What is this constant in the gravitational acceleration formula?

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Homework Help Overview

The discussion revolves around understanding the gravitational acceleration formula, specifically the constant μE in the context of a satellite orbiting Earth. Participants are exploring the implications of this constant and its relationship to other gravitational concepts.

Discussion Character

  • Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to clarify the meaning of μE and its distinction from the geocentric gravitational constant. They question whether μE can be derived from the universal gravitational formula. Other participants provide insights into the formula's components and their relationships.

Discussion Status

Some participants have offered clarifications regarding the formula and its components, while others are exploring different interpretations of the constants involved. There appears to be a productive exchange of ideas, though no explicit consensus has been reached.

Contextual Notes

The original poster expresses confusion regarding the application of the gravitational constant in the context of a satellite, indicating a potential misunderstanding of the formula's parameters. There is also mention of varying symbols for gravitational constants in different contexts.

Kyle91
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Homework Statement



Hey all, I'm doing an assignment and I was given the formula below, but I'm unsure what one of the constants is.

Homework Equations



Acceleration = - μEr/r3

The Attempt at a Solution



Below the formula it says "where μE is the gravitational constant for the Earth and r is the position vector of the vehicle". But this is talking about a satellite orbiting Earth, so it can't be 9.8m/s/s, can it?

Am I meant to use μE = u*m1*m2/r2 to find it?

I've used the 'geocentric gravitational constant' elsewhere in the assignment, but it used a different symbol, this isn't it either is it?

Cheers
 
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The correct formula you asked about is

\vec a = -\mu_e \frac{\vec r}{r^3}

\vec r is the position vector of a satellite or any point-like mass with respect to the centre of Earth, and \vec a is its gravitational acceleration. The formula is a special case of the Universal Law of Gravity,

\vec F = -G \frac{m_1 m_2 \vec r}{r^3}

the force a point mass 1 exerts on an other point mass 2 at distance r. The force is parallel and opposite to the vector \vec r pointing to mass 2 from mass 1.
G is the gravitational constant G= 6.67259 ˙10-11 Nm2kg-2.

If the first mass is the Earth, Gm1=GMearthe.

ehild
 
Is that 'Gravitational Constant' the 'Universal Gravitational Constant (6.67*10-11' Nascent?
 
Ignore my above post.

That makes sense ehild! Because F = ma, a = F/m. You remove the mass of the satellite from your second formula and exchange F for a. Leaving you with a = G*mE*r/r3.

Thanks!
 
All right, I see you got it.

ehild
 

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