Nick Jarvis said:
Observer:
He/she will calculate the time taken as length/velocity PLUS the the time taken according to astronaut, so t = 113.78m / 0.88c = 4.31 x 10^-7 PLUS 1.06 x 10^-7 seconds. Is this correct?
How long will the spacecraft be according to the object being thrown? Will this be the same as the observer's calculated length, as the object also moving at 0.6c??
I am finding this so difficult to grasp.
Thanks
Apart from the rest length of the spaceship changing from 180m to 190m, you were right on the first part.
Regarding the object moving within the spaceship: yes, it is an important and valid point that to them the spaceship is moving at 0.6c backwards, so their observations will agree with the "stationary" observer in terms of length contraction.
The final point is the time for this object to travel the length of the ship according to the stationary observer. The trick here is to note the following fact:
In SR (as in classical physics), if you stay within a single IRF, you may apply the normal addition/subtraction of velocities (for
velocities in your frame).
If ##v## is the velocity of an object in your frame and ##u## is the velocity of another object in your frame, then the "separation" velocity of these two objects in your frame is simply:
##v_s = u - v##
In other words, SR requires no changes to this natural, classical calculation, as long as
everything is measured in your reference frame. It's the same with distances. SR only requires changes when you consider velocities (or distances or times) measured in two different reference frames.
Note that the
velocity addition formula relates velocities as
measured in different frames, as follows.
If ##V## is the velocity of frame S' relative to your frame and ##u'## is the velocity of an object (as measured in frame S'), then the velocity of the object as measured in your fame is:
##u = \frac{V + u'}{1 + Vu'/c^2}##