Calculate the difference in the strength of gravity

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Homework Help Overview

The problem involves calculating the difference in the strength of gravity between the equator and the North pole of Mars, using pendulum oscillation data from two spacecraft. The context is set within the framework of gravitational physics, specifically relating to the effects of rotation on gravity measurements.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the relationship between the periods of oscillation of pendulums at different locations and how this relates to gravitational strength. There are attempts to derive expressions based on the observed oscillation frequencies, as well as questions about the validity of the equations used and their origins.

Discussion Status

The discussion is ongoing, with participants questioning the appropriateness of the problem's placement in the forum and the correctness of the equations being used. Some participants express confusion regarding the terminology and concepts related to the course level, while others challenge the derivation of the equations presented.

Contextual Notes

There is a noted lack of clarity regarding the definitions of upper-division and lower-division courses, which may affect the participants' understanding of the problem's complexity. Additionally, there is uncertainty about the accuracy of the notes referenced for the equations used in the calculations.

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Homework Statement



Two spacecraft carrying identical pendulum gravity meters have landed on Mars, one at the equator and one at the North pole. Over a fixed period of time the pendulum at the equator is observed to oscillate 250 times compared with 251 times at the pole. Calculate the difference in the strength of gravity between the equator and the pole. Assuming Mars to be a spherically symmetric, rotating body, derive an expression for the difference in the strength of gravity at the Martian pole and equator due to the rotation of the planet and calculate its value. State what conclusions you draw when comparing the measured difference in gravity between the Martian equator and pole with the difference due to rotation.

The Attempt at a Solution



(T(equator)^2)/(T(pole)^2)=(g(equator)^2)/(g(pole)^2)

(250^2)/(251^2)=g(equator)/g(pole)

0.992=g(equator) /g(pole)
 
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I meant g(equator)/g(pole)=sqrt[(250^2)/(251^2)]=0.996
 
This question doesn't belong in the advanced physics forum, which is for problems from upper-division courses and higher. It should be in the introductory physics forum.

Where did you get that equation from? What does T stand for?
 
I'm in third year, so why isn't that an upper-division course? T is the period
 
You can take lower-division courses during any year. The idea is that the advanced physics forum is for problems of higher difficulty, typical of a junior-level, senior-level, or graduate physics course.

Where did you get the equation from? Did you derive it? It's incorrect.
 
but its a course designed for third years. still I have no idea what upper or lower division means
 
(T(equator)^2)/(T(pole)^2)=(g(equator)^2)/(g(pole)^2)
so

g(equator)/g(pole)=sqrt[(T(eq)^2)/(T(pole)^2)]
g(equator)/g(pole)=sqrt[(250^2)/(251^2)]

how is (T(equator)^2)/(T(pole)^2)=(g(equator)^2)/(g(pole)^2)
wrong? I found it in the notes
 

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