Frame Dragging

In Gravity by Brian Koberlein3 Comments

Frame dragging is one of these interesting effects that shows up in general relativity. Since gravity is an effect of curved space and time in GR, you get things like wibbly-wobbly spacey-timey gravity waves. This also means that when you rotate a mass, the space and time around it is twisted a bit. In other words, the space and time around a rotating black hole is not only bent due to the black hole’s mass, it is also twisted due to the black hole’s rotation.

So how would this affect the motion of stars around the massive black hole in our galaxy’s core? I’ve plotted the result in the figure below. The solid line represents the path of a close orbiting star if the black hole isn’t rotating. The dotted line represents the star’s path if the black hole is rotating rapidly (75% of its maximum limit). They start off nearly identical, but in the rotating case the star’s orbit doesn’t precess nearly as much. This is because the twisted nature of space around the rotating black hole gives the star a bit of angular momentum (slowing down the black hole just a bit in the process) which shifts its orbit just a bit.


Effect of rotation on orbital motion.

The figure I’ve drawn is an exaggerated case. Even if the supermassive black hole in our galaxy is rotating near its maximum, we wouldn’t see the nearby stars affected by such a large amount. But if we keep watching those stars in the core, we might be able to determine the black hole’s rotation eventually.

What we do know is that frame dragging is a real effect. It’s been observed by a satellite orbiting Earth known as Gravity Probe B. Once again Einstein’s theory holds true.


  1. Since twisting might produce a wave, would an echo result that might bounce off another nearby object setting up a permanent feedback?

  2. Editing my earlier post here to ask, since frame dragging produces a wave, would an echo result that might bounce off another nearby object setting up a permanent feedback?

  3. It would be very interesting to measure this efect for a star orbiting the central black hole of the Milky Way. Provided that this black hole rotates.

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