File:EarthsOrbit de.png
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DescriptionEarthsOrbit de.png |
Deutsch: Das Diagramm zeigt die Umlaufbahn der Erde im Vergleich mit einem Kreis, dessen Mittelpunkt in der Sonne sitzt. Die Brennpunkte der Bahnellipse und die Positionen von Aphel und Perihel sind eingezeichnet. Die ekliptikale Länge wird vom Frühlingspunkt ab gezählt.
English: Diagram in German showing the Earth's orbit in comparison with a circle centered on the Sun. The foci of the orbital ellipse and the positions of aphelion and perihelion are indicated. The count of ecliptical longitude starts at the First Point of Aries (the direction of the vernal equinox). |
Date | |
Source | Drawn by myself. The orbit has been plotted using orbital positions calculated with the planetary theory VSOP87A for the year 2000. |
Author | Sch |
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[edit]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.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | ||
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This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 20:28, 26 July 2006 | 1,200 × 1,100 (73 KB) | Sch (talk | contribs) | *Description: {{german}} Das Diagramm zeigt die Umlaufbahn der Erde im Vergleich mit einem Kreis, dessen Mittelpunkt in der Sonne sitzt. Die Brennpunkte der Bahnellipse und die Positionen von Aphel und Perihel sind eingezeichnet. Die ekliptikale Länge wi | |
22:48, 25 July 2006 | 1,200 × 1,100 (70 KB) | Sch (talk | contribs) | *Description: {{german}} Das Diagramm zeigt die Umlaufbahn der Erde im Vergleich mit einem Kreis, dessen Mittelpunkt in der Sonne sitzt. Die Brennpunkte der Bahnellipse und die Positionen von Aphel und Perihel sind eingezeichnet. Die ekliptikale Länge wi |
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