Hydrostatic equilibrium for stars question

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SUMMARY

The discussion focuses on solving a hydrostatic equilibrium problem for stars using the equation \(\vec{f} - \text{grad} p = 0\). The user has successfully completed part a using the mass function \(m(r) = \int 4\pi r^2 \rho dr\) and seeks assistance for parts a and b. The task involves applying the gradient operator in spherical coordinates to determine the gravitational field at an arbitrary point within the star.

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  • Understanding of hydrostatic equilibrium in astrophysics
  • Familiarity with spherical coordinates
  • Knowledge of calculus, specifically integration
  • Basic concepts of gravitational fields
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  • Research the application of the gradient operator in spherical coordinates
  • Study the principles of hydrostatic equilibrium in stellar structures
  • Explore gravitational field calculations within celestial bodies
  • Investigate software tools for astrophysical simulations
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Astronomy students, astrophysicists, and anyone studying stellar dynamics and hydrostatic equilibrium in stars.

coffeem
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Hi, I have attatched the question. I have done part a using: m(r) = integral(4pir^2rhodr).

Does anyone have any suggestions for parts a and b?

Thanks

p.s. if anyone knows of a freeware program for paints for macs i would appretiate it rather than having to create pdf's lol
 

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for the second part use the equation for hydrostatic equilibrium:

\vec{f}-\text{grad}p =0

Where f force exerted on the volume (in this case gravity).

So write out the gradient operator in spherical coordinates and determine the gravitational field in an arbitrary point inside the star, and you are done.
 

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