Cosmic Microwave Background Anisotropies and the Geometry of the Universe

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In this talk, I review some recent work on cosmic microwave background (CMB) anisotropies in an open universe. I emphasize that the observed CMB anisotropies are still consistent with a low value of $Ω$, and I address the question of whether future CMB measurements will be able to provide information on the geometry of the Universe.
(8 page uuencoded PostScript file), IASSNS-HEP-94/56. To appear in the proceedings of the Case Western Reserve University CMB Workshop

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