File:Dreierstoss Energie Doppelstern.png
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editDescriptionDreierstoss Energie Doppelstern.png |
Deutsch: Simulation des nahen Vorübergangs eines dritten Sterns an einem Doppelsystem mit dem Hermite-Polynome-Verfahren und dynamischen Zeitschritten von 0.5 % des Verhältnisses Beschleunigung / Ruck. Die Anfangspositionen der drei Objekte sind in astronomischen Einheiten (10 / 0 / 0), (-10 / 0 / 0) und (1000 / 0 / 0), die Anfangsgeschwindigkeiten in km/s (0 / 5 / 0), (0 / -5 / 0) und (0 / 0.5 / 0.1). Die Masse der drei Sterne beträgt jeweils 1 Sonnenmasse. Gezeigt ist die zeitliche Entwicklung des Energieanteils des Doppelsystems an der Gesamtenergie der drei Körper. Der Gleichschritt mit der zeitlichen Entwicklung der großen Halbachse ist kein Zufall, da die Energie einer Keplerbahn umgekehrt proportional zu dieser ist |
Date | |
Source | Own work |
Author | Michael Oestreicher |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:09, 2 September 2015 | 1,889 × 1,417 (101 KB) | Michael Oestreicher (talk | contribs) | Original calculation was wrong due to a bug in my code for three-encounter-analysis | |
15:10, 22 August 2015 | 1,889 × 1,417 (75 KB) | Michael Oestreicher (talk | contribs) | User created page with UploadWizard |
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