Abstract. The bulk viscosities of two color-superconducting phases, the color-flavor locked (CFL) phase and the 2SC phase, are computed and compared to the result for unpaired quark matter. In the case of the CFL phase, processes involving kaons and the superfluid mode give the largest contribution to the bulk viscosity since all fermionic modes are gapped. In the case of the 2SC phase, ungapped fermionic modes are present and the process u + d ↔ u + s provides the dominant contribution. In both cases, the bulk viscosity can become larger than that of the unpaired phase for sufficiently large temperatures (T 1 MeV for CFL, T 0.1 MeV for 2SC). Bulk viscosity (as well as shear viscosity) is important for the damping of r-modes in compact stars and thus can potentially be used as an indirect signal for the presence or absence of color-superconducting quark matter.Keywords: Color superconductivity, bulk viscosity PACS: 12.38. Mh,24.85.+p,26.60.+c Color superconductivity in compact stars. -Matter at sufficiently large densities and low temperatures is a color superconductor, which is a degenerate Fermi gas of quarks with a condensate of Cooper pairs near the Fermi surface [1]. At asymptotically large densities, where the quark masses are negligibly small compared to the quark chemical potential µ, three-flavor quark matter is in the color-flavor locked (CFL) state [2]. In this state quarks form Cooper pairs in a particularly symmetric fashion. The gauge group of the strong interactions SU (3) c and the chiral symmetry group SU (3) L × SU (3) R are spontaneously broken down to the group of joint color-flavor rotations SU (3) c+L+R . All quarks participate in pairing, giving rise to energy gaps in all quasifermion modes. Therefore, the lightest degrees of freedom in the CFL phase are Goldstone bosons: the broken chiral symmetry gives rise to an octet, with the lightest modes being the charged and neutral kaons (at not asymptotically large densities, chiral symmetry is an approximate symmetry and the Goldstone modes acquire a small mass). Moreover, the CFL phase is a superfluid, spontaneously breaking baryon number conservation symmetry U (1) B . Hence there is a "superfluid mode" which is exactly massless. Goldstone modes in the CFL phase can be described within effective theories [3,4,5], not unlike conventional chiral perturbation theory of the QCD vacuum. The results given below for the CFL bulk viscosity are computed within these effective theories.While rigorous QCD calculations from first principles can be done at asymptotically large densities, the situation is more complicated at moderate densities. Here we are interested in densities of matter inside a compact star. These densities can be as large as several times nuclear ground state density; however, even then the quark chemical potential is at most of the order of 500 MeV. Therefore, perturbative methods within QCD are not applicable and one has to rely on more phenomenological models. Fur-