  The dark matter problem will be solved only when all of the dark matter is
accounted for. Although wimps may be discovered in direct detection experiments
soon, we will not know what fraction of the dark matter halo they compose until
we measure their local density. In this talk, I will offer a novel method to
determine the mass of a wimp from direct detection experiments alone using
kinematical consistency constraints. I will then describe a general method to
estimate the local density of wimps using both dark matter detection and hadron
collider data when it becomes available. These results were obtained in
collaboration with Gordon Kane at the University of Michigan.
