Take two large masses far from other large ones, just to make things simpler. Fix them to each end of a rigid rod with a device for measuring attractive force between the two. Make sure the axis
a running through both centres of mass has a stable direction, referred to the fixed stars, let things settle nicely and then measure the attractive force,
f. Knowing the two masses and the distance
r between them,
f should match up the well known calculation, proportional to both masses for given
r.
Now, surely there are many things wizzing along at velocities approaching
c and in various directions. From these frames of reference the pair of masses will be wizzing at that velocity, the opposite way. For some directions,
r will be contracted, while it won't for directions at right angles to
a. For such observers, what should the attractive force between the two masses be?
Think carefully...
