We combine new measurements of the thermal emission from the Centaur 1
997 CU26 with published optical photometry to determine the geometric
albedo (0.045 +/- 0.010) and effective diameter (302 +/- 30 km). While
these values are model dependent, they clearly show that 1997 CU26 is
the largest of the known Centaurs and that its surface is very dark.