PovRay-3.0, the pov file is )
No pages on the English Wikipedia link to this file. (Pages on other projects are not counted.)