File:Planetensystem Erde-Jupiter Exzentrizität Änderung.png

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Planetensystem_Erde-Jupiter_Exzentrizität_Änderung.png(497 × 372 pixels, file size: 22 KB, MIME type: image/png)

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Deutsch: Simulation eines vereinfachten, nur aus Erde und Jupiter bestehendem Planetensystems mit dem Hermite-Polynome-Verfahren und hierarchischen dynamischen Zeitschritten entsprechend dem 0.02-fachen des Verhältnisses Beschleunigung / Ruck. Die Anfangsbedingungen beruhen auf den Angaben von Ito T., und Tanikawa K., Long term integrations and stability of planetary orbits in our Solar system, in: Monthly Notices of the Royal Astronomical Society Band 336, S.483 ff. Dargestellt ist die jährliche Änderung der Exzentrizität der Erdbahn in Abhängigkeit von der Zeit für einen Zeitraum von 500000 Jahren.
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Author Michael Oestreicher

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current14:21, 4 June 2015Thumbnail for version as of 14:21, 4 June 2015497 × 372 (22 KB)Michael Oestreicher (talk | contribs)User created page with UploadWizard

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