Strength of gravitational waves vs. electromagnetic waves If the recent gravitational wave's energy had reached us as visible light, how bright would it have been? Stackexchange complains about the form and brevity of the question so i add something... if it is strong enough to move a heavy mirror albeit by a 10000 th of a proton it should be quite strong and intuitively the light of even a bright star shouldn't have that strength.
 A: The only meaningful way to compare "strength" between light and a gravitational wave is via the energy flux they deliver. (Otherwise, how do you compare a stretch in the geometry of space and time with an electric field?)
In that vein, then, a good representative is the first observation, GW150914, which emitted an energy of about $E=3.0\:M_\odot c^2$ in about $\Delta t=0.1\mathrm{\:s}$ at a distance of some $L=440\:\mathrm{Mpc}$, which comes down to an energy flux of
$$
I=\frac{E}{4\pi L^2 \Delta t}\approx 0.23 \:\mathrm{\mu W/cm^2}.
$$
This is equivalent to a weak light source, but it's probably visible by naked eye under suitably dark conditions.
That said, it's important to remark that the gravitational wave should not be thought of as "moving a heavy mirror" by any distance, and certainly not as performing work while doing so. Instead, its action is to expand and contract the space between the mirrors (even as they remain stationary as far as they can tell), as explained e.g. in How does gravitational wave compress space time?.
