Calculating Gravity of a Single Body: Equation and Explanation

In summary, the equation for calculating a single body's gravity is g(r)=-G\frac{m}{r^{2}}\hat{r} for a uniform spherical mass distribution, where G is the gravitational constant, m is the mass of the object, r is the distance from the center of the object, and \hat{r} is the unit vector in the radial direction. This equation only applies for distances outside of the object and assumes a spherically symmetric mass distribution. As you approach the center of the object, the gravitational force decreases and reaches zero at the center. This can be represented by the equation g(r)=-\frac{Gm_{0}}{r_{0}^{3}}r\hat
  • #1
chis
51
0
Sorry to ask such a simple question but I appreciate the level of knowldege you guys have.
What is the equation for calculating a single bodies gravity?
 
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  • #2
The gravitational field strength is = GM/r
(in classical gravity - it's a bit more complicated in general relativity)

It's really just a different way of writing the equation in the other thread for the force on a 1kg object placed at a distance 'r'
 
  • #3
Is r measured from the centre of the object? If so is gravity stronger closer to the centre of the earth.
Thanks by the way
Chris
 
  • #4
Yes The nice thing about Newton's gravity is you can just use the total mass at the 'centre of gravity' and not have to care about the shape or distribution.
The Earth could actually be hollow and as long as it had the same total mass you wouldn't be able to tell - gravity would work just the same.
 
  • #5
So at the centre of an object the value r = 0
 
  • #6
While in Newtonian gravity you treat all an object's mass as if it were located at the center, this assumption is only valid while you are outside of the body. If, for example, you started digging into the earth, you would find that the gravitational force decreases to zero as you approach the center.
 
  • #7
Is there an equation tht reflects this?
 
  • #8
Nabeshin said:
While in Newtonian gravity you treat all an object's mass as if it were located at the center, this assumption is only valid while you are outside of the body.
Furthermore, it's only valid for spherically symmetric mass distributions.
 
  • #9
chis said:
Is there an equation tht reflects this?

Assuming a uniform spherical mass distribution, we have the following equations:

[tex]g(r)=-G\frac{m}{r^{2}}\hat{r} ; r>r_{0}[/tex]
[tex]g(r)=-\frac{Gm_{0}}{r_{0}^{3}}r\hat{r} ; r<r_{0}[/tex]
 

1. What is the equation for calculating the gravity of a single body?

The equation for calculating the gravity of a single body is F = (G * m1 * m2)/r^2, where F is the force of gravity, G is the gravitational constant (6.67 x 10^-11 m^3/kg*s^2), m1 and m2 are the masses of the two bodies in kilograms, and r is the distance between the two bodies in meters.

2. How does the distance between two bodies affect the force of gravity?

The force of gravity is inversely proportional to the square of the distance between two bodies. This means that as the distance between two bodies increases, the force of gravity decreases. For example, if the distance between two bodies is doubled, the force of gravity between them is decreased by a factor of four.

3. What is the gravitational constant and why is it important in the equation?

The gravitational constant, denoted by G, is a fundamental constant in physics that represents the strength of the gravitational force between two objects. It is important in the equation for calculating the gravity of a single body because it determines the magnitude of the force of gravity and ensures that the units of the equation are consistent.

4. Can the equation for calculating gravity be used for any two bodies?

Yes, the equation for calculating the gravity of a single body can be used for any two bodies. However, it is most accurate for two point masses (objects with negligible size) and becomes less accurate for larger or irregularly shaped objects.

5. How is the force of gravity related to the mass of the two bodies?

The force of gravity is directly proportional to the masses of the two bodies. This means that as the masses of the two bodies increase, the force of gravity between them increases as well. For example, if the mass of one body is doubled, the force of gravity between it and the other body will also double.

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