For any eclipse, all three bodies are in the same straight line. For a solar eclipse, the moon is the one in the middle. For a lunar eclipse, the Earth is the one in the middle.
The relativistic formula for the momentum of a particle of mass m and moving at speed v is

where c is the speed of light.
In our problem, the speed in terms of c is

, and the mass (still written in terms of c) is

. Substituting these values in the previous formula, we can find the value of the momentum of the proton:
Newton's third law<span> is for every action, there is an equal and opposite reaction. The statement means that in every interaction, there is a pair of forces acting on the two interacting objects. </span>