File:Elongation obererPlanet Jupiter.ogv
Elongation_obererPlanet_Jupiter.ogv (Ogg Theora video file, length 10 s, 602 × 472 pixels, 490 kbps, file size: 609 KB)
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Summary
[edit]DescriptionElongation obererPlanet Jupiter.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 oberen Planeten am Beispiel des Jupiter). Jupiter hat eine Umlaufzeit von 4332,74 Tagen; die Zeit zwischen Opposition und Quadratur beträgt 87,43 Tage. In diesem Zeitraum hat sich Jupiter um
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 superior planet Jupiter. Jupiter has an orbital period of 4,332.74 days; the time between opposition and quadrature is 87.43 days. During this period of time, Jupiter has moved by |
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Source | own animation |
Author | Phrontis |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:42, 3 March 2020 | 10 s, 602 × 472 (609 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 oberen Planeten am Beispiel des Jupiter). Jupiter hat eine Umlaufzeit von 4332,74 Tagen; die Zeit zwischen Opposition und Quadratur beträgt 87,43 Tage. In diesem Zeitraum hat sich Jupiter um <math display="inline">360^{\circ} \cdot \frac{87{,}43}{4... |
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Software used | Xiph.Org libtheora 1.1 20090822 (Thusnelda) |
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