What Rotation Period Causes 9.8 m/s² Equatorial Acceleration?

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Homework Help Overview

The problem involves determining the rotation period required for objects at the equator to experience a centripetal acceleration of 9.8 m/s². This relates to concepts in rotational motion and gravitational forces.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to solve for the rotation period using the relationship between centripetal acceleration and velocity. Some participants explore the concept of orbital motion around Earth and question the implications of gravitational parameters.

Discussion Status

The discussion is ongoing, with participants providing different perspectives on the problem. Some guidance has been offered regarding the gravitational parameter, but no consensus has been reached on the correct approach or solution.

Contextual Notes

There is a mention of a discrepancy with the original poster's calculation and the feedback received from Webassign, indicating potential constraints in the problem setup or assumptions being made.

lauriecherie
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Homework Statement



What would Earth's rotation period have to be for objects on the equator to have a centripetal acceleration equal to 9.8 m/s^2?

____ min


Homework Equations



Centripetal acceleration is equal to velocity * (2PI/T),
where T is the period in seconds.




The Attempt at a Solution



I set centripetal acceleration equal to 9.8m/s^2 and solved for T. Then I took T and divided it by 60 so I could get the answer in minutes. I came out with 4.97 min which Webassign says is incorrect. Any ideas?
 
Last edited:
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One way to look at it is that if the object is not to fall into the center then calculate the orbit about a mass of Earth at 1 Earth radius.

So what is the period of such an orbit?

V2/R = GM/R2 = ω2R

ω2 = GM/R3 = (2π /T)2

T = 2π*(R3/GM)1/2
 
What does GM stand for?
 
lauriecherie said:
What does GM stand for?

That's sometimes written as μ which is the standard gravitational parameter for earth.

It is the product of Earth's mass and the Universal Gravitational constant.
 

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