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from a non-alignment between principal axes of inertia andThe results reported here were obtained at the 1.5-m the spin axis. The AO data from May 11, 1996, is of sufficient telescope of the Starfire Optical Range (SOR) located near quality that Vesta's lightcurve can be decomposed into its cross-Albuquerque, NM at the USAF Phillips Laboratory. The sectional area and surface brightness components, proving ana-earliest versions of this system have been described by Fugate et al. (1993Fugate et al. ( , 1994 and Fugate (1994). The current hardware configuration and recent experimental data are 1 Observations reported here were made at the Starfire Optical Range presented in the review by Roggeman et al. (1997) and by on Kirtland AFB, NM, which is owned and operated by the United States Air Force Research Laboratory.

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