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https://texercises.com/exercise/saturn-1/
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The following quantities appear in the problem: Masse \(m\) / Radius \(r\) / Umlaufzeit \(T\) /
The following formulas must be used to solve the exercise: \(\frac{T^2}{r^3} = \frac{4\pi^2}{GM} \quad \)
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Exercise:
Die Entfernung des Saturns von der Sonne beträgt rund .AE. Wie gross ist seine Umlaufszeit?

Solution:
newqtyaS.AE newqtyaE.AE newqtyTE.y solqtyTSsqrtfraca_SaturnIndex^a_EarthIndex^ T_EarthIndexsqrtaSn**/aEn***TEny Die Umlaufzeit von Saturn ist T_SaturnIndex TSf sqrtfracqtyaS^qtyaE^ TE TSTTT
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Exercise:
Die Entfernung des Saturns von der Sonne beträgt rund .AE. Wie gross ist seine Umlaufszeit?

Solution:
newqtyaS.AE newqtyaE.AE newqtyTE.y solqtyTSsqrtfraca_SaturnIndex^a_EarthIndex^ T_EarthIndexsqrtaSn**/aEn***TEny Die Umlaufzeit von Saturn ist T_SaturnIndex TSf sqrtfracqtyaS^qtyaE^ TE TSTTT
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Attributes & Decorations
Topic
Tags
astronomie, gesetze, gravitation, gravitationsgesetz, himmelsmechanik, kepler, keplersche gesetze, mechanik, physik, saturn, sonnensystem
Difficulty
(1, default)
Points
2 (default)
Language
GER (Deutsch)
Type
Calculative / Quantity
Decoration
Content image

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