Why are orbits around black holes stable? Black hole theory involves space (or space-time), itself, being sucked into the black-hole, with the event horizon marking the point at which space/space-time is moving faster than the speed of light. I find it really hard to picture how this could be happening while objects maintained a reasonable stable orbit around black holes. If we take the stars that orbit the super massive black hole at the centre of the Milky Way, the orbital dynamics are used to calculate the mass of the black hole, in the normal way. In other words not taking account of the fact space is rushing at some speed inwards toward the black-hole. 
I appreciate I'm missing some knowledge here. That's the motivation for asking the question. 
 A: In the comments you mention Susskind's use of a metaphor involving water flow 7 minutes into this video, but this shouldn't be understood in terms of spacetime behaving fundamentally differently around a black hole as opposed to any other gravitating body. Rather, I suspect Susskind is just referring to the analysis of a black hole in a particular type of coordinate system, Gullstrand–Painlevé coordinates, outlined in conceptual terms on this page. As mentioned on the page, "The Gullstrand-Painlevé metric ... is just the Schwarzschild metric expressed in a different coordinate system" (i.e., different from the Schwarzschild coordinates often used to described the curved spacetime around a non-rotating black hole, with the curvature itself understood as coordinate-invariant). The page goes on to say:

Physically, the Gullstrand-Painlevé metric describes space falling
  into the Schwarzschild black hole at the Newtonian escape velocity.
  Outside the horizon, the infall velocity is less than the speed of
  light. At the horizon, the velocity equals the speed of light. And
  inside the horizon, the velocity exceeds the speed of light.

The author of the page also has a more technical paper elaborating on this coordinate system for pedagogical purposes, titled The river model of black holes. In section II the paper mentions some nice features of this coordinate system:

We demonstrate two features that are the essence of the river model
  for spherical black holes: first, that the river of space can be
  regarded as moving in Galilean fashion through a flat Galilean
  background space [eqs. (14) and (15)], and second, that as a freely-
  falling object moves through the flowing river of space, its
  4-velocity, or more generally any 4-vector attached to the
  freely-falling object, can be regarded as evolving by a series of
  infinitesimal Lorentz boosts induced by the change in the velocity of
  the river from one place to the next [eq. (18)]. Because the river
  moves in a Galilean fashion, it can, and inside the horizon does, move
  faster than light through the background. However, objects moving in
  the river move according to the rules of special relativity, and so
  cannot move faster than light through the river.

Also note that in general relativity, according to Birkhoff's theorem the metric outside the surface of any spherically symmetric, non-rotating massive body, like a star or planet with no angular momentum, is just the spacetime geometry given by the Schwarzschild metric, no different than that of a non-rotating black hole of the same mass (the same sort of thing isn't true for rotating bodies vs. rotating black holes, see the last paragraph on p. 39 of this pdf). So, this presumably means that you could also describe the space outside a non-rotating star in the Gullstrand-Painlevé coordinate system, in terms of space acting like a fluid flowing inwards. 
This needn't imply orbits are impossible though, since in this description an object also has a velocity relative to the local space, and its total velocity is the sum of the velocity of space and its velocity relative to space, just as the total velocity of an object in a fluid can be split up into the velocity of the local fluid plus its velocity relative to the local fluid. See my discussion in this answer about the "Newton's cannon" thought-experiment to get a better intuitive feel for how an object which is constantly experiencing a force (which could be from a fluid) pushing towards the center of a circle can nonetheless move in an orbit due to its own tangential velocity.
A: I feel that in general there is a lot of confusion around what black holes are and what they do. in reality, it only gets very different from other objects such as stars very close to or inside the event horizon; in most circumstances it is simply a heavy object. therefore objects would simply orbit around it like any other massive object, as long as the orbital path does not lie to close to the event horizon.
