I am not positive, but I would suspect that the author is talking about the apparent rotation of the fixed stars when something massive "whizzes by" them at a large velocity - or, alternatively, the same rotation as observed by someone quickly flying past a large mass.
Basically, if you fix a telescope on a guide star, and a massive body "whizzes by", after the body passses the telescope won't be pointing at the guide star anymore, it will have rotated - even if care is taken to design the telescope such that there are no tidal torques on it.
This is true even if the telescope has no angular momentum.
I ran across this effect while working on another problem. I'm not sure what the literature has to say about it, unfortunately - it's not clear what to search for, even if I had better access to the literature.
The most controversial thing I can think of offhand is that one might argue that the effect as described could be predicted from SR by treating gravity as a force as a result of Thomas precession.
The effect is rather similar to the geodetic or "De-sitter' precession that one gets in an orbit around a non-spinning test body. (Google for more info - there are a lot of hits. My statements are based on
http://en.wikipedia.org/wiki/Frame_...agihara_observers_in_the_Schwarzschild_vacuum
which may not be the easiest thing to understand).
The major difference is that the orbit in this case is not circular, it is a "flyby" orbit.
Geodetic precession is one of the things that is going to be measured by gravity probe B. It is somewhat interesting in its own right, but perhaps not as interesting as the Lense-Thiring precession, which is due to the actual rotation of the Earth, and the gravitomagnetic field caused by that rotation.
Note that the reason GP-B is in a polar orbit is so that the geodetic precession effects will occur at right angles to the Lense-Thirring precession.