Gravitational Potential & Gravitational Potential Energy

In summary, this increases the work done to move the mass from infinity to a point in a gravitational field.
  • #1
Jimmy87
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Homework Statement
Understanding the Definitions and Model
Relevant Equations
V = - GM/R and E = - GMm/R
Hi,

I am confused about the negative aspect of these quantities. The definition in my book for gravitational potential is:

"The work done to move a unit mass from infinity to a point in a gravitational field"

I understand that the work done is negative because gravity is doing the work if you starting point is infinity. However, my book has a key points section and says it is "important to understand that moving towards the gravitating mass is a decrease in gravitational potential and moving away represent an increase". This does not make sense in terms of the definition given. If you move further away from Earth then LESS work is done per unit mass bringing it from infinity. I understand the value of the potential will be less negative/more positive so that is a larger number but the fact it increases as you get further away does not make sense with the definition of potential otherwise we would be saying that this increases:

"The work done to move a unit mass from infinity to a point in a gravitational field"

This is the definition of gravitational potential in my book and on numerous websites and it does not increase as you get further from the Earth! There is not an increase in the work done per unit mass from infinity! If it's because the number is more positive that's fine but then the definition needs changing surely!

Can someone please kindly explain. Thank you.
 
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  • #2
Jimmy87 said:
"important to understand that moving towards the gravitating mass is a decrease in gravitational potential and moving away represent an increase"
Decreases in the sense of more negative. There's no contradiction. It does not say the magnitude decreases.
 
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  • #3
Jimmy87 said:
Can someone please kindly explain. Thank you.
One idea is to use positive work. Start at some reference radius ##R_0## and calculate the (positive) work needed to move a unit mass out to a new radius ##R > R_0##. With this reference we have:
$$V^*(R) = \int_{R_0}^R \frac{GM}{r^2} \ dr = \big [-\frac{GM}{r} \big ]_{R_0}^R = - \frac{GM}{R} + \frac{GM}{R_0}$$
Now, we simply change our reference so that ##V(\infty) = 0## by subtracting the constant term ##\frac{GM}{R_0}## to give:
$$V(R) = - \frac{GM}{R}$$
Note that ##V(R)## is increasing as ##R## increases - and has a maximum of ##0## as ##R## goes to infinity.

It's perhaps a good exercise to work all this out for yourself using negative work and a mass coming in from infinity.
 
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FAQ: Gravitational Potential & Gravitational Potential Energy

1. What is gravitational potential?

Gravitational potential is the measure of the potential energy that an object has due to its position in a gravitational field.

2. How is gravitational potential calculated?

Gravitational potential is calculated using the formula U = -GmM/r, where U is the gravitational potential, G is the gravitational constant, m and M are the masses of the two objects, and r is the distance between them.

3. What is gravitational potential energy?

Gravitational potential energy is the energy that an object possesses due to its position in a gravitational field. It is equal to the product of the object's mass, the acceleration due to gravity, and the height of the object above the reference point.

4. How is gravitational potential energy related to gravitational potential?

Gravitational potential energy and gravitational potential are directly related. The change in gravitational potential energy of an object is equal to the negative of the work done by the gravitational force, which is equal to the product of the object's mass and the change in gravitational potential.

5. What are some real-life applications of gravitational potential and gravitational potential energy?

Gravitational potential and gravitational potential energy are important concepts in understanding the motion of objects in space, such as planets orbiting around a star. They are also used in fields such as astrophysics, geology, and engineering for calculations and predictions related to objects in a gravitational field.

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