To find the relative velocity of one galaxy as observed from the other, we use the relativistic velocity addition formula, which states:
where:
is the velocity of the first galaxy relative to Earth (200,000 km/s), is the velocity of the second galaxy relative to Earth (200,000 km/s), is the speed of light (~300,000 km/s).
Plugging in the values:
Calculating the denominator:
So the equation becomes:
Thus, the speed at which an observer in one galaxy would see the other galaxy moving away is approximately 276,000 km/s.
The correct response is:
between 200,000 and 300,000 km/s.