Calculate the gravitational field of a object

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SUMMARY

The discussion focuses on calculating the gravitational field of an object, particularly a black hole, using the formula \(\vec{g} = \frac{GM_1}{r^2} \hat{r}\). It emphasizes that for non-spherical mass distributions, one must integrate the equation by substituting mass \(m\) with differential mass elements \(dm\) based on the object's density function. The principle of superposition is crucial, as it allows the summation of the gravitational fields generated by each \(dm\) in the integral. The conversation highlights the importance of relating the density to the geometry of the problem for accurate calculations.

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  • Concept of the principle of superposition in physics
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taylordnz
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how do you calculate the gravitational field of a object e.g black hole (does it refer to its density and mass?
 
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[tex] \vec{g} = \frac {GM_1} {r^2} \hat{r}<br /> <br /> <br /> [/tex]



if the source mass has a non spherical distribution and you know its density(or density function) you will have to integrate the above equation replacing m by little dm's. Since you must integrate on a geometry, you have to somehow relate the dms to the geometry of the problem (big hint use density) To justify this action, the principle of superposition applies, since it is the superposition of all the little fields generated by the dm's that are added up in the integral. Sorry this answer is so vague, if you can make your question more specific, I can give you a more specific answer.
 
Last edited:
Gza, do you intend that [itex]\vec{r}[/itex] is a unit vector of the r direction?
 

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