Calculating Gravitational Forces and Potential Energy Using Newton's Laws

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SUMMARY

This discussion focuses on calculating gravitational forces and potential energy using Newton's laws, specifically addressing the equations of motion for a system of point masses. The primary equation discussed is the gravitational force equation, $$\vec {F} = \Sigma_{j} \frac{m_{i} m_{j}}{\left(r_j - r_i \right)^{1.5}} \vec{r_j} - \vec {r_i}$$, which leads to the kinetic energy equation $$K = 0.5 m_{i} \Sigma_{j} {g_{j}}^2 t^{2}$$ and potential energy equation $$U = -K$$. The validity of these equations is debated, particularly regarding the assumption of constant force and the implications for energy conservation in an isolated system.

PREREQUISITES
  • Newton's Laws of Motion
  • Gravitational Force Calculations
  • Concept of Kinetic and Potential Energy
  • Vector Calculus in Physics
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  • Study the derivation of gravitational force in Newtonian mechanics
  • Explore the conservation of energy in isolated systems
  • Learn about the role of the gravitational constant (G) in force calculations
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Nirmal Padwal
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Homework Statement
Consider an isolated system of N point objects interacting via gravity. Let the mass and position vector of the ith object be ##m_{i}## and ##\vec{r_i}## respectively. What is the vector equation of motion of the ith object? Write expression for the total kinetic energy ##K## and potential energy ##U## of the system. Demonstrate from the equations of motions that ##K+U## is a conserved quantity
Relevant Equations
1. ##\vec{F} = m \vec {a}##
2. ##K = 0.5 m \frac {d}{dt}{r_{i}}^2##
3. ##U = mgr_{i}##
For the first part, I considered the Force acting on it by all charges as given by
$$\vec {F} = \Sigma_{j} \frac{m_{i} m_{j}}{\left(r_j - r_i \right)^{1.5}} \vec{r_j} - \vec {r_i}
= \Sigma_j m_i \vec {g_j} $$

Where ##\vec{g_{j}}## represents gravitational acceleration of ##m_i## due to jth mass

I approached the problem coordinate-wise i.e first the x coordinate and y and z equations have to be analogous. I equated above equation with ##\vec {F}=m \vec{a}## and integrated twice and then combined results for all three coordinates to get
$$\vec{r_{i}} =\Sigma_j 0.5 g_j t^{2} $$

I assumed the particle of interest starts from rest and initially positioned at origin.. hence no integration constants.

Now I used above formula for K.. i.e I differentiated ##r_{i}## and mulitiplied the result by factor ##0.5 m_{i}## to get
$$K = 0.5 m_{i} \Sigma_{j} {g_{j}}^2 t^{2}$$

Similarly I used above equation of U and got the same equation as for K but with a negative sign (as gravitational forces are attractive). They do add up to zero.

Now, I don't know if this approach is valid or it is just nonsense.. Is it valid?
 
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It would be good if you fixed your latex.
 
Nirmal Padwal said:
$$\vec{r_{i}} =\Sigma_j 0.5 g_j t^{2} $$

I assumed the particle of interest starts from rest and initially positioned at origin.. hence no integration constants.

If you have assumed that the force on particle ##i## from particle ##j## is constant (over time), then that is not going to work in general.
 
I have fixed the latex. The chapter's name is Newtonian Gravity. Force in Newtonian gravity depends only on the masses and relative distances between them right and it is independent of time, isn't it?
 
Nirmal Padwal said:
I have fixed the latex. The chapter's name is Newtonian Gravity. Force in Newtonian gravity depends only on the masses and relative distances between them right and it is independent of time, isn't it?

Not if the masses are free to move. Then the distance between them is changing over time.
 
Nirmal Padwal said:
Homework Statement: Consider an isolated system of N point objects interacting via gravity. Let the mass and position vector of the ith object be ##m_{i}## and ##\vec{r_i}## respectively. What is the vector equation of motion of the ith object? Write expression for the total kinetic energy ##K## and potential energy ##U## of the system. Demonstrate from the equations of motions that ##K+U## is a conserved quantity
Homework Equations: 1. ##\vec{F} = m \vec {a}##
2. ##K = 0.5 m \frac {d}{dt}{r_{i}}^2##
3. ##U = mgr_{i}##

For the first part, I considered the Force acting on it by all charges as given by
$$\vec {F} = \Sigma_{j} \frac{m_{i} m_{j}}{\left(r_j - r_i \right)^{1.5}} \vec{r_j} - \vec {r_i}
= \Sigma_j m_i \vec {g_j} $$

Where ##\vec{g_{j}}## represents gravitational acceleration of ##m_i## due to jth mass

I approached the problem coordinate-wise i.e first the x coordinate and y and z equations have to be analogous. I equated above equation with ##\vec {F}=m \vec{a}## and integrated twice and then combined results for all three coordinates to get
$$\vec{r_{i}} =\Sigma_j 0.5 g_j t^{2} $$

I assumed the particle of interest starts from rest and initially positioned at origin.. hence no integration constants.

Now I used above formula for K.. i.e I differentiated ##r_{i}## and mulitiplied the result by factor ##0.5 m_{i}## to get
$$K = 0.5 m_{i} \Sigma_{j} {g_{j}}^2 t^{2}$$

Similarly I used above equation of U and got the same equation as for K but with a negative sign (as gravitational forces are attractive). They do add up to zero.

Now, I don't know if this approach is valid or it is just nonsense.. Is it valid?

You got K+U=0? Consider our solar system. It is approximately isolated,interacts via gravity and consist of finite bodies. Since all the hypothesis are true ,our solar system should have 0 net energy which is not true since the energy of system is negative in this case. The flaw in reasoning is equation of ##r_i## in terms of ##g_j##. Please fix it, I didn't check. Alternatively,try differentiating K+U w.r.t time and show that it is 0!
 
Nirmal Padwal said:
2. ##K = 0.5 m \frac {d}{dt}{r_{i}}^2##
Did you mean ##\frac{d}{dt}(\vec r \cdot \vec r)##, which is what you wrote? Or did you mean ##\dot {\vec r} \cdot \dot {\vec r}##?

3. ##U = mgr_{i}##
This isn't correct.

For the first part, I considered the Force acting on it by all charges as given by
$$\vec {F} = \Sigma_{j} \frac{m_{i} m_{j}}{\left(r_j - r_i \right)^{1.5}} \vec{r_j} - \vec {r_i}
= \Sigma_j m_i \vec {g_j} $$
Why 1.5 in the exponent in the denominator? Missing factor of ##G##? ##i \ne j##? Also, ##\vec{r_j} - \vec {r_i}## should be in parentheses.
 

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