Recent content by GravityNutt

Consider MT^2/r^3 with M being a mass, T is the period of an orbiting satellite, r is the distance between the center of mass of M and satellite. Consider this a constant, using Kepler's constant. We will call this constant K for these purposes. There are a lot of cool calculations you can do...

When I reduce it to solve for G from Newton's famous equation, it comes out looking odd, I calculate G = (64*pi^10) / c^2. Hope this helps. Thanks

I have been studying gravity for a while on an under graduate level. I have an equation that was derived that uses the speed of light to calculate the gravitational force between two objects. No G needed. Do any of you know of any like equations available that I could compare it with or...