VLBI Solar System Observations. T. M. Eubanks (U.S. Naval Observatory, Washington, D.C., 20392-5100) Although Very Long Baseline Interferometry (VLBI) observations of radio transmitters inside the solar system commenced soon after the initial developme nt of the VLBI technique, at present such observations have made a fairly minor contribution to solar system celestial dynamics. The DE402 ephemeris, for examp le, uses only 16 VLBI observations in all, with typical accuracies of order 3 milli arc seconds (mas), although even this limited amount of information provides an acc urate tie between the extragalactic radio reference frame and the dynamical solar sys tem frame. By contrast, geodetic and astrometric VLBI can determine the position o f natural radio sources to within 0.3 mas in a single observing session, and the accuracy and stability of the radio reference frame is approaching parts in 10-10 and 10 -11 year-1. Solar system VLBI observations at this level of accuracy would make a considerable improvement to the dynamical reference frame, as well as providing new and sensitive tests of general relativity and Mach's principle. The primary limitation in the application of VLBI to solar system dynamics has been the shortage of suitable space missions during the period of extensive developm ent of VLBI in the last 15 years. The cost of operations, and the accuracy of the resu lts, would be considerably enhanced by the development of VLBI beacons, specifically designed to match the capabilities of current VLBI systems. Routine tracking of lunar beacons would complement and enhance results from Lunar Laser Ranging, and could provide a two orders of magnitude improvement in the determination of lun ar inclination changes and the lunar geodesic precession. Beacons placed on select ed Earth crossing asteroids, or on Mars or Mercury, could provide a considerable improvement in determinations in the solar J2 and the relativistic b parameter. This talk will provide a review of past VLBI observations of spacecraft, and de scribe the radio signal structure and preliminary design details of a proposed lunar b eacon.