We present V-J colors of 14 Kuiper Belt objects using new infrared (J) data
combined, in most cases, with simultaneous visible (V) data. We confirm th
e V-J vs absolute magnitude relation reported by Jewitt and Luu (1998) for
the five objects in their data set but demonstrate that the relationship do
es not hold for a larger sample. Kuiper Belt objects exhibit a wide range o
f V-J colors, but there is no correlation with heliocentric distance or orb
ital class. The bimodality seen in BVR colors by Tegler and Romanishin (199
8) is not present in optical-infrared colors. (C) 2000 Academic Press.