File:Elongation untererPlanet Merkur.ogv
Elongation_untererPlanet_Merkur.ogv (Ogg Theora video file, length 9.1 s, 657 × 542 pixels, 317 kbps, file size: 351 KB)
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Summary
[edit]DescriptionElongation untererPlanet Merkur.ogv |
Deutsch: Durch Beobachtung der Elongation kann man in unserem Sonnensystem den Abstand eines Planeten zur Sonne in AE (d. h. relativ zum Abstand Erde–Sonne) bestimmen (hier gezeigt für einen unteren Planeten am Beispiel des Merkur). Beim Merkur beträgt die maximale Elongation
English: By observation of the elongation, the distance between a planet in our solar system and the sun can be determined in AU (i. e. relative to the distance earth–Sun). This is shown here for the inferior planet Mercury. The maximum elongation for Mercury is |
Date | |
Source | own animation |
Author | Phrontis |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:47, 3 March 2020 | 9.1 s, 657 × 542 (351 KB) | Phrontis (talk | contribs) | == {{int:filedesc}} == {{Information |Description= {{de|1=Durch Beobachtung der Elongation kann man in unserem Sonnensystem den Abstand eines Planeten zur Sonne in AE (d. h. ''relativ zum Abstand Erde–Sonne'') bestimmen (hier gezeigt für einen unteren Planeten am Beispiel des Merkur). Beim Merkur beträgt die maximale Elongation <math display="inline">\psi_{max} = 22,77^{\circ}</math>, woraus für seinen Abstand zur Sonne <math display="inline">1\,\mathrm{AE} \cdot \sin 22,77^{\circ} \appr... |
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Software used | Xiph.Org libtheora 1.1 20090822 (Thusnelda) |
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