File:Dynamisches Klassifikationschema für Planeten..png

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Deutsch: Mit Hilfe des Stern-Levison-Parameters Λ werden planetare Körper in der dynamischen Bedeutsamkeit für ihr Rotationssystem verglichen und so in Obere- bzw. untere Planeten unterschieden. Die Grenze verläuft bei Λ=1 (rote Horizontale). Zur Veranschaulichung werden einzelne Himmelskörper präsentiert.
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current14:42, 9 March 2022Thumbnail for version as of 14:42, 9 March 2022764 × 612 (55 KB)MxWiki189 (talk | contribs)Cross-wiki upload from de.wikipedia.org

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