
Originally Posted by
Steve Miller
That's a point I'm confused about. Everything was in motion, all the time. In space, one
could not decide what the own actual status was. Would you agree or not?
On earth it's easier I would say.
This is where the 'frame of reference' idea comes in. If you are just going around the earth in orbits, you can ignore the other motions, and consider "Earth" to be the centre of the frame of reference... temporarily making it the centre of the universe for the simplicity of visualization. If however you need to go to another body, you need to make something else the frame of reference, for instance going to the moon, you have the earth as the frame of reference (acting as a fixed point for calculatons) until you enter the moon's dominant gravity "Sphere of influence" after which you ignore the Earth and calculate based on the Moon being a fixed reference point. If you are going to Mars, you consider Earth the centre of reference until you achieve escape velocity, and then you can consider the Sun to be the centre fixed point of reference... until you approach mars and slow down to orbit that body. The hard points come when you are in the 'transition' zone where the langrange points start happening, and then large newtonian equasions start being needed to work out what's going on.
But unless you want to work for NASA, usually the simplified "Relevant frame of reference" and "Orbit is falling" is good enough for the concepts to work... good enough to even simulate/play with the Orbiter program and get yourself to the moon and back in the simulator.