I have a couple questions on gravity

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SUMMARY

This discussion focuses on the fundamental principles of gravity, specifically the gravitational force equation F_G = -G(mM/r^2) and the gravitational field due to a point mass, expressed as -GM/r^2. It emphasizes the importance of understanding Newtonian gravity before delving into Einstein's theories. The conversation also highlights how to calculate mass from density using the integral of density over volume or the formula for a sphere's volume. Key concepts include gravitational force, mass, and density.

PREREQUISITES
  • Understanding of Newtonian gravity and gravitational force equations
  • Basic knowledge of calculus for integrating density
  • Familiarity with concepts of mass and density in physics
  • Awareness of gravitational constant (G) and its significance
NEXT STEPS
  • Study the derivation and applications of the gravitational force equation F_G = -G(mM/r^2)
  • Explore the concept of spacetime curvature in Einstein's General Relativity
  • Learn about the relationship between mass, density, and gravitational fields
  • Investigate the implications of gravitational fields in astrophysics and cosmology
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Students of physics, educators, and anyone interested in understanding the principles of gravity and its mathematical formulations.

Darkroman
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My physics knowledge is barely 101 so bare with me. However I've always wondered about gravity, just never took much time to look it up. I was hoping you could help me out a bit on it, perhaps give me some internet links to learning resources.

Is there an equation to state (let's say an ideal or perfect celestial sphere about 10,000 miles in diameter, and density is on the order of 2) how much gravity it has (or is it better to say how much it curves spacetime)?

Can you make a connection between the mass an object has with the amount of gravity? How about density?

Thanks in advance.
 
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Yes. The gravitational field due to a point mass (in units of acceleration) is -GM/r^2. Any massive object with a spherically symmetric mass density distribution (eg. a planet or a star) can be modeled as a point mass at the centre of the sphere so that you can use this equation (as long as r > radius of the body).

That's the Newtonian (classical) theory. I don't suggest learning Einstein's version before this.
 
So, if you want to calculate the gravitational force a massive object of mass M exercises on some other mass m, it would be done like this:
F_G = -G\frac{mM}{r^2}. Where F_G is the gravitational force, G the gravitational constant and r the distance between the two objects. (either as size or vector)
If you only know the density of the object, you can calculate the mass like this:
{\int\int\int}_V \rho(x,y,z) dV or, if the density \rho is constant: \rho \times V = \frac{4}{3} \pi R^3 \rho
Hope this helps!
 

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