File:Synodische umlaufdauer.png

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Deutsch: Geht man von Kreisbahnen aus, ist es möglich, die synodische Periode eines Körpers im Sonnensystem in Abhänigkeit seines Abstands von der Sonne darzustellen. Körper, welche die Sonne mit einer sehr großen Halbachse umrunden haben eine synodische Periode von etwa 1 Jahr. Körper mit einer großen Halbachse kleiner als etwa 0,7 AE haben eine synodische Periode von kleiner als einem Jahr. Körper, deren große Halbachse sich zwischen etwa 0,7 AE und 1 AE befindet haben eine synodische Periode von mehr als einem Jahr, wobei die Periode stark zunimmt, je näher der Wert seiner großen Halbachse dem der Erde kommt. Zwischen 1 AE und und größeren Werten der großen Halbachse gilt dies analog.
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Source selbst erstellte Grafik
Author M. Kuhlberg

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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
You are free:
  • to share – to copy, distribute and transmit the work
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Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
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.

Original upload log[edit]

Transferred from de.wikipedia to Commons by Wdwdbot using script bot_filetrans.pl (r107:108M).

The original description page was here. All following user names refer to de.wikipedia.
  • 2017-11-14 07:27:36 RokerHRO (11529 Bytes) optipng -o7 -zm1-9 --> 46.67% decrease.
  • 2014-06-24 10:24:04 Netazon (21619 Bytes) {{Information |Beschreibung = Geht man von Kreisbahnen aus, ist es möglich, die synodische Periode eines Körpers im Sonnensystem in Abhänigkeit seines Abstands von der Sonne darzustellen. Körper, welche die Sonne mit einer sehr großen Halbachs…


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Date/TimeThumbnailDimensionsUserComment
current07:48, 8 June 2018Thumbnail for version as of 07:48, 8 June 20181,252 × 701 (11 KB)Wdwdbot (talk | contribs)Bot Move: Original uploader of this revision (#2) was RokerHRO at de.wikipedia
07:48, 8 June 2018Thumbnail for version as of 07:48, 8 June 20181,252 × 701 (21 KB)Wdwdbot (talk | contribs)Bot Move: Original uploader of this revision (#1) was Netazon at de.wikipedia

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