On the Anomalous Acceleration of 1I/2017 U1 `Oumuamua

Abstract

We show that the $P\sim 8\mathrm{h}$ photometric period and the astrometrically measured $A_{\mathrm{ng}}\sim 2.5\times 10^{-4}\mathrm{cm}{\mathrm{s}}^{-2}$ non-gravitational acceleration (at $r\sim 1.4\mathrm{AU}$) 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 $a\times b\times c$ ellipsoid, this model produces a pendulum-like rotation of the body and implies a long semi-axis $a\sim 5A_{\mathrm{ng}}{P}^2/4{\pi }^2\sim 260\mathrm{m}$. This scale agrees with the independent estimates of `Oumuamua's size that stem from its measured brightness, assuming an albedo of $p\sim 0.1$, 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 $\sim 10\%$ of its total mass during the $\sim 100\mathrm{d}$ span of its encounter with the inner Solar System and had an icy composition with a very low $[\mathrm{C}/\mathrm{O}]\lesssim 0.003$. 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 $M_{\mathrm{p}}\sim M_{\mathrm{Nep}}$ 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

References in corpus (5)

• Interstellar Interloper 1I/2017 U1: Observations from the NOT and WIYN Telescopes
• 1I/2017 U1 (`Oumuamua) is Hot: Imaging, Spectroscopy and Search of Meteor Activity
• Amateur telescopes discover a kilometre-sized Kuiper belt object from stellar occultation
• Realistic Detectability of Close Interstellar Comets
• Could 1I/'Oumuamua be an icy fractal aggregate?

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• Fitting the Light Curve of 1I/`Oumuamua with a Nonprincipal Axis Rotational Model and Outgassing Torques
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• On The Spin Dynamics of Elongated Minor Bodies with Applications to a Possible Solar System Analogue Composition for `Oumuamua
• Shape-Driven Selection Effects for Aspherical Near-Earth Objects in Systematic Surveys