Newtonian Gravity: Describing as Vector Field

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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 [tex]\vec{x}_{0}=(x_{0},y_{0},z_{0})[/tex] with mass [itex]m_{0}[/itex]

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

The force [itex]\vec{F}[/itex] 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:

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

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