I have a couple questions on gravity

  • Thread starter Thread starter Darkroman
  • Start date Start date
  • Tags Tags
    Couple Gravity
AI Thread Summary
Gravity can be quantified using the equation F_G = -G(mM/r^2), where F_G is the gravitational force, G is the gravitational constant, m and M are the masses of the objects, and r is the distance between their centers. For a spherically symmetric mass distribution, such as a celestial sphere, it can be treated as a point mass at its center for calculations outside its radius. The gravitational field strength can also be derived from the density of the object, allowing for mass calculations using volume integrals. Understanding Newtonian gravity is recommended before exploring Einstein's theories. This foundational knowledge is essential for grasping the relationship between mass, density, and gravitational effects.
Darkroman
Messages
5
Reaction score
0
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.
 
Physics news on Phys.org
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!
 
I think it's easist first to watch a short vidio clip I find these videos very relaxing to watch .. I got to thinking is this being done in the most efficient way? The sand has to be suspended in the water to move it to the outlet ... The faster the water , the more turbulance and the sand stays suspended, so it seems to me the rule of thumb is the hose be aimed towards the outlet at all times .. Many times the workers hit the sand directly which will greatly reduce the water...

Similar threads

Replies
13
Views
2K
Replies
5
Views
2K
Replies
12
Views
2K
Replies
42
Views
6K
Replies
9
Views
3K
Replies
5
Views
2K
Replies
18
Views
1K
Replies
2
Views
37K
Back
Top