CAN MINOR PLANETS BE USED TO ASSESS GRAVITY IN THE OUTER SOLAR SYSTEM?

摘要

The twin Pioneer spacecraft have been tracked for over 30 years as they headed out of the solar system. After passing 20 AU from the Sun, both exhibited a systematic error in their trajectories that can be interpreted as a constant acceleration toward the Sun. This Pioneer effect is most likely explained by spacecraft systematics, but there have been no convincing arguments that that is the case. The alternative is that the Pioneer effect represents a real phenomenon and perhaps new physics. What is lacking is a means of measuring the effect, its variation, its potential anisotropies, and its region of influence. We show that minor planets provide an observational vehicle for investigating the gravitational field in the outer solar system and that a sustained observation campaign against properly chosen minor planets could confirm or refute the existence of the Pioneer effect. In addition, even if the Pioneer effect does not represent a new physical phenomenon, minor planets can be used to probe the gravitational field in the outer solar system, and since there are very few intermediate-range tests of gravity at the multiple-AU distance scale, this is a worthwhile endeavor in its own right.