Background
Say I weigh $80 \mathrm{kg}$, and I happen to fall to the ground with an acceleration of roughly $9.81 \frac m{s^2}$, I would, using Newton's second law of motion, $F = ma$, come to the conclusion that the gravitational force between me and Earth is roughly $800 N$ (rounded for simplicity).
Question
Using Newton's law of universal gravity, $F = G \frac{m_1, m_2}{r^2}$, it seems more difficult to conclude the same result, simply because of the way Earth's mass overpowers the calculation. Moreover, it's not obvious to me what the distance $r$ is between me and the Earth.
Can this formula be used in a reliable way between two objects with such vastly different masses, and "wonky" distance?
Own thoughts
The reason I call it a "wonky" distance is because
using a distance of $r = 0$ is out of the question. I can't divide by it, and besides, Earth probably doesn't pull with all its force emanating from the point on the surface closest to me
using a distance of $r = \text{Earth's radius}$ also seems like an oversimplification. Presumably it's not just the very center of the planet that's pulling on me, but rather the entire thing, in different directions, with different magnitudes (verification needed)
I assume the formula would make more sense if I were in deep space, and the distance was such that the radius of the planet was almost negligible? Nevertheless, would the formula hold if I used sufficiently precise values for $G$ and the mass of Earth? Or is it near impossible because of some other factor?
Similar questions
I submit that it does not answer my question because the second object is the moon, which already has a distance that trivializes the radius of Earth, and my measly mass.