Gravitation force caused by uniform rod

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SUMMARY

The gravitational force exerted by a thin uniform rod of length L on a point mass located at a distance R perpendicular to the rod's center is calculated using the formula g = -\frac{2G\rho}{R}*(L/\sqrt{L^2+4R^2}). The derivation involves integrating the gravitational contributions from differential mass elements along the rod, utilizing the gravitational constant G and linear mass density ρ. The integration limits are set from -L/2 to +L/2, and the y-components of the gravitational force cancel out, simplifying the calculation.

PREREQUISITES
  • Understanding of gravitational force equations, specifically g = -\frac{GM}{r^2}
  • Familiarity with calculus, particularly integration techniques
  • Knowledge of trigonometric functions and their applications in physics
  • Concept of linear mass density (ρ) in relation to gravitational force
NEXT STEPS
  • Study the derivation of gravitational force from continuous mass distributions
  • Learn about the application of trigonometric substitution in integrals
  • Explore gravitational field calculations for different geometries, such as disks and spheres
  • Investigate the use of numerical methods for gravitational force calculations in complex systems
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Students in physics, particularly those studying classical mechanics, as well as educators and professionals involved in gravitational field analysis and mathematical physics.

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Homework Statement


What is the gravitational force caused by a thin uniform rod of length L on a point mass located perpendicular to the rod at it's center? Assume the point mass is a distance R perpendicular to the rod.


Homework Equations


[tex]g = - \frac{GM}{r^2}\hat{r} = - G\rho \int \frac{dV}{r^2}\hat{r}[/tex]


The Attempt at a Solution



[tex]g = -G\rho \int \frac{Rdx}{\sqrt{x^2+R^2}^3}[/tex]
[tex]x = Rtan(\phi)[/tex]
[tex]g = -\frac{G\rho}{R} * ( \frac{x}{\sqrt{x^2+R^2}} )[/tex]
Using limits of integration from -L/2 to +L/2 to yield:
[tex]g=-\frac{2G\rho}{R}*(L/\sqrt{L^2+4d^2})[/tex] after removing a factor of 4 from the (L/2)^2 from the square root.

Since the y components cancel, I took theta to be the angle nearest the point mass, and called rhat cos(theta) which I evaluated to R/sqrt(x^2+R^2) which could combine with the r^2 in the denominator from the gravity equation.

If this is wrong, I'll be glad to provide more steps to see where I went wrong. I ended up with a 1/(x^2+R^2)^(3/2) in the integral, so I did a trig substition to integrate it, and came up with the formula wikipedia has in its irrational integrals table, so I'm pretty sure that's alright, but wasn't sure if I set it up right.
 
Last edited:
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Looks okay to me. This is how I did it (I get the same integrand form)

[tex]d\vec{f} = \frac{Gdm}{R^2+x^2}\left(-\cos\theta \hat{i} + \sin\theta \hat{j}\right)[/tex]

where

[tex]\cos\theta = \frac{R}{\sqrt{R^2+x^2}}[/tex]
[tex]\sin\theta = \frac{x}{\sqrt{R^2+x^2}}[/tex]

The integrand over [itex]\hat{i}[/itex] is an odd, so it integrates to zero ([itex]x[/itex] ranges from [itex]-L/2[/itex] to [itex]L/2[/itex]). You get

[tex]\vec{f} = -\hat{j}G\lambda R\int_{-L/2}^{L/2}\frac{1}{(x^2+R^2)^{3/2}}dx[/tex]
 
Last edited:

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