The interferometer mirrors used to detect gravitational waves are usually described as moving when a gravitational wave passes. This is an easy to understand explanation, but is it correct? Moving 40 kg mirrors is easy to imagine, but suppose that a gravitational wave passes a neutron star with 2 solar masses (4 x 1030 kg) and a typical radius of 11 km. Such a neutron star has a fundamental acoustic oscillation time estimated to be about 0.1 ms. Therefore, gravitational wave frequencies less than about 500 Hz, treat this as a "rigid" acoustic body. Does the center of mass of such a neutron star move when a gravitational wave passes? A “yes” answer has problems with conservation of momentum and explaining which direction the motion will occur. A “no” answer must explain how the distance between two interferometer mirrors changes without any displacement of the center of mass of the mirrors.