Imagine an arbitrary point in space. It is within the gravitational 'potential' of *every* mass (although billions of ly away) in the entire universe. 

Since every mass adds a tiny fraction, what is the *total* gravitational 'potential' energy in this point?

**Edit:**

Let point masses be located distance $r_i$ from the point and have masses $m_i$, then the 'potential' is

$$\Phi = - G \sum_{i} \frac{m_i}{r_i}.$$

I'm looking for this value averaged over all points in space. How does this depend on the shape of our universe or can we measure it?

 - For example gravity on my location is given by
$$ 9.81 m/s^2 \text{(earth )} + 6 mm/s^2 \text{(sun)} + 200 pm/s^2 \text{(milky way)} +  ?  \text{(rest of the universe)}.$$