Newtonian Gravity: Describing as Vector Field

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Newtonian gravity can be described as a vector field generated by a mass located at a specific point in space. The gravitational force per unit mass at any other point is given by a formula that accounts for the distance between the two points and the mass involved. This force can be expressed in Cartesian coordinates or transformed into spherical coordinates, emphasizing the radial nature of gravitational attraction. The force acting on another mass is derived by multiplying the gravitational field by the mass of the object. Overall, this framework illustrates how gravity operates as a vector field in space.
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how would you describe Newtonian gravity as a vector field?
 
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Well, as a simple case, suppose you've got a mass positioned at location \vec{x}_{0}=(x_{0},y_{0},z_{0}) with mass m_{0}

Then, for any spatial point (x,y,z)=\vec{x}\neq\vec{x}_{0}
that mass generates at that point a force per unit mass:
\vec{f}(x,y,z)=-\frac{Gm_{0}}{||\vec{x}-\vec{x}_{0}||^{3}}(\vec{x}-\vec{x}_{0})

The force \vec{F} acting upon an object of mass M situated at (x,y,z) is then found by multiplying f with M.
 
Another form you sometimes see assumes that the mass is at the origin, and uses spherical coordinates:

\vec F (r, \theta, \phi) = - \frac{G m_0}{r^2} \hat r

where \hat r is the unit vector in the outward radial direction at that particular point.
 
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