On the Anomalous Acceleration of 1I/2017 U1 `Oumuamua
arXiv:1903.04723 · doi:10.3847/2041-8213/ab0bb5
Abstract
We show that the photometric period and the astrometrically measured non-gravitational acceleration (at ) of the interstellar object 1I/2017 (`Oumuamua) can be explained by a nozzle-like venting of volatiles whose activity migrated to track the sub-solar location on the object's surface. Adopting the assumption that `Oumuamua was an elongated ellipsoid, this model produces a pendulum-like rotation of the body and implies a long semi-axis . This scale agrees with the independent estimates of `Oumuamua's size that stem from its measured brightness, assuming an albedo of , appropriate to ices that have undergone long-duration exposure to the interstellar cosmic ray flux. Using ray-tracing, we generate light curves for ellipsoidal bodies that are subject to both physically consistent sub-solar torques and to the time-varying geometry of the Sun-Earth-`Oumuamua configuration. Our synthetic light curves display variations from chaotic tumbling and changing cross-sectional illumination that are consistent with the observations, while avoiding significant secular changes in the photometric periodicity. If our model is correct, `Oumuamua experienced mass loss that wasted of its total mass during the span of its encounter with the inner Solar System and had an icy composition with a very low . Our interpretation of `Oumuamua's behavior is consistent with the hypothesis that it was ejected from either the outer regions of a planetesimal disk after an encounter with an embedded planet or from an exo-Oort cloud.
6 Pages, 3 Figures, Accepted for Publication in ApJL. Spin dynamic animations may be found here: https://github.com/DSeligman/Spin_Animations_Oumuamua