NON-GRAVITATIONAL ACCELERATION OF THE ACTIVE ASTEROIDS

Comets can exhibit non-gravitational accelerations caused by recoil forces due to anisotropic mass loss. So might active asteroids. We present an astrometric investigation of 18 active asteroids in search of non-gravitational acceleration. Statistically significant (signal-to-noise ratio (S/N) > 3) detections are obtained from. three objects: 313P/Gibbs, 324P/La Sagra, and (3200) Phaethon. The strongest and most convincing detection (> 7 sigma in each of three orthogonal components of the acceleration), is for the similar to 1 km diameter nucleus of 324P/La Sagra. A 4.5 sigma detection of the transverse component of the acceleration of 313P/Gibbs (also similar to 1 km in diameter) is likely genuine too, as evidenced by the stability of the solution to the rejection or inclusion of specific astrometric data sets. We also find a 3.4 sigma radial-component detection for similar to 5 km diameter (3200) Phaethon, but this detection is more sensitive to the inclusion of specific data sets, suggesting that it is likely spurious in origin. The other 15 active asteroids in our sample all show non-gravitational accelerations consistent with zero. We explore different physical mechanisms,. which may give rise to the observed non-gravitational effects, and estimate mass-loss rates from the non-gravitational accelerations. We present a revised momentum-transfer law based on a physically realistic sublimation model for future work on non-gravitational forces, but note that it has little effect on the derived orbital elements.