  We study stars in M theory. First, we obtain the analog of Oppenheimer --
Volkoff equations in a suitably general set up. We obtain analytically the
asymptotic solutions to these equations when the equations of state are linear.
We study perturbations around such solutions in several examples and, following
a standard method, use their behaviour to determine whether an instability is
present or not. In this way, we obtain a generalisation of the corresponding
results of Chavanis. We also find that stars in M theory have instabilities.
Therefore, if sufficiently massive, such stars will collapse. We discuss the
significance of these (in)stabilities within the context of Mathur's fuzz ball
proposal.
