General Potential Gravitational Energy

In summary, the equation U= GMm/r has many applications, such as calculating an object's escape velocity from Earth and determining changes in gravitational potential energy as an object moves away from Earth's surface. This equation is used when the object is too far from Earth for the simpler equation U = mgy to accurately represent changes in gravitational potential energy. The reference point for U = GMm/r is at r = infinity, while the reference point for U = mgy can be chosen as convenient for the specific problem being solved.
  • #1
jubaitca
4
0
I was just wondering if there were any applications of the equations
U= GMm/r. Which basically means we are not to involve anything on Earth's surface.

Thx
 
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  • #2
jubaitca said:
I was just wondering if there were any applications of the equations U= GMm/r.
Sure. Whenever you need the gravitational PE between two objects. For example, you can use this to calculate the velocity that an object needs to have so that it doesn't fall back down to Earth (so-called "escape velocity").

Which basically means we are not to involve anything on Earth's surface.
For objects that stay near the Earth's surface, it's more convenient to use U = mgy to study changes in gravitational PE. But if the object gets too far from the surface, the value of "g" decreases, and that simple equation no longer works accurately. That's when you need to use U = -GMm/r.

Note that the reference point where U = 0 is different for each formula. (The reference point is arbitrary, since only changes in U matter.) When using U = mgy, the reference point is some position where y = 0, chosen as convenient for the problem that you are trying to solve; when using U = -GMm/r, the reference point is at r = infinity.
 
  • #3
jubaitca said:
I was just wondering if there were any applications of the equations
U= GMm/r. Which basically means we are not to involve anything on Earth's surface.

Thx
Sure there are. See the example I layed out at

http://www.geocities.com/physics_world/gr/red_shift.htm

What you're looking for is at the bottom of the page.

Pete
 

FAQ: General Potential Gravitational Energy

1. What is General Potential Gravitational Energy?

General Potential Gravitational Energy is a type of potential energy that exists between two objects due to their gravitational attraction. It is a measure of the work that would be needed to move an object from its current position to a reference position where the gravitational force is zero.

2. How is General Potential Gravitational Energy calculated?

The formula for General Potential Gravitational Energy is E = mgh, where E is the energy, m is the mass of the object, g is the acceleration due to gravity, and h is the distance between the two objects. This formula is based on the gravitational potential energy equation derived by Sir Isaac Newton.

3. What factors affect General Potential Gravitational Energy?

The factors that affect General Potential Gravitational Energy include the masses of the objects, the distance between them, and the strength of the gravitational force. The greater the mass and the closer the distance between the objects, the higher the potential energy will be.

4. What is the relationship between General Potential Gravitational Energy and kinetic energy?

General Potential Gravitational Energy and kinetic energy are two forms of energy that are related to each other. As an object falls towards the ground, its potential energy decreases and its kinetic energy increases. When the object reaches the ground, all of its potential energy is converted into kinetic energy.

5. How is General Potential Gravitational Energy used in real life?

General Potential Gravitational Energy is used in many everyday applications, such as hydroelectric power plants, roller coasters, and even simple activities like throwing a ball. It is also an important concept in fields such as astronomy and physics, as it helps us understand the behavior of objects in our universe.

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