Abstract
We use the proper motions (PM) of half a million red giant stars in the Large Magellanic Cloud measured by Gaia to construct a 2D kinematic map of mean PM and its dispersion across the galaxy, out to 7 kpc from its centre. We then explore a range of dynamical models and measure the rotation curve, mean azimuthal velocity, velocity dispersion profiles, and the orientation of the galaxy. We find that the circular velocity reaches similar to 90 km s(-1) at 5 kpc, and that the velocity dispersion ranges from similar to 30-40 km s(-1) in the galaxy centre to similar to 15-20 km s(-1) at 7 kpc.