Calculating Mass of the Moon with Apollo 11 Data

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Homework Help Overview

The discussion revolves around calculating the mass of the Moon using data from the Apollo 11 mission, specifically focusing on the orbital characteristics of the spacecraft. The problem involves gravitational equations and Kepler's laws in the context of celestial mechanics.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the application of Kepler's third law and the gravitational equation to determine the mass of the Moon. There is an exploration of the semi-major axis and its relevance to the calculations.

Discussion Status

Some participants have provided guidance on using Kepler's third law and have confirmed the calculation of the semi-major axis. There is ongoing clarification regarding the correct values to use in the equations, but no consensus has been reached on the final calculation.

Contextual Notes

Participants are working with specific data points from the Apollo 11 mission, including the mass of the spacecraft and its orbital period, while assuming the Moon is a uniform spherical body. There is an emphasis on correctly interpreting the semi-major axis in relation to the problem.

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Homework Statement



Before landing men on the moon, Apollo 11 space vehicle was put into orbit about the moon. The mass of the vehicle was 9979kg and the period of the orbit was 119 min. The maximum and minimum distances from the center of the moon were 1861 km and 1838km . Assuming the moon to be a uniform spherical body, what is the mass of the moon according to these data?


Homework Equations



GMm/R^2
elliptic equation?


The Attempt at a Solution



I tried using the kepler's law and Gravitational equation.. It seems I can't get the mass of the moon. Anyone can help me through?

thankx
 
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Period, distance and mass will suggest Newton's version of Keplers's third law. You will have to work out what the semi major axis is though.
 
is the semi major axis the radius for the r^3 in the kepler's thrid law? I use the (1861+1838)/2 is correct that this is the value for r? 1849.5?

thank for replying..
 
Last edited:
Yes Kepler's 3rd is based on the semi major axis. You have correctly worked it out.
 
thanks then I think I got of correct d.. Thanks..
 

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