TurtleMeister said:
Another misunderstanding I may have had is that in the past I have always associated the third law pair with objects and not forces. So in my thought experiment there is only one third law pair while I am in free fall (the force pulling me and the force pulling the object). But when I touch the surface another pair appears? How does this other pair, or other pairs if there are more, differ from the single pair while I am in free fall?
Newton's third law is about objects and forces.
Backing up a bit, what are Newton's laws? As taught by most, Newton's laws leave concepts such as time, mass, and force as undefined terms. (Similarly, point, line, and plane are undefined terms in Euclidean geometry.) I'll delve into those if you want.
Another concept that isn't quite explicit in Newtonian mechanics is the superposition principle. The net force acting on some object is the vector sum of the individual forces acting on the object. Arnold Sommerfeld, nominated for the Nobel prize a record 81 times (he never got it) and teacher of six Nobelists, saw the superposition principle as so important that he called it Newton's fourth law.
With this in mind, consider the forces acting on / exerted by the Earth's Moon. Newton's law of gravitation says that the Moon is subject to gravitational forces from the Earth and the Sun, and also all of the other planets in the solar system and even everything else in the universe. The superposition principle is what let's us add all of these forces together to yield the net force on the Moon. Here's the rub: You aren't going to be able to find an equal but opposite reaction to this net force. You need to look to the individual forces to find those equal but opposite reactions.
Now let's look at something a bit closer to Earth, a vehicle in low Earth orbit. We have the same gravitational third law pairs as before, but now atmospheric drag also comes into play. Once again the superposition principle let's you compute the net force and once again you won't be able to find an equal but opposite reaction to this net force. You must look to the individual forces to find the third law pairs. Atmospheric drag reduces the vehicle's speed with respect to the Earth, so per Newton's third law the vehicle must speed up the atmosphere (by a tiny, tiny bit).
Now let's get down to the Earth and look at a person at the equator standing still on a scale on the rotating Earth. I'm going to ignore the Sun, the Moon, and all the rest of the stuff in the universe. Even ignoring all that, there are still a whole lot of third law interactions to consider. One way to compute the net force is to once again apply the superposition principle. I'll do that later. An alternative is to use Newton's second law, which is a kinematic theorem. The person is in uniform circular motion, rotating at 1 revolution per sidereal day at a distance of 6378 km from the Earth's rotation axis. This corresponds to a centripetal acceleration of 0.033915 m/s
2. Assuming the person masses 70 kg, the net force on the person is 2.37405 Newtons. Whatever the myriad of forces that act on the person are, we know from kinematics that the net force is necessarily 2.37405 Newtons directed toward the center of the Earth.
So what are the forces acting on the person? Gravity pulls the person toward the center of the Earth, the normal force pushes the person up, and buoyancy also gives a slight upward force. We can compute the buoyant force and gravity, we know the net force, so now we can calculate the normal force. Finally, the third law tells us what the person is doing to the scale, the Earth, and the atmosphere -- but only if we consider the individual components of the net force.
Note that by putting the person on the equator all of these forces, including the net force, are directed toward or away from the center of the Earth. Things get hairier away from the equator.